1200 Imperatrix
1200 Imperatrix is a carbonaceous Hygiean asteroid from the outer regions of the asteroid belt, approximately in diameter. It was discovered by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory on 14 September 1931. The asteroid was named after the Latin word for empress.
Orbit and classification
Imperatrix is a member of the Hygiea family, a very large asteroid family named after 10 Hygiea, the main belt's fourth-largest asteroid. 'mperatrix orbits the Sun in the outer main-belt at a distance of 2.7–3.4 AU once every 5 years and 4 months. Its orbit has an eccentricity of 0.11 and an inclination of 5° with respect to the ecliptic.The body's observation arc begins with its first identification as at Simeiz Observatory in March 1913, more than 18 years prior to its official discovery observation at Heidelberg.
Physical characteristics
Imperatrix is an assumed C-type asteroid which is also the overall spectral type of the Hygiea family.Rotation period
In August 2000, a rotational lightcurve of Imperatrix was obtained from photometric observations at the River Oaks Observatory in Texas. Lightcurve analysis gave a rotation period of 13.34 hours with a brightness variation of 0.23 magnitude. In September 2011, photometric observations by French amateur astronomers Pierre Antonini and René Roy gave a refined period of 17.769 hours with an amplitude of 0.21 magnitude.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, Imperatrix measures between 36.00 and 43.64 kilometers in diameter and its surface has an albedo between 0.04 and 0.0714.The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0545 and a diameter of 39.39 kilometers based on an absolute magnitude of 10.8.
Four stellar occultation events by 1200 Imperatrix have been observed, all in 2021.