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F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
1379 Lomonosowa (prov. designation : 1936 FC ) is a stony background asteroid from the central regions of the asteroid belt , approximately 19 kilometers (12 miles) in diameter. Discovered by Grigory Neujmin at the Simeiz Observatory in 1936, the asteroid was later named after Russian physicist and astronomer Mikhail Lomonosov .[2] [15]
Discovery
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Lomonosowa was discovered on 19 March 1936, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula.[15] On the same night, it was independently discovered by Serbian astronomer Petar Đurković at Uccle Observatory in Belgium.[2] The Minor Planet Center only recognizes the first discoverer.[15] A first precovery of Lomonosowa was taken at the Lowell Observatory in October 1905. The asteroid was first identified as 1933 SG1 at Heidelberg Observatory in September 1933.[15]
Orbit and classification
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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 .[1] The body's observation arc begins with its first precovery at Lowell Observatory in October 1905.[15]
Naming
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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 .[2] The official naming citation was published by the Minor Planet Center in June 1955 (M.P.C. 1252 ).[16] He is also honored by the craters Lomonosov on the Moon and Lomonosov on Mars.[2]
Physical characteristics
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Lomonosowa has been characterized as a common, stony S-type asteroid .[13]
Lightcurves
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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 (U=2/3/2 ).[9] [12] [13] 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.[10] [11] One study also found two spin axis of (72.0°, −84.0°) and (265.0°, −46.0°) in ecliptic coordinates (λ, β).[11]
Diameter and albedo
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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.[5] [6] [7] [8] 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.[4]
References
[ edit ]
^ a b c d e Schmadel, Lutz D. (2007). "(1379) Lomonosowa". Dictionary of Minor Planet Names . Springer Berlin Heidelberg . p. 112 . doi :10.1007/978-3-540-29925-7_1380 . ISBN 978-3-540-00238-3 .
^ a b "Asteroid 1379 Lomonosowa – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019 .
^ a b c d e "LCDB Data for (1379) Lomonosowa" . Asteroid Lightcurve Database (LCDB). Retrieved 27 October 2017 .
^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos" . The Astrophysical Journal . 791 (2 ): 11. arXiv :1406.6645 . Bibcode :2014ApJ...791..121M . doi :10.1088/0004-637X/791/2/121 . Retrieved 27 October 2017 .
^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids" . The Astrophysical Journal Letters . 759 (1 ): 5. arXiv :1209.5794 . Bibcode :2012ApJ...759L...8M . doi :10.1088/2041-8205/759/1/L8 . Retrieved 27 October 2017 .
^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal . 741 (2 ): 25. arXiv :1109.6407 . Bibcode :2011ApJ...741...90M . doi :10.1088/0004-637X/741/2/90 .
^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan . 63 (5 ): 1117–1138. Bibcode :2011PASJ...63.1117U . doi :10.1093/pasj/63.5.1117 . (online , AcuA catalog p. 153 )
^ a b c Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry" . The Astronomical Journal . 150 (3 ): 35. arXiv :1504.04041 . Bibcode :2015AJ....150...75W . doi :10.1088/0004-6256/150/3/75 . Retrieved 27 October 2017 .
^ a b Hanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011). "A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method" . Astronomy & Astrophysics . 530 : 16. arXiv :1104.4114 . Bibcode :2011A&A...530A.134H . doi :10.1051/0004-6361/201116738 . Retrieved 27 October 2017 .
^ a b c Durech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016). "Asteroid models from the Lowell photometric database" . Astronomy and Astrophysics . 587 : 6. arXiv :1601.02909 . Bibcode :2016A&A...587A..48D . doi :10.1051/0004-6361/201527573 . Retrieved 27 October 2017 .
^ a b Brinsfield, James W.; Higgins, David (September 2008). "The Rotational Period of 1379 Lomosonowa" . The Minor Planet Bulletin . 35 (3 ): 122. Bibcode :2008MPBu...35..122B . ISSN 1052-8091 . Retrieved 27 October 2017 .
^ a b c d e Binzel, R. P. (October 1987). "A photoelectric survey of 130 asteroids" . Icarus . 72 (1 ): 135–208. Bibcode :1987Icar...72..135B . doi :10.1016/0019-1035(87 )90125-4 . ISSN 0019-1035 . Retrieved 27 October 2017 .
^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results" . Icarus . 261 : 34–47. arXiv :1506.00762 . Bibcode :2015Icar..261...34V . doi :10.1016/j.icarus.2015.08.007 . Retrieved 27 October 2017 .
^ a b c d e "1379 Lomonosowa (1936 FC)" . Minor Planet Center . Retrieved 27 October 2017 .
^ Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008) . Springer Berlin Heidelberg. p. 221 . doi :10.1007/978-3-642-01965-4 . ISBN 978-3-642-01964-7 .
External links
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R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=1379_Lomonosowa&oldid=1195682039 "
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