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Gliese Catalogue of Nearby Stars

star catalogue

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionAug 23, 2026
Entity authorityQ1045111 ↗
Source-derived summary

The Gliese Catalogue of Nearby Stars (German pronunciation: [ˈɡliːzə], English GLEE-zə) is a star catalogue listing stars located within 25 parsecs (82 ly) of the Sun.

First edition and supplements

In 1957, German astronomer Wilhelm Gliese published his first star catalogue of 915 known stars within 20 parsecs (65 ly) of Earth, listing their known properties and ordered geographically by right ascension. Stars in the first catalogue are designated by coding GL NNN, the N representing the consecutive integer number based on this order.

Gliese published an update as the Catalogue of Nearby Stars in 1969, all known stars to 22 parsecs (72 ly), which catalogued 1,529 stars, encoded as Gl NNN.NA (prefix Gl and the entries of twelve years before gained a .0 affix; the more than 500 additional stars were recorded using interspersed 0.1, 0.2 etc. numbering). This list therefore numbered from 1.0 to 915.0 as no stars were entered after 915.0. and retained a strict right ascension order.

A Supplement published in 1970 by Richard van der Riet Woolley and associates, extended the range out to 25 parsecs (82 ly). This supplement added catalogue numbers in the range 9001–9850 using the now deprecated Wo prefix, sharing today the GJ prefix given to the later series of the catalogues.

Succeeding editions

Gliese published an extension to the second edition of the catalogue in 1979 in collaboration with Hartmut Jahreiß.

Editorial summary

“Gliese Catalogue of Nearby Stars” enters the record as star catalogue. Crown Archives preserves that source wording while asking what Gliese, Catalogue and Nearby can confirm, complicate or overturn.

Editorial reviewA concise reference frame for defining the subject, testing terminology and identifying the institution closest to the evidence. The current lead gives the account dated anchors—1957, 1969, 1970, 1979—that can be checked directly. The linked authority record independently contributes the date 1957. Its strongest next move is a source search built around Gliese, Catalogue and Nearby.
Editorial analysis

Why this record matters

“Gliese Catalogue of Nearby Stars” is worth following because a concise public description often conceals a longer documentary argument. Here, Gliese, Catalogue and Nearby provides the most credible route into that argument.

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 Aug 23, 2026. The linked authority identifier is Q1045111. None of the 2 selected statements returned an explicit reference. The first chronological checks are 1957, 1969, 1970 and 1979.

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.

Best used for
  • Subject orientation
  • Search vocabulary
  • Locating named sources
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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 “Gliese Catalogue of Nearby Stars”, its source revision and the description used here.
  2. Expand the search: follow Gliese Catalogue of Nearby Stars primary sources, Gliese Catalogue of Nearby Stars archive and Gliese 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 “Gliese Catalogue of Nearby Stars” 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.