5335 Damocles

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5335 Damocles
Discovery A
Discoverer Robert H. McNaught
Discovery date February 18, 1991
Alternate
designations
B
1991 DA
Category Damocloid
Orbital elements C
Epoch January 1, 2006 (JD 2453736.5 )
Eccentricity (e) 0.87
Semi-major axis (a) 11.84 AU
Perihelion (q) 1.58 AU
Aphelion (Q) 22.10 AU
Orbital period (P) 14880.90 d, 40.74 a
Mean orbital speed 6.67 km/s
Inclination (i) 61.95 °
Longitude of the
ascending node
(Ω)
.02°
Argument of
perihelion
(ω)
191.25°
Mean anomaly (M) 133.07°
Physical characteristics D
Dimensions ~ 10 km
Mass
Density
Surface gravity
Escape velocity
Rotation period 10.2 h
Spectral class S
Absolute magnitude 13.3
Albedo (geometric)
Mean surface
temperature
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5335 Damocles is the archetype of the Damocloids, asteroids that are inactive nuclei of Halley Family and long period comets. It was discovered in 1991 and named after Damocles, a figure of Greek legend.

When Damocles was discovered, in 1991 by Robert H. McNaught, it was found to be on an orbit completely different from all others known. Damocles' orbit reached from inside the aphelion of Mars to as far as Uranus. It seemed to be in transition from a near-circular outer solar system orbit to an eccentric orbit taking it to the inner solar system. [1] Duncan Steel, Gerhard Hahn, Mark Bailey, and David Asher carried out projections of its long term dynamical evolution, and found a good probability that it will become an Earth-crosser asteroid, and may spend a quarter of its life in such an orbit. Damocles will have a stable orbit for tens of thousands or years before and after the present, because its highly inclined orbit does not take it near Jupiter or Saturn.

There is some speculation[[1]] that 5335 Damocles may have a meteor shower associated with it on Mars from the direction of Draco.


  1. ^ Steel, D. "Rogue Asteroids and Doomsday Comets", page 127-8. Wiley & Sons, 1995






See also: List of asteroids

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