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SOUTH 

AUSTRALIAN 

MUSEUM 



±±j/ j/ 



DESCRIPTION OF TWO NEW LARVAL SMARIDIDAE (ACARINA) FROM 

AUSTRALIA 

R. V. SOUTHCOTT 



Summary 

Two new Australian larvae of Smarididae (Acarnia) are described, Smaris arenicola sp. nov. and 
Sphaerotarsus monticolus sp. nov., both from South Australia, from soil and litter. Each is the 
second species known as larva in its genus; both earlier described species were also Australian. The 
term AME is introduced in the coding of the metric data of the larval dorsal scutum. 



DESCRIPTION OF TWO NEW LARVAL SMARIDIDAE (ACARINA) FROM AUSTRALIA 



R. V. SOUTHCOTT 



SOUTHCOTT, R. V. 1997. Description of two new larval Smarididae (Acarina) from Australia. 
Records of the South Australian Museum 30(1): 1-12. 

Two new Australian larvae of Smarididae (Acarina) are described, Smarts arenicola sp. nov. 
and Sphaerotarsus monticolus sp. nov., both from South Australia, from soil and litter. Each is 
the second species known as larva in its genus; both earlier described species were also 
Australian. The term AME is introduced in the coding of the metric data of the larval dorsal 
scutum. 

R. V. Southcott, Honorary Research Associate, South Australian Museum, North Terrace, 
Adelaide, South Australia 5000. Manuscript received 1 May 1996. 



The mite family Smarididae Vitzthum, 1929 is 
cosmopolitan, most members being known as 
adults. The adults (and deutonymphs) are small 
mites, of a generally flattened stature, living as 
predators in litter or under the bark of trees. These 
mites are mostly known from their adult instars. 
The larvae are probably all ectoparasitic on small 
arthropods, as is the case with most other 
members of the superfamily Erythraeoidea. Thus 
one Australian larva, Smarts prominens (Banks, 
1916) , has been found as an ectoparasite of small 
Psocoptera (Womersley & Southcott 1941). A 
taxonomic and historical review of the family was 
given by Southcott (1961a). Seven genera are 
known as larvae (Southcott 1995). Of these two 
are Australian, each with a single described 
species; that of Smarts prominens (Banks, 1916) 
(by Womersley & Southcott 1941), and of 
Sphaerotarsus leptopilus Womersley & Southcott, 
1941 (by Southcott 1960). The present paper 
describes a further new species in each of these 
genera, both from South Australia, and known 
only as larvae. 



Materials And Methods 

Specimens described in this paper were 
obtained by Berlese funnel extractions of samples 
of soil and litter in South Australia. They were 
collected as active larvae, and each was confined 
individually in a small tube and various small 
arthropods were introduced as potential hosts, in 
an effort to elucidate life histories. 

The larvae were eventually mounted in Hover's 
medium after first being cleared in 50% lactic acid 
solution. Microscopy was done with the use of 



Leitz Ortholux/Laborlux microscope equipped 
with phase contrast and polarizing facilities. 
Drawings were made with the use of a drawing 
apparatus. 

Chaetotaxic and other nomenclature and coding 
are as in Southcott (1961b, c, 1963, 1992, 1995). 
The code AME is introduced as a measure of the 
anterior central emargination of the dorsal scutum. 
(In my previous papers I had misinterpreted the 
use of this term as ASBM, which was introduced 
by Fain & Elsen 1987). AME may be formally 
defined as the distance between the anterior end 
of the scutum, in the midline, to the central 
anterior point of the scutum; hence AME=ASBa - 
ASBM (Fain & Elsen). 

The terms protorostral, deutorostral and 
tritorostral will be used for the anterior setae of 
the gnathosoma, following Newell (1957). 

All measurements are in micrometres (]im) 
unless otherwise stated. 

All specimens will be deposited in the South 
Australian Museum (SAM). 

Systematics 

Family SMARIDIDAE Vitzthum 

Smarididae Vitzthum, 1929: 69, 70; Womersley 
& Southcott 1941: 61; Southcott 1946: 173; 1948: 
252; 1960: 149; 1961a: 174; 1961b: 413; 1961c: 
133; 1963: 159; 1995: 57; Shiba 1976: 189. 

Erythraeidae Womersley, 1934: 218 (part). 

Smarisidae Grandjean, 1947: 1. 

For other synonymy see Southcott 1961b: 413— 
414. 



R. V. SOUTHCOTT 



Genus Smarts Latreille 

Smarts Latreille, 1796: 180; Womcrsley & 
Southcott 1941: 63; Southcott 1946:175; 1948: 
252; 1960: 155; 1961a: 176-177; 1961b: 438: 
1961c: 133; 1963: 163; 1995:63. 

Sclerosmaris Grandjean, 1947: 3, 53. 

For other synonymy see Southcottl961b: 438- 
439. 

Key To Larval Smaris 

— PDS 27-29 jam long. AL scutalae blunt- 
ended. Sternala I thickened, well setulose 

S. prominens (Banks, 1916) 

— PDS 28 45 |im long. AL scutalae pointed. 

Sternala I narrow, lightly setulose 

5". arenicola sp. nov. 



Smaris arenicola sp. nov. 
(Figs 1A-D, 2A,B) 

Material examined 

Holotype. South Australia: Loveday, 7 
8.ix.l985, R. V. Southcott, larva ACA2158 from 
soil and litter sample TX244, site Map: 
Department of Lands, South Australia , Barmera- 
Loveday, 2nd Edition 1:10,000 6929-26, MR 
466055 (140°25'03 M E, 34°17 , 25"S), extracted by 
Berlese funnel live 6.x. 1985; to Hover's medium 
28.1.1991. SAM. 

Paratypes. Same data as holotype, 21 larvae 
from same site and sample, ACA2150, 21 52— 
2156, 2159-2173, extracted live similarly 
24.ix.l985-10.x.l985; Hover's medium. SAM. 

Diagnosis of larva 

Anterior scutalae pointed. Gelli 65-72 um 
long. PDS 28^15 um long. 

Description of larva (from slide-mounted 
holotype, supplemented by paratypes) 

Colour in life red. Idiosoma 245 long, 180 
wide; total length of animal 330. 

Dorsal scutum transverse, oval, with slight 
central anterior emargination, minutely porose. 
Scutalae slender, pigmented, AL pointed, PL 
blunt-ended, with adnatc to slightly outstanding 
setules. AL scutalae placed anterolaterally on 
scutum; PL placed posterolateral^; all near edge 
of scutum. Anterior sensillary setae placed about 
midway between levels of AL and PL scutalae 
bases; sockets of posterior sensillary setae lightly 



protruding, placed at about middle of posterior 
border of scutum. Anterior sensillary setae thin, 
but thicker than the filamentous posterior 
sensillary setae; all with slight setules in distal 
two-thirds, longer distally. 
Metric data as in Table I. 

Dorsal idiosomal setae about 41 in number, 
pigmented, blunt-ended, with short, barbed 
setules; anterior setae in indistinct rows across 
dorsum; posterior setae form a denser group. 

Ventral surface of idiosoma: two sternalae 
between coxae I, pigmented, pointed, lightly 
setulose; sternalae II vestigial, presenting as small 
domes c, 5 across, between coxae II; between 
coxae III two intercoxalae 28 long, similar to 
sternalae I. Behind coxae III c. 1 1 setae similar to 
dorsals, 27-36 long, arranged approximately 2, 4, 
4, 1, with a denser grouping towards posterior 
pole. 

Legs fairly short and thick, similar to those of 
Smaris prominens (see Womersley & Southcott 
1941); lengths (including coxae and claws): I 380, 
II 370, III 410. Coxalae and other leg scobalae 
pigmented, setulose, pointed. Supracoxala to leg I 
a slender, blunted peg, 5 long. 

Leg specialized setae: SoGeI.77pd(23), 
VsGeI.90pd(4), SoTiI.50d(38), SoTiI.70pd(33), 
CpTi.75d(8)+SoTiI.76d(28), SoTil.78d(12), 
VsTiI.83pd(6). SoGeII.51pd(15), SoTiIL03d(16), 
SoTiII.78d(10). SoGeIII.52d(14), SoTiIII.03d(12). 
Tarsus I with SoTaI.37d(45), curved, strong, 
pointed; FaTaI..40ad(6); tarsus I also with an 
accompanying trichobothriala to the solenoidala, 
with several long setules, at .44d, seta 40 long. 
Tarsus II with SoTaIL35d(18), slender, nearly 
recumbent. FaTall appears as a minute vestigial 
structure immediately alongside, i.e. posterior to, 
SoTalL All tarsi with a long, slender, blade-like 
empodium, 23 -27 long, over-reaching lateral 
claws, which are paired on each tarsus, about 18 
long, each a pad with a number of long ventral 
onychotrichs. 

Gnathosoma robust, pyriform, 77 long by 75 
wide (combined). Cheliceral digits S-shaped, 16 
long, sharp-pointed. Protorostral (galeal) seta 
simple, slender, pointed, 14 long. Deutorostral 
seta simple, conical, 7 long. Tritorostral setae 
simple, slender, pointed, 21 long. Palpal setal 
formula 0, 0, 1, 1, 3, 7 (including solenoiodala 
and terminala (eupathidala)); all setae (except 
palptarsal solenoidala) pointed; femorala, genuala 
and tibialae 1 and 2 setulose. Odontus pointed, 
hook-like, with two dorsal supplementary spurs 
behind tip. Palpal supracoxala dorsal in position, 
a clavate rod 5 long. 



TWO NEW LARVAL SMARIDIDAE 



I. 

y 



30 




FIGURE 1. Smarts arenicola sp. nov., larva. A, B holotype; A, Dorsal view, on left legs omitted beyond trochanters; 
B, Dorsal idiosomal seta ('b' in A). C, D Paratypes: C, Teratological dorsal scutum of ACA2156; D, teratologics! 
dorsal scutum of AC A2 161. (Each to nearest scale.) 



R. V. SOUTHCOTT 




FIGURE 2. Smaris arenicola sp. nov., larva, holotype. A, Ventral view, on left legs omitted beyond trochanters. B, 
Tip of palp, ventral view, further enlarged. 



TWO NEW LARVAL SMARIDIDAE 



TABLE 1 . Metric data for Smarts arenicola sp. nov. larvae (*for maximum values) 





Holotype 


n 


range 


mean 


s.d. 


c.v. 


Character 














AW 


47 


22 


43^19 


45.5 


1.37 


3.0 


PW 


50 


22 


42-53 


48.3 


2.35 


4.9 


SBa 


22 


21 


19-23 


22.1 


1.01 


4.6 


SBp 


16 


21 


13-16 


15.0 


0.921 


6.1 


LX 


8 


21 


6-12 


8.81 


1.21 


13.7 


ASBa 


20 


21 


15-22 


17.8 


1.83 


10.3 


AME 


2 


21 


1-3 


2.10 


0.436 


20.8 


1SD 


15 


21 


14-17 


15.0 


0.805 


5.4 


L 


38 


21 


34^39 


35.8 


1.34 


3.7 


W 


63 


21 


58-72 


63.7 


3.44 


5.4 


AAS 


16 


21 


14-16 


15.1 


0.831 


5.5 


A-P 


20 


21 


15-20 


16.9 


1.64 


9.7 


AL 


56 


21 


45-64 


55.1 


3.54 


6.4 


PL 


43 


22 


36^7 


42.1 


2.83 


6.7 


ASE 


40 


21 


36-44 


39.7 


1.93 


4.9 


PSE 


65 


19 


60-73 


66.2 


3.92 


5.9 


DS 


31-38 


22 


38^5* 


41.0* 


1.79* 


4.4* 


'Oc' 


37 


22 


36^2 


38.1 


1.98 


5.2 


MDS 


32 


22 


32-38 


34.4 


1.99 


5.8 


PDS 


31-38 


22 


38-45* 


40.8* 


2.05* 


5.0* 


Gel 


68 


22 


60-69 


64.7 


1.93 


3.0 


Til 


66 


22 


60-69 


64.7 


2.12 


3.3 


Tal(L) 


68 


22 


64-73 


68.5 


2.39 


3.5 


Tal(II) 


33 


22 


27-35 


32.2 


2.56 


7.9 


Til/Gel 


0.97 


22 


0.92-1.07 


1.00 


0.0340 


3.4 


Gell 


62 


22 


55-64 


59.3 


2.44 


4.1 


Till 


66 


22 


62-68 


65.6 


1.89 


2.9 


TaII(L) 


50 


22 


47-60 


52.8 


3.15 


6.0 


TaII(H) 


27 


22 


20-31 


26.4 


3.06 


11.6 


Till/Gell 


1.06 


22 


1.02-1.19 


1.11 


0.0490 


4.4 


Gelll 


68 


22 


65-72 


67.9 


1.77 


2.6 


Tilll 


93 


22 


86-93 


89.9 


2.04 


2.3 


Talll(L) 


55 


22 


49-61 


56.3 


2.64 


4.7 


Talll(H) 


26 


22 


20-29 


25.0 


2.29 


9.2 


Tilll/Gelll 


1.37 


22 


1.28-1.38 


1.32 


0.0360 


2.7 


AW/ISD 


3.13 


21 


2.75-3.36 


3.04 


0.187 


6.1 


ISD/A-P 


0.75 


21 


0.75-1.07 


0.887 


0.0913 


10.3 


AW/A P 


2.35 


21 


2.15-3.00 


2.71 


0.260 


9.6 


StI 


18 


22 


18-29 


22.4 


2.97 


13.3 


Cxi 


42 


22 


40-53 


44.0 


2.59 


5.9 


CxII 


22 


21 


20-31 


23.3 


2.51 


10.8 


CxIII 


31 


21 


26-36 


32.1 


2.78 


8.6 


Til/AW 


1.40 


22 


1.32-1.56 


1.42 


0.0668 


4.7 


Tilll/AW 


1.98 


22 


1.83-2.12 


1.98 


0.0666 


3.4 


AW/AL 


0.84 


21 


0.70-1.02 


0.829 


0.05^9 


7.2 


AL/AAS 


3.50 


20 


2.81-4.27 


3.65 


0.341 


9.3 


Tilll/Til 


1.41 


22 


1.28-1.44 


1.39 


0.0402 


2.9 


Till/PW 


1.32 


22 


1.22-1.57 


1.36 


0.0768 


5.6 


LAV 


0.60 


21 


0.47-0.64 


0.56 


0.0416 


7.4 


PW/AW 


1.06 


22 


0.93-1.18 


1.06 


0.0545 


5.1 


AL/PL 


1.30 


21 


1.13-1.52 


1.31 


0.112 


8.5 



R. V. SOUTHCOTT 



Etymology 

The specific epithet arenicola means 'sand- 
dwelling' (Latin), a reference to the site of capture. 

Biology 

All larvae were captured free. In an attempt to 
find possible hosts larvae were introduced 
individually into small tubes, and various small 
arthropods introduced as potential hosts. These 
included various insects: small moths, small 
hemipterans (aphids, psyllids, a ?mirid), small 
Diptera and wingless Psocoptera; also a small 
spiderling. However, no attempt at paras itization 
by any of the mites was observed. 



Genus Sphaerotarsus Womersley 

Sphaerotarsus Womersley, 1936: 119; 
Womersley & Southcott 1941: 63, 73; Southcott 
1960: 149; 1961a: 177; 1961b: 144; 1963: 211; 
1995:57,63. 

Definition of larva 

One eye on each side. Anterior sensillary bases 
anterior to AL scutalae bases; posterior sensillary 
bases posterior to PL scutalae bases. Palpal tibial 
claw (odontus) apically simple or with narrow 
terminal split, and an outstanding basal accessory 
tooth. Genu I with 3-6 solenoidalae. Tibia I with 
four solenoidalae. 



Key To Larval Sphaerotarsus 

PDSto 127 umlong 

.. S. leptopilus Womersley & Southcott, 1941 

PDS to 86 um long S. monticolus sp. nov. 



Sphaerotarsus monticolus sp. nov. 
(Figs. 3A,B, 4A,B) 

Material examined 

Holotype. South Australia. Mt. Lofty, 5 
20.x. 1991, R. V. Southcott, larva ACA2556, in 
damp soil and litter in Eucalyptus obliqua forest, 
sample TX320, site at Map: Adelaide 6628 111, 
1:50,000, MR 897282 (138 41'47" E., 34°58'03 M 
S.), sample collected 5.x. 1991, extracted live by 
Berlese funnel 20.x. 1991. Cleared with 50% lactic 
acid, mounted in Hover's medium. 

Paratypes. South Australia. Hope Forest, 
ll.ix.1980, RVS, in moss under Eucalyptus 
baxteri forest, at Map Reference Milang 1:63,360 
617393 (138°36'19 M E., 35°18'06"S.), site TX198, 



extracted by Berlese funnel 1 4-23. ix. 1980. 
Stirling, at Map Reference Adelaide 1:50,000, 2nd 
Edtn., 934258 (138 o 44*0"E., 34°59 , 30"S.), 
ll.xi.1984, RVS, sample TX232 of soil, litter and 
grass under Eucalyptus hueberiana y extracted by 
Berlese funnel 17.xU984. 

Diagnosis of larva 
PDS to 66 u.m long. 

Description of larva (from slide-mounted 
holotype) 

Colour in life: idiosoma orange, legs pale 
orange. Idiosoma 325 long, 220 wide. Total length 
to tip of cheliceral digits 410; in life these 
dimensions were 300, 200, 380 respectively. 

Dorsal scutum trapezoidal, with rounded 
anterior end and acute posterior end; scutum 
minutely porosc. Scutum has a sclerotized ridge 
enclosing the anterior and posterior sensillary 
areas, of a tear-drop shape, the point posteriorad, 
and within the bases of the four scutalae. Scutalae 
pointed, with many fine, pointed setules. Anterior 
sensillary setae thicker than the filamentous 
posterior sensillary setae; all sensillary setae with 
fine setules in distal half of setal shaft. 

Metric data as in Table 2. 

Eyes 1+1, lateral to scutum, 18 across. 

Dorsum of idiosoma with 24 setae, pigmented, 
expanding slightly distally, blunt-ended, with 
many fine setules; setae arranged approximately 
6,4,2,4,2,4,2. 

Ventral surface of idiosoma: sternalae I pointed, 
setulose; sternalae II absent; anterior to coxae III a 
pair of intercoxalae similar to sternalae I, 36 long, 
60 apart. Behind coxae III are 10 pointed, setulose 
setae, arranged 4, 2, 2, 2. 

Legs somewhat longer than idiosoma; lengths 
(including coxae and claws): I 400, II 395,, III 
495. Leg scobalae pointed, lightly setulose. 
Supracoxala to leg I blunted, 4 long. 

Leg specialized setae: TbGeI.44ad(25), 
TbGeI.44pd(22), SoGeI.60pd(23), SoGeI.67d(16), 
SoGeI.76pd(17), VsGeI.90d(3), TbTiI.48pd(28), 
TbTiI.53ad(29), TbTiI.54pv(27), TbTiI.54av(29), 
SoTiI.61pd(30), SoTiL67d(30), SoTiI.77pd(30), 
CpTiI.80ad(9)+ScTiI.82ad(30), SoTiI.86d(25), 
VsTiI.95pd(2). VsGeII.88d(l), SoTill. 1 ld(14), 
SoTilI.86d(10). SoTiIII.09d(18). 

Tarsus I with SoTaI.17ad(20), TbTaI.20pd(22), 
CpTaI.40ad(9)+SoTaI.42ad(22), FaTaL58ad(l), 
CpTaI.70d(6)+TbTaI.71d(29). Tarsus II with 
SoTaII.39d(20). Lateral tarsal claws with a few 
slender onychotrichs; empodium slender, over- 
reaching lateral claws. 



TWO NEW LARVAL SMAR1DIDAE 




B 



TF 



/ 



¥<v 




10 



50 



FIGURE 3. Sphaerotarsus monticolus sp. nov., larva, holotype. A, Dorsal view, legs omitted beyond trochanters. B, 
Dorsal idiosomal seta (V in A), further enlarged. 



R. V. SOUTHCOTT 



100 




FIGURE 4. Sphaerotarsus monticolus sp. nov., Larva, holotype. A, Ventral view, legs omitted beyond trochanters. B, 
Tip of palp, ventral view, farther enlarged. 



TWO NEW LARVAL SMARIDIDAE 




FIGURE 5. Sphaerotarsus monticolus sp. nov., larva, holotype. Legs I, II, III. (All to scale shown.) 



R. V. SOUTHCOTT 



TABLE 2. Metric data for Sphaerotarsus monticolus sp. nov. larvae (*for maximum values) 





Holotype 


n 


range 


mean 


s.d. 


c.v. 


Character 














AW 


43 


10 


36-47 


41.7 


2.98 


7.2 


PW 


55 


10 


47-66 


56.8 


6.44 


11.3 


SBa 


8 


10 


6-13 


10.6 


2.17 


20.5 


SBp 


12 


10 


11-14 


12.2 


1.40 


11.5 


LX 


17 


10 


15-23 


20.1 


3.00 


14.9 


ASBa 


10 


10 


9-16 


13.4 


2.76 


20.6 


AME 





10 


0-1 


0.10 


0.316 


3.2 


ISD 


35 


10 


30-38 


34.5 


2.99 


8.7 


L 


66 


10 


63-78 


72.1 


5.24 


7.3 


W 


64 


10 


59-75 


67.3 


6.38 


9.5 


AAS 


19 


10 


15-22 


17.5 


2.01 


11.5 


A-P 


19 


10 


14-30 


21.7 


5.29 


24.4 


AL 


58 


10 


57-78 


66.6 


7.88 


11.8 


PL 


51 


10 


57-80 


67.8 


9.26 


13.7 


ASE 


21 


10 


21-29 


25.9 


2.85 


11.0 


PSE 


49 


10 


49-68 


57.5 


6.43 


11.2 


DS 


42-66 


10 


55-86* 


73.5* 


10.5* 


14.2* 


'Oc.' 


45 


10 


45-73 


58.5 


9.92 


17.0 


MDS 


45 


10 


40-73 


54.4 


11.8 


21.8 


PDS 


66 


10 


55-86* 


73.5* 


10.5* 


14.2* 


Gel 


73 


10 


72-82 


76.5 


3.37 


4.4 


Til 


91 


10 


82-97 


89.6 


4.93 


5.5 


Tal(L) 


55 


10 


52-67 


60.4 


5.19 


8.6 


Tal(H) 


22 


10 


22-33 


27.2 


9.15 


33.6 


Til/Gel 


1.25 


10 


1.11 1.25 


1.16 


0.0372 


3.2 


Gell 


60 


10 


56-85 


62.0 


4.00 


6.5 


Till 


85 


10 


76-86 


82.3 


4.27 


5.2 


TaII(L) 


52 


10 


51-60 


55.7 


3.71 


6.7 


Tall(II) 


18 


10 


18-26 


22.4 


2.41 


10.8 


Till/Gcll 


1.02 


10 


1.02 1.40 


1.28 


0.107 


8.3 


Gelll 


78 


10 


72-90 


82.0 


6.86 


8.4 


Till! 


124 


10 


114-140 


127.0 


8.56 


6.7 


Talll(L) 


63 


10 


62-75 


66.8 


4.54 


6.8 


Talll(H) 


17 


10 


17-24 


21.5 


2.22 


10.3 


Tilll/Gelll 


1.59 


10 


1.48-1.74 


1.56 


0.0707 


4.5 


AW/ISD 


1.23 


10 


1.05-1.67 


1.24 


0.184 


14.9 


ISD/A-P 


1.84 


10 


1.20-2.29 


1.66 


0.340 


20.5 


AW/A-P 


2.26 


10 


1.54-3.36 


2.04 


0.596 


29.2 


StI 


34 


10 


29-35 


32.9 


1.79 


5.4 


Cxi 


49 


10 


49-62 


55.6 


4.03 


7.3 


CxII 


37 


10 


34-48 


38.0 


4.22 


11.1 


CxIII 


34 


10 


33—41 


37.6 


3.57 


9.5 


Til/AW 


2.12 


10 


1.81-2.28 


2.16 


0.184 


8.5 


Tilll/AW 


2.88 


10 


2.66-3.50 


3.08 


0.242 


7.9 


AW/AL 


0.74 


10 


0.51-0.82 


0.635 


0.0901 


14.2 


AL/AAS 


3.05 


10 


2.59-4.59 


3.85 


0.608 


15.8 


Tilll/Til 


1.36 


10 


1.36-1.50 


1.44 


0.0505 


3.5 


Till/PW 


1.55 


10 


1.27-1.61 


1.43 


0.144 


10.0 


LAV 


1.03 


10 


1.03-1.17 


1.07 


0.0572 


5.3 


PW/AW 


1.26 


10 


1.01-1.61 


1.40 


0.198 


14.2 


AL/PL 


1.02 


10 


0.88 1.09 


0.988 


0.0601 


6.1 



TWO NEW LARVAL SMARIDIDAE 



It 



Gnathosoma comparatively slender; cheliceral 
bases 64 long by 50 wide (combined); cheliceral 
blades 16 long, slender, curved, pointed. 
Protorostral setae simple, pointed, 9 long. 
Deutorostral setae small, pointed, c. 5 long. 
Tritorostral setae slender, simple, pointed, c. 18 
long. Palpi fairly robust, with setal pattern 0, 0, 1, 
1, 3, 7 including solenoidala and eupathidala 
(terminala). Palpal femorala and genuala blunt- 
ended, setulose; palpal tibiala 1 pointed, setulose; 
palpal tibialae 2 and 3 simple, pointed. Odontus 
simple, with strong ventral, conical, blunted tooth. 
Supracoxala not identified. 

Etymology 

The specific epithet is an adjective, meaning 
'mountain dwelling' (Latin). 

Biology 

Some observations were made on the living 



larva ACA2121. On capture it appeared active 
and healthy; it was identified in life by being 
weighted down on a slide by a small cover glass, 
and examined at 400 diameters magnification. 
After release it became quite active again. It was 
placed in a small dry tube, and droplets of water 
given .Various small arthropods recovered from 
the berlesate were offered as potential hosts over 
several days: a small coccid (Hemiptera), 7-8 
Collembola (?Isotomidae) and an immature 
psocopteran. However, no attempt at parasitization 
was observed during the nine days it survived in 
the tube. 



Acknowledgments 

The work was done with the support of a grant from 
the Australian Biological Resources Study. 



References 



BANKS, N. 1916. Acarians from Australian and 
Tasmanian ants and ant-nests. Transactions of the 
Royai Society of South Australia 40: 224-240. 

FAIN, A., & ELSEN, P. 1987. Observations sur les 
larves du genre Leptus Latreille, 1795 (Acari, 
Erythraeidae) d'Afrique centrale. Revue de Zoologie 
Africaine 101: 103-123. 

GRANDJEAN, F. 1947. Etude sur les Smarisidae et 
quelques autres Erythraeoides (acariens). Archives de 
Zoologie experimental et generate 85 (1): 1-126. 

LATREILLE, P. A. 1796 'Precis des Caracteres 
generiques des insectes, disposes dans un ordre 
naturel.' Prevot, Paris, & F. Bourdeaux, Brive, an 5 
de la R. 

NEWELL, I. M. 1957. Studies on the Johnstonianidae 
(Acari, Prostigmata). Pacific Science 11 (4): 396 
466. 

SHIBA, M. 1976. Taxonomic investigation on free-living 
Prostigmata from the Malay Peninsula. Nature & Life 
in Southeast Asia 7: 83-229. 

SOUTHCOTT, R. V. 1946. On the family Smarididae 
(Acarina). Proceedings of the Linnean Society of New 
South Wales 70 @-4A 173-178. 

SOUTHCOTT, R. V. 1948. Larval Smarididae (Acarina) 
from Australia and New Guinea. Proceedings of the 
Linnean Society of New South Wales 72 (5-6): 252- 
264. 

SOUTHCOTT, R. V. I960. Notes on the genus 
Sphaerotarsus (Acarina, Smarididae). Transactions 
of the Royal Society of South Australia 83: 149-161 . 

SOUTHCOTT, R. V. 1961a. Notes on the genus 



Caeculisoma (Acarina: Erythraeidae), with comments 
on the biology of the Erythraeoidea. Transactions of 
the Royal Society of South Australia 84: 163-178. 

SOUTHCOTT, R. V. 1961b Studies on the systematics 
and biology of the Erythraeoidea, with a critical 
revision of the genera and subfamilies. Australian 
Journal of Zoology 9 (3): 367-610. 

SOUTHCOTT, R. V. 1961c . Description of two new 
Australian Smarididae (Acarina), with remarks on 
chaetotaxy and geographical distribution. 
Transactions of the Roval Society of South Australia 
85: 133-153. 

SOUTHCOTT, R. V. 1963. The Smarididae (Acarina ) 
of North and Central America and some other 
countries. Transactions of the Royal Society of South 
Australia 86: 159-245. 

SOUTHCOTT, R. V. 1992. Revision of the larvae of 
Leptus Latreille (Acarina: Erythraeidae) of Europe 
and North America, with descriptions of post-larval 
instars. Zoological Journal of the Linnean Society 
105(1): 1-153. 

SOUTHCOTT, R. V. 1995. A new larval smaridid mite 
(Acarina: Smarididae) from Costa Rica. Acarologia 
36(1): 57-64. 

VITZTHUM, H. 1929. Ordnung Milben, Acari. Pp. 1- 
112 in 'Die Tierwelt Mitteleuropas', Volume 3, 
Section 7. Quelle & Mayer: Leipzig. 

WOMERSLEY, H. 1934. A revision of the trombid and 
erythraeid mites of Australia with descriptions of new 
genera and species. Records of the South Australian 
Museum 5 (2): 179-254. 



12 R. V. SOUTHCOTT 

WOMERSLEY, H. 1936 Additions to the trombidiid and WOMERSLEY, H., & SOUTHCOTT, R. V. 1941 . Notes 

erythraeid acarine fauna of Australia and New on the Smarididae (Acarina) of Australia and New 

Zealand. Linnean Society's Journal-Zoology 40 Zealand. Transactions of the Royal Society of South 

(269): 107-121. Australia 65 (1): 61 78. 



A NEW SHRIMP OF THE GENUS RHYNCHOCINETES FROM THE 
GREAT AUSTRALIAN BIGHT (CRUSTACEA : DECAPODA : 

RHYNCHOCINETIDAE) 

Junji Okuno 



Summary 

A new shrimp of the family Rhynchocinetidae, Rhynchocinetes enigma, is described and illustrated 
on the basis of two males and an ovigerous female from the Great Australian Bight. This species is 
readily distinguished from the other eleven congeners by the absence of an arthrobranch from the 
third maxilliped or lack of an arthrobranch on the pereiopods. It represents the fourth 
rhynchocinetid species from depths exceeding 100 m. 



A NEW SHRIMP OF THE GENUS RHYNCHOCINETES FROM THE GREAT 
AUSTRALIAN BIGHT (CRUSTACEA: DECAPODA: RHYNCHOCINETIDAE) 

JUNJI OKUNO 



OKUNO, J. 1997. A new shrimp of the genus Rhynchocinetes from the Great Australian Bight 
(Crustacea: Decapoda: Rhynchocinetidae). Records of the South Australian Museum 30(1): 
13-18. 

A new shrimp of the family Rhynchocinetidae, Rhynchocinetes enigma, is described and 
illustrated on the basis of two males and an ovigerous female from the Great Australian Bight. 
This species is readily distinguished from the other eleven congeners by the absence of an 
arthrobranch from the third maxilliped, or lack of an arthrobranch on the pereiopods. It 
represents the fourth rhynchocinetid species from depths exceeding 1 00 m. 

J. Okuno, Natural History Museum and Institute, Chiba, 955-2 Aoba-cho, Chuo-ku, Chiba 
260, Japan. Manuscript received 9 September, 1996. 



Caridean shrimps belonging to the family 
Rhynchocinetidae are distinguished from other 
carideans in the combination of having a typically 
movable rostrum, fine transverse striae on the 
surface of the carapace and abdominal somites, 
the first two pairs of pereiopods robust, with 
fingers bearing long lateral and terminal spines, 
and the second pereiopod with the carpus entire, 
not subdivided. To date, this family includes two 
genera, Rhynchocinetes H. Milne-Edwards and 
Cinetorhynchus Holthuis (Okuno 1996b, in 
press). 

Through the courtesy of Ms K. Gowlett-Holmes 
of the South Australian Museum, Adelaide 
(SAM), I was able to examine two male and one 
ovigerous female specimens of an unfamiliar 
Rhynchocinetes species collected by trawling from 
the Great Australian Bight at depths between 1 1 3 
and 170 m. These specimens do not possess 
arthrobranchs, although the previously described 
congeners at least have arthrobranchs on the third 
maxilliped and the first pereiopod. Because of 
these differences, they are described herein as new 
species. 

The postorbital carapace is abbreviated as CL, 
and the type specimens are deposited in SAM. 



Rhynchocinetes enigma sp. nov. 
(Figs. 1-3) 



Material Examined 

Holotype. Male (SAM C5599, 6.8 mm CL), 
34°17'S, 132°42'E, Great Australian Bight, 



approximately 1 5 km west-south-west of Pearson 
Islands, 140-160 m depth, 'F. V. Comet', April 
16,1989. 

Paratypes. Ovigerous female (SAM C5598, 9.0 
mm CL), 33°12'S, 130°53'E, Great Australian 
Bight, 250 km south-south-west of Ceduna, 113 
m depth, <F. R. V. Soela', August 5, 1981. Male 
(SAM C5600, 7.6 mm CL), 33°18'S, 127°38'E, 
Great Australian Bight, approximately 115 km 
south-west of Eucla, 170 m depth, 'F. V. Comet', 
January 17, 1989. 

Diagnosis 

A species of Rhynchocinetes without 
arthrobranchs on maxillipeds and pereiopods. 
Dorsal rostral margin armed with three 
subterminal teeth. Fourth abdominal somite with 
distinct posteroventral tooth on pleuron. 
Ambulatory pereiopods with meri bearing three 
spines, and dactyli with four accessory claws 
posterior to terminal claw. Endopod of male first 
pleopod with distinct lobe on outer margin. 

Description 

Carapace (Fig. 2A) covered with fine transverse 
striae, armed with two acute teeth on dorsal 
median carina, anterior tooth just behind rostral 
articulation, posterior tooth feebly articulated with 
carapace; supraorbital spine acute, considerably 
longer than spines on dorsal median carina, 
directed anteriorly; antennal spine acute, 
supported by a feeble carina, directed anteriorly; 
pterygostomial spine small, distinct. Rostrum 
(Fig. 2A) articulated with carapace, 1.10 - 1.28x 
as long as carapace; dorsal margin armed with 



14 



J. OKUNO 




FIGURE 1 . Rhynchocinetes enigma sp. nov., holotype male (SAM C5599, 6.8 mm CL). Scale bar = 5 mm. 



two teeth in the basal half, and with three small 
teeth subterminally; ventral margin armed with 
eleven teeth, large proximally, elongate, 
decreasing distally. 

Abdominal somites (Fig. 1) covered with fine 
striae; first three somites with the pleuron 
marginally rounded; pleura of fourth and fifth 
somites with distinct posteroventral tooth; sixth 
somite 0.48 0.50x as long as carapace, with 
acute posteroventral spine, with strongly hooked 
anal spine between bases of uropods, directed 
posteriorly. Telson (Fig. 2B) 0.57 - 0.63x as long 
as carapace, 1.16 - 1.30x as long as sixth 
abdominal somite, armed dorsally with three pairs 
of spines; midpoint of posterior margin 
triangularly produced, with three pairs of spines, 
median pair longest. 

Eyes well developed, with large, globular 
cornea; stalk much more slender than cornea. 

Antennular peduncle (Fig. 2C) reaching 
midlength of scaphocerite; stylocerite long, 
reaching or slightly shorter than level of distal 
margin of antennular distal segment; proximal 
segment with distolateral spine reaching distal 
margin of antennular median segment and small 
proximal lateral tooth, ventrally with acute spine 



at mesial margin; thickened part of upper 
antennular flagellum slightly overreaching rostral 
apex. 

Antenna (Fig. 2D) with scaphocerite 0.84 - 
0.93x as long as carapace, 4.20x as long as 
maximum width, distolateral spine acute, 
distinctly overreaching end of lamella; carpocerite 
reaching proximal quarter length of scaphocerite; 
basicerite with acute ventrolateral spine and with 
rounded protrusion just above the spine. 

Mandible (Fig. 3A) with robust three- 
segmented palp, distal segment rounded, with 
dense setae marginally; incisor process well 
developed, with six marginal teeth; molar process 
obliquely truncate distally, with finely ridged 
distal end. 

First maxilla (Fig. 3B) with slender palp armed 
distally with single long stout spiniform setae; 
proximal endite distinct, rounded, marginally with 
numerous setae; distal endite armed with ten stout 
spines on mesial margin. 

Second maxilla (Fig. 3C) with well developed 
tapering palp; proximal endite slightly truncate; 
distal endite bilobed, upper lobe rather broader 
than lower lobe; scaphognathite large, 
overreaching level of tip of palp, anterior lobe with 



A NEW RIIYNCHOCINETID SHRIMP 



15 




FIGURE 2. Rhynchocinetes enigma sp. nov., holotype male (SAM C5599, 6.8 mm CL). A, carapace with rostrum; B, 
telson, dorsal aspect; C, right antennular peduncle, dorsal aspect; D, right antenna, ventral aspect; E, right firstpereiopod; 
F, right second peretopod; G, right third pereiopod; H, same dactylus; I, endopod of right first pleopod; J, right second 
pleopod; K, right uropod, dorsal aspect. Scale bars; A = 2.5 mm; B, C = 1 mm; D, K - 2 mm; E, G = 1 .5 mm; F = 3 mm* 
H-J = 0.5mm. 



16 



J. OKUNO 



TABLE 1 .Rhynchocinetesenigma,T\ew species. Branchial 
formula. 





Maxillipeds 


Pereiopods 




I 


II 


III 


I 


II III TV V 


Pleurobranchs 

Arthrobranchs 

Podobranchs 

Epipods 

Exopods 


1 
1 


1 
1 
1 


1 
1 


1 
1 


1111 
1 1 1 





feebly quadrate distal end, posterior lobe tapering, 
with elongate plumose setae posteriorly, mesial 
margin convex. 

First maxilliped (Fig. 3D) with endites 
distinctly separated, distal endite concave 
marginally, distinctly larger than proximal endite 
with slightly rounded margin; palp long, 
apparently two-segmented; exopod with long 
flagellum, caridean lobe distinct. 

Second maxilliped (Fig. 3E) with well 
developed podobranch; epipod slightly pointed 
distally; exopod well developed, tapering; dactylar 
segment with truncate distal margin; propodal 
segment with external margin rounded, mesial 
margin expanded; ischiomeral segment distinct. 

Third maxilliped (Fig. 3F) slightly shorter than 
tip of scaphocerite; exopod slightly shorter than 
distal margin of antepenultimate segment, 
tapering, with dense long setae; ultimate segment 
with six spines terminally, 0.59 - 0.62x as long as 
carapace, 2.00 - 2.24x as long as penultimate 
segment; penultimate segment 0.28 - 0.29x as 
long as carapace. 

Branchial formula as shown in Table L 

First pereiopod (Fig. 2E) chelate, moderately 
robust, falling slightly short of midlength of 
scaphocerite; chela 0.44 - 0.45x as long as 
carapace, 2.00 - 2.24x as long as carpus, tips of 
both fingers with dark terminal claws; carpus 0.21 
- 0.25x as long as carapace, with acute spine at 
distal end of dorsal margin; mcrus dorsodistally 
acute. 

Second pereiopod (Fig. 2F) chelate, much more 
slender than first pereiopod, reaching distal sixth 
of length of scaphocerite; chela 0.40x as long as 
carapace; carpus entire, 0.59 - 0.65x as long as 
carapace, 1.50 - 2.03x as long as chela. 

Third pereiopod (Fig. 2G) reaching distal end of 
scaphocerite; ischium with single spine; merus 
0.74 - 0.8 lx as long as carapace, 1.50 - 2.03x as 
long as carpus, with three almost equidistant 
spines; carpus 0.37 - 0.4 lx as long as carapace, 



with two spines on outer surface; propodus 0.69x 
as long as carapace, 1.68x as long as carpus, with 
about six short spinules on flexor margin; dactylus 
(Fig. 2H) with four accessory claws posterior to 
terminal largest claw, decreasing in size 
proximal ly. 

Fourth pereiopod reaching distal fifth of length 
of scaphocerite, spinulation resembling that of 
third pereiopod; merus 0.67 - 0.72x as long as 
carapace, 1.86 -1.94x as long as carpus; carpus 
0.34 - 0.38x as long as carapace; propodus 0.69x 
as long as carapace, 1.81x as long as carpus. 

Fifth pereiopod slightly shorter than midlength 
of scaphocerite; spinulation resembling those of 
two anterior ambulatory pereiopods; merus 0.56 - 
0.62x as long as carapace, 1.57 -1.72x as long as 
carpus; carpus 0.32 - 0.37x as long as carapace; 
propodus 0.58 - 0.66x as long as carapace, 1.79 - 
1.80x as long as carpus. 

Endopod of male first pleopod (Fig. 21) with 
distal end rounded; well developed appendix 
interna at midlength of mesial margin, distal end 
of appendix with dense cincinnuli; distinct lobe at 
distal third of outer margin of endopod. 

Endopod of male second pleopod (Fig. 2J) with 
appendices masculina and interna at distal two 
fifths of outer margin; appendix masculina broad, 
with distal margin rounded, fringed with dense 
setae; appendix interna considerably more slender 
and shorter than appendix masculina, with dense 
cincinnuli at distal end. 

Uropodal exopod and endopod (Fig. 2K) 
slightly overreaching distal end of telson, exopod 
with a fixed and a movable spine at distal fifth of 
outer margin, the former considerably shorter than 
the latter. 

Coloration 
Unknown. 

Distribution 

Known only from the Great Australian Bight. 



Discussion 

Most rhynchocinetid shrimps are found around 
coral or rocky reefs in shallow waters, although 
three species, R. australis Hale, 1941, R. balssi 
Gordon, 1936 and R. ikatere Yaldwyn, 1971 are 
known from deep waters at depths in excess of 
100 m (Hale 1941, Yaldwyn 1971, Holthuis 
1972). The present new species represents the 
fourth rhynchocinetid shrimp obtained from such 
deep waters. Okuno (1996a) suggested that the 



A NEW RHYNCHOCINETID SHRIMP 




FIGURE l.Rhynchocinetes enigma sp. nov., paratype male (SAM C5600, 7.6 mm CL). A, right mandible;B, right first 
maxilla; C, right second maxilla; D, right first maxilliped; E, right second maxilliped; F, right third maxilliped; G, right 
branchial region. Setae omitted on C, D, E. Scale bars; A-E = 1 mm; F = 2 mm; G = 3 mm. 



18 



J. OKUNO 



TABLE 2. Specific list of Rhynchocinetes accompanied with number of arthrobranch (max. = maxilliped; per. = 


pereiopod). 








3rd max. 


1 st per. 


2nd per. 


3rd per. 


4th per. 


5th per. 


R. australis Hale 


2 




1 


„ 


_ 





R. balssi Gordon 


2 




_ 


- 


- 


- 


R. brucei Okuno 


2 






1 


- 


— 


R. conspiciocellus Okuno et Takeda 


2 






- 


- 


- 


R. durbanensis Gordon 


2 






1 


- 


- 


R. enigma sp. nov. 


- 


- 


- 


- 


- 


- 


R. ikatere Yaldwyn 


2 






- 


- 


- 


R. kuiteri Tiefenbacher 


2 






1 


- 


- 


R. rathbunae Okuno 


2 






1 


- 


- 


R. serratus (H. Milne-Edwards) 


2 






1 


- 


- 


R. typus H. Milne-Edwards 


2 






1 


1 


- 


R. uritai Kubo 


2 






- 


- 


- 



temperate and subtropical Rhynchocinetes species 
all have a limited distributional range. Therefore, 
R. enigma probably occurs in southern Australian 
waters only. 

Eleven species belonging to the genus 
Rhynchocinetes were previously known (Okuno 
1996a). Rhynchocinetes enigma differs distinctly 
from the other species by the absence of an 
arthrobranch on all the maxillipeds and 
pereiopods (Fig. 3G). The other Rhynchocinetes 
species always have two small arthrobranchs on 
the third maxilliped and a developed arthrobranch 
on at least the first pereiopod (Table 2). In both 
Rhynchocinetes and Cinetorhynchus, the number 
of arthrobranchs varies at the species level (see 
Table 2; Okuno 1996b), and except for the number 
of arthrobranchs, there is no unique morphological 



character that distinguishes the new species from 
other Rhynchocinetes species. Therefore, I am 
inclined to place the new species in 
Rhynchocinetes, rather than establishing a new 
genus to accommodate it. 

Etymology 

The species name enigma refers to the 
enigmatical status within the genus, because of 
the absence of all arthrobranchs. 



Acknowledgments 

I am grateful to Ms K. Gowlett- Holmes for sending 
me the specimens on loan. I also thank Dr L. B. Holthuis 
for critically reading the manuscript and giving me 
valuable suggestions. 



References 



GORDON, I. 1936. On the macruran genus 
Rhynchocinetes, with description of a new species. 
Proceedings of the Zoological Society of London 
1936: 75-88. 

HALE, H. M. 1941. Decapod Crustacea. B. A. N. Z. 
Antarctic Research Expedition 1929-1931, Reports- 
Series B (Zoology and Botany) 4(9): 257-286. 

HOLTHUIS, L. B. 1972. The Crustacea Decapoda 
Macrura (the Alpheidae excepted) of Easter Island. 
Zoologische Mededelingen, Leiden 46: 29 54, 2 pis. 

OKUNO, J. 1996a. Rhynchocinetes rathbunae, a new 
shrimp from the Hawaiian Islands (Crustacea: 
Decapoda: Rhynchocinetidae). Pacific Science 50(3): 
309-316. 



OKUNO, J. 1996b. Cinetorhynchus manningi, a new 
shrimp (Crustacea: Decapoda: Caridea: 
Rhynchocinetidae) from the western Atlantic. 
Proceedings of the Biological Society of Washington 
109(4): 725-730 

OKUNO, J. in press. Review on the genus 
Cinetorhynchus Holthuis, 1995 from the Indo-West 
Pacific (Caridea: Rhynchocinetidae). in 'Le Benthos 
des Fonds Meubles des Lagons de Nouvelle- 
Caledonie'. Etudes et Theses, Ed. B. Richer de 
Forges, ORSTIOM, Paris. 

YALDWYN, J. C. 1971. Preliminary descriptions of a 
new genus and twelve new species of natant decapod 
Crustacea from New Zealand. Records of the 
Dominion Museum 7: 85-94. 



POMPHORHYNCUS HERONENSIS SP. NOV. (ACANTHOCEPHALA: 

POMPHORHYNCHIDAE) FROM LUT JANUS CARPONOTATUS 

(LUTJANIDAE) FROM HERON ISLAND, AUSTRALIA 

SYLVIE PlCHELIN 



Summary 

Pomphorhynchus heronensis sp. nov. is described from Lutjanus carponotatus (lutjanidae) from 
Heron Island, Australia. The new species can be distinguished easily from all other species of the 
genus by the combination of the following characters: a relatively short neck with a symmetrical 
bulb (bulb/total neck length ratioo = 1: 0.5), 15-17 longitudinal rows with 13-16 hooks per row of 
which the apical hooks (7-8 per row) have roots and are larger than the basal hooks and are 
arranged in slightly spiral rows whereas the basal hooks (6-8 per row) have no roots and are 
arranged in straight rows, a proboscis receptacle that does not extend beyond the bulb and atypical 
cement glands. This is the first species of Pomphorhynchus described from Australia and represents 
one of the few species of that genus known from a marine host. 



POMPHORHYNCHVS HERONENSIS SP. NOV. (ACANTHOCEPHALA: 

POMPHORHYNCHIDAE) FROM LUTJANUS CARPONOTATUS (LUTJANIDAE) 

FROM HERON ISLAND, AUSTRALIA 



SYLVIE PICHELIN 



PICHELIN, S. 1997. Pomphorhynchus heronensis sp. no v. (Acanthocephala: 
Pomphorhynchidae) from Lutjanus carponotatus (Lutjanidae) from Heron Island, Australia. 
Records of the South Australian Museum 30(1): 19-27. 

Pomphorhynchus heronensis sp. nov. is described from Lutjanus carponotatus (Lutjanidae) 
from Heron Island, Australia. The new species can be distinguished easily from all other species 
of the genus by the combination of the following characters: a relatively short neck with a 
symmetrical bulb (bulb/total neck length ratio - 1: 0.5), 15-17 longitudinal rows with 13-16 
hooks per row of which the apical hooks (7-8 per row) have roots and are larger than the basal 
hooks and are arranged in slightly spiral rows whereas the basal hooks (6-8 per row) have no 
roots and are arranged in straight rows, a proboscis receptacle that does not extend beyond the 
bulb and atypical cement glands. This is the first species of Pomphorhynchus described from 
Australia and represents one of the few species of that genus known from a marine host. 

S. Pichelin, South Australian Museum, North Terrace, Adelaide, South Australia 5000. 
Manuscript received 29 April 1996. 



There are four genera of Pomphorhynchidae: 
Pomphorhynchus Monticelli, 1 905, Longicollum 
Yamaguti, 1935, Tenuiproboscis Yamaguti, 1935 
and Paralongicollum Amin, Bauer and Sidorov, 
1991. Of these, only species of Longicollum have 
been recorded in Australia (Edmonds 1989, 
Roubal 1993). There are about 25 species of 
Pomphorhynchus (see Amin 1985, Ortubay et ah 
1991, Wang & Guo 1983). This study describes a 
new species of Pomphorhynchus from Lutjanus 
carponotatus (Lutjanidae) from Heron Island, 
Australia. 



Materials And Methods 



dried, gold sputter-coated and examined under a 
scanning electron microscope operating at 5- 
lOkV. Some worms were serially sectioned and 
stained with Mayer's haematoxylin and eosin. 
Drawings were made with the aid of a camera 
lucida and added to by hand. Measurements, 
presented as the range with the mean followed by 
the standard deviation in parenthesis, are given in 
micrometres; where measurements are presented 
in paired sets separated by a multiplication sign, 
the first figure is length, the second width. Sample 
size is given after each measurement. Type 
material has been deposited in the Australian 
Helminthological Collection (AHC), South 
Australian Museum. 



Twelve Lutjanus carponotatus were collected 
using handlines in the Wistari Channel, Heron 
Island and dissected for parasites. 
Acanthocephalans were removed from the 
intestine; host tissue surrounding the neck 
including the bulb of the worms was removed 
using micropins and forceps. Specimens were 
placed in a cavity block in tap water and 
refrigerated to encourage the eversion of the 
proboscis and then fixed in Berland's fluid and 
stored in 70% alcohol. Specimens were stained 
with Mayer's haematoxylin and mounted in 
Canada balsam. Lactophenol was used to clear 
specimens temporarily for description and 
measurement. Some worms were critical point 



Systematics 

Class PALAEACANTHOCEPHALA 

Family POMPHORHYNCHIDAE Yamaguti, 
1939 

Genus Pomphorhynchus Monticelli, 1905 

Pomphorhynchus heronensis sp. nov. 
(Figs 1-7) 

Type host: Lutjanus carponotatus- (Lutjanidae). 
Other hosts: two specimens from intestine of 1 of 



20 



S. PICHELIN 




FIGURE 1 . a, Proboscis showing two distinct hook types, 
b, apical hooks, and c, basal hooks on proboscis. Scale 
bars: a = 200, b and c = 20. 



5 Cheilinus trilobatus (Labridae) from Heron I., 

Qld, Aust. 

Type site: Rectum - neck and proboscis of 

parasites bulging through rectal wall into body 

cavity of host; infections easily diagnosed from 

outside gut. 

Type locality: Heron I. (23°27' S, 151°55' E), 

Qld, Aust. 

Material: holotype (male) AHC 30345; paratypes 

AHC 27665-27683, 30346. 

Infection rate: 9 of 12 infected. 

Description 

General 

Proboscis cone to pear shaped with slight 
anterior swelling; 2 distinct types of hooks (Figs 
la-c, 2) present. Apical proboscis hooks large 
29.5-51.0 (43.2 ± s.d. 6.6) (n=19) (Fig. lb); root 
25.3-48.5 (39.6 ± s.d. 4.7) (n=15) with slight 
indentation of base; hooks arranged in 15-17 



slightly spiralling rows of 7-8 hooks per row. 
Basal proboscis hooks small 14.8-23.5 (18.2 ± 
s.d. 2.3) (n=10) (Fig. lc), slender with vestigial or 
no roots arranged in 15-17 straight rows of 6-8 
hooks per row. Neck short (neck length: trunk 
length = 1: 0.32-0.61 (1: 0.44 ± s.d. 0.09) 
(n=20)), uniformly cylindrical from trunk level 
until abruptly swells to form symmetrical bulb 
encircling neck; bulb without protrusions or other 
irregularities, may be either spherical or slightly 
wider than long. Proboscis receptacle 923-1307 
(1100 ± s.d. 123) x 161-231 (188 ± s.d. 23) 
(n=10) (Fig. 3) double walled, extends from base 
of proboscis to base of bulb; does not extend into 
trunk. Trunk widest anteriorly, tapering 
posteriorly. Lemnisci 2, slender, 980-2674 (1696 
± s.d. 702) (n=6) long. 

Males 

Total length 7780-13500 (10724 ± s.d. 2213) 
(n=15) (Fig. 4). Trunk 552O-10000 (7409 ± s.d. 
1426) x 1000-2120 (1572 ± s.d. 357) (n=ll) at 
widest point. Neck length including bulb 2250- 
3440 (2735 ± s.d. 522) (n=6); neck width 
excluding bulb 280-620 (392 ± s.d. 100) (n=10); 
bulb 950-1900 (1362 ± s.d. 369) (n=6) x 1360- 
2500 (1856 ± s.d. 441) (n=5); bulb/total neck 
length ratio 1: 0.42-0.59 (1: 0.5) (n=6). Lemnisci 
do not extend beyond anteriormost testis. Testes 2, 
ovoid, 360-840 (609 ± s.d. 124) x 246 520 (377 
± s.d. 90) (n=14), in tandem or diagonal, in 
anterior third of trunk. Cement glands number 
undetermined, probably 2 (Figs 5a -c); glands 
pyriform at level of seminal vesicle but become 
tubular and convoluted as they extend to 
posteriormost margin of testis. Proximal part of 
cement glands, seminal vesicle and Safftigen's 
pouch contained within genital sheath (Fig. 5a); 
ligament sac envelops convoluted tubular part of 
cement glands, sperm duct and testes. Safftigcn's 
pouch pyriform, widest part measures 538 (n=l), 
thick-walled, partly enveloped by cement glands. 
Sperm duct emerges from seminal vesicle, runs 
anteriorly to testes; union of sperm duct and testes 
not seen. Seminal vesicle small, obscured by 
proximal part of cement glands. Bursa with 
pointed digitiform rays and 2 concentric rings of 
circumbursal receptors (Fig. 6). 

Females 

Total length 6630-14000 (9593 ± s.d. 2317) 
(n=21) (Fig. 7a). Trunk 4300-8540 (6157 ± s.d. 
1194) x 1200-2960 (1761 ± s.d. 310) (n=16) at 
widest point. Neck length including bulb, 2000 
3700 (2703 ± s.d. 445) (n=14); neck width 



POMPHORHYNCHUS HEROENENSIS SP. NOV. 



21 




Wt/M 





^JmT^ ^. 




















nnnMHnn 



FIGURE 2. SEM of proboscis showing apical hook (arrow) and basal hook (arrowhead). Scale bar = 50. 



excluding bulb 300-500 (373 ± s.d. 42) (n=14); 
bulb 900-1900 (1333 ± s.d. 350) x 1250-2400 
(1699 ± s.d. 444) (n=16); bulb/total neck length 
1: 0.41-0.59 (1: 0.50) (n=14). Female 
reproductive system consists of ovarian balls, 
ligament sac, uterine bell, uterus, well formed 
vaginal funnel, 2 consecutive vaginal sphincters 
and bulb (Fig. 7b); ligament sac broken in all 
specimens examined. Eggs ovoid to fusiform with 
small polar prolongations of middle membrane 
(Fig. 7c), 98 129 (112 ± s.d. 7) x 27-35 (33 ± 
s.d. 3) (n=15); eggs may be present in neck and 
bulb. 



Discussion 

The present specimens belong to the genus 
Pomphorhynchus according to acanthocephalan 
keys by Amin (1987a) and Amin el al. (1991) 
because they have a neck with a true bulb 
anteriorly and lack the spirally twisted neck which 
is characteristic of Longicollum. 

The number of rows of hooks and the number 
of hooks per row are similar in most species of 
Pomphorhynchus including Pomphorhynchus 
heronensis sp. nov. However, all species of 
Pomphorhynchus except P. heronensis appear to 



22 



S. PICHELIN 




FIGURE 3 . 1 Iorizontal section through the proboscis recep- 
tacle. Scale bar =500. 



have a proboscis receptacle that extends well 
beyond the bulb and, in many instances, into the 
trunk. The atypical shape and number of the 
cement glands in P. heronensis (see below) also 
distinguishes it from all other pomphorhynchid 
species. Further features that can differentiate this 
new species from other similar species of 
Pomphorhynchus are given below. The new 
species can further be differentiated from P. 
patagonicus Ortubay, Ubeda, Semenas and 
Kennedy, 1991, P. sebastichthydis Yamaguti, 
1939 and P. yamagutii Schmidt and Hugghins, 
1973 because they possess asymmetrical bulbs 
(Ortubay et at 1991, Schmidt & Hugghins 1973, 
Yamaguti 1939). Pomphorhynchus yunanensis 
Wang, 1981 differs by having 12 rows of hooks 
with only 5 6 proboscis hooks per row (Wang 



1981). P. lucyi Williams and Rogers, 1984 differs 
by having a considerably longer neck (Williams 
& Rogers 1984) relative to that of P. heronensis. 
Pomphorhynchus cylindericus Wang and Guo, 
1983 and P. bosniacus Kiskaroly and Cankovic, 
1969 have fewer than 15 rows of proboscis hooks 
with 9 or fewer hooks per row (Wang and Guo 
1983, Kiskaroly & Cankovic 1969); also the testes 
of P. cylindericus are more posterior than those of 
P. heronensis. Pomphorhynchus laevis (Zoega in 
Muller, 1776) and P. intermedins Engelbrecht, 
1957 have the last basal hooks on the proboscis 




-peg 



FIGURE 4. Male specimen (holotype), bulb slightly col- 
lapsed. Scale bar ~ 2000. Legend: 1, lemnisci; t, testis; teg, 
tubular part of cement glands; s, Safftigen's pouch; peg, 
posterior part of cement glands; b, bursa with bursal rays. 



POMPHORHYNCHUS HEROENENSIS SP. NOV. 



23 



a 






FIGURE 5. Transverse sections through a male specimen showing: a, the proximal ends of Safftigen's pouch, cement 
glands and seminal vesicle; b, the cement glands partially enveloping Safftigen's pouch (160u further anterior from 
previous section);c, the widening of Safftigen's pouch (70u from previous section). Fig. 5a-c drawn to same scale. Scale 
bar = 500. Legend: s, Safftigen's pouch; peg, posterior part of cement glands; sv, seminal vesicle. 



larger than those immediately preceding (Golvan 
1969). P. heronensis does not have this feature; 
the last basal hook only appears longer when the 
other hooks of P. heronensis are not fully exposed. 
P. intermedins, like many other species of the 
genus, does not appear to possess the two very 
distinct sizes of hooks on the proboscis seen in the 
new species. Two distinct sizes of hooks can be 
seen on the proboscis of P. laevis as shown in 



Brown et ah (1986, Fig. 5) but in addition to the 
differences mentioned above P. laevis has fewer 
hooks per row (13-20 rows with 8-13 hooks) 
(Brown et ah 1986) than P. heronensis. Thus, the 
new species can be distinguished easily from all 
other species of the genus by the combination of 
the following characters: a relatively short neck 
with a symmetrical bulb (bulb/total neck length 
ratio 1:0.5; neck including bulb/trunk length ratio 



24 



S. PICHELIN 






/ 




..■ ' 



\ v 



* 




FIGURE6.Lightphotomicrographofcloacalbursashowingbursal rays (arrow) and two circles of circumbursal receptors 
(arrowheads). Scale bar = 250. 



