1108 Demeter
1108 Demeter, provisional designation, is a dark asteroid from the inner regions of the asteroid belt, approximately in diameter. It was discovered on 31 May 1929, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory near Heidelberg, Germany. The asteroid was named after Demeter, the Greek goddess of fruitful soil and agriculture. It has a rotation period of 9.846 hours.
Orbit and classification
Demeter is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. Based on osculating Keplerian orbital elements, it has also been classified as a member of the Phocaea family, a large family of stony asteroids, different to Demeter spectral type .It orbits the Sun in the inner main-belt at a distance of 1.8–3.1 AU once every 3 years and 9 months. Its orbit has an eccentricity of 0.26 and an inclination of 25° with respect to the ecliptic. The asteroid was first observed at the Italian Observatory of Turin, three days prior to its official discovery observation at Heidelberg. The body's observation arc begins at Yerkes Observatory in December 1930.
Physical characteristics
In the Tholen classification, Demeter spectral type is ambiguous, closest to a carbonaceous C-type and somewhat similar to an X-type asteroid.Rotation period
In June 2016, a rotational lightcurve of Demeter was obtained from photometric observations by American astronomers Tom Polakis and Brian Skiff at the Command Module Observatory in Tempe, Arizona. Lightcurve analysis gave a rotation period of 9.846 hours with an amplitude of 0.12 magnitude. Observations by the Spanish OBAS group, also taken during the 2016-opposition, gave a concurring period of 9.870 hours and a brightness variation of 0.11 magnitude. The results supersede previous observations by Robert Stephens, Olivier Thizy, René Roy and Stéphane Charbonnel from July 2001, which gave a period of 9.70 and 9.701 hours with an amplitude of 0.12 and 0.14 magnitude, respectively.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, Demeter measures between 25.285 and 31.33 kilometers in diameter and its surface has a low albedo between 0.0229 and 0.05.The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0464 and a diameter of 25.61 kilometers based on an absolute magnitude of 11.91.