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Q83477292

peculiar star in the constellation Eridanus
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Q83477292

Summary

Q83477292 is a peculiar star[1].

Key Facts

  • Q83477292's instance of is recorded as peculiar star[2].
  • Q83477292's constellation is recorded as Eridanus[3].
  • Q83477292's spectral class is recorded as CEMP-r/s[4].
  • Q83477292's catalog code is recorded as BPS CS 29526-0110[5].
  • Q83477292's catalog code is recorded as 2MASS J03274362-2300299[6].
  • Q83477292's catalog code is recorded as Gaia DR2 5098658004678548352[7].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.35'}[8].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.71'}[9].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.587'}[10].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.367'}[11].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.367'}[12].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.116'}[13].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.834'}[14].
  • Q83477292's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2673'}[15].
  • Q83477292's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3201'}[16].
  • Q83477292's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+208.35'}[17].
  • Q83477292's metallicity is recorded as {'unit': '1', 'amount': '-2.11'}[18].
  • Q83477292's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+757.5184'}[19].
  • Q83477292's SIMBAD ID is recorded as BPS CS 29526-0110[20].
  • Q83477292's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+51.93183144276290'}[21].
  • Q83477292's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-23.00831422334470'}[22].
  • Q83477292's epoch is recorded as J2000.0[23].
  • Q83477292's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6800'}[24].
  • Q83477292's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+12600'}[25].
  • Q83477292's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-90.456'}[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] ↑ . Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  10. [11] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  11. [12] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  12. [13] ↑ . Broadband UBVRCIC Photometry of Horizontal‐Branch and Metal‐poor Candidates from the HK and Hamburg/ESO Surveys. I. wikidata.org.
  13. [14] ↑ . Broadband UBVRCIC Photometry of Horizontal‐Branch and Metal‐poor Candidates from the HK and Hamburg/ESO Surveys. I. wikidata.org.
  14. [15] ↑ . Gaia Data Release 2. wikidata.org.
  15. [16] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . Subaru/HDS study of extremely metal-poor star CS 29498-043 : abundance analysis details and comparison with other carbon-rich objects. wikidata.org.
  17. [18] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . 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). Q83477292. Retrieved May 7, 2026, from https://4ort.xyz/entity/q83477292
MLA “Q83477292.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q83477292.
BibTeX @misc{4ortxyz_q83477292_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q83477292}}, year = {2026}, url = {https://4ort.xyz/entity/q83477292}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q83477292 — https://4ort.xyz/entity/q83477292 (retrieved 2026-05-07)

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