1078 Mentha
1078 Mentha, provisional designation, is a stony background asteroid from the inner regions of the asteroid belt, approximately 13 kilometers in diameter. It was discovered on 7 December 1926, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. Only in 1958, it was realized that this object was a rediscovery of an already numbered but lost asteroid.
The asteroid was named after the flowering plant of the mint family, Mentha. It has a longer-than average spin rate of 85 hours and possibly an irregular, elongated shape.
Identification with former lost asteroid
Sometimes, discovered objects turn out to be a rediscovery of a previously lost minor planet. This can be determined by calculating the "new" object's orbit backwards and checking its past positions against those previously recorded for the lost object. Nowadays these identities between two objects are found before they are numbered.In 1958, however, French astronomer André Patry at Nice Observatory found such identity between Mentha,, and the lost minor planet 864 Aase,, which had never been re-observed after its discovery by Max Wolf in 1917. Since it was realized that Mentha and Aase were one and the same object, the Minor Planet Center resolved this conflict by keeping everything associated with "1078 Mentha", adding the two oppositional observations by Max Wolf from 1917, and completely vacated "864 Aase", reusing its name and number for another, unrelated discovery made by Reinmuth.
Orbit and classification
Mentha is a non-family asteroid of the main belt's background population. It orbits the Sun in the inner asteroid belt at a distance of 2.0–2.6 AU once every 3 years and 5 months. Its orbit has an eccentricity of 0.14 and an inclination of 7° with respect to the ecliptic.The asteroid was first observed as at Heidelberg in February 1907. The body's observation arc begins at Simeiz Observatory in March 1924, almost four years prior to its official discovery observation at Heidelberg.
Physical characteristics
In the Tholen classification, Mentha is a common stony S-type asteroid.Rotation period
In February 1989, a first rotational lightcurve of Mentha was obtained from photometric observations by Polish astronomer Wiesław Wiśniewski. Lightcurve analysis gave a well-defined rotation period of 85 hours with a brightness variation of 0.87 magnitude. In February 2013, a similar period of 82.870 hours with an amplitude of 0.65 magnitude was measured by astronomers at the Palomar Transient Factory in California. A high brightness amplitude is typically indicative for an elongated rather than spherical shape. Its long period is close to that of slow rotators.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, Mentha measures between 9.94 and 15.37 kilometers in diameter and its surface has an albedo between 0.126 and 0.343.The Collaborative Asteroid Lightcurve Link agrees with Petr Pravec's revised WISE data and takes an albedo of 0.1641 and a diameter of 13.68 kilometers based on an absolute magnitude of 11.9.