Khirtharia is an extinct Raoellidae artiodactyl which inhabited what is now northern India and Pakistan during the middle-upper Eocene (early Lutetian).
The endocranial cast of the brain of K. inflata showed that the brain of Khirtharia was slightly smaller than that of Indohyus. The Neurocranium had a volume of approximately 5.5 cubic centimeters. The small size of the brain is smaller than the brain size of contemporary artiodactyls, showing that whales evolved from artiodactyls of relatively low brain size. It was also hypothesized that the small brain size of Khirtharia could be an adaptation to a semi-aquatic life, supporting the position of Raoellidae as the sister group to Cetacea.
Discovery
Khirtharia was named by G.E. Pilgrim in the year 1940.
These remains were placed under the species
K. dayi.
In 1972, the new
taxon Bunodentus inflatus was discovered by A. Ranga Rao, which was synonymized with
Khirtharia under the new species
K. inflata.
was described by Thewissen. Gingerich, and Russel (1978) from the remains of a single tooth.
Orliac and Ducrocq (2012) found that the tooth was more similar to
Khirtharia, and thus created
K. major.
was named by Thewissen et al. (2001) from northern Pakistan.
Classification
External classification
The placement of
Khirtharia has varied throughout the history of the taxon, although it is currently a member of Raoellidae. When
Khirtharia was first discovered by Pilgrim (1940), it was assigned to
Helohyidae.
However, Dehm and Oettingen-Spielberg (1958) moved
Khirtharia, along with
Haqueina, to
Dichobunidae.
When Coombs and Coombs (1977) reevaluated Helohyidae, they determined that the remains of
Khirtharia were not diagnostic of any particular family of artiodactyls, and therefore left
Khirtharia as an artiodactyl of uncertain position.
In 1981, the family Raoellidae was created, with
Khirtharia being one of the three
Genus included, along with
Raoella (a junior synonym of
Indohyus) and
Kunmunella. After the results of a phylogenetic analysis by Orliac and Ducrocq (2012), it was determined that
Khirtharia, along with
Metkatius, were the most derived members of Raoellidae.
This result was confirmed by a phylogenetic analysis performed by Rana et al. (2021) in their description of
Rajouria.
Internal classification
The first species of the genus
Khirtharia to be named was
K. dayi, which is also the type species.
K. dayi was named in 1940 by G. E. Pilgrim from a fragmentary
mandible and
maxilla with some of their respective
Premolar and molars.
In 1980, Robert M. West suggested that
Bunodentus, at the time known only from an isolated molar and fragmentary mandible, was synonymous with
Khirtharia dayi, although this change was only officially enacted by Kumar and Sahni (1985) who believed
B. inflatus was different enough from
K. dayi to warrant being placed under a different species.
Since there was only one species of
Bunodentus,
B. inflatus,
Khitharia gained the species
K. inflata.
Likewise,
Indohyus major was named by Thewissen et al. (1978) from a single molar in Pakistan. It was named
I. major due to the size of the tooth, being approximately twice the size of other raoellid teeth.
Orliac and Ducrocq found that this tooth was more similar to
Khirtharia, however, and assigned it to the new species
K. major.
was named by Thewissen et al. (2001) from the remains of a single molar in northern Pakistan.
The species name (meaning gold in
Latin) refers to the color of the sediments which the fossil was found in.
Description
Khirtharia is a raoellid that lived during the early Lutetian age. It is most similar to
Metkatius in that it had bunodont teeth. As a raoellid,
Khirtharia was relatively small, although there was large interspecific variety in size.
K. dayi
K. dayi is the type and smallest species of
Khirtharia, and one of the two smallest species of Raoellidae as a whole.
Within
K. dayi, there are two similar but distinct morphs: a more common one with relatively small molars and the other, more rare, one with relatively large molars.
Upper Dentition
The first premolar is single-rooted, while the second is double-rooted. The second premolar is narrow and non-molarized; in life it would have appeared similar to a canine. The tooth is widest posteriorly because of a relatively large postero-lingual (tongue-side) shelf. The third premolar is similar to the second; it is non-molarized and has a postero-lingual shelf. However, the third molar was slightly larger and there were large vertical grooves. The fourth premolar represents a transition from the canine-like first to third premolars to the molars. There are only two cones on the tooth, both situated in teh front portions. Because of this, the posterior section of the tooth is low and flattened. The cone on the labial (lip) side of the tooth is larger than the protocone, which it is connected to by a ridge.
