1067 Lunaria
1067 Lunaria, provisional designation, is a stony Itha asteroid from the outer regions of the asteroid belt, approximately 18 kilometers in diameter. It was discovered on 9 September 1926, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named after the flowering plant Lunaria.
Orbit and classification
Lunaria is a member of the Itha family, a very small family of asteroids, named after its parent body 918 Itha.It orbits the Sun in the outer asteroid belt at a distance of 2.3–3.4 AU once every 4 years and 10 months. Its orbit has an eccentricity of 0.19 and an inclination of 11° with respect to the ecliptic. The body's observation arc begins at Heidelberg in October 1926, one month after its official discovery observation.
Physical characteristics
Lunaria has been characterized as both L- and S-type asteroid by Pan-STARRS photometric survey. The overall spectral type for the Itha family is that of a stony S-type.Rotation period
In July 1984, a first rotational lightcurve of Lunaria was obtained by American astronomer Richard Binzel. Lightcurve analysis gave a rotation period of 7.74 hours with a brightness variation of 0.13 magnitude. In September 2004, Donald Pray at the Carbuncle Hill Observatory derived a refined period of 6.057 hours with an amplitude of 0.27 magnitude from photometric observations.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, Lunaria measures between 15.43 and 22.968 kilometers in diameter and its surface has an albedo between 0.1240 and 0.298.The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 18.07 kilometers based on an absolute magnitude of 11.08.