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337 Devosa

Devosa (minor planet designation: 337 Devosa) is a large Main belt asteroid. It was discovered by Auguste Charlois on 22 September 1892 in Nice. The asteroid is orbiting the Sun at a distance of 2.38 AU with a period of 3.68 years and an eccentricity (ovalness) of 0.14. These orbital elements are similar to that of the large asteroid 4 Vesta.[3] The orbital plane of 337 Devosa is tilted at an angle of 7.85° to the plane of the ecliptic.[1]

337 Devosa
Discovery
Discovered byAuguste Charlois
Discovery date22 September 1892
Designations
(337) Devosa
Pronunciation/dɪˈvsə/
Named after
(unknown)
1892 E
Main belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.6 yr (45,130 d)
Aphelion2.71030 AU (405.455 Gm)
Perihelion2.05546 AU (307.492 Gm)
2.38288 AU (356.474 Gm)
Eccentricity0.13741
3.68 yr (1,343.4 d)
169.690°
0° 16m 4.616s / day
Inclination7.85443°
355.479°
98.6063°
Physical characteristics
Dimensions59.11±2.3 km[1]
63.87±3.14 km[2]
Mass(1.08±0.16)×1018 kg[2]
Mean density
7.91±1.65 g/cm3[2]
4.653 h (0.1939 d)
0.1614±0.013
X[1]
8.74

This is classified as an X-type asteroid in the Tholen system[1] and Xk type in the Bus-DeMeo taxonomy, with spectral properties similar to mesosiderites.[3] It spans a girth of 59±2 km and has a rotation period of 4.65 h.[4]

References

  1. ^ a b c d e "337 Devosa (1892 E)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
  2. ^ a b c 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.
  3. ^ a b Vernazza, P.; et al. (August 2009), "Plausible parent bodies for enstatite chondrites and mesosiderites: Implications for Lutetia's fly-by", Icarus, 202 (2): 477–486, Bibcode:2009Icar..202..477V, doi:10.1016/j.icarus.2009.03.016.
  4. ^ Ockert-Bell, M. E.; et al. (December 2010), "The composition of M-type asteroids: Synthesis of spectroscopic and radar observations", Icarus, 210 (2): 674–692, Bibcode:2010Icar..210..674O, doi:10.1016/j.icarus.2010.08.002.

External links

  • 337 Devosa at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 337 Devosa at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters


devosa, devosa, minor, planet, designation, large, main, belt, asteroid, discovered, auguste, charlois, september, 1892, nice, asteroid, orbiting, distance, with, period, years, eccentricity, ovalness, these, orbital, elements, similar, that, large, asteroid, . Devosa minor planet designation 337 Devosa is a large Main belt asteroid It was discovered by Auguste Charlois on 22 September 1892 in Nice The asteroid is orbiting the Sun at a distance of 2 38 AU with a period of 3 68 years and an eccentricity ovalness of 0 14 These orbital elements are similar to that of the large asteroid 4 Vesta 3 The orbital plane of 337 Devosa is tilted at an angle of 7 85 to the plane of the ecliptic 1 337 DevosaDiscoveryDiscovered byAuguste CharloisDiscovery date22 September 1892DesignationsMPC designation 337 DevosaPronunciation d ɪ ˈ v oʊ s e Named after unknown Alternative designations1892 EMinor planet categoryMain beltOrbital characteristics 1 Epoch 31 July 2016 JD 2457600 5 Uncertainty parameter 0Observation arc123 6 yr 45 130 d Aphelion2 71030 AU 405 455 Gm Perihelion2 05546 AU 307 492 Gm Semi major axis2 38288 AU 356 474 Gm Eccentricity0 13741Orbital period sidereal 3 68 yr 1 343 4 d Mean anomaly169 690 Mean motion0 16m 4 616s dayInclination7 85443 Longitude of ascending node355 479 Argument of perihelion98 6063 Physical characteristicsDimensions59 11 2 3 km 1 63 87 3 14 km 2 Mass 1 08 0 16 1018 kg 2 Mean density7 91 1 65 g cm3 2 Synodic rotation period4 653 h 0 1939 d Geometric albedo0 1614 0 013Spectral typeX 1 Absolute magnitude H 8 74This is classified as an X type asteroid in the Tholen system 1 and Xk type in the Bus DeMeo taxonomy with spectral properties similar to mesosiderites 3 It spans a girth of 59 2 km and has a rotation period of 4 65 h 4 References Edit a b c d e 337 Devosa 1892 E JPL Small Body Database NASA Jet Propulsion Laboratory Retrieved 11 May 2016 a b c Carry B December 2012 Density of asteroids Planetary and Space Science vol 73 pp 98 118 arXiv 1203 4336 Bibcode 2012P amp SS 73 98C doi 10 1016 j pss 2012 03 009 See Table 1 a b Vernazza P et al August 2009 Plausible parent bodies for enstatite chondrites and mesosiderites Implications for Lutetia s fly by Icarus 202 2 477 486 Bibcode 2009Icar 202 477V doi 10 1016 j icarus 2009 03 016 Ockert Bell M E et al December 2010 The composition of M type asteroids Synthesis of spectroscopic and radar observations Icarus 210 2 674 692 Bibcode 2010Icar 210 674O doi 10 1016 j icarus 2010 08 002 External links Edit337 Devosa at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 337 Devosa at the JPL Small Body Database Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters This article about an asteroid native to the asteroid belt is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title 337 Devosa amp oldid 1123266550, wikipedia, wiki, book, books, library,

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