NGC 60
spiral galaxy in the constellation Pisces

NGC 60 is an Sc type spiral galaxy in the Pisces constellation. It was discovered on 2 November 1882 by Édouard Stephan.
NGC 60 is noticed for its unusually distorted spiral arms, which are commonly due to gravitational effects of neighboring galaxies, but there are no galaxies around NGC 60 to allow this.
Supernova
One supernovae has been observed in NGC 60:
SN 2023zba (Type II-P, mag. 18.8) was discovered by the Catalina Real-time Transient Survey on 7 December 2023.
Begin with the source’s own compact description: “NGC 60” is spiral galaxy in the constellation Pisces. The dossier treats that line as a proposition to test through spiral, galaxy and constellation, not as a finished interpretation.
Why this record matters
The phrase “spiral galaxy in the constellation Pisces” supplies a clear boundary for inquiry. It also exposes the unanswered questions: who defined that boundary, when it became stable and which sources sit outside it.
Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Sep 3, 2026. The linked authority identifier is Q50654. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1882 and 2023.
Overview language is designed for orientation and should not be treated as a substitute for the evidence cited beneath it. The lead is largely declarative, so disagreement and counter-evidence require a deliberate search beyond the opening account. 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 “NGC 60”, its source revision and the description used here.
- Expand the search: follow NGC 60 primary sources, NGC 60 archive and spiral 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 “NGC 60”?
- What terminology or title could unlock a more precise catalogue search?
- Which cited source is closest to the event, object or claim?
Search terms from this dossier
This entry incorporates text from “NGC 60” 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.