1:0.44), 15-17 longitudinal rows with 13-16 
hooks per row of which the apical hooks (7-8 per 
row) have roots and are larger than the basal 
hooks and are arranged in slightly spiral rows 
whereas the basal hooks (6-8 per row) have no 
roots and are arranged in straight rows, a 
proboscis receptacle that does not extend beyond 
the bulb and atypical cement glands. 

Some females, but not males, of the new species 
show deformities similar to those described by 
Am in et al. (1991) for specimens of 
Paralongicollum nemacheili Amin et al, 1991. 
Other than the enlarged dorsal trunk region, 
deformed females did not appear to differ from 
normal females. Both normal and deformed 
females had eggs that were dispersed throughout 
the trunk and occasionally into the bulb; no eggs 
were present in the deformed part of the gravid 
female. The presence of eggs in the bulb seems 
uncommon in other pomphorhynchids but has 
been reported in P. kashmirensis Kaw, 1941 by 



Kaw (1941) and in P. sebastichthydis by 
Yamaguti (1939). The presence of eggs may well 
be an artefact of the method of fixing or preserving 
and is certainly not a useful taxonomic character. 

The cement glands of P. heronensis appear 
atypical for the family. Normally, 
pomphorhynchids are said to have six cement 
glands. In this species however, there appear to be 
only two very long glands. A study of serial 
sections showed that the proximal part of the 
glands are pyriform and closely surround 
Safftigen's pouch and the seminal vesicle. The 
glands then narrow out and run alongside the 
sperm duct up to the testes. Monorchic specimens 
of P. heronensis (n=2) appear to have the same 
arrangement of cement glands as normal males. 
Cement glands in species of Pomphorhynchus are 
not usually long but there is at least one other 
species, Filisoma longcementglandatus Amin and 
Nahhas, 1994, that has cement glands that may 
reach up to 16.00 mm in length (Amin & Nahhas, 



POMPHORHYNCHUS HEROENENSISSV. NOV. 



25 



a 





FIGURE 7.a,Femalespecimen, bulbslightlycollapsed,b, uterine bell,c, egg. Scale bars: a=2000,b==500,c = 50. Legend: 
I, lemnisci; o, ovarian ball; ub, uterine bell; ut, uterus; v, vaginal runnel; sph, sphincters, bu, bulb. 



1994). Why P. heronensis should have cement 
glands so different from other pomphorhynchids 
is unknown. It is proposed here that the generic 
diagnosis be amended to include the variable 
nature of the cement glands seen in P. heronensis. 
Two circles of circumbursal receptors similar to 
those described by Brown (1987) were seen in one 
male specimen. Bursal rays were also noted in the 
same specimen. Neither circumpenial receptors 
nor muscular suckers in the bursa as those 



described by Brown (1987) and Doyle and 
Gleason (1991) could be seen in the new species. 
Although Brown (1987) considered the receptors 
may be useful taxonomically, these structures 
were not used as such in this paper because they 
were difficult to see. Brown (1987, Fig. 3) also 
showed the presence of vesicles in the bursa. 
However, Doyle and Gleason (1991) reported 
muscular suckers on the inner bursal surface and 
suggested that the vesicles noted by Brown (1987) 



26 



S. PICHELIN 



could have been a ballooning out of the muscular 
suckers caused by the method of preparation. A 
male with an hyperextended bursa would probably 
not be able to hold the female in position and thus 
fail to copulate. 

Many acanthocephalans show size dimorphism; 
noteworthy is that both males and females of P, 
heronensis appear to be the same length. Also, 
there appeared to be an absence of very young 
stages. Although some juvenile pomphorhynchids 
appear able to detach from the gut, move and 
reattach to another region (Amin 1987b) no 
pomphorhynchids in the present study were found 
other than in the rectum. The lack of juvenile 
stages may indicate that hosts are not continuously 
infected throughout the year or that there is some 
mechanism restricting establishment of new 
parasites. Brown (1986) provided evidence to 
show that populations of P. laevis could reach a 
ceiling level and that parasite establishment could 
be density-dependent. However, in some cases it 
appears that this ceiling level is not reached 
because the critical resource, e.g. space, is only 
limited briefly (Bates & Kennedy 1991). 

Pomphorhynchids have been recorded from a 
wide range of teleosts (see Golvan & de Buron 
1988). Amin (1987c) recognised three categories 
of hosts for P. bulbocolli Linkins in Van Cleave, 
1919: principal, accessory and occasional hosts. 
In this study, L. carponotatus is considered as a 
principal host for P. heronensis because female 
pomphorhynchids with ovarian balls, immature 
and mature shelled acanthors were regularly 
recovered, all parasites were firmly attached and 
none were found extraintestinally. This is 
consistent with the findings by Brown et al. 
(1986) and Amin (1987c) who considered the 
regular presence of mature gravid females as an 
indication that the parasite is in its preferred 
definitive host. It is also consistent with the 
observations made by Kennedy (1984) that P. 
laevis in its non-preferred hosts were smaller, 
immature, weakly attached and many were 
recovered in extraintestinal sites. 

Most species of Pomphorhynchus occur in 



freshwater fishes. Some exceptions such as 
Pomphorhynchus laevis have been recorded from 
both freshwater and marine fishes (see, for 
example, Kennedy 1984). Although, it has been 
suggested that the freshwater P. laevis is a 
different strain from the marine P. laevis and that 
each strain has a preferred host (see Kennedy 
1984); currently there is thought to be three strains 
(see Kennedy et al 1989, Kennedy 1996). The 
preferred position in the preferred marine host of 
P. laevis is the rectum whereas the preferred 
position in freshwater host is more anterior (see 
Kennedy 1984). All the specimens of P. 
heronensis recovered for this study were found in 
the rectum of its host, L. carponotatus. Lutjanus 
carponotatus is not known from freshwater 
habitats (Allen & Talbot 1985) and thus the 
posterior position of the parasite cannot be 
correlated with a response to changing salinity as 
shown by Kennedy (1984) for P. laevis under 
certain circumstances. 

Specimens of Pomphorhynchus heronensis 
were also recovered from one of five Cheilinus 
trilobatus in the present study and from one of 
five from another study of helminths in fishes of 
Heron Island (Cribb pers. comtn.). In these 
specimens the parts of the worms that had 
penetrated the gut wall (i.e. the neck including the 
bulb) were decayed. Had this deterioration 
resulted from the worms being reproductively 
exhausted followed by death in situ, then worms 
in similar condition should have been found in L. 
carponotatus; none were. It may be that C. 
trilobatus is an unsuitable or at best an occasional 
host for P. heronensis but further material is 
needed to negate the possibility of other factors 
influencing the presence or absence of these 
parasites, such as the distribution of intermediate 
hosts and seasonality. 



Acknowledgments 

I am grateful to Dr T. H. Cribb for donating specimens 
of this species and reading this manuscript 



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FIELD IDENTIFICATION OF FEMALE LITTLE BROWN BATS 
VESPADELUS SPP. (CHIROPTERA : VESPERTILIONIDAE) IN SOUTH 

AUSTRALIA 

L. F. QUEALE 

Summary 

Five morphologically similar species of little brown bats occur in South Australia; Vespadelus 
finlaysoni, V. darlingtoni, V. regulus, V. baverstocki and V. vulturnus. As males can be identified 
by the shape of their penes, the emphasis of this paper is on methods to differentiate the females of 
these similar species. Characters are listed here for identifying female Vespadelus bats, particularly 
for use in the field, using external measurements and geographic distribution data. Vespadelus 
finlaysoni and V. darlingtoni were found to be generally distinguished on size alone and V. 
vulturnus to be distinguished on a wing measurement ratio. Vespadelus regulus and V. baverstocki 
presented the greatest difficulty for identification. However this study shows that these two species 
can be distinguished 90% of the time. Areas of allopatry, parapatry and sympatry are also discussed. 



FIELD IDENTIFICATION OF FEMALE LITTLE BROWN BATS VESPADELUS SPP. 
(CHIROPTERA : VESPERTILIONIDAE) IN SOUTH AUSTRALIA 



L. F. QUEALE 



QUEALE, L. F. 1997. Field Identification of female little brown bats Vespadelus spp. 
(Chiroptera: Vespertilionidae) in South Australia. Records of the South Australian Museum 
30(1): 29-33. 

Five morphologically similar species of little brown bats occur in South Australia; Vespadelus 
finlaysoni, V. darlingtoni, V. regulus, V. baverstocki and V. vulturnus. As mates can be 
identified by the shape of their penes, the emphasis of this paper is on methods to differentiate 
the females of these similar species. Characters are listed here for identifying female Vespadelus 
bats, particularly for use in the field, using external measurements and geographic distribution 
data. Vespadelus finlaysoni and V. darlingtoni were found to be generally distinguished on size 
alone and V. vulturnus to be distinguished on a wing measurement ratio. Vespadelus regulus 
and V. baverstocki presented the greatest difficulty for identification. However this study shows 
that these two species can be distinguished 90% of the time. Areas of allopatry, parapatry and 
sympatry of species are also discussed. 

L. F. Queale, South Australian Museum, North Terrace, Adelaide, South Australia 5000. 
Manuscript received 20 June 1 996. 



The bats once referred to as a single species of 
Eptesicus (E. pumilus) are now regarded as nine 
species of Vespadelus (Kitchener et al. 1987, 
Volleth & Tidemann 1991). This diversity has 
only recently been recognised and many of the 
species' morphologies are very similar, so that 
practical problems in the field of specimen 
identification have not yet been completely solved. 

The current taxonomy follows Kitchener et al. 
(1987) who revised the genus using a combination 
of morphological features. Their conclusions were 
confirmed by allozyme electrophoresis (Adams et 
al. 1987) which showed a minimum of nine 
species. Males of the five South Australian 
species, Vespadelus finlaysoni, V darlingtoni, V 
regulus, V. baverstocki and V. vulturnus, can be 
unambiguously identified using penis glans 
morphology (Reardon & Flavel 1987) but a 
reliable method is not available for female 
morphology. Many of the characters used by 
Kitchener et al (1987) were internal features and 
cannot be used for field identification. Geographic 
variation within species further complicates 
identification. 

The aim of the present study was to provide 
simple field methods for identifying female 
Vespadelus spp. using external characters. 
Outside South Australia other workers have found 
that there is more overlap in forearm lengths 
between species (Tidemann 1981, Lumsden & 
Bennett 1995). I found that limiting this study to 



South Australia, the task of identification can be 
made easier. These methods will prove useful in 
other states, although because of geographical 
variation there may be some differences. 

Materials And Methods 

Initially, 127 adult female Vespadelus bats (9 
V. darlingtoni, 11 V. finlaysoni, 50 V. regulus, 38 
V. baverstocki and 15 V vulturnus) from the spirit 
preserved mammal collection of the South 
Australian Museum were examined for this study. 
Adults were distinguished by ossification of wing 
bone epiphyses. Specimens in the collection were 
collected from widely separated localities to take 
account of regional variation within South 
Australia. Based on the results of previous 
investigations (Carpenter et al. 1978, McKean et 
al 1978, Tidemann et al. 1981, Kitchener et al. 
1987) and the ease of measurement and 
assessment, the following characters were selected 
for examination: 

1 ) forearm (= radius) length 

2) ratio of phalanx I to metacarpal length on 
digit 111 

3) geographic distribution 

4) colour of skin and fur 

Wing bone length measurements (to the nearest 
0.1 mm) were taken, using dial calipers, from 
joint to joint (outside) when the joints were bent 
(see Reardon and Flavel 1987). 



30 



L, F. QUEALE 



Distribution maps were compiled for each 
species using females that had been reliably 
identified by electrophoresis (n=45) and males 
identified by glans penes (n=133), following the 
method of Reardon and Flavel (1987). 

General colour of skin and fur were also noted 
to aid identification. 

To test the reliability of the characters described 
above, an additional 40 bats were analysed using 
electrophoresis of liver enzymes. The 
discriminating enzymes used were: aspartate 
aminotransferase, carbonate dehydratase, p- 
hosphogluconatc dehydrogenase, dipeptidase, 
tripeptide aminopeptidase, glucose-6-phosphate 
isomerase, mannose-6-phosphate isomerase (see 
Adams et al. 1987). 



30,0 -1 










it H buventvcki 








__•—, Hi v - regulus 


« 20.0 — 
6* 










O 15.0 - 

c 

V 

3 
















5.0 - 


















0.0 - 


r" 

















26.5 270 ti.% 2X.0 2X.5 29.0 29.5 30.0 30 5 310 315 32. B 31.5 33 33 5 

Forearm length (mm) 

FIGURE 1 . Size ranges in forearm length of female V. 
haverstocki and V, regulus in South Australia, showing 
the degree of overlap. 



Results And Discussion 



Forearm Length 

Forearm ranges of Vespadelus spp. from South 
Australia were smaller than those of Kitchener et 
al. (1987). Two size groups were evident (see also 
Kitchener et al 1987): Vespadelus finlaysoni and 
V. darlingtoni were separated from other species 
by their greater forearm length (Table 1). Females 
of these two species exceded 33.0 mm whereas 
the other three were usually less than 33.0 mm. 
The three smaller species (V. regulus, V. 
vulturnus and V. haverstocki) form a species 
group which is referred to here as the "regulus 
complex'. 

Within the 'regulus complex' in South 
Australia there were two subgroups based on 
forearm length, with a larger species, V. regulus, 
and two smaller species, V, haverstocki and V. 
vulturnus. There was considerable overlap in 
forearm length between V. haverstocki and V. 
vulturnus. Among adult females, 90% of V. 
regulus had forearm lengths greater than 30.5 
mm, while all V. vulturnus and 95% of V, 
haverstocki measured less than 30.5 mm. Fig. 1 
shows the overlap in forearm length of females. 



Ratio of Phalanx I: Metacarpal of Digit III 

The ratio of phalanx I to the metacarpal on the 
third wing digit was used by Kitchener et al. 
(1987) to distinguish V, vulturnus from other 
species. Table 2 shows ratio ranges calculated for 
the three "regulus complex' species using only 
specimens identified by electrophoresis. Since sex 
does not affect this character (Kitchener et al. 
1987), sexes were combined in the table. The data 
demonstrate a clear distinction between V. 
vulturnus (ratio > 0.396) and the other two species 
(ratio < 0.395) and confirm previous findings 
(Kitchener et al. 1987). Vespadelus haverstocki 
and V. regulus cannot be distinguished using this 
ratio. 

Distribution and Habitat 

Figs 2 to 6 show the geographical distribution 
of each species. Initially these maps were drawn 
using only bats that were identified by 
electrophoresis or penis morphology. Bats 
identified on wing measurements were examined 
later and all fell within the distribution ranges 
already recorded for the species. Habitat 
information has been taken from Carpenter et al. 
(1978) Reardon and Flavel (1987) and Lumsden 
and Bennett (1995). 



TABLE 1. Means and ranges of forearm length (mm) of 
female Vespadelus species in South Australia. 



Species 



SD 



Range 



V. darlingtoni 


35.80±0.99 


(34.7-38.1) 


9 


V. finlaysoni 


34.45±0.86 


(33.0-35.5) 


11 


V. regulus 


31.37±1.14 


(29.3-33.1) 


50 


V. haverstocki 


29.12±0.95 


(27.0-30.9) 


38 


V, vulturnus 


28.47±1.24 


(26.2-30.6) 


15 



TABLE 2. Range of ratios of phalanx I : metacarpal of digit 
III of Vespadelus spp. of the ' regulus complex' in South 
Australia. Males and females included. 



Species 



Ratio 



V. regulus 
V, haverstocki 
V. vulturnus 



0.34O-0.395 
0.340-0.395 
0.396-0.420 



50 
38 
15 



LITTLE BROWN BATS IN SOUTH AUSTRALIA 



31 




134° 



26° 



30° 



34° 




26° 



30° 



FIGURE 2. Distribution of V. darlingtoni in South 
Australia. 



Vespadelus darlingtoni (Fig. 2) is confined to 
forested areas in the wetter southern and eastern 
regions of the State; 

Vespadelus finlaysoni (Fig. 3) occurs in arid 
northern areas of South Australia in mountain 
ranges and rocky country in association with 
mines and caves; 



FIGURE 4. Distribution of V. regulus in South Australia. 

Vespadelus regulus (Fig. 4) occurs in the south 
and east of South Australia in mallee woodlands 
and forests. It roosts in tree hollows and buildings. 
It is the only species found on Yorke and Eyre 
Peninsula; 

Vespadelus baverstocki (Fig. 5) is found over a 
wide area in the arid and semi-arid woodlands 
and shrublands of the State and roosts in tree 
hollows and buildings; 



26° 



30° 




-38° 



FIGURE 5. Distribution of V. baverstocki in South 
FIGURE 3 . Distribution of V. finlaysoni in South Australia. Australia. 



32 



L. F. QUEALE 




26° 



30° 



34° 



FIGURE 6. Distribution of V. vulturnus in South 
Australia. 



Vespadelus vulturnus (Fig. 6) is found in 
woodlands and forests of the south-eastern region 
of the State, and along the River Murray. It roosts 
in tall trees along the River Murray and in the 
South East (Reardon & Flavel 1987). 

Vespadelus regulus and V. darlingtoni are the 
only species of the genus to date recorded on 
Kangaroo Island. 

There are several areas of sympatry for 
Vespadelus species in the State. The range of V. 
finlaysoni is shared with that of V. baverstocki 
(Figs 3 and 5) but the former species is not found 
in the regions occupied by the other two 'regulus 
complex' species. The northern limits for V. 
regulus and the southern ranges of V. baverstocki 
overlap in central Eyre Peninsula and the Murray 
Mallee (Fig. 4). In this region it has been 
suggested that V. baverstocki prefers Acacia spp. 
open woodland and V. regulus, the mallee (C. 
Kemper, T. Reardon pers. comm., Lumsden and 
Bennett 1995). Vespadelus vulturnus inhabits 
wetter, tall forested areas. Considerable overlap 
occurs between all three 'regulus complex' 
species in the River Murray region (Figs 4-6). 
Here a corridor of sympatry follows the 250 mm 
isohyet which coincides with the separation of 
eucaiypt (mallee) and Acacia spp. woodland 
(Griffin & MacCaskill 1986) and the well-watered 
riverine eucaiypt forest. 



Colour 

Differences in fur colour have been noted 
between Vespadelus species (McKean et al. 1978; 
Kitchener et al. 1987; Reardon & Flavel 1987). 
The fur of V. darlingtoni is very dark brown, as is 
the skin on the forearms. By contrast, the fur of V. 
finlaysoni is grey. The 'regulus complex' species 
share a third colouration type in which the fur is 
bicoloured, the hairs having brown bases and pale 
tips. The ventral surface of the body is lighter than 
the dorsal surface. Hence colour is not useful for 
distinguishing between the species of the 'regulus 
complex'. 

Electrophoresis 

To test the key (below) an additional sample of 
female bats, with accompanying frozen tissue, was 
identified using the key as 26 V. baverstocki, 10 
V. regulus and four V. vulturnus. Then allozyme 
electrophoresis was performed on this sample. The 
allozyme comparisons confirmed that the 
morphological characters had correctly predicted 
the identifications of all 40 specimens. This 
confirmation indicates that despite overlap in 
some characters, the key can be used with 
confidence to distinguish the species. 

Species summaries 

Vespadelus darlingtoni may be easily 
distinguished from the 'regulus complex' species 
by its greater size (forearm length) and from V. 
finlaysoni by its dark colour and distribution. 

Vespadelus finlaysoni is similarly distinguished 
by its large size from the ^regulus complex' 
species. There is a size overlap with V regulus 
but there is no overlap in distribution. 

Vespadelus vulturnus is separated from the two 
larger species, V finlaysoni and V. darlingtoni on 
size r with no overlap in forearm measurements. A 
size overlap occurs rarely with V regulus and 
more commonly with V. baverstocki and may be 
distinguished from these on the basis of the 
phalanx I: metacarpal ratio. 

Vespadelus regulus may be distinguished from 
V. darlingtoni on size and colour, from V. 
finlaysoni on distribution and partly on size, and 
from V. vulturnus partly on size and wing ratios. 

Vespadelus baverstocki can be readily 
distinguished on size from the two largest species, 
V. finlaysoni and V. darlingtoni. It can be 
separated from V. vulturnus on the basis of 
phalanx I: metacarpal ratio. In many cases it can 
be separated from V. regulus on size. When this is 
not successful electrophoresis must be employed. 



LITTLE BROWN BATS IN SOUTH AUSTRALIA 



33 



Key To Female Vespadelus In South Australia 

1. — Forearm greater than 33 mm 2 

Forearm less than 33 mm 3 

2, — Latitude south of 33°S V. darlingtoni 

Latitude north of 33°S V. finlaysoni 

3 — Ratio of phalanx I: metacarpal of digit 
111 greater than 0.39; latitude south of 
33°S V. vultumus 

Ratio of phalanx I; metacarpal of digit 
ITT less than 0.39; locality variable 4 

4. — Forearm usually greater than 30.5 mm; 
mallee habitat/coastal or latitude south 
of 34°S V. regulus 

Forearm usually less than 30.5 mm; arid 
habitat/inland or usually latitude north of 
34°S V. baverstocki 

Note on males 

Although males can be identified by penis 
morphology, this can prove difficult in the field. 
The characters discussed above can be used to 
identify males. However my data indicate that 
male forearms tend to be shorter than females. 



TABLE 3. Ranges of forearm length (mm) of male 
Vespadelus species in South Australia. 



Species 


x SD 


Range 


n 


V. darlingtoni 


34.9±0.51 


(33.5-38.1) 


14 


V. finlaysoni 


33.2±0.64 


(32.4-34.4) 


13 


V. regulus 


30.3±0.96 


(28.5-33.1) 


51 


V. baverstocki 


29.2±0.96 


(26.7-30.7) 


29 


V. vultumus 


27.7±1.33 


(25.2-29.5) 


16 



Thus the key can be used with some discretion as 
an aid in identification of males. The one 
exception is that the identification key and species 
summaries do not distinguish easily between male 
V. regulus and V. baverstocki on forearm lengths 
(see Table 3). 



Acknowledgments 

I wish to thank M. Hutchinson for his advice and 
encouragement. I am also grateful to K. Bowshall-Hill 
for drawing the maps. I wish to thank the two referees 
whose comments greatly improved the final paper, and 
my husband B. McHenry for encouragement and help in 
completing the manuscript. 



References 



ADAMS, M., BAVERSTOCK, P. R., WATTS, C. H. S. 
& REARDON, T. B. 1987. Electrophoretic resolution 
of species boundaries in Australian Microchiroptera. 
L Eptesicus (Chiroptera: Vespertilionidae). 
Australian Journal of Biological Sciences 40: 143- 
162. 

CARPENTER, S. M., McKEAN, J. L. & RICHARDS, 
G. C. 1978. Multivariate morphometric analysis of 
Eptesicus (Mammalia: Chiroptera) in Australia. 
Australian Journal of Zoology 26: 629-638. 

GRIFFIN, T. & MacCASKILL, M. (Eds) 1986. k Atlas 
of South Australia'. South Australian Government 
Printer: Adelaide. 

KITCHENER, D. J., JONES, B. & CAPUTI, N. 1987, 
Revision of Australian Eptesicus (Microchiroptera: 
Vespertilionidae). Records of the Western Australian 
Museum 13: 427-500. 

LUMSDEN, L. F. & BENNETT, A. F. 1995. Bats of a 
semi-arid environment in south-eastern Australia: 



biogeography, ecology and conservation. Wildlife 
Research 22: 217-240. 

McKEAN, J. L., RICHARDS, G. C. & PRICE, W. J. 

1978. A taxonomic appraisal of Eptesicus 
(Chiroptera: Vespertilionidae) in Australia. Australian 
Journal of Zoology 26: 529-537. 

REARDON, T. B. & FLAVEL, S. 1987. 'A Guide to the 
Bats of South Australia'. South Australian Museum: 
Adelaide. 85pp. 

TIDEMANN, C. R., WOODSIDE, D. P., ADAMS, M. 
& BAVERSTOCK, P. R. 1981. Taxonomic separation 
of Eptesicus (Chiroptera: Vespertilionidae) in 
southeastern Australia by discriminant analysis and 
electrophoresis. Australian Journal of Zoology 29: 
119-128. 

VOLLETH, M. & TIDEMANN, C. R. 1991. The origin 
of the Australian Vespertilionidae bats, as indicated 
by chromosomal studies. Zeitschrift fiir 
Saugetierkunde 56: 321 330. 



FOUR NEW SPECIES OF ANTIPORUS SHARP (COLEOPTERA, 

DYTISCIDAE) FROM AUSTRALIA, WITH NOTES ON A. FEMORALIS 

(BOH.) AND A. INTERROGATIONS (CLARK) 

C. H. S. Waits 



Summary 

Four new species of Antiporus are described from Australia: A. jenniferae sp. nov., A. 
hollingsworthi sp. nov., A. willyamsi sp. nov. and A. pembertoni sp. nov. The distribution of A. 
femoralis (Boh.) and A. interrogationis (Clark) in Australia is reviewed. A key to the Australian 
species is provided. 



FOUR NEW SPECIES OF ANTIPORUS SHARP (COLEOPTERA, DYTISCIDAE) 

FROM AUSTRALIA, WITH NOTES ON A. FEMORAHS (BOH.) 

AND A. INTERROGATIONS (CLARK) 

C. H. S. WATTS 



WATTS, C. H. S., 1997. Four new species of Antiporus Sharp (Coleoptera, Dytiscidae) from 
Australia, with notes on A. femoralis (Boh.) and A. interrogaiionis (Clark). Records of the 
South Australian Museum 30(1): 35-42. 

Four new species of Antiporus are described from Australia: A. jenniferae sp. nov., A. 
hollingsworthi sp. nov., A. willyamsi sp. nov. and A. pembertoni sp. nov. The distribution of A. 
femoralis (Boh.) and A. interrogaiionis (Clark) in Australia is reviewed. A key to the Australian 
species is provided. 

C. H. S. Watts, South Australian Museum, North Terrace, Adelaide, South Australia 5000. 
Manuscript received, 28 February 1996. 



The species of Antiporus were last revised by 
Watts (1978) who recognised six species. In 1984 
Brancucci (1984) resurrected A. interrogaiionis 
(Clark) from synonymy with A. femoralis (Boh.). 
In this paper I take the opportunity to describe 
four additional species of Antiporus Sharp from 
Australia and to review the distribution of A. 
femoralis (Boh.) and A. interrogaiionis. One of 
the new species, A. jenniferae, is close to A. 
simplex Watts, one, A. willyamsi, has unusual 
sexual hairs on the front and middle trochanters 
and the other two belong to a group of dark 
coloured Antiporus with enlarged metafemora in 
the males (A. femoralis, A. interrogaiionis, A. 
wilsoni Watts, A. hollingsworthi n. sp. and A. 
pembertoni n.sp.). Males of this A. femoralis 
group are easily separated on the shapes of the 
metafemur, proclaw and aedeagus. Females are 
difficult to distinguish, other than A. 
interrogaiionis which can be recognised by the 
colour on the pronotum. 

The new species arc rare in collections, 
although this may in part reflect a lack of 
collecting particularly in south-west Australia. 

The collections from which specimens were 
examined are listed under the following 
abbreviations: 

AM Australian Museum, Sydney. 
ANIC Australian National Insect Collection, 

Canberra. 
BMNH Natural History Museum, London. 
MV Museum of Victoria, Melbourne. 
SAMA South Australian Museum, Adelaide. 
WAM Western Australian Museum, Perth. 
UQIC Entomology Department Queensland 
University, Brisbane. 



Systematics 
Key To Australian Species Of Antiporus Sharp 

— Protarsus with 2 claws Females 2 

— Protarsus with 1 claw Males 10 

: — Relatively large (> 6mm), predominantly 
reddish-yellow, elytra with 5-6 often 
incomplete long dark lines 

A. gilberti (Clark) 

— Not with above combinations of characters 
3 

— Protarsi black. Relatively small (<4mm) .. 
A. jenniferae sp. nov. 

— Protarsi reddish-yellow, same colour as 
rest of leg 4 

At least the basal segment of mesotarsi 
enlarged in comparison with protarsi 5 

— Segments of mesotarsi similar to those on 
protarsi or smaller 6 

Elytron with small and large punctures, 
all mesotarsal segments larger than those 
of protarsi, elytra with lighter streaking in 
younger specimens ...A. willyamsi sp. nov 

— Elytra with uniform punctuation, only 
basal segment of mesotarsi enlarged, 
elytra uniformly dark red-brown to black . 
A. wilsoni Watts 

— Smaller (< 3.5mm) 7 

— Larger (>3. 5 mm) 8 



36 C.H.S. WATTS 

7 — Elytron dark, usually with three reddish- — Protarsi reddish-brown, same colour as 

yellow spots, pronotum reddish-yellow rest of leg 15 

with dark front and rear borders 

A. bakewelli (Clark) 15 — Elytron unicolorous, except for slightly 

. r i . paler sutural region and sides. Metacoxal 

— Elytron and pronotum uniformly red- ,. , A - , ■ , 01 

, J r ,.,,,, lines evenly diverging anteriorly. Claw 

brown A. simplex Watts , ,J , , ■ /, -., 

£ on protarsus relatively straight, with 

8 _ More or less uniformly dark reddish- small basal tooth (Fig. 21) .. 

brown, elytron tip often appears truncated A ' sim P lex Watts 

A. blakei (Clark) — Elytron with one or more pale patches. 

— Elytra normally black with or without Metacoxal lines much less divergent in 

lighter markings. Tip of elytron pointed . 9 antenor ^f than '" mid ^- Cla f on 

protarsus sickle-shaped, with large basal 

9 — Black portion in centre of pronotum not tooth (Fig. 18) A. bakewelli (Clark) 

reaching front border 

A, interrogationis (Clark) 16 — A - femoralis complex. The species are 

best separated by characters of the 

— Black portion in centre of pronotum aedeagus and melafemur given in Figs 

reaching front border !_ 15 In addition the b i ack portion in 

.... A. hollingsworthi sp. nov. (W.A. only), thc centrc of fe pronotum does not reacn 

1A. pembertoni sp. nov. (W.A. only, the front border in A interrogationis 

female unknown), A.femoralis (Boh.) whereas it does in the other species. 

10 — Prominent cup-like tuft of long golden 

setae on mesotrochanters (Fig. 28). 

Segments of mesotarsus larger than Antip or us femoralis (Boheman, 1858) 

segments of protarsi ( Fl § s 7 ' 8 & 9 ) 

A. willyamsi sp. nov. ^ 

Number examined, 83. 

— Mesotrochanters without such a tuft of Brancucci (1984) clarified the relationships 
setae. Segments of mesotarsus smaller between this widespread and common species and 
than those of protarsus 11 A interrogationis (Clark). It can be separated 

r , , . ., from this species by characters of the aedeagus 

11 — Metafemur produced on inside near apex , . e a u • *u a i * u 

r r T - and metafemur and in having the dark patch on 

" ** the middle part of the pronotum reaching the 

— Metafemur simple 13 anterior border. In this last character it is similar 

to the other members of the A. femoralis group. It 

12 — Relatively large (>6 mm), predominantly differs from these in cha racters mentioned under 

reddish-yellow, elytron with several long ±c diffcrcnt spccics and in ust ratcd m thc figures. 

black lines. Metafemur with prominent 

narrow triangular process on inside near Distribution 

a P ex A - gUberti (Clark) Australian Capital Territory: Black 

— Predominantly dark-brown to black. Mountain, ANIC; Hackett, ANIC; Mt Coree, 
Metafemur broadly produced on inside ANIC; O'Connor, ANIC. New South Wales: 
near apex 16 Allyn River, ANIC; Galston, ANIC; Queanbeyan, 

ANIC; Sydney, MV, ANIC; Waratah, SAMA; 

13 — Larger (length > 4.5 mm). Mesotibia Williams River, ANIC. South Australia: 

strongly triangularly produced in middle Bcachport, AM; Eyre Peninsula, SAMA; 

on outside A. blakei (Clark) Kangaroo Island, SAMA; Lucindale, SAMA; Port 

— Smaller (length < 3.7 mm). Mesotibia Lincoln, AM, SAMA. Tasmania: 11 km NNW 
simple or thickened and angular but Blackland, ANIC; Eaglehawk Neck, AM; 
never as above 14 Georgetown, MV; Hobart, MV; Launceston, MV; 

" ' Liffey Valley, ANIC; Waldheim, UQIC. Victoria: 

14 Protarsi black in contrast to red-brown 4 km W. Ballan, MV; L. Barracoota, MV; Cape 
colour of rest of leg Otway, MV;10 km NW Dartmouth Dam, MV; La 

A. Jennifer ae sp. nov. Trobe, SAMA; L. Lcarmonth, ANIC;10 km NW 



FOUR NEW SPECIES OF ANT1PORUS 



37 












10 



11 



12 







15 




FIGURES 1-15. la, dorsal view of aedeagus of A. hollingsworthi; lb, lateral view of aedeagus of A. 
hollingsworlhi showing apical appendage; 2, proclaw of male A. hollingsworlhi; 3, postfemur of A. hollings- 
worthi. 4, dorsal view of aedeagus of A. interrogationis; 5, proclaw of male A. interrogationis; 6, postfemur of 
A. interrogationis. 7, dorsal view of aedeagus of A. femoralis; 8, proclaw of ma\t A. femoralis; 9, postfemur of 
A.femoralis. 10, dorsal view of aedeagus of^. pembertoni; 11, proclaw of male A, pembertoni; 12, postfemur 
of A. pembertoni. 13, dorsal view of aedeagus of A. wilsoni; 14, proclaw of male^. wilsoni; 15, postfemur of.4. 
wilsoni. 



38 



C. H. S. WATTS 



Lexton, MV; Montmorency, SAMA; Mt Buffalo, 
MV; Mudgee, ANIC; Myrtleford, MV; Oakleigh, 
MV; Reservoir, MV; Werribee, MV. Western 
Australia: 9 mi NE by E Esperance, ANIC; 
Geraldton, MV; King George Sound, ANIC; 
Mullewa, SAMA; Ravensthorpe, ANIC; Stirling 
National Park, ANIC; Swan River, SAMA; 
Wilga, ANIC. 



Antiporus interrogationis (Clark, 1862) 
(Figs 4, 5 & 6) 

Number examined, 62. 

As pointed out by Brancucci (1984), A. 
interrogationis is clearly distinct from A. 
femoralis with which I had previously 
synonymised it (Watts 1978). Apart from the 
aedeagus (Fig. 4) and metafemur (Fig. 6), A. 
interrogationis differs from the other members of 
the A. femoralis group by the dark patch on the 
middle part of the pronotum usually not reaching 
the anterior border. 

Distribution 

Australian Capital Territory: Black 
Mountain, ANIC; Paddy's River, ANIC. New 
South Wales: 37 km E Hay, SAMA. South 
Australia: Naracoorte, UQIC. Victoria: 4 km W 
Ballan, MV; Bright, SAMA, MV, AM; 
Buninyong, MV; Delatite, MV; Delley's Dell 
Grampians, SAMA; Dividing Range, SAMA; 
Eltham, MV; Glen Valley, MV; Hamilton, MV; 
L. Purrumbete, MV; L. Wendouree, MV; Linga, 
MV; Melbourne, ANIC, MV; Merrimans Creek, 
MV; Mitta Mitta River, MV; Montmorency, 
SAMA; Mt Buffalo, SAMA; Nelson, SAMA; 
Noorinbee North, MV; Six Mile Creek 
Dartmouth, MV; 8 km NE Toolangi, MV; 
Warburton, MV; Werribee, MV; Yarra River, 
MV; Yarrawonga, MV. 



Antiporus jenniferae sp. nov. 

(Figs. 25, 26 & 27) 

Description (number examined 63). 

Length 3. 4-3. 6mm. Oblong-oval, convex, 
widest behind middle, elytron somewhat elongate 
posteriorly, tip sharp. Reddish yellow, portions of 
elytra a bit darker, sutural lines narrowly darker 
and bordered with pale strip, apical portions 
lighter; protarsi darker almost black in some 
specimens. Strongly, densely, and evenly 
punctured throughout. Pronotum and elytron 



narrowly margined, elytron moderately serrate 
towards apex, except for short distance near tip. 
Apical segments of both maxillary and labial palpi 
weakly bifid at tips. Prothoracic process narrowly 
lanceolate, rounded, almost keeled in cross 
section, slightly narrowed between procoxae. 
Metacoxal lines raised, moderately separated, 
diverging slightly posteriorly, widening to about 
twice their narrowest width anteriorly. Some long 
setae arising from pit in centre of sternite numbers 
three and four. A line of long setae towards sides 
of elytron. 

Male: Pro- and mesotarsi moderately expanded, 
first and second segments as long as wide, claw 
on protarsus thickened, strongly bent near base, 
abruptly narrowing to sharp point at apex, with 
large basal tooth. Mesotibia robust, broadly but 
weakly indented on inner side in middle. Seta tufts 
on mesotrochantcrs somewhat thicker than on 
female. 

Female: Mesotarsi a little expanded, protarsi 
less so, Protarsus with two simple claws. 

Remarks 

A. jenniferae can be distinguished from all 
other Antiporus by its relatively small size, and its 
black protarsi. It appears closest to A. simplex and 
A. bakewelli. From A. simplex it differs by its 
black protarsi, elytral colour pattern which 
although less marked than in A. bakewelli is 
clearly present, the aedeagus having a broader tip 
and widening slightly in the middle compared 
with the more parallel-sided aedeagus in A. 
simplex and the spine at the base of the claw on 
the male protarsi being larger than in A. simplex. 
Based on the small numbers of specimens of both 
species available it appears to be a little larger. 
From A. bakewelli it differs in its black protarsi, 
less marked and more diffuse elytral colour 
pattern, the aedeagus with a broader tip, and the 
claw on the male protarsi being straightcr in 
comparison with the smoothly sickle-shaped claw 
of A. bakewelli. 

Distribution 

Most specimens are from Cape York Peninsula, 
but it is also known from Adelaide River, N.T. (in 
BMNH) and Synnot Creek in northern W.A. (in 
ANIC). 

Types 

Holotype male: "25K. N. Coen Qld. 29/9/84 C. 
Watts" in SAMA. 

Paratypes: 1, "12.40S 142°40E Qld Batavia 
Downs Hmsd. 17-23 Jun. 1992 T.A. Weir, at 



FOUR NEW SPECIES OF ANTIPORUS 



39 




A 16 



* * 




17 



18 




v~ 



I I 



19 




20 



21 




22 




23 



24 




■; y 




nh 



25 




26 



27 




FIGURES 16-27. 16 & 17, dorsal and lateral view of aedeagus of A. bakewelli; 18, lateral view of male^ 
hakewelli proclaw. 19 & 20, dorsal and lateral view of aedeagus of ,4. simplex; 21, lateral view of male A. 
simplex proclaw. 22 & 23, dorsal and lateral view of aedeagus of ,4. willyamsi; 24, lateral view of male A. 
willyamsi proclaw. 25 & 26, dorsal and lateral view of aedeagus of A. jenniferae; 27, lateral view of A. 
jenniferae proclaw. 



40 



C. H. S. WATTS 



light", in ANIC; 2, "12.40S 142.40E Batavia 
Downs Qld 03-10 Mar 1993 at light, I. 
Cunningham", in ANIC; 1, "16.318 126. IE 
CALM site 25/1 Synnot Ck W.A. 17-20 June 
1988 T.A. Weir", in ANIC; 1 1 "25k N. Coen Qld 
29/9/85 C. Watts", in SAMA; 1, "24M.S. 
Musgrave N.Q. 20.5.72 J.C. Brooks at light", in 
ANIC; 1, "13.34S 142.32 E Qld, 17 km N.W. by 
W. of Rokeby (Vardons Lagoon) 27 Oct. 1992, T. 
Weir, P. Zborowski, Small pool with debris", in 
ANIC; 56, "Qld Mt. Molloy 2 km S. 30/3/96, C. 
Watts", in SAMA. 

Antiporus pembertoni sp. nov. 

(Figs 10, 11 & 12) 

Description (number examined 1). 

Length 4.6mm. Oblong oval, dark red brown - 
black, front of head, sides of pronotum broadly 
and sides of elytron narrowly but diffusely light- 
testaceous. Ventral surface testaceous, sides of 
meso and metasterna darker, apical tips of 
metatibiae darker. Dorsal surface rather finely 
punctured, stronger laterally, punctures on head a 
little smaller than eye facets, punctures at rear of 
pronotum towards sides and on adjacent areas of 
elytra tending to join in roughly longitudinal lines. 
Ventral surface much more strongly punctured, 
strongly rugose-punctate laterally. Pronotum 
narrowly but clearly margined, elytron weakly so. 
Prothoracic process narrow, strongly raised, sides 
sub-parallel, bluntly tipped. Metacoxal lines well 
separated, sub-parallel in posterior third and 
anterior quarter, diverging in between so that 
anteriorly about twice the distance apart as 
posteriorly, area between coxal lines and forward 
onto mesosterum depressed. 

Male: Protarsi moderately expanded, protarsal 
claw large, slender, with well developed slender 
basal tooth. Mesotibia weakly indented on inner 
margin towards apex. Metafemur broadly 
expanded on inner edge at apex, some strong 
punctures and weak longitudinal ridging on 
expanded area. 

Female: Unknown 

Remarks 

More weakly punctured than the other species 
in the A. femoralis complex, with the large 
punctures along the front of the pronotum distinct 
and more than twice the size of others on the 
pronotum. Characters of the male aedeagus and 
metafemur are diagnostic. Known only from a 
single specimen I collected in a small stream in 
cleared land near Pemberton. 



Distribution 

Known only from unique type from near 
Pemberton, S.W. Australia. 

Type 

Holotype male: "W. Aust. 15 km N.W. 
Pemberton, 17 May 1987, C. Watts" in SAMA, 



Antiporus hollingsworthi sp. nov. 
(Figs 1,1a, 2, & 3) 

Description (number examined 15). 

Length 4.1^. 6mm. Oblong oval, convex. Dark 
red-brown, appendages lighter. Strongly evenly 
and densely punctate throughout, punctures 
smaller on head than elytra, punctures at rear of 
pronotum towards sides and on adjacent areas of 
elytra tending to join in linear longitudinal lines, 
punctures towards sides of metacoxae and 
sternites and on elytral epipleura very close 
together and tending to coalesce. Pronotum and 
elytra narrowly margined except for short distance 
at tips of elytra, lacking serration, sides of elytra 
before apex appear weakly and broadly flanged 
from some angles. Prothoracic process narrow, 
blunt, strongly carinate. Metacoxal lines sub- 
parallel in anterior and posterior third, rapidly 
diverging in middle. 

Male: Pro- and mesotarsi moderately expanded. 
First and second segments wider than long. Claw 
on protarsus strongly bent near base, straight with 
parallel sides in middle, rapidly narrowing at apex 
basal tooth subobsolete. Mesotibia a little 
thickened, weakly and broadly indented on inner 
edge in middle. Apical ventral edge of mesofemur 
expanded a little. Inner ventral edge of metafemur 
with large, broad, triangular expansion in apical 
third. Parameres robust, broad, aedeagus arrow- 
headed with thin protuberance above tip arising 
from neck of arrow. 

Female: Pro- and mesotarsi a little expanded; 
claws, meso- and metafemur and tibia simple. 

Remarks 

Antiporus hollingsworthi is a member of the A. 
femoralis group. It appears closest to A. wilsoni 
from the south-east of Australia which it 
resembles in the pronotal and elytral grooving, 
thickened male mesotibia and expanded 
metafemur. 

Antiporus hollingsworthi can be separated from 
both A. femoralis and A. interrogationis by the 
lack of pronounced paler areas on the head, 
pronotum and elytra, although some specimens of 



FOUR NEW SPECIES OF ANTIPORUS 



41 



A. hollingsworthi do have head, pronotum and 
elytral patches paler than the rest of the upper 
surface. The tendency of the punctures on the rear 
edge of the pronotum and the adjacent areas on 
the elytra to link up and form grooves is more 
pronounced than in either A. femoralis or A. 
interrogationis and the triangular expansion on 
the male metafemur is more rounded than in either 
of these species. A. femoralis and A. 
interrogationis also lack the thickened and 
indented mesotibia present in A hollingsworthi^ 
A. wilsoni and to a lesser extent in A. pembertoni. 
Antiporus hollingsworthi is more strongly 
punctured than A. pembertoni and the males have 
differently shaped metafemora (Fig. 3). It differs 
from A. wilsoni by characters of the aedeagus, by 
the indentation on the male mesotibia being more 
central, and in having a triangular rather than a 
rounded expansion to the male metafemur. 
Antiporus hollingsworthi differs from all other 
Antiporus species (and all Australian Dytiscidae) 
by the apical appendage on the aedeagus. 

Distribution 

So far A. hollingsworthi is known only from 
Perth and Carrington, W.A. and from two 
unlocalised localities in the South-west. However, 
of all the Australian regions this is the most poorly 
sampled for water beetles so it is likely to be more 
abundant than the few known specimens indicate. 

Types 

Holotype male: "W. Aust. Maidavale, 27th 
April 1990, C. Watts", in SAM A. 

Paratypes: 1 male, 7 females, same data as 
Holotype, in SAMA; 1 female "Perth 10/65 DE", 
in SAMA; 1 female "S.W.A. ?Rotnest, Edward", 
in SAMA; 1 male "JT201", in SAMA; 1 male, 1 
female "R.P. McMillan, Carrington, 19.7.53", in 
WAM. 

Etymology 

Named after Rod Hollingsworth, a strong 
supporter of Natural History at the South 
Australian Museum. 



Antiporus willy amsi sp. no v. 

(Figs 22, 23, 24 & 28) 

Description (number examined 4). 

Length 3.4-3.6 mm. Oblong-oval. Widest 
behind middle. Testaceous, head, lateral quarters 
of pronotum, patches on elytra and appendages 



lighter, metafemur and tibia tend to be a little 
darker towards their apices, lighter patches on 
elytron tending to form broad longitudinal streaks. 
Strongly, densely and evenly punctate, punctures 
on discs of pronotum and head weaker, 
particularly on head, a few scattered much smaller 
punctures on disc of pronotum and elytra. 
Pronotum narrowly but distinctly margined, elytra 
less so. Prothoracic process with central keel, 
narrow between procoxae. Metacoxal lines raised, 
sub-parallel in posterior half and anterior quarter, 
diverging in between, about twice the distance 
apart anteriorly compared with posteriorly, 
reaching mesofemur. Some long setae arising 
from pits in centre of sternites three and four, and 
a line of long setae on dorsal surface of elytron 
close to side. 

Male: Protarsi expanded, second segment 
broadest, mesotarsi strongly expanded, first and 
second segments largest, sub-equal. Mesofemur 
and mesotibia stouter than profemur and protibia. 
Protarsus with single claw, strongly bent, long and 
narrow, with well developed basal tooth and weak 
bulbous area in middle. Protrochanters with well 
marked cup-like tuft of golden setae, 
mesotrochanters with a much larger scallop- 
shaped tuft of similar setae. Metafemur stout, 
ventral inner apical region with scattered large 
punctures and about four longitudinal grooves/ 
ridges. 

Female: Protarsus with two weak claws. 
Mesotarsi moderately expanded, first and second 
segments largest, sub-equal. Mesotibia stout. 

Remarks 

The species is easily recognised by the 
spectacular development of the setae on the 
trochanters of the male which is unlike anything I 




FIGURE 28. 
willyamsi. 



Meso- and metatrochanters of A, 



42 



C. H. S. WATTS 



have seen on other beetles. The very broad 
mesotarsi in the male and the striped elytral colour 
pattern in teneral individuals are also distinctive. 

Since collecting the original specimens in 1983, 
I have revisited the locality (a deep, narrow, 
spring-fed drainage ditch in acidic soil) a number 
of times without success. Biologically the area has 
now changed considerably from a healthy habitat 
with numerous species to one that is almost 
devoid of insect life although physically little 
changed. 



Distribution 

Known only from the type locality in the south- 
east of South Australia and from Healesville, 
Victoria. 

Types 

Holotype male: "10 km S. Robe, S.A., 1/83, C. 
Watts", in SAMA. 

Paratypes: 2 females, same data as holotype, in 
SAMA; 1 female, "Healesville, V. 12/68, C. 
Watts", in SAMA. 



Checklist Of Australian Antiporus Sharp 



A. bakewelli (Clark, 1862) 
A. hlakei (Clark, 1862) 
A.femoralis (Boheman, 1858) 
A. gilberti (Clark, 1862) 
A. hollingsworthi sp. nov. 
A. Jennifer ae sp. nov. 



A. pembertoni sp. nov. 
A. simplex Watts, 1978 
A. willyamsi sp. nov. 
A. wiisoni Watts, 1978 
A. interrogationis (Clark, 



1862) 



Acknowledgments 



References 



The curators of the collections listed earlier are 
thanked for allowing me to examine specimens in their 
care. Mrs Vicki Wade typed the manuscript and Mr R. 
Gutteridge drew the illustrations. All these are thanked 
for their support and help. 



BRANCUCCI, M. 1984. Notes on some species of the 
genus Antiporus (Coleoptera: Dytiscidae). Aquatic- 
Insects 6: 149-152. 

WATTS, C. H. S. 1978. A revision of the Australian 
Dytiscidae (Coleoptera). Australian Journal of 
Zoology, Supplementary series No 57: 1-166. 



THYLACiSUS MEGiRL4.\f< A NEW SPECIES OF THYLACINE (MARSUPEAL1A: 
THYLACINIDAE) FROM THE ONGKVA LOCAL FAUNA OF CENTRAL AUSTRALIA 



PETER F. MURRAY 



MURRAY* P. F. 1997. Thyhwitws megirianr, a new species of thylacitie (Marsupialia: 
Thylaeinidae} from the Oneeva Locai Fauna oi' Central Australia. Records of the South 
Australian Atu.xeum 3G< I): 43-61 r 

Approximately 10% larger than a maximum-seized Tasmanian wolf, the laic M ioccne' early 
pliocene Thylaciniu megirinni n. sp, exhibits some similarities to the Sate Miocene thylacinid, 
T. potens Woodbwnc l9o7 arid early to mid-Miocene ^imiyaanus ificksom Muirhead and 
Archer 1590, while simultaneously expressing several derived features in common with the 
Recent ihylacLtiu. 7" cy^OLtphuius. Other ihan the presence of a tiny stylar cusp-Hlce strucuue 
distal to stylar cusp D on M\ which could be an artefact of wear, T. megiriani shows no 
defi title uniquely derived characters Lhat would exclude i\ from ancc-slry of the recently extinct 
T. cyn&cepttalus. 

Peter P. Murray, Museums and Art Galleries of the Northern Territory, PO Box 2109 Alice 
Springs, Northern Territory 0871, Austraha. Manuscript received 14 October, 1996, revised 3 
Marth. 1 997. 



Fossil vertebrates were first described from the 
Alcoota Local Fauna al Alcoota (Fig. 1), northeast 
of Alice Springs, by Woodburne (1967). The 
strati graphically superposed Qngcva Local Fauna 
contains certain taxa lhat are more derived than 
those from the nearby Alcoota Local Fauna 
(Murray, Megirian & Wells 1993, Megirlon, 
Murray & Wells 19%). Among its characteristic 
species is a zygomaturine diprotodontid, Kolopsis 
yperus Murray* Mcgirian & Wells, which is 
probably synonymous with the Chcltenhamian- 
aged Zygoma f urns gtilt Stirlon 1967. A", yp&us is 
iiiore similar lo Zygomaturus species than is the 
Akoota Local Fauna species Koi&psis torus 
Woodburne 1967. Thylacinus megiriani appears 
to be analogously derived in comparison to the 
Alcoota Local Fauna thylacinc, T. patens. 

A direct ancestor of T. cynocephatus has not 
been identified, I! rosfroiis, T. spelaean and T. 
major are considered to be synonymous with T. 
cynocephatMS (Dawson J9S2). Other thylacinids 
are considered lo be too primitive or too 
specialised (Archer 1982, Muirhead & Archer 
1990, Muirhead 1992, Wroc pcrs. com.). 
Ambiguity in the homology of the posterior stylar 
euspules on (he molars of T. cynocephcttus has 
resulted in a less than definitive resolution of late 
Tertiary thylacinid phylogcny. T. megiriani 
provides some additional: evidence pertaining to 
the homology of the cusps and some hypotheses 
of ihc phytogeny o\^ Ihe recent species of 
Thvlacinw are discussed. 



Matejuals And Methods 

As is often the case with Ongeva LF fossils, 

NTM P961S is not an ideal specimen, having 
been found in a number of pieces scattered 
throughout a hard nodule of calcareous sandstone. 
As fragments were extracted more or less 
individually, including fragments of the molar 
teeth, the specimen was glued together at ihe 
excavation silc along what appeared to be the 
likely contacts.. The fragile condition of the 
specimen dictated lhat several coals of Synocryl 
(Bcdacryl) be applied to harden and hold it 
together securely. However, this compound 
sometimes has ihe disadvantage of obscuring 
important morphological details, particularly 
when fine particles of the matrix become 
incorporated with the solution, sometimes 
suppressing surface detail and occasionally even 
mimicking small structures. 

So it was with this specimen, that certain 
features of the restoration seemed untenable, such 
as a slight overlap of thy P~- alveolus with that of 
the P 1 . As Thylacinus potcn.i has no appreciable 
diastema between these teeth, this arrangement 
appeared to be plausible, though further cleaning 
of the matrix and excess Synocryl from the 
specimen, in response to an observation by one of 
the referees, proved that it had not been restored 
corrcclly. This revelation provoked a more radical 
program of disassembly and cleaning of the 
specimen which I was initially afraid to attempt 




135°E 

FIGURE 1 . Locality map; the Dngcva LF ih located un Akoota Station, near Alice Springs Northern Territory. 



due lo its extreme fragility. The new restoration 
has greatly improved the resolution of the 

specimen, to the extent thai many of my initial 
observations can be slated more confidently; 
though as will be discussed some features of the 
specimen remain equivocal. 

As the first draft of (his paper was based on the 
original restoration, I have briefly described and 
illustrated the modifications [ made lo the 
specimen to avoid confusion with, any errant 
copies of the earlier manuscript. 1 ani extremely 
grateful to my referees fur alerting me to (he 
possibility thai the specimen might be distorted, 
and for drawing to my attention several other 
morphological features, resulting, I believe, in a 
much improved account of the species. 



Systemaiics 

Family THYLACINIDAE Bonaparte 1838 
Thyluiinus me&iritmin. sn, 

Hoiatype 
NTM P9618 (field ref. no, SQ107), left maxilla 

with P 1 , P\ M 1 " 1 . 

Type focatity 

Hill l h South Quarry, approximately 2 km 
southwest of the junction of Ongeva and Waite 
Creeks, Alcoota Station, Northern Territory, 

latitude 22 a 52'5, Longiludc, L34*2TE The Type 



THYLA ONUS MEWRIAM N .SP. 



45 




FIGURE 2. Photograph of the fcft maxilla of Thylaeinu* megiriani n. sp. (NTM P9G18); A, lateral aspect; B, 
palatal aspect. This photograph depidLs iht: field reiteration of the specimen in which the fragment containing P 1 
and P 2 had been glued approximately S.O mm posterior 10 its Lorrea position, lcadiri|f to the initial impression rhat 
the posterior root of P ] was adjacent to, or sightly overlapped thai of P*. Note- also thai the M'istwistcd medially 
(H) and is nearly a centimetre out of alignment with MP. 



was recovered from a sandy siltstone channel 

deposit in the Watte Formation, approximately 
10m above the fossitiferous lacustrine scdimenls 
containing the Alcoola Local Fauna (Murray, 
NU'iiiruin &. WdLs H'93. Megirian, Murray & 
Wells 1996), (Fig, I). 

Fauna 
Ongeva Local Fauna (Murray et at. 19931. 

Rock unit and age 

Waire Formation, Cheltenhamian equivalent, 
laic Miocene-?cailv Pliocene. 



Specific diagnosis 

A Eargc, long-snouted thylacinid, equal to, or 
larger than T- cynocephahs bul less massive than 
r. p&tens; much larger than N. dicks on? 
(Muirhead and Archer 1990) and T. macknesxi 
(Muirhead 3992). P 1-2 shorter and narrower than 
in T. potem, P in line with P 2 \ contrasting with 
T. poterts in which P 1 is obliquely oriented and 
situated medial to the midline of the canine 
alveolus, P 5 large as in T. patens. Premolar 
diaslcmata longer than in T. potens and in 
Ntmhacinus dicksoni? more comparable to T. 
cynocephalus. "M 1 J longer and narrower than in 




B 



FIGURE 3. Outlines depicting changes made to the initial restoration of the specimen; solid outline represents the 
new restoration; compare with Fig. 2. A, lateral aspect; B, palatal aspect. The specimen was taken apart at its 
primary joins, cleaned of excess Synocryl and glue, and reassembled. The anterior fragment of the rostrum was 
carefully cleaned revealing a labial expansion representing the anterior alveolus of P 3 . It was glued in place at what 
is probably the minimum distance from P 3 , as no definite contact could be identified. Removal of additional matrix 
from a fragment of palate that previously did not seem to fit anywhere on the specimen, revealed the inner lining 
of the anterior P 3 root and was glued in position. The M 3 was twisted out of alignment with the molar row by about 
15°. This region of the specimen, which consisted primarily of impacted matrix and bone fragments was 
embedded in modelling clay, then softened in acetone and pushed gradually back into its correct position. The 
area above and internal to the M 3 was then reinforced with dental plaster. These changes resulted in a significant 
transformation of the occlusal outline of the specimen, which subsequently lost some of its resemblances to T. 
potens. 



THYLACINUS MEGIRIANI N.SP. 



47 




1 j 



ALV/C 










ALV/M4 



B 

FIGURE 4, Drawing of corrected restoration of T. megiriani n. sp. (NTM P9618) left maxilla; A, lateral aspect; 
B, palatal aspect. Abbreviations: AC, precingulum; ALV/, alveolus; B, stylar cusp B; C, canine; D, stylar cusp 
D; E, stylar cusp E (brackets [E] indicate doubtful, or if worn, the approximate position of a structure); IEM, 
interdental embrasure; IOF, infraorbital foramen; MI. ..3, molars; ME, metacone; MJS, maxillojugal suture; 
PI ...3, premolars; PA, paracone; PC, postcingulum. 



T. potens though relatively shorter in proportion to 
their width than in T. cynocephalus. Agrees 
meristically with T. cynocephalus in that M 3 is 
slightly longer than M 2 , differing from T. potens 
and Nimbacinus dicksoni in which M 2 is slightly 
longer than M 3 . Length of molars exceeds anterior 
width from protocone to parastyle; stylar shelf 



considerably narrower than in T. potens; 
metastylar spur much larger than parastylar corner 
on M\ contrasting with T. potens in which they 
are more nearly equal-sized; stylar cusp D present 
on M 1- " 3 as in Nimbacinus dicksoni and probably 
as in T, potens; rudimentary stylar cusp E present 
on M 2 , absent in T. potens and in T. cynocephalus 



48 



P. F. MURRAY 



but present on M 1 2 in Nimbacinus dicksoni. 
Rudimentary anterior cingulum present on M 2 in 
contrast to Nimbacinus dicksoni in which it is 
well-developed on M'~\ T. potens in which it is 
present on M 2 ~ 3 and T. macknessi in which it is 
present on M 1 , the only upper molar known for 
that species. A small precingulum is present on 
M 2 of T. megiriani. Ectoflex of M 2 ~ 3 less 
pronounced than in T. potens but greater than in 
T. cynocephalus. Paraconal reduction on M'~ 3 
comparable to that of T. cynocephalus; protocones 
on M 23 reduced, similar to T. cynocephalus. 
Infraorbital foramen opens above posterior half of 
M 2 as in T. cynocephalus, unlike T. potens in 
which it opens above M 1 ; maxillojugal suture 
nearly reaches the margin of infraorbital foramen, 
approaching the condition in T. cynocephalus and 
in contrast with Nimbacinus dicksoni in which it 
terminates considerably short of the margin of the 
foramen. 

