Discovery | |
---|---|
Discovered by | K. Korlević |
Discovery site | Višnjan Obs. |
Discovery date | 23 October 1998 |
Designations | |
MPC designation | (10415) Mali Lošinj |
Named after
|
Mali Lošinj (Croatian island) |
1998 UT15 · 1925 VM 1962 WE1 · 1977 TN3 1987 SW20 · 1988 VW7 |
|
main-belt · (outer) | |
Orbital characteristics | |
Epoch 16 February 2017 (JD 2457800.5) | |
Uncertainty parameter 0 | |
Observation arc | 53.71 yr (19,616 days) |
Aphelion | 3.0657 AU |
Perihelion | 2.9117 AU |
2.9887 AU | |
Eccentricity | 0.0258 |
5.17 yr (1,887 days) | |
82.480° | |
0° 11m 26.88s / day | |
Inclination | 14.426° |
221.70° | |
298.92° | |
Physical characteristics | |
Dimensions |
±0.135 13.514 ±0.112 km 14.912 ±0.70 km 16.20 18.77 km (calculated) |
±20.6153 240.5115h | |
0.057 (assumed) ±0.019 0.128 ±0.0344 0.1521 |
|
C · X | |
±0.44 · 11.8 · 11.9 · 11.54±0.002 (R) · 12.36 11.911 | |
10415 Mali Lošinj, provisional designation 1998 UT15, is a dark asteroid and very slow rotator from the outer region of the asteroid belt, approximately 16 kilometers in diameter. It was discovered by Croatian astronomer Korado Korlević at Višnjan Observatory, Croatia, on 23 October 1998.
The C-type asteroid is also classified as a X-type body. It orbits the Sun at a distance of 2.9–3.1 AU once every 5 years and 2 months (1,887 days). Its orbit has an eccentricity of 0.03 and an inclination of 14° with respect to the ecliptic. The first used precovery was obtained at Goethe Link Observatory in 1962, extending the asteroid's observation arc by 36 years prior to its discovery. The first unused observations were made at Heidelberg Observatory in 1925.
In 2013, photometric observations at the U.S. Palomar Transient Factory, California, rendered an rotational light-curve that showed a rotation period of ±20.6153 hours with a brightness amplitude of 0.48 in 240.5115magnitude (U=2). A body of this size usually rotates within hours once around its axis.