HIP 41378 c explained
HIP 41378 c |
Discovered: | June 2016 |
Discovery Method: | Transit |
Apsis: | astron |
Period: | 31.70603±0.00006[1] d |
Semimajor: | 0.2061±0.0024 au |
Inclination: | 88.477±0.0.06 |
Star: | HIP 41378[2] |
Mean Radius: | 2.727±0.06 |
Mass: | 4.4±1.1 |
HIP 41378 c (also known as EPIC 211311380 c) is an exoplanet orbiting around the F-type star HIP 41378. It has a radius about 2.7 times that of Earth.[2]
See also
Notes and References
- 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.
- Web site: HIP 41378 c CONFIRMED PLANET OVERVIEW PAGE . NASA Exoplanet Archive . 2016-07-07.