Skip to content
Surf Wiki
Save to docs
general/periodic-comets

From Surf Wiki (app.surf) — the open knowledge base

168P/Hergenrother

Periodic comet


Periodic comet

FieldValue
name168P/Hergenrother
image168p-hergenrother.jpg
caption168P/Hergenrother during its 2012 outburst as imaged from the Mount Lemmon Observatory
discovery_ref
discovererCarl W. Hergenrother
discovery_siteCatalina Sky Survey
discovery_date22 November 1998
mpc_nameP/1998 W2, P/2005 N2
orbit_ref
epoch25 February 2023 (JD 2460000.5)
observation_arc21.12 years
earliest_precovery_date21 November 1998
obs3,631
perihelion1.357 AU
aphelion5.817 AU
semimajor3.587 AU
period6.794 years
eccentricity0.62169
inclination21.615°
asc_node355.43°
arg_peri15.041°
mean188.01°
tjup2.663
Earth_moid0.420 AU
Jupiter_moid0.001 AU
physical_ref
mean_diameter0.91 km
M17.0
M215.2
magnitude8.0
(2012 apparition)
last_p5 August 2019
next_p18 May 2026

(2012 apparition)

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. It was last observed in January 2020 and may have continued fragmenting after the 2012 outburst.

Observational history

Discovery

On 22 November 1998, Carl W. Hergenrother spotted a new comet from CCD images taken by Timothy B. Spahr a day earlier with the Catalina Sky Survey's 0.41 m telescope. Preliminary orbital calculations by Brian G. Marsden reveal that the comet has a periodic orbit of 6.78 years. At the time, the comet was a 17th-magnitude object within the constellation Ursa Minor.

Between 2000 and 2002, Kazuo Kinoshita and Shuichi Nakano independently used the comet's positions during its 1998 apparition to predict its next perihelion date, which is around 2 November 2005. It was successfully recovered by Australian astronomer, David Herald, on 6 November 2005.

2012 outburst

The comet came to perihelion on 1 October 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 19 October, images by the Virtual Telescope Project showed a dust cloud trailing the nucleus. Images by the 2 m Faulkes Telescope North on 26 October, confirm a fragmentation event. The secondary fragment was about magnitude 17. Further observations by the 8.1 m Gemini telescope show that the comet fragmented into at least four parts in six fragmentation events.

2019 apparition

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

Physical characteristics

Observations conducted by the Spitzer Space Telescope between 2006 and 2007 showed that Hergenrother's nucleus was originally about 0.96 km in diameter before it fragmented on its 2012 outburst. This was later revised to 0.91 km upon reanalysis of data in 2020.

References

Notes

Citations

| access-date= 2025-04-01 }}

| display-authors= 5

| access-date= 2025-04-01 }}

| access-date= 2025-04-01

| access-date= 2016-10-18 }}

| access-date= 2014-06-20 }}

| access-date= 2012-02-20 }}

| doi-access= free }}

| access-date= 2012-11-06 | archive-date= 2012-11-08 | archive-url= https://web.archive.org/web/20121108035433/http://blogs.discovermagazine.com/badastronomy/2012/11/05/breaking-up-is-easy-to-do-if-youre-a-comet/ | url-status= dead }}

| access-date= 2012-10-28 }}

| access-date= 2012-02-25 }}

Info: Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

Want to explore this topic further?

Ask Mako anything about 168P/Hergenrother — get instant answers, deeper analysis, and related topics.

Research with Mako

Free with your Surf account

Content sourced from Wikipedia, available under CC BY-SA 4.0.

This content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.

Report