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Research dossier · General Reference

NGC 895

galaxy in the constellation Cetus

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 3, 2026
Entity authorityQ1040034 ↗
Source-derived summary

NGC 895 is an unbarred spiral galaxy located around 98 million light-years away in the constellation Cetus. NGC 895 was discovered November 28, 1856 by R. J. Mitchell. NGC 895 is not known to have much star-formation, and is not known to have an active galactic nuclei.

Editorial summary

This brief starts where responsible research should: with the source description of “NGC 895” as galaxy in the constellation Cetus. Everything that follows is an evidence route, not borrowed authority.

Editorial reviewA dependable orientation record for establishing vocabulary, names and a first evidence trail. The current lead gives the account dated anchors—1856—that can be checked directly. The selected authority fields contribute no independent date. The account is most persuasive where galaxy, constellation and Cetus can be independently traced.
Editorial analysis

Why this record matters

The subject matters to the general reference register because the source frames it as galaxy in the constellation Cetus. Its deeper value depends on whether names, dates, institutions and citations support that framing.

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 Q1040034. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1856.

Critical limits

The absence of detail may reflect summary conventions rather than a lack of surviving documentation. 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.

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 895”, its source revision and the description used here.
  2. Expand the search: follow NGC 895 primary sources, NGC 895 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 895”?
  2. Which cited source is closest to the event, object or claim?
  3. What terminology or title could unlock a more precise catalogue search?
Subject index

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Source & attribution

This entry incorporates text from “NGC 895” 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.