Etymology 

It is my privilege to name this species after Dirk 
Megirian, Geologist, Museums and Art Galleries 
of the Northern Territory, Darwin, NT; who 
discovered and meticulously extracted the 
specimen. 

Description 
Maxilla 

Thylacinus megiriani n. sp. consists of a 
maxilla that was recovered from nodular 
calcareous sandstone matrix in about a dozen 
pieces (Figs 2-4, 7). All but a few small 
fragments have been assembled into the left side 
of the animal's snout which includes the base of 
the zygomatic arch to just below the orbit and the 
infraorbital foramen and canal, to the posterior 
margin of the canine alveolus. The full extent of 
the missing jugal is clearly inscribed by its suture. 
In palatal aspect the maxilla is shallowly concave 
on the labial side and the snout was constricted 
behind P ! much as in T. cynocephalus. The base 
of the zygomatic arch is convex and marked by a 
pair of low, irregular crests. The higher one, 
corresponding to the maxillojugal suture, extends 
obliquely upwards to immediately behind the 
opening of the infraorbital foramen. 

The infraorbital foramen is a large, 
approximately 9.0 mm by 10.5 mm opening 
situated 21.0 mm above the approximate middle 
of the posterior half of M 2 (Figs 4, 7). Its position 
in T. megiriani is similar to that of T. 
cynocephalus and differs from the more anteriorly 
situated opening in T. potens, above M 1 . Anterior 



to the infraorbital foramen, a shallow, oval fossa 
extends to above P 3 , anterior to which, the lateral 
margin of the rostrum becomes convex. 

A fragment of the maxillary palate extending 
from P 1 to P 2 is broken at the median suture, A 
prominent median palatal ridge is apparent, 
parallel to which runs a deep, 5,0 mm wide 
palatal groove. The palatal width at between the 
posterior roots of P 1 would have been about 24.0 
mm, approximately 5.0 mm wider than in T. 
potens. The palate is narrower at this point in T, 
potens because the posterior roots of P 1 are angled 
inwards and are also larger, whereas they are 
aligned with the median base of the canine 
anteriorly and the P 2 posteriorly in T. megiriani 
and T. cynocephalus (Figs 2-5). 

Three additional fragments of the palate can be 
approximated to adjacent structures medial to P 3 - 
M 1 (Figs 3, 4) as additional removal of matrix and 
Synocryl revealed the inner margin of the P 3 
alveolus on the largest of the fragments. The 
premolar diastemata are similar to those of T. 
potens in that the P 1 and the P 2 are widely 
separated, whereas the diastema between P 2 and 
P 3 is shorter (Figs 5, 6). In the original restoration 
of T. megiriani (Figs 2, 3) it appeared that the 
posterior root of P 2 might have overlapped the 
labial side of the anterior root of P 3 by about 3.0 
mm. The specimen is broken at this point and the 
contacts were not quite congruent, causing the 
anterior part of the snout to twist out of alignment. 
This contact was taken apart and cleaned, 
revealing more of the P 2 alveolus and a straight 
section of diastema, indicating that a P 2 /P 3 
diastema of at least 5.0 mm is actually present 
(Fig. 6). The premolars of T. megiriani are large 
and posteriorly directed, though in proportion to 
the molars, the First and second premolar crowns 
and their alveoli are absolutely and relatively 
smaller than those of T. potens (Figs 2-6, Table 
1) but the P 3 crown, though not the alveolus, is 
similar in size to that of T. potens. The lengths of 
the premolar alveoli of T. megiriani are as 
follows: P 1 , 10.5 mm; P 2 , 15.0 mm; P 3 , 18.5 mm. 
Corresponding measurements of T. potens are: P ! , 
-15 mm;P 2 , 17.5 mm; P 3 , 20.5 mm (Fig. 6). 

Reconstruction 

The reconstructed snout of T. megiriani is 
compared with that of T. potens and T. 
cynocephalus in Fig. 5. This reconstruction, based 
on modifications of the original restoration of the 
specimen (Fig. 3) indicates that although it is 
comparable in size and robustness to T. potens, its 
shape is more similar to that of T. cynocephalus 






THYLACINUS MEGIRIANIN. SP. 



49 





10 20 30 40 50 
l I I 




FIGURE 5. Reconstruction of the rostrum of T. megiriani n. sp. for comparison with those of T. potens and T, 
cynocephalus, drawn to scale. Comparative lengths of the premolar alveoli are indicated by brackets. T. megiriani 
n. sp. is approximately the same size as T. potens, both species being considerably larger and more robust than 
the Recent Tasmanian Wo\f,Thylacinus cynocephalus. T. megiriani differs from T. potens in having a wider, less 
constricted palate at the level of P 1 , in its alignment of the premolars, and in having smaller P'~ 2 alveoli and longer 
P^diastemata, all features shared with T, cynocephalus. Distinctive features of the rostrum and palate of T. potens 
include the large size and oblique emplacement of P 1 , distinct narrowing of palate at the level of P 2 , separate rather 
than confluent P' and canine alveoli, emplacement of the P' internal to the canine base, the incisive foramina are 
formed within a deep, oval pit, (apparently absent in T. megiriani) and the palatal fenestrae are small. 



50 



P. F. MURRAY 



15 6.2 17.5 2.0 20 

j — i i 




FIGURE 6. Diagram comparing proportional features of the cheek tooth rows of A, Thylacinus potens, B, T. 
megiriani n. sp. andC, Thylacinus cynocephalus, all drawn to the same length from anterior P l to the metastylar 
tip of M 3 , measurements in millimetres. Refer to scale and actual measurements given above, as brackets show 
relative rather than scaled dimensions of the alveoli and the length of the metastylar spur from ectoflexus to tip. 
The P 3 alveolus in?", potens, damaged on both sides, is a composite restoration; note the relatively and absolutely 
longer diastema between P 1 and P 2 in T. megiriani, suggesting that the P 2 /P 3 diastema was probably slightly 
longer than restored. The two pieces were glued at this point because no additional surface was available to 
provide a secure union. Observe that the diastemata in T. cynocephalus are approximately equal lengths. 



in being more drawn out in the premolar region 
and in the premolar rows lying essentially parallel 
to each other, rather than converging at the level 
of P 2 . As the restored P 2 /P 3 diastema is a minimum 
dimension, the snout of T. megihani may actually 
have been slightly longer than depicted. The 
distinctive median pit for the incisive foramina in 
T. potens appears to have been absent in T. 
megiriani. Note also that the P 1 alveolus is 
confluent with the canine alveolus in T. 
cynocephalus and T. megiriani, whereas in T. 



potens they are separated by a bony ridge. 
Longitudinal palatal crests define the lateral 
margins of the palatine fenestrae in T. potens. 
Similar crests in T. megiriani are situated further 
apart, indicating that the palatal fenestrae were 
probably wider. 

Premolars 

P 1 is a small two-rooted premolar closely 
resembling that of T. cynocephalus. The crown is 
8.5 mm long and 4.5 mm wide. The anterior 



THYLACINUS MEGIRIANI N.SP. 



51 



B 



D 




FIGURE 7. Diagram comparing the position of the infraorbital foramen relative to interproximal MVM 2 and its 
relationship to the maxillojugal suture in A, Thylacinus cynocephalus; B, Thylacinus megiriani n. sp.; C, 
Nimbacinus dicksoni (NTM P907-3) and D, Thylacinus potens. In this series, the infraorbital foramen in 
Thylacinus potens is positioned more anteriorly than in the other species under consideration. A more anteriorly 
situated infraorbital foramen is a primitive feature in didelphoids, dasyurids and probably thylacinids. However, 
the infraorbital foramen in Nimbacinus is situated more posteriorly than in T, potens, an otherwise much more 
derived species. Note that the maxillojugal suture lies well posterior to the foramen in Nimbacinus, whereas it 
reaches or nearly reaches the posterior margin of the foramen in T. potens, as it does in T megiriani and T. 
cynocephalus. This relationship is a derived feature, suggesting that the forward position of the foramen in T. 
potens is a secondary, rather than a primary condition, indicative of a derived state. Abbreviations: IOF, 
infraorbital foramen; LJS, lacrimojugal suture; MJS, maxillojugal suture. 



52 



P. F. MURJRAY 



margin of the crown commences with an enamel 
bulge about 3.0 mm above the alveolus. The 
posterior profile is steeper, longer and slightly 
concave, terminating in an enamel thickening 1.0 
mm above the alveolus (Figs 2-4, Table 1) 

P 2 is represented by its anterior root and 
posterior alveolus. Its alveolus is about 15.0 mm 



long, 2.5 mm shorter than that of T. potens. The 
posterior alveolus is slightly larger in diameter 
than the anterior one. 

P 3 is considerably the largest premolar. The 
length of the crown at the base of the enamel is 
about 16.5 mm. The circular, heavily worn 
posterobasal cuspule is 8.5 mm transversely, 




FIGURE 8. Photographs of the left M 1 " 3 ofThylacinus megiriani n. sp.; A, M 1 " 3 , taken before correction of the 
position of M 3 on the specimen; B, enlargement of M 3 showing stylar cusp D and possible aberrant stylar cusp 
E, which may actually be a peculiar wear artefact; C, paste-up showing the approximately correct alignment of 
the M 2 metastyle with the parastylar corner of M 3 . Because of its dislocation, the occlusal surface of M 3 is tilted 
more lingually than those of M 1-2 , revealing the entire buccal side of the crown and resulting in the misleading 
impression that the metacone is situated more posterolingually than it actually is. Note the faint, postcingulum- 
like structure on M\ the small precingulum on M 2 and absence of same on M 3 ; The remnant stylar cusp E on M 2 
is indistinct in A, but is faintly visible in C. 



THYLACINVS MEGIRIANI N.SP. 



53 



while the width across the anterior enamelled part 
of the crown immediately above the posterobasal 
cuspule is 7.0 mm. The crown is heavily worn on 
the anterior and posterior surfaces where distinct 
wear facets result in a steep, slightly biconcave 
profile. 

Molars. 

M 1 is heavily worn (Figs 2, 4, 8A, 9C). Both 
the paracone and metacone have been ground 
flush with the stylar shelf. The remnant base of 
the paracone indicates that it was probably 
reduced relative to the metacone. A remnant V- 
shaped 'wall' of vertical facets above the 
premetacrista and centrocrista are faintly visible 
on the specimen. Stylar cusp D, situated 
immediately posterior to the labial cleft, is the 
highest relief on the worn occlusal surface. Stylar 
cusp E is not apparent. The protocone is round 
and slightly constricted near its base. A faint 
cingulum-Iike crest extends from a low bulge 
located about mid-way between the base of the 
protocone and the metastylar tip, though its exact 
form and extent is obscured by a layer of calcite. 
The length of the tooth along the stylar crest is 
14.7 mm. Its transverse width from the protocone 
to the parastyle is 12.3 mm and its posterior width 
from protocone to metastyle is 16.0 mm. The M' 
of T. megiriani is similar, but relatively longer 
than the equivalent tooth in T. potens (Fig. 9B) 
differing from that of N, dicksoni (Muirhead & 
Archer 1990) in its reduced stylar shelf, reduced 
paracone and absence of an anterior cingulum 
(Fig. 9A) and from that of T, macknessi 
(Muirhead 1992) in its retention of a distinct stylar 
shelf remnant with a large stylar cusp D, in the 
reduction of the paracone, in the absence of an 
anterior cingulum, and in having a steep facet or 
'wall' above the paracone and metacone bases 
(Fig. 9D). 

M 2 is considerably larger than M 1 and broader 
transversely, though slightly shorter across the 
stylar wings than M 3 (Figs 2, 4, 8A, C, 9C; Table 
1). Its length from parastyle to metastyle is 16.8 
mm. Its anterior transverse dimension from 
protocone to parastyle is 15.0 mm and its posterior 
transverse dimension from protocone to metastyle 
is 19.5 mm. The parastylar corner is small 
compared to the metastylar corner. The smaller, 
lower and narrower paracone is cleanly divided 
from the metacone by a mesial continuation of the 
labial cleft. Approximately 3.0 mm distal to the 
labial cleft and 2.0 mm labiad of the metacone is 
a prominent stylar cusp D. It is connected to the 
metacone by a short crest. Separated by a shallow 



labial groove from stylar cusp D is a second, much 
smaller enamel expansion situated about 3.0 mm 
anterior the metastyle, which appears to represent 
a remnant stylar cusp E. Although not prominent, 
the tiny cusp has a small wear facet and a labial 
bulge on the stylar shelf is evident. The 
anterotingual surface between the protocone and 
parastyle is distinctly convex and emarginated by 
a short, though strong precingulum. The protocone 
is smaller than on M 1 and is more U-shaped than 
rounded. Remnants of the pre-and post- 
protocristae extend from either side of the apex of 
the protocone to the bases of the paracone and 
metacone respectively. A small, but distinct lobe 
is situated immediately above the dentine-enamel 
junction, approximately midway between the 
metastyle and the protocone. In overall shape, the 
M 2 of T. megiriani is structurally intermediate 
between Nimbacinus dicksoni and T. potens, but 
differs from both in having a much reduced 
parastylar wing, reduced paracone and relatively 
reduced height of the stylar shelf. There is no 
indication of stylar cusp E on T. potens, but the 
cusp is well -developed, though small, in 
Nimbacinus dicksoni, 

M 3 is slightly longer and more slender across 
the metastyle and protocone than M 2 . The 
anterolingual and posterolingual emarginations 
are reduced and the precingulum is rudimentary 
(Figs 2, 4, 8B, C, 9C; Table 1). The parastylar 
spur is smaller in proportion to its metastylar 
component than in the previous molar, though the 
ectoflex is more pronounced on M 3 than on M 2 . 
The length of the crown from parastyle to 
metastyle is 17.4 mm. Its anterior transverse 
dimension is 16.1 mm and its posterior transverse 
dimension is 20.3 mm. Though heavily worn, it is 
apparent that the paracone was originally low, 
narrow and much smaller than the metacone, 
which in turn, is high, transversely elongated and 
anteroposteriorly narrow. As in Thylacinus 
cynocephalus, the preparacrista is short and the 
internal angle formed by the preparacrista and 
postmetacrista is more obtuse than in T. potens. 
Prominent pre- and postprotocristae meet at the 
apex of the narrow, V-shaped protocone. Both 
crests extend to near the cusps of the paracone 
and metacone accentuating a furrow-like occlusal 
fossa between them. Stylar cusp D is situated -3.0 
mm posterior to the labial cleft in the same 
position relative to the posterolabial base of the 
metacone as in M 2 . It is connected to the metacone 
by a low crest. A possible rudiment of stylar cusp 
E is situated about 4.0 mm anterior to the 
metastyle. Though small, it is more obvious than 



54 



P. F. MURRAY 



C if D [ 




12 3 4 5 

_L_I l_l 

MM 



C CCR 

B PPC PRMC 




12 3 4 5 

ME I I I I LJ 



MM 




LLLL 
MM 



POPC PRMC 



POPC / PRMC 
CCR 



FIGURE 9. Comparison of M 1 " 3 of T. megirianin. sp. with thylacinid species: A, Nimbacinus dicksoni (NTM 
P907-3); B, Thylacinus potens; C, Thylacinus megiriani; D, Thylacinus macknessi (M 1 reversed for 
comparison); E, Thylacinus cynocephalus. Abbreviations: AC, precinguium; B, stylar cusp B; C, stylar cusp 
C; CCR, centrocrista;D, stylar cusp D; E, stylar cusp E;ef,ectoflexus;gv, natural orwear groove in stylar shelf; 
MCL, metaconule; ME, metacone; MS, tip of metastyle; PA, paracone; PC, postcingulum; PCL, paraconule; 
PMC, postmetacrista; POPC, postparacrista; PR, protocone; PRMC, premetacrista; PSC, crest connecting 
metacone and stylar cusp D. 



THYLACINVS MEGIRIANI N.SP. 



55 



TABLE 1. Measurements of cheek teeth of Thylacinus megiriani compared with those of T. potens and T. 
cynocephalus. 







T. megiriani 


T. potens 


T . potens 


T. cynocephalus 






NTMP9618 


CPC6746 


UCMP 66971 


sample means 
(Woodbume 1967) 




L 


8.5 


— _ 


— 


6.2 


P 1 


W 


4.5 


— 


— 


3.3 




L 


<12.0 


12.4 


— 


8.3 


P 2 


W 


<5.0 


5.5 


— 


3.8 




L 


16.5 


16.0 


— 


10.6 


P 3 


W 


8.5 


8.8 


— 


5.0 




L 


14.7 


12.0 


— 


10.9 


M 1 


W, 


12.3 


12.8 


— 


11.5 




w 2 


16.0 


13.5 


— 


11.5 




L 


16.8 


15.7 


— 


13.2 


M 2 


w i 


15.0 


13.9 


— 


10.0 




w 2 


19.5 


17.5 


— 


15.0 




L 


17.4 


15.2 


14.6 


15.1 


M 3 


w t 


16.1 


15.9 


14.7 


12.0 




w 2 


20.3 


19.0 


17.5 


17.8 



the structure in the equivalent position on M 2 . It 
consists of a nearly circular raised enamel ridge 
with an oval wear facet or pit in the centre (Fig. 8 
B, C). After long deliberation of the structure 
under the microscope, I have concluded that it 
could represent a freakish wear pattern, but that it 
also indicates that thicker, more obdurate enamel 
is located where stylar cusp E would be 
anticipated. The enamel on the molars of this 
specimen is uniformly quite thick and it may be 
the case that some of these small structures, 
including the postcingulum-like crests on M 12 
might be the result of an exceptionally active 
enamel organ. A -3.0 mm wide attrition furrow 
between stylar cusp D and the equivocal cusp E 
extends vertically some 4.0 mm up the labial side 
of the stylar crest. 

Meristic gradients of the molars are as follows: 
metastyle to parastyle length, M'<M 2 <M 3 ; 
ectoflex, M'<M 2 <M 3 ; Protocone base diameter, 
M'>M 2 >M 3 ; Paraconc, M l >M 2 >M 3 ; Metacone 
diameter, M ! ?M 2 >M 3 ; Metacone height, 
M l ?M 2 <M 3 ; Parastyle length, M'>M 2 >M 3 ; 
Metastyle length, M'<M 2 <M 3 ; Precingulum, M 1 
nil M 2 present M 3 nil; Stylar cusp D, M'>M 2 >M 3 ; 
Stylar cusp E, ? M 1 , weakly expressed on M 2 , ? 
M 3 ; ?Postcingulum length, M'>M 2 nil on M 3 . 



Discussion 

The similarity in size and robusticity of T. 
megiriani to T. potens contributed to some of the 
errors in the initial restoration and interpretation 
of the fragmentary specimen. The new restoration 
of the fossil indicates that T. megiriani was a 
long-snouted species, proportionally more similar 
to T. cynocephalus than to T. potens. The length 
of the diastema between P 2 and P 3 is a minimum 
estimation, as no definite contact between the two 
fragments of the snout could be identified. The 
posterior margin of the fragment containing P 2 
shows a definite lateral expansion for the anterior 
root of P 3 , but the actual alveolar margin and 
internal lining of compact bone is absent (Fig. 3). 
Consequently, Thylacinus potens appears to have 
undergone proportional changes in the rostrum, 
possibly a forward adjustment of the zygomatic 
root to shift the line of action of the masseter 
muscle more anteriorly. Apparently related to 
differences in the proportions of the snout is the 
position of the infraorbital foramen in T. potens. 
In that species the foramen is situated more 
anteriorly than in Nimbacinus dicksoni, yet the 
maxillojugal suture terminates close to the margin 
of the foramen as in T. megiriani and T. 



56 



P. F. MURRAY 



cynocephalus (Fig. 7). In Nimbacinus, the 
maxillojugal suture terminates a considerable 
distance posterior to the foramen. This particular 
combination of characters suggests that the 
condition in T. potens is secondary, or specialised 
rather than primitive, having occurred in 
conjunction with telescoping of the base of the 
rostrum. 

Another specialisation in T. potens, now 
apparent, is the obliquity and rather large size of 
the P l alveolus, which is part of an overall 
proportional shift of the cheek tooth row in 
relation the rostrum. In Nimbacinus dicksoni, the 
P 1 is relatively small and lies in direct line with 
P 2 -3 as in T, megiriani and T. cynocephalus 
indicating that the condition is derived. However, 
the position of the P 3 relative to the canine in T, 
potens is like that of Nimbacinus dicksoni in lying 
medial to the canine and in being separated from 
the canine alveolus by a small bony crest. These 
latter features are probably symplesiomorphic, 
whereas the relationship of the P 3 to the canine 
alveoli in T. megiriani and T. cynocephalus is 
probably synapomorphic. 

Comparison of the molar morphology among T. 
potens, T. megiriani and Nimbacinus dicksoni 
shows a similar mixture of plesiomorphic and 
derived character states (Fig. 9A-E). In some 
aspects, such as molar shape and development of 
the stylar shelf, T. megiriani resembles 
Nimbacinus dicksoni more than it does T. potens. 
In T. potens the stylar shelf is high and wide, yet 
appears to show more reduction of the stylar cusps 
than T. megiriani and certainly more reduction 
than in Nimbacinus in which the stylar cusps D 
and E are well-developed on M 1 2 , though cusp E 
is absent on M 3 . T. potens shows a much greater 
development of the ectoflex on M 2 ~ 3 than either T. 
megiriani or Nimbacinus dicksoni. These appear 
to be derived characters of the dentition of T. 
potens, which however, also shows some 
plesiomorphic states relative to T. megiriani and 
T. cynocephalus in retaining a well-developed 
precingulum on M 2 ~\ in retaining large protocone 
bases and in the length of M 2 exceeding the length 
of M 3 . T. megiriani is derived relative to 
Nimbacinus dicksoni and T. potens in M 3 being 
slightly longer than M 2 , in having more slender 
and proportionally longer metastylar spurs, in 
having reduced protocones and more reduced 
paracones, in the loss of the precingulum on M 3 
and in having a more obtuse angle between the 
preparacrista and the postmetacrista. These 
features of T. megiriani trend towards the more 
derived states found in the molars in T. 



cynocephalus. However, T. megiriani is 
plesiomorphic relative to T. potens in retaining a 
vestige of stylar cusp E on M 2 and if the structure 
on M 3 represents a stylar cusp, it is autapomorphic 
(?reversal, eg. Marshall et al. 1994) among all 
known thylacinids in that respect. 

The heavily worn condition of M' of Thylacinus 
megihani renders comparison with the unworn 
equivalent of T. macknessi (Muirhead 1992) 
somewhat less informative. Thylacinus macknessi 
possess a well-developed anterior cingulum, 
which is clearly absent in T. megiriani. In T. 
macknessi the pre-and postprotocristae do not 
ascend the paracone and metacone bases to form 
acute crests as they do in all other thylacines 
including the M 1 of T. megiriani. The stylar shelf 
is well-developed on the M 1 of T. megiriani and 
much reduced in T. macknessi. The molar is 
broken in a critical position in relation to the 
position of stylar cusp D. In T. megiriani, stylar 
cusp D is very large and lies immediately adjacent 
to the metacone. This suggests that the cusp may 
have been reduced in T. macknessi. This 
comparison agrees in ail aspects with Muirhead's 
(1992) observations that T. macknessi is more 
derived in the development of these features than 
T. cynocephalus, yet plesiomorphic in the 
retention of the anterior cingulum and 
autapomorphic in its extension from stylar cusp B 
to the base of the protocone. 

Stylar cusp homologies among thylacines were 
more ambiguous when T. potens was the only 
fossil form of any antiquity known (Archer 1982). 
The expression of the cusps in Nimbacinus 
dicksoni is now well-documented, and accords 
with other members of the family Thylacinidae 
(Muirhead & Archer 1990). in Nimbacinus 
dicksoni, stylar cusps B, D and E are present on 
M'~ 2 and stylar cusp D is present on M 3 whereas 
cusp E is absent from that tooth. In T. potens, 
stylar cusp D is definitely present on M 3 and 
almost certainly was present on M'~ 2 , though the 
crowns are damaged in the region that the cusps 
are usually situated. There is no sign of stylar cusp 
E on M 2 ~ 3 in that species. In T. megiriani, stylar 
cusp D is well-developed on M 1-3 whereas stylar 
cusp E is rudimentary on M 2 . 1 am disinclined to 
attribute any phylogenetic significance to the 
cusp-like structure in the position of stylar cusp E 
on the M 3 of T. megiriani, although its putative 
existence is duly noted should future finds serve 
to either verify or negate its presence. 

In T. cynocephalus, stylar cusps are absent on 
M 2-3 in conjunction with the reduction of the stylar 
shelf A small stylar cusp occupying the usual 



THYLACINUS MEGIR1ANI N.SP. 



57 



Ni. dicksoni T. macknessi L potens T, megiriani 
1 \ — \ \ 

2 




phalus 



FIGURE 10. Character distribution in species ofThylacinidae. 1-16 are apomorphic, 17-23 are plesiomorphic: 
1, loss of 'wall' below postparacrista and premetacrista; 2, transverse narrowing of molars and loss of sty lar cusp 
D on M 2 ~ 3 ; 3, widened, elevated stylar crest, suppression of stylar cusp E at least on M 2 ; 4, increased ectoflex; 5, 
lengthened premolar diastemata; 6, confluent P'-C diastema; 7, elongation of metastyle, reduced parastyle, 
obtuse angle between preparacrista and postmetacrista, M i longer than M 2 ; 8, reduced stylar shelf; 9, reduced 
protocone; 10, loss of precingulum and increased concavity of anterior margin of M 3 ; 1 1, reduced ectoflexus; 12, 
posterior position of infraorbital foramen above middle of M 2 ; 13, reduced paracone; 14, loss of precingulum on 
M 1 ; 15, forward extension of maxillojugal suture to posterior margin of infraorbital foramen; 16, large body size; 
17, (plesiomorphic) absence of diastema between P 2 /P 3 ; (plesiomorphic) notched precingulum on M 2 -M 3 ; 19, 
(plesiomorphic) P 1 situated lingual to canine; 20, (plesiomorphic) retention of precingulum on M 1 ; (plesiomorphic) 
21, large paracone; 22, (plesiomorphic) metaconid on M 3 ; 23 (plesiomorphic) small body size. 



topological position of stylar cusp E is present on 
M 1 . This cusp was initially identified by Archer 
(1982) as stylar cusp E. Subsequently, Muirhead 
and Archer (1990) identified the cusp as stylar 
cusp D that had become reduced and migrated 
posteriorly in conjunction with the elongation of 
the metastyle. The predisposition of the stylar 
cusps in T. megiriani supports the latter 
conclusion, in that if stylar cusp E was present, it 
was already extremely reduced relative to stylar 
cusp D. Moreover, there is no satisfactory 



explanation of the fate of stylar cusp D had cusp E 
been retained, as its amalgamation with the 
metacone, analogous to Sarcophilus (Crabb 1982) 
appears to have been highly unlikely (Stephen 
Wroe, pers. com.). 



PhyJogenetic position of T. megiriani 

The character evaluations employed here are 
based on those of Muirhead and Archer (1990). 
As the new species exhibits additional structures, 



58 



P. F. MURRAY 



the character polarities pertaining to those 
structures are based on the observations made in 
the discussion. An hypothesis of the phylogenesis 
of T. megiriani is drawn from the following 
postulations (Fig. 10): 

Thylacinus cynocephalus-T. megiriani 
synapomorphies: lengthened premolar 
diastemata, confluent canine-P' alveoli, 
posteriorly situated infraorbital foramen (in 
line with middle of posterior half of M 2 ), 
elongation and narrowing of the metastyle of 
M 3 (including M 3 longer than M 2 , reduced 
width of parastyle, obtuseness of angle of 
postmetacrista and premetacrista and 
reduction of height of stylar shelf), greatly 
reduced paracone particularly on M 2-3 , 
reduction of diameter of protocone base, loss 
of precingulum and concave profile of 
anterior surface of M 3 , reduction of ectoflexus 
on M 2 " 3 . 

Thylacinus potens-T. megiriani-T. 
cynocephalus synapomorphies; loss of 
precingulum on M 1 , forward extension of 
maxillojugal suture to margin of Infraorbital 
foramen, possibly large size. 
Thylacinus potens-Nimbacinus dicksoni 
symplesiomorphies; absence of diastema 
between P 2 and P\ presence of precingulum 
on M 2 ' 3 , P 1 situated lingual side of canine. 
Thylacinus macknessi-Nimbacinus dicksoni 
symplesiomorphies: retention of anterior 
cingulum on M 1 , large (unreduced) paracone, 
possibly small size, remnant metaconid on 
M 3 . 

Thylacinus megiriani-Nimb acinus dicksoni 
symplesiomorphy: expression of stylar cusp 
EonM 2 . 

Thylacinus megiriani apomorphies: possible 
expression of stylar cusp E on M 3 (reversal?), 
possible expression of anterobasal cuspule or 
small postcingulum on M' 2 (?neomorphic). 
Thylacinus potens apomorphies: extreme 
development of labial emargination of 
molars, stronger ectoflexus on M 2 ~\ forward 
position of infraorbital foramen, obliquity and 
large size of P 1 , enlarged trigonid and/or 
reduced talonid in lowers. 
Thylacinus macknessi apomorphies: extreme 
reduction of stylar shelf, absence of crests 
ascending lingual bases of paracone and 
metacone, postparacrista and premetacrista 
connect low in the crown basin consequently 
the lingual wall below the paracone and 
metacone is absent. 
Thylacinus cynocephalus apomorphies: 



extreme elongation of metastyle on all 
molars, extreme reduction of stylar shelf, loss 
of stylar cusp D on M 2 " 3 . 
Probably because there are so few species and 
relatively few characters due to the fragmentary 
nature of the fossils, the resulting phytogeny 
seems to be fairly straight-forward (Fig. 11). 
Among the species considered, Nimbacinus 
dicksoni is by far the least derived form. In 
contrast, T. macknessi, while retaining more 
plesiomorphic features than any of the remaining 
species, is simultaneously more specialised than 
T. cynocephalus. It is therefore the least likely 
candidate for ancestry of any of the three later 
species (T. potens, T. megiriani and T. 
cynocephalus). T. potens is also highly derived in 
its extreme thickening of the labial emargination 
of the molars, deep ectoflex, relatively narrow 
talonid and possibly in some degree of rostro- 
facial proportional sliding. This species shows 
subtle modification of the relative proportions of 
the snout that are probably secondary because the 
forward extent of the maxillojugal suture relative 
to the infraorbital foramen appears to be 
synapomorphous with T. megiriani and T. 
cynocephalus. In several respects, T. megiriani is 
the least derived of the large species in retaining a 
rudimentary stylar cusp E on M 2 , in retaining 
large stylar cusps D on M 1-3 and in retaining a 
general proportional similarity in its molars to 
those of Nimbacinus dicksoni. However, other 
characters of T. megiriani show closer 
resemblances to those of T. cynocephalus than 
observed in any of the other species. 

In general appearance, the differences between 
T. megiriani and T potens are quite subtle. Its 
large size and robustness, relatively small, broad 
molars, large P 3 , presence of stylar cusp D and 
deep maxilla all bear a close resemblance to T. 
potens, to the extent that when I first saw the 
specimen in the field, I thought it might represent 
an extreme individual variation of the latter 
species. This resemblance biased my initial 
restoration of the specimen, although in spite of 
this, its detailed differences considerably 
outweighed the introduced and genuine 
similarities. It is an important feature of the 
specimen that while the state of many of its 
characters show an unambiguous trend towards T. 
cynocephalus, it is probably further removed 
structurally from the modern species than it is 
from T. potens. A reasonable stage of evolution 
estimation for the time of separation of T. potens 
and the lineal ancestor of T megiriani would be 
in the later part of the mid-Miocene. 



THYLACINUS MEGIRJANI N.SP. 



59 



T. cynocephalus T. meairiani T. potens 
8 7 



T. mackness 



Ni. dicksoni 




FIGURE 1 1 . Subjective dendrogram depicting hypothesis of phylogenetic relationships among thylacinid species; 
1, loss of stylarcusp E on M 3 , loss of high postcingulum M'~\ plesiomorphic states of large paracone and small 
size; 2, more posterior position of infraorbital foramen; 3, reduced sty lar shelf, loss of 'wall' above postparacrista, 
centrocrista and premetacrista, extended precingulum M 1 ; 4, loss of precingulum on M 1 , forward extension of 
maxillojugal suture to margin of infraorbital foramen, large size, reduction of stylar cusp E on ?all molars; 5, 
widened, elevated labial emargination of molars, increased ectoflex on M 2-3 , loss stylar cusp E on at least M 2 ; 6, 
increased length premolar diastemata, reduced stylar shelf, reduced parastyle and paracone, lengthened metastyle, 
reduced ectoflex, more posteriorly situated infraorbital foramen; 7, possible neomorphic faint, low postcingulum 
on M 1 " 2 , possible stylar cusp E on M 3 ; 8, increased reduction of stylar shelf, increased elongation of metastyle, 
stylar cusp D confined to M ! , reduced ectoflex. 



Paleobiology and biochronology 

The Ongeva Local Fauna shows a distinct 
faunal change from the underlying Alcoota LF. A 
zygomaturine, close to, if not synonymous with 
Zygomaturus gilli is the dominant large herbivore, 
apparently replacing Plaisiodon centralis which it 
resembles somewhat in size and general 
morphology. A species of the crocodile Quinkana 
is relatively common, whereas the dominant 
Alcoota crocodilian, Bam, is absent. Though the 
sample is too small to be definitive, it would 



appear that T. megiriani had replaced the Alcoota 
LF thylacinid species, T. potens by Ongeva times. 
A new small ratite bird, possibly a dromornithid, 
is also present in the Ongeva LF (Megirian, 
Murray & Wells 1996). 

Continuity with the Alcoota LF is indicated by 
the presence of Kolopsis torus Woodburne 1 967, 
Dorcopsoides sp., Dromornis sp. cf. D. stirtoni 
and Ilbandornis sp. The Ongeva K. torus appears 
to be little changed from the Alcoota population, 
suggesting a fairly short interval between the two 
local faunas. Because the depositional 



60 



P. F. MURRAY 



circumstances of the two faunas differ, it is not 
entirely clear as to whether the samples represent 
distinct communities within a basically stable 
environment or are a reflection of more general, 
possibly fairly rapid changes in the biotic 
attributes of the region. 

Thy/acinus patens is a highly specialised 
thylacinid showing as least as much, if not more, 
derivation in its molar morphology from 
Nimbacinus dicksoni than T. megiriani. The 
increased width of the stylar area and relative 
widening of the trigonids and narrowing of the 
talonids of the lower molars, combined with its 
robust skeletal attributes, indicate that T. potens 
was capable of shearing and crushing highly 
resistant tissues, and may have been somewhat 
hyena- or Osteoborus-Yike in its habits. T. 
megiriani shows an incipient trend towards the 
extreme camassialisation that distinguishes T. 
cynocephalus; consequently it may have been 
more actively predacious in its habits than T. 
potens. It is likely that the two species would have 
considerable overlap in their habitat preference 
and behaviour. Given their close similarities and 
large size, it seems improbable that they would 
have occurred sympatrically. Such large predatory 
species usually have a considerable range, and it 
is therefore a more plausible speculation that T. 
megiriani represents a successional replacement 
of T. potens rather than an addition to the 
previously existing fauna. 



and the small -si zed, extreme shearing 
modifications of T. macknessi. The addition of 
this specimen to the small existing collection of 
fossil thylacines seems to help clarify and simplify 
our current understanding of the phylogeny of the 
group. 

Thylacinus macknessi indicates that a highly 
derived shearing complex had evolved in the early 
to mid Miocene among thylacinids, but did not 
lead to the development of the Recent thylacine 
species, T. cynocephalus, which appears to have 
originated in the late Pliocene. It is likely therefore 
that extreme camassialisation in the larger 
thylacinid species took place in the late Cainozoic, 
perhaps in response to the radiation of 
macropodine species that commenced in the early 
to mid Pliocene (Flannery 1989). A tempting 
speculation, based on the circumstantial evidence 
for periodic drought in Alcoota times (Murray & 
Megirian 1992) is that there may have been an 
abundance of carrion over a sufficient duration to 
have selected for a large mammalian scavenging 
species. Following subsequent climatic 
amelioration in the terminal Miocene, the hyena- 
like T. potens was out-competed by the more 
predacious T. megiriani. The subsequent loss of 
Thylacinus potens as a possible scavenging 
predator may have left the somewhat less 
productive scavenging niche open, recruiting a 
smaller species; namely, the ancestor of the living 
Tasmanian Devil, Sarcophilus harrisi. 



Conclusions 

As in T. potens, the new species has a large P 3 , 
retains stylar cusp D and has transversely wide 
molars. T. megiriani differs from T. potens in 
many of the features that also serve to distinguish 
the latter from T. cynocephalus. These include 
reduced ectoflex of M 2 * 3 and stylar shelf on M 3 , 
increase in the length relative to width of M 3 , 
narrow protocones, reduction of P 1-2 relative to the 
molars, alignment of the premolar row and 
infraorbital foramen opening above posterior M 2 . 
T. megiriani shows no definite structural features 
that would preclude it from ancestry of T. 
cynocephalus and shows a number of 
synapomorphous features including reduced 
paracone and lengthened postmetacrista. T. 
megiriani is less specialised within the 
morphological extremes of the large size and 
powerful shearing/crushing dentition of T. potens 



Acknowledgments 

I am indebted to Jeannette Muirhead and Alex 
Baynes for their useful comments on the first draft 
of this paper. Their observations led to the correction 
of a number of important details relating to the 
original restoration of the specimen and several key 
morphological features of which I was unaware were 
generously and courteously pointed out to me. I 
thank Dirk Megirian for his outstanding contribution 
to all aspects of the excavation, interpretation and 
documentation of the Alcoota/Ongeva Locality and, 
of course, for giving me the opportunity to describe 
and name this interesting species after him. I am very 
grateful to Ian Archibald, the NT Museum's 
Preparator/Taxidermist who photographed and 
printed the bromides under difficult circumstances. I 
also thank Rod Wells and the Flinders University 
students who participate in the Alcoota excavations 
annually. The field work at Alcoota is partially 
supported by an NT Heritage Grant. 



THYLACINUS MEGIRIAN! N.SP. 



61 



References 



ARCHER, M. 1982. Review of Miocene thylacinids 
(Thylacinidae, Marsupialia), the phylogenctic position 
of the Thylacinidae and the problem of apriorisms in 
character analysis. Pp 445-76 In 'Carnivorous 
Marsupials'. Ed. M. Archer. Royal Zoological Society 
of New South Wales: Sydney. 

CRABB, P. L., 1982. Pleistocene dasyurids 
(Marsupialia) from southwestern NewSouth Wales. 
Pp. 512-16 h 'Carnivorous Marsupials'. Ed. M. 
Archer. Royal Zoological Society of New South 
Wales: Sydney. 

DAWSON, L. 1982. Taxonomic status of fossil 
thylacines (Thy/acinus, Thylacinidae, Marsupialia) 
from Late Quaternary deposits in eastern Australia. 
Pp. 527-36 In 'Carnivorous Marsupials'. Ed. M. 
Archer. Royal Zoological Society of New South 
Wales: Sydney. 

FLANNERY, T. 1989. Phylogeny of Macropodoidea; a 
study in convergence. Pp. 447-506 In Kangaroos, 
Wallabies and Rat Kangaroos. Ed. G. Grigg, P. 
Jarman and I. Hume. Surrey Beatty and Sons and the 
Royal Zoological Society of New South Wales, 
Sydney. 

MARSHALL, C, RAFF, E. & RAFF, R. 1994. Dollo's 
law and the death and resurrection of genes. 
Proceedings of the National Academy of Science, 
USA. 91:12283-12287. 

MEGIRIAN, D., MURRAY, P. & WELLS, R. 1996. The 
Late Miocene Ongeva Local Fauna of Central 
Australia. The Beagle, Records of the Museums and 
Art Galleries of the Northern Territory. 13: 9-38. 



MUIRHEAD, J. & ARCHER, M. 1990. Nimbacinus 
dicksoni, a plesiomorphic thylacine 

(Marsupialia:Thylacinidae) from Tertiary deposits of 
Queensland and the Northern Territory. Memoirs of 
the Queensland Museum 28(1): 203-221. 

MUIRHEAD, J. 1992. A specialised thylacinid, 
Thylacinus macknessi, (Marsupialia: Thylacinidae) 
from Miocene deposits of Riversleigh, Northwestern 
Queensland. Australian Mammalogy 15: 67-76. 

MURRAY, P. & MEGIRIAN, D. 1992. Continuity and 
contrast in middle and late Miocene vertebrate 
communities from the Northern Territory. The Beagle, 
Records of the Northern Territory Museum of Arts 
and Sciences 9(1): 89-110. 

MURRAY, P., MEGIRIAN, D. & WELLS, R. 1993. 
Kolopsis yperus sp. nov. (Zygomaturinae, 
Marsupialia) from the Ongeva Local Fauna: new 
evidence for the age of the Alcoota fossil beds of 
central Australia. The Beagle, Records of the 
Northern Territory Museum of Arts and Sciences 
10(1): 155-172. 

STIRTON, R. A. 1967. New species of Zygomaturus 
and additional observations on Meniscolophus, 
Pliocene Palankarina Fauna, South Australia. Bureau 
of Mineral Resources, Geology and Geophysics, 
Australia, Bulletin 85: 129-150. 

WOODBURNE, M. O. 1967. The Alcoota Fauna, 
Central Australia: an integrated palaeontologicai and 
geological study. Bureau of Mineral Resources, 
Geology and Geophysics, Australia, Bulletin 87: 1- 
187. 



SOUTH 

AUSTRALIAN 

MUSEUM 



VOLUME 30 PART 1 
JULY 1997 
ISSN 0376-2750 



CONTENTS 



ARTICLES 

1 R. V. SOUTIICOTT 

Description of two new 



13 J. OKUNO 

A new shrimp of the genus Rhynchocinetes from the Great Australian Bight 
(Crustacea: Dccapoda: Rhynchocinetidac). 



19 S. PICHELIN 

Pomphorhynchus heronensis sp. nov. (Acanthoccphala: Pomph 
Lutjanus carponotatus (Lutjanidac) from Heron Island, Australi; 



udae) trom 



29 L. F. QUEALE 

Field Identification of female iittlc brown bats Vespadelus spp. (Chiroptera: 
Vcspertilionidae) in Souti 

35 C. H. S. WATTS 

Four new species of Antiporus Sharp (Colcoptera, Dytiscidae) from Australia, with 
notes on A. femoralis (Boh.) and A. intcrrogationis (Clark). 



43 P. F. MURRAY 

Thylacinus megiriani, a new species of thylacine (Marsupialia 
the Onseva Local Fauna of Central Australia. 



ylacinidae) trom 



Published by the South Australian Museum, 
North Terrace, Adelaide, South Australia 5000 



SOUTH 

AUSTRALIAN 

MUSEUM 



\JtnE .IT MR ^fi 



JANUARY 



A NEW SPECIES OF MULTIPHASED CORBULIPORA MACGILLIVRAY, 1895 
(BRYOZOA: CRIBRIOMORPHA) FROM SOUTHWESTERN AUSTRALIA. 



P. E. BOCK & P. L. COOK 



Summary 



A new Recent species of the cribriomorph genus Corbulipora, C. inopinata, is described from 
several localities in the western part of the Great Australian Bight. All species of Corbulipora, both 
Recent and fossil, are known to occur in several phases. The form of the subcolonies, and the 
characters of the component zooids may be very different in each phase, and subcolonies are 
capable of separate existence. C. inopinata occurs in an encrusting phase, in a flustriform, ovicellate 
phase, and a bilaminar rooted phase. All zooids have some form of cribriomorph frontal shield, 
unlike some of those of the closely related C. tubulifera. The shield has, however, different 
characters in each phase. 



A NEW SPECIES OF MULTIPHASED CORBULIPORA MACGILLIVRAY, 1895 
(BRYOZOA: CRIBRIOMORPHA) FROM SOUTHWESTERN AUSTRALIA. 



P. E. BOCK & P. L.COOK 



BOCK, P. E. & COOK, P. L. 1998. A new species of multiphased Corhulipora MacGillivray, 
1895 (Bryozoa: Cribriomorpha) from southwestern Australia. Records of the South Australian 
Museum 30(2): 63-68. 

A new Recent species of the cribriomorph genus Corbulipora, C. inopinata, is described 
from several localities in the western part of the Great Australian Bight. All species of 
Corhulipora, both Recent and fossil, are known to occur in several phases. The form of the 
subcolonies, and the characters of the component zooids may be very different in each phase, 
and subcolonies are capable of separate existence. C. inopinata occurs in an encrusting phase, 
in a flustnform, oviccllate phase, and a bilammar rooted phase. All zooids have some form of 
cribriomorph frontal shield, unlike some of those of the closely related C. tubulifera. The shield 
has, however, different characters in each phase. 

P. E. Bock, Royal Melbourne Institute of Technology, Latrobe Street, Melbourne, Victoria 
3001, and P. L. Cook, Associate, Museum of Victoria, Swanston Street, Melbourne, Victoria, 
3000. Manuscript received 2 April 1997. 



The occurrence of distinct phases of correlated 
colony growth form and zooid morphology in 
species of Corbulipora has been described in 
some detail by Bock and Cook (1994; in press). 
Essentially, the function of the phases appears to 
be the same in all species. The first, ancestrulate 
phase is minute, encrusts shells and shell 
fragments, and may even have an interstitial 
existence. It establishes the colony and results 
from the settlement and metamorphosis of a 
motile larva. The second, erect phase is cellularine 
or flustrine, and arises from stalk-like kenozooids 
and autozooids growing from the peripheral pore- 
chambers of the zooids of the primary phase. This 
phase develops ovicells and large interzooidal 
avicularia. The second phase gives rise in various 
ways to a small, bilaminar or frontally budded 
third phase, which is known, in Recent species, to 
be anchored by numerous rhizoids. As the 
ovicelled second phase tends to be thinly calcified, 
the delicate subcolonies may easily be destroyed, 
or at least detached from their origins. The 
bilaminar phase maintains the position of the 
colony and develops further ovicellate 
subcolonies, which may be able to alternate with 
it more than once (Bock & Cook in press). 

Collections of bryozoans, made by the R.V. 
Franklin, using an epibenthic sled, from localities 
in the western Great Australian Bight in July 
1995, have produced a wealth of specimens and 



species. These include subcolonies of C. 
tubulifera and of an undescribed species of 
Corbulipora, which has several distinctive 
features. 



Materials And Methods 

Specimens are stored in the Collections of the 
Museum of Victoria (MOV) and South Australian 
Museum (SAM). Specimens for scanning electron 
microscopy were coated with gold. 

The Stations from which specimens of 
Corbulipora were obtained were as follows: 

C. inopinata sp. nov. 

GAB 118 34°59'S, 1 19°00'E, 85m. Young non- 
ancestrulate colonies encrusting worn adeonid and 
lunulite colonies of bryozoans. 

GAB 098 34°39'S, 122°26'E, 156m. 1 phase-2 
subcolony with numerous avicularia. 

GAB 093 34°32'S, 122°58'E, 95m. 1 phase-1 
subcolony and 1 phase-2 subcolony with ovicells. 

GAB 083 34°21'S, 124°08'E, 180m. 2 phase-1 
subcolonies encrusting Turhtella shells. 

GAB 049 33°53*S, 125°22'E, 156m. 4 phase-2 
subcolonies, developing into phase-3 at tips, one 
repeating phase-2. 

GAB 056 33°19'S, 125°43'E, 73m. 2 large phase- 



64 



P. E. BOCK & P. L. COOK 



2 subcoionies, one with ovicells, developing from 
phase-3 subcoionies. 

GAB 045 33°25'S, H$*5WE, 143.5m. 3 small 
phase-3 subcoionies with stalks. 

GAB 020 33°20'S, 129°18'E, 157m. 9 small 
phase-2 subcoionies. 2 developing from phase-3 
subcoionies. 

GAB 013 33°06*S, 130°00'E, 101m. 2 phase-2 
subcoionies, one with ovicells, and one phase-3 
with numerous rhizoids and one phase-2 
subcolony. 

GAB 014 33°16'S, 130°00'E, 155m. 2 phase- 3 
subcoionies developing into phase-2 subcoionies, 
plus 5 isolated stalks. 

C. tuhulifera (Hincks) 

GAB 019 33°22'S, 129°19'E, 301m. 7 phase-2 
subcoionies, and 2 phase-3 subcoionies. 



Systematics 

Order Cheilostomatida Busk, 1852 

Superfamily Cribrilinoidea Hincks, 1879 

Family Cribnlinidae Hincks, 1879 

Genus Corbulipora MacGillivray, 1895 

Corbuiipora MacGillivray, 1895:60; Wass 
1975:168; Bock & Cook, 1994:33; in press. 

Corbulipora inopinata sp.nov. 

(Figs 1-6) 

Material Examined: HOLOTYPE MOV, 
F80665, GAB Stn 049, subcolony including 
phase-2 developing into phase-3 and then 
repeating phase-2. 









f. 









FIGURES 1-2. Corbulipora inopinata sp.nov. 1, subcolony showing phase-2 autozooids and two ovicelled zooids 
at the proximal end (arrowed). Intermediate zooids leading to two astogenetic generations of phase-3 zooids at the 
growing tip (GAB Stn 049) X22; 2, phase-3 subcolony with marginal pore chambers and autozooids with occluded 
orifices (GAB Stn 020) X40. 



NEW SPECIES OF MULTIPHASED CORBULIPORA 



65 




FIGURES 3-4. Corbulipora inopinata sp.nov. 3, phase-2 zooids with ovicells and simple frontal spines (GAB Stn 
049, see also Fig.l). X80; 4, phase-3 zooids with complex frontal shields (GAB Stn 049, see also Fig.l) X70. 



Paratypes: Rest of material 
L755, GAB Stn 049 part. 



including SAM 



Description 

Corbulipora with colony including three 
subcolony phases. Primary phase encrusting, 
ancestrula not seen; primary triad zooids with 
frontal shield of 16 simple spines. All zooids 
with a distinct, smooth gymnocyst, and 
communicating through small pore-chambers. 
Remaining primary-phase zooids with frontal 
shields with 16-18 spines, separated by 3-4 
series of small lacunae and with two concentric 
series of raised pelmatidia. Calcified orifice with 
3 spines, lateral pair often bifid. Second, flustrine 
phase inferred to arise from primary phase. 
Fronds developing from stalk kenozooids and 
elongated autozooids, often in quadriserial 
groups; series bifurcating to form fronds 10-12 
zooids wide and 150 astogenetic generations 
long, bifurcating up to 4 times. Autozooids with 
distinct gymnocyst and 14-16 flattened spines 



overarching the frontal membrane. Brooding 
zooids with enlarged, curved, sometimes 
medially fused oral spines and large 
hyperstomial ovicell. Ovicell frontal with median 
suture and paired entooecial areas. Aviculana 
scattered, rare in presence of ovicells. Rostrum 
elongated, narrows not raised distally; slightly 
expanded and rounded terminally, mandible 
hinged on a delicate bar, orientated distally. Tips 
of fronds with 3^4 astogenetic generations of 
zooids with intermediate morphologies leading 
to the third, bilaminar phase subcolonies. These 
form small, expanded groups of zooids with 
shields similar to phase-1 subcolonies, with two 
concentric series of raised pelmatidia. Zooids 
have a small orifice, sometimes partially 
occluded by the fusion of enlarged oral spines. 
Numerous rhizoids develop from marginal pore- 
chambers, together with stalk kenozooids and 
elongated stalk autozooids with a small opesia 
and marginal spines, which are the origin of 
repeated subcolonies of phase-2. 



66 



P. E, BOCK & P. L. COOK 





JW^ 


' /flf ' 


||| 


-f ■ 






%'■ •-:•■':- 










& 








1 e '^1 




■ 




▼ 1^^^ 




| 






I m^ 




k 


^«r 






i ^ ■.. ^*^?p 










c- ■' 



■i>-.:?-:?^$ 



Hi 



Ho, 






*'-H- 



IIP 




■-::■%.■■■ 



Ik 



If 



^ 



FIGURES 5-6. Corbulipora inopinata sp.nov. 5, phase-2 autozooids, note enlarged pair of distal spines (GAB Stn 
098) XI 00; 6, phase-2 autozooids and avicularium (GAB Stn 098) X80. 



Etymology' 

fnopinus L. - - unexpected: referring to the 
occurrence of a second Recent species of 
Corbulipora with multiphase growth. 

Remarks 

The three phases of C inopinata resemble those 
of C. tuhulifera closely, but differ in several 
respects. The most noticeable difference is in the 
occurrence of a spinous shield in the autozooids of 
the second, flustrine phase. The spines are 
flattened and generally do not fuse centrally, 
although the enlarged suboral spines of marginal 
zooids may be fused. In addition, the avicularia of 
C inopinata are much narrower, and are not 
raised distally, as are those in C. tuhulifera, and 
the mandibles are hinged on a delicate, but 
complete bar. The palate is much longer in 
proportion to the proximal gymnocyst than in C. 
tuhulifera. Other differences are small, but 
distinct and consistent. Although no ancestrula 
has been preserved, one of the small, phase- 1 
colonies encrusting Turhtella from Stn GAB 083 



possesses a post-ancestrular triad of very small 
zooids. These all have a shield of simple spines, 
very similar to the one post-ancestrular zooid of 
the triad in C, ornata (Bock & Cook, in press, 
fig. 1). Subsequent zooids have two series of 
pelmatidia, which do not develop until later in 
astogeny in C. tuhulifera. The orifices of this 
stage are also wider than those of C. tuhulifera. 
No stalk zooids have been preserved arising from 
the encrusting phase m C inopinata, but by 
analogy with C. tuhulifera, these are presumed to 
be identical with those which arise from phase-3 
bilaminar subcolonies. These consist of one or two 
pairs of kenozooids 2.5mm long, often 
accompanied or succeeded by one or more pairs of 
elongated zooids 2mm long, each with a small 
opesia surrounded by 8-12 short, simple spines. 
Thus the stalks differ from those of C. tuhulifera 
in being more robust, with more zooidal elements, 
and in the occurrence of autozooids with an 
opesia, rather than kenozooids, early in astogeny. 
The zooids of intermediate morphology at the tips 
of the fiustnne phase-2 fronds attain a complete 



NEW SPECIES OF MULTIPHASED CORBULIPORA 



67 



shield of phase-3 autozooids within 4 astogenetic 
generations. First, the flattened spines fuse 
medially, leaving a row of small lacunae. A single 
series of pelmatidia develops on the spines of the 
next generation of zooids, and a paired series, with 
3-4 lacunae, develops on the shields of 
subsequent generations. The small calcified orifice 
is complete within the next generation or two. 
Although the general appearance of the autozooids 
of the bilaminar phase is very like those of C. 
tubulifera, they have a smaller orifice. Although 
these are often partially occluded by the oral 
spines, they do not usually exhibit the series of 
changes resulting in complete closure of the 
orifice which occurs in C. tuhulifera (Wass 1975). 
In one specimen from GAB Stn 020, the spines 
are enlarged and nearly occlude the orifice (Fig. 

2). 

One of the specimens from GAB Stn 013 
illustrates the relationship and probable functions 
of phase-2 and phase-3 subcolonies particularly 
well. It consists of a small bilaminar phase-3 
subcolony comprising approximately 60 
autozooids. More than 50 rhizoids arise from the 
marginal pore-chambers, and on one face of the 
subcolony these are involved with and adhere to 
minute shell and bryozoan fragments. On the edge 
of the other face, one quadriserial stalk, 15mm 



TABLE 1. Comparative measurements in mm of 
Corbulipora inopinata sp.nov. and C. tubulifera 
(Hincks). Lz, lz length and width of autozooid; lo, width 
of orifice; Lov, lov, length and width of ovicell; Lav, lav, 
length and width of avicularium; Lp, length of 
avicularian palate. 



Character 


C. inopinata 


C. tub\ 


ulijera 


Phase 1 








(including primary 








zooids in mms) 








Lz 


0.41 -0.70 


0.45- 


-0.74 


lz 


0.35-0.50 


0.38- 


-0.50 


lo 


0.12-0.17 


0.10- 


-0.13 


Phase 2 








Lz 


0.98-1.30 


0.78- 


-1.32 


lz 


0.26-0.29 


0.25- 


-0.33 


Lov 


0.21-0.23 


0.23- 


-0.27 


lov 


0.24-0.26 


0.28- 


0.33 


Lav 


0.60 - 0.75 


0.65- 


-0.96 


lav 


0.15-0.17 


0.22 


0.26 


Lp 


0.43-0.51 


0.31 


0.35 


Phase 3 








Lz 


0.50-0.75 


0.54 


0.87 


lz 


0.37-0.50 


0.32 


-0.54 


lo 


0.09-0.10 


0.10 


0.14 



long, consisting of two generations of quadriserial 
kenozooids and 10-12 generations of elongated 
autozooids, gives rise to a phase-2 flustrine 
subcolony about 30mm long, with more than 40 
astogenetic generations. It seems almost certain 
that the one face of the bilaminar phase was 
buried in the surface sediments, whereas the 
flustrine frond extended above the surface. This 
subcolony is quite small; two flustrine subcolonies 
from Stn 056 extend up to 70mm and include 
10,000 to 12,000 zooids, many of which are 
ovicelled. These would protrude well above the 
surface of the bottom sediment, allowing the 
larvae to be released easily. 

The similarities in phase structure found in C. 
inopinata and C. tubulifera reinforce the 
inferences previously made by Bock and Cook 
(1994; in press) as to the nature and relationships 
of the known phases in C. ornata and C. 
suggerens, from the Victorian Tertiary. They also 
strongly suggest that the ovicellate phase of C, 
suggerens was a thinly calcified cellularine 
subcolony type, which has not been preserved as a 
fossil. 

C. inopinata occurs in the western Bight 
together with C. tubulifera, but from shallower 
waters. In Bass Strait, and from Tasmania, C. 
tubulifera is known from a wide range in depth 
from 40m to 800m. It appears to be at the limits 
of its range south east of Eucla, in deep water. 
Wass (1975) first described Corbulipora 
oriparma, which is the bilaminar phase of C. 
tubulifera, from three localities. The holotype was 
from northeast Tasmania, the other specimens 
were from the eastern part of the South Australian 
coast. Subsequently, Wass and Yoo (1983) 
recorded C. oriparma from 12 localities, 
extending from near Perth to southwest of Eucla. 
These are similar to many of the localities from 
which specimens have been recently examined, 
and which have produced C. inopinata. None of 
Wass and Yoo's (1983) localities was from a 
greater depth than 158 m, far shallower than the 
most westerly known locality for C. tubulifera. 
Only examination of the specimens recorded by 
Wass and Yoo (1983) can decide their identity. 

Acknowledgments 

We should like to thank Dr Yvonne Bone (University 
of Adelaide) and the Master and crew of CSIRO R.V. 
'Franklin' for the opportunity for one of us (P.E.B.) to 
take part in the sampling programme in July 1995, 
which led to the discovery of the species described here. 
We are also grateful to Mr D. McDonald for his help in 
preparation of this paper. 



68 



P. E. BOCK & P. L. COOK 



References 



BOCK, P. E. & COOK, P. L. 1994. Occurrence of three 
phases of growth with taxonomically distinct zooid 
morphologies. Pp 33-36 in Hayward, P. J., Ryland, J. 
S. & Taylor, P. D. (eds): Biology and Paleobiology 
of Bryozoans. Olsen & Olscn: Fredensborg. 

BOCK, P. E. & COOK, P. L. in press. A revision of the 
genus Corbulipora MacGillivray (Bryozoa: 
Cribriomorpha). Memoirs of the Museum of Victoria. 

BUSK, G. 1852. Catalogue of Marine Polyzoa in the 
Collection of the British Museum. Part 1 
Cheilostomata (Part).: viii, 1-54, vi. Trustees of the 
British Museum, London. 



HINCKS, T. 1879. On the classification of British 
Polyzoa. Annals and Magazine of Natural History 
(5)3:153-164. 

MACGILLIVRAY, P. H. 1895. A Monograph of the 
Tertiary Polyzoa of Victoria. Transactions of the 
Royal Society of Victoria, 4:1 166. 

WASS, R. E. 1975. A revision of the Bryozoan Genus 
Corbulipora MacGillivray. Proceedings of the Royal 
Society of Victoria 87:167-173. 

