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1083 Salvia (prov. designation : 1928 BC ) is a stony background asteroid from the inner regions of the asteroid belt . It was discovered on 26 January 1928, by astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany.[1] The assumed S-type asteroid has a rotation period of 4.2 hours and measures approximately 10 kilometers (6.2 miles) in diameter. It was named after the flowering plant Salvia (sage).[3]
Orbit and classification [ edit ]
Located in the region of the Flora family ,[9] Salvia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements .[5] [6] It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.8 AU once every 3 years and 7 months (1,298 days; semi-major axis of 2.33 AU ). Its orbit has an eccentricity of 0.18 and an inclination of 5° with respect to the ecliptic .[4] The asteroid was first observed as A910 AA at Heidelberg Observatory on 7 January 1910, where the body's observation arc begins 18 years later, with its official discovery observation on 26 January 1928.[1]
This minor planet was named after the flowering plant Salvia (sage), a genus of herbs or shrubs that belong to the mint family . The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 102 ).[3]
Reinmuth's flowers [ edit ]
Due to his many discoveries, Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between (1009) and (1200) . This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia , that were all named after plants, in particular flowering plants (also see list of minor planets named after animals and plants) .[12]
Physical characteristics [ edit ]
Salvia is an assumed stony S-type asteroid , which corresponds to its observed albedo (see below) .[9]
Rotation period and poles [ edit ]
In March 1992, a rotational lightcurve of Salvia was obtained from photometric observations by Polish astronomer Wiesław Wiśniewski . Lightcurve analysis gave a well-defined rotation period of 4.23 hours with a brightness amplitude of 0.61 magnitude (U=3 ).[11] A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database, gave a concurring period of 4.281429 ± 0.000001 hours, as well as two spin axis of (165.0°, −59.0°) and (358.0°, −58.0°) in ecliptic coordinates (λ, β).[13]
Diameter and albedo [ edit ]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), Salvia measures between 8.927 and 10.283 kilometers in diameter and its surface has an albedo between 0.2103 and 0.2184.[7] [8] [10] The Collaborative Asteroid Lightcurve Link adopts Petr Pravec 's revised WISE data, that is an albedo of 0.2103 and a diameter of 10.28 kilometers based on an absolute magnitude of 12.25.[9]
References [ edit ]
^ "salvia" . Oxford English Dictionary (Online ed.). Oxford University Press . (Subscription or participating institution membership required.)
^ a b c Schmadel, Lutz D. (2007). "(1083) Salvia". Dictionary of Minor Planet Names . Springer Berlin Heidelberg . p. 92 . doi :10.1007/978-3-540-29925-7_1084 . ISBN 978-3-540-00238-3 .
^ a b c d "JPL Small-Body Database Browser: 1083 Salvia (1928 BC)" (2017-07-05 last obs.). Jet Propulsion Laboratory . Retrieved 28 November 2017 .
^ a b "Asteroid 1083 Salvia – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 13 March 2020 .
^ a b c d "Asteroid 1083 Salvia" . Small Bodies Data Ferret . Retrieved 26 October 2019 .
^ 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 .
^ 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 e f g "LCDB Data for (1083) Salvia" . Asteroid Lightcurve Database (LCDB). Retrieved 28 November 2017 .
^ a b c d Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations" . Icarus . 221 (1 ): 365–387. Bibcode :2012Icar..221..365P . doi :10.1016/j.icarus.2012.07.026 . Retrieved 28 November 2017 .
^ a b c Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids" . Abstracts of the Lunar and Planetary Science Conference . 26 : 1511. Bibcode :1995LPI....26.1511W . Retrieved 28 November 2017 .
^ Schmadel, Lutz D. (2007). "(1054) Forsytia". Dictionary of Minor Planet Names . Springer Berlin Heidelberg . p. 90 . doi :10.1007/978-3-540-29925-7_1055 . ISBN 978-3-540-00238-3 .
^ 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 28 November 2017 .
External links [ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=1083_Salvia&oldid=1195679978 "
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