Kappa Phoenicis
star in the constellation Phoenix
κ Phoenicis, Latinized as Kappa Phoenicis, is a single star in the southern constellation of Phoenix. It is visible to the naked eye as a white-hued point of light with an apparent visual magnitude of 3.94. The distance to this star is approximately 77.7 light years based on parallax, and it is drifting further away with a radial velocity of +11 km/s. It is a member of the Castor Moving Group of co-moving stars.
This object has a stellar classification of A5IVn, which matches the spectrum of an A-type subgiant star with "nebulous" lines due to rapid rotation. It is 348 million years old and is spinning with a projected rotational velocity of 245 km/s. The star has 1.7 times the mass of the Sun and 2.0 times the Sun's radius.
This brief starts where responsible research should: with the source description of “Kappa Phoenicis” as star in the constellation Phoenix. Everything that follows is an evidence route, not borrowed authority.
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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 Dec 20, 2025. The linked authority identifier is Q3812902. None of the 0 selected statements returned an explicit reference.
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This entry incorporates text from “Kappa Phoenicis” 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.