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Q80209837

rotating variable star in the constellation Cygnus
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Q80209837

Summary

Q80209837 is a rotating variable star[1].

Key Facts

  • Q80209837's instance of is recorded as rotating variable star[2].
  • Q80209837's instance of is recorded as star[3].
  • Q80209837's instance of is recorded as near-infrared source[4].
  • Q80209837's constellation is recorded as Cygnus[5].
  • Q80209837's spectral class is recorded as M0V[6].
  • Q80209837's child astronomical body is recorded as Q76083633[7].
  • Q80209837's catalog code is recorded as Gaia DR2 2131059972237410560[8].
  • Q80209837's catalog code is recorded as KIC 10525049[9].
  • Q80209837's catalog code is recorded as 2MASS J19092737+4747067[10].
  • Q80209837's catalog code is recorded as KOI-4252[11].
  • Q80209837's catalog code is recorded as Kepler-1948[12].
  • Q80209837's catalog code is recorded as Gaia DR3 2131059972237410560[13].
  • Q80209837's catalog code is recorded as TIC 158489110[14].
  • Q80209837's type of variable star is recorded as rotating variable star[15].
  • Q80209837's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.706'}[16].
  • Q80209837's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.016'}[17].
  • Q80209837's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.871'}[18].
  • Q80209837's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.913515'}[19].
  • Q80209837's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.64'}[20].
  • Q80209837's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.13354422'}[21].
  • Q80209837's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.611'}[22].
  • Q80209837's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+0.09207'}[23].
  • Q80209837's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+15.57129955'}[24].
  • Q80209837's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.0818'}[25].
  • Q80209837's metallicity is recorded as {'unit': '1', 'amount': '+0.12'}[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 and differential rotation of active Kepler 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] ↑ . Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . The Revised TESS Input Catalog and Candidate Target List. wikidata.org.
  22. [23] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  23. [24] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  24. [25] ↑ . Gaia Early Data Release 3. wikidata.org.
  25. [26] ↑ . Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts. 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). Q80209837. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80209837
MLA “Q80209837.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80209837.
BibTeX @misc{4ortxyz_q80209837_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80209837}}, year = {2026}, url = {https://4ort.xyz/entity/q80209837}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80209837 — https://4ort.xyz/entity/q80209837 (retrieved 2026-05-07)

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