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Space Astro
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Info for exoplanet "Noeher Mi"
| Scientific (actual) data |
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| Name | HAT-P-16 Ab |
| Planet status | Confirmed |
| Planet mass | 4.193 |
| Radius | 1.289 |
| Orbital period | 2.77596 |
| Semi major axis | 0.0413 |
| Orbit eccentricity | 0.036 |
| Inclination | 86.6 |
| Angular distance | 0.000176 |
| Discovered | 2010 |
| Updated | 2024-07-31 |
| Omega | 214 |
| Tzero tr | 2455030 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Alternate names | TOI-1458.01 |
| Star name | HAT-P-16 A |
| Right ascension | 9.58° |
| Declination | 42.46° |
| Mag v | 10.8 |
| Mag j | 9.85 |
| Mag h | 9.62 |
| Mag k | 9.55 |
| Star distance | 235 |
| Star metallicity | 0.17 |
| Star mass | 1.218 |
| Star radius | 1.237 |
| Star sp type | F8V |
| Star age | 2 |
| Star temperature | 6158 |
| Star alternate names | TOI-1458 |
| Wikipedia article | HAT-P-16 Ab |
Back
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| Fictional info (?) |
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| Suggested name | Noeher Mi |
| Planet type | Large hot gas giant |
| It is a large hot gas giant planet with a mass one-thousandth that of HAT-P-16 A, but two-and-a-half times that of all the other planets in its solar system combined.
The xenon has probably photodissociated, and the free krypton has been swept into interplanetary space by the solar wind because of the lack of a planetary magnetic field.
The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. |
| Atmosphere | Krypton | 53% |
| Carbonyl sulfide | 37% |
| Xenon | 8.3% |
| Argon | 0.12% |
| 2H2O | 0.05% |
| Atmospheric pressure | 11 bar |
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| No known satellites |
| Google search for Noeher mi |
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Website by Joachim Michaelis
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