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'''Dres''' je pátá planeta<ref>According to the [[w:IAU definition of planet|IAU definition of planet]], | '''Dres''' je pátá planeta<ref>According to the [[w:IAU definition of planet|IAU definition of planet]], |
Revision as of 02:59, 25 December 2014
Dres | ||
Dres as seen from orbit. | ||
Dwarf planet of Kerbol | ||
Orbital Characteristics | ||
Semi-major axis | 40 839 348 203 m [Note 1] | |
Apoapsis | 46 761 053 692 m [Note 1] | |
Periapsis | 34 917 642 714 m [Note 1] | |
Orbital eccentricity | 0.145 | |
Orbital inclination | 5 ° | |
Argument of periapsis | 90 ° | |
Longitude of the ascending node | 280 ° | |
Mean anomaly | 3.14 rad (at 0s UT) | |
Sidereal orbital period | 47 893 063 s | |
2 217 d 1 h 37 m 43.1 s | ||
Synodic orbital period | 11 392 903,3 s | |
Orbital velocity | 4 630 - 6 200 m/s | |
Physical Characteristics | ||
Equatorial radius | 138 000 m | |
Equatorial circumference | 867 080 m | |
Surface area | 2,3931396×1011 m2 | |
Mass | 3,2190937×1020 kg | |
Standard gravitational parameter | 2,1484489×1010 m3/s2 | |
Density | 29 242,045 kg/m3 | |
Surface gravity | 1,13 m/s2 (0.115 g) | |
Escape velocity | 558,00 m/s | |
Sidereal rotation period | 34 800,000 s | |
1 d 3 h 40 m 0 s | ||
Solar day | 34 825,305 s | |
1 d 3 h 40 m 25.3 s | ||
Sidereal rotational velocity | 24,916 m/s | |
Synchronous orbit | 732,24 km | |
Sphere of influence | 32 832 840 m [Note 1] | |
Atmospheric Characteristics | ||
Atmosphere present | No | |
Scientific multiplier | ||
Surface | 8 | |
Splashed | N/A | |
Near space | 7 | |
Outer space | 6 | |
Recovery | 6 | |
|
Dres je pátá planeta[1] Kerbolího systému. Nachází se mezi Dunou a Joolem na jakési nakloněné a excentrické orbitě. Má to být herní analog pro Ceres. It is similar to Moho and Eeloo in that it has no atmosphere and no natural satellites. Dres has the least gravity of any planet in the Kerbol system. While it is classified as a dwarf planet by the developers, it currently meets the I.A.U.'s definition of a planet.
Geography
The surface of Dres appears light grey and is rocky and uneven, similar to that of Mün, with a surface covered in regolith rubble. Unlike the Mun, Dres has large patches of what appear to be ice. The highest points are just under 5.7 km in altitude. One notable geographic feature is a canyon just south of the equator which is several kilometers deep.
Reference Frames
Time warp | Minimum Altitude |
---|---|
1× | Any |
5× | 10 000 m |
10× | 10 000 m |
50× | 30 000 m |
100× | 50 000 m |
1 000× | 100 000 m |
10 000× | 200 000 m |
100 000× | 300 000 m |
Gallery
A topographical projection map of Dres, accurate as of 0.18.
A topographic height map of Dres as of version 0.18.1 made with the ISA MapSat plugin.
Changes
- Initial Release
Notes
- ↑ According to the IAU definition of planet,
Planeta je kosmické těleso, které:
- obíhá po oběžné dráze Slunce,
- Má určitou hmotnost pro dosažení hydrostatické rovnováhy (přibližně kulatý tvar),
- "Vyčistilo okolí" okolo své oběžné dráhy.
Kosmické těleso Dres obíhá hvězdu Kerbol, has a nearly spherical shape, and has cleared its neighborhood of debris. It is most likely defined as a dwarf planet by the developers as an asteroid belt near Dres will be developed in later versions.