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Space Astro
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Info for exoplanet "Raose Pya"
Scientific (actual) data |
Planet | Kepler-155 c |
Planet status | Confirmed |
Radius | 0.2 |
Orbital period | 52.6618 |
Semi major axis | 0.242 |
Discovered | 2014 |
Updated | 2021-02-05 |
Tconj | 2455020 |
Impact parameter | 0.78 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19135899+5104550 c, K00438.02, KIC 12302530 c, KOI-438 c, KOI-438.02, WISE J191358.98+510454.5 c |
Star name | Kepler-155 |
Right ascension | 288.5° |
Declination | 51.08° |
Mag j | 12.533 |
Mag h | 11.888 |
Mag k | 11.805 |
Star distance | 295.99 |
Star metallicity | -0.363 |
Star mass | 0.58 |
Star radius | 0.62 |
Star sp type | M0 V |
Star temperature | 4508 |
Star alternate names | 2MASS J19135899+5104550, KIC 12302530, KOI-438, WISE J191358.98+510454.5 |
Wikipedia article | Kepler-155 c |
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Fictional info (?) |
Suggested name | Raose Pya |
Planet type | Cold planet |
It is a cold planet planet with a mass one-thousandth that of Kepler-155, but two-and-a-half times that of all the other planets in its solar system combined. This planet is named after the deity Raose Pya, the goddess of the underworld.
At this time it may appear as a bright star-like object, but is often far more difficult to observe than Kyomyo.
Raose Pya is gravitationally locked with Kepler-155 in a 2:1 spin-orbit resonance, and rotates in a way that is unique in its solar system.
Optical ground-based telescopes are typically limited to resolving features about 345 kilometers across when Raose Pya is closest because of Kyomyo's atmosphere.
It may also have a rocky core of heavier elements, but like the other cold planets, Raose Pya lacks a well-defined solid surface.
In 1589, images from Daedalus 5 showed Raose Pya as an almost featureless planet in visible light, without the cloud bands or storms associated with the other cold planets. |
Atmosphere | Formaldehyde | 84% |
Ethane | 12% |
Methane | 2.9% |
Atmospheric pressure | 0.001 bar |
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No known satellites |
Google search for Raose pya |
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Website by Joachim Michaelis
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