Astronomy:(120132) 2003 FY128
From HandWiki
| 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
