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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
Hesperia (minor planet designation : 69 Hesperia ) is a large, M-type main-belt asteroid . It was discovered by the Italian astronomer Giovanni Schiaparelli on April 29, 1861[1] from Milan , while he was searching for the recently discovered 63 Ausonia .[7] It was his only asteroid discovery. Schiaparelli named it Hesperia in honour of Italy (the word is a Greek term for the peninsula).[8] The asteroid is orbiting the Sun with a period of 5.14 years, a semimajor axis of 2.980 AU , and eccentricity of 0.165. The orbital plane is inclined by an angle of 8.59° to the plane of the ecliptic .
Hesperia was observed by Arecibo radar in February 2010.[5] Radar observations combined with lightcurve -based shape models, lead to a diameter estimate of 110 ± 15 km (68 ± 9.3 mi ). The radar albedo is consistent with a high-metal M-type asteroid .[5] In the near infrared , a weak absorption feature near a wavelength of 0.9 μm can be attributed to orthopyroxenes on the surface.[9] A meteorite analogue of the reflectance spectra from 69 Hesperia is the Hoba ataxite .[10]
References
[ edit ]
^ a b
"Editorial Notice" (PDF) . The Minor Planet Circulars . MPC 94743-95312: 94743. 29 August 2015. Retrieved 4 September 2015 .
^ Noah Webster (1884) A Practical Dictionary of the English Language
^ "Hesperian" . Oxford English Dictionary (Online ed.). Oxford University Press . (Subscription or participating institution membership required.)
^ a b c d "JPL Small-Body Database Browser: 69 Hesperia" (2011-09-07 last obs). Jet Propulsion Laboratory . Retrieved 27 January 2012 .
^ a b c Shepard, Michael K.; Harris, Alan W.; Taylor, Patrick A.; Clark, Beth Ellen; Ockert-Bell, Maureen; Nolan, Michael C.; et al. (2011). "Radar observations of Asteroids 64 Angelina and 69 Hesperia" (PDF) . Icarus . 215 (2 ): 547–551. arXiv :1104.4114 . Bibcode :2011Icar..215..547S . doi :10.1016/j.icarus.2011.07.027 .
^ a b Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science , vol. 73, pp. 98–118, arXiv :1203.4336 , Bibcode :2012P&SS...73...98C , doi :10.1016/j.pss.2012.03.009 . See Table 1.
^ De Meis, S. (2011), "A few aspects of Schiaparelli's studies", Memorie della Societa Astronomica Italiana , 82 : 290, Bibcode :2011MmSAI..82..290D .
^ Schmadel, Lutz D. (2003), Dictionary of Minor Planet Names , Springer Science & Business Media, p. 22, ISBN 978-3-540-00238-3 .
^ Hardersen, Paul S.; et al. (May 2005), "Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids", Icarus , 175 (1 ): 141−158, Bibcode :2005Icar..175..141H , doi :10.1016/j.icarus.2004.10.017 .
^ Neeley, J. R.; et al. (August 2014), "The composition of M-type asteroids II: Synthesis of spectroscopic and radar observations", Icarus , 238 : 37−50, arXiv :1407.0750 , Bibcode :2014Icar..238...37N , doi :10.1016/j.icarus.2014.05.008 .
External links
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Data from Wikidata
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=69_Hesperia&oldid=1195661671 "
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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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