astro.wikisort.org - Asteroid787 Moskva is a minor planet orbiting the Sun. It is a dynamic member of the Maria asteroid family orbiting near the 3:1 Kirkwood gap.[4] This is an S-type (stony) asteroid spanning 27 km.[5] The surface mineralogy is consistent with mesosiderite silicates.[4]
787 Moskva A three-dimensional model of 787 Moskva based on its light curve |
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Discovered by | G. N. Neujmin |
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Discovery site | Simeis |
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Discovery date | 20 April 1914 |
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MPC designation | (787) Moskva |
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Pronunciation | [1] |
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Alternative designations | 1914 UQ |
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Epoch 31 July 2016 (JD 2457600.5) |
Uncertainty parameter 0 |
Observation arc | 100.47 yr (36695 d) |
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Aphelion | 2.8690 AU (429.20 Gm) |
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Perihelion | 2.2090 AU (330.46 Gm) |
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Semi-major axis | 2.5390 AU (379.83 Gm) |
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Eccentricity | 0.12996 |
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Orbital period (sidereal) | 4.05 yr (1477.7 d) |
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Mean anomaly | 18.5642° |
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Mean motion | 0° 14m 37.032s / day |
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Inclination | 14.852° |
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Longitude of ascending node | 183.890° |
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Argument of perihelion | 126.135° |
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Mean radius | 13.755±1.4 km |
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Synodic rotation period | 6.056 h (0.2523 d)[3][2] |
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Geometric albedo | 0.2559±0.062 |
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Absolute magnitude (H) | 9.7 |
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Object 1914 UQ, discovered 20 April 1914 by Grigory Neujmin, was named 787 Moskva, after the capital of Russia, Moscow (and retains that name to this day). Object 1934 FD discovered on 19 March 1934 by C. Jackson was given the sequence number 1317. In 1938, G. N. Neujmin found that asteroid 1317 and 787 Moskva were, in fact, the same object. Sequence number 1317 was later reused for the object 1935 RC discovered on 1 September 1935 by Karl Reinmuth; that object is now known as 1317 Silvretta.
Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado in 1999 were used to build a light curve for this object. The asteroid displayed a rotation period of 6.056 ± 0.001 hours and a brightness variation of 0.62 ± 0.01 in magnitude.[3]
References
- Noah Webster (1884) A Practical Dictionary of the English Language
- "787 Moskva (1914 UQ)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
- Warner, Brian D. (January 2011), "Upon Further Review: IV. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory", The Minor Planet Bulletin, vol. 38, no. 1, pp. 52–54, Bibcode:2011MPBu...38...52W.
- Fieber-Beyer, S. K.; Gaffey, M. J.; Kelley, M. S.; Reddy, V.; Reynolds, C. M.; Hicks, T. (2011), "The Maria asteroid family: Genetic relationships and a plausible source of mesosiderites near the 3: 1 Kirkwood Gap", Icarus, 213 (2): 524–537, Bibcode:2011Icar..213..524F, doi:10.1016/j.icarus.2011.03.009.
- Husárik, M., "CCD Photometry of Asteroids at the Skalnate Pleso Observatory and Shapes Modelling Methods." (PDF), In British/Czech and Slovak INYS workshop Many Faces of the Universe: From Solar System to Cosmology, pp. 30–1, retrieved 15 August 2021.
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На других языках
[de] (787) Moskva
(787) Moskva ist ein Asteroid des Hauptgürtels, der am 20. April 1914 vom russischen Astronom Grigori Nikolajewitsch Neuimin in Simejis entdeckt wurde.
- [en] 787 Moskva
[ru] (787) Москва
(787) Москва (лат. Moskva) — астероид из группы главного пояса, который входит в состав семейства Мария. Он был открыт 20 апреля 1914 года советским (в то время российским) астрономом Григорием Неуйминым в Симеизской обсерватории и назван в честь города Москвы[1].
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