spinner
x
This website is using cookies, in order to track this cookie warning and other popups, for managing login sessions, and for website analytics. We do not collect or store personally identifiable information, nor track or display advertising related information. That's Fine
 - Galactic Exploration Catalog - 
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
NAME
Miller MannMiller Mann
SYSTEMNAME
Dryi Aug AA-A h283Dryi Aug AA-A h283
CATEGORY
Stellar FeaturesStellar Features
CATEGORY 2
REGION
Empyrean StraitsEmpyrean Straits
LATITUDE
LONGITUDE
CALLSIGN
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

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
OBSERVATORY
All content is licensed under Creative Commons (CC BY‑NC‑SA 3.0)

This website is not an official tool for the game Elite: Dangerous and is not affiliated with Frontier Developments. All information provided is based on publicly available information and data supplied by players, and may not be entirely accurate. 'Elite', the Elite logo, the Elite: Dangerous logo, 'Frontier' and the Frontier logo are registered trademarks of Frontier Developments plc. All rights reserved. All other trademarks and copyrights are acknowledged as the property of their respective owners.

Special thanks go to all commanders and explorers who graciously upload their data to EDDN, EDSM, and EDAstro to make all of this possible. We wouldn't exist without your data contributions. For any bug reports or feature suggestions, please visit our forum thread.