Revision for Miller Mann
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| Previous Revision, by Richard Fluiraniz M. [2022-08-28 19:07:54] | → | Selected revision, by CMDR Marx [2022-08-28 19:54:17] |
| DISCOVERER |
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| NAME |
| Miller Mann | → | Miller Mann |
| SYSTEMNAME |
| Dryi Aug AA-A h283 | → | Dryi Aug AA-A h283 |
| CATEGORY |
| Stellar Features | → | Stellar Features |
| CATEGORY 2 |
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| REGION |
| Empyrean Straits | → | Empyrean Straits |
| LATITUDE |
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| LONGITUDE |
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| CALLSIGN |
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| SUMMARY |
| Miller Mann has the closest orbit to a Black Hole of any Atmospheric Landable body discovered. | → | Miller Mann has the closest orbit to a black hole of any thin atmospheric landable body discovered, as of 2022-08-28. |
| DESCRIPTION |
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Named after two planets in the movie Interstellar 2014, Miller Mann it's a planetary body like no other. Consisting of a Thin Helium atmosphere this land-able HMC orbits at only ~12Ls away from the Black Hole, with an orbital period of 4.9 hours. It also has three geological signals, one of which are Silicate Vapor Geysers.
Even at these close distances the gravitational lensing isn't visible, however two of the other black holes in system are enough to produce distortion even at ~220Ls which is visible form the surface of Miller Mann.
Miller Mann's system also contains three other black holes, four other stars, and a few other planets.
Both Y and T Class Brown Dwarfs have wide rings compared to body size. Black Holes C and B are in a tight orbit with an orbital period of 2.4 hours. Black Hole D orbits at ~19,000Ls.
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Miller Mann is a landable High Metal Content planet with a Thin Helium atmosphere that orbits a Black Hole only 12 ls away from the Black Hole, completing an orbit every 4.9 hours. It also has three geological signals, one of which are Silicate Vapour Geysers:
Even at these close distances the gravitational lensing of the parent black hole isn't visible. However, two of the other black holes in system are massive enough to produce distortion that's visible even at their distances of around 220 ls.
Miller Mann's system also contains three other black holes, four other stars, and a few other planets.
Both brown dwarfs (classes T and Y) have wide rings compared to body size. Black holes C and B are in a tight binary orbit with an orbital period of 2.4 hours around the barycenter. The fourth black hole (D) orbits at around 19,000 ls from the main star.
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| JOURNAL |
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| OBSERVATORY |
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