497 Iva is a main-belt asteroid orbiting the Sun, not to be confused with 1627 Ivar. It was discovered by American astronomer R. S. Dugan on 4 November 1902, and was named for Iva Shores, the young daughter of the family where he was staying in Heidelberg.[3] This object is orbiting at a distance of 2.85 AU with a period of 4.82 yr and an eccentricity of 0.3. The orbital plane is inclined at an angle of 4.8° to the plane of the ecliptic.[2]

This asteroid is classified as an M-type asteroid and is considered anhydrous[4] but oxidized.[5] Further analysis of the spectra suggests the "presence of either an olivine or high-Ca pyroxene phase in addition to orthopyroxene ± Type B clinopyroxene".[6] Analysis of light curves based on photometric data show a rotation period of 4.621±0.001 h with a brightness variation of 0.34±0.02 in magnitude.[7]

References

  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ a b "497 Iva (1902 KJ)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 6 May 2016.
  3. ^ Schmadel, Lutz D. (2013), Dictionary of Minor Planet Names, Springer Berlin Heidelberg, p. 83, ISBN 9783662066157
  4. ^ Birlan, M.; et al. (November 2007), "Spectral properties of nine M-type asteroids" (PDF), Astronomy and Astrophysics, 475 (2): 747–754, Bibcode:2007A&A...475..747B, doi:10.1051/0004-6361:20077914.
  5. ^ Busarev, V. V.; Taran, M. N. (November 2002), Warmbein, Barbara (ed.), "On the spectral similarity of carbonaceous chondrites and some hydrated and oxidized asteroids", Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany, Noordwijk, Netherlands: ESA Publications Division, pp. 933–936, Bibcode:2002ESASP.500..933B, ISBN 92-9092-810-7.
  6. ^ Hardersen, Paul S.; et al. (December 2011), "The M-/X-asteroid menagerie: Results of an NIR spectral survey of 45 main-belt asteroids", Meteoritics & Planetary Science, 46 (12): 1910–1938, Bibcode:2011M&PS...46.1910H, doi:10.1111/j.1945-5100.2011.01304.x
  7. ^ Warner, Brian D. (July 2009), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 December - 2009 March", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 36 (3): 109–116, Bibcode:2009MPBu...36..109W.


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