Amor group
Also known as Earth-grazing asteroids, one of three groups
of near-Earth asteroids. The
orbits of Amor asteroids have perihelia
between 1.017 AU (Earth's aphelion distance) and 1.3 AU (Mars' perihelion
distance). The prototype of the group is the one-km-wide (1221) Amor, discovered
in 1932 by Eugène Delaporte. The largest members are (1036) Ganymed,
with a diameter of 40 km, and (433) Eros.
About 1,500 Amors have been catalogued.
Amor asteroids vary widely in composition, which indicates they have come
from different parts of the main asteroid belt
and have been perturbed into their present orbits by either Jupiter
or Mars. Close approaches to Earth and Mars
can further alter their paths so that they temporarily become Earth-crossing
Apollo group asteroids. About one in ten
Amors will cross Earth's orbit in the course of a few hundred to a few thousand
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
|