Astronomy:(120132) 2003 FY128

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(120132) 2003 FY128
2003fy128-19960410.gif
Precovery image of 2003 FY128 taken by the Palomar Observatory in 1996[1]
Discovery
Discovered byNEAT
Discovery date26 March 2003
Designations
(120132) 2003 FY128
none
Minor planet categorydetached object[2]
Orbital characteristics[3]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc8159 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)
Eccentricity0.25584
Orbital period351.53 yr (128397 d)
Mean anomaly28.257°
Mean motion0° 0m 10.094s / day
Inclination11.757°
Longitude of ascending node341.68°
175.26°
Earth MOID36.0755 AU (5.39682 Tm)
Jupiter MOID31.6621 AU (4.73658 Tm)
Physical characteristics
Dimensions460±21 km[4]
Rotation period8.54 h (0.356 d)
Geometric albedo0.079±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

  1. Lowe, Andrew. "(120132) 2003 FY128 Precovery Images". http://andrew-lowe.ca/120132.htm. 
  2. 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. 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. 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. Bibcode2012A&A...541A..92S. 

External links