168P/Hergenrother
periodic comet in the Solar System

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 (16 in) 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.
The public source identifies “168P/Hergenrother” as periodic comet in the Solar System. This brief keeps that definition visible, then builds a research path around 168P, Hergenrother and periodic.
Why this record matters
A short description can identify a subject without explaining its stakes. For “168P/Hergenrother”, the useful work is to connect “periodic comet in the Solar System” to the records capable of establishing context and consequence.
Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Sep 22, 2026. The linked authority identifier is Q3272131. The first chronological checks are 1998, 2005, 2020 and 2012.
The absence of detail may reflect summary conventions rather than a lack of surviving documentation. The source lead contains qualifying language; that uncertainty should survive quotation, summary and reuse. Authority statements aid reconciliation but still require their own references, qualifiers and ranks to be checked.
How to read it
Use the entry as an orientation point, then follow its citations and revision history. Names, dates and institutional relationships should be checked against the original record.
- Subject orientation
- Search vocabulary
- Locating named sources
The closest primary source, responsible institution and strongest cited specialist reference.
Three-step research path
- Establish the record: confirm the title “168P/Hergenrother”, its source revision and the description used here.
- Expand the search: follow 168P/Hergenrother primary sources, 168P/Hergenrother archive and 168P research across catalogues and specialist indexes.
- Test the account: compare the strongest cited source with the responsible institution’s current record and note any disagreement.
Questions for further research
- Which source most directly establishes the central claim about “168P/Hergenrother”?
- What terminology or title could unlock a more precise catalogue search?
- Which institution is responsible for the underlying evidence?
Search terms from this dossier
This entry incorporates text from “168P/Hergenrother” on English Wikipedia. Contributors are listed in the page history. Text is available under the Creative Commons Attribution-ShareAlike 4.0 License. Selected authority identifiers and statements are retrieved from Wikidata under CC0; their references and qualifiers remain part of the verification path.