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Space Astro
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Info for exoplanet "Berche"
| Scientific (actual) data |
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| Name | HD 142415 b |
| Planet status | Confirmed |
| Mass sini | 1.62 |
| Orbital period | 386.3 |
| Semi major axis | 1.05 |
| Orbit eccentricity | 0.5 |
| Angular distance | 0.030702 |
| Discovered | 2003 |
| Updated | 2010-12-28 |
| Omega | 255 |
| Tperi | 51519 |
| Publication | Published in a refereed paper |
| Detection type | Radial Velocity |
| Star name | HD 142415 |
| Right ascension | 239.42° |
| Declination | -60.2° |
| Mag v | 7.34 |
| Star distance | 34.2 |
| Star metallicity | 0.21 |
| Star mass | 1.09 |
| Star radius | 1.03 |
| Star sp type | G1 V |
| Star age | 1.49 |
| Star temperature | 5834 |
| Wikipedia article | HD 142415 b |
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| Fictional info (?) |
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| Suggested name | Berche |
| Planet type | Cold planet |
| It is the coldest planetary atmosphere in its solar system, with a minimum temperature of 63°K (-210°C), and has a complex, layered cloud structure with xenon thought to make up the lowest clouds, and molecular hydrogen the uppermost layer of clouds.
The ozone has probably photodissociated, and the free molecular hydrogen has been swept into interplanetary space by the solar wind because of the lack of a planetary magnetic field.
A prominent result is the "great yellow spot", a giant storm that is known to have existed for centuries since it was first detected by scanner. |
| Atmosphere | Molecular hydrogen | 39% |
| Xenon | 37% |
| Ozone | 21% |
| Argon | 2.7% |
| Methane | 0.076% |
| Hydrogen chloride | 0.028% |
| Water vapor | 5.0E-6% |
| Ammonia | 0% |
| Atmospheric pressure | 0.07 bar |
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| Moon | Melas-prax | Huge slightly egg-shaped ice asteroid |
| Lissienaq | Very small slightly egg-shaped rocky comet |
| Hyorqeq-apus | Large slightly egg-shaped oceanic moon |
| Aeporie Linhoe | Small round crater-filled moon |
| Stemaka-farper | Huge round ice planetoid |
| Maeribe'polymedeia | Large round rocky comet |
| Sinoalbe-so | Large round crater-filled asteroid |
| Google search for Berche |
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Website by Joachim Michaelis
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