CACrown ArchivesThe cinema collection
EN/FR
Search
Menu
Research dossier · General Reference

NGC 4260

galaxy

Cross-disciplinary reference desk with index cards, atlas, dictionary and catalogue
General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 3, 2026
Entity authorityQ1110237 ↗
Source-derived summary

NGC 4260 is a barred spiral galaxy in the constellation Virgo. Its velocity with respect to the cosmic microwave background is 2,122±24 km/s, which corresponds to a Hubble distance of 102.1 ± 7.2 Mly (31.29 ± 2.22 Mpc). However, six non-redshift measurements give a much farther distance of 131.33 ± 6.17 Mly (40.267 ± 1.891 Mpc). It was discovered by German-British astronomer William Herschel on 13 April 1784.

Editorial summary

The public source identifies “NGC 4260” as galaxy. This brief keeps that definition visible, then builds a research path around galaxy.

Editorial reviewA dependable orientation record for establishing vocabulary, names and a first evidence trail. The current lead gives the account dated anchors—1784—that can be checked directly. The selected authority fields contribute no independent date. Its value is orientation rather than verdict, with galaxy providing the first useful test.
Editorial analysis

Why this record matters

A short description can identify a subject without explaining its stakes. For “NGC 4260”, the useful work is to connect “galaxy” to the records capable of establishing context and consequence.

Evidence profile

The citation trail is more important than the brevity of the summary: it shows where individual claims can be examined in context. The source revision retrieved here is dated Sep 3, 2026. The linked authority identifier is Q1110237. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1784.

Critical limits

Overview language is designed for orientation and should not be treated as a substitute for the evidence cited beneath it. 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.

Best used for
  • Subject orientation
  • Search vocabulary
  • Locating named sources
Verify next

The closest primary source, responsible institution and strongest cited specialist reference.

Three-step research path

  1. Establish the record: confirm the title “NGC 4260”, its source revision and the description used here.
  2. Expand the search: follow NGC 4260 primary sources, NGC 4260 archive and galaxy research across catalogues and specialist indexes.
  3. Test the account: compare the strongest cited source with the responsible institution’s current record and note any disagreement.

Questions for further research

  1. Which source most directly establishes the central claim about “NGC 4260”?
  2. What terminology or title could unlock a more precise catalogue search?
  3. Which institution is responsible for the underlying evidence?
Subject index

Search terms from this dossier

Source & attribution

This entry incorporates text from “NGC 4260” 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.