Question: 83 Leonis Bb, also catalogued as HD 99492 b or abbreviated 83 Leo Bb, is an extrasolar planet approximately 58 light-years away in the constellation of Leo, also called by which term that's one of the big cats in the Felidae family and a member of genus "Panthera"?

Context articles: Lion
HD 189733 b
HD 17156 b
83 Leonis
14 Herculis b
83 Leonis Bb
HD 102272 b
Gliese 777 b
Gliese 777 c
HD 10647 b

The lion ("Panthera leo") is one of the big cats in the Felidae family and a member of genus "Panthera".
 It has been listed as Vulnerable on the IUCN Red List since 1996, as populations in African range countries declined by about 43% since the early 1990s.
 Lion populations are untenable outside designated protected areas. Although the cause of the decline is not fully understood, habitat loss and conflicts with humans are the greatest causes of concern.
 The West African lion population is listed as Critically Endangered since 2016.
 The only lion population in Asia survives in and around India's Gir Forest National Park and is listed as Endangered since 1986.
HD 189733 b is an extrasolar planet approximately 63 light-years away from the Solar System in the constellation of Vulpecula.
 The planet was discovered orbiting the star HD 189733 A on October 5, 2005, when astronomers in France observed the planet transiting across the face of the star.
 With a mass 13% higher than that of Jupiter, HD 189733 b orbits its host star once every 2.2 days at an orbital speed of 152.5 km/s , making it a hot Jupiter with poor prospects for extraterrestrial life.
 Being the closest transiting hot Jupiter to Earth, HD 189733 b is a subject for extensive atmospheric examination.
 The atmosphere of HD 189733b has been extensively studied through high- and low-resolution instruments, both from ground and space.
 HD 189733 b was the first extrasolar planet for which a thermal map was constructed, to be detected through polarimetry, to have its overall color determined (deep blue), to have a transit detected in X-ray spectrum and to have carbon dioxide detected in its atmosphere.
HD 17156 b is an extrasolar planet approximately 240 light-years away in the constellation of Cassiopeia.
 The planet was discovered orbiting the yellow subgiant star HD 17156 in April 2007.
 The planet is classified as a relatively cool hot Jupiter planet slightly smaller than Jupiter but slightly larger than Saturn in a so-called "torched orbit".
 This highly-eccentric three-week orbit takes it approximately 0.0523 AU of the star at periastron before swinging out to approximately 0.2665 AU at apastron.
 Its eccentricity is about the same as 16 Cygni Bb, a so-called "eccentric Jupiter".
 Until 2009, HD 17156 b was the transiting planet with the longest orbital period.
83 Leonis, abbreviated 83 Leo, is a binary star system approximately 58 light-years away in the constellation of Leo (the Lion).
 The primary star of the system is a cool orange subgiant star, while the secondary star is an orange dwarf star.
 The two stars are separated by at least 515 astronomical units from each other.
 Both stars are presumed to be cooler than the Sun.
14 Herculis b or 14 Her b is an extrasolar planet approximately 59 light-years away in the constellation of Hercules.
 The planet was found orbiting the star 14 Herculis, with a mass that would likely make the planet a Jovian planet roughly the same size as Jupiter but much more massive.
 It was discovered in July 1998 by the Geneva Extrasolar Planet Search team.
 At the time of discovery it was the extrasolar planet with the longest orbital period, though longer-period planets have subsequently been discovered.
83 Leonis Bb, also catalogued as HD 99492 b or abbreviated 83 Leo Bb, is an extrasolar planet approximately 58 light-years away in the constellation of Leo (the Lion).
 The planet was discovered in January 2005 by the California and Carnegie Planet Search team, who use the Doppler spectroscopy method to detect planets.
 It orbits in a close orbit around the star, completing one orbit in about 17 days.
HD 102272 b is an extrasolar planet approximately 1,200 light-years away in the constellation of Leo.
 The planet was discovered orbiting the K-type giant star HD 102272 in 2008.
 The planet was discovered by the radial velocity method, using the Hobby-Eberly Telescope.
 Another planet, HD 102272 c, was also discovered orbiting the same star.
 The discovery was announced in June 2008.
 HD 102272 b orbits at an average of 0.614 astronomical units away from its star, with a mass at least 5.9 ± 0.2 times that of Jupiter.
Gliese 777 b, also known as Gliese 777 Ab or HD 190360 b, is an extrasolar planet approximately 52 light-years away in the constellation of Cygnus.
 The planet was discovered orbiting the primary star of the Gliese 777 system in June 2002 (by the Geneva Extrasolar Planet Search Team) using the radial velocity method.
 The planet is at least one half more massive than Jupiter but roughly the same size as Jupiter.
 Because the inclination of the planet's orbit is not known, the true mass is unknown.
 But it is unlikely to be much more than the given minimum mass.
Gliese 777 c, often catalogued as Gliese 777 Ac or simply HD 190360 c, is an extrasolar planet approximately 52 light-years away in the constellation of Cygnus.
 The planet was discovered orbiting the primary star of the Gliese 777 system in 2005 using the radial velocity method and confirmed in 2009.
 The planet was once called the "smallest extrasolar planet discovered", but this is currently no longer the case.
 With a minimum mass just 18 times that of the Earth, the planet is likely a "hot Neptune" planet, a small Jovian planet, or possibly a large terrestrial planet (a super-Earth).
HD 10647 b, also catalogued as q Eridani b, is an extrasolar planet approximately 57 light-years away in the constellation of Eridanus (the River).
 The planet is a mid-Jovian that orbits 103% farther from the star than Earth to the Sun.
 It takes about 33 months to orbit with semi-amplitude of 17.9 m/s.