Revision for Miller Mann | ||
Previous Revision, by WhirlWind [2022-08-28 02:25:23] | → | Selected revision, by WhirlWind [2022-08-28 02:33:38] |
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 | ||
The closest Atmospheric Land-able Body orbiting a Black Hole. | → | Miller Mann has the closest orbit to a Black Hole of any Atmospheric Land-able body discovered. |
DESCRIPTION | ||
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Named after two planets in the movie Interstellar 2014, Miller Mann has the closest orbit to a Black Hole of any Atmospheric Land-able body discovered. 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. | → |
Named after two planets in the movie Interstellar 2014, Miller Mann has the closest orbit to a Black Hole of any Atmospheric Land-able body discovered. 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. |
JOURNAL | ||
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OBSERVATORY | ||
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