exoplanet_descriptions/kepler-420_ab.txt Dahete'gebyu (Kepler-420 Ab) - Astro
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Info for exoplanet "Dahete'gebyu"


Scientific (actual) data
NameKepler-420 Ab
Planet statusConfirmed
Planet mass1.45
Radius0.94
Orbital period86.6477
Semi major axis0.382
Orbit eccentricity0.772
Inclination89.66
Discovered2014
Updated2024-07-28
Omega141.3
Tconj2455010
Tzero tr2455010
Lambda angle74
Temperature (kelvin)511
PublicationPublished in a refereed paper
Detection typePrimary Transit
Alternate namesKOI-1257 b, 2MASS J19245404+4455385 b, K01257.01, KIC 8751933 b, KOI-1257.01, WISE J192454.01+445538.5 b, KOI-1257 Ab, TIC 159647910 b
Star nameKepler-420 A
Right ascension291.23°
Declination44.93°
Mag j13.222
Mag h12.827
Star distance900
Star metallicity0.27
Star mass0.99
Star radius1.13
Star sp typeG5V
Star age9.3
Star temperature5520
Star alternate names2MASS J19245404+4455385, KIC 8751933, KOI-1257 A, WISE J192454.01+445538.5, KOI-1257, TIC 159647910
Wikipedia articleKepler-420 Ab

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Fictional info (?)
Suggested nameDahete'gebyu
Planet typeCold gas giant
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.

Having almost no atmosphere to retain heat, it has surface temperatures that vary diurnally more than on any other planet in its solar system, ranging from 105°K (-168°C) at night to 350°K (77°C) during the day across the equatorial regions.

It is radically different from Earth in other respects. The atmospheric pressure at the planet's surface is 80 bar, or roughly the pressure found 1080 m under the oceans of Earth.

Because of its fast rotation, the planet's shape is that of an oblate spheroid (it has a slight but noticeable bulge around the equator). The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries.

tricky voyage.
AtmosphereOzone64%
Oxygen21%
Krypton14%
Carbonyl sulfide0.031%
Atmospheric pressure80 bar
artist's rendition
No known satellites
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