astro.wikisort.org - AsteroidIva (minor planet designation: 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]
497 Iva Modelled shape of Iva from its lightcurve |
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Discovered by | Raymond Smith Dugan |
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Discovery site | Heidelberg |
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Discovery date | 4 November 1902 |
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MPC designation | (497) Iva |
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Pronunciation | [1] |
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Alternative designations | 1902 KJ |
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Epoch 31 July 2016 (JD 2457600.5) |
Uncertainty parameter 0 |
Observation arc | 113.45 yr (41,438 d) 113.45 yr (41438 d) |
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Aphelion | 3.7065 AU (554.48 Gm) |
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Perihelion | 1.9966 AU (298.69 Gm) |
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Semi-major axis | 2.8516 AU (426.59 Gm) |
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Eccentricity | 0.29981 |
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Orbital period (sidereal) | 4.82 yr (1,758.8 d) 4.82 yr (1758.8 d) |
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Mean anomaly | 242.202° |
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Mean motion | 0° 12m 16.848s / day |
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Inclination | 4.8205° |
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Longitude of ascending node | 6.3305° |
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Argument of perihelion | 3.5819° |
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Synodic rotation period | 4.620 h (0.1925 d) |
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Absolute magnitude (H) | 10.02 |
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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
- Noah Webster (1884) A Practical Dictionary of the English Language
- "497 Iva (1902 KJ)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 6 May 2016.
- Schmadel, Lutz D. (2013), Dictionary of Minor Planet Names, Springer Berlin Heidelberg, p. 83, ISBN 9783662066157
- 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.
- 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.
- 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
- 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.
External links
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На других языках
[de] (497) Iva
(497) Iva ist ein Asteroid des Hauptgürtels, der am 4. November 1902 vom Astronomen Raymond Smith Dugan in Heidelberg entdeckt wurde.
- [en] 497 Iva
[es] (497) Iva
(497) Iva es un asteroide perteneciente al cinturón de asteroides descubierto el 4 de noviembre de 1902 por Raymond Smith Dugan desde el observatorio de Heidelberg-Königstuhl, Alemania.
Está nombrado en honor de Iva Shores.[2]
[ru] (497) Ива
(497) Ива (лат. Iva) — астероид главного пояса, который принадлежит к металлическому спектральному классу M. Он был открыт 4 ноября 1902 года американским астрономом Раймондом Дуганом в обсерватории Хайдельберг и назван в честь дочери первооткрывателя[1].
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