Ra-Shalom has been characterized as a
C-type and
X-type asteroid on the
Tholen and
SMASS taxonomic scheme, respectively. It has also been characterized as a
K-type asteroid. In 1981, the asteroid was detected using radar, revealing a relatively smooth surface at decimeter scales.
Rotation period based 3D-model of
Ra-Shalom In August 2016, a rotational
lightcurve of
Ra-Shalom was obtained from photometric observations by American astronomer
Brian Warner. Lightcurve analysis gave a well-defined
rotation period of 19.89 hours with a brightness amplitude of 0.55
magnitude (). A large number of previous photometric observations gave a period between 19.79 and 19.8201 hours with a brightness amplitude between 0.3 and 0.41
magnitude.
Diameter and albedo According to
Spitzer Space Telescope's ExploreNEOs survey, the Japanese
Akari satellite, and NASA's
Keck Observatory,
Ra-Shalom measures between 1.98 and 2.79 kilometers in diameter and its surface has an
albedo between 0.080 and 0.177. The
Collaborative Asteroid Lightcurve Link adopts an albedo of 0.082 and a diameter of 2.78 kilometers with an
absolute magnitude of 16.054. == Notes ==