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Z Canis Majoris

variable star in the constellation Canis Major

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 9, 2026
Entity authorityQ5174381 ↗
Source-derived summary

Z Canis Majoris (Z CMa) is a B-type star in the constellation of Canis Major. It has an average apparent visual magnitude of approximately 10, though has brightened by 1-2 magnitudes in irregular outbursts in 1987, 2000, 2004 and 2008.

Arville D. Walker of the Harvard College Observatory discovered that the star is a variable star, from the examination of 275 photographs taken between 1899 and 1921. Her discovery was announced in 1921, and the star received its variable star designation, Z Canis Majoris, in 1922.

The star is a complex binary system only 300,000 years old with two main components separated by about 250 astronomical units (AU). The southeast component is an FU Orionis star (a type of pre-main-sequence star in a phase of very high mass accretion resulting in an accretion disk which dominates the optical spectrum) that is 1,300 times as luminous as the Sun, has 3 times its mass and 13 times its diameter and a surface temperature of 10,000 K. The northwest component is a Herbig Ae/Be star that has been calculated to be 12 times as massive as the Sun with a dust shell photosphere 1,690±30 times its diameter and a blackbody temperature of 980 K, the star shines with a luminosity 2,400 times greater than that of the sun, though there is some uncertainty about its properties. It is enveloped in an irregular roughly spherical cocoon of dust that has an inner diameter of 20 and outer diameter of 50 AU. The cocoon has a hole in it through which light shines that covers an angle of 5 to 10 degrees of its circumference. Both stars are surrounded by a large envelope of in-falling material that left over from the original cloud that formed the system. Both stars are emitting jets of material, that of the Herbig Ae/Be star being much larger - up to 11.7 light-years (3.6 parsecs) long.

It is unclear whether the most recent (and brightest) brightening in 2008 was due to the Herbig Ae/Be star increasing in luminosity or a hole appearing in the cocoon.

Editorial summary

Begin with the source’s own compact description: “Z Canis Majoris” is variable star in the constellation Canis Major. The dossier treats that line as a proposition to test through Canis, Majoris and variable, not as a finished interpretation.

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—1987, 2000, 2004, 2008—that can be checked directly. The selected authority fields contribute no independent date. For this dossier, Canis, Majoris and variable is the immediate research focus.
Editorial analysis

Why this record matters

The phrase “variable star in the constellation Canis Major” 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.

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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 9, 2026. The linked authority identifier is Q5174381. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1987, 2000, 2004 and 2008.

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Source & attribution

This entry incorporates text from “Z Canis Majoris” 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.