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4222 Nancita (prov. designation : 1988 EK1 ) is a bright background asteroid and upcoming Mars-crosser on an eccentric orbit from the inner regions of the asteroid belt . It was discovered on 13 March 1988, by American astronomer Eleanor Helin at Palomar Observatory in California, United States.[9] The S-type asteroid has a rotation period of 3.9 hours and measures approximately 9 kilometers (5.6 miles) in diameter. It was named after the discoverer's daughter-in-law, Nancy Coker Helin.
Orbit and classification [ edit ]
Nancita is a non-family asteroid from the main belt's background population when applying the hierarchical clustering method to its proper orbital elements . It will become a Mars-crossing asteroid in June 2019. It orbits the Sun in the inner main-belt at a distance of 1.7–3.1 AU once every 3 years and 8 months (1,331 days). Its orbit has an eccentricity of 0.29 and an inclination of 4° with respect to the ecliptic .[1] The asteroid was first observed as 1950 TF4 at McDonald Observatory in 1950. Its observation arc begins at Crimea–Nauchnij in 1968, when it observed as 1968 QL1 , or 20 years prior to its official discovery observation at Palomar.[9]
This minor planet was named in honor of Nancy Coker Helin, daughter-in-law of the discoverer, and wife to Bruce Helin, after whom the minor planet 2430 Bruce Helin had previously been named. Nancy is described by the discoverer as a talented singer, composer and teacher, who has brought music and joy to her family.[2] The official naming citation was published by the Minor Planet Center on 2 December 1990 (M.P.C. 17466 ).[10]
Physical characteristics [ edit ]
In the SMASS classification , Nancita is a common S-type asteroid .[1]
Rotation and shape [ edit ]
A rotational lightcurve of Nancita , obtained from photometric observations at the Australian Hunters Hill Observatory (E14 ) and collaborating stations in 2006, gave a well-defined rotation period of 3.8732 hours with a high brightness amplitude of 0.97 in magnitude (U=3 ), indicating that the body has a non-spheroidal shape.[7]
Diameter and albedo [ edit ]
According to the surveys carried out by the Infrared Astronomical Satellite IRAS , the Japanese Akari satellite, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , Nancita measures between 8.5 and 9.7 kilometers in diameter and its surface has an albedo in the range of 0.21 to 0.27.[3] [4] [5] [6] The Collaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS.[8]
References [ edit ]
^ a b Schmadel, Lutz D. (2007). "(4222) Nancita". Dictionary of Minor Planet Names – (4222) Nancita . Springer Berlin Heidelberg . p. 361. doi :10.1007/978-3-540-29925-7_4187 . ISBN 978-3-540-00238-3 .
^ a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0" . NASA Planetary Data System . 12 : IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode :2004PDSS...12.....T . Retrieved 16 March 2020 .
^ 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 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters" . The Astrophysical Journal . 741 (2 ): 20. arXiv :1109.4096 . Bibcode :2011ApJ...741...68M . doi :10.1088/0004-637X/741/2/68 . Retrieved 5 December 2016 .
^ 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 . Retrieved 2 May 2016 .
^ a b Higgins, David; Pravec, Petr; Kusnirak, Peter; Reddy, Vishnu; Dyvig, Ron (September 2006). "Asteroid lightcurve analysis at Hunters Hill Observatory and collaborating stations - summer 2005/6" (PDF) . Minor Planet Bulletin . 33 (3 ): 64–66. Bibcode :2006MPBu...33...64H . ISSN 1052-8091 . Archived from the original (PDF) on 19 March 2020. Retrieved 19 March 2020 .
^ a b c "LCDB Data for (4222) Nancita" . Asteroid Lightcurve Database (LCDB). Retrieved 2 May 2016 .
^ a b "4222 Nancita (1988 EK1)" . Minor Planet Center . Retrieved 2 May 2016 .
^ "MPC/MPO/MPS Archive" . Minor Planet Center . Retrieved 2 May 2016 .
External links [ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=4222_Nancita&oldid=1201891104 "
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