exoplanet_descriptions/kepler-1201_b.txt Shura Hyobu-byo (Kepler-1201 b)
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Info for exoplanet "Shura Hyobu-byo"


Scientific (actual) data
NameKepler-1201 b
Planet statusConfirmed
Radius0.204
Orbital period15.1873
Discovered2016
Updated2021-02-05
Tconj2454970
PublicationAnnounced on a website
Detection typePrimary Transit
Alternate names2MASS J19382755+4049594 b, K02345.01, KIC 5629538 b, KOI-2345 b, KOI-2345.01, WISE J193827.55+404959.0 b
Star nameKepler-1201
Right ascension294.62°
Declination40.83°
Mag j13.562
Mag h13.265
Mag k13.157
Star distance1202
Star metallicity0.03
Star mass1.15
Star radius1.24
Star age2.95
Star temperature6177
Star alternate names2MASS J19382755+4049594, KIC 5629538, KOI-2345, WISE J193827.55+404959.0
Wikipedia articleKepler-1201 b

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Fictional info (?)
Suggested nameShura Hyobu-byo
Planet typeCold planet
It has the longest rotation period (445 days) of any planet in its solar system and rotates in the opposite direction to most other planets.

The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to Kepler-1201, which reoccurs over the so-called synodic period approximately every 110 days.

The molecular hydrogen has probably photodissociated, and the free water vapor has been swept into interplanetary space by the solar wind because of the lack of a 2H2O layer.

Its north and south poles, therefore, lie where most other planets have their equators.
AtmosphereWater vapor51%
Argon31%
Molecular hydrogen9.6%
2H2O5.8%
Ethane2%
Sulfur dioxide2.0E-6%
Atmospheric pressure90 bar
artist's rendition
No known satellites
Google search for Shura hyobu-byo


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