The first molar is square-shaped. There are four large cusps which are rounded; they were likely used for crushing plant matter. The paracone is the largest cusp while the hypocone is the smallest. The first molar is very transverse. The second molar is significantly larger than the first and, as opposed to being square in shape, is trapezoidal. Cingulum are less apparent than the first molar. The second molar is has bulbous cusps. As with the first molar, the paracone is the largest of the cusps.
Lower Dentition
While the first and second premolars were not preserved, Ranga Rao postulated that the first premolar was single-rooted while the second premolar was double-rooted. The third premolar is large and triangular, with prominent cingulum. The fourth premolar is slightly larger than the third. It is more
Premolar than the upper fourth premolar.
The lower molars of Khirtharia lack the paracone. The lower molars are highly bunodont. There is a large ridge connecting the protocone and metacone and a large ridge conencting the hypocone and entocone. The largest molar is the third.
Skull
By being in the same genus,
K. dayi's skull is similar to the better-preserved skull of
K. inflata. The snout is broad. There is a prominent preorbital
foramen above the third premolar. The orbits are open posteriorly and there is no
postorbital bar, showing that
Khirtharia was likely omnivorous. The
Jugal bone bone connects to the maxilla above the second molar. The
Choana connect to the throat just after the third molar. There is a large parietal crest, although a relatively minor sagittal one.
Mandible
There is a specimen of
K. dayi where the entire mandible is preserved except for the most posterior portion of the coronoid. Symphysis occurs before the first premolar in one specimen, although in another it ends at the seconds premolar. The mandible is shallow for the first two premolars, but it quickly grows in height by about 20% with the last two. The
Mandible begins immediately after the third molar. It is tall and vertical. The angle is enlarged, especially posteriorly so that it extends bast the head of the mandible.
K. inflata
Khirtharia inflata differs from
K. dayi in terms of size in that it is between the size of the two morphs and slight dental differences.
The premaxilla is elongated and the maxilla is tall.
The incisors are caniniform and raptorial, likely adapted to seizing prey.
Compared to
K. dayi,
K, inflata has more bunodont and squarish upper molars; the upper molars of
K. inflata are similar to the lower molars of
K. dayi. The lower molars are also more bunodont and the hypocone is the largest cusp (in
K. dayi the metacone is the largest cusp). The lower molars are also longer than in
K. dayi. All molars have cusps separated from each other by valleys.
The skull is relatively rectangular, with the height staying of the skull slowly decreasing anteriorly until the beginning of the
Nostril, where it is about half of its maximum height. While there is a
sagittal crest, it is minor.
K. aurea
Khirtharia aurea is known from relatively sparse remains. Depending on the validity of
K. major as a species of
Khirtharia,
K. aurea is either the largest or second largest species of
Khirtharia.
The molars of
K. aurea have more prominent cingulum than in both
K. dayi and
K. inflata. Unlike
K. inflata, the hypocone is reduced to the point of being smaller than the protocone and the cusps are (unsurprisingly) less inflated than in
K. inflata. The two known upper molars are large and bunodont. In the left first molar, the metacone is taller and narrower than the protocone, which is the largest cusp overall. The hypocone is much smaller than the protocone and shifted labially. In the third molar, the paracone being the largest cusp. The protocone is less tall than the paracone, although roughly the same in the other dimensions.
In 2007, a study came out stating that the holotype specimen, previously identified as a third molar, could possibly be a second molar.
K. major
K. major is a possible species of
Khirtharia known only from two molars. It is the largest species of
Khirtharia and the largest raoellid as a whole; it is twice the size of
Indohyus indirae. It is different from all other species of
Khirtharia in that it has an elongated third molar, larger hypocone, and a variety of other small morphogical differences.
Paleobiology
Khirtharia was most similar to
Metkatius in terms of its paleobiology due to the shared bunodont nature of their teeth, although
Khirtharia's teeth were even more bunodont than those of
Metkatius.
The incisors of
Khirtharia were caniniform, which is an adaptation for catching and holding onto potential prey.
The molars are bunodont, which is a characteristic of omnivorous taxa. Since
Khirtharia also had the most bunodont teeth of any raoellid, this suggests it had the most carnivorous diet of any raoellid.
Due to being a raoellid,
Khirtharia was almost certainly semi-aquatic.
Therefore,
Khirtharia was probably an omniverous semi-aquatic chevrotain-like creature.
See also
-
Evolution of cetaceans
-
Cetacea
-
Pakicetus
-
Glossary of mammalian dental topography
