词条 | Kepler-41b |
释义 |
| name = Kepler-41b | discovered = July 29, 2011 | discovery_method = Transit | apsis = astron | semimajor = {{val|0.03101|0.0004}} AU | eccentricity = 0 (fixed) | period = {{val|1.85555820|0.00000052}} d | inclination = {{val|82.51|0.09}} | semi-amplitude = {{val|84|11}} | star = Kepler-41 | mean_radius = {{val|1.29|0.02}} {{Jupiter radius|link=y}} | mass = {{val|0.56|0.08}} {{Jupiter mass|link=y}} | density = {{val|0.33|0.04}} g cm−3 | albedo = 0.2 | single_temperature = {{val|1790|31}} }}Kepler-41b, formerly known as KOI-196b, is a planet in the orbit of star Kepler-41. It is a hot Jupiter with about the density of water. It reflects about a third of the starlight it receives.[8] References1. ^1 {{cite journal | title=SOPHIE velocimetry of Kepler transit candidates IV. KOI-196b: a non-inflated hot Jupiter with a high albedo | url=http://www.aanda.org/articles/aa/full_html/2011/12/aa17807-11/aa17807-11.html | last1=Santerne | first1=A. | last2=Bonomo | first2=A. S. | last3=Hébrard | first3=G. | last4=Deleuil | first4=M. | last5=Moutou | first5=C. | last6=Almenara | first6=J.-M. | last7=Bouchy | first7=F. | last8=Díaz | first8=R. F. | display-authors=1 | journal=Astronomy and Astrophysics | volume=536 | at=A70 | year=2011 | arxiv=1108.0550 | bibcode=2011A&A...536A..70S | doi=10.1051/0004-6361/201117807 }} [1]}}{{extrasolar-planet-stub}} 4 : Exoplanets discovered by Kepler (spacecraft)|Exoplanets discovered in 2011|Cygnus (constellation)|Giant planets |
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