CACrown ArchivesThe cinema collection
Menu
Research dossier · General Reference

42 Orionis

star in the constellation of Orion

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 12, 2026
Entity authorityQ1749342
Source-derived summary

42 Orionis, also known as c Orionis or c Ori, is a triple star system in the constellation Orion. Its apparent magnitude is 4.59 and it is approximately 900 light years away based on parallax.

The primary star, Aa, has one spectroscopic companion Ab of magnitude 6.3 and separation 0.16", and a more distant companion B of 7.5 magnitude at 1.6" separation. Preliminary results published in 2026 give an orbtal period of 69.2 years, an eccentricity of 0.23 and an inclination of 28.1° for the inner companion.

42 Orionis is surrounded by NGC 1977 one of a smaller fainter group of named nebulae just north of the Orion Nebula. 42 Ori is the star which excites and illuminates NGC 1977.

Editorial summary

The public source identifies “42 Orionis” as star in the constellation of Orion. This brief keeps that definition visible, then builds a research path around Orionis, star and constellation.

Editorial reviewA practical starting point whose main value is the path it opens into stronger specialist and primary sources. The current lead gives the account dated anchors—2026, 1977—that can be checked directly. The selected authority fields contribute no independent date. Its value is orientation rather than verdict, with Orionis, star and constellation providing the first useful test.
Editorial analysis

Why this record matters

A short description can identify a subject without explaining its stakes. For “42 Orionis”, the useful work is to connect “star in the constellation of Orion” to the records capable of establishing context and consequence.

Evidence profile

Vocabulary and entity names are the principal evidence signals here, because they determine the precision of every later search. The source revision retrieved here is dated Sep 12, 2026. The linked authority identifier is Q1749342. None of the 0 selected statements returned an explicit reference. The first chronological checks are 2026 and 1977.

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
Verify next

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

Three-step research path

  1. Establish the record: confirm the title “42 Orionis”, its source revision and the description used here.
  2. Expand the search: follow 42 Orionis primary sources, 42 Orionis archive and Orionis 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 “42 Orionis”?
  2. Which institution is responsible for the underlying evidence?
  3. What terminology or title could unlock a more precise catalogue search?
Subject index

Search terms from this dossier

Source & attribution

This entry incorporates text from 42 Orionis” 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.