WASS, R. E. & YOO, J. J. 1983. Cheilostome Bryozoa 
from the Southern Australian Continental Shelf. 
Australian Journal of Marine and Freshwater 
Research 34: 303-354. 



THE ARCHAEOLOGY OF LAKE SYSTEMS IN THE MIDDLE COOPER 
BASIN, NORTH-EASTERN SOUTH AUSTRALIA. 



ELIZABETH WILLIAMS 



Summary 



This paper presents the final report of a study of the archaeology of a number of lake systems 
located in the middle section of the Cooper Basin and neighbouring areas near Innamincka, South 
Australia. The paper outlines the results of archaeological fieldwork carried out during 1987 in one 
area within the region and relates this to other research undertaken in 1986 and 1989 in other parts 
of the middle of the Basin. 



THE ARCHAEOLOGY OF LAKE SYSTEMS IN THE MIDDLE COOPER BASIN 
NORTH-EASTERN SOUTH AUSTRALIA. 



ELIZABETH WILLIAMS 



WILLIAMS, E. 1998. The archaeology of lake systems in the middle Cooper Basin, north- 
eastern South Australia. Records of the South Australian Museum 30(2): 69-91. 

This paper presents the final report of a study of the archaeology of a number of lake systems 
located in the middle section of the Cooper Basin and neighbouring areas near Innamincka, 
South Australia. The paper outlines the results of archaeological fieldwork carried out during 
1987 in one area within the region and relates this to other research undertaken in 1986 and 
1989 in other parts of the middle of the Basin. 

E. Williams, World Heritage Unit, Department of Environment, Sport and Territories, Canberra, 
Australia Capital Territory, 2601. Manuscript received 3 1 June, 1995. 



The lakes forming the main focus of this study 
are located within an extensive linear dunefield, 
the Strzelecki desert, which forms part of 
Australia's continental dunefield. Although 
archaeological research has been undertaken along 
the main channel of the Cooper in the middle 
Cooper basin, particularly the Innamincka area 
(Hughes & Lampcrt 1980, McBryde 1987), the 
archaeology of the region's series of lake systems 
had not been studied until this research 
programme. Given that at least a number of the 
lakes hold fresh water for some considerable time, 
and that this is a strikingly unusual feature of arid 
areas generally, it is very likely that the lakes 
would have been the major focus of occupation for 
at least the recent period and possibly for extended 
periods in the past. As well, it is possible that 
landforms associated with the lakes such as 
source-bordering dunes preserve information 
about Pleistocene climates and changing 
environmental conditions, and possibly also about 
Pleistocene human occupation. A study of the 
lakes therefore had the potential to contribute to 
our knowledge of not only the recent occupation 
of the region but also that of past settlement, and 
possibly, the wider question of how Australia's 
arid zone itself was occupied. 

In structuring the project, a preliminary analysis 
of the region revealed considerable variation of 
the nature and types of lakes. The study was 
designed to examine this variability in relation to 
human settlement. The study was designed as 
follows. I examined the archaeology of examples 
of the three major types of lake systems in the 
region. These are the semi-permanent lakes of the 
Coongie system, fed by the Cooper's North- West 



Branch; small isolated salt lakes marking the edge 
of the Cooper Basin, and a series of ephemeral 
lakes to the north of the Basin fed by local 
drainage and precipitation. The results of this 
work are presented below. In the latter sections of 
my discussion I compare this information with 
that obtained from sites located in a relatively 
waterless core of the dunefield located in the 
southern part of the Strzelecki desert. The 
concluding part of the paper outlines a number of 
speculative hypotheses about the occupation of the 
region and of Australia's arid zone in general. 

Work carried out in the Coongie lake system 
has previously been reported on in Williams 
(1988) and that undertaken in the Strzelecki 
dunefield summarised in Smith, Williams and 
Wasson (1991). The current study draws this 
research together to present a comprehensive view 
of the region's archaeology. 



General Environmental Features Of The Region, 
Including Those Important For Human Occupation 

The study area lies in one of the most arid parts 
of Australia. The region is covered by an extensive 
linear dunefield and receives the lowest rainfall 
reading of any area of the continent (125 mm per 
annum). Despite the aridity there are reliable 
water sources here in the form of the Cooper 
Creek channel, its overflow system - the North- 
West Branch, and associated lakes fed by the 
channel systems. The amount of water in this 
drainage complex does not reflect local rainfall 
patterns and predominantly derives from received 
precipitation falling many hundreds of kilometres 



70 



E. WILLIAMS 



to the north-east during the wet season in the 
upper parts of the Cooper catchment in north-west 
Queensland. 

Given the arid setting of the region, water was a 
valuable resource and one of the most important 
features for human occupation. This is confirmed 
by the distribution of archaeological material 
within the Coongie lake system - site size and 
stone artefact density increases in relation to the 
location of permanent and semi-permanent water 
sources (Williams 1988: 59). 

Another important feature for occupation was 
the availability of good quality stone suitable for 
artefact manufacture. Stone sources are extremely 
localised here and are either scarce or entirely 
absent within most of the linear dunefield itself. 
Some stone is available in the form of pebbles 
carpeting the surface of the gibber plains or 'stony 
deserts' located on the edges of the study area but 
this source only exists in the form of small 
nodules, not necessarily suitable for all types of 
artefact manufacture. The most extensive areas of 
stone are found in outcropping areas of hard rock 
within areas of dissected tablelands located on the 
margins of the study area. 

Although the availability of resources such as 
water and stone were crucial, the two resources 
do not always coincide geographically. In the area 
immediately surrounding Innamincka where are 
found the extensive deep waterholes of the main 
Cooper channel and the abundant good quality 
stone resources of the locality's mesas and 
dissected tablelands, the two resources are 
abundant and lie close together. In the Coongie 
lakes system located within the stone-free linear 
dunefield, although water resources are extensive, 
good quality stone lies at least 60 km away. 
Therefore one of the major features of the 
archaeology of the region relates to how people 
balanced their need for stone with that for water 
and how this varied from one area to another. 
Because this feature is responsible for much of 
the patterning of the archaeology of the Basin and 
neighbouring areas, it is the major focus for this 
study. 

A second and related focus concerns the 
antiquity of human occupation of the region. This 
topic is reported on in detail in Smith, Williams 
and Wasson (1991) and is also discussed here. 

The structure of the paper is as follows. Given 
that the environment places such strong 
constraints on human occupation in the region, a 
general overview of climatic and geographic data 
is presented first, including material on 
environmental chronologies. This is followed by a 



brief summary of historical accounts of how 
Aboriginal people were observed to be using the 
area at the time of European contact, in order to 
present a picture of the occupation of the area at 
least for the recent past. The paper then reports on 
archaeological sites investigated, including an 
analysis of stone artefacts from a selected sample 
of sites. I conclude with a brief discussion of some 
of the theoretical implications of my work. 



The Contemporary Environmental Srtting 

A number of the environmental parameters for 
the region have already been presented in 
Williams (1988). This section does not repeat this 
material and instead provides more detailed 
information on localities previously discussed and 
new data on areas not referred to in other 
publications. 

The main focus of the study area is a series of 
lake systems within the Strzelecki desert. On the 
east and west the Strzelecki is bounded by stony 
country, comprising gibber plains and areas of 
dissected tablelands. The latter consists of the low, 
but locally steep escarpments and small mesas of 
the geological features known as the Innamincka 
and Cordillo domes. 

The aridity of the area has been noted above. 
Precipitation in the region is unpredictable and 
erratic, with no systematic seasonal patterning. 
Evaporation is extremely high, at least one order 
of magnitude greater than precipitation (Reid and 
Gillenl988: 16). 

Three of the lake systems which form part of 
the study area are discussed in some detail here. 
They are the freshwater lakes of the Coongie 
system, a ring of salt lakes which mark the 
boundary of the Cooper drainage system, and 
another chain of lakes which lie to the north of the 
system and to the west of Cordillo Downs station. 
For convenience I refer to this latter group of lakes 
as the 'Cordillo lakes'. 

The Coongie system 

The Coongie system comprises a series of large, 
shallow, irregularly-shaped lakes lying within the 
linear dunefield. The lakes are fed by a tributary 
of the Cooper, the North- West Branch. The system 
has a complex hydrology and is described here in 
its constituent sections from south to north. 
Closest to the North-West Branch feeder channel 
are three lakes: Coongie, Marroocoolcannie and 
Maroocutchanie, which are fed directly from the 
North-West Branch. Two lakes lying further 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



71 




T^ 



JUT 



Stony desert 
(Cordillo Dome) 



* Cordillo Downs if] 



\ 



Stony desert 



\ 



\ 



■ \K l f\A !\v\\\\0*to Lake Koonoomoorinna ,} v \ ' L 1 ' ^h>\sVi' i* 
t ffy \y%TiIlie Lakes y\ \ \\\\\\ \M*> I wllUw \ 






Stony desert 
(Innamincka Dome) 




FIGURE 1. Regional map of north-east South Australia showing the sites mentioned in the text 



72 



E. WILLIAMS 




^5 Salt Lakes ^"^ Source bordering dunes 



FIGURE 2. Map of the Coongie and Cordillo lake systems. 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



73 



north, Toontoowaranie and Goyder, are fed by 
interconnecting creeks from overflow from the 
first three lakes. To the north again are a further 
three lakes: Marradibbadibba, Lady Blanche and 
Sir Richard, which fill from overflow from Lake 
Goyder. In this paper I refer to all of the lakes 
collectively as the 'Coongie system'. 

A further series of lake and channel systems 
also have some connection either to the Coongie 
system or the North-West Branch channel. It is 
noted that although they do hold water at certain 
times (as observed by the explorer, John McKinlay 
in 1862), the Coongie system, at least in the recent 
past, held the most extensive and most reliable 
sources of water. Little is currently known about 
their hydrology and for this reason the lakes do 
not form part of this study. 

The North-West Branch which joins the Cooper 
west of Innamincka diverts most of the flow of 
the main Cooper channel northwards. For the area 
west of Innamincka relatively little water thus 
flows down the main Cooper channel on to Lake 
Eyre (Mike Steele, Innamincka store, pers. 
comm.). The Coongie system therefore catches 
most of the water coming down the Cooper 
channel. Flow down the Cooper derives from two 
sources: local precipitation and received rainfall 
which falls as far as 500 km upstream in the 
channel country of western Queensland. This 
latter precipitation falls mostly during the summer 
monsoon and contributes the major portion of the 
Cooper's flow. In contrast to local rainfall its 
timing is relatively predictable. Water from the 
summer monsoon rains takes about three months 
to come down the channel, first reaching the 
Coongie about late autumn (Barry Saunders, 
Innamincka region, pers. comm.). 

Despite this level of predictability, the amount 
of water which actually comes down the channel 
and the exact time of year when it arrives 
markedly fluctuates in relation to variability in the 
timing and effectiveness of rainfall in the upper 
Cooper catchment. Nonetheless, there are 
predictable water sources in the form of deep, 
permanent waterholes which are often a couple of 
kilometres in length, located along the channels 
of the main drainage systems such as the Cooper 
and the North- West Branch. 

With the possible exception of Coongie, the 
lakes do not hold water on a permanent basis. 
Oral tradition amongst current residents of the 
Innamincka region suggests that Coongie Lake 
itself holds water for most of the year, although 
the nature and amount of water it holds is difficult 
to quantify because of a lack of historical records. 



The other lakes in the system hold water for 
months at a time but the extent and duration is 
highly variable and depends on a number of 
factors. These include the amount of water coining 
down the Cooper from rainfall in the northern 
catchment, local precipitation, the position of the 
lake relative to the North-West Branch and the 
season of the year (evaporation is highest during 
summer). 

Despite variability in the amount of water held 
in the Coongie system, the presence of often 
extensive supplies of fresh water in an otherwise 
extremely arid environment is extremely rare 
within Australia. The region consequently 
supports a very productive and diverse ecology, 
but one which varies in relation to water levels in 
the lakes and channels. The variability does not 
decrease overall productivity, and in fact is 
responsible for the high biodiversity of the region. 
The chain of lakes, with its complex sequence of 
rising and falling water levels is biologically 
highly productive. The lakes provide a diverse 
range of constantly changing habitats and have 
the potential to support the largest number and 
widest range of resources in the region. The major 
resources found here are: birds, especially 
waterbirds; fish, crayfish and mussels; dry-land 
and aquatic plants, and some mammal species. 

Biological studies of the system reveal this very 
high productivity (Reid and Gillcn 1988, Reid and 
Puckeridge 1990). Reid and Gillen for example 
recorded 161 separate bird species in the Coongie 
system and estimated that during the year under 
study (1986 - a wet year when all lakes in the 
system held water for much of the time) 20 000 
waterbirds permanently occupied the lake chain. 
(1988: 184, 198). 

Because of the interconnectedness of the 
system, rising and falling levels in one lake affect 
other lakes in the chain. Given that most of the 
plant and animal species in the region are oriented 
to specific environmental niches, variation in 
water levels consequently provides a much wider 
range of habitats than would otherwise be 
available along a permanent waterhole where 
water levels remain relatively constant. For 
example, although water levels in one lake may 
begin to fall with evaporation, certain species of 
waterbirds whose habitat is that of more shallow 
water will migrate in to the lake while those 
whose habitat is that of deeper water will move to 
another lake where water levels are rising. The 
differential fluctuation of water levels means that 
the lakes have the potential to carry the largest 
biomass of plants and animals in the region 



74 



E. WILLIAMS 



because they are providing a wide range of 
ecological zones. The permanent waterholes on 
channels and rivers carry a relatively lower 
biomass because their environments are much less 
variable. Water levels fluctuate significantly less 
in these deep waterholes, supporting a smaller, 
but more predictable range of resources. 

Salt lakes or 'salinas ' 

These irregular-shaped lakes lie in a ring along 
the northern and western boundary of the Cooper 
drainage basin and mark the boundaries of that 
system. They are located in the midst of the linear 
dunefield and are deflation hollows cut to 
groundwater level. This type of feature has been 
termed a 'salina' (Macumber 1980). Their salinity 
derives from the fact that in the region the 
groundwater is saline. Although no hydrological 
studies of the salinas in this area have been 
undertaken, it appears that for the recent past at 
least, they are permanently saline. In contrast to 
the Coongie system they therefore support 
relatively few plant and animal resources. 

The Cordillo lakes 

To the north of the Coongie system, beyond the 
salt lakes, lie another series of irregularly-shaped 
lakes. As with the salinas, no formal studies of 
these have been undertaken and there are no 
records of how often they fill. 

Cartographic and field observations of the 
locality suggest that there are at least ten lakes in 
the system, connected by a series of channels. It 
appears that they fill from local run-off from the 
stony country of the Cordillo dome to the east. 
Their hydrology, unlike the Coongie system, 
therefore reflects local precipitation. The lakes 
were dry when fieldwork in the area was 
undertaken (1987), despite the years 1986 - 1987 
having been much wetter than average in terms of 
local rainfall. This suggests that considerable local 
precipitation is required to fill them and they thus 
remain dry for very long periods of time. They are 
not salinas though, and small pools of fresh water 
were present in 1987 in a few places along the 
channels linking the lakes. The predominantly dry 
character of the lake system suggests that it 
supports relatively few plant and animal resources 
in comparison to the Coongie, but the presence of 
some areas of freshwater indicates that more 
resources are supported than the saline lakes. 

The region's current environment is not 
necessarily the same as today as in the past. Over 
time there have been significant changes in 
climate, hydrology and landforms, with 



consequent effect on the human occupation of the 
region. 



Past Environments - Dunefield And Floodplain 
Research 

Much of the information on past regional 
climates has been summarised and presented 
elsewhere (Williams 1988) and so here I briefly 
refer to this work and also discuss new data which 
has arisen as a result of the study. R. Wasson has 
developed an environmental chronology for the 
region, based on stratigraphic sequences derived 
from longitudinal dunes and floodplain sediments 
(for references see Williams 1988). A summary of 
his findings and a discussion of their implications 
for the hydrology of the lakes follows. 

Wasson's work indicates that before 22 000 
years ago the Cooper had a higher velocity than 
today and was flooding out to a much greater 
extent. Although geomorphological studies of the 
Coongie lakes themselves have not been 
undertaken, Wasson's data suggest that if the 
Coongie system was in operation during this 
period it would have held considerably more water 
than today. As well, groundwater levels for the 
region as a whole would have been higher, 
indicating that the lake depressions which are now 
salinas may have held fresh water, Current work 
does not indicate whether local precipitation was 
also high at this time, so that it is not possible to 
model processes which may have been occurring 
in the Cordillo lakes. 

Around 22 000 years ago, the Cooper's velocity 
decreased, Hooding of the outer floodplain 
decreased and it is likely that the water table 
lowered as well. Consequently it is likely that what 
are now salinas would have changed from fresh 
water at this time. Lake levels in the Coongie 
system may have become lower. About 20 000 
years ago conditions were windier and more arid, 
activating a period of dune building throughout the 
linear dunefield. The dune sediment was drawn 
from the deposits formed from the continuing, 
reduced flooding of the outer floodplain. These 
climatic conditions and the consequent dune 
building persisted until around 16 000 years ago. 
At about 1 2 500 years ago the flooding-out of the 
outer floodplain ceased, removing the sediment 
available for dune building. 

Dune building began again in the later 
Holocene, although on a smaller scale than in the 
late Pleistocene. Wasson (1986: 79) notes that this 
event is enigmatic, since in contrast to the late 



ARCHAEOLOGY OF THE MIDDLE COOPER BASrN 



75 



Pleistocene there seems to have been no climatic 
change occurring on a scale large enough to be 
able to mobilise sediments. He has speculated that 
it is possible, although not yet conclusively 
demonstrated, that the phenomenon could be 
related to more intensive human occupation of the 
region. If such intensive occupation took place, 
the erosion resulting from Aboriginal firing of 
vegetation to aid the procurement of food 
resources, together with clearing of trees and other 
vegetation to provide fuel for campfires and earth 
ovens, may have caused greater mobility in 
sediments. 



Past Environments - Studies Of Lakeshore 
Features 

The environmental data presented above is 
derived from a study of dunefield and floodplain 
sediments and presents a broad regional 
chronology. Is it possible to develop a chronology 
for the lake systems themselves? 

A formal study of the geomorphology of the 
lake systems was beyond the scope of this study 
so I developed a smaller project, more 
complementary to the archaeological work. This 
involved an examination of whether landform 
features such as source-bordering dunes, which 
have the potential to contain information on lake 
chronology, had developed on lakeshore margins. 
These transverse dunes, Twidale's 'leeside 
mounds' (1972; 85-86), are similar to the lunettes 
of semi-arid regions. They are formed when 
longshore drift transports debris to beaches or lee 
shores of lakes. This sediment is then locally 
redistributed by the wind before being trapped by 
vegetation close to the lake margin. 

The work was complementary to the 
archaeological survey in the sense that it was 
anticipated that source-bordering dunes were also 
likely to be a focus for human occupation. 
Systematic survey of these features would not 
only have the potential to reveal information 
about environmental features but also about 
human occupation, and the chronology of such 
occupation. 

The project comprised an examination of 
examples of source-bordering dune features for 
each of the lake systems discussed earlier. Aerial 
photographs were used to identify the features and 
distinguish them from the linear dunes of the 
continental dunefield. The transverse dunes are 
paler in colour and generally trend east-west in 
contrast to the north-south longitudinal dunes. 



Once they were identified on the aerial 
photographs I travelled to them on the ground and 
systematically surveyed all exposures for any 
archaeological material. 

Access to the features by vehicle was often 
difficult and in a number of cases access was by 
helicopter. Regarding the dating of the dunes it is 
noted that at the time the work was undertaken 
only radiocarbon dating was available to the 
study. Thus if organic material suitable for such 
dating was not present in-situ the dunes were 
unable to be directly dated. The results of the 
work are presented below. 

The Coongie system 

Information on a number of the source- 
bordering dunes of the Coongie system is outlined 
in detail in Williams (1988: 58-60). A summary 
of the work is presented here along with new data 
on other parts of the system. 

The analysis of aerial photographs, maps and 
the survey work itself revealed that while some 
features such as colour of the source-bordering 
dunes are similar across the system there is major 
variability in the number, size and location of the 
features. A common feature is that all dunes are 
pale in colour and have little or no carbonate 
formation within their profiles, and they contain 
intermittent scatters of artefacts on their surface - 
typologically the artefacts appear to be late 
Holocene in age. All of these factors suggest the 
dunes are recent features. When cores of the 
dunes were exposed by erosion and these sections 
were examined, no organic or archaeological 
material was found in-situ, with the exception of 
one site at Lake Marradibbadibba - Lake Goyder 
1 . Details of this site are presented in Williams 
(1988: 60) where it is noted that it dates to the 
relatively recent past 810-130 BP (ANU 5424) 
thus confirming the recent age of the transverse 
features. 

There is considerable variation in dune shape 
and alignment across the system. Some lakes had 
a low and amorphous single transverse dune (such 
as Toontoowaranie); others had a higher and more 
distinct single dune (Coongie, Marroocoolcannie). 
Still others had multiple transverse dunes, one 
behind the other (five in the case of Lake Lady 
Blanche, yet none on the neighbouring Lake Sir 
Richard, and five or more in the floodplain 
between Coongie and Toontoowaranie). Location 
of dunes relative to lakes ranged from north, to 
north-east and east. 

Given that the study of the dunes was only a 
preliminary one, it has not been possible to 



76 



E. WILLIAMS 



determine what factors are responsible for the 
variation in dune features. It is likely that since 
there is major variation in the shape and size of 
the lakes themselves and how they fill relative to 
channel features and other lakes, and marked 
fluctuations in the amount of water coming into 
the system and the timing of when these events 
occur, it is probable that these factors are 
responsible for much of the variation. 

The morphology and colour of the dunes 
indicates that they are of late Holocenc rather than 
Pleistocene age. Two hypotheses could explain 
their recent age. The first proposes that the lake 
system was active in the Pleistocene, but since tt is 
still in operation today, receiving what can be 
major flows of water and often flooding out 
extensively, any Pleistocene shore features have 
either been swept away by previous high-water 
events or are well buried below flood deposits. In 
1974 for example, the entire system flooded out - 
aerial and satellite photography reveals water 
extending for hundreds of square kilometres with 
only the tops of linear and transverse dunes visible. 
Krieg and Callen note that the Coongic system is 
one of net sediment accumulation (1990: 60) and it 
is thus possible that many older lake-shore features 
have been disturbed or buried by sedimentation. 

The second hypothesis proposes that the lake 
system may not have been in operation in the 
Pleistocene. Recent work by Callen and Bradford 
(1992) presents data showing that the current 
situation, in which most of the ilow down the 
Cooper channel west of Innamincka is diverted 
north up the North-West Branch, may be very 
sensitive to minor changes in topology resulting 
from such factors as tectonic activity or shifts in 
sedimentation or the location of dune features 
(transverse and longitudinal). Slight movements 
on faults or in sedimentary features of only 1-2 
metres within a large, low angle fan formed by 
the Cooper immediately west of Innamincka may 
be sufficient to create major changes in channel 
direction, and thus whether the Cooper flow is 
diverted either along the Branch, along another 
channel such as the main Cooper channel or even 
southwards down Strzclecki creek. Given this 
sensitivity to change it is possible that during the 
Pleistocene the North-West Branch may not have 
been carrying the main Cooper flow and the lakes 
may not have functioned as they do today. 

Because a detailed study of the geomorphology 
of the Coongie system has not been undertaken it 
is not possible to resolve these competing 
hypotheses. It is nevertheless possible to conclude 
that whatever the reason, the lake-shore features 



currently exposed within the area do not provide a 
window onto the Pleistocene. 

The salt lakes 

Two of the larger salinas in the region, Coorie 
Coorie Tillie and Lake Deception, were chosen for 
analysis. Although the lakes lie some 100 km 
from each other, the form of their transverse dunes 
is virtually identical, in direct contrast to the 
variability of the Coongie system. As well, the 
transverse dunes themselves are very different to 
those of the Coongie. 

Each lake has a low, flat, pale-coloured 
transverse dune on its northern edge. These have 
been extensively gullied to expose older-looking 
sediments which are redder in colour and more 
compact with a pronounced carbonate horizon. It 
is likely that further analysis would confirm that 
the sediments are of Pleistocene age. 

A systematic survey of the length of each dune, 
including an examination of the many sections of 
dune core exposed by erosion, revealed that the 
small amount of archaeological material present 
all lay within recent sediments on the dune 
surface, rather than in the Pleistocene core. 

In contrast to the Coongie, there are no large 
amounts of water coming into the system to 
modify or distort landform features. The salinas 
are groundwater features, and do not fill from any 
channels. The dunes' consistency in nature and 
form could result from similarity in formation and 
hydrology operating on the lakes. Unlike the 
Coongie, the transverse dunes appear to have the 
potential to preserve Pleistocene sediments but no 
stratified archaeological material is currently 
visible within their profiles. 

The Cordillo lakes 

This system has a set of source-bordering dunes 
different from both the Coongie system and the 
salinas. Like the salinas and unlike the Coongie 
system, there appeared to be a strong consistency 
in the number, form and structure of the features 
across the lake margins. 

On the northern edge of the lakes is a sequence 
of three transverse dunes trending east-west, and 
located one behind the other. The dune closest to 
the lake edge is quite low, less than a metre in 
height and pale in colour. Behind this is another, 
slightly higher, pale-coloured dune which is 
beginning to blow out into small longitudinal 
dunes. Behind this again is another higher dune, 
distinctly orange in colour with a pronounced 
carbonate horizon, which has almost completely 
blown out into longitudinal dunes. 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



77 



The outermost dune is heavily eroded and it is 
likely that it is Pleistocene in age. Samples of 
carbonate from within the profile of the dune from 
Lake Koonoomorinna were dated using 
radiocarbon techniques and returned the relatively 
recent dates of 3930-80 BP (ANU 6182) and 
4560-80 BP (ANU 6182). John Head of ANU 
Radiocarbon Laboratory notes that the samples are 
not dating the formation of the dune itself, only 
the last major phase of mobilisation of carbonates 
within the dune. Such mobilisation would have 
taken place during the last period of stable high- 
water levels in the region and the samples are 
probably dating this event (pcrs. comm.). 

A complete survey of all of the dunes from one 
lake, Koonoomoorinna, revealed that stone 
artefacts are scattered across the surface of each 
dune, but that no artefacts or organic material 
were present in-situ within the cores of the 
features, including the Pleistocene dune. An 
analysis of a number of samples of the artefacts is 
presented later in the paper but it is noted here 
that those seen had features characteristic of 
artefacts dating to the mid-late Holocene. 

It is suggested that the regularity in source- 
bordering dune spacing and form for the Cordillo 
lake system is, like the salinas, reflecting 
consistency in processes involved in formation 
and filling. The lakes fill from run-off within the 
local catchment, and in contrast to the Coongie 
system there is significantly more regularity in 
their hydrological processes and many fewer flood 
events to affect the morphology of lake-shore 
features. Like the salinas and in contrast to the 
Coongie system, the transverse dunes appear to 
have the potential to preserve Pleistocene 
sediments but, as with the salinas, no in-situ 
archaeological material is currently visible within 
their profiles. 

It is not known at this stage why the lakes 
preserve a group of three transverse dunes. Each 
dune may reflect a period of relative stability in 
lake levels so that the position of the dunes, one 
behind the other, may indicate a shrinking lake 
basin since higher levels in the later Pleistocene. 
Alternatively, the position of the dunes may 
reflect the fact that all lakes in the region, 
including the Coongie system, are slowly 
migrating southwards over time (Bob Wasson 
pers. comm.). The presence of the dunes may 
reflect both factors. 

Following this presentation of climatic and 
environmental information, the next section places 
the region in a more recent context by 
summarising historical accounts of how 



Aboriginal people occupied the area at the time of 
contact with European people. The section draws 
on information presented in Williams (1988) and 
Layton, Foley and Williams (1991: 258-259) and 
also presents new material. 



Historical Accounts Of Subsistence And 
Settlement 

Citing McKinlay (1862), who was the first 
European to travel through the entire middle 
Cooper lake system, the region was densely 
populated at the time of contact. McKinlay's 
expedition, which was one of those initiated to 
search for Burke and Wills, involved the party 
spending several months in the lake system in 
1861-1 862. During this time they were 
systematically examining each of the lakes and 
channel systems of the North- West Branch in their 
search for the missing explorers. 

McKinlay saw more than 700 people in the 
region during his travels, including more than 300 
people camped along Hamilton Creek, 
immediately west of Lake Toontoowaranie in the 
Coongie system, 200-300 people along the North- 
West Branch just south of Coongie Lake itself, 
and at least 150 people around Lake Lady Blanche 
(1862: 37, 38, 46). Because of the length of time 
he spent in the region he was also able to observe 
how people utilised fluctuations in water levels 
across the lakes. 

McKinlay 's information shows that population 
densities were highest around the large, 
permanent waterholes on the channels of the 
Norlh-West Branch and the Cooper itself, and 
those lakes within the North-West Branch system 
which were currently holding water. Group 
composition appears to have been relatively fluid. 
Large aggregations of 1 50 or more were formed to 
take advantage of the flush of food resources 
which appeared as lakes began to fill. As they 
dried out again, people moved to other lakes, 
following the water, or split into small groups to 
harvest other resources or move on to other areas. 
Permanent or semi-permanent camps of between 
twenty and forty people were found along the 
permanent waterholes of the channel systems and 
this observation is also consistent with that of 
King, the surviving member of the Burke and 
Wills party who was cared for by Aboriginal 
people in the Innamincka region (Burke and Wills 
1861). At these more settled camps habitations 
comprised substantial huts. 

Important food resources were fish, crayfish 



78 



E. WILLIAMS 



and mussels; waterbirds, and the variety of plant 
foods which germinated after flooding or local 
rain, especially nardoo. People favoured the lakes 
and rivers but after rain in the local catchment 
dispersed into small groups and travelled out into 
the drier dune country (McKinlay 1862: 49; Jones 
1979). In these latter areas a flush of resources 
including small mammals, reptiles and certain 
types of plant foods, especially seed plants, 
appeared after the rain. 

Although there are no ethnographic 
observations of how the Cordillo system was used, 
it can be hypothesised that after local rain areas 
such as this became a focus for occupation, the 
water sources it now held resulting in a relative 
abundance of food. It is also possible that if semi- 
permanent pools of water remained for a 
considerable time throughout the year in the 
shallow channels between the lakes, some small 
groups of people might have occupied the region 
on a more permanent basis. 

While historical accounts mention the existence 
of the salt lakes there are no direct ethnographic 
observations of people using these areas. This 
implies that they were not favoured areas for 
occupation on a day-to-day basis. 

Dealing with periods of resource stress 

Although the Cooper lakes and channel systems 
contain a large range of food resources for much 
of the year, it appears that periods of resource 
stress were common, especially during droughts. 
Although there are no direct observations of the 
study area itself during these periods, historical 
material in Reuther (1981) provides information 
on strategies used by Aboriginal communities in 
the north-east of South Australia generally, to deal 
with the major fluctuations in environmental 
conditions characteristic of the region. 

Reuther noted that when resources were 
abundant, for example in periods after rain, 
communities utilised natural surpluses in a variety 
of ways. Large gatherings were organised to take 
advantage of the abundance of food and these 
aggregations had the primary function of 
satisfying social obligations through, for example, 
trade and exchange (1981; vol. 1: 42, 47^8). As 
well as these activities, people harvested more 
than they needed for immediate consumption, 
processing and storing the surplus for later use. 
Seeds, fish and grubs were the resources most 
favoured for this type of processing (1981 : vol. 1: 
13, 47^18, 232, 273, 491; vol. 2: 547, 772, 835, 
915, 927; vol. 4: 1852; vol. 7: 458, 549, 659). 
As well as these measures to maximise the 



productivity of a region, according to Reuther the 
distribution of food resources was also artificially 
managed. He recorded that rats and caterpillars 
were moved from one area to another so as to 
increase stocks in particular regions (1981 : vol. 2: 
811-812; vol. 9: 232). Plant foods were 
propagated through the broadcasting of seed and 
the distribution of the branches of a particular vine 
species (1981: vol. 1: 107; vol. 7: 450). Areas of 
stream channels were dammed to increase stocks 
of fish (1981: vol. 8: 23). As well, certain 
localities were not utilised and were left in reserve 
for use during lean times, access to especially 
productive areas was strictly controlled and the 
boundaries of group territories were rigorously 
enforced (1981: vol. 1: 101, 123-128, 412; vol. 2: 
559, 751, 1044; vol. 3: 1255, 1259). 
Transgressions, such as cases of people trying to 
obtain more food resources than their due, or 
attempting to accumulate resources, were severely 
punished according to Reuther, even by death 
(1981: vol. 1: 12-13, 123-129; vol. 2: 793-794). 
Further, instances were recorded of particular 
groups attempting to appropriate others' territory, 
sometimes successfully (1981 vol.1: 415; vol. 2: 
896). 

During times of drought people fell back to 
those areas which had water, and fish and stored 
food resources were the main foods consumed 
(1981 vol. 1: 520; vol. 2: 547, 616, 758 ? 915, 950; 
vol. 2: 1259; vol. 4: 1740). Although Reuther 
doesn't specify these areas, it is likely that the 
Coongie system and the Cooper channel near 
Innamincka were used in this manner. 

Despite measures to counteract the effects of 
drought or a lack of surface water, local groups 
still suffered considerable stress. Reuther noted 
that many people perished at these times, from 
thirst, heat exhaustion or starvation (1981: vol. 1: 
424, 535; vol. 2: 994-995, 1036; vol. 4: 1741- 
1742, 1926, 2108; vol. 8:75, 118). 



Factors Other Than Food Resources Affecting 
Settlement 

It is a truism to state that it is not only the 
acquisition of food resources which affects the 
choice and nature of settlements. Access to raw 
materials necessary for the manufacture of goods 
and for trade, such as stone, wood, ochre, resin, 
bone, shell and the narcotic pituri, was another 
important determinant. 

Historical accounts show that the Innamincka 
region was an important centre both for the 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



79 



production of technological items, especially 
stone artefacts and for a related reason, as a 
crucial node in the vast exchange network which 
spanned the continent (Kerwin and Breen 1981: 
286 and McBryde 1987). Innamincka was 
especially renowned for its extensive grindstone 
quarries (see Reuther 1981 vol.2: 899-900, 
McBryde 1987). The quarries, other important 
sites involved in the extraction of resources and 
the manufacture of goods, and the exchange 
networks of the Lake Eyre Basin generally, are 
currently being studied by McBryde and are thus 
not reported on here. 

Although factors such as the utilisation of items 
for artefact manufacture and the location of trade 
and exchange networks are, as outlined above, 
crucial factors involved in settlement, not all of 
these features are equally archaeologically visible. 
For this reason I have chosen to look at one aspect 
that is more archaeologically visible than others, 
namely the characteristics of stone artefacts on 
lake-side sites and what these data, and other 
characteristics of the sites themselves, can tell us 
about Aboriginal use of the region. As outlined, 
stone suitable for the manufacture of artefacts is 
not uniformly distributed across the region and 
with the exception of Innamincka, stone sources 
and water sources do not generally coincide. 

Two main sources of stone arc present in the 
study area. Silcrete, chert and chalcedony are 
found as smallish pebbles on the surface of gibber 
plains, while better quality and more extensive 
areas of hard rock, comprising outcrops of chert, 
chalcedony, silcrete, quartzite and sandstone are 
found within the geological features known as the 
Innamincka and Cordillo domes (South Australia 
Department of Mines and Energy staff: pers. 
comm. and personal observation). Discrete areas 
of outcropping hard rock also occur within the 
linear dunefield south of the Cooper channel and 
east of Strzelecki creek (see Smith, Williams and 
Wasson 1991: 185). 

Although there are no historical accounts of 
how Aboriginal people in the region quarried and 
used stone, apart from Reuther's observations on 
the Innamincka grindstone quarries, field 
observations and geological data can be used to 
determine what may have been favoured sources. 
It appears that while gibber pebbles were utilised, 
this took place on a relatively limited basis 
compared to other sources because of the 
relatively small size of the nodules of stone that 
could be worked. Outcropping areas of hard rock 
were thus favoured over gibber pebbles because 
they provided larger fragments of stone and were 



more uniform in quality. As well, certain types of 
stone such as sandstone were not available as 
pebbles and were only located within hard rock 
localities. 

Using data from geological mapping of the 
region and advice from South Australian 
Department of Mines and Energy staff, it is 
estimated that the Coongie system lies at least 60 
km from good quality stone sources while the 
Cordillo lakes lie at least 20 km distant. 
Particular stone sources which would have been 
favoured include: the silcrete (including 
chalcedony, cherts, cherty silcretes and 
quartzites) of the Cordillo surface which caps 
the mesas and cuestas of the Cordillo and 
Innamincka regions and also includes the 
silicified Eyre formation and the silicified 
Winton formation; the Eyre formation which 
includes sandstones suitable for grindstone 
manufacture, and also small pebbles of agate and 
fossil wood, and the Cadelga limestone which 
includes a cherty limestone. 

Surrounding these outcrops of hard rock and 
extending outwards for five kilometres or so are 
areas of gibber containing pebbles and larger 
blocks of stone eroded from these formations. 
Some of this material would have been utilised as 
well. 



A Model For Archaeological Site Distribution 
WiTHrN The Lake Systems 

Historical observations can be combined with 
information on the availability of stone to present 
a model of how the lake systems were utilised. 
The model makes a number of assumptions, 
namely that there is a relationship between the 
availability of water and food resources; and 
intensity of occupation as reflected by the size and 
nature of archaeological sites. Cutting across these 
factors are others relating to the availability of 
stone, the most common material found on sites. 
Using models developed by other researchers such 
as Hiscock (1987), it is hypothesised that there 
will be a general correspondence between the 
morphology of artefacts on a site and distance 
from the stone source. These models predict that 
as one moves significant distances from stone 
sources, characteristics of extreme reduction of 
stone material will be found in assemblages such 
as recycling, rejuvenation and rationing. 
Combining these different models, we can develop 
a unified set of hypotheses regarding the 
patterning of archaeological material. 



80 



E, WILLIAMS 



The Coongie system 

The Coongie lakes, with their abundance of 
food sources, and availability of water for at 
least part of the year, were areas with a high 
population density relative to other lakes in the 
region. Large and diverse occupation sites will 
be found in those areas which contain the most 
predictable and extensive areas of water. Such 
places include the permanent waterholes on the 
channels, the inlets to lakes, and those parts of 
the lakes that are deeper relative to the rest of 
the lake basin and thus hold water for a longer 
period of time. These latter areas are found on 
the southern margin, since as outlined above, the 
lakes in the region are slowly migrating 
southwards, cutting into longitudinal dunes on 
their southern shore. Their southern end is thus 
their deepest section. 

It is anticipated that given the known high 
population densities of at least the recent past, 
there will be a correspondingly high density of 
archaeological material (especially stone 
artefacts) on the large, favoured occupation 
sites. It is likely that on these sites people 
would not have moved as much compared to 
areas which contained less predictable 
resources. We can therefore expect evidence 
for the manufacturing and maintenance of 
tools such as stone artefacts. Given that the 
sites were used on a longer-term basis we can 
also expect a higher proportion of formal tool 
types than on sites with more unreliable water 
sources, and a greater proportion of finer- 
grained, good quality stone. As well, it is 
likely that a relatively larger number of 
artefacts will have edge damage from activities 
such as trampling, because of high population 
densities at the sites and residential stability 
(Scott Mitchell pers comm). 

Because it is possible that people from other 
areas may have been using these localities as 
refuges in times of resource stress, it is also 
expected that these places will contain a wider 
range of raw material than at other sites, 
including stone brought in from other regions. 
Because stone sources lay some considerable 
distance away (60+ km), primary reduction was 
unlikely to have been undertaken here and the 
stone may have been 'rationed'. Cortex, an 
indication of primary reduction, will be rare on 
pieces. Flakes and cores will be small in size 
and noticeably reduced. High population 
densities and length of site occupation may have 
exacerbated the incidence of rationing, so that 
these features will be particularly marked at the 



large sites near permanent or semi-permanent 
water. 

The salt lakes 

Given the absence of fresh water in these 
localities it is anticipated that they were not 
favoured as occupation sites. In times of high local 
rainfall it is possible that the lakes may have filled 
to some extent with rainwater run-off from the 
surrounding dunes. At these times salt levels may 
have decreased and they might have been used on 
a temporary basis as people pushed out into the 
dunefields after rain. 

The salt lakes may have had another role, as 
navigation aids for people travelling through the 
dunefield. They are often the only notable features 
present within extensive areas of dunes and are 
visible for some distance because of the sun 
sparkling on the salt surface. 

I conclude that the sites were used, albeit on a 
much more limited basis than the Coongie and 
Cordillo system. It is likely that groups using them 
were small in size and highly mobile. There is 
likely to be a correspondingly low density of 
artefacts, relative absence of formal tools, a more 
limited range of raw material types present and a 
lower proportion of good quality fine-grained raw 
material on occupation sites. Little manufacture or 
maintenance of artefacts will have been carried 
out on site. Given that the lakes are often well 
within the dunefield and thus some distance from 
stone sources, the stone discarded here will have 
been noticeably reduced. 

The Cordillo lakes 

With their better resources than the salt lakes 
the Cordillo lakes are likely to have been the 
subject of more intensive occupation but on a less 
pronounced basis than the better-watered Coongie 
system. It is anticipated that sites will be smaller 
in size than in the Coongie and fewer artefacts 
will be present. Because people occupied these 
sites for shorter periods of time it is expected that 
there will be less evidence for the manufacturing 
and maintenance of stone artefacts. A lower 
number and a smaller range of formal tool types 
will be present, and there will be less variation in 
raw material type. Larger sites are more likely to 
be located in areas of more predictable water and 
food resources such as the inlets to lakes or the 
small waterholes on channels. 

Given that the Cordillo lakes are closer to raw 
material sources than the Coongie it is expected 
that stone artefacts will not be reduced as much. 
Cores will be more common and cores and flakes 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



81 



will be heavier and larger in size, on average. A 
higher proportion of flaked pieces will contain 
cortex. 



The Archaeological Surveys: General 
Archaeological Features Of The Lake Systems 

Before presenting material on the 
archaeological sites examined as part of the study 
I will outline some of the factors affecting the 
location and recording of archaeological material 
in the field. 

The visibility of archaeological material, 
especially stone artefacts, is reasonable compared 
to many other areas. The aridity of the region 
means that dense vegetation is often absent and 
much of the ground surface is exposed. This also 
means that stone sources are relatively 
straightforward to detect. Open sites are the major 
archaeological site type in the region because rock 
formations which form rock shelter sites are 
extremely rare here. Only one shelter (a very small 
and shallow one located near Innamincka) is 
known for the whole region. Although open sites 
arc the major site type available for analysis, given 
the good ground surface visibility this is not 
necessarily the problem that it is in other regions. 
Stratified sites are extremely rare nevertheless and 
it is often very difficult to determine whether 
archaeological material is unequivocally in-situ, 
has been deflated down from other units, or 
otherwise re-deposited. 

I will present general features of the 
archaeology of the lake systems first and compare 
them with my model. In the following sections I 
will discuss more detailed analyses of 
assemblages from a sample of collected sites so as 
to make a comparison between localities within 
the region. 

The Coongie system 

The results of this work are presented in 
Williams (1988) and are briefly summarised here, 
along with other material from 1987 surveys. 
Before outlining this information it is noted that 
not all of the lakes in the Coongie system were 
surveyed for archaeological sites. Coongie itself 
was not examined because it was already being 
systematically surveyed by a team of 
archaeologists from the South Australian 
Aboriginal Heritage Branch, (now within the 
Department of State Aboriginal Affairs), in 
relation to the development of a management plan 
for the region. The results of that study are not yet 



available for analysis. Lake Goyder was not 
examined because in the years which formed the 
subject of my fieldwork (1986-1987) the lake was 
flooding out and thus conditions were not 
conducive to archaeological survey. 

The most common site type around the lakes 
surveyed for the study comprised scatters of stone 
artefacts. In all sites surveyed these scatters were 
either located within upper recent sediments or 
appeared to have deflated down from such units 
to sit as a lag on more compacted surfaces. On 
many of the sites, scatters of freshwater mussel 
shell were also present. Although not all the 
margins of every lake were examined, it appeared 
that stone and shell was present as an intermettent 
scatter intermittently around the margins of 
lakes that were surveyed (Toontoowaranie, 
Marroocutchanie). These were often present as 
small scatters of shell with numbers of artefacts, 
similar to Meehan's (1982) 'dinnertime camps'. 
Artefact density and site size increased as one 
approached permanent water sources and the 
largest sites were found in the areas outlined 
earlier - permanent waterholes on the channels, 
the inlets to lakes, and the deeper, southern 
margins of the lakes. These latter sites often 
incorporated extensive scatters of shell as well. 
Compared to the large sites, site size and density 
of material was comparatively low on the pale- 
coloured transverse dunes. On these sites stone 
artefacts and scattered termite mound hearth 
fragments were the most common form of 
material. 

Typologically, most, if not all artefacts dated to 
the mid to late Holocene. The main types noted 
were tula adzes and adze slugs, points, backed 
blades, small scrapers, cores, flakes and fragments 
of large, flat grindstones of the type described by 
Smith (1986). As well, single examples of large, 
cube-shaped silcrete cobbles which were 
commonly ground on one or more surfaces and in 
some cases also had flakes removed from edges 
and had thus been used as large cores, were often 
also present. Raw materials favoured for artefact 
manufacture were chalcedony, chert, cherty 
silcrete, a coarser-grained silcrete, and quartzite. 

Other artefacts such as edge-ground axes and 
flaked pieces of quartz crystal were also found but 
appeared to be restricted in distribution to the 
lakes most difficult to access by vehicle. It appears 
that such artefacts were formerly present on other 
lake-side sites but, together with other types of 
artefacts such as complete grindstones, have been 
removed by collectors (a conclusion supported by 
oral tradition in the region and also personal 



82 



E. WILLIAMS 



observation of collections held by individuals 
resident in the region). 

Apart from the occasional large silcrete cobbles 
and remaining grindstones left on sites, stone 
artefacts were mostly small in size and appeared 
to be noticeably reduced. As well, although 
density of stone material varied with location, even 
on sites with comparatively higher numbers of 
artefacts, density was still relatively low compared 
to artefact scatters found in many other parts of the 
continent. On the larger sites average density for 
collected sites was of the order of 6-8 artefacts/ 
square metre while on the smaller sites maximum 
densities were only 2-A artefacts/square metre. 

Occasionally larger flakes and horsehoof cores 
were found on sites or located as isolated finds 
within the dunefield or near lakes. There appeared 
to be no consistency in their location though and 
these were often in association with artefacts that 
typologically dated to the mid to late Holocene. 
As well, they were not noticeably patinated or 
weathered, and did not appear to be derived from 
Pleistocene sedimentary contexts, suggesting that 
most of these are mid to late Holocene in age. 

Hearth material, usually fragments of burnt 
termite mound, was often scattered across sites 
and isolated hearths were also present. The 
amount of hearth material rose in density on the 
larger sites and on these latter places fragments of 
bone (mostly that of fish and small mammals) 
were often found as well. The large sites are 
indeed extensive - examples up to 10 000 square 
metres and 7 000 square metres in extent 
respectively are described in Williams (1 988: 59). 

Dating of material on sites confirms that 
implied by the typology of artefacts, that is, of the 
late Holocene. Details of radiocarbon dates are 
provided in Williams (1988). 

The archaeological data is consistent with the 
ethnographic observations that the Coongie lake 
system was extensively used and densely 
populated. The presence of good quality raw 
material and a range of artefact types, including 
formal tools and manufacturing debris, suggests 
that residential stability could have been fairly 
high in comparison to other areas. This is also 
supported by the wide range of archaeological 
material present, including bone and shell. The 
small size and marked reduction of artefacts 
indicates rationing of raw material was taking 
place and this is consistent with the distance of 
the area from stone sources. 

The salt lakes 
As expected, within the areas sampled for sites 



for Coorie Coorie Tillie and Lake Deception, 
archaeological material existed in very low 
densities. At Coorie Coorie Tillie for example, 
along the 5 km stretch of the transverse dune on 
the northern margin of the lake only five isolated 
artefacts were seen: three amorphous flakes, one 
tula slug and one small core. All artefacts were 
manufactured from silcrete. Archaeological 
material was similarly rare at Lake Deception. 
Sites comprising occasional small, discrete groups 
of artefacts were found in the vicinity of both 
lakes but not within the transverse dune systems. 
Instead they were set back one or two longitudinal 
dunes from the lake margin, on the surfaces of 
small claypans. 

The sites found in these areas comprised small 
(mostly less than 30 artefacts), discrete scatters of 
stone artefacts. Density was very low, much less 
than 1 artefact/square metre. Neither mussel shell 
nor animal bone was present on these sites or on 
other parts of lake margins but occasionally 
examples of isolated termite mound hearths were 
found in association with the stone artefact 
scatters. 

One of the termite mound hearths at Coorie 
Coorie Tillie was dated. To examine particular 
features of the region's environment which may 
be affecting dates, the material was separated into 
a humic and non-humic fraction and each sample 
separately dated. The humic fraction returned a 
date of 1150 180 BP (ANU 6181) and the non- 
humic: 710 170 BP (also ANU 6181). The 
disparity in the dates can be explained as follows. 
John Head, ANU Radiocarbon Laboratory, 
confirms that the non-humic fraction, comprising 
clay particles, binds to younger carbon and clay 
material, biasing the date and making it too 
young. To account for this the non-humic 
fraction, which although comprising polymers 
which can incorporate younger carbon, was 
treated with solvents so as to extract the older 
carbon which is more likely to be reflecting the 
true age of the sample (pers. comm.). The older 
carbon is dated and the result, 1 150 180 BP, is the 
best estimate of the sample's true age. 

Apart from the differences in density and site 
composition from the Coongie sites, other 
distinguishing features were also apparent. Most 
of the artefacts were manufactured from a 
relatively restricted range of raw material, 
assemblages being dominated by a grey, 
comparatively coarse-grained silcrete. Some cores 
were present and also occasional formal tool types 
such as tulas, scrapers or points. Artefacts 
appeared to be noticeably larger than those at 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



83 



Coongie. Because of the low density of material, 
and also given the difficulty of access to the sites, 
collections of artefacts were not made when the 
sites were visited and so a more formal 
comparison between these features and other lake 
systems is not possible. The low density of 
material present on these lakes suggests that while 
they were utilised, they were not favoured for 
occupation. The restricted range of raw material 
found, its contrast in quality to the fine-grained 
material found on the Coongie system and the 
relative absence of manufacturing debris, indicates 
people used these areas on an opportunistic basis. 
The low numbers of artefacts present also 
suggests that group sizes were relatively low. 

The Cordillo lakes 

Vehicular access to the lakes was difficult 
because of their remote location and thus only one 
lake. Koonoomoorinna, was surveyed in detail. 
Reconnaissance trips to other lakes in the region 
revealed that the general patterning of sites on this 
lake is similar to that on others. 

As for other parts of the study region, the most 
common site types seen were scatters of stone 
artefacts. Formal tool types were similar to those 
observed on the Coongie sites, comprising tulas 
and other adzes, scrapers, points, fragments of 
grindstones and the large silcrete cobbles with 
ground and/or flaked surfaces. Formal types did 
not appear to be as common within assemblages 
as for the Coongie and no shell or bone was 
present on sites. The range of raw material did not 
seem as extensive and Finer grained raw material 
such as chert and chalcedony was found in lower 
densities. Artefacts appeared to be larger in size 
and not as heavily reduced. 

Hearths were also not as common and no hearth 
sites were observed on any of the sites ringing the 
immediate margin of the lake. A small number of 
hearths were found in the inter-dune corridors one 
or more dunes back from the lake margin. One, 
comprising burnt calcrete nodules, was dated and 
returned a 'modern 1 radiocarbon age (100.2, 1.8 
%M, ANU 6183), although this sample may have 
been contaminated by younger carbon from the 
surrounding locality (John Head pers. comm.). 

The densest, most extensive scatters of artefacts 
were found in those areas with the most reliable 
sources of water - inlets, the southern margin of 
lakes, and on the edges of possibly semi- 
permanent waterholes along the channels which 
connect the lakes. A large scatter along one of the 
channel waterholes contained a number of hearths. 
Intermittent, low density scatters of artefacts were 



found along the lake margins and on the 
transverse dunes to the north. 

The archaeological patterning is consistent with 
the hypothesis that the Cordillo lakes were utilised 
more than the salt lakes but less than the better- 
watered Coongie area. This is supported by the 
fact that the Cordillo sites contained a smaller 
range of archaeological material than the Coongie 
sites (no shell or bone, hearths not as common, a 
lower density of formal tool types and of better 
quality stone). The relative lack of reduction of 
artefacts could indicate either less residential 
stability or a closer distance than Coongie to raw 
material sources, or both. 

Now that I have presented general observations 
of the archaeology of the lake systems I will 
outline the results of the more detailed 
comparisons between sites. This work provides a 
more fine-grained analysis of differences that may 
exist across lake systems and between systems. 



More Detailed Comparison Of Assemblages 
From Individual Sites 

Because of the relatively low density of 
artefactual material within the region, for reasons 
of statistical analysis I only made formal 
collections from large sites. The sites analysed in 
this way are outlined below, along with the results 
of the analysis. 

Before discussing the sites it is noted that 
although some of the analysis of the material was 
published in a preliminary form by Smith, 
Williams and Wasson (1991, see for example 
Tables 1 1 and 12), a number of the figures in that 
paper vary slightly from those presented in this 
publication. This is due to the fact that the results 
of the analysis of the Coongie sites outlined in the 
1991 paper were only at a preliminary stage. The 
material presented in the current paper reflects the 
completed analysis of the assemblages. 

Sites chosen for analysis 

Five sites were chosen for analysis: 
Marroocoolcannie 2 (MCO 2), Toontoowaranie 1 
(TTW 1), Lake Lady Blanche midden (LLB), 
Koonoomoorinna inlet (KOI) and 
Koonoomoorinna second white transverse dune 
(KSW). The first three sites are located on 
Coongie lakes - their name indicates on which 
lake they are situated, and the latter two sites are 
located on the southern-most of the Cordillo lakes, 
Koonoomoorinna. All sites comprise large, 
discrete scatters of stone artefacts, together with 



E. WILLIAMS 



other material such as shell and bone in some 
cases. 

The lakes were chosen for sampling and 
analysis to determine whether there were any 
major changes in stone artefact manufacture and 
discard across the Coongie system, Each site was 
chosen because it was the most extensive seen for 
the sampled areas of that particular lake. MCO 2 
lies along the western margin of the channel 
feeding from Lake Marroolcoocannie to Lake 
Marroocutchanie. It covers an area of 
approximately 2 600 square metres and comprises 
a scatter of artefacts and shell deflating down from 
the uppermost recent unit of a pale, longitudinal 
dune. The material exists as a lag on a blow-out 
within the dune. At the western end of the site is a 
localised area of burnt shell and bone, the latter 
comprising the remains offish and small mammal 
species. A hearth, which lies on the eastern part of 
the site, dated to 1 130 1 10 BP (ANU 429). 

A baseline was laid through the middle of the 
scatter so as to bisect both the area of burnt bone 
and the hearth. All artefacts along a strip 60 m 
along the baseline and 1 m either site of it were 
collected for analysis. 

TTW 1 lies further to the north than MCO 2, 
located on the southern margin of Lake 
Toontoowaranie. It covers an area of 7000 square 
metres and comprises stone artefacts, shell and 
the remains of the collapsed, wooden framework 
of a domed hut, all lying on recent sediments on 
the top of a longitudinal dune. A sample of shell 
from the site returned a date of 330 80 BP (ANU 
5425). A 20 x 2 metre grid was laid out within the 
centre of the scatter and all artefacts within this 
were collected. 

LLB lies to the north and west of MCO 2 and 
TTW 1, on the inlet channel to Lake Lady 
Blanche, one of the terminal lakes in the Coongie 
system along with Lake Sir Richard. These two 
lakes hold water for a shorter period of time than 
those closer to the North-West Branch. When the 
lake was visited in August 1987 it was dry and 
had a salt crust on the lake floor. This was in 
contrast to the other Coongie lakes which were all 
full of water. 

The site comprises a large scatter of stone 
artefacts, shell and bone extending for 12 000 
square metres, eroding out of the uppermost units 
of a recent, white transverse dune associated with 
the inlet channel and flood-out zone of the lake. 
The bone comprises fish bone and golden perch 
otoliths. It is the largest and richest site in the 
inlet area. A 15 x 15 metre grid was laid out on 
the eastern edge of the exposure, where the 



densest scatter of shells, otoliths and artefacts was 
eroding out of the sand. All artefacts within the 
grid were collected. 

The relative lack of water in the lake compared 
to others in the Coongie system reflects the 
distribution of sites in the area. Large sites such 
as this one, which are not only extensive but 
contain a variety of material, are restricted to the 
margins of the inlet channel. Isolated scatters of 
stone artefacts are found on the surface of the 
complex of at least five separate transverse dunes 
lying to the north-east of the lake, but these sites 
are small, discrete scatters of stone artefacts and 
do not contain shell, bone or hearth material. 

Although the lake contains water on fewer 
occasions than others in the system, it was much 
favoured by Aboriginal occupants. McKinlay 
visited the lake in January 1862 and found it full 
of water, * between five and six feet deep, and 
seven and three quarter miles in circumference ... 
and tens of thousands of pelicans on it ... with 
innumerable other birds ... and plenty of fish* 
(1862: 38). There was a large camp of at least 150 
people on the lake when McKinlay was there and 
he observed that fish and 'nardoo 1 was their chief 
sustenance (1862: 42). 

For the Cordillo lake, Koonoomoorinna, two 
areas were sampled for artefacts. Both sites, KOI 
and KSW were the most extensive discrete 
scatters of artefacts seen within the vicinity of the 
lake and this is why they were chosen for analysis. 

KOI is a very extensive scatter of artefacts 
which follows the inlet to Lake Koonoomoorinna 
for several hundred metres. The site comprised 
stone artefacts only - no shell, hearths or bone 
were present. A small part of the site (10 m by 2 
m) where the densest collection of artefacts was 
found, was gridded and a collection made. 

KSW comprises a discrete scatter of artefacts 
lying as a lag within a blow-out in the second 
transverse dune north of the lake. Like KOI, only 
stone artefacts were present within the site. 

MCO 2 and TTW 1 lie 65 km from sources of 
outcropping hard rock in the Innamincka dome 
and 60 km from the Cordillo dome sources. LLB 
lies 40 km from the Cordillo dome sources and 65 
km from the Innamincka dome. KOI and KSW lie 
30 km from the Cordillo dome and 90 km from 
the Innamincka dome. 

For comparative purposes, the five lake-shore 
sites are compared with each other and also with 
one from the waterless core of the dunefield, site 
JSN. This latter site, which is reported on in 
Smith, Williams and Wasson (1991), comprises a 
scatter of stone artefacts and hearth material, and 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



85 



Table 1. Characteristics of artefacts within assemblages, 
excluding ground pieces 

Site mean weight % flakes % cores % formal 

in gm, (sd) tool types 



Table 3. Mean weights of cores (gm) 



Site 



mean 



sd 



KSW 


7.55 (17.57) 


70.4 


3.4 


3.8 


n=291 










KOI 


5.14(20.53) 


48.4 


4.2 


2.6 


n=308 










LLB 


2.65 (7.11) 


45.2 


0.6 


11.9 


n=336 










TTW1 


1.74(3.33) 


59.5 


— 


4.2 


n=264 










MC0 2 


2.17(8.32) 


50.1 


0.6 


5.6 


n=661 










JSN 


6.6 (sd not 


37.3 


2.7 


not 


n=407 


available) 






available 



is the only known Pleistocene site in the region. 
Hearths from the locality date to around 14 000, 
10 000 and 2 500 BP. Associated with the hearths 
and lying as a lag on two inter-dune pans within 
longitudinal dunes is an extensive scatter of 
artefacts. Despite the Pleistocene dates for the 
hearths, analysis of the stone artefacts strongly 
suggests that they are late Holocene in age (Smith, 
Williams and Wasson 1991: 184). 

