1139 Atami
Discovery | |
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Discovered by | Okuro Oikawa and Kazuo Kubokawa |
Discovery date | 1929-Dec-01 |
Orbital characteristics | |
Epoch Orbital Elements at Epoch 2454200.5 (2007-Apr-10.0) TDB | |
Aphelion | 2.44538167801902 AU |
Perihelion | 1.4506609472059 AU |
1.94802131261246 AU | |
Eccentricity | 0.25531566938534 |
993.0908555984342 days 2.72 years | |
172.9145575307504 ° | |
Inclination | 13.0888203094939 ° |
213.4316068527716 ° | |
206.4535499752972 ° | |
Known satellites | 1[2] |
Physical characteristics | |
Dimensions | ~6km[2] |
27.44 h | |
S (Tholen) S (SSMASSII) | |
12.51 mag | |
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1139 Atami is a Mars-crossing asteroid orbiting the Sun. It makes a revolution around the Sun once every 3 years. It completes one rotation once every 27 hours. It was discovered by Okuro Oikawa and Kazuo Kubokawa on December 1, 1929.[1] It is named after a harbor near Tokyo, Japan. Its provisional designation was 1929 XE.[3]
Binary system
Photometric and Arecibo echo spectra observations in 2005 confirmed a 5 km (3 mi) satellite orbiting at least 15 km (9 mi) from the primary.[2] Due to the similar size of the primary and secondary the Minor Planet Center lists this as a binary companion.[4]
References
- 1 2 "JPL Small-Body Database Browser: 1139 Atami (1929 XE)". Retrieved October 17, 2007.
- 1 2 3 "Electronic Telegram No. 430". IAU Central Bureau for Astronomical Telegrams. 2006-03-14. Retrieved 2011-01-25.
- ↑ Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names. Springer. ISBN 3-540-00238-3.
- ↑ "Satellites and Companions of Minor Planets". IAU Central Bureau for Astronomical Telegrams. 2009-09-17. Retrieved 2011-01-25.
External links
- Orbital simulation from JPL (Java) / Ephemeris
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