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Q80972335

peculiar star in the constellation Pavo
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Q80972335

Summary

Q80972335 is a peculiar star[1].

Key Facts

  • Q80972335's instance of is recorded as peculiar star[2].
  • Q80972335's constellation is recorded as Pavo[3].
  • Q80972335's spectral class is recorded as CEMP-no[4].
  • Q80972335's catalog code is recorded as BPS CS 22891-0200[5].
  • Q80972335's catalog code is recorded as 2MASS J19351908-6142243[6].
  • Q80972335's catalog code is recorded as UCAC2 4691264[7].
  • Q80972335's catalog code is recorded as UCAC3 57-457709[8].
  • Q80972335's catalog code is recorded as DENIS J193519.0-614224[9].
  • Q80972335's catalog code is recorded as Gaia DR2 6445220927325014016[10].
  • Q80972335's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.93'}[11].
  • Q80972335's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.77'}[12].
  • Q80972335's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.995'}[13].
  • Q80972335's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.461'}[14].
  • Q80972335's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.414'}[15].
  • Q80972335's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.79'}[16].
  • Q80972335's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6279'}[17].
  • Q80972335's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1135'}[18].
  • Q80972335's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+137.2'}[19].
  • Q80972335's metallicity is recorded as {'unit': '1', 'amount': '-4.06'}[20].
  • Q80972335's SIMBAD ID is recorded as BPS CS 22891-0200[21].
  • Q80972335's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.82949025727450'}[22].
  • Q80972335's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-61.70677066976000'}[23].
  • Q80972335's epoch is recorded as J2000.0[24].
  • Q80972335's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4490'}[25].
  • Q80972335's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+3'}[26].

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] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  4. [5] ↑ . SIMBAD. 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] ↑ . Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. wikidata.org.
  11. [12] ↑ . Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. 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] ↑ . The DENIS database, 3rd Release. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . A search for stars of very low metal abundance. VI. Detailed abundances of 313 metal-poor stars. wikidata.org.
  19. [20] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  20. [21] ↑ . 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] ↑ . A search for stars of very low metal abundance. VI. Detailed abundances of 313 metal-poor stars. wikidata.org.
  25. [26] ↑ . The Chemical Abundances of Stars in the Halo (CASH) project. II. A sample of 14 extremely metal-poor stars. wikidata.org.

Class ancestry

  1. [1] ↑ . Wikidata. wikidata.org.

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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). Q80972335. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80972335
MLA “Q80972335.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80972335.
BibTeX @misc{4ortxyz_q80972335_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80972335}}, year = {2026}, url = {https://4ort.xyz/entity/q80972335}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80972335 — https://4ort.xyz/entity/q80972335 (retrieved 2026-05-07)

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