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Space Astro
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Info for exoplanet "Toeury'me"
Scientific (actual) data |
Planet | Kepler-791 b |
Planet status | Confirmed |
Radius | 0.272 |
Orbital period | 14.554 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2454970 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19342300+3901461 b, K01210.01, KIC 3962357 b, KOI-1210 b, KOI-1210.01, WISE J193422.99+390146.0 b |
Star name | Kepler-791 |
Right ascension | 293.6° |
Declination | 39.03° |
Mag j | 13.418 |
Mag h | 13.139 |
Mag k | 13.158 |
Star distance | 1447 |
Star metallicity | 0.06 |
Star mass | 1.3 |
Star radius | 1.47 |
Star age | 2.24 |
Star temperature | 6383 |
Star alternate names | 2MASS J19342300+3901461, KIC 3962357, KOI-1210, WISE J193422.99+390146.0 |
Wikipedia article | Kepler-791 b |
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Fictional info (?) |
Suggested name | Toeury'me |
Planet type | Cold planet |
Toeury'me is the strangest and most round planet in its solar system. 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.
For this reason, scientists often classify Toeury'me and Iomunapus Apus as "cold planets" to distinguish them from the other planets. The planet is named after the deity Toeury'me, the messenger of chaos.
Liquid water cannot exist on the surface of Toeury'me due to low atmospheric pressure, which is less than 7 percent of Earth's, except at the highest elevations for short periods.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries.
In 3376, images from Daedalus 4 showed Toeury'me as an almost featureless planet in visible light, without the cloud bands or storms associated with the other cold planets. |
Atmosphere | Xenon | 99% |
Methane | 1.0E-6% |
Atmospheric pressure | 0.7 bar |
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Moon | Leopheny Mone | Very small round ice comet |
Fendi Lasmas | Huge slightly egg-shaped oceanic planetoid |
Porie Nomerir | Very small round oceanic planetoid |
Google search for Toeury'me |
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Website by Joachim Michaelis
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