Dres - Galileo88/JNSQ GitHub Wiki
Pale, large, and seemingly unattractive, Dres hides in plain sight. It is the largest known body in the inner asteroid belt, measured by both radius and gravioli serving size. Dres has been observed enough to be confirmed as Mun-like in size and density, and also to be the loneliest world around, second to Hamek.
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Rational Resources Classification:
Ocean | Surface | Atmosphere | Exosphere |
---|---|---|---|
None | Rock-Ice | None | ExoRock |
From the PDF included in the download:
Bulk Params | Orbital and Rotational Params | ||
---|---|---|---|
Classification | Dwarf planet | Semi-major Axis | 112,687,000 km |
Radius | 360 km sea level, 361.6 km mean | Perihelion | 96,347,385 km |
Mass | 2.28515×1021 kg | Aphelion | 129,026,615 km |
Gravitational Parameter | 1.52513×1011 m3/s2 | Orbit eccentricity | 0.145 |
Mean density | 11,540 kg/m3 | Orbit inclination | 5° |
Surface gravity | 0.12 g ASL | Longitude of ascending node | 280° |
Escape velocity | 920 m/s | Argument of periapsis | 90° |
Bond Albedo | 0.2 | Sidereal orbit period | 5.2038 years |
Solar irradiance | 151 W/m2 | Synodic period | 451.83 days |
Black-body temperature | 152 K | Mean orbital velocity | 8,629 m/s |
Natural satellites | None | Sidereal rotation period | 4.5 hours |
Solar day | 4.5009 hours | ||
Synchronous orbit altitude | 645 km | ||
Sphere of influence | 90,298 km |