Kepler-7b: a transiting planet with unusually low density

David W. Latham...[et al.], W.J. Borucki, D.G. Koch, Lars C. Astrup Buchhave

93 Citationer (Scopus)

Abstract

We report on the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, M P = 0.43 M J, but the radius is 50% larger, R P = 1.48 R J. The resulting density, ¿P = 0.17 g cm–3, is the second lowest reported so far for an extrasolar planet. The orbital period is fairly long, P = 4.886 days, and the host star is not much hotter than the Sun, T eff = 6000 K. However, it is more massive and considerably larger than the Sun, M = 1.35 M and R = 1.84 R , and must be near the end of its life on the main sequence
OriginalsprogEngelsk
TidsskriftThe Astrophysical Journal Letters
Vol/bind713
Udgave nummer2
Sider (fra-til)L140-L144
Antal sider4
ISSN0004-637X
DOI
StatusUdgivet - 20 apr. 2010

Fingeraftryk

Dyk ned i forskningsemnerne om 'Kepler-7b: a transiting planet with unusually low density'. Sammen danner de et unikt fingeraftryk.

Citationsformater