791 Ani

791 Ani ("prov. designation": "or" ) is a very large asteroid of the Meliboea family, located in the outer regions of the asteroid belt. It was discovered on 29 June 1914, by Russian astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula. The dark carbonaceous C-type asteroid has a rotation period of 11.2 hours and measures approximately kilometers, with a mean-diameter of . It was named after the historic Armenian city of Ani.
Orbit and classification.
When applying the hierarchical clustering method (HCM) to its proper orbital elements, "Ani" is a member of the Meliboea family (), a small family of carbonaceous asteroids in the outer main belt, named after its principal body, 137 Meliboea. However, according to another HCM-analysis by Milani and Knežević (AstDyS), it is a background asteroid as this analysis does not recognize the Meliboea family. "Ani" orbits the Sun in the outer asteroid belt at a distance of 2.5–3.7 AU once every 5 years and 6 months (2,015 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.19 and an inclination of 16° with respect to the ecliptic. The body's observation arc begins at Algiers Observatory in North Africa on 6 December 1915, some 17 months after its official discovery observation at Simeiz Observatory.
Naming.
This minor planet was named after the medieval city of Ani, which was destroyed by an earthquake in 1319. The ruins of the former capital of the Armenian kingdom are located near the border to Armenia, in what is now Turkey. Ani was known as "the city of 1001 churches". The was also mentioned in "The Names of the Minor Planets" by Paul Herget in 1955 ().
Physical characteristics.
In the Tholen classification, "Ani" is a common, carbonaceous C-type asteroid. It is also a common C-type in the Tholen-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), while in the survey's SMASS-like taxonomic variant, the asteroid is a hydrated carbonaceous subtype (Ch).
Rotation period and poles.
In May 2018, a rotational lightcurve of "Ani" was obtained from photometric observations by American amateur astronomer Tom Polakis at the Command Module Observatory in Arizona . Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude ().
In June 2002, Brian Warner at his Palmer Divide Observatory first observed this asteroid and later derived a period of hours and an amplitude of magnitude, based on poor data (). In December 2004, and in May 2007, two periods of and with a corresponding amplitude of and magnitude were determined by European astronomers Raymond Poncy as well as Yves Revaz, Raoul Behrend, Alain Klotz, Michel Hernandez, Robert Soubie, Jean-François Gauthier, Bernard Tregon, Pierre Antonini, Laurent Bernasconi, Federico Manzini , Yassine Damerdji and Horacio Correia. The two periods are slightly longer than twice Polakis period solution (). In April 2007, astronomers at the Oakley Observatory , Indiana, obtained a period of hours and an amplitude of magnitude (). In February 2011, French amateur astronomer René Roy determined a period of hours and a brightness variation of magnitude ().
A modeled lightcurve by Josef Ďurech and Josef Hanuš, using photometric data including from the "Lowell Photometric Database" and from the Wide-field Infrared Survey Explorer (WISE) was published in 2018. It gave a sidereal period of and two spin axes at (94.0°, −25.0°) and (269.0°, 4.0°) in ecliptic coordinates (λ, β).
Diameter and albedo.
According to the surveys carried out by the Japanese Akari satellite, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), and the Infrared Astronomical Satellite IRAS, "Ani" measures (), () and () kilometers in diameter and its surface has an albedo of (), () and (), respectively. The "Collaborative Asteroid Lightcurve Link" adopts the results obtained by IRAS, that is, an albedo of 0.0329 and a diameter of 103.52 kilometers based on an absolute magnitude of 9.25. Alternative mean-diameter measurements published by the WISE team include (), (), () and () with corresponding albedos of (), (), () and (). On 7 April 2000, an asteroid occultation of "Ani" gave a best-fit ellipse dimension of () with a good quality rating of 3. These timed observations are taken when the asteroid passes in front of a distant star.