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Space Astro
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Info for exoplanet "Duspa"
| Scientific (actual) data |
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| Planet | HAT-P-13 b |
| Planet status | Confirmed |
| Planet mass | 0.85 |
| Radius | 1.28 |
| Orbital period | 2.91624 |
| Semi major axis | 0.0426 |
| Orbit eccentricity | 0.0142 |
| Inclination | 83.3 |
| Angular distance | 0.000199 |
| Discovered | 2009 |
| Updated | 2017-01-05 |
| Omega | 223 |
| Tzero tr | 2455180 |
| Tzero tr sec | 2454780 |
| Publication | Published in a refereed paper |
| Detection type | Primary Transit |
| Star name | HAT-P-13 |
| Right ascension | 129.88° |
| Declination | 47.35° |
| Mag v | 10.62 |
| Star distance | 214 |
| Star metallicity | 0.43 |
| Star mass | 1.22 |
| Star radius | 1.56 |
| Star sp type | G4 |
| Star age | 5 |
| Star temperature | 5638 |
| Wikipedia article | HAT-P-13 b |
Back
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| Fictional info (?) |
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| Suggested name | Duspa |
| Planet type | Hot gas giant |
| Orbiting within Tianomia's orbit, Duspa is an inferior planet and never appears to venture far from HAT-P-13; its maximum angular distance from HAT-P-13 (elongation) is 70 degrees.
The planet is named after the deity Duspa, the bringer of the sky.
As seen from HAT-P-13, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two years.
Duspa's hazy clouds render observation of its surface difficult in ultraviolet light, and the first detailed maps did not emerge until the arrival of the Magellan orbiter 28 years ago. |
| Atmosphere | Ozone | 24% |
| Ethane | 23% |
| Molecular hydrogen | 19% |
| Argon | 14% |
| Formaldehyde | 6.8% |
| Hydrogen chloride | 5.9% |
| Methane | 4.7% |
| Krypton | 1.5% |
| Xenon | 0.22% |
| Carbonyl sulfide | 0.00086% |
| Hydrogen deuteride (HD) | 0% |
| Atmospheric pressure | 0.28 bar |
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| No known satellites |
| Google search for Duspa |
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Website by Joachim Michaelis
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