Stereospondyls first definitively appeared during the
early Permian, as represented by fragmentary remains of a
rhinesuchid from the Pedra de Fogo Formation of
Brazil. Rhinesuchids are one of the earliest groups of stereospondyls to appear in the fossil record and are predominantly a
late Permian clade, with only one species,
Broomistega putterilli, from the
Early Triassic of
South Africa. However, almost all other groups of stereospondyls are not known from any Paleozoic deposits, which remained dominated by non-stereospondyl
stereospondylomorphs. The taxonomically unresolved
Peltobatrachus pustulatus, which has historically been regarded as a stereospondyl, is also known from the late Permian of
Tanzania. Several more fragmentary records are known from horizons spanning the Permo-Triassic boundary in South America, such as the rhinesuchid-like
Arachana nigra from Uruguay and an indeterminate mastodonsaurid from Uruguay. Following the Permo-Triassic mass extinction, stereospondyls are abundantly represented in the fossil record, particularly from Russia, South Africa, and Australia. This led Yates & Warren (2000) to propose that stereospondyls had sheltered in a high-latitude refugium that would have been somewhat shielded from the global effects of the extinction, and that they subsequently radiated from present-day Australia or Antarctica. Recent discoveries of a diverse rhinesuchid community in South America alongside non-stereospondyl stereospondylomorphs have led to an alternative hypothesis for a radiation from western Gondwana in South America. including
Koolasuchus, the youngest known stereospondyl (late Early Cretaceous) from what is now
Australia. There is also sparse evidence for the persistence of some trematosauroids into the Jurassic of Asia. If the recent hypothesis that
Chinlestegophis, a Late Triassic stereospondyl from North America, is indeed a stem
caecilian is correct, then stereospondyls would survive to the present day. == Lifestyle and ecology ==