| Discovery | |
|---|---|
| Discovered by | WISE Catalina Sky Survey |
| Discovery date | 3–9 June 2010 28 October 2010 |
| Designations | |
| 2010 TJ175 | |
| Active asteroid Outer main-belt | |
| Orbital characteristics [1] [2] | |
| Epoch 21 November 2025 (JD 2461000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 21.58 years |
| Earliest precovery date | 16 October 2001 |
| Aphelion | 3.719 AU |
| Perihelion | 1.765 AU |
| 2.742 AU | |
| Eccentricity | 0.35636 |
| 4.539 years | |
| 131.10° | |
| Inclination | 10.897° |
| 53.625° | |
| 290.46° | |
| Earth MOID | 0.792 AU |
| Jupiter MOID | 1.842 AU |
| Physical characteristics [1] | |
| 0.5±0.1 km [3] | |
| 2 hours [3] | |
| 0.243 | |
| (g–r) = 0.44±0.07 [4] | |
| 17.36 | |
2010 LH15 is an unnamed active asteroid located in the outer main asteroid belt. It was first discovered by the Wide-field Infrared Survey Explorer satellite between 3 and 9 June 2010, and later on October 2010 by the Catalina Sky Survey, the latter of which mistakenly identified it as a separate object named 2010 TJ175. [5] In 2023, Colin O. Chandler later reported that cometary activity was detected from DECam imagery taken in September 2019, [6] likely caused by sublimation of material from its surface. [4]