JSN was chosen as a comparative site for the 
lakeside sites because it comprises the only known 
extensive scatter of stone artefacts for the core 
dunefield region. Most core dunefield sites only 
consist of an isolated artefact or very small 
scatters of stone artefacts (personal observation). 
The large size of the artefact sample (N = 407) 
from JSN and the fact that the artefacts appear to 
be late Holocene in age, similar in age to the 
lakeside sites, makes it the only comparative 
material currently available for the Coongie and 
Cordillo sites. 



KSW 

KOI 
LLB 
TTW1 
MC0 2 

JSN 



10 


58.29 


50.49 


13 


42.62 


81.75 


2 


13.7 


1.90 


4 


7.65 


6.56 


12 


89.2 


57.9 



% artefacts 


with cortex 


12.4 


11.0 


4.29 


9.2 


3.2 


20.0 



Table 4. Percentage of artefacts larger than 1 cm in 
length which contain cortex. 

Site 



KSW 
KOI 
LLB 
TTW 1 
MC0 2 
JSN 



Analysis of the sites 

Broad characteristics of the stone artefact 
assemblages are presented in Table 1. As 
predicted by the model, the Coongie assemblages 
have features reflecting an extreme degree of 
reduction. Artefacts (all pieces of stone on the site 
worked in some way, excluding ground pieces) 
are extremely small in size (measured by mean 
weight in grams) and cores are very rare, or even 
non-existent in the case of TTW 1 . The Coongie 
sites are very similar to each other but are different 
to both the Cordillo sites and JSN, which contain 
larger artefacts and a greater number of cores 
respectively. 

The differences in mean weight between the 



Table 2. Values of t 
weights of artefacts 



for comparison between mean 



Table 5. Raw material composition of the assemblages 
(excluding small shatter < 1cm in length and including 
ground pieces) 



Site KSW 


KOI 


LLB 


TTW 1 MCO 2 


Site 


% Finer 


% Coarser 


% Very coarse 


KSW 

KOI not 


- 




- 




grained 


grained 


grained (eg 
sandstone) 


significant 


- 




— — 


KSW (n-278) 


47.1 


41.7 


11.2 


LLB t = 4.71 


t = 2.11 


- 


- - 


KOI (n-239) 


37.2 


59.0 


3.8 


TTW1 t = 5.33 


t = 2.72 


not 




LLB (n=223) 


72.6 


19.3 


8.1 






significant 


- - 


TTW 1 (n-223) 


66.4 


27.4 


6.3 


MC0 2 t = 6.48 


t = 3.22 


not 


not 


MC0 2(n=659) 


59.8 


23.7 


16.5 






significant 


significant 


JSN(n-401) 


59.5 


33.2 


7.4 



86 



E.WILLIAMS 



Table 6. Mean weights and mean lengths of complete flakes for different raw material types. Standard deviations are 
shown in brackets. Note: Only those artefacts > 1 cm in length have been included in this analysis because of the 
difficulty in determining whether smaller pieces were derived from finer or coarser-grained raw material. Ground 
pieces and sandstone have also been excluded from the sample. 



Site 



mean weight (gm) 
of complete flakes 



mean weight (gm) 

of debitage>l cm 

in length 



Mean length (mm) 
of complete flakes 





finer 


coarser 


finer 


coarser 


finer 


coarser 




grained 


grained 


grained 


grained 


grained 


grained 


KSW 


3.9(4.1) 


12.0(18.6) 


3,2 (2.7) 


7.4(14.1) 


25.0 (9.4) 


31.7(13.6) 


KOI 


2.3 (2.6) 


6.71 (15.6) 


2.3 (2.9) 


5.0(7.1) 


17.8(7.1) 


25.2 (14.60) 


LLB 


1.3(2.0) 


2.1 (2.8) 


3.1 (4.6) 


9.3 (21.8) 


15.8(5.1) 


19.1 (6.8) 


TTW1 


0.9(1.1) 


4.8 (6.4) 


1.0(1.7) 


7.4(14.9) 


15.8(6.1) 


26.3 (14.7) 


MC0 2 


0.9(1.5) 


8.0 (24.3) 


0.9 (0.9) 


3.5 (5.3) 


15.2(5.3) 


23.5(16.2) 


JSN 


3.1 (3.2) 


4.7 (10.6) 


5.6(13.0) 


3.5 (6.4) 


not available 



Coongie and Cordillo assemblages are significant 
at the 0.05 level (Table 2). The figures for JSN are 
not available for comparison but it is anticipated 
that if they had been available, the mean weight 
of the assemblage would be statistically different 
to the Coongie sites but of the same order as the 
Cordillo assemblages. 

As predicted by the model, the three groups of 
sites are very different in relation to the reduction 
of cores (Table 3). The cores from the Coongie 
sites are extremely small and, as outlined in 
Smith, Williams and Wasson (1991:187), very 
close to the theoretical limit at which bipolar 
techniques become necessary for further reduction. 
Consistent with this is the observation that in a 
further attempt to ration raw material, worked-out 
or small, broken cores have been recycled into 
small scrapers in the Coongie assemblages (N=9 S 
mean weight = 8.2 gm, sd = 4.9). The Cordillo 
sites contain cores that are noticeably larger and 
heavier than those on the Coongie sites, while 
JSN contains on average larger cores again. There 
is no evidence that cores have been recycled as 
implements at either the Cordillo sites or at JSN. 

The Cordillo sites contain proportionately 
greater number of flaked pieces with cortex than 
Coongie (Table 4), which is as predicted given 
that they lie closer to raw material sources, 
although the figures for TTW seem high in 
comparison to the other Coongie sites. The JSN 
assemblage contains an unusually high number of 
flakes with some degree of cortex. This feature is 
unexpected and as well as the relatively larger size 
of cores and flakes, indicates that the JSN 
assemblage shows neither the effect of relatively 
large distance from stone sources, nor mediating 



responses offsetting a diminishing stock of stone 
(see Smith, Williams and Wasson 1991: 187). 
This issue is discussed in more detail later in this 
paper. 

Regarding raw material composition for 
assemblages, Table 5 shows that the Coongie sites 
contain proportionately more finer grained 
material (classified here as chalcedony, chert and 
cherty silcrete) than either the Cordillo sites or 
JSN and this is as expected (coarser-grained 
material has been classified here as granular 
silcrete and quartzite). Table 6 shows that flakes 
and debitage from fine-grained material arc on 
average smaller in size and lighter in weight than 
those from coarser-grained material, but this docs 
not explain all the variation in size between 
assemblages between sites in different areas. Fine- 
grained flakes and debitage from the Coongie sites 
are in virtually every case smaller in size and 
lighter in weight than fine-grained pieces from 
either the Cordillo sites or JSN. 

As well as these trends, the Coongie sites also 
show a wider range of raw materials as predicted. 
MCO 2 has 13 major types of raw material, TTW 
1 has eight types, LLB has seven, KOI has five 
and KSW has seven. 

In terms of the artefact analysis it was decided 
not to differentiate artefacts with retouch from 
those where this feature appeared to be absent. 
This is because of the difficulty found in 
unambiguously identifying examples of retouched 
pieces within the Coongie and Cordillo 
assemblages. Numbers of artefacts within the 
assemblages contained what I recorded in my 
analysis as 'edge damage', where I describe this 
as an edge where very small flakes had been 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



87 



removed and there is also a gloss or polish (visible 
under low-power magnification). However given 
the small size and thin cross-section of many of 
the flaked pieces it was impossible to determine 
whether this edge damage had occurred as a result 
of use, or as deliberate retouch, or from some other 
process such as flaking or trampling for example. 
Accordingly it was not possible to examine one of 
my hypotheses, that sites near more permanent 
water sources would show more edge damage 
from trampling. 

Because of the difficulties in identifying what 
had caused the edge damage, none of the statistics 
for this feature have therefore been listed for this 
analysis. It is noted that in the assemblages 
examined there were very few artefacts with 
pronounced retouch (where this involved larger 
flakes being removed along an edge and/or very 
obvious polish) which did not also comprise a 
formal tool type such as a scraper, adze, point or 
backed blade. For the very few artefacts which did 
not fit in to a formal category they were 
nonetheless listed under 'formal types' in my 
tables. 

Given that this classification methodology 
differed from that used for the JSN artefacts, it 
has not been possible to compare the two groups 
in a formal sense. Nonetheless some comparison 
are possible. 

In terms of my category of 'formal tool types', 
the Coongie sites contain a greater proportion of 
these artefacts than the Cordillo sites (Table I), as 
predicted. Adzes such as tulas and tula slugs 
formed the largest proportion of formal types in 
the Coongie sites (59% for MCO 2, 45% for TTW 
1 and 55% for LLB). The remaining implement 
types comprised scrapers, points and backed 
flakes. For the Cordillo sites in contrast there is 
greater variation in the formal types of stone tools 
represented on sites. Adzes comprised 36% of the 
formal types present at KOI but only 18% of those 
at KSW. At KOI scrapers comprise the most 
common formal type (50%) while at KSW, points, 
backed flakes and backed blades are the most 
common type at 64%. 

Regarding the artefacts comprising formal 
types, it was expected that examples will be more 
heavily reduced at sites near permanent water. 
Examining the largest sample of a formal type 
available, tula adzes and tula adze slugs, it is 
found that this is not the case. There is no clear 
trend in mean weights between the Coongie sites 
(MCO 2: mean - 8.5 gm, sd - 5.02, n = 15; 
TTW 1: mean = 3.25 gm, sd - 1.35, n = 2; LLB: 
mean - 14.18 gm, sd = 1 0. 1 , n = 1 9) or between 



the Coongie and Cordillo sites (KOI: mean = 
3.7, sd= 1.0, n = 2; KSW: mean - 6.8, sd = 2.7, 
n = 2). 

This suggests a number of factors. While 
overall characteristics of the assemblages 
presented in Table 1 show that stone was being 
curated and rationed in a very intensive way for 
the Coongie sites, the variability in size at discard 
for tulas and tula slugs, especially the relatively 
higher weights for the LLB site, suggest that 
occasionally the site occupants were not behaving 
as if raw material was as scarce as it appeared to 
be. This suggests that while certain factors such 
as the balancing of procurement of food and water 
sources with that of raw material is responsible 
for much of the variation seen on sites, people did 
not always behave as if this was the only equation 
affecting the nature of occupation and discard of 
stone artefacts. 

Although the JSN assemblage has been 
classified according to a different typology, a 
preliminary analysis of it reveals that formal types 
are rarer than at either the Coongie or Cordillo 
sites. This is consistent with the model. As well, 
it is further observed that adzes are not present on 
the site. A possible explanation for this relates to 
the lack of hardwood trees within the core 
dunefield region supplying suitable wood for 
adzing activities. The absence of such trees is very 
likely related to the availability of water - 
hardwood specimens being found on the banks of 
waterholes and lakes. 



Comparison Of The Trends In TirE Assemblages 
With Data From Other Parts Of The Arid Zone 

The trends seen in the assemblages for the 
region are also echoed in other arid zone work 
available for comparison. The major study which 
provides comparative data is that of Veth (1993) 
for the Western Desert region, Western Australia. 
His analysis shows similar patterning to that 
outlined above, with features of assemblages from 
sites at permanent waters indicating more 
intensive stone reduction than for cither semi- 
permanent waters or ephemeral water sites. His 
data show that differences in intensity of reduction 
are not as clear between semi-permanent and 
ephemeral water sites as they are between these 
sites and more permanent ones (see 1993: Tables 
8.21-8.31). For a number of features, ephemeral 
sites show trends characteristic of more intensive 
reduction than semi-permanent sites, which is not 
predicted by Veth's model. This appearance of 



88 



E. WILLIAMS 



conflicting trends also appears to be echoed by 
comparisons between the Cordillo sites and JSN. 
The sites are more similar to each other than they 
are to the Coongie sites but there is much 
variation in the nature and direction of trends 
between the two groups. This suggests that the 
permanent sites, in Veth's sample and mine, form 
clear groups but other sites, while showing some 
similar trends, are more variable. 

The association of higher proportions of formal 
types in assemblages, especially adzes, with more 
predictable water sources, is also a trend noted by 
Veth (1993: 95-96). Veth also found that there 
was some patterning in the amount of reduction of 
tula adzes and relation to water sources but that 
there was a considerable degree of variation 
(1993: 98-101) and this is also found in my 
samples. 

In his discussion of his results of the artefact 
analysis, Veth concludes that the timing and 
intensity of site use are the major factors 
responsible for variation in the assemblages, 
rather than distance to raw material sources and 
the operation of specific discard criteria (1993: 
101). This also seems to be the case for the north- 
east South Australian sites, as I will outline 
below. 



Major Factors Affecting The Patterning Of 
Sites In The Region 

One of the predictions of my model of site 
patterning is that apart from water sources, 
availability of stone sources is be one of the most 
important factors responsible for trends seen and 
that Aboriginal occupants favoured raw material 
sources closest to the site. 

An examination of the JSN assemblage reveals 
that the people who visited the site did not behave 
in this manner. Rather than using the closest stone 
to the site (40-50 km to the east) for artefact 
manufacture and discard, the sourcing of stone 
artefacts from the site indicates that they instead 
used stone from Della-Dullingari which lies 115 
km away, to the north-east (Smith, Williams and 
Wasson 1991: 185). Despite the use of such 
distant material, the assemblage does not have 
features characteristic of extreme reduction 
(Smith, Williams and Wasson 1991: 185-189). 
Cores have not been noticeably curated and have 
not been recycled as other implements. Mean 
weight of artefacts is significantly greater than for 
the Coongie sites, despite the fact that utilised 
stone sources are considerably further away than 



for the Coongie. Flaked pieces contain much 
higher proportions of cortex, also consistent with 
less intense reduction. 

The patterning of the JSN assemblage is 
characteristic of a situation where raw material is 
closer rather than further away. Yet the paradox 
can be resolved if we instead see stone source 
utilisation in terms of re-supply time rather than 
just in terms of linear distance of stone source 
from occupation site. For example, if people 
stopped at JSN as part of a journey to the Della- 
Dullingari region, they would have been aware 
that they were only a couple of days away from 
being able to replenish stone sources. As well, it 
is likely that the duration of visits to the JSN were 
relatively short, so that the demand for stone was 
easily met by the stock-in-hand without recourse 
to the recycling and the extreme reduction of stone 
evident at the Coongie sites (Smith, Williams and 
Wasson 1991: 188). 

The JSN site shows that it is not necessarily 
linear distance from the closest stone sources that 
is a major factor in the patterning of stone artefact 
manufacture and discard. The key factors are 
instead the length of time spent at the site, which 
in turn relates to the length of time before the 
group could replenish stone sources. 

This line of reasoning can be applied to the 
Coongie sites as well. The extreme reduction of 
stone reflected by the assemblages can be seen as 
the archaeological correlate of residential stability 
within the lake system relative to other 
environments in the region. It appears that people 
chose to stay closer to the lakes even if it meant 
that they were restricting their access to stone, 
thus triggering what appears to have been 
significant pressure on the way they used the 
resource. This is despite the fact that they could 
have chosen to be more mobile, travelling more 
often between stone sources and the lakes. In this 
latter case, features of such extreme reduction 
would not be visible in assemblages. 

Therefore, like Veth for the Western Desert 
region, I see the main determinant of site 
patterning in the Coongie and surrounding areas 
as relating to the timing and intensity of site 
use rather than to distance from raw material as 
such. 

This indication of relative residential stability in 
the Coongie, combined with the high population 
densities observed in the area at the time of 
contact implies that the system may have been 
vulnerable to significant stress given the extreme 
environmental fluctuations characteristic of the 
region. It is likely that the system worked 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



89 



smoothly when resources were abundant but in 
cases when an anticipated flow of fresh water 
failed to come down the Cooper or when there 
was widespread drought, it is possible there were 
major problems. The fact that the current situation 
where the Coongie captures most, if not all of the 
Cooper flow, is potentially very unstable and 
channel flow could be completely switched on 
and off as a result of only slight environmental 
shifts, would exacerbate this. 

Ethnographic observations support the notion 
that stresses were operating on the system. The 
rigid sanctions outlined earlier involving the 
enforcement of group boundaries and access to 
resources indicate this, along with the 
information that many people in what is now the 
north-east South Australian region perished 
during droughts. Further, Wasson's observation 
of a dune mobilisation event in the late Holocenc 
that might be linked to the intensity of the 
occupation of the region, is another feature that 
suggests the system might have been under some 
stress. 

Evidence for 'intensification '? 

It is tempting to suggest that the characteristics 
of the mid-late Holocene occupation of the region 
reflect an intensive settlement pattern and are 
derived from a process of 'intensification' (see 
also Williams 1988: 61). For example, all of the 
dates for occupation sites for the Coongie system 
fall within the late Holocene and on all sites 
recorded within the region, including JSN, the 
typology of artefacts suggests a mid-late Holocene 
date. While it is tempting to conclude the region 
does provide evidence consistent with the 
operation of such a process, as in my 1988 paper I 
am cautious about maintaining that these features 
provide definite evidence. I take this position 
because it is likely that the environmental 
instability could be causing major biases in the 
archaeological record. Such instability could be 
selectively removing older sites from the 
archaeological record, or rendering them 
archaeologically invisible through sedimentation, 
or even resulting in vast fluctuations in channel 
flow thus affecting the filling of lakes. I therefore 
conclude that while the evidence for 
intensification is persuasive, further 
geomorphological work is needed to more fully 
expand on factors affecting the visibility of 
archaeological material. 

Given these issues, can any conclusions can be 
drawn about the occupation of the arid zone, 
especially that of the more distant past? 



Early Occupation Of The Arid Zone 

1 will conclude the paper with some brief and 
speculative comments about models relating to 
when the arid zone was first occupied on a 
consistent basis. 

As noted in Smith, Williams and Wasson 
(1991: 190) the evidence from the JSN site 
indicates regular use of the dunefield region 
during the late Pleistocene, when there was 
probably also occupation of the riverine corridors. 
The presence of Velesunio shell at JSN in a 
Pleistocene context is tangible evidence of some 
link with these riverine habitats. The nature of the 
archaeological material present on the site 
suggests that late Pleistocene use did not involve 
much on-site stone working and that this changed 
some time during the mid-late Holocene when 
visits to the area appear to have become more 
prolonged and to have involved the grinding of 
seeds and the manufacture and maintenance of 
chipped stone artefacts (ibid). 

Dating of hearths to the period around 12 000 
BP for hearths on the lower reaches of Coopers 
Creek (Veth, Hamm and Lampert 1990) is also 
consistent with late Pleistocene occupation of 
what is now north-east South Australia. 

Despite the presence of the dunefield site of 
JSN, Veth (1993) has developed a model 
suggesting that the continent's core arid zones 
were only colonised as recently as 5 000 years 
ago. Veth maintains that the evidence for 
Pleistocene occupation of JSN does not disprove 
his model since the Strzelecki dunefield region is 
located within an area of co-ordinated drainage, 
thus implying that it was not part of the core arid 
zone (1993: 111). 

Veth's model is an interesting one, but it could 
prove difficult to test. His 'core arid zones' 
comprise the deserts of the Great Sandy Desert, 
Great Victoria and Simpson Deserts. These 
regions are by definition sandy deserts and are 
thus areas where outcrops of hard rock are rare 
and therefore rock shelters with potential 
Pleistocene sediments are either non-existent or 
uncommon. Rockshelters such as those examined 
by Veth (1993) in the Gibson Desert, have late 
Holocene occupation resting directly on bedrock 
and thus do not provide contexts for the 
examination of occupation (or the lack of it) for 
the period before the late Holocene. 

The fact that the presence of rockshelter sites 
which preserve Pleistocene sediments is so crucial 
for the examination of whether Pleistocene 
occupation took place or not, is shown by Veth's 



90 



E. WILLIAMS 



discussion of his model (1993: Chapter 9). All of 
the eleven Pleistocene sites and early Holocene 
sites which lie a considerable distance from co- 
ordinated drainage, and thus form the basis of his 
model, are rockshelters. 

Knowing that rockshelter sites which preserve 
Pleistocene sediments are likely to be extremely 
rare in the regions important for Veto's model, it is 
also unlikely that Pleistocene open sites will be 
easy to locate. Extensive outcrops of hard rock are 
not common in the sandy deserts and thus stone 
suitable for the manufacture of artefacts is also a 
scarce commodity. It is therefore likely that stone 
artefact manufacture, one of the maj or 
archaeological indicators of human occupation, has 
to take place on a relatively intensive basis before it 
becomes archaeologically visible in these regions. 
The JSN site for example indicates that Pleistocene 
occupation is not as archaeologically visible as 
regards stone artefact discard as is mid-late 
Holocene occupation. This evidence is 
complemented by my findings for the study area 
that artefacts do not appear to be present within 
visible Pleistocene contexts. This is despite that fact 
that we know from the evidence of JSN that people 
were using the region during the late Pleistocene. 

Further, the logistical difficulties of carrying out 
systematic archaeological surveys for sites in 
remote locations such as sandy deserts, compound 
these problems. JSN was not found as the result 
of systematic archaeological sampling but was 
instead located virtually by accident during the 
course of a geomorphological study of the 
dunefield by Wasson. 

The question of when the core arid zones were 
first occupied on a systematic basis thus remains 
a challenging one. Until this question is resolved, 
JSN remains the continent's sole example of a 
Pleistocene site located within the midst of the 



continental dunefield, albeit a dunefield in the 
vicinity of co-ordinated drainage. The spur to the 
finding of Pleistocene sites within Veth's 'core 
arid zones' will be to expand further on the nature 
of the continent's Pleistocene occupation and to 
also determine the antecedents of the patterning 
seen in the mid-late Holocene. 



Acknowledgments 

The project reported on in this paper was funded 
jointly by the National Research Fellowship Scheme and 
the Department of Prehistory, Research School of Pacific 
Studies, (now the Division of Archaeology and Natural 
History), the Australian National University. I thank 
these bodies for support. The Australian Heritage 
Commission also provided some assistance and I thank 
Betty Meehan particularly in this regard. Bob Wasson 
was instrumental in encouraging me to initiate the 
Coongie project and I especially thank him for his advice 
and support during the course of the work. SANTOS 
provided much logistical support for fieldwork and I 
particularly thank Oleg Morozow and Steve Tunstall for 
their assistance. The Aboriginal Heritage Branch gave 
permission for collection of sites and the excavation of 
JSN. Chris Dodd (then Aboriginal Liaison Officer, SA 
NPWS) gave approval for the excavation of JSN and I 
especially thank him for his assistance with work on the 
site. I wish to thank all of the people who provided 
assistance in the field: Doreen Bowdery, Nick Drayson, 
Ros Fraser, Parry Kostiglou, Gary Dunnett, Pam and 
Colin McDonald, Ben Smith, Barney Stevens, Steve 
Sutton, and Keryn Walsh. I am also indebted to Barry 
Saunders and Vince for their advice and support in the 
field, and the Royal Flying Doctor Service whose radio 
network was invaluable in such a remote area. I 
particularly thank my co-worker at JSN, Mike Smith; 
useful advice and discussion on ideas in this paper were 
provided by him, Bob Wasson and Barry Cundy. I am 
also especially grateful to Win Mumford for her work 
on the maps and illustrations. 



References 



BURKE, R. O. & WILLS, W. J. 1861. 'The Burke and 
Wills Exploring Expedition'. Wilson & Mackinnon: 
Melbourne. 

CALLEN, R. A. and BRADFORD, J. 1992. The Cooper 
Creek fan and Strzelecki Creek - hypsometric data, 
Holocene sedimentation and implications for human 
activity. Mines and Energy Review, South Australia 
158: 52-57. 

HISCOCK, P. 1981. Raw material rationing as an 
explanation of assemblage differences: a case study 
of Lawn Hill, north-western Queensland. Pp. 178- 
190 in 'Archaeology at ANZAAS, Canberra'. Second 



printing. Ed. G K Ward. Canberra Archaeological 
Society: Canberra. 

HUGHES, P. J. & LAMPERT, R. J. 1980. 

Pleistocene occupation of the arid zone of south- 
east Australia: research prospects for the CoopeT 
Creek-Strzelecki Desert region. Australian 
Archaeology 10: 52-67. 

JONES, W. 1979. 'Up the creek: hunter-gatherers in the 
Cooper Basin.' B.A. (Hons) thesis, University of 
New England: Armidale. 

KERWIN, B. & BREEN, J. G. 1981. The land of stone 
chips. Oceania 51: 236-31 1. 



ARCHAEOLOGY OF THE MIDDLE COOPER BASIN 



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KREIG, G. W. & CALLEN, R A. 1990. Coongie Lakes 
Control Zone - a map and note for the surface 
geology and terrain. Mines and Energy Review, 
South Australia 157: 59-61. 

LAYTON, R, FOLEY, R, & WILLIAMS, E. 1991. The 
transition between hunting-and-gathering and 
specialized husbandry of resources. Current 
Anthropology 32: 255-274. 

MCBRYDE, I. 1987. Goods from another country: 
exchange networks and the people of the Lake Eyre 
Basin. Pp. 252-273 in 'Australians to 1788'. Ed. D. 
J. Mulvaney & J. P. White. Fairfax, Syme and 
Weldon Associates: Sydney. 

MCKINLAY, J. 1862. 'McKinlay's Journal of 
Exploration in the Interior of Australia'. F. Balliere: 
Melbourne. 

MACUMBER, P J. 1980. The influence of groundwater 
discharge on the Mallee landscape. Pp. 67-84 in 
'Aeolian Landscapes in the Semi-arid Zone of South- 
eastern Australia. Eds. R. R. Storrier & M E 
Stannard. Australian Society of Soil Science: Wagga 
Wagga. 

MEEHAN, B. 1982. 'Shelibed to Shell Midden'. 
Australian Institute of Aboriginal and Torres Strait 
Islander Studies: Canberra. 

REID, J. R. W. & GILLEN, J. 1988. The Coongie 
Lakes Study. Unpublished consultancy report to the 
South Australian Department of Environment and 
Planning: Adelaide. 

REID, J. R. W. & J. T. PUCKERIDGE. 1990. Coongie 
Lakes. Pp. 119-131 in 'Natural history of the north- 
east deserts'. Ed. M. J. Tyler, C .R. Twidale, M. 
Davies and Wells, C. B. Royal Society of South 



Australia Occasional Publications 5. Royal Society 
of South Australia: Adelaide. 

REUTHER, J. G. 1981. 'The Diari'. Volumes 1-13. 
Translated by the Reverend P. A. Schcrer. Australian 
Institute of Aboriginal and Torres Strait Islander 
Studies, Canberra. 

SMITH, M. A. 1986. The antiquity of seed-grinding in 
Central Australia. Archaeology in Oceania 21: 29-39. 

SMITH, M. A., WILLIAMS, E, & WASSON, R. J. 
1991. The archaeology of the JSN site: some 
implications for the dynamics of human occupation 
in the Strzelccki desert during the late Pleistocene. 
Records of the South Australian Museum 25: 175- 
192. 

TWIDALE, C. R. 1972. Landform development in the 
Lake Eyre region, Australia. The Geographical 
Review 62: 40-70. 

VETH, P. M. 1993. Islands in the Interior: the dynamics 
of prehistoric adaptations within the arid zone of 
Australia. International Monographs in Prehistory. 
Archaeological Series 3 

VETH, P. M, HAMM, G. & LAMPERT, R. J. 1990. The 
archaeological significance of the Lower Cooper 
Creek. Records of the South Australian Museum 24: 
43-66. 

WASSON, R J. 1986. Geomorphology and Quaternary 
history of the Australian continental dunefields. Pp. 
419-432 in J. C. Vogel, Ed. 'Late Cainozoic 
Palaeoclimates of the Southern Hemisphere'. A. A. 
Balkema: Rotterdam. 

WILLIAMS, E. 1988. The archaeology of the Cooper 
Basin: report on fieldwork. Records of the South 
Australian Museum 22: 53-62. 



REVISION OF AUSTRALIAN AMPHIOPS ERICHSON, ALLOCOTOCERUS 
KRAATZ AND REGIMBARTIA ZAITZEV (COLEOPTERA: HYDROPHILIDAE) 

C.H.S. WATTS 
Summary 



The Australian members of the Hydrophilid genera Amphiops (five species), Allocotocerus (three 
species) and Regimbartia (one species) are revised and redescribed. Keys to species of Amphiops 
and Allocotocerus are given. Amphiops austrinus, Amphiops micropunctatus and Allocotocerus 
yalumbaboothbyi are described as new. 



REVISION OF AUSTRALIAN AMPHIOPS ERICHSON, ALLOCOTOCERUS KRAATZ AND 
REGIMBARTIA ZAITZEV (COLEOPTERA: HYDROPHILIDAE) 



C. H. S. WATTS 



WATTS, C. H. S. 1998. Revision of Australian Amphiops Erichson, Allocotocerus Kraatz and 
Regimbartia Zaitzev (Coleoptera: Hydrophilidae). Records of the South Australian Museum 
30(2): 93-106. 

The Australian members of the Hydrophilid genera Amphiops (five species), Allocotocerus 
(three species) and Regimbartia (one species) are revised and redescribed. Keys to species of 
Amphiops and Allocotocerus are given. Amphiops austrinus, Amphiops micropunctatus and 
Allocotocerus yalumbaboothbyi are described as new. 

C. H. S. Watts, South Australian Museum, North Terrace, Adelaide, South Australia 5000. 
Manuscript received 15 April 1997. 



The three genera included in this revision are 
grouped for convenience not phylogeny although 
both Allocotocerus Kraatz, 1883 and Regimbartia 
Zaitzev, 1908 belong in the same tribe (Berosini) 
and they and Amphiops Erichson, 1843 are 
frequently mixed together in collections. All are 
wet-tropical beetles with, at the generic level, a 
wide distribution outside Australia (Hansen 
1991). They are all relatively small very deep- 
bodied insects with Amphiops and Allocotocerus 
having almost spherical bodies. They occur 
commonly in pools and swamps around the 
tropical coast from the Kimberley to about 
Sydney. 

The most recent taxonomic work on the 
Australian species was by J. Balfour- Browne who 
briefly commented on them and described 
Allocotocerus tibialis and Amphiops 
queenslandicus (Balfour-Browne 1939) and 
Hansen, 1991 who discussed their generic 
placement. 

Material was examined from the following 
collections. 

AM Australian Museum, Sydney 

ANIC Australian National Insect Collection 
BM(NH) Natural History Museum, London 
NMV Museum of Victoria 
NTM Northern Territory Museum 

QDPIM Queensland Department of Primary 

Industries, Mareeba 
QM Queensland Museum, Brisbane 

SAMA South Australian Museum, Adelaide 
UQIC University of Queensland Insect 

Collection, Brisbane 
WAM Western Australian Museum, Perth. 



Systematics 

The three genera can be separated from other 
Australian aquatic Hydrophilids by the following 
characters (after Hansen 1991). 

Amphiops: Size 2.5^.5 mm. Dark brown to 
black. Eyes divided into upper and lower portions 
by extensions of side of head. Elytra 
approximately as high as long, without striae. 
Meso- and meta-tibiae without swimming hairs. 
First ventrite very short, with a fringe of fine setae 
rising from its basal margin. 

Allocotocerus: Size 3.5^.5 mm. Black. Meso- 
and meta-tibiae with swimming hairs. Eyes 
normal. Elytra as high as long, virtually without 
striae. 

Regimbartia: Size 3.5-5.0 mm. Black. Meso- 
and meta-tibiae with swimming hairs. Eyes 
normal. Elytra high, about 2.8x longer than 
height, with distinct striae. 

For more detailed descriptions and discussion 
of the affinities of these genera see Hansen, 1991. 



Amphiops Erichson, 1843 

Australian Amphiops are all very similar and 
are best separated by the male genitalia. Indeed I 
have found it impossible to reliably separate A. 
queenslandicus J. Balfour-Browne and A. 
duplopunctatus Blackburn by any other means. 
The best general character is the form of the 
clytral punctation, in particular the interstrial 
punctation on the sides of the elytra. There are 
three more or less distinct size classes of elytral 
interstrial punctures: 1) large, about the size of 
the strial punctures; 2) small, between about 20- 



94 



C. H. S. WATTS 



60% of the larger ones; 3) micro, which are 
normally no more than pin pricks even under 
moderate magnification. 



Key to Australian Amphiops 

Interstrial punctures consisting of a few large 
punctures and a few to numerous micro 
punctures, the small size seemingly absent 
(Figs 1&3). Systematic punctures on pronotum 
large and distinct 2 

Interstrial punctures consisting of large, small 
and micro punctures with small predominating 
(Figs 2 & 4) 3 

Central lobe of aedeagus not hooked (Fig. 13). 
First elytral stria (close to suture) distinct, 
traceable (anteriorly) well beyond apex of 
scutellum. Scutellum always moderately 
punctate A. micropunctatus sp.nov. 

Central lobe of aedeagus hooked at tip (Fig. 
14). First elytral stria virtually absent. 
Scutellum lacking punctures or weakly 

punctate with very small punctures 

A. australicus Blackburn. 

Central lobe of aedeagus hooked at tip (Fig. 9). 
Small punctures on sides of elytra relatively 
small, < 1/4 diameter of adjacent large 
punctures (Fig. 4). Serial punctures easily 
traceable at apex A. austrinus sp.nov. 

Central lobe of aedeagus rounded, parameres 
straight. Small punctures on sides of elytra 
relatively large, many 1/2 size of adjacent 
punctures (Fig. 2). Serial punctures may be 
hard to trace at apex 4 

Basal portion of aedeagus shorter than 
parameres (Fig. 10). Size <3.9 mm. Elytra 
often with a vague series of darker patches in 
alternate interstriae 

A. duplopunctatus Blackburn 

Basal portion of aedeagus nearly twice length 
of parameres (Fig. 11). Size > 3.5 mm. Elytra 
without series of dark patches 

A. queenslandicus J. Balfour-Browne. 



Amphiops austrinus sp. nov. 

Description (number examined 5) Figs 4, 9 

Length 3.4-4.0 mm. Broadly oval, elytra deep, 
almost as high as long. Reddish-brown, disk of 
pronotum a little darker as are serial punctures. 
Head broad, strongly punctate with variously 
sized punctures, confluent at front. Pronotum 
broad, punctures of various sizes, weak on disk 



grading to strong laterally, systematic series 
distinct. Elytron very weakly punctured near 
suture, grading to strong laterally; in middle at 
side serial punctures strong, large, somewhat 
difficult to trace; large punctures separated by 
own diameter or a bit less, small punctures, which 
alternate with larger ones, are very much smaller; 
interstrial punctures of three distinct sizes, largest 
as large or larger than those in serial lines, 
separated by own width or less, small punctures 
more numerous, very much smaller, 1/4-1/3 
diameter of large ones, in places third size group 
of minute (micro) punctures present. 

Aedeagus squat, basal portion shorter than 
parameres. Apical portion of central lobe narrow, 
weakly tapering, considerably shorter than 
parameres, ending in small broad hook. Parameres 
broad in basal half, narrow in apical, strongly 
curved downwards near tip, tips truncated and a 
little enlarged. 

Distribution 

Only known for the type localities in south-east 
Queensland. 

Types 

Holotype: 'Brisbane 1/64, CW\ SAMA. 

Paratypes: 4, 'Qld Pctrie, 10 km W, 23/1 1/95, 
C. Watts', SAMA. 

Remarks 

In most characters similar to A. duplopunctatus 
and A. queenslandicus. Apart from the male 
genitalia A. austrinus differs from both of these 
by the greater contrast in size between the large 
and small interstrial punctures on elytra, caused 
primarily by the comparatively small size of the 
small punctures. In A. duplopunctatus and A. 
queenslandicus the small interstrial punctures 
become quite prominent towards the side and 
apex, often reaching half the size of the larger 
ones. In A. austrinus, apart from very near the 
elytron edge, the small punctures remain much 
smaller than the larger ones. The downward curve 
of the parameres and the apical hook on the tip of 
the central lobe of the aedeagus, also clearly set it 
apart from these two species. 



Amphiops australicus Blackburn, 1898 

Description (number examined 234 ) Figs 3, 14 

Length 2.7^.0 mm. Broadly oval, elytra deep, 
about as high as long. Brown, sometimes with 
distinct darker blotches on elytron, to black with 



AMPHIOPS, ALLOCOTOCERUS AND REGIMBARTIA 



95 



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FIGURES 1^4. Pattern of punctures near anterior-lateral angle of elytron. 1, Amphiops micropunctatus; 2, Amphiops 
duplopunctatus; 3, Amphiops australicus; 4, Amphiops austrinus. 



some vague lighter areas. Head broad, moderately 
to strongly punctate, punctures mainly small with 
scattered much larger ones, becoming stronger 
and denser in front, confluent and rugose along 
front margin. Pronotum broad, weakly punctured, 
punctures almost obsolete on disk but becoming 
stronger laterally, much smaller than eye facet, 
systematic punctures small, about size of eye 
facet. Elytra weakly punctured on disk, becoming 
stronger laterally. At side in middle, serial 
punctures about puncture-width apart, lacking 
alternating small punctures. Interstrial area usually 
only with large punctures which are 
approximately same size, and approximately same 
size as serial punctures, about a puncture-width 



apart or somewhat greater. Areas of elytra near 
the scutellum and laterally may have indistinct 
micro punctures. 

Aedeagus elongate, basal piece about same 
length as parameres. Central lobe narrow, 
narrowing to point, tip with upward hook, shorter 
than parameres. Parameres elongate, broad in 
basal half, narrow in apical, tips weakly expanded, 
curved downwards in apical fifth. 

Type 

Holotype female: '5074T', 'Adelaide R, NW 
Australia, J. J. Walker', 'Blackburn Coll 1910- 
236', 'Amphiops australicus, Blackburn', with 
round type label, BM(NH). Seen. 



96 



C. H. S. WATTS 



Distribution 

Northern Territory 

11 km SW by S Borroloola, ANIC; Cahills 
Crossing, ANIC; 7 km NW by N of Cahills 
Crossing, ANIC; Gimbar Stn, NTM; Howard 
Springs, SAMA; Holmes Jungle, NTM; Jabiru, 
NTM; Junction of Arnhem Hwy and Oenpelli Rd, 
NTM; Kakadu NP, NTM; Koongarra, ANIC; 
Magela Ck, ANIC; McArthur R, ANIC; 19 km E 
by S of Mt Borradaile, ANIC; 30 km WSW Mt 
Cahill, ANIC; 9 km N of E Mudginbarry HS, 
ANIC; Nourlangie Ck, ANIC; 18 km E by N 
Oenpelli, ANIC; Tindale, ANIC, NMV; UDP 
Falls, NTM; 12°40S 132°54E, ANIC; 12°06S 
133°04E,ANIC. 

Queensland 

12°08S 142°16E, ANIC; 12°22S 142°37E; 
12°06S 142°33E, ANIC; 14°51S 142°58E, 
ANIC; 18°33S 138°11E, ANIC; Archer Bend, 
SAMA; Batavia Downs HS, ANIC; Barron 
Falls, ANIC; Bertiehaugh Ck, ANIC; Cairns, 
ANIC; 110 km S Coen, NMV; East Claudie R, 
UQIC; 110km S Coen, NMV; 70 km SW 
Greenvale, SAMA; Hann R, ANIC; Lakefield 
NP, QDPIM; 50M N. Laura, UQIC; 72 km NW 
Laura, ANIC; 21 km E Mareeba, QDPIM; 
Moreton, ANIC; 2 km NNE Mt Tozer, ANIC; 9 
km ENE Mt Tozer, ANIC; 3 km NE Mt Webb, 
ANIC; 10 km WNW Rokeby, ANIC; Wenlock 
R, ANIC. 

Western Australia 

14°25S 126°40E, ANIC; 14°52S 125°50E, 
ANIC; 14°52S 125°50E, ANIC. 

Remarks 

Among Australian Amphiops, A. australicus 
can only be confused with A. micropunctatus due 
to the virtual lack of small and micro punctures on 
the elytra. Amphiops micropunctatus has more 
extensive micro punctures over the elytra but these 
can be missed if the specimen is at all dirty or the 
light poor. The two species are best separated by 
the much more strongly punctate scutellum and 
the quite well developed first elytral stria on A. 
micropunctatus, compared to the virtually 
impunctate scutellum region in A. australicus. I 
have not seen any black specimens of A. 
micropunctatus but light coloured A. australicus 
are occasionally encountered, usually with well 
marked dark patches on elytra. The tip of the 
aedeagus in A. australicus is hooked, in A. 
micropunctatus it is not. 



Amphiops duplopunctatus Blackburn, 1898 

Description (number examined 65 ) Figs 2,10 

Length 3.0-3.9 mm. Broadly oval, elytra deep, 
as high as long. Dark reddish-brown, elytra with 
vague lighter patches. Head broad, strongly 
punctate, punctures of varying size, often 
becoming confluent along front margins. 
Pronotum broad, weakly punctured on disc, 
becoming stronger laterally, punctures of various 
sizes, systematic series moderately distinct, 
relatively small, about same size or a little larger 
than eye facets. Elytra weakly and shallowly 
punctured on disc, becoming much stronger 
towards sides. At side, in middle, serial punctures 
large, easy to trace, each separated by own width 
or less, alternating with a small puncture. 
Interstrial punctures of three sizes, largest a bit 
smaller than serial punctures and most separated 
by more than their width, small punctures much 
more numerous and 1/3-1/2 diameter of large 
ones, numerous and relatively large micro 
punctures. 

Aedeagus with basal piece shorter than 
parameres, apical portion of central lobe 
narrowing to thin point, lacking any apical 
thickening or hook, shorter than parameres. 
Parameres wide in basal half, narrow in apical 
half, tips rounded not curved. 

Types 

Holotype female: '6370 Qu. T.', 'Blackburn 
Coll 1910 236', 'Amphiops duplopunctatus, 
Blackburn', BM(NH). Seen. 

Lectotype: 'Queensland Blackburn's Coll.', 
'Amphiops duplopunctatus BL. co-type', 
dissected and remounted, SAMA. Seen. 

Distribution 

Northern Territory 

Daly R Crossing, NTM, ANIC; Darwin, 
ANIC, NTM, SAMA; 11km NE of E of 
Darwin, ANIC; Gimbat Stn, NTM; Holmes 
Jungle, ANIC, NTM, SAMA; Howard River, 
NTM; Howard Springs, NTM, SAMA; 
Humpty Doo, NTM, QDPIM; 10 km N of 
Jabiru, NTM, QDPIM; 29 km W by N Jabiru, 
NTM, ANIC; Keep River NP, NTM, ANIC; 
Magela Ck, ANIC; 12 km NNW Mt Cahill, 
NTM, ANIC; 19km WSW Mt Cahill, ANIC; 
9km N by E of Mudginbarry, ANIC; Nabarlek 
Dam, ANIC; 6km SW by S Oenpelli, ANIC; 
Sth Alligator R, ANIC; 15 km SE Wangi, 
NTM; Yungaburra, NTM, QDPIM; 16°02S 
130°23E, NTM. 



AMPHIOPS, ALLOCOTOCERUS AND REGIMBARTIA 



97 



f 











FIGURES 5-8. Ventral view of mesofemur (top) and metafemur (bottom). 5, Male Allocotocerus yalumbabooihbyi, 
6, Female Allocotocerus yalumbaboothbyi; 7, Male Allocotocerus tibialis; 8, Female Allocotocerus tibialis. 



Queensland ANTC; Caloundra, SAMA; Claudie R, UQIC; 

Bamaga, SAMA, UQIC; Barringtonia Lagoon Dalhousic R, ANIC; East Claudie R, UQIC; 

W Cape York, QM; Batavia Downs HS, ANIC; Flinders Is, SAMA; 12 km SW Heathlands, 

Bertihaugh Ck, ANIC; 8 km N Bluewater, ANIC; Holroyd R, ANIC; Iron Range, UQIC; 

SAMA; 9km N Bluewater, SAMA; Burster Ck, Jordine R, UQIC; Kuranda, SAMA; Lawn Hill, 



98 



C. H S. WATTS 



ANIC; Lake Barrine, AN1C; Lake Tinaroo, 
ANIC; 73km NW of W Laura, ANIC; Lockerbie, 
UQIC; 9 km NNW Lockhart R, ANIC; 18 km N 
Mareeba, QDP1M; Mazlin Ck, QDPIM, ANIC; 3 
km ENE Mt Tozer, ANIC; 9 km ENE Mt Tozer, 
ANIC; 11 km ENE Mt Tozer, ANIC; Murphy's 
Ck, UQIC; Normanby R, ANIC; Pascoe R, ANIC; 
N Pine River, QM; Redcliffe, UQIC; Ripley, 
SAMA; 27km NW by W Rokeby, ANIC; 
Schramm Ck, ANIC; Townsville, SAMA, 20km S 
Townsville, SAMA; 3 km WSW Ussher Point, 
ANIC; Wenlock R crossing, ANIC; 18°35S 
138°03E, ANIC; 18°40S 138°20E, ANIC. 

Western Australia 

Carson Escarpment, ANIC; Drysdaie R, ANIC; 

Remarks 

If reference material is available A. 
duplopunctatus can be relatively easily separated 
from A. austrinus by its stronger interstrial 
punctation, but lacking reference specimens it can 
only be separated with certainty from this species 
by its aedeagus. 

Typical A. duplopunctatus are smaller, higher 
and often darker than A. queenslandicus and have 
stronger large punctures on elytra. In many A. 
duplopunctatus, particularly from the Northern 
Territory, many of the large serial punctures on 
the sides of the elytra are less than a puncture- 
width apart, a condition I have not seen in any A. 
queenslandicus. Except for particularly dark 
specimens, A. duplopunctatus usually has quite 
regular darker blotches in alternate elytral 
interstriae variably distinct. Amphiops 
queenslandicus lacks these and has more 
uniformly coloured elytra although the punctures 
are often darker particularly laterally. Amphiops 
duplopunctatus is also smaller than A. 
queenslandicus (<3.9 mm as compared to >3.5 
mm). 

Balfour-Browne (1939), considered A. 
duplopunctatus to be possibly no more than a 
subspecies of A. australicus, an opinion based 
mainly on a perceived close similarity of the male 
genitalia. The male genitalia of what I take to be 
A. australicus and A. duplopunctatus are clearly 
distinct (the types are female). The markedly 
different punctation also differentiates the two 
species. 

Amphiops micropunctatus n. sp. 

Description (number examined 30) Figs 1,13 
Length 2.7-4.3 mm. Oval, elytron deep, a little 



longer than high. Reddish-brown, punctures on 
elytron darker. Head broad, moderately strongly 
punctate, punctures tending to be either big or 
small, smaller predominating, becoming 
confluent on front margin. Pronotum broad, 
moderately punctate, punctures of varying sizes, 
stronger laterally, systematic series distinct, 
comparatively large, many over twice size of 
adjacent punctures, nearly twice size of eye facet. 
Elytra weakly and shallowly punctured on disc, 
becoming much stronger towards sides. Laterally 
in middle serial punctures large, easy to trace, 
about a puncture-width apart; interstrial area 
shiny, punctures of two sizes, the larger sparse, 
most > 2x width apart, somewhat smaller than 
strial, the smaller, more numerous, very small 
(micro), in contrast to other punctures, becoming 
obsolete laterally. 

Aedeagus with basal piece about same length 
as parameres, parameres wide in basal half, 
narrow in apical, tips broadly rounded, central 
lobe narrow, tip bluntly pointed, reaching nearly 
to end of parameres. 

Remarks 

In colour and size resembling A. 
duplopunctatus but differing from it in punctation 
and in the shape of the aedeagus which has the 
central lobe larger than in A. duplopunctatus. The 
absence of the 'small' size of interstrial punctures 
in the species resembles A. australicus and readily 
separates these two species from the other 
Australian Amphiops which have the interstrial 
areas much more punctate. From A. australicus 
(and most other Australian Amphiops) it differs 
by having the first (sutural) elytral stria quite well 
developed as well as a greater development of 
very small (micro) punctures on the elytra, 
although an occasional A. australicus may have 
quite extensive micro punctation. 

This species is only known from a limited area 
of North Queensland. Judging from the localities 
it is possible that it is a closed forest species. The 
specimens from the West Claudie basin and 
Lockhart River were taken in October from still 
pools in closed forest. No other habitat 
information is available. 

Types 

Holotype male: 'Australia, N Qld 15 km WNW 
of South Johnstone "Light Trap' 11 , 'Fay and 
Halfpapp 1986', QDPIM. ** 

Paratypes: 2 same data as holotype, QDPIM; I, 
'Australia N Qld Tolga 3', '1986 J. D. Brown 
light Trap', QDPIM; 1, 'Cow Bay, N of Daintree 



AMPHIOPS, ALLOCOTOCERUS AND REGIMBARTIA 



99 







11 




13 



14 




FIGURES 9-14. Ventral view of aedeagus. 9, Amphiops austrinus; 10, A. duplopunctatus; 11, A. queenslandicus\ 
12, Regimbartia attenuata\ 13, Amphiops micropunctatus; 14, /*. australicus. 



100 



C. H. S. WATTS 



N Qld, 15-22nd March 1984 I. C. Cunningham', 
QDPIM; 2, '12°43S 143°17E, 9 km ENE of Mt 
Tozer 5- 10th July 1986 T Weir and A. Calder\ 
ANIC; 3, '12.44S 143. 14E 3 km ENE of Mt 
Tozer 28th Jun - 4th July 1986 T Weir and A. 
Calder', ANIC; 10, '15°03S 145°09E 3 km NE 
Mt Webb 30th April - 3rd May 1981 A Calder', 8 
ANIC, 2 SAMA. 

Distribution 

Queensland 

Dead Horse Ck, ANIC; East Claudic R, UQIC; 
Gordon Ck nr Claudie R, UQIC; Iron Range, 
UQIC; 9km NNW Lockhart R, ANIC; 3.5km SW 
by S Mt Baird, ANIC; 2km NNE of Mt Tozer, 
ANIC; 6km ENE Mt Tozer, ANIC; 11km ENE 
Mt Tozer, ANIC; Mt Webb Nat. Pk, ANIC; West 
Claudie R, ANIC. 



Amphiops queenslandicus Balfour-Browne, 
1939 

Description (number examined 34 ) Fig. 1 1 

Length 3.5-5.3 mm. Broadly oval, elytra deep, 
almost as high as long. Dark reddish-brown, elytra 
with vague darker/lighter areas and many serial 
punctures black. Head broad, strongly punctate, 
punctures of varying sizes becoming confluent 
along front margin. Pronotum broad, moderately 
punctate on disc becoming stronger toward sides, 
systematic punctures moderate, about 3x size of 
adjacent punctures, a little larger than eye facet. 
Elytra with small but sharp punctures on disc 
becoming much stronger laterally. At sides in 
middle, large serial punctures relatively small, 
most separated by more than their widths, small 
alternating punctures relatively large, some 
approaching 1/2 width of larger ones; interstrial 
punctures of three sizes: large, larger than serial 
punctures, separated by more than their width, 
small much more numerous, relatively large, 1/4- 
1/2 diameter of large ones, micro punctures 
present over most of elytra. 

Aedeagus elongate, basal piece nearly twice 
length of parameres. Central lobe shorter than 
parameres, narrowing to a point, apex not swollen 
or hooked. Parameres broad basally, becoming 
narrower apically, tips rounded, weakly curved 
downwards. 



handwritten locality (which I cannot read), 
BM(NH). Seen. 

Paratypes: 6, same data as Holotype (except 
handwritten label and Type designation); 1, male, 
'Rockingham austral', 'Australia' Amphiops 
queenslandicus M. J. Balfour-Browne det., all in 
BM(NH) with round paratype labels. Seen. 

Distribution 

Northern Territory 

S Alligator R, QM; Black Point Coburg Pen, 
ANIC; 5km NNW Cahills Crossing, ANIC; 7km 
NW by N Cahills Crossing, ANIC; Coastal Plains 
Research Station, ANIC; Daly R Mission, ANIC; 
Darwin, SAMA; Fogg Dam, NTM; Howard 
Springs, SAMA; Humpty Doo, ANIC; Jabiru, 
NTM; Jim Jim, ANIC, NTM; Kakadu NP, NTM; 
Kapalga, QM; Koongarra, ANIC; 12km NNW Mt 
Cahill, ANIC; 19km WSW Mt Cahill, ANIC; 9km 
N by E of Mudginbarry HS, ANIC; Oenpelli, AM; 
6km SW by S Oenpelli, ANIC; 12°40S 132°22E, 
QM. 

Queensland 

Ashgrove, QM; Ayr UQIC; Bowen, SAMA; 
Brisbane, UQIC; Bulburin St Forest via Many 
Peaks, UQIC; Caloundra, SAMA; Cooloola, QM; 
East Claudie R, UQIC; Gatton, UQIC; Homehill, 
SAMA; Ingham, UQIC; Ipswich, AM; Iron 
Range, UQIC; Lockerbie UQIC; Many Peaks, 
UQIC; S Pine R, QM; Ripley, SAMA; 
Rockhampton, ANIC, SAMA; 20 km S 
Townsville, SAMA; 37 km S Townsville, SAMA. 

Remarks 

The distinctive male genitalia readily identify 
this species. Amphiops duplopunctatus is smaller 
with the elytra not quite as deep, elytral punctures 
weaker and usually differently coloured (see under 
A. duplopunctatus). 

Amphiops queenslandicus also closely 
resembles A. austrinus but in this case the weaker, 
smaller punctures on the elytra of A, austrinus 
seem different enough to enable reliable 
separation. However, the male genitalia should be 
used wherever possible. 



Regimbartia Zaitzev, 1908 



Types 

Holotype male: 'Queensland Australia', 
'Amphiops queenslandicus Type J. Balfour- 
Browne det.', with round Type label and a 



Regimbartia attenuates (Fabricius,1801) 

= Volvulus scaphiformis Fairmaire, 1879 
Synonymy after d'Orchymont, 1932. 



AMPH10PS. ALLOCOTOCERUS AND REGIMBARTIA 



101 



Description (number examined 89) Fig. 12 

Length 3.6-5.0 mm. Narrowly boat-shaped, 
high, sides of elytra subparallel, perpendicular, 
black, shiny, appendages testaceous. Head 
deflexed, eyes large, punctures moderate 
scattered, weaker on disc, those forward of eye 
about size of eye facet, systematic punctures 
inward from eye relatively small, about size of 
eye facet. Pronotum broad, weakly and sparsely 
punctured on disc, more strongly towards sides 
where they are about same size as on front of 
head; systematic punctures few and hard to trace. 
Elytra more strongly punctured, somewhat 
stronger at sides than on disc, each elytron with 
10 serial lines, inner two incomplete anteriorly, 
for the most part serial punctures joined forming 
sharp grooves. Mesosternum with strong narrow 
keel, apical sternite with short sharp spine in 
midline at apex. 

Male: Protarsi with two basal segments 
moderately expanded dorso-vcntrally. 

Types 

Hydrophilus attenuate! Fabricius. Ceylon. Type 
not located. 

Volvulus scaphiformis ? Holotype. Rockhampton 
Fairmaire, ?in Museum Godeffroy. Not seen. 

Distribution 



Northern Territory 

Bessie Springs, ANIC; 11 km SW by S of 
Borroloola, ANIC; 30 km NE by E of Borroloola, 
ANIC; 48 km SW by S Borroloola, ANIC; 1 km 
N of Cahills Crossing, ANIC; 7 km NW by N 
Cahills Crossing, ANIC; Daly River, NTM 
Darwin, ANIC, SAMA; Elsey Creek, ANIC 
Fcrgusson R, ANIC; Fogg Dam, ANIC, NTM 
Howard Springs, SAMA; Jabiru, NTM 
Katherine, NTM; Keep River NP, ANIC; Lake 
Bennett, NTM; Magela Ck, ANIC; Manton 
Reservoir, NTM; 2 km N Mudginberri HS, ANIC; 
6 km N by E Mudginberri, ANIC; Nourlangie Ck, 
ANIC; Roper R, ANIC; South Alligator R, QM; 
U.D.P. Falls, NTM; 

Queensland 

Archer Bend, SAMA; Ayr, UQIC; Brisbane. 
MV, QM, UQIC; Cairns, ANIC, QM; Calliope R, 
ANIC; Caloundra, SAMA; Cape Flattery, DPIM; 
Chillagoe, DPIM; Claudie R, UQIC; East Claudie 
R, QIC; Clermont, AM; Cooktown, MV; 40M N 
Cooktown, UQIC; Duaringa, AM; Edungalba, 
ANIC; Einasleigh, DPIM; Frenchman's Creek via 
Rockhampton, UQIC; Gin Gin, UQIC; Gregory 
River Hotel, DPIM; Homehill, SAMA; Kirrama 



Rng, QM; Karumba, UQIC; Lakefield NP, ANIC; 
Mackay, SAMA; Mareeba, ANIC, DPIM; 18km 
N Mareeba, DPIM; Mary Ck, ANIC; Mclvor R, 
UQIC; Mt Garnet, SAMA; 3.2 km SW of Mt 
Inkerman, ANIC; Mt Molloy, ANIC, QM; 3 km 
ENE Mt Tozer, ANIC; 6 km ENE Mt Tozer, 
ANIC; Nordcllo Lagoon, DPIM; 11km WSW 
Petford, DPIM; N Pine R, QM, UQIC; 
Rockhampton, SAMA; 67 km E Roma, QM; 
Samford, UQIC; Silver Plains CP, DPIM; 15km 
WNW South Johnstone, DPIM; Starbright HS, 
DPIM; Strathmore Stn, DPIM; Tolga, DPIM; 
Townsville, QM; Walkamin, DPIM; 40km S 
Weipa, DPIM; Yaamba, UQIC; Yeppoon, UQIC; 
18°38 S 138°11 E, ANIC; 18°34 S 138°08 E, 
ANIC. 

Western Australia 

Channley R, ANIC; Derby, SAMA; Fitzroy R, 
ANIC; 12 km S Kalumburu Mission, ANIC; 
Kunanurra, DPIM; 1 km NNE Millstream, ANIC; 
Synnot Ck, ANIC; 14°53 S 125°45 E, SAMA. 

New South Wales 

Eccleston, UQIC. 

Remarks 

Once known, this distinctive water beetle is 
unlikely to be confused with any other Australian 
species. It is relatively common in shallow 
swamps and dams along the coast from northern 
New South Wales to the Kimberlcy. Beyond 
Australia the species has a wide distribution in 
South-east Asia as far west as Sri Lanka. 

I have followed d'Orchymont (1932 p. 709) for 
the name of this widespread species. 



Allocotocerus Kraatz, 1883 

The three Australian species of Allocotocerus 
(- Globaria Latreille) are all moderately sized, 
highly spherical insects with the ventral surface 
shiny black. Within Australia they can only be 
confused with species of Amphiops, particularly 
A. queens landicas which is of a similar size and 
shape. The even, regular punctation, uniformly 
black ventral surface, and swimming hairs on the 
legs in Allocotocerus readily separate them from 
Amphiops. 

There is little to separate the species other than 
the sexual characters of the aedeagus, trochanter 
setae and the labrum. 

The first described and best known species, A, 
punctatus, is common and widespread in slowly 



102 



C. H. S. WATTS 



moving water and in swamps in eastern Australia bit larger than size of eye facet, systematic 

from northern New South Wales northwards. It punctures virtually absent. Pronotum narrower 

appears to be absent from the Northern Territory than elytra, punctures on disc much weaker than 

and northern Western Australia where its place is on head, becoming considerably stronger towards 

taken by A. tibialis and A. yalumbaboothbyi. front comers, systematic punctures few, sparse 

Conversely these species likewise have not been and hard to find. Elytra covered with very even 

recorded from the east coast. punctures in same area but much stronger laterally 

An additional species (the type species, A. than on disc, serial punctures 1.5-2x diameter of 

bedeli Kraatz 1883) occurs in New Guinea, adjacent punctures, reduced to 2-3 short lines 

Unfortunately the holotype does not appear to be midway along side of elytron. Midline of 

in the Deutsches Entomologisches Institut in mesosternum with strong, tall spike between 

Eberswalde. In its place is a label written by mesocoxae. First ventrite constricted in middle 

Korschefsky in 1937 indicating it was lost (Lothar with rather wide strong midline carina. 

Zerche pers. com.). The recognition of this species Metasternum with two strong carinae in midline 

and any possible influence on the nomenclature with deep gap between them, the anterior one 

of Australian species must await the collection of cylindrical and angled backwards, the posterior 

further specimens from New Guinea. one anvil shaped in lateral view. 

Male: Labrum prominent, front edge deeply 

bifid. Protibia triangular in cross-section. 

