Английская Википедия:1379 Lomonosowa

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1379 Lomonosowa (prov. designation: Шаблон:Mp) is a stony background asteroid from the central regions of the asteroid belt, approximately Шаблон:Convert in diameter. Discovered by Grigory Neujmin at the Simeiz Observatory in 1936, the asteroid was later named after Russian physicist and astronomer Mikhail Lomonosov.[1][2]

Discovery

Lomonosowa was discovered on 19 March 1936, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula.[2] On the same night, it was independently discovered by Serbian astronomer Petar Đurković at Uccle Observatory in Belgium.[1] The Minor Planet Center only recognizes the first discoverer.[2] A first precovery of Lomonosowa was taken at the Lowell Observatory in October 1905. The asteroid was first identified as Шаблон:Mp at Heidelberg Observatory in September 1933.[2]

Orbit and classification

Lomonosowa is a non-family asteroid of the main belt's background population.[3] It orbits the Sun in the central asteroid belt at a distance of 2.3–2.8 AU once every 4.01 years (1,464 days). Its orbit has an eccentricity of 0.09 and an inclination of 16° with respect to the ecliptic.[4] The body's observation arc begins with its first precovery at Lowell Observatory in October 1905.[2]

Naming

This minor planet was named after Russian physicist and astronomer Mikhail Lomonosov (1711–1765). He discovered the atmosphere of Venus and the principle of mass conservation.[1] The official Шаблон:MoMP was published by the Minor Planet Center in June 1955 (Шаблон:Small).[5] He is also honored by the craters Lomonosov on the Moon and Lomonosov on Mars.[1]

Physical characteristics

Lomonosowa has been characterized as a common, stony S-type asteroid.[6]

Lightcurves

Several rotational lightcurve of Lomonosowa have been obtained from photometric observations since the 1980s. Lightcurve analysis gave a rotation period between 24.482 and 24.71 hours with a brightness amplitude of 0.45 to 0.63 magnitude (Шаблон:Small).[7][8][6] The asteroid's lightcurve has also been modeled using photometric observations from various sources. Modelling gave a concurring sidereal period of 24.4845 and 24.4846 hours.[9][10] One study also found two spin axis of (72.0°, −84.0°) and (265.0°, −46.0°) in ecliptic coordinates (λ, β).[10]

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, Lomonosowa measures between 18.690 and 20.45 kilometers in diameter and its surface has an albedo between 0.1584 and 0.218.[11][12][13][14] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 17.82 kilometers based on an absolute magnitude of 11.11.[15]

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies

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