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Q89095681

Algol variable in the constellation Lyra
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Q89095681

Summary

Q89095681 is an Algol variable[1].

Key Facts

  • Q89095681's instance of is recorded as Algol variable[2].
  • Q89095681's constellation is recorded as Lyra[3].
  • Q89095681's spectral class is recorded as A3V[4].
  • Q89095681's spectral class is recorded as A4V[5].
  • Q89095681's catalog code is recorded as GSC 03124-01348[6].
  • Q89095681's catalog code is recorded as TYC 3124-1348-1[7].
  • Q89095681's catalog code is recorded as 2MASS J19033272+3941003[8].
  • Q89095681's catalog code is recorded as ASAS J190333+3941.0[9].
  • Q89095681's catalog code is recorded as KIC 4544587[10].
  • Q89095681's catalog code is recorded as Gaia DR1 2100291234547472768[11].
  • Q89095681's catalog code is recorded as Gaia DR2 2100291238846888192[12].
  • Q89095681's type of variable star is recorded as eclipsing binary star[13].
  • Q89095681's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.577'}[14].
  • Q89095681's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.523'}[15].
  • Q89095681's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.482'}[16].
  • Q89095681's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.582'}[17].
  • Q89095681's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.83'}[18].
  • Q89095681's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.95'}[19].
  • Q89095681's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.7501'}[20].
  • Q89095681's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3447'}[21].
  • Q89095681's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-47.9'}[22].
  • Q89095681's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.8'}[23].
  • Q89095681's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-21.1'}[24].
  • Q89095681's metallicity is recorded as {'unit': '1', 'amount': '-0.24'}[25].
  • Q89095681's metallicity is recorded as {'unit': '1', 'amount': '-0.22'}[26].

Body

Definition and Type

Q89095681's instance of is recorded as Algol 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] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  4. [5] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. 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] ↑ . Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  14. [15] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  15. [16] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  16. [17] ↑ . The All Sky Automated Survey. The Catalog of Variable Stars in the Kepler field of view. wikidata.org.
  17. [18] ↑ . The Tycho-2 catalogue of the 2.5 million brightest stars. wikidata.org.
  18. [19] ↑ . The Tycho-2 catalogue of the 2.5 million brightest stars. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. 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.
  23. [24] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  24. [25] ↑ . Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.. wikidata.org.
  25. [26] ↑ . 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). Q89095681. Retrieved May 7, 2026, from https://4ort.xyz/entity/q89095681
MLA “Q89095681.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q89095681.
BibTeX @misc{4ortxyz_q89095681_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q89095681}}, year = {2026}, url = {https://4ort.xyz/entity/q89095681}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q89095681 — https://4ort.xyz/entity/q89095681 (retrieved 2026-05-07)

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