Dres - Galileo88/JNSQ GitHub Wiki

Dres

Description

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.

Trivia

?

RR

Rational Resources Classification:

Ocean Surface Atmosphere Exosphere
None Rock-Ice None ExoRock

Specs

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
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
⚠️ **GitHub.com Fallback** ⚠️