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Q80393702

rotating variable star in the constellation Cygnus
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Q80393702

Summary

Q80393702 is a rotating variable star[1].

Key Facts

  • Q80393702's instance of is recorded as rotating variable star[2].
  • Q80393702's instance of is recorded as star[3].
  • Q80393702's instance of is recorded as near-infrared source[4].
  • Q80393702's constellation is recorded as Cygnus[5].
  • Q80393702's catalog code is recorded as Gaia DR2 2080309161204049792[6].
  • Q80393702's catalog code is recorded as KIC 9966219[7].
  • Q80393702's catalog code is recorded as 2MASS J19495481+4648567[8].
  • Q80393702's catalog code is recorded as TIC 273373114[9].
  • Q80393702's catalog code is recorded as KOI-3401[10].
  • Q80393702's type of variable star is recorded as rotating variable star[11].
  • Q80393702's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.4249'}[12].
  • Q80393702's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.200'}[13].
  • Q80393702's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.816'}[14].
  • Q80393702's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.732'}[15].
  • Q80393702's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.7006434'}[16].
  • Q80393702's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.924'}[17].
  • Q80393702's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.9853214'}[18].
  • Q80393702's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3730'}[19].
  • Q80393702's metallicity is recorded as {'unit': '1', 'amount': '-0.04'}[20].
  • Q80393702's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+728.332'}[21].
  • Q80393702's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+297.47835775886125'}[22].
  • Q80393702's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+46.81572522867833'}[23].
  • Q80393702's epoch is recorded as J2000.0[24].
  • Q80393702's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5638'}[25].
  • Q80393702's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+17800'}[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] ↑ . 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] ↑ . Photometric amplitude distribution of stellar rotation of KOIs--Indication for spin-orbit alignment of cool stars and high obliquity for hot stars. wikidata.org.
  11. [12] ↑ . Gaia Data Release 2. wikidata.org.
  12. [13] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy. wikidata.org.
  25. [26] ↑ . The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy. 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). Q80393702. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80393702
MLA “Q80393702.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80393702.
BibTeX @misc{4ortxyz_q80393702_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80393702}}, year = {2026}, url = {https://4ort.xyz/entity/q80393702}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80393702 — https://4ort.xyz/entity/q80393702 (retrieved 2026-05-07)

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