TOI-4127 b explained

Caption:	TOI-4127 b is a eccentric Jupiter, Gas giant type planets with a high eccentric orbit.
TOI-4127 b
Discovery Method:	Transit
Discovered:	2023
Discoverer:	TESS
Extrasolarplanet:	Yes
Eccentricity:	0.75
Inclination:	89.3
Mass:	2.3
Mean Radius:	1.096

TOI-4127 b is a confirmed gas giant type exoplanet orbiting the faint F-type main-sequence star TOI-4127, about 1,042 light years away from earth. The planet is known as a warm Jupiter, a type of gas giant exoplanet that is not a hot Jupiter but is also not a cold Jupiter.^{[1] [2]}

Physical characteristics

This planet has a mass of 2.3 and a radius of 1.096 .^[3]

Orbital characteristics

TOI-4127 b orbits TOI-4127 at a distance of 0.3081 astronomical units (AU) and an orbital eccentricity of 0.75. The planet takes 56.4 days to orbit its parent star. Its orbit lies at a orbital inclination of 89.3°. The exoplanet orbits its parent star at a high eccentricity making it also a eccentric Jupiter.^[4]

Notes and References

1. Web site: Robert Lea . 2023-04-12 . New 'warm Jupiter' exoplanet discovered by NASA's planet-hunting satellite . 2023-11-01 . Space.com . en.
2. Web site: Exoplanet-catalog . 2023-11-01 . Exoplanet Exploration: Planets Beyond our Solar System . en.
3. Web site: Martin . Pierre-Yves . 2023 . Planet TOI-4127 b . 2023-11-01 . . en.
4. Gupta . Arvind F. . Jackson . Jonathan M. . Hebrard . Guillaume . Lin . Andrea S. . Stassun . Keivan G. . Dong . Jiayin . Villanueva . Steven . Dragomir . Diana . Suvrath Mahadevan . Mahadevan . Suvrath . Wright . Jason T. . Almenara . Jose Manuel . Blake . Cullen H. . Boisse . Isabelle . Cortes-Zuleta . Pia . Dalba . Paul A. . 2023-06-01 . A High-Eccentricity Warm Jupiter Orbiting TOI-4127 . The Astronomical Journal . 165 . 6 . 234 . 10.3847/1538-3881/accb9b . 2303.14570 . 0004-6256. free .