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Ross 695

red dwarf star in the constellation Corvus

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionDec 22, 2025
Entity authorityQ15981315
Source-derived summary

Ross 695, also known as Gliese 465, is a red dwarf star in the southern constellation of Corvus. The distance to this star, based on parallax measurements by the Gaia spacecraft, is 28.947 light-years (8.875 parsecs). It is the nearest star in this constellation. Despite its closeness, this star is intrinsically faint and, at apparent magnitude 11.27, is too faint to be seen with the unaided eye.

This star has a spectral type of M2.0V; with around 26.2% the mass and 27.1% the radius of the Sun, but only 0.98% its luminosity. The effective temperature of the star is 3490 K, giving it a reddish hue. Its iron-to-hydrogen ratio appears to be lower than that of the Sun.

Investigation of its radial velocity has failed to find any evidence of a planetary companion.

Editorial summary

Begin with the source’s own compact description: “Ross 695” is red dwarf star in the constellation Corvus. The dossier treats that line as a proposition to test through Ross, dwarf and star, not as a finished interpretation.

Editorial reviewA dependable orientation record for establishing vocabulary, names and a first evidence trail. The current 133-word lead offers orientation but no explicit four-digit date, so chronology should not be assumed. The selected authority fields contribute no independent date. For this dossier, Ross, dwarf and star is the immediate research focus.
Editorial analysis

Why this record matters

The phrase “red dwarf star in the constellation Corvus” 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.

Evidence profile

Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Dec 22, 2025. The linked authority identifier is Q15981315. None of the 0 selected statements returned an explicit reference.

Critical limits

A concise general-reference account can conceal disagreements about scope, terminology or the weight assigned to individual sources. 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.

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

Three-step research path

  1. Establish the record: confirm the title “Ross 695”, its source revision and the description used here.
  2. Expand the search: follow Ross 695 primary sources, Ross 695 archive and Ross 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

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Source & attribution

This entry incorporates text from Ross 695” 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.