Key to Australian Allocotocerus Aedeagus with basal portion strongly bent, 2.5x 

length of parameres which are broad for whole 
Labrum strongly extended forward, strongly | engthj central lobe broad e t for short 

blfld male ^ P mctatUS (B^kburn) narrow port]0n at apcx MeSQ _ and ^ 

Labrum normal, often hidden beneath clypeus, trochanters with widely scattered short, stout setae 

not blfid - 2 on ventral face. 

Protibia light yellow with darker apical portion Female: Labrum little exposed, front edge not 

A.punctatus (Blackburn) bifid. Protibia of normal shape, contrast between 

Protibia lighter than other legs but without dark a P ical P ortion and yellow on rest of proleg 

darker apical portion 3 often less pronounced than in male. Meso- and 

meta-trochanters with scattered, sparse, short, 

Setae on outer posterior angle of ventral stout setae on ventral face. 
surface ot mesofemur more developed than 

those on metafemur (Figs 7 & 8). Aedeagus Type 

with parameres broad with rounded tips, \j , . n^n«oi *™ », ™ *^*^ .***,>, 

central [lobe sharply pointed, much shorter than Holotype: T2328' 'Blackburn coll 1910-236', 

parameres (Fig. 16) Volutus punctatus, Blackburn', BM(NH). Seen. 

A. tibialis (Balfour-Browne) _ . 

„ c ., . Distribution 

Setae on metafemur equally poorly or slightly 

more developed than on mesofemur (Figs 5 & Queensland 

6). Aedeagus with parameres narrowing to 8 km N Bluewater, SAMA; Cardstone, ANIC 

point, central lobe broad with narrow spine at 40 km N Coen, SAMA; 70 km N Coen SAMA" 

tip, as long as parameres (Fig. 17) Caloundra, SAMA; 29 km NW by W Cooktowni 

A -y^rnbaboothbyi, V .no,. ANJC; 4Q km N Cooktown? SAMA; , ngham 

ANIC; Lakefield NP, QDPIM; 18 km N Mareeba, 
QDPIM, ANIC; Mary Ck, ANIC; Mc Ivor R, 
ANIC; Townsville, MV; Moorehead R, ANIC; 
Moreton, ANIC; Mt Coolum, ANIC; 20 km S 
Townsville, SAMA; 37 km S Townsville, SAMA; 
Weniock R Crossing, ANIC; 15°17S 145°10E, 
ANIC. 



1 — 



2 — 



Allocotocerus punctatus (Blackburn, 1888) 



Description (number examined 112) Fig. 15 

Length 3.5-4.5 mm. Oval, elytra high, height 
only a little less than length. Black, shiny, 
appendages lighter, yellowish with darker terminal 
portion to tibia. Head narrow, front margin 
broadly and quite deeply concave, sides of 
clypeus narrowly margined, rather evenly covered 
with moderate punctures which are weaker in 
middle than at sides, those forward from eyes a 



Remarks 

In overall shape, punctation and colour closely 
similar to A. tibialis and A. yalumbaboothbyi but 
the male characters readily separate it from these 
species. Male A. yalumbaboothbyi and A. tibialis 



AMPHIOPS, ALLOCOTOCERUS AND REG1MBARTIA 



103 






15 



16 



17 



FIGURES 15-17. Ventral view of aedeagus. 
Allocotocerus valumbaboothbvi. 



15, Allocotocerus punctatus; 16, Allocotocerus tibialis; 17. 



lack the very distinctive labrum and protibia of 
male A. punctatus. In A. punctatus the dark apical 
portion of the protibia separates both male and 
female from the other species which have more 
uniformly coloured protibiae. In both male and 
female A. tibialis, the number and density of setae 
on the trochanters are much larger than in A. 
punctatus. 

The species is relatively common in coastal 



dams and swamps from northern Southern 
Queensland to Cape York, often found together 
with the similarly shaped Amphiops. 



Allocotocerus tibialis (Balfour-Browne, 1939) 

Description (number examined 61) Figs 7, 8, 16 
Length 4.5-5.0 mm. Oval, elytra high, height 



104 



C. H. S. WATTS 



only a little less than length. Black, shiny, 
appendages dark-testaceous. Head narrow, front 
edge widely and moderately concave, sides of 
clypeus margined, strongly punctured, 
punctures in front of eyes larger than eye facet, 
systematic punctures inwards from eye few and 
hard to trace, punctures on disc somewhat 
weaker than elsewhere, about size of eye facet. 
Pronotum narrow, somewhat more weakly 
punctured than head particularly on disc, 
systematic punctures few and hard to find. 
Elytron punctured rather more strongly than on 
pronotum and head, punctures much weaker on 
disc than on sides where they are strong and 
less than a puncture-width apart. Serial 
punctures few or absent, if present little larger 
than adjacent punctures. Mesosternum with 
moderately tall, sharp spine in midline. Midline 
of metasternum with two distinct carinae, 
separated by deep gap, anterior carina 
cylindrical and angled strongly backwards, 
posterior one broader and curving backwards 
and upwards when viewed from side. First 
abdominal ventrite narrowed in middle half, 
midline with rather narrow and strong carina, 
ventrites two and three narrowed in central half, 
weakly bulbous/carinate in midline. Area 
between ventrites deeply grooved. Fourth 
ventrite weakly narrowed anteriorly, smooth, 

Male: Labrum simple. Protibia a little flattened 
and widened, tarsi unmodified. Mesotrochanters 
stout with a well-marked group of long golden 
setae on anterior apical ventral angle, inner half 
of ventral face lacking punctures/setae. 
Metatrochanters stout with a less well-developed 
group of setae in same place, metatibia stout. 
Aedeagus long, sinuate, relatively broad, basal 
piece about 1.5x length of parameres, parameres 
broad, subparallel, rounded at tips, central lobe 
narrowing progressively to tip, shorter than 
parameres. 

Types 

Holotype male; 'Adelaide River 92-2\ '4969', 
'Globaria tibiale mihi J. Balfour-Browne det.' 
with red type label, BM(NH). Seen. 

Lectotypes: 1, 'Adelaide River, NW Australia 
J. J. Walker', L G. C. Champion Coll. B,M. 1927- 
409' with red (allotype) type label, BM(NH), 10 
same data, in BM(NH); 3, same data as holotype, 
BM(NH). Seen. 

Distribution 

Northern Territory 

Gimbat Sin, NTM; 6 km E Humpty Doo, 



QDPIM; Jabiru, NTM; 10 km N Jabiru, QDPIM; 
Junction of Arnhem Hwy and Oenpelli Rd, NTM; 
Magela Ck, ANIC; 19 km E by S Mt Borradaile, 
ANIC; 8 km E Mt Cahill, ANIC; 46 km WSW Mt 
Cahill, SAMA; Nabarlek Dam, ANIC; 
Nourlangie, ANIC; UDP Falls, NTM; Wildman 
R,NTM. 

Remarks 

Both male and female A. tibialis can be 
separated from A. punctatus and A 
yalumbaboothbyi by the more extensive 
development of setae on the mesotrochanters. The 
elytral striae are also usually much weaker or 
absent in this species but at least traceable in the 
others. The species has not been recorded from 
the east coast and appears to have a rather 
restricted distribution in coastal Northern 
Territory. Here it occurs commonly, often with A. 
yalumbaboothbyi. 

Amphiops tibialis can also be separated from 
the very similar A. yalumbaboothbyi by the 
differently shaped posterior mesosternal 
protuberance: in A. tibialis this is thicker and 
curved upwards behind in lateral view whereas it 
is straight in A. yalumbaboothbyi. 



Allocotocerus yalumbaboothbyi sp. nov. 

Description (number examined 51) Figs 5, 6, 17 

Length 3.5^.5 mm. Oval, elytra high, only a 
little longer than high. Black, shiny, ventral 
surface and appendages dark-testaceous, proleg 
yellowish. Head narrow, front margin broadly and 
quite deeply concave, rather evenly covered with 
moderate punctures which are a little weaker on 
disc than at sides, those forward from eyes a bit 
larger than size of eye facet, systematic punctures 
virtually absent. Pronotum narrower than elytra, 
punctures on disc much weaker than on head, 
becoming considerably stronger towards front 
corners, systematic punctures few and hard to 
find. Elytra covered with very even punctures 
which become much stronger laterally, serial 
punctures reduced to 2-3 short lines on each 
elytron towards sides in middle; midline of 
mesosternum with tall sharp spike forward of 
mesotrochanters, midline of metasternum with 
two strongly raised carinae separated by short 
deep gap, front carina in shape of backwardly 
inclined broad spine, rear carina oval shaped on a 
broad pedestal when viewed laterally. First 
ventrite moderately constricted in middle with a 
narrow but well marked central carina extending 



AMPHIOPS, ALLOCOTOCERUS AND REGIMBARTIA 



105 



forward between metatrochanters. Second sternite 
also constricted but without carina, fourth not 
restricted. Sutures between ventrites wide, deep, 
well-marked. 

Male: Labrum small, usually contracted, not 
bifid, protibia not expanded, basal two segments 
of protarsi a little expanded with ventral hairs. 
Mesotrochanters with a few scattered, short spines 
on apical ventral surface. Mesotrochanters with 
longer more numerous setae forming a sparse 
brush along posterior ventral portion of 
metatrochanter. Aedeagus long, sinuate with 
relatively broad basal portion which is about 2.5x 
length of parameres. Parameres narrow, evenly 
narrowing to quite sharp tip. Central lobe as long 
as parameres. In a number of specimens the 
parameres are twisted and splayed out, 
presumably an artefact of preservation, but one 
that I have not seen in other species. 

Female: Basal segment of protarsi not weakly 
expanded, with ventral hairs. Mesotrochanters 
with a few sparse, stout setae on ventral face at 
apex, metatrochanter with similar setae restricted 
to apical half. 

Types 
Holotype male: '12°22S 133°01E 6 km SW by 

5 of Oenpelli NT, 30. v. 73, at light E. G. 
Matthews', SAM A. 

Paratypes: 4, 'W Australia Mitchell Plateau 
14°40S 125°44E 23 Sept 1982 B. V. Timms\ 
SAMA; 4, '13°34S 132°15E\ 'Moline Rockhole' 

6 km E by E of Mt Daniela 23. v. 1974, NT T. 
Weir and T. Angeles', NTM; 6, '12°32S 132°50E 
Koorgarra 15 km E of Mt Cahill NT, 15.xi.1972, 
T. Weir and A. Allwood', NTM; 11, 'NT UDP 
Falls, 18-19th July 1980, M. B. Malipatil 
Freshwater Pool', NTM; 20, '12°49S 132°51E, 
15 km E by N of Mt Cahill NT, 29.X.72, light 
trap, E. Britton 1 , ANIC. 



Distribution 

Northern Territory 

8 km E by N of Mt Cahill, NTM; 19 km E by N 
Mt Cahill, NTM; Junction of Amhem Hwy and 
Oenpelli Rd, NTM; Kambolgie Ck, SAMA; 
Koongarra, NTM; Wildman R, NTM. 

Remarks 

Virtually indistinguishable from A. tibialis and 
A. punctatus other than by sexual characters. 
Males can be easily separated from A. punctatus 
by the lack of a large bifid labrum, from A. tibialis 
by the weaker development of setae on the 
mesotrochanters. In A. tibialis the mesotrochanter 
setae are longer and denser often to the extent of 
matting together. They are also more restricted to 
the apical portion of both meso- and meta- 
trochanters than in A. yalumbaboothbyi. 

Separation of female specimens is more 
difficult. Female A, punctatus have the prolegs 
pale yellow with a more or less obviously darker 
terminal portion to the tibia. In both A. 
yalumbaboothbyi and A. tibialis the tibiae lack 
the darker apical portion. The setae on both meso- 
and meta-trochanters of female A. 

yalumbaboothbyi and A. punctatus are small and 
sparse. In A. tibialis they are more developed 
particularly on the mesotrochanter. 



Acknowledgments 

The curators of the collections listed earlier provided 
ready access to specimens in their care. Ms D. Churches 
and Ms C. Home typed the manuscript and Mr R. 
Gutteridge prepared the drawings. Mrs M. Anthony and 
Mrs J. Evans helped with library aspects. Dr E. 
Matthews greatly improved the manuscript. I thank all 
these people without whom my task would have been 
much greater. 



References 



BALFOUR-BROWNE, J. 1939. Contribution to the 
study of the Palpicornia Part III. Annals and 
Magazine of Natural History 11(4): 289-310. 

BLACKBURN, T. 1888. Notes on Australian 
Coleoptera with descriptions of new species. 
Proceedings of the Linnean Society of New South 
Wales 111(2): 805-875. 

BLACKBURN, T. 1898. Further notes on Australian 
Coleoptera, with descriptions of new genera and 
species. Transactions of the Roval Society of South 
Australia 22: 221-233. 



ERICHSON, W. F. 1843. Beitrag zur Insecten-Fauna 
von Angola, in: besondere Beziehung zur 
geographischen Verbreitung der Insecten in Afrika. 
Archiv fur Naturgeschichte 9: 199-267. 

FABRICIUS, J. C. 1801. Systema Eleutheratorum...I, 
24+506pp. Kiliae. 

FAIRMAIRE, L. 1879. Descriptions dc Coleopteres 
nouveaux ou peu connus du Musee Godeffroy 
(Hydrophilidae). Journal Museum Godeffroy 24: 
80-83. 



06 



C. H. S. WATTS 



HANSEN, M. 1991. The Hydrophiloid Beetles. 
Phylogeny, Classification and a Revision of the 
Genera (Coleoptera: Hydrophiloidea). Biologiske 
Shifter 40: 367pp. 

KRAATZ, G. 1883. Allocotocerus nov. gen. 
Hydrophilidarum. Deutsche Entomologische 
Zeitschnft 27: 14-15. 

ORCHYMONT, A. 1932. Zur Kenntnis der 



kolbenwasser Kafer (Palpicomia) von Sumatra, Java 
und Bali. Archives Hydrobiologica. Supplement Band 
IX (Tropische Binnengewassen 1 1): 623-714. 

ZAITZEV, F. A. 1908. Catalogue des Coleopteres 
aquatiques des families Dryopidae, Georyssidae, 
Cyathoceridae, Heteroceridae et Hydrophilidae. 
Trudy russkogo Entomologicheskogo Obshchestva 
38: 283-420. 



DOUGLAS MAWSON: THE GEOLOGIST AS EXPLORER 



D. W. CORBETT 



Summary 



Douglas Mawson was a born explorer. His professional career as a geologist and academic in 
Australia demonstrates this aspect of his character as clearly as his exploits in the Antarctic. Science 
and exploration dominated his life and motivated his endeavours, and the inseparable link between 
them was his pursuit of knowledge of glaciation-both ancient and modem. This paper reviews the 
diversity and wide geographical extent of his geological investigations, principally in South 
Australia, during the first half of the twentieth century at a time when the geology of large areas of 
the State was still largely unknown. The manner of his achievement and his distinguished 
contribution to the advance of geological knowledge in South Australia exemplify Mawson as the 
explorer-geologist. 



DOUGLAS MAWSON: THE GEOLOGIST AS EXPLORER 



D. W. CORBETT 



CORBETT, D. W. 1998. Douglas Mawson: the geologist as explorer. Records of the South 
Australian Museum 30(2): 107-136. 

Douglas Mawson was a born explorer. His professional career as a geologist and academic 
in Australia demonstrates this aspect of his character as clearly as his exploits in the Antarctic. 
Science and exploration dominated his life and motivated his endeavours, and the inseparable 
link between them was his pursuit of knowledge of glaciation — both ancient and modern. This 
paper reviews the diversity and wide geographical extent of his geological investigations, 
principally in South Australia, during the first half of the twentieth century at a time when the 
geology of large areas of the State was still largely unknown. The manner of his achievement 
and his distinguished contribution to the advance of geological knowledge in South Australia 
exemplify Mawson as the explorer-geologist. 

D. W. Corbett, Honorary Research Associate, South Australian Museum. North Terrace, 
Adelaide, South Australia 5000. 



Douglas Mawson was a geologist with a broad 
scientific background and diverse interests within 
his discipline, as a review of his publications will 
verify (see Innes and Duff 1990). Known and 
honoured as one of the great Antarctic explorers, 
the prime motivation behind his achievement was 
the pursuit of scientific knowledge, which he 
coupled with the innovative use of the latest 
available technology. With the exception of Otto 
Nordenskjold, geologist and leader of the Swedish 
Antarctic Expedition (1901-03), Mawson was the 
only science-trained expedition leader in the heroic 
age of South Polar exploration and his approach 
marked the beginning of the modern age of 
Antarctic exploration. 

Mawson's career as a geologist and his 
scientific reputation were built in South Australia 
during his many years in the geology department 
at the University of Adelaide. While this paper 
focusses on the academic aspects of Mawson's 
life more than his Antarctic exploits, it is 
impossible to disentangle the two strands of 
endeavour. Down south he was the scientific- 
explorer; in the arid outback of South Australia he 
was the explorer-scientist. His major researches 
inextricably linked the two vastly different 
environments, for it was the opportunity to study 
an ice-age at first-hand and to equip himself better 
as an interpreter of past glaciations that inspired 
Mawson to venture south with Shackleton in 
1907, 

The circumstances of time and place (early 
twentieth century South Australia, much of it little 



known geologically) and his life-long interests in 
glaciation, ancient and modern, determined that 
Mawson the geologist and Mawson the explorer 
were one and the same and through his extensive 
investigations in South Australia he personifies 
both the adventurous and the enquiring spirit. 

Mawson's Antarctic exploits have been 
chronicled by historians, fellow-expedition 
members and in his own classic account 'The 
Home of the Blizzard'. His career as a 
scientist, and notably an assessment of his 
geological work, have been less well treated, 
although aspects of them are covered in the 
biography by his wife (Mawson 1962) and by 
Alderman (1967); by Parer and Parer-Cook 
(1983); in the biographical summary by Jacka 
(1986) and by Sprigg (1986). This paper presents 
a review, with emphasis on Mawson's career as a 
geologist in South Australia and his contribution 
to geological knowledge of the State. 



Early Years 

As one of the first generation of geologists 
trained in Australia, Mawson brought an 
Australian rather than European perspective to his 
work. Although born in Yorkshire, England on 
the 5th May, 1882, he was only two years old 
when his family migrated to Sydney and he grew 
up staunchly independent and thoroughly 
Australian in outlook— as the promotion of his 
Antarctic expeditions was to demonstrate. He 



108 



D. W. CORBETT 



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DOUGLAS MAWSON GEOLOGIST 



109 




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entered the University of Sydney in 1 899 at the 
age of 16, doing well in Physics, Chemistry and 
Mining on the way to his Bachelor of Engineering 
degree in 1901. But it was in geology that he 
excelled, gaining first class honours in 1900 and 
being awarded the petrology prize, and 
subsequently, in 1905, completing a B.Sc in 
geology. His inspiration came from the 
charismatic personality and the dynamic teaching 
of the Professor of Geology, T. W. Edgeworth 
David, who in turn was quick to recognise the 
abilities of the young science student. David was 
to become Mawson's mentor, fellow expeditioner 
and lifelong friend and confidant. 

One of David's many preoccupations was 
ancient glaciation. As a young geologist in Britain 
he had followed with interest the debate on the 
nature of the latest (Pleistocene) Ice Age and the 
evidence of a much older glaciation (Permo- 
Carboniferous) discovered in India. Working for 
the New South Wales Geological Survey in the 
late 1880s he confidently identified glacial 
deposits in the Permo-Carboniferous rocks of the 
Hunter Valley. In 1901 he visited Mount 
Kosciusko where he immediately recognised the 
work of glaciers in the tarns, moraines and ice- 
sculpted valleys in the high country (David et al. 
1901) — his views effectively settling a dispute 
that had continued ever since W. B. Clarke had 
reported evidence of glaciation there half a century 
earlier. Meanwhile in South Australia Walter 
Howchin had discovered glacial sediments, older 
than any known to that time, in the Sturt Gorge 
near Adelaide (Howchin 1901). These deposits 
(the Sturt Tillite) were assigned to the Cambrian 
but were later shown to be even older (late 
Precambrian), extending the evidence of past 
glaciation in both time and space and acting as a 
spur to the search for further clues to a former 
frigid earth. 

David was Australia's first 'national' 
geologist, with interests spread well beyond his 
base in New South Wales. He had particularly 
strong links with South Australia through Walter 
Howchin, with whom he had collaborated in the 
field on such diverse matters as Cambrian fossils 
and glacial geology. It was perhaps inevitable 
that Mawson should become interested in these 
new developments which were extending the 
frontiers of Australian geology but his studies 
initially led him in other directions. In 1902 he 
was appointed Junior Demonstrator in chemistry 
and the following year he took six months leave 
of absence to make a trip to the South West 
Pacific. 



The New Hebrides 1903 

Mawson's first opportunity to explore and 
engage in adventurous fieldwork was due to the 
initiative and recommendation of David, who had 
a long-sustained interest in the geology of the 
Pacific basin. It was to prove a testing assignment 
for Mawson, requiring him to work under arduous 
and at times dangerous conditions, making the 
most of general short excursions from the ship as 
it sailed through the island archepelago, strung 
out over a vast area of ocean. Little known 
geographically away from the coastal fringe, the 
interiors were rugged and thickly covered with 
dense rainforest making access difficult while the 
native inhabitants had a reputation for being 
unpredictable and at times hostile. 

Apart from a scanty record of previous 
investigations, the New Hebrides (Fig. 1) were a 
geological 'terra incognita' and for Mawson a 
challenge he was eager to meet: 'A great field 
was now open before us ... nothing has yet been 
gleaned as to the true nature of the rocks forming 
this extensive chain of islands'. 

Mawson (and W. F. Quaifc, a biologist) arrived 
at Vila, on the island of Elate and the chief town 
in the group on 13 April 1903. His first 
observations were made in the low hills around 
the town where a raised coral reef overlay volcanic 
sediments. This general geological situation was 
confirmed at locations further north along the 
coast where much thicker reef deposits overlay the 
'foundation rocks' — a variable series of tuffaceous 
volcanics including agglomerates and pumice-rich 
beds (Fig. 2). 

From Efate the ship steamed north to Malckula 
where Mawson wrote: 'The natives of Malekula 
are the most uncertain of any of the inhabitants of 
the group, having not yet abated from cannibal 
habits; indeed war was raging between the 
Natives ... at the time of our visit. For this and 
other reasons wc were unable to examine this 
region very thoroughly'. Nevertheless he was able 
to make some investigations and excursions into 
the interior. Reaching Espiritu Santo, the largest 
island, a base was established at the mission 
settlement of Tangoa on the south coast and an 
assault made on Losumbuna (5 520 feet), the 
highest mountain in the New Hebrides, The 
interior mountains had never been explored by 
Europeans and the challenge was irresistible. 
Accompanied by three native guides, Mawson and 
Quaife negotiated two subsidiary peaks before bad 
weather, difficult terrain and, crucially, their 
guides' refusal to continue, forced a retreat. 



DOUGLAS MAWSON GEOLOGIST 



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D. W. CORBETT 



Although disappointed at not reaching their 
objective, Mawson collected specimens and made 
sketch sections of the rugged hinterland (Fig. 3). 
Fieldwork proved more productive along the coast 
where three separate pyroclastic units intruded by 
a variety of igneous rocks were found. An earlier 
report of older basement rocks (gneiss) in this part 
of the island could not be confirmed despite 
diligent searching. 

The northern-most islands in the chain were 
covered in a cursory reconnaissance, but enough 
to confirm the volcanic nature and essentially 
basic composition of the Banks Group. Arriving 
back in Vila in mid-August after four months 
away, the expedition was greeted by a minor 
earthquake with another tremor following a few 
days later — enough to indicate the seismic 
instabilty of the region. Finally, investigations in 
the Havannah Harbour area provided key sections 
in the local sequence of volcanic sediments and 
overlying reef deposits. 

The New Hebrides expedition was inevitably 
very much a reconnaisance and Mawson was 
keenly aware of the limitations of his survey. One 
of the strengths of his published report (Mawson 
1905) was his inclusion of all previous references, 
both published and unpublished, to the geology 
and physical features of the islands. The general 
seismicity of the region, already well documented, 
and which Mawson himself experienced, he 
attributed to local volcanic sources, recognising 
also the importance of regional tectonic 
movements along major faultlines. He wrote: 
'before long numerous seismological stations will 
be distributed through the South Pacific Islands, 
as only by analysing such data as would result, 
can definite decisions regarding the present earth- 
movements in this much-troubled area be arrived 
at*. It was to be fifty years before that hope began 
to be realised. 

An anticipation that because the old rocks of 
nearby New Caledonia were mineral-rich, the New 
Hebrides might be similarly endowed was quickly 
dispelled because of the geological youthfulness of 
the islands. Sulphur deposits and iron-bearing 
sands were the only resources considered to be of 
possible future commercial value. Within the 
regional context of the Pacific basin, Mawson 
viewed the New Hebrides island arc as of late 
Tertiary age, one of a series of parallel arcs which 
were remnants of a much fragmented continental 
mass. Folding and over-thrusting, associated with 
volcanicity, against a rigid foreland lying to the 
west (New Caledonia), had been followed by major 
faulting and sea- floor subsidence. 



The evidence for elevation which most 
impressed Mawson were the raised coral reefs. 
These capped the Tertiary deposits and ranged in 
terraces rising to over 2 000 feet (609 metres). 
They were estimated to be post-Pliocene in age, 
and gave a clear indication of continued tectonic 
activity since the middle Tertiary. 

His published account of the New Hebrides 
expedition put the islands on the map geologically 
and established Mawson as a resourceful and 
perceptive field worker, competent in many areas 
of geology and with a flair for synthesis. He 
foreshadowed many of the more recent 
interpretations of south-west Pacific region 
geology made in the light of Plate Tectonic theory, 
with the New Hebrides viewed as an island arc of 
volcanic lavas and pyroclastic rocks and intrusions 
adjacent to a deep ocean trench and above a 
steeply dipping seismic zone. 



Early Researches 

On returning to the University, Mawson was 
soon involved in research (with fellow student 
and later Antarctic explorer Griffith Taylor) on 
the igneous rocks in the Bowral-Mittagong area, 
south-west of Sydney. The Mittagong study 
(Taylor and Mawson 1903) was the first of many 
on the petrography and petrology of igneous 
rocks in their regional setting which was to 
remain a prime interest in the years ahead. About 
this time Mawson also began investigations into 
the radioactive properties of minerals. This was a 
pioneer study in Australia, closely following the 
discovery of radioactivity by Becquerel in 1896 
and the follow-up work by the Curies which led 
to the isolation of radium in 1898 and the 
recognition that uranium and thorium-bearing 
minerals were radioactive. Mawson reviewed 
these recent researches and carried out tests on 
natural waters, mud, soil and air. He was 
required to construct his own analytical 
equipment, notably a gold-leaf electroscope, and 
a large number of Australian minerals was tested 
including the only two known occurrences of 
uranium-bearing minerals in Australia and which 
gave the predicted high readings. The other 
minerals found to test positive were mainly 
monazites from various tin- fields around 
Australia. His short paper (Mawson & Laby 
1904) marked the beginning of a life-long 
interest in the geological occurrence of 
radioactive minerals and their economic 
potential. 



DOUGLAS MAWSON GEOLOGIST 



113 



South Australia 1905 

Late in 1904, Mawson, with the support and 
encouragement of David, was appointed to the 
position of Lecturer in Mineralogy and Petrology at 
the University of Adelaide. He arrived to take up 
his academic duties full of enthusiasm and with 
high expectations but was immediately confronted 
with a lack of suitable accommodation and facilities 
for geology due to the University's chronic shortage 
of funds. Frustrations developed which were to dog 
him for many years, including the necessity to forge 
a working relationship with the only other member 
of the Geology Department, Walter Howchin. 
Already with an established international reputation 
and with a great deal of experience of South 
Australian geology, Howchin was 60 years of age 
when Mawson, 23, arrived on the scene. It seems 
there were tensions from the start. The question of 
'spheres of activity' (Mawson's phrase) provided 
an immediate and ongoing irritant, to be 
temporarily removed when Mawson went south in 
1907. 

The geology of South Australia was known in 
broad outline at the beginning of the century 
(Corbett et al 1986) This was due predominantly 
to the work of three men: Ralph Tate, the first 
geologist appointed to the University (1875- 
1901); Walter Howchin, Methodist Minister and 
enthusiastic amateur until his appointment to the 
University after Tate's death in 1901; and H. Y. 
L. Brown, the first Government Geologist who 
was to act as a one-man Geological Survey from 
1882 until 1912. While Tate and Howchin worked 
mainly, though not exclusively, close to home in 
the Mount Lofty Ranges, Brown had been 
carrying out some epic geological explorations in 
the northern regions of the State which at that 
time included the Northern Territory. He 
published the first geological map of South 
Australia in 1883, revising it periodically. His 
1 899 map was a remarkable achievement and in 
its essentials remains little changed today. 

Tate had discovered glacial features at Hallett 
Cove in 1877; Howchin subsequently 
demonstrating the widespread evidence for this 
glaciation outside the Adelaide region and 
establishing a Permo-Carboniferous age for the 
event by about 1900. In 1901 Howchin, as 
mentioned previously, had discovered the much 
older glacials in the Sturt Gorge, a few miles 
south of Adelaide. But perhaps the most 
significant of all the early breakthroughs was the 
finding of Cambrian fossils in the old rocks on the 
western flank of the Mount Lofty Ranges 



(Howchin 1897). Howchin thereafter concentrated 
much of his effort on determining the stratigraphy 
of the western ranges. 

It was Howchin' s clearly expressed 
'prerogative' to work in most areas of the State 
that prompted Mawson to choose the remote 
Olary-Broken Hill area for his first extensive field 
investigations. It was a decision both judicious 
and timely. Not only did this work extend 
Howchin' s researches on the supposed Cambrian 
rocks of the Mount Lofty Ranges into the Olary 
Spur and over the border to Broken Hill and the 
Barrier Ranges, but the problems presented by the 
region also satisfied his interests in mineralogy, 
petrology, and stratigraphy and his discoveries 
were to influence his future involvement with 
glacial deposits both ancient and modem. 

The explorer-geologist was severely tested in 
the harsh environment near the north-east state 
border. It was (and is) an arid, inhospitable and 
sparsely inhabited country. Previous investigations 
had centred on and around the Broken Hill ore- 
body itself — the largest silver-lead ore body in the 
world. While little was known of the origin of the 
ore-body and its stratigraphic controls, Mawson 
set himself the task of ascertaining the broader 
regional context of the deposit. His methods 
involved covering the ground in a series of 
traverses on foot, horseback, bicycle and on 
occasions, by motor vehicle. He was to determine 
and define two major rock divisions in the Olary- 
Broken Hill region: 

1. An older basement complex of metamorphic 
rocks including gneiss, schist, amphibolite and 
granite of Precambrian age which he named 
the Willy ama Complex, and 

2. A younger series of sedimentary rocks, in part 
metamorphosed, of assumed Cambrian age 
including a wide variety of rock types, the most 
notable and persistent being boulder-beds and 
related sediments of glacial origin. This he 
named the Torrowangee Series. 

In January 1907, the Australasian Association 
for the Advancement of Science (AAAS), held its 
meeting in Adelaide and Mawson gave two 
(unpublished) papers based on his recent field 
work and particularly concerned with the glacial 
beds. His interest in these beds and a desire to 
reach a full understanding of their nature and 
origin was developing rapidly. Many years later 
he wrote to Edgeworth David that his commitment 
to glacial geology dated from December 1906 
when his Olary field investigations were well 
underway. Matters moved very rapidly at the end 
of 1907. Mawson heard, through David (who was 



114 



D. W. CORBETT 



to join the British Antarctic Expedition), that the 
leader, Ernest Shackleton, was to visit Adelaide 
briefly on his way to New Zealand to join the 
'Nimrod'. Mawson successfully requested a 
meeting and volunteered his services for the 
summer season. Within three days Shackleton had 
offered Mawson the position as physicist for the 
duration of the expedition. The opportunity to 
realise his ambition to experience 'an ice-age in 
being' was too good to miss. He accepted, quickly 
arranging for a ' locum' to cover his absence from 
the University, and left Adelaide before the end of 
December bound for the Antarctic. 



South With Shackleton - the British Antarctic 
Expedition 

David was senior geologist on the expedition 
with Raymond Priestley, a young man with no 
formal qualifications in science, as his deputy. 
Mawson as physicist had no official role in this 
area. Yet from the start David involved his old 
student in the geological program and in two of 
the three main journeys undertaken by the 
expedition — the ascent of Mount Erebus and the 
trek to the South Magnetic Pole. Mawson played 
a crucial role, both as a young and vigorous team 
member and a valuable contributor to the 
geological work, which David was quick to 
acknowledge in his final report (David & Priestley 
1914). Here Mawson is referred to as 
Mineralogist, Chemist and Physicist to the 
expedition (the study of Antarctic ice — its 
crystallisation, granulation and other properties- — 
was considered by David as much a matter of 
mineralogy as of physics). The report incorporates 
much of Mawson's thinking and his contribution 
to it was wide-ranging, covering mineralogy and 
petrology and stratigraphy, as well as economic 
geology implications and broad- scale 
considerations of Antarctic geology within a 
global context. 

Mawson and David were both in the small party 
which reached the summit of Mount Erebus 
(3 794 m) on 8 March. Mawson made a traverse 
map of the eight day journey which provided its 
share of adventures (Shackleton 1911). He also 
took photographs and collected rock specimens. 
Later that winter (June 14) the volcano was seen 
in eruption from their base, steam issuing from 
the crater, although no lava was observed on the 
flanks of the cone. 

With the coming of spring, preparations were 
made for the two major assaults of the expedition; 



Shackleton's push for the geographic pole and an 
attempt by a northern party (David, Mawson and 
McKay) to reach the South Magnetic Pole. The 
route was along the coast of Victoria Land as far 
as the Drygalski Glacier Tongue, where they were 
to turn inland climbing onto the Polar Plateau 
towards the pole. A general survey of the geology 
of the coast and where possible of the Western 
Mountains was an important part of the program. 
The early stage of the journey was along the edge 
of the sea-ice with outcrops confined to occasional 
rocky bluffs projecting from under the ice-cap. 
Observations were made at Cape Bernacchi 
(marble), Cape Irizar, Granite Harbour and Depot 
Island. The rocks encountered were highly altered 
(metamorphic) and included gneiss and schist 
together with granite (itself metamorphosed) and 
basic lavas. Looking inland through field-glasses, 
these lavas were seen at a higher level to overlie 
the granites and in turn to be succeeded by 
stratified rocks which were taken to be the Beacon 
Sandstone, discovered and described by Ferrar 
(1907) on Scott's first expedition (1901 03). 
David described Depot Island as \.. most 
wonderful geologically and a perfect elysium for 
the mineralogist'. Mawson relished the variety of 
rocks and minerals they found, among them 
epidote, pyrite, copper pyrites (chalcopyritc), 
garnet and manganese oxides, some of which he 
thought might prove of economic value. Certain of 
the rocks, notably the gneiss and granite reminded 
him of those in the Broken Hill area. Meanwhile 
the ubiquitous glacial debris (moraine) dumped at 
the melting ice-front was a rich source of 
supplementary evidence of what lay further inland, 
below the ice-cap. Erratics at one locality were 
very similar to the Victor Harbor Granite. 

The ascent of the plateau became an ordeal and 
any thoughts of geology were replaced by 
concentrating on the dash for the magnetic pole. 
The elusive and ever-wandering point was reached 
on 16 January 1909. The return journey proved a 
battle for survival and the party was very fortunate 
to make the rendezvous with the 'Nimrod' and 
safety. 

The information collected by the Magnetic Pole 
parly made a valuable contribution to the 
geological results of the expedition. Notably, 
David and Mawson were able to build on Ferrar's 
earlier work and show that Victoria Land 
comprised a basement complex of metamorphic, 
igneous and mineral-rich rocks of assumed 
Precambrian age, overlain by a sedimentary 
sequence, which, on the limited evidence 
available, included rocks intermediate in age 



DOUGLAS MAWSON GEOLOGIST 



115 




FIGURE 4. Mawson, seated, on his return from Antarctica, 1909. Howchin stands at his right shoulder. Photo: P. 
Driver-Smith. 



between the basement and the Beacon Sandstone. 
For Mawson the expedition proved a 
stimulating and scientifically rewarding 
experience. His desire to experience modern 
glacial processes in action had been achieved and 
the insights gained were to be developed on his 
next journey south and later applied to the ancient 
glacial deposits of South Australia. Above all, his 
participation in the Shackleton expedition had 
determined his lifelong interest in the southern 
continent. 



Interlude 

Mawson returned to Adelaide in April 1909 to 
a hero's welcome (Fig. 4), but within a few weeks 
he was back in the Olary-Broken Hill country, 
hiring a horse and dray and continuing his 
investigations among the mineralised rocks and 
the ancient glacial beds of the arid north. After 
completing his fieldwork, he spent some time in 
Broken Hill writing up his results, and on 
laboratory studies of the mineralogy and 
petrography of the key rock types. He was 
particularly impressed by the pegmatites which 
were such a prominent feature of the region and 
wrote: 'In no other part of the world can pegmatite 
formations occur on a more extensive scale'. The 



study of pegmatites was at that time in its infancy 
and Mawson recognised that in Olary he had 
evidence of their importance as 4 a connecting link 
between the igneous rocks and the differentiated 
products economically worked as ore deposits'. 
His fieldwork, and the subsequent published 
review (Mawson 1912a; Fig. 5) of all aspects of 
the geology and economic geology of this 
important and yet little known mineral province, 
was a major contribution to South Australian 
geology and earned him the degree of D.Sc. from 
the University of Adelaide in 1909. 

While in Broken Hill he examined and valued 
several mineral collections from the mines on 
behalf of the South Australian Museum. Some of 
them included specimens of outstanding quality. 
Mawson had first acted for the Museum in 1906, 
when he had successfully acquired the Dunstan 
Collection from the Wallaroo Mines. In 1908 he 
was appointed Honorary Curator of Minerals, thus 
beginning a long and productive association with 
the Museum which was to last his lifetime, and 
which became crucial in later years, as no full- 
time curator responsible for the collection was 
appointed until 1956. The Mawson-Museum 
connection cannot be treated in any more detail 
here. 

Early in December 1909, Mawson left Adelaide 
for London on board the SS 'Mongolia'. He was 



116 



D. W. CORBETT 




FIGURE 5. MawsoTTs interpretation of the geology near 
Olary, South Australia (1912b). Courtesy ANZAAS. 



keen to go to the Antarctic again and full of ideas 
for a scientific program that he hoped would 
appeal to either Shackleton or Scott, both of whom 
he knew had plans for expeditions south. Scott 
was very keen to enlist Mawson (even offering 
him a place in the final polar party), but was not 
prepared to consider any modification of his own 
plans which were already well advanced. 
Discussions were long and frank but when 
Mawson learned that the position of chief scientist 
(which he might have accepted) had been filled 
and his proposal for a western party to explore 
King George V Land unacceptable, he declined 
Scott's offer. He was simply not prepared to 
compromise his purely scientific approach to 
Antarctic exploration. As for Shackleton, initially 
Mawson maintained friendly relations with his 
former leader, even visiting a gold prospect in 
Hungary which Shackleton was convinced would 
make his fortune (and Mawson's too if he came in 
with him as an investor). But becoming 
increasingly disillusioned with Shackleton's 
erratic behaviour and lack of firm plans, Mawson 
followed him to America in an attempt to pin him 
down; and the two signed an agreeement that an 
expedition would leave late in 1911 and should 
Shackleton be unavailable as leader Mawson was 
to take over and receive all Shackleton's support 
and assistance in raising funds. Ever the realist, it 
was clear to Mawson that the responsibility for 
mounting the expedition was most likely to be his 
and so it proved. He was then faced with the 
daunting task of raising funds quickly and in 
competition with Scott who had a head start and 
the advantage of being based in London. Mawson 
returned to Adelaide. For the next eight years the 
Antarctic was to dominate his life. But for a brief 
interlude he returned to academic life and his 
research activities and to these we now return. 



Radioactive Minerals: Radium Hill and Mount 
Painter 

Mawson's involvement with radioactive 
minerals had been renewed soon after his arrival 
in South Australia when in May 1906 carnotite, a 
highly radioactive mineral, was found in ore taken 
from a mine 24 miles east-south-east of Olary. H. 
Y. L. Brown visited the site and issued a report in 
which he speculated that the mineral was a 
decomposition product of primary uranium ores 
occurring at depth. In August, Mawson obtained 
samples which he passed over to E. H. Rennic, 
Professor of Chemistry, for analyses which 



DOUGLAS MAWSON GEOLOGIST 



117 




s g 



FIGURE 6. Geological cross-section in the Mt Painter 
Arkaroola area (1912b). Courtesy ANZAAS. 



suggested that black minerals initially identified 
as magnetite, were far more complex. This 
prompted Mawson to visit the mine and make a 
detailed survey of the exposed reefs which had 
been pegged originally in the belief that the 
prominent black mineral was a tin-bearing ore. 
Further examination showed that while the 
magnetic iron/titanium mineral was dominant in 
the main reef, a rarer black mineral with a 
distinctive and very brilliant lustre also occurred 
as grains, streaks and cubic crystals. Analysis 
shows that in addition to a high percentage of iron 
and titanium the mineral also contained rare earth 
elements together with uranium, vanadium and 
chromium. Mawson proposed the name Davidite 
for what he believed to be a new mineral species 
in honour of his former teacher (Mawson 1906). 
He also identified Roscoelite, a bright green 
vanadium-bearing mineral. At a time when 
knowledge of radioactive minerals was in its 
infancy, Mawson recognised the deposit as a 
significant discovery, possibly of economic 
importance, and named the locality Radium Hill. 
He was optimistic but cautious in his appraisal: 
'This body of radio-active ore is, in the matter of 
quantity, much the most important yet discovered 
in Australia. Its low grade, however, introduces 
serious difficulties to commercial enterprise in this 
direction'. Radium Hill was to have a long but 
intermittent history based on the working of its 
radioactive lodes (Fig. 7), and Mawson was to 
renew his interest in the deposit in the 1920s. 

Mawson visited the Flinders Ranges for the first 
time towards the end of 1910, during his short 
spell in Adelaide between Antarctic expeditions. 
He had received a visit from W. B. Greenwood, 
the owner of Umberatana Station, who had 
brought some specimens of a bright green mineral 
which Mawson identified as torbernite, an 
hydrated phosphate of copper and uranium. 
Greenwood had been prospecting in the northern 
ranges on behalf of the Mines Department for 
several years and had become annoyed when 
specimens, including the green mineral, which he 
had left at the Department some time before had 
not received attention; whereupon he had retrieved 
them and taken them to the University. Excited by 
the prospect of another radioactive mineral deposit 
in South Australia, Mawson headed north and, 
with Greenwood and renowned prospector Harry 
Fabian, made an examination of the geology and 
mineral occurrences in this most rugged and 
inaccessible part of the Flinders, attempting to 
place the local geology in the broader regional 
context (Fig. 6). The short visit marked the 



118 



D. W. CORBETT 



beginning of his long and fruitful association with 
the geology and mineral resources of the region 
and his field notebook for the trip is full of detail 
of his observations and the excitement of 
discovery; for example: 'The results of my recent 
journey have been in the highest degree 
satisfactory... My main objective was the 
investigation of the metamorphic rocks eastward 
of Yudnamutana in connection with the 
interpretation of the Barrier Ranges, a subject in 
which I have long been absorbed. . . ' 

With regard to the potential of the uranium- 
bearing lodes he wrote : '... the outcrop is on the 
whole low grade, though richer patches are met 
with at intervals. Improvement may be expected 
below. The ore can be treated very inexpensively 
and this will offset the low-grade character. So far 
as I am aware this is the most extensive 
uraniferous lode formation in the world'. The back 
of his field notebook contains estimates of costing 
for ore extraction, transport, freight and handling, 
including comparisons for treatment on the spot, 
at Port Pirie or in England. There would be a need 
for roads and wells and for camels to bring out the 
ore. If the grade proved high enough, he foresaw 
the setting up of a company to work the ore — the 
Radium Extraction Company. He even worked out 
the capital required - £20 000. These estimates 
may have been doodlings around the campfire, at 
the latest they were put on paper soon after his 
visit, and they have an immediacy which reveal 
Mawson's keen interest in the region, its 
economic potential and his desire to be part of the 
action. He was not to return north for more than a 
decade. Over the next few years some intermittent 
mining activity took place at Mount Painter, but 
with the outbreak of World War I activity ceased. 



South Again - The Australasian Antarctic 
Expedition (AAE) 1911-14 

In January, 191 1, Mawson gave a lecture to the 
combined geology and engineering groups at the 
annual meeting of the AAAS in Sydney. It was a 
fund raising exercise designed to appeal to 
national pride as well as pointing out the scientific 
and future economic potential of the southern 
continent. He stressed that: 'the collection of 
scientific data (was) obligatory upon us ... its 
mountains were blessed with mineral resources ... 
(and) it holds among its fossil strata secrets 
especially interesting to Australians'. Science was 
to be linked to technology and the latest 
developments — the wireless and motor sledges — 



still to be tested down south, were seen as a vital 
aid to scientific exploration. The burdens of 
leadership were enormous leaving little time for 
any geological researches of his own, but Mawson 
recruited a strong team of four geologists who 
were to carry out valuable surveys over a great 
expanse of territory. Cecil Madigan, later to join 
his leader at the University of Adelaide, was 
appointed meteorologist. 

Reaching the area selected for the expedition's 
base, the expedition ship 'Aurora' had great 
difficulty in breaking through the ice barrier and 
was forced to cruise westward; Mawson had 
hoped to find the Antarctic continent in these 
latitudes bounded by a rocky and attractive coast 
like that in the vicinity of Cape Adare, the nearest 
well-explored region. The poor prospects of 
carrying out extensive geological work under such 
conditions must have been a blow, but Mawson 
was impressed and awed by the sheer physical 
presence and power of the ice and its dominance 
of the environment: 'The land was so 
overwhelmed with ice that, even at sea-level, the 
rock was all but entirely hidden. Here was an ice- 
age in all earnestness; a picture of northern Europe 
during the Great Ice Age some fifty thousand 
years ago' (Mawson 1915, 1996 p. 40). 

The main base was established at Cape Denison 
(Commonwealth Bay) and a western base party, 
including two geologists, some 1 500 miles (2 400 
km) further along the coast to the west on the 
edge of the Shackleton Ice-Shelf. The vicinity of 
Cape Denison was comparatively ice-free 7 and the 
geologists were able to study glacial erosion and 
deposition at first hand. The rocks outcropping 
near the main base were predominantly 
metamorphic — folded and contorted gneiss and 
schist of presumed Precambrian age. Evidence of 
ore-bearing minerals was also found, among them 
iron, copper and molybdenum which Mawson 
believed gave promise of larger bodies in the 
vicinity and indicated the probability of mineral 
wealth beneath the continental ice-cap. Around 
the edge of the ice margin, the terminal moraines 
were 'a veritable museum'. Rocks, showing every 
variety in colour and form, were assembled, 
transported from far and wide over the great 
expanse of the continent ... The story of the buried 
land to the south is in large measure revealed in 
the samples brought by the ice and so 
conveniently dumped' (Mawson 1915, 1996 pp. 
74-76). After a particularly severe winter with 
hurricane force winds, the summer journeys 
commenced, and much valuable scientific work 
carried out. A western party made a particularly 



DOUGLAS MAWSON GEOLOGIST 



119 



interesting find, the first meteorite from 
Antarctica, duly named the 'Adelie Land 
Meteorite 7 , and the first of many to be found in 
later years. 

Mawson himself, with Ninniss and Mertz and 
the dogs, set off on the longest and most 
ambitious of all the journeys, striking east on a 
southerly course in an attempt to cover as much 
territory as possible in the time available. The 
story of that harrowing journey which cost the 
lives of both of Mawson's companions, and of his 
miraculous return against overwhelming odds just 
in time to see the 'Aurora' disappear over the 
horizon, is an epic story of endurance, fortitude 
and sheer will power which has been well told by 
Mawson himself in L The Home of the Blizzard' 
(Mawson 1915) and by Bickel (1977). Mawson 
and the small remnant of the expedition left 
behind to search for him had to face another 
Antarctic winter. The 'Aurora' returned in 
December 1913 and on the 26 February 1914, 
Mawson arrived back in Adelaide. 



The War Years and After 

The expedition was home, but for Mawson 
there was to be no respite and it was to be a 
further six eventful years before he was able to 
resume an ordered academic life again. The First 
World War began as he was returning from an 
overseas business trip to Europe concerned with 
the wind-down of the expedition, and by 1916, 
after travelling to the United States, he was back 
in Britain where he spent the remainder of the war 
on highly responsible government work with the 
Ministry for Munitions. He did not return to 
Adelaide until May 1919. Back at the University 
he found that little had changed in his absence 
except that Walter Howchin had been awarded the 
title of Honorary Professor in Geology and 
Palaeontology in 1918. Mawson (1944a) wrote 
later: '1 was not a little confounded. 1 would have 
packed up and left immediately but for the 
supreme consideration of faithfully recording and 
adequately publishing the immense mass of data 
received during my Antarctic Expedition'. Early 
in 1920 he talked with Howchin about the future: 
'stating that I was not prepared to continue at 
Adelaide for another year under the then existing 
inadequate arrangements for geology'. There was 
no prospect of the much-needed new building for 
geology and Mawson tied himself to a 
compromise twenty year agreement on additional 
accommodation which proved increasingly 



inadequate as years went by, and which he was 
later to regret. Meanwhile, Howchin's continuing 
presence at the University was perceived by 
Mawson as a hindrance to the satisfactory 
development of the Geology Department and it 
must have been a great relief to him when 
Howchin, then 75, decided to retire at the end of 
the year. 

In 1 92 1 Douglas Mawson was appointed to the 
newly created Chair of Geology and Mineralogy, 
and Dr Cecil Madigan, his old comrade from the 
Antarctic, joined him as Lecturer the following 
year. Mawson and Madigan were to be the only 
two staff members in the Geology department for 
much of the inter-war period. The establishment 
of the new department and his teaching and 
administrative duties (not to mention continuing 
Antarctic matters) took precedence in the early 
1920s but field investigations were resumed in 
both the Olary region and the north Flinders 
Ranges. While he built on his work in the 
Boolcomatta area, locating several key sections 
spanning the junction between the basement and 
overlying sedimentary sequence, he was never to 
resume a sustained fie Id work program in the 
region, despite the urgings of David. 

David's retirement at the end of 1923 and the 
politics involved in choosing his successor proved 
unsettling for Mawson who at that time was still 
not fully committed to staying in Adelaide and 
applied for the job, and although the best qualified 
of the candidates, he was ultimately unsuccessful 
because of David's influence on the course of 
events and his (perhaps over-zealous) loyalty and 
support to Leo Cotton, his deputy and locum for 
many years, who was appointed to the Chair. The 
outcome certainly posed strains on the David- 
Mawson relationship, and further tensions and 
distractions were to follow when David's 
increasing obsession with the search for supposed 
Precambrian fossils focussed on the old rocks in 
South Australia (see also pl24, End of an Era). 
On an earlier visit to Adelaide in 1921, David had 
found what he believed to be arthropod remains in 
the old rocks at Reynella (long considered by 
Howchin as Early Cambrian) tentatively placing 
them in the late Precambrian (Proterozoic) and 
proposing a new division the Adelaide Series. 

Meanwhile, Mawson turned his attention to the 
north Flinders once again. He had published a 
brief comparison of the Mount Painter and Olary 
provinces (Mawson 1912b), but the results of his 
investigations around Mount Painter in 1910 were 
treated more fully in a long-delayed paper 
(Mawson 1923) in which he recognised a core of 



120 



D. W. CORBETT 



:•' 




MM 



FIGURE 7. The Radium Hill Mine, soon after its discovery. Mawson, 1944b, pi. 19. Courtesy Royal Society of South 
Australia.. 



* #:i 




FIGURE 8. Mount Gee, viewed from the west. Mawson, 1944b, pi. 19. Courtesy Royal Society of South Australia. 



DOUGLAS MAWSON GEOLOGIST 



121 



Precambrian igneous and metamorphic rocks 
overlain by a sedimentary series similar in many 
respects to those overlying the basement in the 
Adelaide region. He followed David's lead in 
applying the term Adelaidean (Adelaide Series) to 
these sediments and suggesting a Proterozoic (late 
Precambrian) rather than Cambrian age. Igneous 
activity included two acid phases, the second with 
pegmatites and aplites followed by a volcanic 
phase characterised by vesicular basalts. The 
mineralisation of the Mount Painter-Mount Gee 
area, notably the quartz reef at Mount Gee and the 
uranium minerals (torbernite and autunite) at 
Mount Painter, was described in detail (Fig. 8). 

Following Mawson's enthusiastic report on the 
uranium potential of the area after his initial visit 
in 1910, several companies had been floated and 
prospecting carried out on Radium Ridge and 
Mount Gee. Meanwhile the Mines Department 
had been more cautious but in favour of further 
prospecting. Sporadic attempts at developing the 
prospects (notably the No. 6 workings) had 



languished during the war, but in 1924 there was 
renewed interest in radioactive ores world-wide 
and a return to the Mount Painter field seemed 
justified. Consequently, Mawson returned north in 
November 1924 and spent much of his time in the 
Mount Painter area on detailed study of the 
mineralised rocks but also in broader scale 
assessment of the regional context of the 
mineralisation. 

The regional geology of the Flinders Ranges 
was little known at this time. Howchin had made 
a pioneer traverse from west to east at the level of 
the Parachilna Gorge in 1907 but the results were 
not published until 1922. While on his return trip 
from the north, Mawson had the good fortune to 
make a particularly significant discovery just west 
of the Italowie Gorge. It was a case of the 
prepared mind recognising the significant 
evidence and provides a good example of 
Mawson's versatility as a geologist, for fresh from 
the mineral riches of the Mount Painter country he 
was now to show that he had a good eye for a 




FIGURE 9. Entenng Yudanamutana. Mawson, 1923, pi. 33. Courtesy Royal Society of South Australia. 



122 



D. W CORBETT 



fossil also. What he found were 'curious 
markings' on roadside outcrops of limestone which 
'on inspection ... was found to be due to massed 
fossil heads of a Cryptozoon-Wkt alga ... developed 
in a massive formation, the algal remains 
constituting the bulk of at least some of the beds' 
(Mawson 1925). Similar structures had been 
reported from the MacDonnell Ranges by 
Chewings and described by Howchin (1914) but 
there was as yet no general agreement on their 
stratigraphic position. Mawson inclined towards an 
Early Cambrian age, but David, on hearing of the 
find thought they might be older (Proterozoic). Very 
little was then known of Precambrian life forms; 
most of the obscure remains described being 
referred to as Crpytozoon (hidden life)— but the 
recently announced discovery of algal fossils in 
Precambrian rocks in Montana by Walcott 
suggested that the Flinders rocks might be of 
similar age. David certainly believed so and urged 
Mawson to investigate further. Mawson's 



'Cryptozoons' are now recognised as algal 
stromatolites, These columnar and dome-shaped 
structures produced by the trapping of sedimentary 
particles by mats of blue-green algae are the earliest 
abundant fossils and are well developed in certain 
of the Precambrian rock formations in the Flinders 
Ranges. Mawson, however, was not to be 
pressured into narrow specialisation and continued 
his wide-ranging investigations of Flinders Ranges 
geology (Figs 9, 10), publishing further papers in 
the mid 1920s. One was on the volcanic rocks of 
the Wool tana area (Mawson 1926a), first 
encountered in Arkaroola Creek in 1910 and 
subsequently examined near Wooltana on a brief 
visit in 1924. There he found a thick sequence of 
volcanics — vesicular lavas, tuffs and agglomerates 
overlain by boulder beds and finer sediments which 
he described as: 'most probably of fluvio-glacial 
and glacial origin'. Large granite boulders higher 
in the section were even more convincing, leaving: 
\.. no doubt in my mind ... as to the glacial nature 




FIGURE 10. The quartzitc of the Yudanamutana Gorge. Mawson, 1923, pi. 33. Courtesy Royal Society of South 
Australia. 



DOUGLAS MAWSON GEOLOGIST 



123 



of these beds,..' Sediments above the glacials, 
unsuccessfully searched for fossils, were believed 
of likely Late Precambrian age. 

Another spin-off from the 1924 North Flinders 
trip was a visit to the Paralana Hot Springs which 
interested Mawson because of the radioactive 
nature of the waters (Mawson 1927a). For a short 
period about this time an enterprising doctor had 
sought to capitalise on the supposed therapeutic 
qualities of the spring by setting up a spa on the 
site, although with no success. The springs are 
situated close to the faulted junction between the 
old rocks of the ranges and the younger sedimentary 
basin to the east. While most geologists supported 
an origin from deep-seated basin waters, Mawson 
speculated on a possible contribution from the 
highly uranium-rich rocks lying to the west. He 
collected water and gas for examination, hoping the 
latter would prove rich in helium. Unfortunately the 
samples did not survive the journey back to 
Adelaide. The highly active gas which at first 
puzzled the analysts, has since proved to be rich in 
radon; the water is much less radioactive. 

Mawson had made a brief visit to the Willouran 
Ranges on the north western flank of the Flinders 
in 1920. From here he described and named the 
Willouran Series—a thick sequence of 
sandstones, slates and calcareous beds underlying 
a dominant quartzite formation and forming a 
synclinal structure (Mawson 1927b). Sediments of 
probable fluvio-glacial origin were also found in 
the eastern part of the area. 

Mawson's activities in the Flinders Ranges 
during the 1920s were essentially of a 
reconnaissance nature and based on relatively 
little time, overall, spent in the field. The 
information included in the papers cited above 
demonstrate how much he could gain from a brief 
investigation, displaying his strength as a field 
worker and skill in rapidly appraising the 
geological situation in unknown country, and 
revealing his pre-eminence as an explorer- 
geologist. Work carried out during this period, 
while not yet part of a coordinated research 
programme, provided the basis for his later 
systematic approach to regional studies in the 
1930s and 1940s. 

Away from his empirical work in the field, he 
demonstrated a comparable ability to synthesise 
existing knowledge in a lengthy treatment of the 
igneous rocks of South Australia, delivered as a 
Presidential Address at the AAAS meeting at 
Perth in August 1926 (Mawson 1926b). This was 
an important review, given the widespread 
distribution and importance of igneous rocks, 



notably in the older terrains of the State, but also 
in those of younger age. By discussing them 
region-by-region in their structural and 
stratigraphic context, he produced what was 
essentially a geology of the State. One issue of 
particular interest, not to be resolved for many 
years, was the age of the highly metamorphosed 
sediments on the eastern flank of the Mount Lofty 
Ranges and their associated intrusives. With 
reference to Howchin's view that these rocks were 
the equivalents of the Adelaide Series, Mawson 
urged caution, pointing out: 'the geological 
mapping of the Ranges is yet only in the early 
stages (and) final conclusions are unsafe until 
more detailed petrology and complete geological 
mapping have been accomplished'. As for the 
Victor Harbor granites Mawson comments 
perceptively: 'there is yet no convincing evidence 
against the assumption of an early Palaeozoic age 
for this granite'. 



Central Australia 1927 

In November 1927, Mawson and Madigan 
made a short visit to Alice Springs and the 
Western McDonnell Ranges to check a mineral 
occurrence which had excited local interest. A 
white crystalline substance, long known to the 
aborigines and which burned with a fierce flame, 
was thought possibly to have some connection 
with petroleum. Specimens had been brought to 
Adelaide (initially to Madigan), and identified by 
Mawson as potassium nitrate (saltpetre or nitre) a 
rare mineral with some economic use in the 
chemical and explosives industries. Realising the 
opportunity for geological exploration in an area 
still little known geologically, Mawson quickly 
organised an expedition to investigate. They 
travelled north by train to Alice Springs, and their 
car journey out through the western ranges from 
Alice Springs blazed a trail through country never 
traversed by vehicle before. The deposit proved to 
be of organic origin, the long-time accumulation 
of animal droppings, of scientific but not 
economic interest. 

