(459883) 2014 JX55
Discovery | |
---|---|
Discovered by | Mt. Lemmon Survey |
Discovery date | 2007-03-10 |
Designations | |
Aten asteroid, Mercury crosser, Venus crosser | |
Orbital characteristics[1] | |
Epoch 2454170.5 (2007-Mar-11.0) | |
Aphelion | (0.979 AU) |
Perihelion | (0.0116 AU) |
357.052 Gm (2.387 AU) | |
Eccentricity | 0.787 |
148.114 d (0.41 a) | |
Average orbital speed | km/s |
° | |
Inclination | 8.477° |
° | |
° | |
Physical characteristics | |
Spectral type | S-type |
19.591 | |
2007 EB26 is one of the closest orbiting object to the Sun and second object ever numbered minor planet to have an orbit completely interior to that of the earth. It is classified as an Atira NEO Near Earth Object but does not cross Earth's orbit.
Discovery and naming
Discovered on March 10th 2011
Characteristics
Of note, this is one of the closest orbiting body to the sun, approaching within 0.116 AU of the sun approximately every 148 days, before leaving for a distance of 0.979 AU and does not cross the Earth's orbit. Only (137924) 2000 BD19 has a closer orbit, 0.092AU, although 2000 BD19 goes beyond Earth's orbit.
Mass
Unknown
Family relationships
Like Atira, 2007 EB26 is a numbered minor planet completely inside the orbit of earth.
Occultations
References
- ^ "JPL Small-Body Database Browser:". Retrieved May 2013.
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External links
- shape model deduced from lightcurve
- Yeomans, Donald K. "Horizons system". NASA JPL. Archived from the original on 28 March 2007. Retrieved 20 March 2007.
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suggested) (help) — Horizons can be used to obtain a current ephemeris.
References
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