2004 Lexell
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2004 Lexell, provisional designation Template:Mp, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7.5 kilometers in diameter. The asteroid was discovered on 22 September 1973, by Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula, and later named for Swedish-Russian astronomer and mathematician Anders Johan Lexell.[1][2]
Classification and orbit
Lexell is a member of the Flora family, one of the largest collisional populations of stony asteroids. It orbits the Sun at a distance of 2.0–2.3 AU once every 3 years and 2 months (1,169 days). Its orbit has an eccentricity of 0.08 and an inclination of 2° with respect to the ecliptic.[3]
The asteroid was first identified as Template:Mp at the Finnish Turku Observatory in November 1938, extending the body's observation arc by 35 years prior to its official discovery observation at Nauchnij.[2]
Physical characteristics
Pan-STARRSTemplate:' photometric survey characterized Lexell as a LS-type asteroid, which transitions between the common S-type and rare L-type asteroid.[4]
Rotation period
In March 2013, two rotational lightcurves of Lexell were obtained from photometric observations by Gary Haagen at Stonegate Observatory, Massachusetts, and by a group of astronomers at the Oakley Southern Sky Observatory (E09Script error: No such module "Check for unknown parameters".), Australia. Lightcurve analysis gave a well-defined rotation period of 5.441 and 5.4429 hours with a brightness variation of 0.45 and 0.42 magnitude, respectively (U=3/3Script error: No such module "Check for unknown parameters".).[5][6]
In February 2013, observations made by French amateur astronomer Pierre Antonini gave a concurring period of 5.44 hours with an amplitude of 0.51 magnitude (U=3-Script error: No such module "Check for unknown parameters".).[7]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lexell measures 7.255 and 7.456 kilometers in diameter and its surface has an albedo of 0.306 and 0.2908, respectively.[8][9] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 7.82 kilometers based on an absolute magnitude of 12.7.[10]
Naming
This minor planet was named after Anders Johan Lexell (1740–1784), a Swedish-Russian astronomer and mathematician. The official Template:MoMP was published by the Minor Planet Center on 15 October 1977 (M.P.C. 4238Script error: No such module "Check for unknown parameters".).[11] The lunar crater Lexell was also named in his honor, as is Lexell's Comet, of which he computed its orbit.[1]
References
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External links
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Template:AstDys
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