(120132) 2003 FY128, also written as (120132) 2003 FY128, is a trans-Neptunian object.
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. Though if Neptune migrated outward, there would have been a period when Neptune had a higher eccentricity.
It was discovered on March 26, 2003, by the NEAT program at the Palomar Observatory, California.
- ^ a b Marc W. Buie (2006-04-02). "Orbit Fit and Astrometric record for 120132". SwRI (Space Science Department). Retrieved 2009-01-22.
- ^ a b "JPL Small-Body Database Browser: 120132 (2003 FY128)". 2006-04-02 last obs. Retrieved 2009-01-22.
- ^ a b Santos-Sanz, P., Lellouch, E., Fornasier, S., Kiss, C., Pal, A., Müller, T. G., Vilenius, E., Stansberry, J., Mommert, M., Delsanti, A., Mueller, M., Peixinho, N., Henry, F., Ortiz, J. L., Thirouin, A., Protopapa, S., Duffard, R., Szalai, N., Lim, T., Ejeta, C., Hartogh, P., Harris, A. W., & Rengel, M. (2012). “TNOs are Cool”: A Survey of the Transneptunian Region IV - Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS