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283 Emma

From Wikipedia, the free encyclopedia
Main-belt asteroid

283 Emma
A three-dimensional model of 283 Emma based on its light curve
Discovery
Discovered byAuguste Charlois
Discovery date8 February 1889
Designations
(283) Emma
Pronunciation/ˈɛmə/[1]
A889 CA,1980 FJ12
Main belt (Emma)
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc122.26 yr (44655 d)
Aphelion3.49701 AU (523.145 Gm)
Perihelion2.59675 AU (388.468 Gm)
3.04688 AU (455.807 Gm)
Eccentricity0.14773
5.32yr (1942.6d)
17.07 km/s
127.107°
0° 11m 7.148s / day
Inclination7.99162°
304.369°
53.7020°
Knownsatellites1 (9±5 km)[3]
Physical characteristics
Dimensions148.06±4.6 km(IRAS)[2]
160±10 km (AO)[3]
Mass1.38×1018 kg[4]
0.81±0.08 g/cm3[4]
6.896 h (0.2873 d)[2]
0.0262±0.002[2] (Dark)
8.72[2]

283 Emma is a largeasteroid of theasteroid belt and the namesake of theEmma family. It was discovered byAuguste Charlois on 8 February 1889, inNice, France. The reason for its name is unknown.[5]

Measurements made with theIRAS observatory give a diameter of145.70±5.89 km and ageometric albedo of0.03±0.01. By comparison, the MIPSphotometer on theSpitzer Space Telescope gives a diameter of145.44±7.72 km and a geometric albedo of0.03±0.01. When the asteroid was observedocculting a star, the results showed a diameter of148.00±16.26 km.[6]

Satellite

[edit]

A companion for 283 Emma was detected on 14 July 2003 by W. J. Merline et al. using theKeck II telescope and is designatedS/2003 (283) 1. The discovery was reported in theInternational Astronomical Union Circular (IAUC) 8165.[7] The satellite orbits at asemi-major axis of about 581 km with an eccentricity of 0.12.[3] Emma has aHill sphere with a radius of about 28,000 km.[3]

References

[edit]
  1. ^"Emma".Dictionary.com Unabridged (Online). n.d.
  2. ^abcde"JPL Small-Body Database Browser: 283 Emma".Solar System Dynamics (2008-10-30 last obs). Retrieved11 May 2016.
  3. ^abcdMarchis, Franck; P. Descamps; J. Berthier; D. hestroffer; F. vachier; M. Baek; A. Harris; D. Nesvorny (2008). "Main Belt Binary Asteroidal Systems With Eccentric Mutual Orbits".Icarus.195 (1):295–316.arXiv:0804.1385.Bibcode:2008Icar..195..295M.doi:10.1016/j.icarus.2007.12.010.S2CID 119244052.
  4. ^abJim Baer (12 December 2010)."Recent Asteroid Mass Determinations". Personal Website. Archived fromthe original on 29 January 2009. Retrieved17 July 2015.
  5. ^Lutz D. Schmadel (2003).Dictionary of Minor Planet Names (5th ed.). Springer Science & Business Media. p. 40.ISBN 978-3-540-00238-3.
  6. ^Ryan, Erin Lee; et al. (April 2012), "The Kilometer-Sized Main Belt Asteroid Population as Revealed by Spitzer",arXiv:1204.1116 [astro-ph.EP]
  7. ^IAUC 8165: S/2003 (283) 1; NOVAE IN M31 (Report). IAU. 27 July 2003.

External links

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