283 Emma
A three-dimensional model of 283 Emma based on its light curve. | |
Discovery | |
---|---|
Discovered by | Auguste Charlois |
Discovery date | 8 February 1889 |
Designations | |
Main belt (Eos) | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 122.26 yr (44655 d) |
Aphelion | 3.49701 AU (523.145 Gm) |
Perihelion | 2.59675 AU (388.468 Gm) |
3.04688 AU (455.807 Gm) | |
Eccentricity | 0.14773 |
5.32 yr (1942.6 d) | |
Average orbital speed | 17.07 km/s |
127.107° | |
0° 11m 7.148s / day | |
Inclination | 7.99162° |
304.369° | |
53.7020° | |
Known satellites | 1 (9±5 km)[2] |
Earth MOID | 1.601 AU (239.5 Gm) |
Jupiter MOID | 1.97626 AU (295.644 Gm) |
Jupiter Tisserand parameter | 3.207 |
Physical characteristics | |
Dimensions |
±4.6 km ( 148.06IRAS)[1] 160±10 km (AO)[2] |
Mass | 1.38×1018 kg[3] |
Mean density | 0.81±0.08 g/cm³[3] |
Equatorial surface gravity | unknown |
Equatorial escape velocity | unknown |
6.896 h (0.2873 d)[1] | |
±0.002 0.0262[1] (Dark) | |
Temperature | unknown |
unknown | |
8.72[1] | |
|
283 Emma is a large asteroid of the asteroid belt. It was discovered by Auguste Charlois on February 8, 1889, in Nice, France. The reason for its name is unknown.[4]
Measurements made with the IRAS observatory give a diameter of 145.70 ± 5.89 km and a geometric albedo of 0.03 ± 0.01. By comparison, the MIPS photometer on the Spitzer Space Telescope gives a diameter of 145.44 ± 7.72 km and a geometric albedo of 0.03 ± 0.01. When the asteroid was observed occulting a star, the results showed a diameter of 148.00 ± 16.26 km.[5]
Satellite
A companion for 283 Emma was detected on 14 July 2003 by W. J. Merline et al. using the Keck II telescope and is designated S/2003 (283) 1. The announcement is contained in the International Astronomical Union Circular (IAUC) 8165.[6] The satellite orbits at a semi-major axis of about 581 km with an eccenticity of 0.12.[2] Emma has a hill sphere with a radius of about 28,000 km.[2]
References
- 1 2 3 4 5 "JPL Small-Body Database Browser: 283 Emma" (2008-10-30 last obs). Retrieved 11 May 2016.
- 1 2 3 4 Marchis, 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.
- 1 2 Jim Baer (2010-12-12). "Recent Asteroid Mass Determinations". Personal Website. Retrieved 2015-07-17.
- ↑ Lutz D. Schmadel, Dictionary of Minor Planet Names, 5th edtn. (2003), Appendix 11, p.40.
- ↑ Ryan, Erin Lee; et al. (April 2012), "The Kilometer-Sized Main Belt Asteroid Population as Revealed by Spitzer", eprint arXiv, arXiv:1204.1116, Bibcode:2012arXiv1204.1116R.
- ↑ S/2003 (283) 1 (Circular No. 8165)
External links
- Orbital simulation from JPL (Java) / Ephemeris
- Orbits of Binary Asteroids with Adaptive Optics (VLT images)
- 283 Emma at the JPL Small-Body Database