HIP 41378 b explained

HIP 41378 b
Discovered:	June 2016
Discovery Method:	Transit
Apsis:	astron
Period:	15.57208±0.00002 d
Semimajor:	0.1283 au
Inclination:	88.75±0.13^[1]
Star:	HIP 41378^[2]

HIP 41378 b (also known as EPIC 211311380 b) is an exoplanet orbiting around the F-type star HIP 41378. It has a radius about 2.6 times that of Earth.

See also

• Lists of exoplanets
• Gliese 1132 b, rocky exoplanet with a confirmed atmosphere.
• Mu Arae c, in the constellation Ara
• Planetary system

Notes and References

1. 1911.07355. Santerne. A.. An extremely low-density and temperate giant exoplanet. Malavolta. L.. Kosiarek. M. R.. Dai. F.. Dressing. C. D.. Dumusque. X.. Hara. N. C.. Lopez. T. A.. Mortier. A.. Vanderburg. A.. Adibekyan. V.. Armstrong. D. J.. Barrado. D.. Barros. S. C. C.. Bayliss. D.. Berardo. D.. Boisse. I.. Bonomo. A. S.. Bouchy. F.. Brown. D. J. A.. Buchhave. L. A.. Butler. R. P.. Collier Cameron. A.. Cosentino. R.. Crane. J. D.. Crossfield. I. J. M.. Damasso. M.. Deleuil. M. R.. Delgado Mena. E.. Demangeon. O.. 29. astro-ph.EP. 2019.
2. Web site: HIP 41378 b CONFIRMED PLANET OVERVIEW PAGE . NASA Exoplanet Archive . 2016-07-07.