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Q89025971

peculiar star in the constellation Aquarius
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Q89025971

Summary

Q89025971 is a peculiar star[1].

Key Facts

  • Q89025971's instance of is recorded as peculiar star[2].
  • Q89025971's constellation is recorded as Aquarius[3].
  • Q89025971's spectral class is recorded as CEMP-r/s[4].
  • Q89025971's catalog code is recorded as BPS CS 22887-0048[5].
  • Q89025971's catalog code is recorded as GPM 341.686319-11.143964[6].
  • Q89025971's catalog code is recorded as 2MASS J22464461-1108425[7].
  • Q89025971's catalog code is recorded as Gaia DR2 2604742840043317760[8].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.87'}[9].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.26'}[10].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.588'}[11].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.31'}[12].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.965'}[13].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.743'}[14].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.674'}[15].
  • Q89025971's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7643'}[16].
  • Q89025971's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0878'}[17].
  • Q89025971's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-84'}[18].
  • Q89025971's metallicity is recorded as {'unit': '1', 'amount': '-1.70'}[19].
  • Q89025971's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+919.2866'}[20].
  • Q89025971's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+341.68592234803040'}[21].
  • Q89025971's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-11.14511589601830'}[22].
  • Q89025971's epoch is recorded as J2000.0[23].
  • Q89025971's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6500'}[24].
  • Q89025971's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+2240'}[25].
  • Q89025971's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-88.854'}[26].

Body

Definition and Type

Q89025971's instance of is recorded as peculiar star[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] ↑ . 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] ↑ . Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. wikidata.org.
  9. [10] ↑ . Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. wikidata.org.
  10. [11] ↑ . A search for nitrogen-enhanced metal-poor stars. wikidata.org.
  11. [12] ↑ . A search for nitrogen-enhanced metal-poor stars. 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] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . A search for stars of very low metal abundance. II. wikidata.org.
  18. [19] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. 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] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  24. [25] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  25. [26] ↑ . Gaia Data Release 2. 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). Q89025971. Retrieved May 7, 2026, from https://4ort.xyz/entity/q89025971
MLA “Q89025971.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q89025971.
BibTeX @misc{4ortxyz_q89025971_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q89025971}}, year = {2026}, url = {https://4ort.xyz/entity/q89025971}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q89025971 — https://4ort.xyz/entity/q89025971 (retrieved 2026-05-07)

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