HIP 41378 d explained
| HIP 41378 d |
| Discovered: | June 2016 |
| Discovery Method: | Transit |
| Apsis: | astron |
| Period: | 278.3618 ± 0.0005[1] d |
| Semimajor: | 0.88 ± 0.01 au |
| Star: | HIP 41378[2] |
HIP 41378 d (also known as EPIC 211311380 d) is an exoplanet orbiting around the F-type star HIP 41378. It has a radius about 3.5 times that of Earth.[2] Planetary orbit is significantly inclined to the equatorial plane of the parent star, misalignment been equal to 57.1°.
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 d CONFIRMED PLANET OVERVIEW PAGE . NASA Exoplanet Archive . 2016-07-08.
