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Q80639183

peculiar star in the constellation Eridanus
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Q80639183

Summary

Q80639183 is a peculiar star[1].

Key Facts

  • Q80639183's instance of is recorded as peculiar star[2].
  • Q80639183's constellation is recorded as Eridanus[3].
  • Q80639183's spectral class is recorded as CEMP-no[4].
  • Q80639183's catalog code is recorded as HE 0432-1005[5].
  • Q80639183's catalog code is recorded as 2MASS J04350131-0959363[6].
  • Q80639183's catalog code is recorded as Gaia DR2 3185294604533440640[7].
  • Q80639183's catalog code is recorded as HE 0432-1005a[8].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1'}[9].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.150'}[10].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.664'}[11].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.564'}[12].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.973'}[13].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.446'}[14].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.926'}[15].
  • Q80639183's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.6895'}[16].
  • Q80639183's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1663'}[17].
  • Q80639183's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+197.86'}[18].
  • Q80639183's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+198.00'}[19].
  • Q80639183's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+199.60'}[20].
  • Q80639183's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+197.30'}[21].
  • Q80639183's metallicity is recorded as {'unit': '1', 'amount': '-3.06'}[22].
  • Q80639183's metallicity is recorded as {'unit': '1', 'amount': '-3.21'}[23].
  • Q80639183's SIMBAD ID is recorded as HE 0432-1005[24].
  • Q80639183's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+68.75550969804720'}[25].
  • Q80639183's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+68.75547417'}[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] ↑ . Bright metal-poor stars from the Hamburg/ESO survey. I. Selection and follow-up observations from 329 fields. 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] ↑ . Broadband UBVRCIC Photometry of Horizontal‐Branch and Metal‐poor Candidates from the HK and Hamburg/ESO Surveys. I. wikidata.org.
  15. [16] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . The Chemical Abundances of Stars in the Halo (CASH) project. II. A sample of 14 extremely metal-poor stars. wikidata.org.
  19. [20] ↑ . The Chemical Abundances of Stars in the Halo (CASH) project. II. A sample of 14 extremely metal-poor stars. wikidata.org.
  20. [21] ↑ . The Chemical Abundances of Stars in the Halo (CASH) project. II. A sample of 14 extremely metal-poor stars. wikidata.org.
  21. [22] ↑ . Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis. wikidata.org.
  22. [23] ↑ . The Chemical Abundances of Stars in the Halo (CASH) project. II. A sample of 14 extremely metal-poor stars. wikidata.org.
  23. [24] ↑ . wikidata.org.
  24. [25] ↑ . Gaia Data Release 2. wikidata.org.
  25. [26] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. 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). Q80639183. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80639183
MLA “Q80639183.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80639183.
BibTeX @misc{4ortxyz_q80639183_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80639183}}, year = {2026}, url = {https://4ort.xyz/entity/q80639183}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80639183 — https://4ort.xyz/entity/q80639183 (retrieved 2026-05-07)

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