1837 Osita
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1837 Osita ( ''prov. designation'': ) is a stony
Flora asteroid The Flora family (''adj. Florian''; ; also known as ''Ariadne family'') is a prominent family of stony asteroids located in the inner region of the asteroid belt. It is one of the largest families with more than 13,000 known members, or approxi ...
from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 16 August 1971, by American astronomer James Gibson at the Yale–Columbia Southern Station of the Leoncito Astronomical Complex in Argentina, who named it after his wife Ursula ("Osita").


Orbit and classification

The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the
inner Interior may refer to: Arts and media * ''Interior'' (Degas) (also known as ''The Rape''), painting by Edgar Degas * ''Interior'' (play), 1895 play by Belgian playwright Maurice Maeterlinck * ''The Interior'' (novel), by Lisa See * Interior de ...
main-belt at a distance of 2.0–2.4  AU once every 3 years and 3 months (1,196 days). Its orbit has an eccentricity of 0.09 and an inclination of 4 ° with respect to the ecliptic. ''Osita'' was first identified as at
Goethe Link Observatory The Goethe Link Observatory, observatory code 760, is an astronomical observatory near Brooklyn, Indiana, United States. It is owned by Indiana University and operated by the Indiana Astronomical Society https://iasindy.org/about.html, which eff ...
in 1962, extending the body's observation arc by 9 years prior to its official discovery observation.


Physical characteristics

PanSTARRSs large-scale survey also classified ''Osita'' as a rare AQ-type, having intermediate spectral characteristics of an A and Q type asteroid.


Rotation period

In February 2006, a rotational lightcurve of ''Osita'' was obtained from photometric observation by French amateur astronomer René Roy, giving a well-defined
rotation period The rotation period of a celestial object (e.g., star, gas giant, planet, moon, asteroid) may refer to its sidereal rotation period, i.e. the time that the object takes to complete a single revolution around its axis of rotation relative to the ...
of 3.81880 hours with a brightness variation of 0.48 magnitude (). Photometric observations in the R-band at the
Palomar Transient Factory The Palomar Transient Factory (PTF, obs. code: I41), was an astronomical survey using a wide-field survey camera designed to search for optical transient and variable sources such as variable stars, supernovae, asteroids and comets. The projec ...
in October 2011, gave a concurring period of 3.8186 hours and an amplitude of 0.59 magnitude (). A third period of 3.81880 hours was derived from a large international data-mining collaboration in February 2016 ().


Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, ''Osita'' measures between 7.53 and 7.94 kilometers in diameter, and its surface has an albedo between 0.194 and 0.216. The ''Collaborative Asteroid Lightcurve Link'' assumes an albedo of 0.24 – derived from
8 Flora Flora (minor planet designation: 8 Flora) is a large, bright main-belt asteroid. It is the innermost ''large'' asteroid: no asteroid closer to the Sun has a diameter above 25 kilometres (20% that of Flora), and not until 20-km 149 Medusa was dis ...
, the largest member and namesake of this orbital family – and calculates a diameter of 7.14 kilometers with an absolute magnitude of 12.9.


Naming

This minor planet was named by the discoverer for his wife Ursula ("Osita" is the Spanish equivalent). She volunteered as an assistant and actively participated in the observations by measuring or reducing more than 150 positions of comets and minor planets. The official was published by the
Minor Planet Center The Minor Planet Center (MPC) is the official body for observing and reporting on minor planets under the auspices of the International Astronomical Union (IAU). Founded in 1947, it operates at the Smithsonian Astrophysical Observatory. Function ...
on 20 February 1976 ().


References


External links


Asteroid Lightcurve Database (LCDB)
query form

)
Dictionary of Minor Planet Names
Google books

– Observatoire de Genève, Raoul Behrend

– Minor Planet Center * * {{DEFAULTSORT:Osita 001837 Discoveries by James B. Gibson (astronomer) Named minor planets 19710816