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Q85904204

rotating variable star in the constellation Lyra
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Q85904204

Summary

Q85904204 is a rotating variable star[1].

Key Facts

  • Q85904204's instance of is recorded as rotating variable star[2].
  • Q85904204's constellation is recorded as Lyra[3].
  • Q85904204's spectral class is recorded as G5[4].
  • Q85904204's catalog code is recorded as KIC 8409779[5].
  • Q85904204's catalog code is recorded as 2MASS J18463536+4426075[6].
  • Q85904204's catalog code is recorded as Gaia DR2 2117402212455657984[7].
  • Q85904204's type of variable star is recorded as rotating variable star[8].
  • Q85904204's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.495'}[9].
  • Q85904204's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.026'}[10].
  • Q85904204's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.931'}[11].
  • Q85904204's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.8173'}[12].
  • Q85904204's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-29.5'}[13].
  • Q85904204's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-13.2'}[14].
  • Q85904204's metallicity is recorded as {'unit': '1', 'amount': '+0.03'}[15].
  • Q85904204's metallicity is recorded as {'unit': '1', 'amount': '+0.07'}[16].
  • Q85904204's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+281.64730331646960'}[17].
  • Q85904204's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.43541082654320'}[18].
  • Q85904204's epoch is recorded as J2000.0[19].
  • Q85904204's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5316'}[20].
  • Q85904204's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5208'}[21].
  • Q85904204's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+21000'}[22].
  • Q85904204's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+24500'}[23].

Body

Definition and Type

Q85904204's instance of is recorded as rotating variable star[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] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. wikidata.org.
  8. [9] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  9. [10] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  10. [11] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  11. [12] ↑ . Gaia Data Release 2. wikidata.org.
  12. [13] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  13. [14] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  14. [15] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  15. [16] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  20. [21] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  21. [22] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  22. [23] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.

Class ancestry

  1. [1] ↑ . Wikidata. wikidata.org.

📑 Cite this page

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). Q85904204. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85904204
MLA “Q85904204.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85904204.
BibTeX @misc{4ortxyz_q85904204_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85904204}}, year = {2026}, url = {https://4ort.xyz/entity/q85904204}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85904204 — https://4ort.xyz/entity/q85904204 (retrieved 2026-05-07)

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