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HD 123657

star in the constellation Boötes

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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 authorityQ1749017
Source-derived summary

HD 123657 (BY Boötis) is a star in the northern constellation of Boötes, near the end of the handle of the Big Dipper. It is a fifth-magnitude star, and can be spotted to the unaided eye in sufficiently dark skies, far from light pollution. Based on stellar parallax measurements, it is about 540 light-years distant.

This is a slow irregular variable with an apparent magnitude varying between 4.98 and 5.33. The variability of the brightness of HD 123657 was announced by Joel Stebbins and Charles Morse Huffer in 1928, based on observations made at Washburn Observatory. The star was given its variable star designation, BY Boötis, in 1973.

HD 123657 has a spectral classification of M4.5III, placing it as a cool red giant that exhausted its hydrogen supply.

Editorial summary

The public source identifies “HD 123657” as star in the constellation Boötes. This brief keeps that definition visible, then builds a research path around star, constellation and Boötes.

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—1928, 1973—that can be checked directly. The selected authority fields contribute no independent date. Its value is orientation rather than verdict, with star, constellation and Boötes providing the first useful test.
Editorial analysis

Why this record matters

A short description can identify a subject without explaining its stakes. For “HD 123657”, the useful work is to connect “star in the constellation Boötes” to the records capable of establishing context and consequence.

Evidence profile

Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Aug 23, 2026. The linked authority identifier is Q1749017. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1928 and 1973.

Critical limits

The absence of detail may reflect summary conventions rather than a lack of surviving documentation. 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.

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  1. Establish the record: confirm the title “HD 123657”, its source revision and the description used here.
  2. Expand the search: follow HD 123657 primary sources, HD 123657 archive and star 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.

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Source & attribution

This entry incorporates text from HD 123657” 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.