Phocaea group
A cluster of asteroids in the main asteroid
belt that were perturbed into high inclination (21 to 25°) orbits
by the gravitational effect of the major planets, notably Jupiter,
during the earliest period of solar system. The group is named after its
first discovered member, (25) Phocaea, found in 1853 by the French astronomer
Jean Chacornac (1823-1873), although its largest member is the C-class asteroid
(105) Artemis, with a diameter of 126 km. Most of the Phocaea group is a
ragbag assemblage of objects without a common ancestry; however, certain
members, including (323) Brucia, (852) Wladilena, and (1568) Aisleen, may
form a true Hirayama family.
| Data for Phocaea |
| diameter |
72 km |
| spectral class |
S |
| semimajor axis |
2.402 AU |
| perihelion |
1.79 AU |
| aphelion |
3.01 AU |
| inclination |
21.6° |
| period |
3.72 years |
Related category
ASTEROIDS
AND OTHER MINOR PLANETS: TYPES AND GROUPS
Also on this site: Encyclopedia
of Alternative Energy & Sustainable Living
Encyclopedia
of History
BACK TO TOP
|