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Alpha Caeli

star in the constellation Caelum

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 26, 2026
Entity authorityQ1196004 ↗
Source-derived summary

Alpha Caeli is a binary star system in the southern constellation Caelum. Its name is a Bayer designation that is Latinized from α Caeli, and abbreviated Alpha Cae or α Cae. With a combined apparent visual magnitude of 4.45, it is only visible to the naked eye in places far from light pollution, but still is the brightest star in the constellation. Parallax measurements by the Gaia spacecraft indicate a distance of 66.48 light-years (20.38 pc) to Alpha Caeli. It has a relatively low radial velocity, estimated at 0.7 km/s relative to the Sun.

This system consists of an F-type star of magnitude 4.46 and a small red dwarf of magnitude 12.5. As of 2008, they are separated by 6.6" in the sky. A debris disk has been detected around the primary component of the system.

Physical properties

Primary

The primary component (α Caeli A) has a spectral classification of F2V, meaning that it is an ordinary F-type main-sequence star, currently fusing hydrogen into helium at its core. It is estimated to be 1.5 billion years old, has 50% more mass and has 1.55 times the Sun's radius.

Editorial summary

The public source identifies “Alpha Caeli” as star in the constellation Caelum. This brief keeps that definition visible, then builds a research path around Alpha, Caeli and star.

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—2008—that can be checked directly. The selected authority fields contribute no independent date. Its value is orientation rather than verdict, with Alpha, Caeli and star providing the first useful test.
Editorial analysis

Why this record matters

A short description can identify a subject without explaining its stakes. For “Alpha Caeli”, the useful work is to connect “star in the constellation Caelum” 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 26, 2026. The linked authority identifier is Q1196004. None of the 0 selected statements returned an explicit reference. The first chronological checks are 2008.

Critical limits

The absence of detail may reflect summary conventions rather than a lack of surviving documentation. 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
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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 “Alpha Caeli”, its source revision and the description used here.
  2. Expand the search: follow Alpha Caeli primary sources, Alpha Caeli archive and Alpha 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 “Alpha Caeli”?
  2. Which cited source is closest to the event, object or claim?
  3. Which institution is responsible for the underlying evidence?
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Source & attribution

This entry incorporates text from “Alpha Caeli” 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.