Astronomy:(120132) 2003 FY128
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Discovery | |
---|---|
Discovered by | NEAT |
Discovery date | 26 March 2003 |
Designations | |
(120132) 2003 FY128 | |
none | |
Minor planet category | detached object[2] |
Orbital characteristics[3] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 3 | |
Observation arc | 8159 days (22.34 yr) |
|{{{apsis}}}|helion}} | 62.551 astronomical unit|AU (9.3575 Tm) |
|{{{apsis}}}|helion}} | 37.066 AU (5.5450 Tm) |
49.809 AU (7.4513 Tm) | |
Eccentricity | 0.25584 |
Orbital period | 351.53 yr (128397 d) |
Mean anomaly | 28.257° |
Mean motion | 0° 0m 10.094s / day |
Inclination | 11.757° |
Longitude of ascending node | 341.68° |
175.26° | |
Earth MOID | 36.0755 AU (5.39682 Tm) |
Jupiter MOID | 31.6621 AU (4.73658 Tm) |
Physical characteristics | |
Dimensions | 460±21 km[4] |
Rotation period | 8.54 h (0.356 d) |
Geometric albedo | 0.079±0.010[4] |
Absolute magnitude (H) | 4.8[3] |
(120132) 2003 FY128 (provisional designation 2003 FY128) is a trans-Neptunian object with a diameter of about 460 km.[4] It orbits the Sun at a distance of about 49.81 astronomical units.[3] It was discovered on 26 March 2003 by the NEAT program at the Palomar Observatory, California .
Classification
It is classified as a detached object by the Deep Ecliptic Survey (DES), since its orbit appears to be beyond the current control of Neptune.[2] Though, if Neptune migrated outward, there would have been a period when Neptune had a higher eccentricity.
References
- ↑ Lowe, Andrew. "(120132) 2003 FY128 Precovery Images". http://andrew-lowe.ca/120132.htm.
- ↑ 2.0 2.1 Marc W. Buie (2006-04-02). "Orbit Fit and Astrometric record for 120132". SwRI (Space Science Department). http://www.boulder.swri.edu/~buie/kbo/astrom/120132.html. Retrieved 2009-01-22.
- ↑ 3.0 3.1 3.2 "JPL Small-Body Database Browser: 120132 (2003 FY128)". https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=120132. Retrieved 7 April 2016.
- ↑ 4.0 4.1 4.2 Santos-Sanz, P.; Lellouch, E.; Fornasier, S.; Kiss, C.; Pal, A.; Müller, T. G.; Vilenius, E.; Stansberry, J. et al. (2012). ""TNOs are Cool": A survey of the trans-Neptunian region". Astronomy & Astrophysics 541: A92. doi:10.1051/0004-6361/201118541. Bibcode: 2012A&A...541A..92S.
External links
Original source: https://en.wikipedia.org/wiki/(120132) 2003 FY128.
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