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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
956 Elisa (prov. designation : A921 PE or 1921 JW ) is a Flora asteroid from the inner regions of the asteroid belt , approximately 10.5 kilometers (6.5 miles) in diameter. It was discovered on 8 August 1921, by German astronomer Karl Reinmuth at the Heidelberg Observatory .[1] The V-type asteroid has a rotation period of 16.5 hours. It was named after Elisa Reinmuth, mother of the discoverer.[4]
Orbit and classification [ edit ]
When applying the synthetic hierarchical clustering method (HCM) by Nesvorný , Elisa is a member of the Flora family (402 ), a giant asteroid family and the largest family of stony asteroids in the main-belt.[6] [12] : 23 However, according to another HCM-analysis by Milani and Knežević (AstDys), it is a background asteroid as this analysis does not recognize the Flora asteroid clan .[13]
Elisa orbits the Sun in the inner asteroid belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,273 days; semi-major axis of 2.3 AU ). Its orbit has an eccentricity of 0.20 and an inclination of 6° with respect to the ecliptic .[5] The body's observation arc begins at Heidelberg Observatory on 9 August 1921, the night after its official discovery observation.[1]
This minor planet was named after Elisa Reinmuth, mother of the discoverer Karl Reinmuth . The naming was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 92 ).[4]
Physical characteristics [ edit ]
In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Elisa is a V-type asteroid .[6] [11] These asteroids are also called "Vestoids", thought to have originates from an ejecting impact event on 4 Vesta .[14] [15]
Rotation period [ edit ]
In July 2008, a rotational lightcurve of Elisa was obtained from photometric observations by Matthieu Conjat at Nice Observatory in France. Lightcurve analysis gave a well-defined rotation period of 16.492± 0.006 hours with a brightness variation of 0.36± 0.02 magnitude (U=3 ).[9] [10] During the same opposition, Vladimir Benishek at Belgrade Observatory (057 ) and Lucy Lim with the Spitzer -team determined a period for this asteroid of 16.5075± 0.0007 and 16.494± 0.001 hours with an amplitude of 0.37± 0.02 and 0.35± 0.02 magnitude, respectively (U=3/3– ).[8] [16]
Diameter and albedo [ edit ]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE) and the Spitzer Space Telescope , Elisa measures 10.474± 0.208 and 10.6± 0.5 kilometers in diameter and its surface has an albedo of 0.147± 0.022 and 0.142± 0.022 , respectively.[7] [8] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a Flora asteroid of 0.24 and calculates a diameter of 10.31 kilometers based on an absolute magnitude of 12.1.[9] The WISE team has also published two smaller mean-diameters of 8.02± 1.09 km and 8.40± 0.67 km with higher albedos of 0.41± 0.21 and 0.362± 0.071 .[6] [9]
References [ edit ]
^ (German Names)
^ Noah Webster (1884) A Practical Dictionary of the English Language
^ a b c Schmadel, Lutz D. (2007). "(956) Elisa". Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p. 84 . doi :10.1007/978-3-540-29925-7_957 . ISBN 978-3-540-00238-3 .
^ a b c d "JPL Small-Body Database Browser: 956 Elisa (A921 PE)" (2020-01-05 last obs.). Jet Propulsion Laboratory . Retrieved 14 February 2020 .
^ a b c d "Asteroid 956 Elisa" . Small Bodies Data Ferret . Retrieved 14 February 2020 .
^ 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 .
^ a b c d Lim, Lucy F.; Emery, Joshua P.; Moskovitz, Nicholas A. (June 2011). "Mineralogy and thermal properties of V-type Asteroid 956 Elisa: Evidence for diogenitic material from the Spitzer IRS (5-35 μm) spectrum" (PDF) . Icarus . 213 (2 ): 510–523. Bibcode :2011Icar..213..510L . doi :10.1016/j.icarus.2010.12.006 .
^ a b c d "LCDB Data for (956) Elisa" . Asteroid Lightcurve Database (LCDB). Retrieved 14 February 2020 .
^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (956) Elisa" . Geneva Observatory. Retrieved 14 February 2020 .
^ a b Lazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004). "S3OS2: the visible spectroscopic survey of 820 asteroids" (PDF) . Icarus . 172 (1 ): 179–220. Bibcode :2004Icar..172..179L . doi :10.1016/j.icarus.2004.06.006 . Retrieved 14 February 2020 .
^ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV . pp. 297–321. arXiv :1502.01628 . Bibcode :2015aste.book..297N . doi :10.2458/azu_uapress_9780816532131-ch016 . ISBN 978-0-8165-3213-1 .
^ "Asteroid 956 Elisa – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 14 February 2020 .
^ M. Florczak; D. Lazarro & R. Duffard (2002). "Discovering New V-Type Asteroids in the Vicinity of 4 Vesta". Icarus . 159 (1 ): 178. Bibcode :2002Icar..159..178F . doi :10.1006/icar.2002.6913 .
^ V. Carruba; et al. (2005). "On the V-type asteroids outside the Vesta family". Astronomy & Astrophysics . 441 (2 ): 819–829. arXiv :astro-ph/0506656 . Bibcode :2005A&A...441..819C . doi :10.1051/0004-6361:20053355 .
^ Benishek, Vladimir; Protitch-Benishek, Vojislava (April 2009). "CCD Photometry of Asteroids at the Belgrade Astronomical Observatory: 2008 January-September" (PDF) . Minor Planet Bulletin . 36 (2 ): 35–37. Bibcode :2009MPBu...36...35B . ISSN 1052-8091 . Archived from the original (PDF) on 6 November 2020. Retrieved 14 February 2020 .
External links [ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=956_Elisa&oldid=1190799585 "
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a d d i t i o n a l t e r m s m a y a p p l y . B y u s i n g t h i s s i t e , y o u a g r e e t o t h e T e r m s o f U s e a n d P r i v a c y P o l i c y . W i k i p e d i a ® i s a r e g i s t e r e d t r a d e m a r k o f t h e W i k i m e d i a F o u n d a t i o n , I n c . , a n o n - p r o f i t o r g a n i z a t i o n .
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