168P/Hergenrother Explained

168P/Hergenrother
Discoverer:Carl W. Hergenrother
Discovery Date:November 22, 1998
Designations:P/1998 W2
P/2005 N2
Epoch:March 6, 2006
Semimajor:3.632 AU
Perihelion:1.426 AU
Aphelion:5.839 AU
Eccentricity:0.6075
Period:6.923 a
Inclination:21.8934°
Last P:August 5, 2019
October 1, 2012
November 2, 2005
Next P:2026-May-18
Earth Moid:0.4abbr=unitNaNabbr=unit

168P/Hergenrother is a periodic comet in the Solar System. The comet originally named P/1998 W2 returned in 2005 and got the temporary name P/2005 N2. The comet was last observed in January 2020, and may have continued fragmenting after the 2012 outburst.

2012 outburst

The comet came to perihelion on October 1, 2012, and was expected to reach about apparent magnitude 15.2, but due to an outburst the comet reached apparent magnitude 8. As a result of the outburst of gas and dust, the comet was briefly more than 500 times brighter than it would have been without the outburst. On October 19, 2012, images by the Virtual Telescope Project showed a dust cloud trailing the nucleus. Images by the 2m (07feet) Faulkes Telescope North on October 26, 2012, confirm a fragmentation event. The secondary fragment was about magnitude 17. Further observations by the 8.1m (26.6feet) Gemini telescope show that the comet fragmented into at least four parts.

2019

168P came to perihelion on August 5, 2019, when it was 76 degrees from the Sun. It then made a closest approach to Earth on 6 November 6, 2019, when it was 1abbr=unitNaNabbr=unit from Earth with a solar elongation of about 110 degrees. It was not recovered until January 3, 2020, when it was 141 degrees from the Sun, but only two observations on a single night were reported.

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