K2-136: A Binary System in the Hyades Cluster Hosting a Neptune-sized Planet
Abstract
We report the discovery of a Neptune-size planet ({R}{{p}}=3.0 {R}\oplus ) in the Hyades Cluster. The host star is in a binary system, comprising a K5V star and M7/8V star with a projected separation of 40 au. The planet orbits the primary star with an orbital period of 17.3 days and a transit duration of 3 hrs. The host star is bright (V = 11.2, J = 9.1) and so may be a good target for precise radial velocity measurements. K2-136A c is the first Neptune-sized planet to be found orbiting in a binary system within an open cluster. The Hyades is the nearest star cluster to the Sun, has an age of 625-750 Myr, and forms one of the fundamental rungs in the distance ladder; understanding the planet population in such a well-studied cluster can help us understand and set constraints on the formation and evolution of planetary systems.
- Publication:
-
The Astronomical Journal
- Pub Date:
- January 2018
- DOI:
- 10.3847/1538-3881/aa9921
- arXiv:
- arXiv:1709.10398
- Bibcode:
- 2018AJ....155...10C
- Keywords:
-
- planets and satellites: detection;
- stars: individual: EPIC 247589423AB;
- K2-136A c;
- K2-136AB;
- Astrophysics - Earth and Planetary Astrophysics
- E-Print:
- 13 pages, 8 figures, 2 tables. Accepted to AAS Journals