Discovery | |
---|---|
Discovered by | Pan-STARRS |
Discovery date | 6 June 2011 |
Orbital characteristics[4] | |
Epoch | 20 Mar 2012 (JD 2456006.5) |
Observation arc | 3.27 years |
Number of observations | 5413 |
Orbit type | Oort cloud |
Aphelion | 68000 AU (inbound)[1] 4500 AU (outbound) |
Perihelion | 0.30161 AU (q) |
Eccentricity | 1.000087 |
Orbital period | Millions of years (inbound) ~107,000 yr (outbound solution for epoch 2050)[1] |
Max. orbital speed | 76.7 km/s (172,000 mph)[2] |
Inclination | 84.199° |
Last perihelion | 10 March 2013[3] |
Jupiter MOID | 0.17 AU |
C/2011 L4 (PanSTARRS), also known as Comet PANSTARRS, is a non-periodic comet discovered in June 2011 that became visible to the naked eye when it was near perihelion in March 2013.[5][6] It was discovered using the Pan-STARRS telescope located near the summit of Haleakalā, on the island of Maui in Hawaii. Comet C/2011 L4 probably took millions of years to come from the Oort cloud. After leaving the planetary region of the Solar System, the post-perihelion orbital period (epoch 2050) is estimated to be roughly 107000 years.[1] Dust and gas production suggests the comet nucleus is roughly 1 kilometer (0.62 mi) in diameter,[7] while based on the absolute nuclear magnitude and a geometric albedo of 0.04 the diameter of the nucleus is over 2.4 kilometers (1.5 mi).[8] A method based on coma magnitude decay function estimated the effective radius at 2.317 ± 0.190 km.[9]
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