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Space Astro
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Info for exoplanet "Dilnar"
| Scientific (actual) data |
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| Planet | HD 94771 b |
| Planet status | Confirmed |
| Mass sini | 0.53 |
| Orbital period | 2164 |
| Semi major axis | 3.48 |
| Orbit eccentricity | 0.39 |
| Discovered | 2022 |
| Updated | 2023-06-15 |
| Omega | 90 |
| Tperi | 2455480 |
| K | 8 |
| Publication | Published in a refereed paper |
| Detection type | Radial Velocity |
| Mass detection type | Radial Velocity |
| Star name | HD 94771 |
| Right ascension | 163.98° |
| Declination | -35.11° |
| Mag v | 7.4 |
| Star distance | 57.618 |
| Star metallicity | 0.22 |
| Star mass | 1.2 |
| Star radius | 1.903 |
| Star sp type | G3/5V |
| Star age | 5.733 |
| Star temperature | 5631 |
| Wikipedia article | HD 94771 b |
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| Fictional info (?) |
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| Suggested name | Dilnar |
| Planet type | Cold planet |
| Dilnar is the fourth planet from HD 94771 and the second-smallest planet in its solar system. Orbiting within Paldelia's orbit, Dilnar is an inferior planet and never appears to venture far from HD 94771; its maximum angular distance from HD 94771 (elongation) is 72 degrees.
It is named after the deity Dilnar, the god of hate.
The planet telescopically displays the complete range of phases, similar to Venus and the Moon, as it moves in its inner orbit relative to HD 94771, which reoccurs over the so-called synodic period approximately every 110 days.
An observer on Dilnar would therefore see only one day every five years.
Dilnar is by far the hottest planet in its solar system, with a mean surface temperature of 566°K (293°C).
In November 2600, NASA reported finding a large amount of underground ice in the Utopia Planitia region of Dilnar.
Dilnar can easily be seen from Paldelia with the naked eye, as can its greenish coloring. |
| Atmosphere | Xenon | 54% |
| Nitric oxide | 37% |
| Hydrogen peroxide | 8.7% |
| Helium | 0.095% |
| Neon | 0.077% |
| Atmospheric pressure | 30 bar |
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| No known satellites |
| Google search for Dilnar |
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Website by Joachim Michaelis
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