Damocloid family
The Damocloid family is an unusual collection of asteroids with
highly elliptical and, sometimes, highly inclined orbits that resemble those
of short-period comets. Because of this
similarity, it is thought that Damocloids may be the dark remains of old
comets. The prototype of the group, 5335 Damocles, was discovered in 1991
by Robert McNaught (1956–) at the Anglo-Australian Observatory and named
for a courtier of the ancient tyrant Dionysus I (The Elder) of Syracuse
who lived in the 4th century BC. Another suspected Damocloid, asteroid
2001 OG108, discovered in July 2001, has an orbit that takes it from just
inside Earth's orbit out as far as Uranus.
If its estimated diameter of 15 km is correct, this would make it one of
the biggest Earth-crossing asteroids known.
Data for 5335 Damocles | |
---|---|
diameter | 15 to 20 km |
semimajor axis | 11.88 AU |
perihelion | 1.58 AU |
aphelion | 22.18 AU |
inclination | 61.9° |
period | 40.6 years |