|Historic desert rat kangaroo range in orange|
The desert rat-kangaroo (Caloprymnus campestris), also called the buff-nosed rat-kangaroo or the plains rat-kangaroo, is an extinct small hopping marsupial endemic to desert regions of Central Australia. It was discovered in the early 1840s and described by John Gould in London in 1843, on the basis of three specimens sent to him by George Grey, the governor of South Australia at the time.
It was formed like a kangaroo, but had the bulk of a small rabbit, and was described as being of a delicate and slender form. Its average body size was estimated to be about 254–282 mm in addition to a 307- to 377-mm-long tail. Its head was short, blunt, and wide, different from that of any kangaroo or wallaby with a naked nose, short and rounded ears.
The colour of its dense, straight, soft fur was appropriate for its desert surroundings. It was very pale yellowish brown, the hairs tipped with sooty brown; interspersed with the under fur were many long brownish white hairs. Its underbelly was described as white with very pale yellowish-brown feet and tail.
A distinguishing feature of this species was the difference in size between the fore and hind limbs. Its fore limbs were quite delicate with bones weighing 1 gram, while its hind limbs are large with bones weighing 12 grams. This difference is related to saltation. Other characteristics related to hopping locomotion include a long, but rather thin tail.
Distribution and habitat
Caloprymnus campestris was thought to occupy a relatively small area in South Australia, extending just over the borders of southwestern Queensland and Northern Territory. It was last seen in 1935 in the eastern Lake Eyre basin of northern Southern Australia
The desert rat-kangaroo lived in the desert regions of Australia, including clay pans, loamy flats, sand ridges, and gibber plain habitats. Its native habitat was very arid, cover is sparse, and consists of saltbush and other chenopods and emu bush.
Ecology and behaviour
Caloprymnus campestris was solitary except for mothers with young offspring. It lived in nests built over shallow depressions in the ground. These nests were excavated or found and are crucial in the desert, where temperatures can be high, while relatively little brush or foliage is available for cover. The "pits" were lined with grass, which females carried to the nest with their tails. The nest would then be covered with twigs to provide cover from the scorching sun. Often, the desert rat kangaroo was found peeking out of the top of the nest to observe its surroundings. This species would spend most of the day taking cover in the nest, and emerge at dusk to feed. Thus, it was at least partially nocturnal.
The desert rat-kangaroo was mainly herbivorous, feeding on foliage and stems of desert vegetation, but has also been found to eat insects such as beetles and weevils. It was so independent of water, it even shunned the succulent plants of the sand hills. It was able to survive without any surface water while feeding on green plants.
It had a distinct method of hopping. Its posture was forward and the long tail was extended when it moved at high speeds. Unlike other marsupials, Caloprymnus would land with the right foot in front of the left foot. It showed great endurance while being chased on horseback at high speeds (Finlayson reported chasing an individual over 12 miles), and "paused only to die".
Females reached sexual maturity at about 11 months, while males reached maturity some two months later. Marked sexual dimorphism was apparent, with females being larger. Females went through estrus at three-week intervals and could mate throughout the year. Although able to mate all year, they had an irregular breeding season when most mating took place. Females with pouched joeys had been found between June and December. Young were born very undeveloped, as is typical of marsupials. Gestation was probably around one to two months, with a pouch period of two to three months. All females were found with only one young at a time. Young remained dependent for over a month after leaving the pouch and soon after would leave permanently.
Rediscovery and extinction
The desert rat-kangaroo was discovered in the early 1840s. However, after these early sightings, it was no longer recorded for 90 years (aside from an unconfirmed report in 1878), and was widely believed to be extinct. This species, even before European colonisation, was apparently never abundant. Following the relief of drought conditions which improved the local habitat, the animal was rediscovered in 1931 when Hedley Finlayson found a thriving colony of them. He made multiple returns, but after a few years, the population disappeared. The last confirmed record of the species came in 1935 from near Ooroowilanie, east of Lake Eyre.
Caloprymnus campestris was well adapted to the extremely barren and arid regions it inhabited; these traits saved it from competition by introduced species like the rabbit or sheep. However, as early as the 1930s, the red fox had spread to the areas inhabited by the desert rat kangaroo. Thus, the rapid decline of the desert rat-kangaroo shortly after its recovery in 1931 correlates with the invasion of its habitat by the fox. Predation by the red fox and cats, as well as variable seasonal patterns and overhunting by indigenous Australians, were blamed for the extinction of this species.
No reliable reports of the species have been made since 1935, but unconfirmed sightings in Queensland followed periods of rain in 1956-1957 and 1974-1975. Also, recent remains of this species have been found in the mid 1980s inside caves.
In view of its amazing recovery following a 90-year period when it was not seen, the extinction of the desert rat-kangaroo is not certain; thus, sightings of this animal would not fall into the cryptozoology category. In similar cases, the broad-faced potoroo was last seen in the late 19th century and is considered extinct, Gilbert's potoroo was considered extinct for 120 years prior to its rediscovery in 1994, and the long-footed potoroo was only discovered in 1967.
The finding of recent remains in the 1980s casts some doubt on the extinction of this species. Professor Ronald Nowak stated in his 2005 book, "perhaps a small population still survives, awaiting the time when it again may increase in response to proper conditions."
- Australasian Mammal Assessment Workshop (2008). Caloprymnus campestris. In: IUCN 2008. IUCN Red List of Threatened Species. Retrieved 29 December 2008. Database entry includes justification for why this species is listed as extinct
- Johnson, C. (2006). "Chapter 1: A brief history of Australia's mammals". Australia's mammal extinctions: a 50,000 year history. Cambridge University Press. p. 278. ISBN 978-0-521-84918-0. OCLC 63187432.
- Finlayson, H. H. (1932-06-11). "Rediscovery of Caloprymnus campestris (Marsupialia)". Nature 129 (3267): 871–871. doi:10.1038/129871b0. Retrieved 2011-09-03.
- Richard Lydekker (1894). A hand-book to the marsupialia and monotremata.
- Francis Harper (1945). Extinct and Vanishing Mammals of the Old World.
- "Caloprymnus campestris — Desert Rat-kangaroo". Australian Department of Sustainability, Environment, Water, Population and Communities. Retrieved 2011-09-03.
- Heddle, Enid Moodie; Millington, Iris (1962), How Australian literature grew, F. W. Cheshire, retrieved 01-08-2009 Check date values in:
- Fisher, D. O.; Blomberg, S. P. (2010-09-29). "Correlates of rediscovery and the detectability of extinction in mammals". Proceedings of the Royal Society B 278 (1708): 1090–1097. doi:10.1098/rspb.2010.1579. PMC 3049027. PMID 20880890. Retrieved 2011-09-03.
- Ronald Nowak (2005). Walker's Marsupials of the World. ISBN 0-8018-8222-2.