In the
Tholen classification, Agamemnon is a dark
D-type asteroid. It has also been characterized as a D-type in both the Tholen- and SMASS-like taxonomy of the
Small Solar System Objects Spectroscopic Survey (S3OS2).
Rotation period Photometric observations of this asteroid during 1997 were used to build a
lightcurve showing a
rotation period of hours with a brightness variation of
magnitude. A 2009 study yielded a period of hours, in reasonable agreement with the previous result.
Diameter and albedo According to the surveys carried out by the Infrared Astronomical Satellite
IRAS, the Japanese
Akari satellite and the
NEOWISE mission of NASA's
Wide-field Infrared Survey Explorer, Agamemnon measures between 131.04 and 185.30 kilometers in diameter, based on a common
absolute magnitude of 7.89 and a surface
albedo between 0.037 and 0.072. A concurring diameter estimate of kilometers from an occultation event
(see below) has also been obtained. The
Collaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS, that is, an albedo of 0.0444 and a diameter of 166.66 kilometers based on an
absolute magnitude of 7.89.
Shape and satellite A 2012 stellar
occultation produced a 2D shape model of roughly (with an irregular, skewed outline) and strong evidence of Agamemnon having a
satellite of approximately kilometers in diameter orbiting at from the primary's center. == Naming ==