Much of the route west ran along the strike of 
the well-exposed sedimentary beds which gave a 
general indication of the southward dipping 
succession between the Precambrian crystalline 
basement and known Ordovician rocks of the 
Horn Valley. Traverses were run and rough 
sections made at several localities along the way, 
including Ellery Creek, and over 10 000 feet of 
strata were measured. In the lower beds 



124 



D W. CORBETT 



'cryptozoal limestones' and organic structures 
similar to those from the Flinders Ranges were 
prominent in several areas, while worm tracks and 
traces of mollusc shells together with algal 
limestones distinct from those lower in the 
sequence were found in the younger beds. On the 
basis of his limited field evidence, the sedimentary 
sequence was divided into two divisions — the 
Pataknurra and Pataoorta Series, once again 
showing his flair for the rapid assessment of the 
general geological situation in a new area. He 
made tentative and essentially correct correlations 
between the central Australian rocks and the older 
sequences in South Australia. This first and, as it 
proved, only venture into central Australian 
geology was a major contribution to knowledge of 
the region, building on and revising the earlier 
work of Tate and Watt (on the Horn Expedition), 
H. Y. L. Brown, C. Chewings and L. K. Ward. 

Mawson visited London the following year 
where he exhibited photographs and specimens at 
the Geological Society. The results of the 
expedition were published by the Society 
(Mawson & Madigan 1930). While circumstances 
determined that Mawson never returned to the 
Centre, it seems likely that he always envisaged 
following up the promising results of his first trip. 
Madigan, meanwhile, had been captivated by the 
Centre and immediately began his own 
independent and wide-ranging researches into the 
geology of the region which were to produce some 
of his best work. This perceived 'take-over' by 
Madigan was resented by Mawson and led to bad 
feeling between the two men, but Mawson was 
soon to be occupied with other matters. 



BANZARE 1929-31 

Mawson was very much involved with 
Antarctic matters from 1929 through into the early 
thirties. BANZARE (The British, Australian and 
New Zealand Antarctic Research Expedition) 
differed from Mawson's previous expeditions in 
being ship-based. The program was carried out on 
two summer cruises (1929-30, 1930-31) and 
while no land bases were established, limited 
sorties were made ashore, notably on some of the 
sub-Antarctic islands. With the emphasis on 
marine science, much of the data was collected by 
systematically sounding the depth of the offshore 
waters, sampling the water column and dredging 
the bottom for biological specimens. Because of 
the nature of the expedition, geological work was 
restricted, although sediments collected from the 



sea-floor adjacent to the land and the variety of 
ice-transported boulders dropped there provided 
abundant evidence of sedimentation and 
sedimentary processes in a modern glacial 
environment. The BANZARE expedition further 
inspired Mawson to continue his study of the 
ancient glacial deposits in the Flinders Ranges, 
and he was to do this with renewed vigour in the 
years ahead. 

The extended geographical and geological 
knowledge of Antarctica resulting from the 
BANZARE voyages enabled Mawson to be the 
first to postulate the existence of an extensive 
landmass lying beneath the southern ice-cap and 
bounded by a wide continental shelf. Much of the 
evidence for the geological make-up of this buried 
continent came from the ocean-floor studies where 
dredged boulders proved to be rocks of continental 
type. Mawson envisaged that the mineral 
resources of Antarctica, the existence of which his 
expeditions had suggested but were yet to be 
proven, would be developed at some time in the 
future, and that underground mining operations 
could be carried out successfully despite the 
problems of climate and terrain. 



End of an Era 

Professor Edgeworth David died in 1934. In his 
later years he had become increasingly obsessed 
with his recognition of 'fossils' in the Precambrian 
rocks of South Australia (David 1928). Most of 
his finds had been made on visits to Adelaide at 
times when Mawson was away overseas or 
otherwise engaged on Antarctic business and had 
no chance to control these incursions. For 
Mawson it was particularly galling for David to 
hint that his old student was sitting on a rich 
treasure trove of Precambrian fossils while he, 
David, made the pickings, even enlisting 
Mawson's students and staff to help him collect. 
Wisely, Mawson held his counsel and 
endeavoured not to be drawn into the matter. It 
soon became clear, to almost all but David, that 
the supposed 'fossils' were in fact inorganic in 
origin (a verdict upheld by later workers), but he 
was to persist in his belief through to the end of 
his life, considering his discoveries in South 
Australia to be the highpoint of his career. 



Deciphering the Flinders 

In the mid- 1930s Mawson renewed his long- 



DOUGLAS MAWSON GEOLOGIST 



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DOUGLAS MAWSON GEOLOGIST 



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standing but formerly sporadic association with 
the Flinders Ranges. Now for the first time with 
fewer distractions, he was able to develop and 
pursue a sustained and systematic ficldwork 
program the results of which constitute his most 
notable contribution to South Australian geology. 
Only a brief resume of this work is given here, to 
be treated more fully in a later paper. 

The Flinders Ranges were sparsely populated in 
the 1930s, and moving around in the outback 
more arduous than today. Roads and tracks were 
in general poorly maintained and motor transport, 
then in its infancy, was still an adventurous 
undertaking. There were no photo-based maps or 
accurate large-scale topographic maps available in 
those days, the only maps available being pastoral 
plans which were quite inadequate as a base for 
geological mapping. Mawson's approach was to 
select key sections which were measured and 
described in detail. In a few of his papers, small- 
scale regional maps were included. He first used 
aerial photography as an adjunct to his ficldwork 
in the late 1940s. Field-camps in the pre- and 
early war years combined the instruction of senior 
(third year) students in field techniques, including 
section measuring, with the gathering of basic 
geological information in country previously 
geologically unknown. 

By 1939, having spent time in the Wooltana, 
Mount Carnarvon, Parachilna Gorge and Italowie 
areas, Mawson's work in the Flinders had reached 
a stage where review was warranted, and two 
publications in that year, on the Late Precambrian, 
and Cambrian successions respectively (Mawson 
1939a, 1939b), detail rock sequences in the 
Brachina Creek-Oraparinna and Wirrealpa Basin 
areas of the central ranges (Fig. 11). The Pound 
Quartzite, the dominant ridge-former of the 
Flinders which occurs some distance 
stratigraphically below the oldest fossiliferous 
Cambrian rocks, was provisionally placed at the 
base of the Cambrian on lithological grounds and 
interpreted as marking the start of a new cycle of 
sedimentation. Defining the Precambrian- 
Cambrian boundary was to become of increasing 
interest to geologists in the years ahead, a task 
made no easier by the lack of fossils and by the 
absence of major breaks in sedimentation in the 
thick Upper Precambrian to Cambrian 
sedimentary sequence in South Australia. In his 
Wirrealpa Basin paper, two important 
fossiliferous units are described: the 
Archaeocyatha Limestone and a younger 
limestone (the Wirrealpa Limestone) first 
described by Howchin but here fully documented 



for the first time with its fossil fauna of algal 
remains {Girvanella), brachiopods (Oboiella), 
pteropods and trilobite fragments (Redlichia). 

Other papers were to follow dealing with 
sequences in the Aroona, Copley, Brachina and 
Wilpena areas and culminating in an important 
review, 'The structural character of the Flinders 
Ranges' (Mawson 1942), which brought together 
the results of his fieldwork program to that time. 
A small scale map (Fig 13) showed the location 
of the key sections measured and the distribution 
of the rocks spanning the four main periods of 
deposition: the Middle Proterozoic and Late 
Proterozoic, the Cambrian and the Tertiary- 
Recent. Key marker beds, including the prominent 
Pound and ABC Quartzites, tillites and 
hieroglyphic limestones were also delineated. A 
cross-section (Fig. 12) indicated the essentially 
simple anticlinal structure of the central ranges. A 
wider-ranging paper (Mawson 1947) extended 
and amplified his earlier work, adding new 
information from the western flank of the ranges 
both in the north (near Copley) and in Mundallio 
Creek to the south. In both areas Mawson 
recognised thick quartzite formations at the base 
of the sequence, pointing out the error made by 
Segnit (1939), working for the Mines Department, 
who had equated these ABC Quartzite sequences 
with the Pound Quartzite. Mawson, however, was 
himself misled in the area west of Quorn where he 
mistook the prominent folded ABC Quartzite as 
Pound Quartzite (here thinly developed). Such are 
the dangers of making correlations on lithological 
grounds in rocks without fossils to act as age 
indicators. 

Mawson also discussed the Flinders succession 
in its broader tectonic framework which he 
considered a major trough of deposition of Late 
Precambrian to Cambrian age and referred to as 
the 4 great synclinal basin' (later to be named the 
Adelaide Geosyncline). His work had 
demonstrated the great thickness of strata 
deposited in the trough which extended south from 
Central Australia to the Adelaide region and lay 
between two ancient Precambrian massifs: 
Yilgamia to the west and Willyamia to the cast. 
The flat-lying sedimentary cover-rocks to the west 
of Port Augusta, believed on lithological and 
structural grounds to be correlates of the basal 
quartzites in the western ranges are now known to 
be ABC Range Quartzite equivalents. Wider 
correlations of the Flinders Ranges succession 
with the rocks of the western Mount Lofty Ranges 
(comparisons with the still largely unresolved 
sequence on the eastern flank of the Mount Lofty 



128 



D. W, CORBETT 



THE CENTRAL AREA OF THE FLINDERS RANGES 




\ \ \ \ \ \ N 



FIGURE 13. Mawson's geological map of the central Flinders Ranges. Mawson, 3942. Courtesy Royal Society of 
South Australia. 



DOUGLAS MAWSON GEOLOGIST 



129 



Ranges still remain highly speculative), with 
Central and Western Australia and also with 
South Africa (Transvaal System) were also 
suggested and discussed (Mawson 1947). 

In the early 1940s Mawson returned to the 
North Flinders investigating the metamorphic 
effects of plug-like granite intrusions in the 
Precambrian country rocks (Mawson & Dallwitz 
1945a,b). This study of both the sedimentary and 
igneous aspects of the geology of the region linked 
his early work on the older mineralised terrains in 
the Mount Painter area with his later concentration 
on unravelling the stratigraphy of the overlying 
sedimentary sequence, 



Ancient Glaciation 

Mawson first encountered evidence of ancient 
glaciation on his trip to the north Flinders in 1910. 
Subsequently he had demonstrated the widespread 
distribution of glacial rocks in the ranges during 



his extensive field investigations (Fig. 14). His 
Antarctic experience of a glaciation-in-being, with 
the diversity of its products and processes, from 
the coarse boulder beds of terminal moraines to 
the finely layered sediments laid down in tranquil 
glacial lakes, had equipped him, as he had 
intended it should, to recognise the varied and not 
always easily interpreted evidences for former ice- 
ages. 

By the late 1940s, Mawson had established the 
stratigraphic position of the Sturt Tillite in many 
areas of the Flinders and also identified a younger 
glacial episode in the Elatina area on the western 
flank of the central ranges (Mawson 1949a). The 
distinctive sediments— coarse sandy beds overlain 
by a thick unstratified boulder bed — first 
encountered in 1938, had initially been thought to 
be of pyroclastic origin (Mawson 1938) because of 
the preponderance of igneous pebbles in the rock. 

Mawson then produced evidence for a third 
glacial event, this time predating the Sturt Tillite 
(Mawson 1949b), in the deeply eroded high 




FIGURE 14. A large striated erratic weathered out of Proterozoic tillite, Yankarunna Station. Photo R. H. Jones. 
Mawson, 1945, pi. 14. Courtesy Royal Society of South Australia. 



130 



D. W. CORBETT 



country of the Bibliando Dome east of Hawker. 
Here a thick sequence of glacials and associated 
beds revealed two extended periods of glaciation 
separated by a well-defined inter-glacial interval. 
The younger glacial event was equated with the 
Stmt Tillite while the older (lower) tillites were 
referred to as the Bibliando stage. 

The clear demonstration of a third glacial phase 
in the history of the geosynclinal basin, with a 
broad range of deposits from boulder tillites 
through coarse fluvio-glacial sediments to fine 
laminated shales, raised such questions as the 
interpretation of past geographies, climates and 
environments, and the cyclic nature and causes of 
glaciation. Mawson, with his deep and extensive 
knowledge of ice-action both ancient and modern, 
was, more than any other geologist of his 
generation, aware of the diversity, complexity and 
the problems associated with interpreting glacial 
evidence. He discussed some of these in his paper 
on Bibliando, which marks the culmination of his 
career-long investigation of glacial phenomena. 
He took the opportunity to view this latest work in 
a broad historical perspective. The early 
discoveries of Selwyn, Tate and Howchin had 
placed South Australia at the forefront of research 
in the study and understanding of past glaciations. 
His own work had extended and clarified that 
knowledge, setting it within the wider context of 
the development of a major Upper Precambrian 
geosyncline, the importance of which had now 
become apparent. 

While the rocks in the Flinders are 
magnificently displayed and accessible for study, 
the lack of fossils in the ancient rocks have always 
made the task of the stratigrapher difficult. 
Mawson, the first geologist to systematically 
approach the task of establishing an ordered 
succession was acutely aware of this problem. As 
his work proceeded and became recognised 
beyond South Australia, he perceived the need for 
a standardisation of geological nomenclature, 
particularly of stratigraphic names, and he was a 
member of the first committee set up by ANZ AAS 
in 1947 which led to a Code of Stratigraphic 
Nomenclature being formalised in 1950. 

Mawson favoured dropping the long- 
established but restricted Adelaide Series of 
David and Howchin and replacing it with the 
Adelaide System which he sub-divided into the 
Torrensian, Sturtian and Marinoan Series 
(Mawson & Sprigg 1950). The defining of the 
Adelaide System marked the end of Mawson's 
work on the old rocks of South Australia. The 
discovery of jellyfish fossils by Reg Sprigg in the 



Pound Quartzitc at Ediacara in 1946 (Sprigg, 
1947, 1949), and the later finds of a diversified 
animal fauna by Flounders and Mincham, led to 
a reappraisal of the stratigraphy of the fossil- 
bearing beds (Glaessner & Daily 1959). 
Relegation of the Pound Quartzite from the base 
of the Cambrian (as previously suggested by 
Mawson) to the uppermost formation in the 
Precambrian meant that the Ediacara fossils, now 
confirmed as the oldest animals known, became 
world famous. 



The South-East 

Contrasting strongly with the rugged grandeur 
of the Flinders Ranges, the geologically youthful 
and topographically unchallenging south-eastern 
region of South Australia attracted Mawson from 
the mid- 1930s. He became interested in the 
problematic 'coorongite', a rubbery bituminous 
substance first discovered in 1852 at Alf Flat east 
of Salt Creek at the southern end of the Coorong 
Lagoon (Fig. 15). A belief that the flammable 
material might be a petroleum product led to 
speculation that oil existed at depth; and several 
(unsuccessful) drilling attempts were made in the 
1880s and again in the 1920s. By then almost all 
investigators had become convinced of the 
vegetable origin of the substance (and it has since 
been shown to be the product of algal blooms). 
Mawson, however, was unconvinced; and he 
inadvertently attracted overseas interest for a brief 
period when he took a visiting petroleum expert 
from Britain (Washington Gray) into the field to 
view the material and Gray went home to 
publicise the find, much to Mawson's chagrin. 
Some biochemical work was carried out overseas 
on the 'algal gel', but the matter was not pursued 
any further. 

More substantial and fruitful work in the region 
led to a series of publications on the small and 
isolated outcrops of granitic rock which protrude 
through the thin Quaternary cover of the Upper 
Southeast. Fieldwork involved exploration on a 
minor scale, for many of the outcrops lay in 
difficult country accessible only on foot or 
horseback and where the outcrops were not 
extensive. The studies were carried out in 
association with students or former students and 
covered a quadrilateral bounded by Meningie and 
Coonalpyn on the north and Kingston and 
Bordertown to the south. The field investigations 
and subsequent analytical work led Mawson to 
recognise a variety of intrusive and extrusive rock 



DOUGLAS MAWSON GEOLOGIST 



131 




FIGURE 15. Mawson, with auger, drilling for coorongite, the Coorong, mid-1 930s. Washington Gray on right. 
Source unknown. 



types in the outcropping basement: granites; 
adamellites and granodiorites; and quartz 
keratophyres (volcanic). Similarities between the 
intrusives of the South-East and those occurring 
along the eastern flank of the Mount Lofty Ranges 
and on Kangaroo Island supported the concept of 
a large granitic batholith existing beneath the 
sedimentary cover, and, on the available evidence. 
Middle to Late Cambrian in age. 



Finale 

Mawson was sixty-three at the end of the 
Second World War and approaching the normal 
age for retirement. He continued on, however, to 
the age of seventy and spent his last university- 
years rounding off his own researches and 
ensuring that his department was left in a healthy 
and secure position to meet the challenges ahead. 



132 



D. W. CORBETT 



THE MAWSON LABORATORIES 

SCHOOL OF GEOLOGY 

UNIVERSITY OF ADELAIDE 




WOODS BAGOT I AT BCUR.KE -SWIT H £^ I R.WI M 

A R. C H 1 T C. C T & . 



FIGURE 16. The proposed Mawson Laboratories. Courtesy Woods Bagot Pty Ltd, Adelaide. 



He had been acutely aware of the greatly increased 
role that geology would be required to play in the 
post-war world. In particular, well trained 
geologists could only be supplied by the 
universities which in turn would need to provide a 
sufficient level of support in terms of 
accommodation, equipment and staffing. In all 
these areas Mawson had been struggling against 
inadequacies for over twenty years. During this 
time, geology had made the best of sub-standard 
accommodation and increasingly inadequate 
provision for research, whereas the rest of the 
University had developed and prospered. It was 
the urgent need for a better deal for geology that 
prompted his memorandum to the University 
authorities in February (1944a). In his 
memorandum Mawson wrote: 'The department 
suffers from insufficiency of room, from 
inadequacy of the laboratories, and from the entire 
absence of any planned layout suitable for a 
science department. All other science departments 
of the University now have buildings specially 
planned for their needs though some are already 
proving too limited in accommodation for the 
flood of students now presenting themselves. Ours 
is an anachronism'. 

He went on to make a very strong case for the 
role of geology in education, its application to 



national development and significantly, South 
Australia's importance as a source of future 
mineral resources. He envisaged Adelaide 
University as a future centre for teaching and 
research in economic and mining geology and 
itemised the basic needs of a modern School of 
Geological Studies, estimating the cost of the new 
development at around £25 000. 

His argument was decisive. The University 
responded appropriately, if belatedly, and the 
Mawson Laboratories were constructed, largely to 
his specifications, between 1949 and 1952 (Fig. 
16). He just had time to move into the new 
building before retirement. By then his staff had 
increased to five and included E. A. Rudd who 
was appointed to the new Chair of Economic 
Geology in 1949, and Martin Glaessner, a 
palaeontologist with an international reputation 
who was to become the authority on the 
Precambrian fossils from Ediacara. Arthur 
Alderman, former student and junior lecturer in 
the department, returned after a period away from 
the University to take over from Mawson as 
Professor of Geology and Mineralogy in 1953. 

In the years following his retirement Mawson 
remained active and influential in Antarctic 
matters and continued his long association with 
the South Australian Museum as Honorary 



DOUGLAS MAWSON GEOLOGIST 



133 



Curator of Minerals and Member of the Museum 
Board. He was appointed Chairman of the Board 
in 1952. 

Douglas Mawson's broad interests in all 
aspects of geological science and his unfailing 
encouragement and support of young people with 
an enquiring mind and an interest in science is 
well illustrated by the background to his last 
published paper (Mawson 1958). It deals with 
australites (small glassy objects of meteoritic 
origin) collected by a young schoolboy, Mervyn 
Pens, from the Murray Plains west of Morgan in 
the mid-1 930s. Mawson had visited the site and 
established a correspondence with young Pens, 
which led to further finds and ultimately to the 
public aquisition of a large and significant 
collection of australites now housed in the South 
Australian Museum. The paper was read before 
the Royal Society of South Australia on 10 
October 1957. Sir Douglas Mawson died on 14 
October 1958. 



Mawson's Legacy 

Mawson's inborn qualities as an explorer, his 
methodical approach to the job in hand, his 
tenacity and resolution and an ability to inspire 
and motivate others were revealed as much in his 
career as an academic geologist as in his exploits 
as an Antarctic explorer. He was essentially a man 
of action, a trail-blazer, single-minded in the 
pursuit of his goals, at times impatient for results, 
and who could, at times, be protective to the point 
of touchiness, of his own areas of interest. His 
inherited characteristics, hard-headed Yorkshire 
practicality, stubborness and reticence, with a 
streak of romanticism (from his father) were 
blended with a pioneer Australian belief in 
opportunity and self-reliance to produce a complex 
character of contrasting and at times conflicting 
elements. He was a man not easily assessed or 
categorised. Geology is arguably the most 
adventurous of all the field sciences (the first 
scientist to visit the moon was a geologist), and 
Mawson in his life and career, both in the 
Antarctic and in his geological investigations in 
outback South Australia, exemplified both the 
scientific-explorer and explorer-scientist. 

Mawson's scientific career spanned, almost 
exactly, the first half of the twentieth century. 
When he entered the University of Sydney in 1899 
the scientific world-view was of a cooling, 
shrinking earth not more than one hundred million 
years old, the limits having been set by the 



physicists. Geologists, whose investigations had 
by then spread to all parts of the globe, intuitively 
sensed a more ancient earth but lacked the means 
to prove it. Mountain belts were seen as a crustal 
adjustment to a cooling interior and most 
geologists accepted the relative permanence of the 
continents and oceans. 

In retrospect, the years 1900-1950 can be 
viewed as a relatively quiet episode in the 
development of geological science, enlivened by 
two developments early in the century : the 
application of the discovery of radioactivity to the 
dating of rocks, and Wegener's hypothesis of 
continental drift. Each in its own time, the first 
rapidly, the second much more slowly, became a 
vital element in the future Plate Tectonic 
revolution. The recognition that the decay of 
radioactive minerals produced heat freed 
geologists from the shackles of a cooling earth 
and a restricted time-scale by providing a source 
of self-sustaining energy and a means of dating 
the crustal rocks. By 1914, the estimated age of 
the earth had been pushed back to over one 
thousand million years. Mawson's work on 
radioactive minerals in Australia as a young 
student and his later discoveries in South 
Australia gave him a pioneer role in this new 
development and he was always very proud of his 
work in this field (see Mawson 1944b). But in his 
day Australia was effectively too remote from the 
rest of the world for its small and largely 
inaccessible deposits to be economically viable, 
and its universities (certainly Adelaide) too poor 
to engage in expensive age-dating equipment. In 
his later years Mawson was keenly interested in 
these developments overseas and their future 
potential for dating the old rocks in Australia. 

Communication between scientists was severely 
curtailed during the two world wars which 
dominated the first half of the century, although 
technical developments during the second war 
were to help revolutionise geological and 
geophysical exploration both on land and in the 
ocean basins. Mawson's own career was savagely 
disrupted by the First World War and his more 
active years were over before the benefits of post- 
Second World War technical advances became 
widely felt. The inter-war years and those 
immediately after the second war were his most 
productive period for research, more particularly 
from the mid- 1930s when his active involvement 
in Antarctic exploration had ended. Although the 
general outline of South Australian geology was 
well known by this time, no systematic work had 
been attempted and for much of the State 



134 



D. W. CORBETT 



information remained highly generalised and 
lacking in detail. As previously indicated, 
Mawson's early researches were essentially 
exploratory reconnaissances, becoming more 
systematic with his work in the Flinders from the 
1930s. His detailed descriptions of rock units and 
measured cross-sections of key sequences 
provided the basis for the regional mapping 
program to be instigated by the Geological Survey 
in the 1960s. 

Mawson's research was very much an integral 
part of the growth and development of his 
department. His field studies in the Flinders were 
carried out with small groups of advanced 
students as part of their course work, while in the 
Southeast he published in collaboration with post- 
graduate and former students as well as directing 
them in projects of their own. His teaching is 
remembered by past students as being of variable 
quality; he was at his best, according to 
Alderman, when extemporising on subjects that 
particularly interested him. There is no doubt that 
he could inspire his students and a considerable 
number went on to make distinguished careers in 
geology and mineralogy, among them E. A. Rudd, 
L. W. Parkin, R. C. Sprigg, W. B. Dallwitz, D. E. 
Thomas, E. R. Segnit, B. Skinner, R. L. Crocker, 
M. Reynolds, B. Daily, R. Sweatman, A. 
Kleeman, B. Forbes and G. Chinner. 

Mawson, the man of action, always seemed to 
have been fighting a lack of time to complete his 
projects; always planning another field trip and, 
one senses, chafing at the administrative burden 
placed on him as a highly responsible and 
consistently conscientious head of department. 
Never an armchair geologist, Mawson did not 
have the time or the inclination to become 
involved with the theoretical issues of the day, the 
most contentious of which was the idea of 
continental drift. Sir Mark Oliphant, a science 
student at the University in the 1920s, has recalled 
attending a debate on the subject between 
Mawson and Wood-Jones the anatomist, during 
which Mawson scathingly dismissed the concept 
of drift, citing the rigidity of the ocean floors and 
the lack of any known mechanism that could 
power the process. 



Sir Douglas Mawson made an outstanding 
contribution to South Australian geology. His list 
of 102 publications, the majority published in the 
Transactions of the Royal Society of South 
Australia, provide the material evidence of his 
work. He also left a strong department which he 
had established and which was developing rapidly 
in teaching and research. While it is idle to 
speculate, one cannot help but wonder what he 
might have accomplished as a geologist if so 
much of his time and energy had not been devoted 
to the Antarctic. He was not able to settle down to 
an ordered academic life and an on-going research 
program until he reached his fifties. From then on 
his geological output was sustained until the end 
of his career. It was a remarkable achievement. 



Acknowledgments 

The research on which this paper is based was begun 
when the author was a staff member in the Mawson 
Graduate Centre for Environmental Studies at the 
University of Adelaide and completed as an Honorary 
Research Associate at the South Australian Museum. It 
relies heavily on a study of the Mawson Papers housed 
in the Special Collections archive of the Barr Smith 
Library, The University of Adelaide, and Mawson's 
published papers. Research was also carried out on the 
Edgeworth David papers held by the Fisher Library at 
the University of Sydney and in the library of the Scott 
Polar Research Institute, Cambridge. 

For valuable assistance during the course of this work, 
thanks are due to: Susan Woodbum and the staff of 
Special Collections, The University of Adelaide; Mr Ken 
Smith, Archivist, The Fisher Library and Professor 
David Branagan, The University of Sydney; Mr Robert 
Headland, Curator and Archivist, The Scott Polar 
Research Institute, Cambridge. 

For on-going encouragement and support for this 
research and for much helpful discussion on matters 
relating to Mawson, grateful thanks are extended to Mr 
Richard Ferguson, Polar historian; Emeritus Professor E. 
A. Rudd, The University of Adelaide; Dr Victor Gostm 
of the Geology Department, The University of Adelaide 
and Dr Allan Pring, Curator of Minerals, The South 
Australian Museum. Particular thanks are due to Dr 
Robin Oliver of the Geology Department, University of 
Adelaide, for his critical review of the original draft of 
this paper, and his many useful suggestions. 



Selected Bibliography of Douglas Mawson 



(See Alderman (1959) for a Memoir and Bibliography of 
Mawson. Innes and Duff (1990) give a complete list 
of his scientific and other papers together with 
biographical works on Mawson). 



903 (with T. G. TAYLOR). The geology of Mittagong. 
Journal and Proceedings of the Royal Society of New 
South Wales 37: 306-350." 



DOUGLAS MAWSON GEOLOGIST 



135 



1904 (with T. H. LABY). Preliminary observations on 
radioactivity and the occurrence of radium in 
Australian minerals. Journal and Proceedings of the 
Royal Society of New South Wales 38: 382-389. 

1905 The geology of the New Hebrides. Proceedings of 
the Linnean Society of New South Wales 3: 400-485. 

1906 On certain new mineral species associated with 
carnotite in the radioactive orebody near Olary. 
Transactions of the Royal Society' of South Australia 
30: 188-193. 

1912a Geological investigations in the Broken Hill area. 
Memoir of the Royal Society of South Australia 2(4): 
211-319. 

1 9 1 2b PreCambrian areas in the north-eastern portion of 
South Australia and the Barrier, New South Wales. 
Reports of the Australasian Association for the 
Advancement of Science 13: 188-191. 

1915 The Home of the Blizzard. Heinemann, London. 
[Extracts quoted are taken from the abridged popular 
edition (Hodder - Stoughton 1930), published as a 
facsimile edition by the Wakefield Press, 1996.] 

1923 Igneous rocks of the Mount Painter belt. 
Transactions of the Royal Society of South Australia 
47; 37^387. 

1925 Evidence and indications of algal contributions in 
the Cambrian and Pre-Cambrian limestones of South 
Australia. Transactions of the Royal Society of South 
Australia 49: 186-190. 

1926a Wooltana basic igneous belt. Transactions of the 
Royal Society of South Australia 50: 192-200. 

1926b A brief resume of present knowledge relating to 
the igneous rocks of South Australia. Reports of the 
Australasian Association for the Advancement of 
Science 18: 229-274 

1927a The Paralana hot spring. Transactions of the 
Royal Society of South Australia 51: 391-397. 

1927b Geological notes on the area along the north- 
eastern margin of the north-eastern portion of the 
Willouran Range. Transactions of the Royal Society 
of South Australia 51 : 386-390. 

1930 (with C. T. MADIGAN). The pre-Ordovician rocks 
of the McDonnell Ranges, Central Australia. 
Quarterly Journal of the Geological Society of 
LondonS6: 415^28. 



1938 The Mount Carnarvon Series of Proterozoic Age. 
Transactions of the Royal Societ\> of South Australia 
62:347-351. 

1939a The Cambrian sequence in the Wirrealpa Basin. 
Transactions of the Royal Society of South Australia 
63(2): 331-347. 

1 939b The late Proterozoic sediments of South Australia. 
Reports of the Australasian and New Zealand 
Association for the Advancement of Science 24: 80- 
88. 

1942 The structural character of the Flinders Ranges. 
Transactions of the Royal Society of South Australia 
66(2): 262-272. 

1944a Unpublished memorandum on housing the 
department of geology, The University of Adelaide. 
February 1944. 

1944b The nature and occurrence of uraniferous mineral 
deposits in South Australia. Transactions of the Royal 
Society of South Australia 68(2): 334-357. 

1945a (with W. B. DALLWITZ). The soda-rich 
leucogranite cupolas of Umberatana. Transactions 
of the Royal Society of South Australia 69(1): 22- 
49. 

1945b (with W. B. DALLWITZ). Scapolitised dolomites 
of Yankaninna. Transactions of the Royal Society of 
South Australia 69(2): 212-216. 

1947 The Adelaide Series as developed along the 
western margin of the Flinders Ranges. Transactions 
of the Royal Society of South Australia 71(2): 259- 
280. 

1949a The Elatina glaciation: a third recurrence of 
glaciation evidenced in the Adelaide System. 
Transactions of the Royal Society of South Australia 
73: 117-121. 

1949b The late Precambrian ice-age and glacial record 
of the Bibliando Dome. Journal and Proceedings 
of the Royal Society of New South Wales 82: 150- 
174. 

1950 (with R. C. SPRIGG). Subdivision of the Adelaide 
System. Australian Journal of Science 13(3): 69- 
70. 

1958 Australites in the vicinity of Florieton, South 
Australia. Transactions of the Royal Society of South 
Australia HI: 161-163. 



References 



ALDERMAN, A. R. 1959. Professor Sir Douglas 
Mawson Memoir and Bibliography. Transactions of 
the Royal Society of South Australia 82: 1-6. 

ALDERMAN, A. R. 1967. The development of geology 
in South Australia. Records of the Australian 
Academy of Science 1(2): 30 52. 

BICKEL, L. 1977. This Accursed Land. Macmillan 
Australia. 



CORBETT, D. W., COOPER, B. J. & MOONEY, P. M. 
1986. 'Geology' in 'Ideas and Endeavours - the 
Natural Sciences in South Australia'. Royal Society of 
South Australia Occasional Publication Number 5. 

DAVID, T. W. E. (with R. HELMS & E. F. PITTMAN) 
1901. Geological notes on Kosciusko, with special 
reference to evidences of glacial action. Proceedings of 
the Linnean Society of New South Wales 26: 26 74. 



136 



D. W. CORBETT 



DAVID, T. W. E. & PRIESTLEY, R. 1914. Geology 
Vol. 1. Reports, on the Scientific Investigations, the 
British Antarctic Expedition, 1907-08. 

DAVID, T. W. E. 1928. Notes on the newly-discovered 
fossils in the Adelaide Series (Lipalian?), South 
Australia. Transactions of the Royal Society of South 
Australia SI: 191-209. 

DAVID, T. W. E. & TILL YARD, R. J. 1936. Memoir 
on fossils of the late Pre-Cambrian (Newer 
Proterozoic) from the Adelaide Series, South 
Australia. Angus and Robertson, Sydney. 

FERRAR, H. T. 1907. Report on the field geology of the 
region explored during the 'Discovery' Antarctic 
Expedition, 1901-04. National Antarctic Expedition 
1901-04, Natural History, 1, Geology (Field 
Geology: Petrography). British Museum, London. 

GLAESSNER, M. F. & DAILY, B. 1959. The geology 
of the late Precambrian fauna of the Ediacara Fossil 
Reserve. Records of the South Australian Museum 
13(3): 369-401. 

HOWCHIN, W. 1897. On the occurrence of Lower 
Cambrian fossils in the Mount Lofty Ranges. 
Transactions of the Royal Society of South Australia 
20(2): 74-86. 

HOWCHIN, W. 1901. Preliminary note on the existence 
of glacial beds of Cambrian age in South Australia. 
Transactions of the Royal Society of South Australia 
25: 10-13. 

HOWCHIN, W. 1914. The occurrence of the Genus 
Cryptozoon in the ? Cambrian of Australia. 



Transactions of the Royal Society of South Australia 
38: 1-10. 

HOWCHIN, W. 1922. A geological traverse of the 
Flinders Range from the Parachilna Gorge to the Lake 
Frome Plains. Transactions of the Royal Society of 
South Australia 46: 46-82. 

INNES, M. & DUFF, H. 1990. 'Mawson's Papers 1 . The 
Mawson Institute for Antarctic Research, The 
University of Adelaide. 

JACKA, F. 1986. Mawson, Sir Douglas(1882-1958). 

Australian Dictionary of Biography 10: 454-457. 
MAWSON, P. 1962. 'Mawson of the Antarctic'. 

Longmans, London. 
PARER, P. & PARER-COOK, E. 1983. 'Douglas 

Mawson the Explorer'. Alella Books ABC. 

SEGNIT, R. W. 1939. 'The Pre-Cambrian Cambrian 
Succession'. Bulletin of the Geological Survey of 
South Australia 18. 

SHACKLETON, E. 1911. 'The Heart of the Antarctic'. 
Heinemann, London. 

SPRIGG, R. C. 1947. Early Cambrian (?) jellyfishes 
from the Flinders Ranges, South Australia. 
Transactions of the Royal Society of South Australia 
72(2): 212-224. 

SPRIGG, R. C. 1949. Early Cambrian 'Jellyfishes' of 
Ediacara, South Australia. Transactions of the Royal 
Society of South Australia 73: 72-99. 

SPRIGG, R. C. 1986. The Adelaide Geosyncline: a 
century of controversy. Earth Sciences History 5(1): 
66-83. 



REVISION OF AUSTRALIAN ENOCHRUS THOMSON 
(COLEOPTERA: HYDROPHILIDAE) 



C.H.S. WATTS 



Summary 



The Australian members of the hydrophilid genus Enochrus are revised and redescribed. A key to 
the fourteen species recognised is given. Six species are described as new: E. aliciae, E. 
eubenangeei, E. isabellae, E. pseudoweiri, E. samae, and E. weiri. The following synonymies are 
proposed: E. mjobergi Knisch, 1921 - E. deserticola (Blackburn, 1896); E. andersoni (Blackburn, 
1896) = E. eyrensis (Blackburn, 1894); E. persimilis Regimbart, 1908 = E. eyrensis (Blackburn, 
1894); E. pullus (Fauvel, 1883) = E. esuriens (Walker, 1858) and E. artensis (Fauvel, 1883) = E. 
maculiceps (MacLeay, 1873). The New Caledonian species E. caledonicus (Fauvel, 1883) is 
considered a synonym of E. elongatus (MacLeay, 1873). 



REVISION OF AUSTRALIAN ENOCHRUS THOMSON 
(COLEOPTERA: HYDROPHILIDAE) 



C. H. S. WATTS 



WATTS, C. H. S. 1998. Revision of Australian Enochrus Thomson (Coleoptera; 
Hydrophilidae). Records of the South Australian Museum 30(2): 137-156. 

The Australian members of the hydrophilid genus Enochrus are revised and redescribed. A 
key to the fourteen species recognised is given. Six species are described as new: E. aliciae, E. 
eubenangeei, E. isabellae, E. pseudoweiri, E. samae, and E. weiri. The following synonymies 
are proposed: E. mjobergi Knisch, 1921 - E. deserticola (Blackburn, 1896); E. andersoni 
(Blackburn, 1896) - E. eyrensis (Blackburn, 1894); E. persimilis Regimbart, 1908 * E. 
eyrensis (Blackburn, 1894); E. pullus (Fauvel, 1883) = E. esuriens (Walker, 1858) and E. 
artensis (Fauvel, 1883) = E. maculiceps (MacLeay, 1873). The New Caledonian species E. 
caledonicus (Fauvel, 1883) is considered a synonym of E. elongatus (MacLeay, 1873). 

C. H. S. Watts, South Australian Museum, North Terrace, Adelaide, South Australia 5000. 
Manuscript received 19 March 1997. 



The hydrophilid genus Enochrus Thomson, 
1859 is world wide in distribution (Hansen 1991). 
In Australia its members are the commonest and 
most widespread hydrophilids and occur in 
virtually all fresh water bodies from small 
stagnant pools to the banks of major rivers and 
lakes. Despite this prominence, their taxonomy is 
so bad that no species can be identified with any 
confidence. Thirteen species have been named and 
several others have been recorded as being present 
but until now no revision has been attempted. 

Australian Enochrus are structurally very 
similar and difficult to separate. Apart from the 
aedeagi the only characters that I have found 
useful are size, the punctation of the upper surface, 
the slope of the mesosternal keel, and the colour 
pattern of the head. The colour pattern of the head 
is often a reasonable indicator of species, whereas 
elytral and pronotal colour can vary from 
predominantly black to totally light reddish in the 
same species. 

Within Enochrus six subgenera are recognised 
(Hansen 1990). Three of these occur in Australia: 
Hydatotrephis MacLeay, 1873 with one species; 
Enochrus Thomson, 1859 with one species; and 
Methydrus Rey, 1885 with 12 species. 

At first sight E. (H.) mastersi is very similar to 
the distantly related Limnoxenus zealandicus 
Broun and is often confused with it in collections. 
Both are moderate sized (10-15 mm), shiny black 
and relatively common, particularly L. 
zealandicus. A closer inspection readily separates 
them: L. zealandicus has well defined punctate 
elytral striae and swimming hairs on the meso- 



and meta-tibiae, both of which are absent in E, 
(H.) mastersi. Characters of the maxillary palpi 
and mesosternum also separate the two genera 
(Hansen 1990). 

The one Australian Enochrus (Enochrus) 
species, E. (E.) peregrinus Knisch, 1922, is small 
and in general appearance resembles several 
Australian Enochrus (Methydrus) species. It is 
known from only one specimen labelled from 
Sydney, although there were three in the original 
collection. It may eventually prove to have been 
mis-labelled and not Australian. 

The remaining 12 Australian species are all in 
the subgenus Methydrus. They are usually small 
(2 8 mm), oval, rather flat species, shiny with 
light-testaceous to black colouring with at least 
the area immediately in front of the eyes 
yellowish. Two species are larger and 
predominantly black, superficially resembling E. 
(H.) mastersi. Chasmogenus nitescens Fauvel 
resembles some Enochrus (Methydrus) species 
and is often confused with it in collections. Its 
small size (< 5 mm) and lack of yellowish areas 
in front of its eyes readily separate it from similar 
sized Enochrus - as well as many structural 
characters mentioned later under 'Systematics'. 

One additional species, Philhydrus marmoratus 
W. MacLeay, 1873, has been included in 
Enochrus in the past but has been shown by 
Gentili, 1981 to belong in Laccobius. 

For a full discussion of synonyms and 
subgenera of Enochrus see Hansen, 1991. 

Despite their being ubiquitous in freshwater the 
biology of Australian Enochrus is poorly known. 



38 



C. H. S. WATTS 



Anderson (1976) described the larvae of E. (M.) 
maculiceps and E. (M.) elongatus and gave brief 
notes on their habitat and breeding. All species 
come readily to light and are often collected in 
large numbers in light traps, particularly in 
northern areas during the wet season from 
December to February. I know of no study of the 
ecology of any Australian species other than 
inclusion in general faunal lists of invertebrates 
collected in various water bodies. 

The collections from which specimens were 
examined are listed under the following 
abbreviations: 

AM Australian Museum, Sydney 

AN1C Australian National Insect Collection 

BM(NH) Natural History Museum, London 

IRSNB Institut Royal des Sciences Naturelles 
de Belgique, Bruxelles 

MNHN Museum National d'Histoire Naturelle, 
Paris 

NMV Museum of Victoria 

NRS Naturhistoriska Riksmuseet, Stockholm 

NTM Northern Territory Museum 

QDPIM Queensland Department of Primary 
Industries, Mareeba 

QM Queensland Museum, Brisbane 

SAMA South Australian Museum, Adelaide 

UQIC University of Queensland Insect 
Collection, Brisbane 

WAM Western Australian Museum, Perth. 



Systematics 

Australian members of the genus Enochrus can 
be separated from other Australian Hydrophilids 
by the following combination of characters. 
Length 2-9 mm, oval, more flattened than convex; 
second segment of maxillary palpi more or less 
curved outwards, apical segment slightly 
asymmetrical with straighter inner face; without 
contiguous ventral keel but with variable keel on 
mesosternum; without swimming hairs on tibiae; 
without strongly marked striae on elytron; with 
systematic punctures (rows or fields of coarse 
setiferous punctures usually distinctly larger than 
others) on head and pronotum (masked in some E. 
malabarensis); in all but E. mastersi and E. 
aliciae at least the area immediately in front of 
eyes lighter (see also Hansen 1991). 

The subgenus Hydatotrephis MacLeay can be 



separated from Australian members of the 
subgenera Enochrus Thomson and Methydrus 
Rey as follows: mesosternal protuberance 
triangular, cone-shaped, abruptly truncated 
posteriorly which does not reach the front edge of 
mesocoxae (Fig. 19), sides of mesosternum evenly 
converging anteriorly, apical and penultimate 
segments of maxillary palpi subequal. Enochrus 
(Methydrus) have a more keel-like mesosternal 
process usually extending backwards between the 
mesocoxae (Figs 15-18; 20), the apical segment 
of the maxillary palpi shorter than penultimate and 
sides of mesosternum subparallel to strongly 
convex anteriorly. Apart from E. (M.) aliciae and 
E. (M.) eubenangeei, the Australian members of 
E. (Methydrus) are smaller (< 8 mm), often 
testaceous in colour, and have at least a lighter 
patch of colour in front of the eyes. 

The aedeagus of E. (H.) mastersi differs from 
that of other Australian Enochrus (Fig. 14; 
Hansen 1990). In these there is a variably shaped 
basal ventral plate beyond which projects a 
thinner apical portion in all but E. (M.) aliciae 
which lacks this apical portion (Fig. 11). In E. 
(H.) mastersi the aedeagus is of more uniform 
construction with a smooth dorsal surface and the 
ventral surface consists of a broad open groove 
formed by infolding of the two sides. 

There is one species, E. (E.) peregrinus Knisch, 
of the subgenus Enochrus in Australia. It is 
similar in looks to the smaller Methydrus species 
but is readily separated from them by the short 
stout maxillary palpi with approximately equal 
sized apical two segments and the diverging 
elytral suture lines. 

By utilising the male genitalia species can be 
differentiated. However without these I have found 
it impossible to reliably separate all species, in 
particular E. weiri and E. pseudoweiri and the 
lighter colour phase of E. deserticola and E. 
maculipes. This is reflected in the keys and 
descriptions that follow. 1 have restricted my 
descriptions to the few characters that serve to 
differentiate the species and I have provided two 
keys, one utilising all available characters, the 
other characters other than the male genitalia. 

Key to Australian Enochrus Thomson 1859, 
not using characters of the male genitalia 

1 . — Maxillary palpi stout, first segment shorter than 
distance from front edge of eye to front of 
clypeus, apical segment subequal in length to 

penultimate 2 

Maxillary palpi more elongate, first segment 



AUSTRALIAN ENOCHRUS 



139 



longer than distance from front edge of eye to 
front margin of clypeus, apical segment about 
2/3 length of penultimate (subgenus 
Methydrus) 3 

2. — > 6.0 mm. Black. Sutural lines on elytra 

subparallel in anterior quarter , 

E. {Hydatotrephis) mastersi (MacLeay) 

— < 5.0 mm. Dark testaceous. Sutural lines on 
elytra diverging noticeably in anterior quarter .. 

E. (Enochrus) peregrinus Knisch 

3. — Large (>6 mm). Black (pronotum may be 

reddish at edges) 4 

Small (< 6 mm). With at least the areas in front 
of eyes reddish-yellow 5 

4. - Punctures towards sides of elytra well 

impressed, not much smaller than others 

E. (M.) euhenangeei sp. nov. 

— Punctures towards sides of elytra subobsolete, 
much smaller than those on disc 

E. (M.) aliciae sp. nov. 

5. — Dorsal surface reddish-yellow, rear of head at 

most somewhat darker. Elytra moderately 
punctate, length > 4.0 mm, pro-, meso- and 

metaclaws modified in male 

E. (M.) elongatus (W . MacLeay) 

- Dorsal surface reddish-yellow to black, rear of 
head dark and much of rest of head in many 
species, males with only pro-claws modified 6 

6. — Dorsal surface strongly punctured, punctures on 

elytra as strong or stronger than those on head, 
many punctures on elytra >half diameter of 
serial punctures which are often hard to trace. 
Front of head 1/3 or more black 7 

— Dorsal surface weakly punctured, punctures on 
elytra tend to be weaker than those on head, 
punctures on elytra < half size of serial 
punctures which are usually distinct 9 

1, — Length >3.5 mm. Black morphs present. 
Maxillary palpi with dark tips 8 

Length < 4.0 mm. Black morphs not known. 

Maxillary palpi usually pale throughout 

E. (E.) malabarensis Regimbart 

8. — Thinner outer portion of mesosternal keel well 

developed (Fig. 16). Front of head 

predominantly black 

E. (M.) eyrensis (Blackburn) 

— Thinner outer portion of mesosternal keel less 
developed (Fig. 15). Amount of black on front 
of head variable E. (M.) samae sp. nov. 

9. — Length 2.2 mm - 2.6 mm. Mesosternal keel 

weakly developed (Fig. 1 8). Front of head > 2/3 
black E. (M.) esuriens (Walker) 

— Length > 2.6 mm. Mesosternal keel well 
developed (Fig. 17) 10 



10. — Larger (4.5-6 mm). Black, except region in 
front of eyes light. Elytral punctures small but 

usually well marked 

E. (M.) isabellae sp. nov. 

— Smaller (3-4.5 mm) E. (M.) deserticola complex 
(£. (M.) deserticola (Blackburn), E. (M.) 
maculiceps (W. MacLeay), E. (M.) weiri sp. nov 
and E. (M.) pseudoweiri sp. nov). (E. (M.) 
deserticola only species with black morphs and 
individuals > 4.2 mm long. Enochrus weiri and 
E. pseudoweiri always have pale palpi.) 



Key to Australian Enochrus incorporating 
characters of the male glnitalia 

— Maxillary palpi stout, pseudo first segment 
shorter than distance from front edge of eye to 
front of clypeus, apical and penultimate 
segments subequal in length 2 

— Maxillary palpi more elongate, pseudo first 
segment longer than distance from front edge of 
eye to front margin of clypeus, apical segment 
noticeably shorter than penultimate (subgenus 
Methydrus) 3 

— > 6.0 mm. Black. Sutural lines on elytra 
subparallel in anterior quarter 

E. (Hydatotrephis) mastersi (MacLeay) 

< 5.0 mm. Dark testaceous. Sutural lines on 
elytra noticeably diverging in anterior quarter .. 
E. (Enochrus) peregrinus Knisch 

— Large (> 6.0 mm). Black (pronotum may be 
reddish at edges) 4 

— Small (< 6.0 mm). With at least the areas in 
front of eyes reddish-yellow 5 

— Aedeagus broad reaching little beyond half 
length of parameres (Fig. 1 1). Parameres flat. .. 

E. (M.) aliciae sp. nov. 

Aedeagus with broad basal piece and long thin 
apical piece bending upwards and reaching 
nearly to end of parameres, which also bend 

upwards (Fig. 10) 

E. (M.) euhenangeei sp. nov. 

— Tips of parameres hooked (e.g. Fig. 4) 6 

— Tips of parameres not hooked (e.g. Fig. 1) 9 

— Dorsal surface reddish-yellow, rear of head at 
most somewhat darker. Aedeagus tip strongly 
crotchet-shaped (Fig. 7). Pro-, meso- and 
metaclaws modified in male 

E. (M.) elongatus (W. MacLeay) 

Variably coloured but always with rear of head 
clearly darker than at least portions of front of 
head. Aedeagus with little or no dorsal/ventral 
expansion at tip, males with only proclaws 
modified 7 



140 



C. H. S. WATTS 



7. — Dorsal surface strongly punctured, many 

punctures on elytra > half size of serial 
punctures E. (M.) eyrensis (Blackburn) 

— Dorsal surface weakly punctured, punctures on 
elytra < half size of serial punctures 8 

8. — Larger (4.5 - 6.0 mm). Black, except in front of 

eyes. Aedeagus shorter and apical portion 
broader (Fig. 6) E. (M.) isabellae sp, nov. 

— Smaller (3.0-4.0 mm). Pale morphs common. 
Aedeagus longer and apical portion thinner 
(Fig. 4) E. (M.) deserticola (Blackburn) 

9. — Length <2.8 mm. Front of head > 2/3 black. 

Mesosternal keel weak (Fig. 18) 

E. (M.) esuriens (Walker) 

— Not as above 10 

1 0. — Dorsal surface strongly punctured, punctures on 

elytra as strong as, or stronger than, those on 
head, many punctures on elytra > half diameter 
of serial punctures 1 1 

— Dorsal surface weakly punctured, punctures on 
elytra tend to be weaker than those on head, 
punctures on elytra < half size of serial 
punctures 12 

11. — Larger (4.4-5.6 mm). Black morphs present. 

Aedeagus with moderate apical pad, inner edges 

of parameres sinuate (Fig. 9) 

E. (M.) samae sp. nov. 

— Smaller (<3.8 mm). No black morphs. 
Aedeagus narrow with, at most, a weak pad, 
inner edges of parameres straight (Fig. 12) 

E. (M.) malabarensis Regimbart 

12. — Tips of parameres truncated or weakly bifid 

(Fig. 8) E. (M.) weir i sp. nov. 

— Tips of parameres rounded (Figs I, 2, 3) 13 

13. — Aedeagus moderately broad with slight to well- 

marked apical pad (Figs 1, 2) 

E. (M.) maculiceps (W. MacLeay) 

— Aedeagus narrow, sharply pointed, lacking 
apical pad (Fig. 3) 

E. (M.) pseudoweiri sp. nov. 



Descriptions 

Subgenus Enochrus 

Enochrus (Enochrus) peregrinus Knisch, 1922 

Types 

Lectotype: 9 'Sidney Mus. Godeffroy No. 
10705, coll. Knisch, coll. d'Orchymont'; 'ex. col. 
Knisch, No. 5251438, coll. d'Orchymont'; 



'Knisch det. 1921, Enochrus peregrinus m'; 
'Coll. A. Knisch, TYPUS', on red card, in 
IRSNB, herein designated. 

Knisch (1922) mentioned three specimens (No. 
10705) in the Hamburg Zoological Museum. I 
have been able to trace only one. He mentioned 
that one was labelled 'M. Regimbart det. 1905' 
and the others with 'Wehncke determ'. The 
surviving specimen, now in Brussels, lacks such a 
label but would otherwise appear to be part of the 
syntype series. 

Description (number examined, 1) 

Length 3.2 mm. Broadly oval. Elytra dark- 
testaceous, pronotum very slightly lighter, head 
black except for small indistinct testaceous patch 
along margin in front of each eye, maxillary palpi 
light-testaceous, tips darker. Punctures on head 
moderate, approaching size of eye facet, most 
separated from each other by at least puncture 
width. Systematic punctures rather sparse, about 
twice diameter of adjacent punctures. Pronotum 
rather weakly and sparsely punctured, serial 
punctures also relatively small, indistinct, about 
2x diameter of adjacent punctures, punctures on 
elytra stronger than on pronotum, sparse, many 2x 
diameter or more apart, a little stronger laterally. 
Serial punctures not traceable. Maxillary palpi 
short, stout, pseudo basal segment not reaching 
front edge of eye, apical and penultimate segment 
subequal in size. 

Male: Unknown. 

Distribution 

Known only from Sydney, the type locality, 

Remarks 

This unique specimen is separated from all other 
Australian Enochrus, other than the much larger E. 
mastersi, by the short stout maxillary palpi. The 
masking of the elytral strial punctures is found only 
in the much larger E, eyrensis and E. samae and in 
E. malabarensis. Enochrus malabarensis differs 
from E. peregrinus by the more normal (for 
Australian species) maxillary palpi, the more 
extensive testaceous areas in front of the eyes and 
lighter coloured elytra. The elytral sutures continue 
to diverge noticeably in anterior quarter whereas in 
E. malabarensis they are subparallel. Most E. 
malabarensis also have stronger punctures, but this 
character is variable and tends to be relatively weak 
in the few Sydney area specimens I have seen. The 
pronotal punctures in E. peregrinus are weaker 
than those on elytra whereas in E. malabarensis 
they are similar sized. 



AUSTRALIAN ENOCHRUS 



141 



The fact that only the type specimen is known 
worries me. For all the other small Australian 
Enochrus, specimens are relatively abundant. 
Also it is the only known specimen in the 
Australian region of the subgenus Enochrus 
(Hansen 1990). This is the sort of situation where 
mislabelling should be considered. This is beyond 
the scope of this revision. 



Subgenus Hydatotrephis 

Enochrus (Hydatotrephis) mastersi (MacLeay) 

Hydatotrephis mastersi MacLeay, 1871 

= Parana simplex Knisch, 1922: Hansen, 1990 

Enochrus (Hydatotrephis) mastersi (MacLeay): 
Hansen, 1990 

Types 

Hydatotrephis mastersi: Lectotype: ( 9- ), (round 
red label), 'K 1950T, "Hydatotrephis mastersi 
Mc L.W. Gayndah'. 'Lectotype: Hydatotrephis 
mastersi W. J. MacLeay designated by M. Hansen 
1990', AM. 

Parana simplex: Lectotype: (unsexed) 'Sidney 
Mus. Godeffroy. No. 10704'; 'Philhydrus x M. 
Regimbart determ. 1905'; 'Parana simplex 
Knisch n.g. et sp. A. Knisch det. 1921', round 
black label; 'Lectotype Parana simplex Knisch 
designated by M. Hansen 1988', IRSNB. 
Synonymy after Hansen 1990. 

Description (number examined, 71) Figs 14, 19 

Size 8.0 mm - 9.1 mm. Broadly oval. Relatively 
flat. Black; lateral edges of elytra, pronotum and 
head, palpi and apical portions of legs diffusely 
dark-testaceous. Maxillary palpi stout, length 
about width of head in front of eyes, apical and 
penultimate segments subcqual in length, together 
a tittle larger than pseudo first segment. Head 
strongly punctured, each about size of eye facet, 
most closer than a puncture width apart, 
systematic punctures 2-3x size of normal 
punctures. Pronotum with punctures a little 
smaller, shallower and more separated than on 
head, systematic punctures well marked, with 
sharp groove sometimes weak or lacking on front 
edge. Elytra punctured as on pronotum, each 
elytron with four rows of larger serial punctures, 
punctures in rows increasing in both number and 
scatter towards sides, elytra weakly grooved and 
flanged laterally, a few scattered large punctures 
between puncture rows two and three counting 
from suture. Mesosternal keel cone-like, strongly 



raised, narrowly triangular from both lateral and 
front views, sharply truncated behind just prior to 
mesocoxal cavities so that no part of the keel 
extends between mesocoxae. 

Male: Aedcagus broad, lacking collar or ventral 
plate, sides folded in ventrally tending to form 
broad channel. Parameres stout, broad, narrowing 
shortly before tips which tend to be turned inward 
to varying degrees. 

Distribution 

Australian Capital Territory 

Black Mt, ANIC; Canberra, SAMA, ANIC; 3 
km E Piccadilly Circus, ANIC; 6 km NE 
Piccadilly Circus, ANIC. 

New South Wales 

Allyn River, ANIC; Barrington River, ANIC; 
Blue Mts, ANIC Chichester St Forrest, ANIC; 
Coffs Harbour UQIC; Como, ANIC; Galston, 
SAMA; Lansdowne via Taree, ANIC; 
Muswellbrook, ANIC; Nerringa, SAMA; 12 km 
NW Nellinger, ANIC; 2km NE by N Rousmill, 
ANIC; Salisbury UQIC; Stanwell Park UQIC; 
Sydney, SAMA, ANIC; Tooloom Plateau via 
Woodenbong UQIC; Ulladulla, ANIC; Valery, 
ANIC; Wee Jasper, ANIC. 

Northern Territory 

30 ml W Alice Springs, SAMA; Stanley 
Chasm, SAMA. 

Queensland 

Brisbane UQIC; Bulburin State Forest via 
Many Peaks UQIC; Bunya Mt, ANIC; Carnarvon 
UQIC; Discot, ANIC; 13 km SW by S 
Gordonvale, ANIC; Joalah Nt Pk Tamborine Mt, 
ANIC; Mt Norman, via Wallangarra UQIC; Mt 
Spec, ANIC; Upper Cedar Ck, via Sandford 
UQIC; 8 km E Wallaman Falls, SAMA. 

Victoria 

Bagots Ck, SAMA; Ferntree Gully UQIC; 
Healesville, SAMA; 10 mis N of Valencia Creek 
via Maffra UQIC; Victorian Alps, SAMA. 

Remarks 

A widespread and relatively common species 
which, within Australian Enochrus, can only be 
confused with E. aliciae and E. eubenangeei. It is 
readily separated from these species by the stout 
maxillary palpi which have the last two segments 
subequal instead of having the apical segment 
about two-thirds the length of the penultimate as 



142 



C. H. S. WATTS 



in all other Australian Enochrus. The cone-like 
shape of the mesosternal keel is also diagnostic. 

Enochrus mastersi is most frequently confused 
with a very different, but similar looking and very 
common species, Limnoxenus zealandicus, of the 
subtribe Hydrobiina. Although very similar in 
general appearance Limnoxenus can be separated 
from E. mastersi by the presence of nine well- 
marked series of punctures on each elytron, 
swimming hairs on the meso- and metatarsi and 
virtual absence of rugose portions on meso- and 
metafemora. 



Subgenus Methydrus 

Enochrus (Methydrus) aliciae sp. nov. 

Types 

Holotype: o\ '15°16*S, 144°59'E, 14 km W by 
N of Hope Vaie Mission, Qld, 8-10 Oct. 1980, T. 
Weir', ANIC. 

Paratypes: 13, same data as holotype, 10 
ANIC, 3 SAMA; 1, '12*31% 132°54'E, 9 km N 
by E of Mudginbarry Hs„ N.T., 10.vi.1973, T. 
Weir and A. Allwood, M3985", NTM. 

Description (number examined, 17) Figs 11, 20 

Length 7.5 mm - 8.2 mm. Broadly oval, 
relatively flat. Shiny, black, appendages, apical 
and lateral edges of head, pronotum and elytra 
dark-reddish. Maxillary palpi moderately long, 
pseudo first segment longer than distance from 
eye to front of clypeus, longer than maxillary stipe, 
apical segment 2 I to 3 / 4 length of penultimate. 
Head strongly punctate, punctures about puncture 
width apart, about size of eye facet or a little 
smaller. Systematic punctures large about 3x size 
of adjacent punctures. Punctures on pronotum 
similar to or a little weaker than those on head, 
systematic punctures well marked, 3~4x diameter 
of adjacent punctures, rear and lateral margins 
weakly grooved and flanged, front margin grooved 
to about level of inner edge of eyes. Elytral 
punctures as on pronotum, more weakly 
impressed towards rear. Serial punctures in four 
loose rows, sparse and indistinct, more numerous 
but more scattered laterally, elytra weakly grooved 
and flanged laterally. Mesosternal pillar well 
marked, triangular in both front and lateral views, 
posterior edge often steeper near top of keel, 
reaching a short distance between mesocoxae. 

