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Q85912224

rotating variable star in the constellation Lyra
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Q85912224

Summary

Q85912224 is a rotating variable star[1].

Key Facts

  • Q85912224's instance of is recorded as rotating variable star[2].
  • Q85912224's constellation is recorded as Lyra[3].
  • Q85912224's spectral class is recorded as F6IV[4].
  • Q85912224's catalog code is recorded as KIC 7677340[5].
  • Q85912224's catalog code is recorded as 2MASS J19201032+4321263[6].
  • Q85912224's catalog code is recorded as Gaia DR2 2102807535627259136[7].
  • Q85912224's type of variable star is recorded as rotating variable star[8].
  • Q85912224's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.465'}[9].
  • Q85912224's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.225'}[10].
  • Q85912224's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.121'}[11].
  • Q85912224's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.5277'}[12].
  • Q85912224's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-33.7'}[13].
  • Q85912224's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-53.5'}[14].
  • Q85912224's metallicity is recorded as {'unit': '1', 'amount': '+0.02'}[15].
  • Q85912224's metallicity is recorded as {'unit': '1', 'amount': '-0.05'}[16].
  • Q85912224's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+290.04302470894450'}[17].
  • Q85912224's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.35733470312750'}[18].
  • Q85912224's epoch is recorded as J2000.0[19].
  • Q85912224's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6048'}[20].
  • Q85912224's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6028'}[21].
  • Q85912224's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+13200'}[22].
  • Q85912224's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+13800'}[23].

Body

Definition and Type

Q85912224'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). Q85912224. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85912224
MLA “Q85912224.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85912224.
BibTeX @misc{4ortxyz_q85912224_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85912224}}, year = {2026}, url = {https://4ort.xyz/entity/q85912224}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85912224 — https://4ort.xyz/entity/q85912224 (retrieved 2026-05-07)

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