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Q86853892

rotating variable star in the constellation Lyra
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Q86853892

Summary

Q86853892 is a rotating variable star[1].

Key Facts

  • Q86853892's instance of is recorded as rotating variable star[2].
  • Q86853892's instance of is recorded as star[3].
  • Q86853892's instance of is recorded as near-infrared source[4].
  • Q86853892's constellation is recorded as Lyra[5].
  • Q86853892's spectral class is recorded as M0V[6].
  • Q86853892's child astronomical body is recorded as Q28856660[7].
  • Q86853892's catalog code is recorded as Gaia DR2 2107240324132394496[8].
  • Q86853892's catalog code is recorded as KIC 9573685[9].
  • Q86853892's catalog code is recorded as 2MASS J18575437+4615092[10].
  • Q86853892's catalog code is recorded as KOI-2057[11].
  • Q86853892's catalog code is recorded as Kepler-1074[12].
  • Q86853892's catalog code is recorded as Gaia DR3 2107240324132394496[13].
  • Q86853892's catalog code is recorded as TIC 164724987[14].
  • Q86853892's type of variable star is recorded as rotating variable star[15].
  • Q86853892's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.876'}[16].
  • Q86853892's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.211'}[17].
  • Q86853892's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.073'}[18].
  • Q86853892's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.990457'}[19].
  • Q86853892's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.083958715'}[20].
  • Q86853892's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.6'}[21].
  • Q86853892's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.6328958'}[22].
  • Q86853892's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.0009'}[23].
  • Q86853892's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-35.191799'}[24].
  • Q86853892's metallicity is recorded as {'unit': '1', 'amount': '-0.141'}[25].
  • Q86853892's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+817000'}[26].

Body

Definition and Type

Recorded instance of include rotating variable star[2], star[3], and near-infrared source[4].

References

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

Direct Wikidata claims

  1. [2] ↑ . SIMBAD. wikidata.org.
  2. [3] ↑ . SIMBAD. wikidata.org.
  3. [4] ↑ . SIMBAD. wikidata.org.
  4. [5] ↑ . wikidata.org.
  5. [6] ↑ . Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts. wikidata.org.
  6. [7] ↑ . 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] ↑ . Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. wikidata.org.
  15. [16] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  16. [17] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  17. [18] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  18. [19] ↑ . Gaia Early Data Release 3. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Early Data Release 3. wikidata.org.
  23. [24] ↑ . APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South. wikidata.org.
  24. [25] ↑ . APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South. wikidata.org.
  25. [26] ↑ . Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?. 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). Q86853892. Retrieved May 7, 2026, from https://4ort.xyz/entity/q86853892
MLA “Q86853892.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q86853892.
BibTeX @misc{4ortxyz_q86853892_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q86853892}}, year = {2026}, url = {https://4ort.xyz/entity/q86853892}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q86853892 — https://4ort.xyz/entity/q86853892 (retrieved 2026-05-07)

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