Male: Aedeagus very short, broad, rounded, 
lacking narrower apical section. Parameres squat, 
inner edge a little sinuate, tips obliquely truncated 



on inside or curved weakly outwards. Proclaw 
straightened with strong basal swelling, mesoclaw 
thickened, curved with basal swelling, metaclaw 
straightened and greatly swollen in basal half. In 
female claws similar but with straightening and 
basal swelling much weaker. 

Distribution 

Known only from the type localities in North 
Queensland and the Northern Territory. 

Remarks 

Readily separated from all other Australian 
Enochrus (Methydrus), other than E. 
eubenangeei, by its large size and almost all-black 
colouring. The very short, broad aedeagus, and 
weak lateral punctures on the elytra separate it 
from the otherwise very similar E. eubenangeei. 

In general appearance it is similar to E. (H.) 
mastersi but readily separated by its longer 
maxillary palpi with the apical segment shorter 
than penultimate. See also under remarks in E. 
mastersi. 



Enochrus (Methydrus) deserticola (Blackburn) 

Philhydrus deserticola Blackburn, 1896 

Enochrus (Lumetus) deserticola (Blackburn): 
Knischl924 

—Enochrus mjobergi Knisch, 1921: syn. nov. 

—Enochrus (Lumetus) mjobergi Knisch: Knisch 
1924 

^Philhydrus temporalis Regimbart, 1908: syn. 
nov. 

^Enochrus (Lumetus) temporalis (Regimbart): 
Knisch 1924 

Types 

Enochrus deserticola: Lectotype: '5487, Bl. 
Paisley T' top specimen of two separately carded 
on same pin, BM(NH), herein designated. 

Paralectotypes: 1 unlabelled but mounted 
below lectotype on same pin, BM(NH); 1 6 '5487 
Palm Cr', ' Philhydrus deserticola Blackb. Co- 
type', SAMA; 3, 'Reedy Hole', NMV; 2, 'Ellery 
Ck\ NMV; 2, 'Paisley Bluff, NMV. 

Enochrus mjobergi: Lectotype: 6 'Cape York 
Penins'; 'Queensl. Mjoberg'; 'Type', ''Enochrus 
(Lum.) mjobergi m. n. sp., A. Knisch 1921 '; 
'Typus', on red label NRS, herein designated. 

Paralectotypes: 1, 'Queensl. Mjoberg Cape 
York Penins'; 'Sjostedt don 1921'; 'Ex Coll. 
Knisch No. 5521544 Coll. d'Orchym'; 'Knis det 



AUSTRALIAN ENOCHRUS 



43 



Enochrus (L.) mjobergi m'; Coll. A. Knisch 
TYPUS', on red card. IRSNB; 3, 'Cape York 
Penins'; 'Queensl. Mjoberg', NRS. Synonymy 
after examination of types. 

Enochrus temporalis: Holotype: 'Avon R'; 
'eaudouce'; ' Philhydrus temporalis, Reg. 
TYPUS % MNHN. Synonymy based on 
descriptions and examination of types (of E. 
temporalis in 1964, not currently available). 

Description (number examined, >1000) Fig. 4 

Oblong oval, length 3.3 mm - 4.9 mm. Two 
colour morphs; one with dorsal surface black 
except light portions in front of eyes, other with 
elytra and pronotum light testaceous and head 
dark testaceous to black except for light testaceous 
area forward from eyes and a little wider than 
eyes, leaving central darker panel of variable 
width on front of head, underside dark testaceous, 
appendages lighter towards extremities except for 
maxillary palpi which usually have apical portion 
of last segment darker. Head covered with small, 
sharply impressed, well separated punctures a lot 
smaller than eye facets, a group of large punctures 
inwards from each eye, at least 4x diameter of 
other punctures. Punctures on pronotum as on 
head, but more shallowly impressed, systematic 
punctures as in E. elongatus, four or more times 
diameter of adjacent punctures. Elytral punctures 
increase somewhat in strength apically and 
laterally, serial punctures large, sparse and quite 
distinct at apex, interstrial punctures varying from 
weak to almost obsolete. 

Mesosternal keel well developed, front edge 
nearly perpendicular, ventral edge straight or 
slightly convex. 

Male: Aedeagus pointed, with weak dorsal pad 
at tip, collar a bit closer to tip than base. 
Parameres outwardly hooked at tips. Proclaw with 
basal lobe and rest of claw somewhat 
straightened. Meso- and mctaclaws, with slight 
basal lobes, weakly curved. 

Female: Claws only slightly weaker than males. 

Distribution 

New South Wales 

Bonville, ANIC; Chichester SF, ANIC 
Clarence River, NMV; Coffs Harbour, ANIC 
Fowlers Gap, ANIC; 10 km N Jabrru, QDPIM 
Lord Howe Island, SAMA; Moree, SAMA 
Valcry, ANIC; Wootton, ANIC. 

Northern Territory 

Adelaide River, ANIC; E Alligator River, AM; 
Bessie Spring, ANIC; Berry Spring, ANIC; 45 



km SW by S Borroloola, ANIC; 7 km NW by N 
Mt Cahill Crossing East Alligator River, ANIC; 8 
km N Mt Cahill, SAMA; 12 km NNW Mt Cahill, 
SAMA; 14 km S by W Cape Crawford, ANIC; 
Cooper Creek, ANIC; Daly River Mission, ANIC; 
170 km E Daly Waters, SAMA; Darwin, ANIC, 
SAMA; Ellery Ck, NMV; 15 km S Elliot, SAMA; 
Harst Bluff, NMV; 12 km NE Humpty Doo, 
QDPIM; Jim Jim Creek, ANIC; Koogarra, ANIC; 
4 km N McArthur R Stn, SAMA; 19 km SSE 
Mataranka, SAMA; 5 km E Mataranka, SAMA; 
Nourlangie Creek, ANIC; 18 km E by N Oenpelli, 
ANIC; Paisley Bluff, NMV; Pine Creek, QDPIM; 
Reedy Hole, NMV; 46 km S Renner Springs, 
SAMA; Stanley Chasm, SAMA, ANIC; 100 km 
W Tennant Creek, QDPIM; Tindal, ANIC; 
Wessel Island, ANIC. 

Queensland 

Ashmore, QM; Atherton, ANIC, QDPIM; 31 
km NE Aramac, SAMA; Bakerville, QDPIM; 
Bamaga, SAMA; Brisbane, QM, UQIC; 
Benaraby, ANIC; 5 mis N Bloomfield River, 
ANIC; Bundaberg, ANIC; Bunya Mts, ANIC; 
Burketown, QM; Cairns, ANIC, SAMA; Calliope 
River, ANIC; Camooweal, QDPIM; Cape 
Tribulation, ANIC; Cardstone, ANIC; Chillagoe 
Creek, ANIC, QDPIM; Coen, QDPIM; 60 km S 
Coen, SAMA; Mt Coolum, ANIC; Cooktown, 
ANIC; 30 mis N Cooktown, UQIC; Crystal 
Creek, ANIC; Cunningham's Gap, ANIC; 
Dalhunty River, SAMA; Edungalba, ANIC; 5 km 
NE Edungalba, SAMA; Eidsvold, ANIC; Emu 
Park, UQIC; Fletcher, QM; Gayndah, UQIC; Mt 
Garnet, ANIC; Greenhills, ANIC; Home Hill, 
QDPIM; Ingham, ANIC, SAMA; Mt Inkerman, 
ANIC; Iron Rng, QDPIM; Julatten, ANIC; Julia 
Creek, SAMA; Kenilworth SF, UQIC; Kingaroy, 
ANIC; Kuranda, ANIC, SAMA; Laura, QDPIM; 
70 km N Laura, QDPIM; 25 km N Laura, 
QDPIM; Mt Lewis, ANIC; Mackay, ANIC; 
Magnetic Isl, SAMA; Malanda, SAMA; 23 km E 
Marecba, QDPIM; Mary Creek, ANIC; Melvor, 
ANIC; 21 mis S Miriam Vale, ANIC; 100 mis S 
Miriam Vale, UQIC; Mission Beach, ANIC; 3 
mis W Mourilyan, ANIC; Mornington Isl 
mission, SAMA; 5 km W Mossman, QM; 
Mossman George Nt Pk., UQIC; Mossman 
George, ANIC; Normanton, QDPIM; Oxley Ck, 
QM; Patuma Dam, ANIC; 9 km W Paluma, 
QDPIM; Prince of Wales Isl, NMV; 8 mis NE 
Proserpine, ANIC; Rocklea, QM; Stanthorpe, 
QM; Mt Spec, ANIC; Stewart Rng, SAMA; 
Tolga, SAMA; Townsville, ANIC, NMV, SAMA; 
9 km ENE Mt Tozer, ANIC; Weipa, QDPIM; 



144 



C. H. S. WATTS 



Windsor Tableland, QDP1M; Yamba, UQIC; 
Yungaburra, QDPIM. 

South Australia 

Arkaba Creek, SAMA; Mambray Creek, 
SAMA; Marne River., SAMA; Mt Remarkable, 
SAMA; 6 km E Nilpinna, SAMA. 

Victoria 

Dimboola, ANIC; Genoa, ANIC; Sea Lake, 

SAMA. 



have, however, been unable to reliably separate 
light coloured females. In general E. deserticola 
are larger and more weakly punctured but 
considerable character overlap occurs between the 
two species. 

In more southern areas E. deserticola overlaps 
with E. eyrensis, E. samae and E. elongatus but 
can be separated from all three by the much 
weaker punctation and in the case of E. elongatus 
by the well-marked dark patterning on the head 
which E. elongatus lacks. 



Western Australia 

6 km NNW Broome, ANIC; Beverley Springs, 
WAM; Cadjeput Rockhole, WAM; Charnley 
River, 25 miles N Beverley Springs, WAM; 
Derby, SAMA; Drysdale River, ANIC; 7 miles 
NE Giles, WAM; Gill Pinnacle, WAM; 
Hammesley Rng, SAMA; Koolan Island, WAM; 
6.5 km N Mt Bell, WAM; Kununurra, ANIC, 
QDPIM; Millstream, ANIC; 5 km SE Millstream 
HS., ANIC: Mitchell Plateau, ANIC; West 
Peewah River, ANIC; Synnott Range, WAM; 
14°53'S, 125°45'E, SAMA. 

Remarks 

A relatively large species showing considerable 
variation in size, colour and strength of dorsal 
punctation making its identification difficult 
without dissection. The two colour morphs are 
well marked and occur together in the same 
populations. Occasional specimens have an 
intermediate dark-testaceous dorsal surface to a 
variable extent. It is my impression that the dark 
form is more common in the north where it is the 
dominant form in many areas. The black morphs 
are readily identified by their weak to moderate 
punctation contrasting markedly with the strong 
punctation in the two other species with black 
morphs, E. eyrensis and E. samae. It is also the 
only species with the combination of tips of the 
parameres hooked, weak to moderate dorsal 
punctures and black patterning on the head. In the 
North-east the species overlaps with E. weiri and 
E. pseudoweiri. These can be separated from most 
E. deserticola by the lack of black morphs, 
somewhat stronger punctation, pale tips to the 
maxillary palpi and the small amount of black on 
the front of the head. An occasional specimen of 
E. deserticola may also have pale palpi tips and 
much reduced black on the front of the head. 

Over most of its range E. deserticola is 
sympatric with E. maculiceps. The two species 
are readily separated by the male genitalia and 
presence of black morphs in E. deserticola. I 



Enochrus (Methydrus) elongatus (W. MacLeay) 

Philhydrus elongatus W. MacLeay, 1 873 

Enochrus (Lumetus) elongatus (W. MacLeay) 
Knisch, 1924 

= Philhydrus caledonicus Fauvel, 1883: syn. nov. 

= Enochrus caledonicus (Fauvel): Knisch, 1924 

Types 

Enochrus elongatus: Lectotype: 'Philhydrus 
elongatus Gayndah McL W'; 'K19506'. Right- 
hand specimen of two mounted on same card, AM 
herein designated. 

Paralectotypes: 1 , same data as lectotype, left- 
hand specimen, AM; 3, on same card, same data 
as lectotype, ANIC; 1, 'Philhydrus elongatus 
McL', 'Griffith Collection Id by A. M. Lea', 'Co- 
Type', SAMA; 1, 'Philhydrus elongatus M. 
Queensland cotype 14629', SAMA. 

Enochrus caledonicus: Lectotype: 'm', 
'Nouvelle Caledonie. Noumea Marais Anse Vata, 
Octobre Saves, ex. coll. Fauvel', 'Coll. et det. A. 
Fauvel Philhydrus caledonicus FvP, '17— 479% 
'lectotype' on red label. Remounted with genitalia 
dissected out, IRSNB. 

Paralectotypes: 1 , 'Nouvelle Caledonie Kanala, 
Rec. Coste, ex coll. Fauvel'; 'Coll. et det A. 
Fauvel Philhydrus caledonicus Fvl.' '17-479', 1, 
'Nouvelle Caledonie. Anse Vata, Noumea Saves', 
'Coll. et det A. Fauvel Philhydrus caledonicus 
Fvl,' IRSNB. Synonymy after examination of 
types. 

Description (number examined, 330) Fig. 7 

Elongate oval, body flattish, length 4.4 mm - 
5.0 mm. Dorsal surface testaceous, diffusely 
blotched, lighter towards sides, rear of head often 
diffusely darker but never distinctly darker than 
rest of head. Ventral surface dark red-brown, 
apical portions of legs lighter, palpi light 
testaceous, tips of maxillary palpi dark brown. 
Head covered with small sharply impressed, well 



AUSTRALIAN ENOCIIRUS 



145 











8 





10 




11 




12 




13 




14 



FIGURES l— 14. Dorsal views of apical portion of male genitalia. 1 & 2, E. maculiceps showing range of variation; 
3, E. pseudoweiri; 4, E. deserticola; 5, E. eyrensis; 6, E. isabellae; 7, E. elongatus, lateral view of median lobe; 8, 
E. weiri; 9, E. samae: 10, E. euhenangeei; 11, E. aliciae; 12, E. malabarensis; 13, E. esuriens; 14, E. mastersi. 



146 



C. H. S. WATTS 



separated punctures, quarter to half size of eye 
facet, a dozen or so much larger punctures 
inwards from each eye. Pronotum similarly 
punctate, a row of systematic punctures about 3x 
diameter of adjacent punctures running inwards 
from each front corner and smaller group of 
similar punctures a little behind middle on each 
side. Elytral punctures slightly stronger than 
those on pronotum, stronger laterally than on 
disc. Serial punctures, larger, sparse, hard to 
trace towards apex. Underside evenly setose- 
punctate, rugose portions of femur, 
approximately three quarters length of femur. 
Mesosternal keel well developed, anterior edge 
curved somewhat, nearly perpendicular, ventral 
edge flat or slightly convex. Notch on apical 
stemite small but well marked. 

Male: Aedeagus with crotchet-shaped hook at 
tip. Tips of parameres outwardly hooked. 
Metaclaws with enlarged basal lobe and rest of 
claw straightened. Pro- and mesoclaws curved 
with thickened basal portion 

Female: Claws curved with thickened basal 
portions. 

Distribution 

Australian Capital Territory 

Black Mt, ANIC. 

New South Wales 

Albury, ANIC; Allyn River, NMV; Armadale, 
ANIC; Balranald, ANIC; Bathurst, AM; Bogan 
River, AM; 20 mis SSW Bourke, SAMA; Broken 
Hill, SAMA; Coonabarabran, AM, ANIC; Cowra, 
AM; Ecceleston, AM; Hay, ANIC; 37 km E Hay, 
SAMA; Mt Kaputar Nat. Pk., ANIC; Kosciusko 
Nt Pk., ANIC; Lake Menindie, SAMA; Menindie, 
SAMA; Narrabri, ANIC; Norfolk Island, ANIC; 
97 km S Tibooburra, NMV. 

Northern Territory 

53 km NE Alice Springs, ANIC; 12 km SW by 
W Alice Springs, ANIC; Top of Ayers Rock, 
WAM; 97 km N Barrow Ck, SAMA; 30 km NE 
by E Borroloola, ANIC; Ellery Creek, NMV; Finke, 
SAMA; Glen Helen, NMV; Stanley Chasm, ANIC; 
15 km East, Vaughan Spring, HS, ANIC. 

Queensland 

Bollon Dist, AM; 42 km Boulia, ANIC: Bunya 
Mts, UQIC; Camooweal, QDPIM; Edgbaston HS, 
SAMA; 5 km NE Edungalba, SAMA; Glen 
Alpin, UQIC; Helidon, UQIC; 6 km E, Kamma, 
ANIC; Mackay, ANIC; MacPherson Rng, Nt Pk., 
AM; Marmor, ANIC; Mt Isa, QDPIM; Mt Spec, 



ANIC; Normanton, QDPIM; Tolga, QDPIM; 
Toowoomba, UQIC. 

South Australia 

Aroona Dam, SAMA; Mt Ban, ANIC; Old Billa 
Kallma HS, SAMA; Blanche Cup Spring, AM; 
Broken Hill, AM; Coopers Creek, SAMA; Coward 
Sp., SAMA; 16 km E Curdimurka, SAMA; 36 km 
ESE Curdimurka, ANIC; 1 1 km NE by Etadunna 
HS, ANIC; Gawler Rngs, SAMA; Lake George 
ANIC; Mt Lofty Rng, AM; Mannum, SAMA 
Marne River, SAMA, McDovall Peak, UQIC 
Murray Bridge, AM, SAMA; Olary, ANIC 
Oodnadatta, SAMA; Paralana Hot Springs, 
SAMA; Quorn, AM; Renmark, SAMA; Roonka 
Stn, SAMA; Roseworthy, SAMA; Scorpion 
Springs CP, SAMA; River Torrens, SAMA; 
Warburton, River, ANIC; Wearing Gorge, SAMA; 
Willochra Ck, SAMA. 

Tasmania 

15 mN Waratah, UQIC. 

Victoria 

Eppalock Res., NMV; Eustace Gap Ck, NMV; 
King Lake Nt Pk., NMV; Kiata, NMV; La Trobe 
River, NMV; Lake Hattah, ANIC; Lilydale, 
SAMA; Little Desert, ANIC; Lake Hattah, NMV; 
Marysville, SAMA; Melbourne, UQIC; Preston, 
NMV; Shepparton, ANIC; Skeleton Ck, SAMA; 
Stawell, SAMA; Swan Hill, NMV; Traralgon Ck, 
NMV; Violet Town, ANIC; East Warburton, 
NMV; Wyperfeld Nt Pk, ANIC. 

Western Australia 

15 km SSE Armadale, ANIC; 102 km SE by E, 
Broome, ANIC; 12 km NE Broome, ANIC; 
Bunbury, ANIC; 23 km NW by W Mt Arid, 
ANIC; 7 miles NE Giles, WAM; Gill Pinnacle, 
WAM; Great Victoria Desert, WAM; Mary sp. 
HS, ANIC; 13 km ESE Mooka H.S., WAM; 
Koolan Island, WAM; Serpentine River, NMV; 
West Peawah River, ANIC; Wilga, ANIC; 
Wmgello, ANIC. 

Remarks 

Enochrus elongatus differs from all other 
Australian Enochrus by the pale coloured dorsal 
surface including the head. It is the only 
Australian species with the tip of the aedeagus 
distinctly hooked upwards and with a basal 
swelling on the meta- and mesoclaws as well as 
the proclaws. 

The rear of the head is variably coloured. In 
many specimens it is darker than the front of the 



AUSTRALIAN ENOCHRUS 



47 



head, but diffusely so and never black and sharply 
delineated from the front as in most other species. 

Enochrus elongatus superficially resembles the 
pale morphs of E. deserticola and E. eyrensis in 
size and colour. It also shares with them, and no 
other Australian species, the hooked parameres. 
Unlike them the black colour morph common in 
these two species does not appear to occur in E. 
elongatus. In both E. deserticola and E. eyrensis 
the head is predominantly black with only small 
patches of yellow-brown on the front angles. In E. 
elongatus the head is uniformly yellow-brown or 
the rear is diffusely darker. In E. deserticola the 
dorsal punctation is much weaker than in E. 
elongatus and in E. eyrensis it is stronger. 

Enochrus elongatus is a widespread and 
common species within Australia including 
Norfolk Island. I can find no significant difference 
between Australian specimens and the types of E. 
caledonicus thus extending the range of E. 
elongatus to New Caledonia. 



Enochrus (Methydrus) esuriens (Walker) 

Philhydrus esuriens Walker, 1858 

Enochrus (Lumetus) esuriens (Walker): Knisch 
1924 

Enochrus (Methydrus) esuriens (Walker): 
d'Orchymont 1927 

= Philhydrus pullus Fauvel, 1883: syn. nov. 

= Enochrus (Lumetus) pullus (Fauvel): Knisch 
1924 

Types 

Enochrus esuriens: Type locality: Ceylon (Sri 
Lanka). Type not seen. 

Enochrus pullus: Lectotype: 6 'Coll. IRSNB, 
Nouvelle Caledonie, Anse Vata, Marais Juill 
Octobre Rec. Saves, ex. coll. FauveF; 'Coll. et det 
A. Fauvel Philhydrus pullus Fvl. IRSNB 17-497', 
IRSNB with red lectotype label, herein 
designated. Seen. 

Paralectotypes: 3 6 , 1 9 7 same data as 
lectotype in IRSNB. 

I have not seen type material of E. esuriens and 
have relied on the work of Balfour-Browne (1939, 
1945) and specimens identified by him in 
BM(NH) for my concept of this widespread 
species which is known from India, through 
South-East Asia to Northern Australia and 
Polynesia. 

Description (number examined, 130) Figs 13, 18 
Length 1.6 mm- 2.3 mm. Oblong-oval. Elytron 



and pronotum light-testaceous, often blotched and 
streaked darker, head black, area in front of eye, 
to about width of eye light-testaceous, central 
black panel two to three times width of lateral 
light area. Ventral surface dark-testaceous, 
appendages lighter towards extremities, whole of 
apical segment of maxillary palpi usually darker. 
Punctures on head moderately strong, systematic 
punctures inwards from eyes about size of eye 
facet and about twice diameter of adjacent 
punctures. Punctures on pronotum somewhat 
weaker, punctures on elytra somewhat stronger 
than on head, those towards apex and laterally 
about half diameter of adjacent serial punctures 
which are often not easy to trace. Mesosternal keel 
weakly developed. 

Male: Aedeagus narrow, pointed, virtually 
lacking terminal dorsal pad, shorter than 
parameres, collar nearer base than tip, parameres 
broad in basal half narrow for most of apical 
half, inner edge only very weakly sinuate, tips 
rounded. Proclaw straightened, strongly swollen 
at base, meso- and metaclaws rounded, swollen 
at base. 

Distribution 

New South Wales 

Wootton, ANIC. 

Northern Territory 

Adelaide River, ANIC; E Alligator River, 
AM; Darwin, ANIC; Humpty Doo, QDPIM; 12 
km N Humpty Doo, QDPIM; 6 km N Humpty 
Doo, QDPIM; Jim Jim Creek, ANIC; 9 km N 
by E Mudginbarry HS, ANIC; 19 km E by S Mt 
Borradaile, ANIC; 12 km NNW Mt Cahill, 
ANIC; Nourlangie Creek, ANIC; Oenpelli, 
AM. 

Queensland 

Annan Falls, ANIC; Ayr, ANIC; 29 km S 
Bamaga, ANIC; Cairns, ANIC, SAMA; Calliope 
River, ANIC; Cardstone, ANIC; 60 km S Coen, 
SAMA; 40 km N Coen, SAMA; Ingham, ANIC; 
Lansdowne St, ANIC; 73 km NW Laura, ANIC; 
Laura, QDPIM; Macleod River, SAMA; 
Mackay, ANIC; Mareeba, QDPIM; Mary Creek, 
ANIC; Mt Baird, ANIC; Mt Coolum, ANIC; Mt 
Ivor River, ANIC; Mt Molloy, ANIC; 2 km NNE 
Mt Tozer, ANIC; 1 1 km ENE Mt Tozer, ANIC; 
8 km E by N of Mt Tozer, ANIC; 12 km S 
Normanton, SAMA; North Pine River, UQIC; 
Port Douglas, ANIC; Redcliff, UQIC; 15 km 
WNW South Johnstone, QDPIM; Townsville, 
ANIC, SAMA; Weipa, QDPIM. 



148 



C. H. S. WATTS 



Western Australia 

Mitchell Plateau, AN1C; Nullagine, WAM. 

Remarks 

Enochrus esuriens' small size (<2.5 mm), 
predominantly black head and weak mesosternal 
keel make it one of the most readily recognised 
species of Australian Enochrus. It is most easily 
confused, not with other Enochrus, but with 
species of Paracymus and Anacaena, These latter 
genera lack the systematic punctures present on 
the head, pronotum and elytra of Enochrus. 



Enochrus (Methydrus) eubenangeei sp. nov. 

Types 

Holotype: <J , 'Qld. Babinda Eubenargee 
Swamp, 1/4/96, C. Watts', SAMA. 

Paratypes: 6, 'Bramston Beach via Innisfail, 
N.Q., 15 Aug. 1987, A. Walford-Huggins, coastal 
melaleuca swamp at light', ANIC; 1, 'N.T. 
Corndorl billabong nr. Jabiru, M.V. light, 
2.x. 1982, MB. MalipatiF, NTM. 

Description (number examined, 8) Fig 10 

Length 7.0- 7.5 mm. Broadly oval, relatively 
flat. Shiny. Black; palpi and tarsi testaceous. 
Maxillary palpi moderately long, pseudo first 
segment longer than distance from eye to front of 
clypeus, longer than maxillary stipe, apical 
segment approximately three-quarters length of 
penultimate. Head strongly punctate, most 
punctures about a puncture width apart, almost 
size of eye facet. Systematic punctures large, about 
3x size of adjacent punctures. Punctures on 
pronotum well marked, similar to those on head, 
not greatly weaker laterally, systematic punctures 
well marked about 3x size of adjacent punctures, 
lateral margins grooved and flanged, front and 
rear margins weakly grooved. Elytral punctures as 
on pronotum, not greatly weaker laterally. Serial 
punctures in four loose rows, relatively well 
marked, more numerous but more scattered 
laterally, elytra weakly grooved and flanged 
laterally. Mesosternal pillar well marked, sharply 
triangular in front view, front edge sloping, ventral 
edge short slightly pointed at rear, rear edge 
vertical in top half. Notch on apical sternite 
shallow, relatively broad. 

Male: Aedeagus with very broad basal portion 
and narrow apical portion which is curved 
upwards. Parameres relatively broad, hooked 
outwards at tips, bent upwards in apical half. 
Proclaws bent, broadly thicker in basal third, 



thickened part ends abruptly, meso- and 
metaclaws curved, basal third somewhat 
thickened, thickened part ending smoothly. 

Remarks 

Enochrus eubenangeei closely resembles E. 
aliciae. Apart from the genitalia it differs from E. 
aliciae in the lateral punctures on pronotum and 
elytra being almost as strong as more central ones 
and a greater extent of black. Based on the 
relatively few specimens of both species that are 
available E. eubenangeei also differs from E. 
aliciae by its black head, whereas in many E. 
aliciae the head has some testaceous colour, and 
by the broader but narrower exposure of the 
membrane between frons and clypeus than in E. 
aliciae where it is shorter but deeper. 

The aedeagi are distinct. Enochrus eubenangeei 
has a normal narrow apical portion to the aedeagus, 
without apical pad but bending strongly upwards. 
Enochrus aliciae has a very broad basal portion 
but, uniquely among Australian Enochrus, lacks 
the apical portion, resulting in the aedeagus 
reaching little beyond half way along the 
parameres. The parameres are rather similar but the 
tips are more obviously hooked in E. eubenangeei 
and they bend noticeably upward in this species. 

In its relatively large size, rounded shape and 
shiny, black appearance, E. eubenangeei also 
resembles E. mastersi. It, and E. aliciae, can be 
most readily separated from this more common 
species by the longer maxillary palpi with the 
apical segment shorter than the penultimate. The 
only other species it could be confused with is E. 
isabellae which is smaller, narrower, has light 
areas in front of its eyes and has the mesosternal 
process long and blade-like. 

Distribution 

Known only from type localities in Northern 
Territory and Queensland. 

Enochrus (Methydrus) eyrensis (Blackburn) 
Philhydrus eyrensis Blackburn, 1894 

Enochrus (Lumetus) eyrensis (Blackburn): 
Knisch 1924 

=s Philhydrus andersoni Blackburn, 1896: syn. nov. 

= Enochrus (Lumetus) andersoni (Blackburn): 
Knisch 1924 

?= Philhydrus persimilis Rcgimbart, 1908: syn. 
nov. 

?= Enochrus (Lumetus) persimilis (Regimbart): 
Knisch 1924 



AUSTRALIAN ENOCHRUS 



149 



15 



16 



17 




18 



FIGURES 15-20. Mesosterna. 15-18, Lateral view of 
mesostcrnal keel. 15, E. samae; 16, E. eyrensis; 17, E. 
maculiceps; 18, E. esuriens. 19 & 20, mesostcrnum. 19, 
E. mastersi (after Hansen 1990); 20, E. aliciae. 



Types 

Enochrus eyrensis: Holotype: 9, 'Blackburn 
coll. 1910-236', 'Philhydrus eyrensis Black 1 , 
remounted with '178T' on original Blackburn 
card, BM(NH), 

Paratypes: 2 'Philhydrus eyrensis Blackb co- 





type', 'Philhydrus eyrensis Blackb, C. Australia 
co-type 8242', SAM A. 

Enochrus andersoni: Holotype: ?sex. 
'Blackburn coll. 1910-236% 'Philhydrus 
andersoni, Blackb' remounted with '178T on 
original Blackburn card, BM(NH). 

Synonymy based on examination of types. 

Enochrus persimilis: Holotype: ?Victoria Aust; 
' Philhydrus persimilis Reg.' MNHN. Synonymy 
based on descriptions and examination of types 
(of E. persimilis in 1964, type not currently 
available). It is possible that my E. samae will 
prove to be this species. 

Description (number examined, 146) Figs 5, 16 

Oblong-oval, length, 3.2 mm - 5.0 mm' Two 
colour morphs exist, one with elytra and pronotum 
testaceous often with sutural lines and strial 
punctures darker, occasionally with disc of 
pronotum darker, head dark-testaceous to black 
with lighter area forward from eyes to about the 
same width as eyes giving a darker central panel 
three to four times the width of one of the lighter 
patches, clypeus dark. Second colour morph has 
the elytra dark-testaceous or black, pronotum a 



50 



C. H. S. WATTS 



similar colour but quite widely but diffusely 
lighter laterally, head as for first colour morph. 
Underside of both morphs dark-testaceous, 
appendages lighter towards extremities, except for 
maxillary palpi which have apical portion of 
apical segment darker. 

Head quite densely covered with relatively 
strong punctures about half size of eye facet, a few 
large punctures inwards from eyes, 2— 3x diameter 
of surrounding punctures. Punctures on pronotum 
slightly stronger, systematic punctures as in E. 
elongatus, 2-3x diameter of adjacent punctures. 
Punctures on elytra rather stronger than on 
pronotum, towards apex approaching size of serial 
punctures, which, as a consequence, are hard to 
trace. 

Mesosternal keel well developed, anterior edge 
weakly curved, nearly perpendicular, ventral edge 
straight or weakly convex, narrow vertical 'blade' 
above an extensive broader base. Notch on apical 
sternite moderately developed. 

Male: Aedeagus narrow, pointed, virtually 
lacking terminal dorsal pad, collar nearer base 
than tip. Parameres outwardly hooked at tip. 
Proclaw a little longer, less curved than in female, 
otherwise little sexual difference in claws. 

Distribution 

Australian Capital Territory 

Black Mt, ANIC; Jarvis Bay, ANIC. 

New South Wales 

Bonville, ANIC; 25 km N Bulahdelah, ANIC; 
Maroota South, ANIC; 8 km SE by S Moruya, 
ANIC; Norfolk Island, ANIC; Queanbeyan, 
ANIC; 17 mis S Woodburn, ANIC; Wootton, 
ANIC. 

South Australia 

Adelaide, SAMA; American River, SAMA; 
Beachport, AM, SAMA; Bool Lagoon, SAMA; 
Coonalpyn, SAMA; Fairview Park Cons Pk, 
SAMA; Hindmash Park, SAMA; Lucindale, 
SAMA; Naracoorte, UQIC; Taratap Stn, SAMA. 

Tasmania 

Scamanden River, NMV; Swansea, SAMA. 

Victoria 

East Pomborneit, ANIC; Lome, SAMA; 
Maffra, UQIC; Otway Rngs, UQIC; Wyperfeld 
Nt Pk, ANIC. 

Western Australia 

Albany, ANIC; Applecross, ANIC; Broomehill, 



WAM; Dumbleyung, WAM; 5 km NE Esperance, 
ANIC; 63 mis E Esperance, ANIC; 9 mis NE by 
N Esperance, ANIC; 19 km E Esperance, ANIC; 
5 km NW Esperance, ANIC; Fitzgerald River Nt 
Pk, ANIC; Karridale, ANIC; Maidavale, SAMA; 
Mt Margaret, ANIC; Mandurah, ANIC; 23 km 
NW by N Mt Arid, ANIC; Perth, ANIC; 8 mis E 
Pinjarra, ANIC; Stirling Rngs, SAMA; 12 km NE 
Wanneroo, WAM; 155 km SW Warburton, 
WAM; Wilga, ANIC. 

Remarks 

This relatively large species is common in both 
the south-east and south-west. 

The relatively strong dorsal punctation separates 
it from all other Australian Enochnis except E. 
samae and the generally much smaller E. 
malabarensis. Enochrus malabarensis is also a 
more northern species and lacks black morphs. 
From E, samae, E. eyrensis differs in having the 
parameres hooked at the tips rather than rounded 
and in a higher, more blade-like mesosternal keel. 
This latter character is, I believe, a good one but is 
hard to see on many specimens and is difficult to 
use if comparative material is not available. 

Enochrus eyrensis appears close to E, tristus 
(Broun) from New Zealand and some Pacific 
Islands in the hooked parameres and strong 
punctations. It differs from this species in having 
the apical portion of the aedeagus shorter than the 
basal and in rounded, not slightly straightened, 
male metaclaws. Enochrus eyrensis differs from 
E. abditus (Sharp) from New Zealand, in details 
of the aedeagus and mesosternal keel. 



Enochrus (Methydrus) isabellae sp. nov. 

Types 

Holotype: 6\ right-hand specimen on card, 
'Qld. Townsville, 10 km NW, 23/3/96, C. Watts', 
SAMA. 

Paratypes: 7, same data as holotype, SAMA; 3, 
'Ayr Qld., 10.ix.1990, W.B. Muir', in ANIC; 1, 
'Ingham, N.Q., 27.L68, J.C. Brooks', ANIC; 1, 
'Blighs Lookout, Cardwell Rng, N.Q. at light, 
30.ix.67, J. Brooks', ANIC; 1, 'Bramston Beach 
via Innisfail, N.Q., 1 5. viii. 1 987, A. Walford- 
Huggins. Coastal mclaleuca swamp at light', in 
ANIC; 6, 'Qld. Nardello's Lagoon nr. Mareeba 
29/3/96, C. Watts', SAMA. 

Description (number examined, 14) Fig 6 

Length 4.5 mm - 5.5 mm. Oval, shiny. Black 
apart from lateral areas of pronotum, region in 



AUSTRALIAN ENOCHRUS 



51 



front of eyes and appendages which are reddish- 
yellow. Tips of maxillary palpi darker. Head quite 
densely punctate, with weak to moderately sized 
punctures, systematic punctures rather sparse, 
somewhat larger than an eye facet and 2-3x size 
of adjacent punctures. Pronotum and elytra 
similarly punctured except that systematic 
punctures a bit larger in comparison with others. 
Mesosternal keel well-developed, narrow, often 
with small protuberance on anterior end. 

Male: Claws on protarsi more bent than in 
female with broad basal portion. Parameres 
hooked apically, aedeagus with apical portion 
shorter than basal, relatively broad, narrowing 
rapidly at tip, slight but noticeable dorsal 
thickening at tip. 

Distribution 

Known only from type localities in Queensland. 

Remarks 

A relatively large nearly totally black species. It 
strongly resembles the black morphs of E. 
eyrensis and E. samae but is much more weakly 
punctured, has a shorter apical portion of the 
aedeagus than in E. eyrensis and has hooked 
parameres which distinguish it from E. samae. 
Compared to the black morph of E. deserticola 
which occurs sympatrically with it, it is larger, 
more strongly punctured and has more extensive 
black on the front of the head than is normal in E. 
deserticola. The male genitalia are relatively 
similar to those of E. deserticola but E. isabellae 
has a broader and shorter apical portion to the 
aedeagus with a more developed apical dorsal/ 
ventral thickening. From E. elongatus it can be 
separated on colour, generally weaker punctation, 
weaker apical hook on aedeagus which ends well 
short of tips of parameres and lack of modified 
meso- and meta-claws in the males. 

The Townsville and Nardello's Lagoon 
specimens were collected from shallow water 
among thick drying reeds at the edge of extensive 
shallow swamps. 

Enochrus (Methydrus) maculiceps (MacLeay) 

Philhydrus maculiceps MacLeay, 1873 

Enochrus (Lumetus) maculiceps (MacLeay); 
Knisch 1924 

= Philhydrus laevigatus Blackburn, 1888: syn. nov. 

- Enochrus (Lumetus) laevigatus (Blackburn): 
Knisch 1924 

= Philhydrus artensis Fauvel, 1883: syn. nov. 



= Enochrus (Lumetus) artensis (Fauvel): Knisch 
1924 

- Enochrus (Lumetus) bryani d'Orchymont, 
1927: syn. nov. 

Types 

Enochrus laevigatus: Holotype: 'Philhydrus 
laevigatus Blackb', BM(NH), 'Blackburn coll. 
1910-236'. Remounted with M552T' on original 
Blackburn label. Synonymy based on examination 
of types. 

Enochrus maculiceps: Lectotype: Male. 
'Philhydrus maculiceps McL W. Gayndah', 
'K19505'. Right-hand specimen of two mounted 
on same card, AM, herein designated. 

Para lee totypes: 1, on same card as lectotype, 
AM; 2, same data as lectotype and mounted on 
one card, in ANIC; "Philhydrus maculiceps McL. 
'Co-type' Griffith collection id by A.M. Lea" ; 1, 
'Philhydrus maculiceps McL. Queensland co-type 
14631', SAM A. Synonymy based on examination 
of types. 

Enochrus artensis: Holotype: 'Nouvelle 
Caledonie He Art*, 'Rec. ex. coll. Fauvel', 'Coll. 
et det. A. Fauvel Philhydrus artensis Fvl\ with 
red Holotype label, IRSNB. 

Paratype: 9 , 'Nouvelle Caledonie Kanata Re 
Deplenche ex. coll. Fauvel'; 'Coll. et det. A. 
Fauvel Philhydrus artensis Fvl, IRSNB 17-479', 
with orange paratype label, IRSNB. Synonymy 
based on examination of types. 

Enochrus bryani: Holotype: 'Savaii Samoa', 
'Salailua v-22-24', 'H. Bryan Jr, Collector', 6, 
'Type', 'A. d'Orchymont det, Enochrus (Lumetus) 
bryani\ Bishop Museum, Honolulu. 

Paratype: 'Enochrus (Lumetus) bryani A. 
d'Orchymont det'; 'Samoan Is. Apia Upolu Is'; 
'female' T Samoa Mars 1924 Coll. d'Orchymont', 
IRSNB. 

Both the types are mounted on card from the 
same source and similarly labelled by 
d'Orchymont. d'Orchymont clearly identified the 
Bishop Museum specimen as the holotype. 
Unfortunately all but a hind tibia and tarsus of the 
holotype has been lost. I base my concept of E. 
bryani on the Brussels paratype and 
d'Orchymont' s description and illustration of the 
aedeagus. 

Description (number examined, 134) Figs 1,2, 17 
Length 2.6 mm 4.0 mm. Elytra testaceous, 
sutural lines, some serial punctures and a rough, 
small patch on each humeral angle darker; 
pronotum testaceous, disk rather darker than 
sides; head with testaceous areas in front of each 



152 



C. H. S. WATTS 



eye much wider than eye, central dark panel about 
half width of lateral light patches, boundary 
between areas often diffuse. Ventral surface dark- 
testaceous, appendages only slightly lighter 
towards extremities, maxillary palpi with tip of 
apical segment darker. Punctures on head 
moderately sized, a few larger punctures inwards 
from eyes a little smaller than eye facets and about 
4x diameter of adjacent punctures. Pronotum 
similarly punctate, systematic punctures relatively 
weak, smaller than eye facets. Interstrial punctures 
on elytra weak, verging on subobsolcte, serial 
punctures also relatively small and weak, both a 
little stronger apically and laterally, on humeral 
angle the serial punctures are about 3x the 
diameter of adjacent punctures but both are small 
and relatively weak. Mesosternal keel moderately 
developed, ventral edge flat except for a well 
developed anterior protuberance. 

Male: Genitalia variable in elongation, 
aedeagus usually relatively broad, narrowing to 
rounded point, collar closer to base than tip. 
Parameres relatively narrow, pointed. Male and 
female claws similar. 

Distribution 

Australian Capital Territory 

Blundello Creek, ANIC; Canberra, SAMA. 

New South Wales 

Albury, ANIC; Ashfield, AM; Balranald, 
NMV; Berry, SAMA; Bogan River, AM; 20 mis 
SSW Bourke, SAMA; Collector, SAMA; Congo, 
ANIC; 9 km NNE Coonabarabran, ANIC; 14 km 
W Coonabarabran, ANIC; Dc Burghs Rng, AM 
Deniliquin, ANIC; 37 km E Hay, SAMA 
Illadulla, ANIC; Jenolan Caves, SAMA 
Kenilworth, ANIC; North Sydney, NMV 
Tooloom Plateau, UQIC; Wallacia, SAMA 
Wilcannia, SAMA; 3 km S Wingellow, ANIC 
Wingham Scrub, ANIC; Wootton, ANIC; Valery, 
ANIC. 

Northern Territory 

30 mis W Alice Springs, ANIC; Stanley 
Chasm, SAMA; 100 mis W Mt Olga, WAM; 30 
km N Wauchopc, ANIC; Yuendumu, SAMA. 

Queensland 

31 km NE Aramac, SAMA; Atherton, QDPIM; 
Babinda, UQIC; Brisbane, UQIC, SAMA; 
Bundaberg, ANIC; Byfield, ANIC; Cardstone, 
ANIC; Clermont, AM; Edungalba, ANIC; Funnel 
Creek, ANIC; 50 mis W Mackay, ANIC; Mt 
Coolum, ANIC; 9 mis S Stanthorpe, ANIC; 



South Australia 

Arkaba Creek, SAMA; 80 mis S Cooper Pedy, 
SAMA; 10 km SE Coward Springs, SAMA; 
Murray River, SAMA; Wintana Station, SAMA. 

Victoria 

Healsville, SAMA; Maffra, UQIC; Nathatia, 
SAMA; Portland, SAMA; 13 km SE Shepperton, 
ANIC; 14 km NW Violet Town, ANIC. 

Western Australia 

Nr Mt Gibson, WAM; 3 km E by N Newman, 
ANIC. 

Remarks 

A widespread and common species resembling 
a small E. deserticola and difficult to separate 
from light morphs of this species without 
reference to the male genitalia. Somewhat more 
strongly punctured than in most E. deserticola. In 
the North-cast, E. maculiceps is sympatric with E. 
weiri and E. pseudoweiri which it closely 
resembles in general form. Both these species are 
a little more strongly punctured and have pale tips 
to their maxillary palpi and usually only a small 
central triangular area of black on the front of the 
head. However E, maculiceps with pale palpi and 
the central black portion on the front of the head 
reduced to a triangle, are not uncommon. 

The male genitalia are variable in elongation, 
from a squatter form with the aedeagus quite 
curved in lateral view, with a strong apical pad 
and with only a small amount of structure apical 
to the pad, through to a more elongate form with 
elongate parameres, nearly straight aedeagus with 
a weak apical pad and a quite pronounced broadly 
triangular portion apical to the pad. 

Some more strongly punctured specimens of E. 
maculiceps may approach weaker punctured 
specimens of E. malabarensis. In E. malabarensis 
the front of the head is nearly all black whereas in 
E. maculiceps the black area is seldom more than 
a third the width of the front of the head. 

I have compared Australian specimens with the 
holotype, a paratype and five other specimens of 
E. artensis Fauvcl from New Caledonia in IRSNB 
including two dissected males and consider that 
E. artensis is a junior synonym of E. maculatus. 



Enochrus (Methydrus) malabarensis 

(Regimbart) 

Philhydrus malabarensis Regimbart, 1903 

Enochrus (Lumetus) malabarensis (Regimbart): 
Kmsch, 1924 



AUSTRALIAN ENOCHRUS 



153 



Types 

Enochras malabarensis: Holotype. 'Make, 
Calicut Ind'; 'Philhydrus ma lobar ens is Reg', 
MNHN. 

Description (number examined, 37) Fig. 12 

Length 2.5 mm - 4.1 mm. Broadly oval. 
Elytron and pronotum coloured as for E. 
pseudoweiri. Head black, areas in front of eyes 
light testaceous to about width of eye, central 
black panel 3-4x width of lateral light area. 
Ventral surface as for E. pseudoweiri, tips of 
maxillary palpi sometimes a little darker than 
rest of palpi. Punctures on head relatively strong, 
often approaching the size of eye facet, 
systematic punctures inwards from eye a little 
larger, sometimes hard to trace. Pronotum 
moderately to strongly punctured, systematic 
punctures often hard to trace. Punctures on elytra 
somewhat stronger towards apex and sides, 
approaching size of serial punctures which, as a 
consequence, may be difficult to distinguish. 
Mesosternal keel moderately developed, 
pronounced protuberance anteriorly, composed 
almost entirely of broad basal portion. 

Male: Aedcagus relatively short, narrow, 
pointed with only slight apical pad, collar 
equidistant from tip and base. Parameres broad in 
basal half, narrow in apical quarter, inner edges 
almost straight, tips rounded. Proclaw rounded or 
weakly straightened strongly swollen at base, 
meso- and metaclaws, rounded. 

Distribution 

New South Wales 

Ashfield, AM; Bondi Heights, AM; Sydney, 
NMV, SAMA. 

Northern Territory 

Black Point Coburg Peninsula, ANIC; Coastal 
Plains Research Stn, ANIC; Crocodile Island, 
SAMA; Darwin, ANIC, SAMA; Groote Eyland, 
SAMA; Howard Springs, ANIC; Kakadu NP, 
ANIC. 

Queensland 

Bowen, SAMA; Brisbane, UQIC; Bundaberg, 
ANIC: Stewart River, SAMA. 



Enochrus. The punctation is strongest in 
specimens from the Darwin area where the 
systematic punctures on pronotum and elytra are 
virtually untraceable. The punctures get weaker to 
the south were some specimens can approach the 
situation in the most strongly punctate E. 
maculiceps, E. pseudoweiri and E. weiri. The 
greater extent of black on the front of the head 
(the pale area reduced to the width of an eye) will 
separate E. malabarensis from these species 
where the black portion covers <l/3 of the head 
width. Enochrus malabarensis has the unusual 
combination of strongly black head with pale tips 
to the maxillary palpi. 

The male genitalia of E. malabarensis differ 
from those of E. maculiceps in that the inner 
margin of the parameres are straight rather than 
sinuate to accommodate the apical pad on the 
aedeagus. Although the tip of the aedeagus in E, 
malabarensis is thickened dorsoventrally, it is not 
laterally expanded (to varying degrees) as in E. 
maculiceps. 

The mesosternal keel is stronger than in E. 
weiri and E. pseudoweiri and most specimens of 
these species lack the pronounced anterior 
downward protuberance found in both E. 
malabarensis and E. maculiceps (Fig. 17). The 
genitalia of E. weiri is distinctive, that of E. 
pseudoweiri quite closely resembles E. 
malabarensis but has a shorter and thinner 
aedeagus. 

Enochrus malabarensis differs from the two 
other strongly punctate Australian Enochrus (E. 
eyrensis and E. samae) by its smaller size, lack of 
black colour morphs, usually pale maxillary palpi, 
stronger punctation particularly on the head and 
the strong downward protuberance at the front of 
the mesosternal keel which is usually lacking in 
E, eyrensis and E. samae. Enochrus malabarensis 
has a generally more northern distribution than 
the other two species but overlaps with E. 
eyrensis on the east coast. The male genitalia 
readily separate the species (Figs 5, 12). 

I have not seen the type of E. malabarensis (it 
is unavailable at this time) and have based my 
concept of this species on specimens identified by 
d'Orchymont from Sulawesi in IRSNB. 



South Australia 

Billa Kalina Station, SAMA. 

Remarks 

The moderate size and strong dorsal punctation 
separate E. malabarensis from all other Australian 



Enochrus (Methydrus) pseudoweiri sp. nov. 

Types 

Holotype: S, '16°03'S to 16°05'S, 145°28'E, 
Cape Tribulation area, Qld., 21-28 Mar 1984, A. 
Calder and T. Weir\ ANIC. 



154 



C. H. S. WATTS 



Paratypes: All male. 4, "Cardwell Rng, N.Q., 
30.9.87, G.B. 'Q363'; 'J. G. Brooks Bequest 
1976', ANIC; 2, '15°03'S, 145°09*E, 3 km NE of 
Mt Webb, Qld., 1-3 Oct. 1980, T. Weir', ANIC; 

1, 'Whitfield Rg., Rd., ca. 486 m, Qld., 3.ii.l970, 
at light, J. G. and J. A. G. Brooks', ANIC; 1, 
<12°44S, 143°17'E, 8 km E by N of Mt Tozer, 
Qld., 7 July 1986, T. Weir and A. Calder', ANIC; 

2, Mclvor Rv., 25 mis N Cooktown, N Qld, 6 
May 1970, S. R. Curtis', one ANIC, one SAMA; 
1, 'Australia, N Qld, Iron Range, 26-31. x.1991, 
Wood, Dunn and Hasenpusch', QDPIM; 1, 'Cow 
Bay, N of Daintree N Qld, 20-1 7-11 1984 1, C. 
Cunningham', QDPIM; 1, 'Cow Bay, N of 
Daintree, Qld., 27/7/82, C. Watts', SAMA; 4, 
'Peach Ck, N Qld., 24/7/87, C. Watts', SAMA; 1, 
'Cairns, C. J. Wild, Jan 91', QM. 



ANIC; Cape Tribulation area, ANIC; 3km S by 
W of Cooktown, ANIC; 25mls N Cooktown, 
ANIC, SAMA; Cooktown, ANIC; 2mls N 
Kuranda, ANIC; 8km E by N of Mount Tozer, 
ANIC; 3km NE of Mount Webb, ANIC; Peack 
Ck, SAMA; 15km WSW South Johnstone, 
QDPIM; Whitfield Rg Rd, ANIC. 

Northern Territory 

Howard Springs, ANIC. 

Remarks 

Apart from the male genitalia and a tendency 
for the darker portion at the front of the head to be 
larger and more diffuse, I can find no difference 
between this species and E. weiri (see under E, 
weiri). 



Description (number examined, 33) Fig. 3 

Length 3.0 mm - 3.6 mm. Oblong oval. Elytra 
testaceous to dark-testaceous, sutural region and 
serial punctures darker; small darker patch on 
humeral angles in many specimens. Pronotum 
dark testaceous centrally, widely lighter laterally. 
Head dark testaceous-black, frons area light 
testaceous except for small triangularly shaped 
dark area with apex often not reaching front of 
head, boundary between darker area and light 
areas indistinct, clypeus dark testaceous, ventral 
surface dark testaceous, appendages somewhat 
lighter towards extremities, maxillary palpi 
lacking darker tip. Head sparsely covered by 
small weak punctures, much smaller than facets 
of eyes, a few larger punctures inward from eyes 
about size of eye facet and 2 3x larger than 
adjacent punctures. Elytral punctures a little 
stronger, shallow. Serial punctures relatively 
weak, hard to trace laterally except on humeral 
angles where they are more distinct and 3-5x the 
diameter of adjacent punctures. Mesosternal keel 
strongly raised, ventral edge weakly convex, 
usually with a distinct anterior protuberance, 
broader basal portion making up most of keel 
with only a narrow thinner section in lateral 
view. 

Male: Genitalia very stout to moderately stout 
overall. Aedeagus very slender, lacking terminal 
pad, collar nearer base than tip. Parameres broad, 
tips rounded. Proclaws curved, strongly swollen 
in basal half, more so than in female. 

Distribution 

Queensland 

Cairns, ANIC; Cardstonc, ANIC; Cardwell, 



Enochrus (Methydrus) samae sp. no v. 

Types 

Holotype: S, 'East Pombomeit, Vic. 24 km 
ESE Camperdown. Temporary pond, Aug. 1978- 
Feb. 1979, P.S. Lake coll.', ANIC. 

Paratypes: 2 6, same data as holotype, 
ANIC; 2 2, '29.01°S, 167.57°E, Norfolk 
Island, Filmy Fern Walk, 14 Nov. - 2 Dec. 
1984, I.D. Naumann ex ethanoP, ANIC; 4 9,4 
6, 'Stonor, Tas: Lea', SAMA; 'Swansea, Tas., 
Jan. C. Watts', SAMA; 1 2, 1 S, M0 km S 
Robe S.A., 1/83, C. Watts', SAMA; 2 & 9 
'Grampians, Vic, 2.63, C. Watts', SAMA; 1 
6, 'Chain of Ponds, S.A., December 1957, C. 
Watts', SAMA; 1 6, 'Mylor, S.A., Aug. 1958, 
C. Watts', SAMA. 

Description (number examined, 47) Figs 9, 15 

Length 4.0 mm - 5.0 mm. Oblong-oval. Elytra 
and pronotum dark-tcstaccous, quite broadly 
lighter at sides, dark area broken up with 
longitudinal rows of spots towards apex, front of 
pronotum often narrowly light-testaceous. Head 
dark-testaceous to black except for broad light- 
testaceous areas forward from eyes, leaving a 
central dark panel which is about the same width 
as one of the pale patches, boundary between the 
dark central panel and pale patches diffuse. 
Underside dark-testaceous, appendages only 
slighter lighter towards extremities, apical portion 
of apical segment of maxillary palpi darker. 
Punctures on head relatively strong, not much 
smaller than eye facet, a few larger punctures 
inward from eyes, about 3x the diameter o£ 
adjacent punctures; pronotal punctures on elytra a 



AUSTRALIAN ENOCHRUS 



155 



little stronger than on pronotum, towards apex and 
laterally approaching size of strial punctures 
which are consequently not easily traced. 
Mesosternal keel moderately developed, triangular 
shaped, broader basal portion makes up most of 
keel. 

Male: Aedeagus broad, well-marked terminal 
dorsal pad, collar nearer to base than to tip. 
Parameres with rounded tips. Male proclaws 
greatly swollen in basal half, strongly curved in 
apical half, female less swollen and more evenly 
curved. 

Distribution 

Australian Capital Territory 

Black Mt., ANIC. 

New South Wales 

Norfolk Isl., ANIC. 

South Australia 

Chain of Ponds, SAM A; Mylor, SAMA; 10 km 
S Robe, SAMA. 

Tasmania 

George Town, SAMA; Stonor, SAMA; 
Swansea, SAMA. 

Victoria 

Grampians, SAMA; Hamilton, NMV; Lome, 
SAMA; Otway Rngs., UQIC; East Pombomcit, 
ANIC. 

Remarks 

In general facies this species is very similar to 
E. eyrensis and at least in the South-east occurs 
sympatrically with it. The strong dorsal punctation 
and patterned head readily separates these two 
species from other Enochrus in the region. 
Enochrus samae differs from E. eyrensis in 
having rounded rather than hooked tips to the 
parameres and in a squatter mesosternal keel. This 
latter character is hard to use if comparative 
material is not available 



Enochrus (Methydrus) weiri sp. nov. 

Types 

' Holotype: o\ M2°44'S, I43°14'E, 3 km ENE of 
Mt Tozer, Qld., 28 Jun - 4 Jul 1986, T. Weir and 
A. Calder', ANIC. 

Paratypes: All S. I, '12°44'S, 143°17*E, 8 km 
E by N of Mt Tozer, Qld., 7 July 1986, T. Weir 
and A. Calder', ANIC; I, '12°44'S, 143°14'E, 3 



km ENE of Mt Tozer, Qld., 28 Jun - 4 Jul 1986, 
T. Weir and A. Calder', ANIC; 2, M2°43'S, 
143°17'E, 9 km ENE of Mt Tozer, Qld., 5-10 July 
1986, T. Weir and A. Calder', one ANIC, one 
SAMA; 1, 'Dejinghe Ck, N.Q., 3 mis SW of 
Yarrabah, 26.x. 1966 E. Bntton, R Trumble', 
ANIC; 1, M6°03'S to 16°05'S, 145°28'E Cape 
Tribulation area, Qld., 21-28 Mar 1984, A. 
Calder and T. Weir\ ANIC; 1, 'Australia, N Qld., 
Cow Bay N of Daintree R, 13. ix. 1990, 
Cunningham and DeFaveri', QDPIM; 1, 
'Australia, N Qld Cow Bay N of Daintree R, 
14.xii. 1987-6.i. 1988, Storey and Cunningham', 
QDPIM. 

Description (number examined, 1 8 with male 
genitalia extracted) Fig. 8 

As for E. pseudoweiri except for male genitalia. 

Male: Aedeagus broadest in middle, tapering to 
a point, lacking any terminal dorsal pad. Tips of 
parameres truncated, weakly bifid. 

Distribution 

Known only from type localities on Cape York 
in North Queensland. 

Remarks 

A tropical species known only from the 
Queensland east coast, north of Cairns. I have 
found no reliable way to separate this species 
and E. pseudoweiri, with which it is sympatric 
over most of its range, other than by the 
distinctively different male genitalia. These 
species can also be readily confused with E. 
maculiceps and with small brown colour morphs 
of E, deserticola which also occur in the region. 
The virtual absence of black on the front of the 
head and pale tips to the maxillary palpi will 
separate them from most examples of these 
species. Most E. weiri lack or have only a small 
downward protuberance at the front of the 
mesosternal keel whereas most E. maculiceps 
have it well developed. The differently coloured 
head and weaker dorsal punctures will readily 
separate E, weiri from the similarly sized E. 
malabarensis. 



Acknowledgments 

I thank the curators of the collections listed earlier for 
allowing me ready access to specimens in their care: Ms 
D. Churches typed the manuscript, Mr R. Gutteridge 
prepared the figures, Mrs M. Anthony and Mrs J. Evans 
helped with the library references and Dr E. Matthews 
helped improve the manuscript. 



156 



C. H. S. WATTS 



References 



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GENTILI, E. 1981. The genera Laccobius and 
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HANSEN, M. 1990. Hydatotrephis MacLeay, a 
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SOUTH 

AUSTRALIAN 

MUSEUM 



VOLUME 30 PART 2 
JANUARY 1998 
ISSN 0376-2750 



CONTENTS 



ARTICLES 

63 P. E. BOCK& P. L. COOK. 

A new species of multiphased Corbulipora MacGillivray, 1895 (Bryozoa; Cribriomorpha) 
from southwestern Australia. 

69 E. WILLIAMS 

The archaeology of lake systems in the middle Cooper Basin, north-eastern South 
Australia. 

93 C. H. S. WATTS 

Revision of Australian Amphiops Erichson, Allocotocerus Kraatz and Regimbartia 
Zaitzev (Coleoptera: Hydrophilidae). 

107 D. W. CORBETT 

Douglas Mawson: the geologist as explorer. 

137 C. H. S. WATTS 

Revision of Australian Enochrus Thomson (Coleoptera: Hydrophilidae).