Characterizing K2 Planet Discoveries: A super-Earth transiting the bright K-dwarf HIP 116454

Autor(en)

Andrew Vanderburg, Benjamin T. Montet, John Asher Johnson, L. A. Buchhave, Li Zeng, Rainer Kuschnig, Werner Wolfgang Weiss

Abstrakt

We report the first planet discovery from the two-wheeled Kepler (K2) mission: HIP 116454 b. The host star HIP 116454 is a bright (V = 10.1, K = 8.0) K1 dwarf with high proper motion and a parallax-based distance of 55.2 ± 5.4 pc. Based on high-resolution optical spectroscopy, we find that the host star is metal-poor with [Fe/H] = -0.16 ± 0.08 and has a radius R∗= 0.716 ± 0.024 R

_⊙ and mass M∗= 0.775 ± 0.027 M

_⊙. The star was observed by the Kepler spacecraft during its Two-Wheeled Concept Engineering Test in 2014 February. During the 9 days of observations, K2 observed a single transit event. Using a new K2 photometric analysis technique, we are able to correct small telescope drifts and recover the observed transit at high confidence, corresponding to a planetary radius of R

_p = 2.53 ± 0.18 R

_⊕. Radial velocity observations with the HARPS-N spectrograph reveal a 11.82 ± 1.33 M

_⊕ planet in a 9.1 day orbit, consistent with the transit depth, duration, and ephemeris. Follow-up photometric measurements from the MOST satellite confirm the transit observed in the K2 photometry and provide a refined ephemeris, making HIP 116454 b amenable for future follow-up observations of this latest addition to the growing population of transiting super-Earths around nearby, bright stars.

Organisation(en)

Institut für Astrophysik

Externe Organisation(en)

Harvard-Smithsonian Center for Astrophysics, National Science Foundation, California Institute of Technology (Caltech), Natural History Museum of Denmark

Journal

The Astrophysical Journal

Band

800

ISSN

0004-637X

DOI

https://doi.org/10.1088/0004-637X/800/1/59

Publikationsdatum

2015

Peer-reviewed

Ja

ÖFOS 2012

103003 Astronomie, 103004 Astrophysik

Schlagwörter

ASJC Scopus Sachgebiete

Astronomy and Astrophysics, Space and Planetary Science

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/2f499565-01ee-44c3-b0c7-f12006c2bed1