WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY

WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY

We confirm the Kepler planet candidate Kepler-410A b (KOI-42b) as a Neptune-sized exoplanet on a 17.8 day, eccentric orbit around the bright (K p = 9.4) star Kepler-410A (KOI-42A). This is the third brightest confirmed planet host star in the Kepler field and one of the brightest hosts of all curren...

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Bibliographic Details
Main Authors: Van Eylen, V., Lund, Mikkel N., Aguirre, V. Silva, Arentoft, T., Kjeldsen, H., Albrecht, Simon H., Chaplin, William J., Isaacson, Howard, Pedersen, M. G., Jessen-Hansen, J., Tingley, B., Christensen-Dalsgaard, J., Aerts, C., Campante, T. L., Bryson, Stephen T.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Institute of Physics/American Astronomical Society 2015
Online Access:http://hdl.handle.net/1721.1/93250

Internet

http://hdl.handle.net/1721.1/93250

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