Gingerich is an assumed carbonaceous
C-type asteroid.
Rotation period and suspected binary In 2007, a rotational
lightcurve of
Gingerich was obtained from
photometric observations by American astronomers at the
Calvin-Rehoboth Robotic Observatory in New Mexico. Lightcurve analysis gave a
rotation period of 2.9392 hours with a brightness amplitude of 0.39
magnitude (). Two years earlier, the same group of astronomers had already observed this object and noted a dip in brightness on the first night of observation. From this, the astronomers suspect the presence of a
minor-planet moon, as the depth and length of the decrease in brightness was typical for an eclipsing event seen among many other synchronous
binary asteroids. However, no orbital period for the satellite could be determined and its existence remains unconfirmed as of 2018.
Diameter and albedo According to the surveys carried out by the Japanese
Akari satellite and the
NEOWISE mission of NASA's
Wide-field Infrared Survey Explorer,
Gingerich measures between 11.808 and 13.24 kilometers in diameter and its surface has an
albedo between 0.111 and 0.139. The
Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 18.43 kilometers based on an
absolute magnitude of 12.4. == Naming ==