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Space Astro
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Info for exoplanet "Thaeu Lamona"
Scientific (actual) data |
Planet | Kepler-552 b |
Planet status | Confirmed |
Radius | 0.352 |
Orbital period | 5.26342 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2455010 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19225944+4814312 b, K00432.01, KIC 10858832 b, KOI-432 b, KOI-432.01, WISE J192259.44+481431.1 b |
Star name | Kepler-552 |
Right ascension | 290.75° |
Declination | 48.24° |
Mag j | 13.198 |
Mag h | 12.877 |
Mag k | 12.78 |
Star distance | 834 |
Star metallicity | 0.01 |
Star mass | 1.03 |
Star radius | 1.04 |
Star age | 3.89 |
Star temperature | 5863 |
Star alternate names | 2MASS J19225944+4814312, KIC 10858832, KOI-432, WISE J192259.44+481431.1 |
Wikipedia article | Kepler-552 b |
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Fictional info (?) |
Suggested name | Thaeu Lamona |
Planet type | Cold planet |
The planet is named after the deity Thaeu Lamona, the messenger of destruction.
Thaeu Lamona is by far the hottest planet in its solar system, with a mean surface temperature of 653°K (380°C).
The rotational period and seasonal cycles of Thaeu Lamona are likewise similar to those of Saobiha Cisco, as is the tilt that produces the seasons.
Its apparent magnitude reaches -3, which is surpassed only by Saobiha Cisco, Lire, and Kepler-552.
In late February 1800, Thaeu Lamona was visited by the New Horizons probe, which used Thaeu Lamona's gravity to increase its speed and bend its trajectory en route to Saobiha Cisco. |
Atmosphere | Sulfur dioxide | 42% |
Xenon | 35% |
Carbon monoxide | 22% |
Molecular hydrogen | 0.049% |
Hydrogen peroxide | 0.0036% |
Hydrogen chloride | 0.00025% |
Atmospheric pressure | 80 bar |
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Moon | Galaa Noehy-psa | Large potato shaped ice moon |
Qeqthel Ga | Huge round rocky moon |
Lahionn Har | Huge round gaseous asteroid |
Google search for Thaeu lamona |
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Website by Joachim Michaelis
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