42355 Typhon
From Wikipedia, the free encyclopedia
Discovery A | |
---|---|
Discoverer | NEAT |
Discovery date | February 5, 2002 |
Alternate designations B |
2002 CR46 |
Category | centaur[1] |
Orbital elements C | |
|
|
Eccentricity (e) | 0.5407609 |
Semi-major axis (a) | 38.162506 AU |
Perihelion (q) | 17.525714 AU |
Aphelion (Q) | 58.799297 AU |
Orbital period (P) | |
Mean orbital speed | ? |
Inclination (i) | 2.4280935° |
Longitude of the ascending node (Ω) |
351.9923803° |
Argument of perihelion (ω) |
159.0020803° |
Mean anomaly (M) | 359.6998644° |
Physical characteristics D | |
Dimensions | 134±13 km |
Mass | ? |
Density | ? |
Surface gravity | ? |
Escape velocity | ? |
Rotation period | ? |
Spectral class | B-V=0.74±0.02 V-R=0.52±0.01 |
Absolute magnitude | 7.65±0.01 |
Albedo (geometric) | 0.10±0.02 |
Mean surface temperature |
? |
42355 Typhon (pronounced /ˈtaɪfɒn/, from Latin: Tȳphōn, Greek: Τυφών) is a centaur that was discovered on February 5, 2002 by the NEAT program. It is named after the monster of Greek myth, Typhon.
[edit] Echidna
Typhon has a single known satellite known as (42355) Typhon I Echidna (pronounced /ɪˈkɪdnə/, from Greek: Έχιδνα). It orbits its primary at ~1300 km, completing one orbit in about 11 days. It's diameter is estimated to be 78±8 km.