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Space Astro
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Info for exoplanet "Tonix'cisco"
| Scientific (actual) data |
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| Name | TOI-2049 b |
| Planet status | Confirmed |
| Planet mass | 1.53 |
| Radius | 1.485 |
| Orbital period | 5.30347 |
| Semi major axis | 0.06919 |
| Orbit eccentricity | 0.054 |
| Inclination | 78.85 |
| Discovered | 2026 |
| Updated | 2026-07-05 |
| Omega | 39 |
| Tzero tr | 2458770 |
| Impact parameter | 0.88 |
| K | 130 |
| Temperature (kelvin) | 1869 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Mass measurement type | Radial Velocity |
| Radius measurement type | Primary Transit |
| Star name | TOI-2049 |
| Right ascension | 346.91° |
| Declination | 56.69° |
| Mag v | 11.4 |
| Star distance | 595 |
| Star metallicity | 0.31 |
| Star mass | 1.57 |
| Star radius | 3.2 |
| Star sp type | F8III-IV |
| Star age | 2.2 |
| Star temperature | 6164 |
| Star alternate names | TYC 4006-1797-1 |
| Wikipedia article | TOI-2049 b |
Back
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| Fictional info (?) |
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| Suggested name | Tonix'cisco |
| Planet type | Hot gas giant |
| The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to TOI-2049, which reoccurs over the so-called synodic period approximately every 174 days.
The methane has probably photodissociated, and the free krypton has been swept into interplanetary space by the solar wind because of the lack of a hydrogen peroxide layer.
Because of its fast rotation, the planet's shape is that of an oblate spheroid (it has a slight but noticeable bulge around the equator). |
| Atmosphere | Krypton | 51% |
| Argon | 47% |
| Methane | 1.4% |
| Hydrogen peroxide | 3.7E-5% |
| Atmospheric pressure | 1.5 bar |
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| No known satellites |
| Google search for Tonix'cisco |
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Website by Joachim Michaelis
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