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Q92331817

W Ursae Majoris variable star in the constellation Cassiopeia
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Q92331817

Summary

Q92331817 is a W Ursae Majoris variable[1].

Key Facts

  • Q92331817's instance of is recorded as W Ursae Majoris variable[2].
  • Q92331817's constellation is recorded as Cassiopeia[3].
  • Q92331817's catalog code is recorded as SBC9 1457[4].
  • Q92331817's catalog code is recorded as CSV 8883[5].
  • Q92331817's catalog code is recorded as GSC 04009-00534[6].
  • Q92331817's catalog code is recorded as NSV 14717[7].
  • Q92331817's catalog code is recorded as SV* BV 326[8].
  • Q92331817's catalog code is recorded as TYC 4009-534-1[9].
  • Q92331817's catalog code is recorded as 1RXS J234833.8+574505[10].
  • Q92331817's catalog code is recorded as UCAC4 739-097062[11].
  • Q92331817's catalog code is recorded as Gaia DR1 1998315894757138816[12].
  • Q92331817's catalog code is recorded as WEB 20682[13].
  • Q92331817's catalog code is recorded as Gaia DR2 1998315899062115072[14].
  • Q92331817's catalog code is recorded as V651 Cas[15].
  • Q92331817's type of variable star is recorded as eclipsing binary star[16].
  • Q92331817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.76'}[17].
  • Q92331817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.21'}[18].
  • Q92331817's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.0355'}[19].
  • Q92331817's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.3290'}[20].
  • Q92331817's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-58.90'}[21].
  • Q92331817's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-8.43'}[22].
  • Q92331817's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-59.20'}[23].
  • Q92331817's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+5.61'}[24].
  • Q92331817's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+107.1926'}[25].
  • Q92331817's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+40.0'}[26].

Body

Definition and Type

Q92331817's instance of is recorded as W Ursae Majoris variable[2].

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

  1. [2] ↑ . SIMBAD. wikidata.org.
  2. [3] ↑ . wikidata.org.
  3. [4] ↑ . SIMBAD. wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . SIMBAD. wikidata.org.
  8. [9] ↑ . SIMBAD. wikidata.org.
  9. [10] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . SIMBAD. wikidata.org.
  12. [13] ↑ . SIMBAD. wikidata.org.
  13. [14] ↑ . SIMBAD. wikidata.org.
  14. [15] ↑ . wikidata.org.
  15. [16] ↑ . Catalogue of suspected variable stars. Moscow, Acad. of Sciences USSR Shternberg,1951 (1981). wikidata.org.
  16. [17] ↑ . The Tycho-2 catalogue of the 2.5 million brightest stars. wikidata.org.
  17. [18] ↑ . The Tycho-2 catalogue of the 2.5 million brightest stars. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.
  21. [22] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.
  22. [23] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.
  23. [24] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.
  24. [25] ↑ . Gaia Data Release 2. wikidata.org.
  25. [26] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.

Class ancestry

  1. [1] ↑ . Wikidata. wikidata.org.

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Use these citations when quoting this entity in research, articles, AI prompts, or wherever provenance matters. We aggregate Wikidata + Wikipedia + authoritative open-data sources; the stitched, scored, cross-referenced view is what 4ort.xyz contributes.

APA 4ort.xyz Knowledge Graph. (2026). Q92331817. Retrieved May 7, 2026, from https://4ort.xyz/entity/q92331817
MLA “Q92331817.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q92331817.
BibTeX @misc{4ortxyz_q92331817_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q92331817}}, year = {2026}, url = {https://4ort.xyz/entity/q92331817}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q92331817 — https://4ort.xyz/entity/q92331817 (retrieved 2026-05-07)

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