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Q86086722

peculiar star in the constellation Cetus
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Q86086722

Summary

Q86086722 is a peculiar star[1].

Key Facts

  • Q86086722's instance of is recorded as peculiar star[2].
  • Q86086722's constellation is recorded as Cetus[3].
  • Q86086722's spectral class is recorded as CEMP-r/s[4].
  • Q86086722's catalog code is recorded as HE 0027-1221[5].
  • Q86086722's catalog code is recorded as BPS CS 31062-0050[6].
  • Q86086722's catalog code is recorded as 2MASS J00303106-1205108[7].
  • Q86086722's catalog code is recorded as Gaia DR2 2423720246374021632[8].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.05'}[9].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7'}[10].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.765'}[11].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.464'}[12].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.405'}[13].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.681'}[14].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.309'}[15].
  • Q86086722's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8803'}[16].
  • Q86086722's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7503'}[17].
  • Q86086722's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.9'}[18].
  • Q86086722's metallicity is recorded as {'unit': '1', 'amount': '-2.5'}[19].
  • Q86086722's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1332.8002'}[20].
  • Q86086722's SIMBAD ID is recorded as BPS CS 31062-0050[21].
  • Q86086722's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.62943061419580'}[22].
  • Q86086722's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-12.08635365294750'}[23].
  • Q86086722's epoch is recorded as J2000.0[24].
  • Q86086722's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5691'}[25].
  • Q86086722's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+83'}[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] ↑ . 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] ↑ . 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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] ↑ . Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis. wikidata.org.
  18. [19] ↑ . Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution. II. Statistical analysis of a sample of 67 CEMP-s stars. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. 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] ↑ . Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis. wikidata.org.
  25. [26] ↑ . Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis. 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). Q86086722. Retrieved May 7, 2026, from https://4ort.xyz/entity/q86086722
MLA “Q86086722.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q86086722.
BibTeX @misc{4ortxyz_q86086722_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q86086722}}, year = {2026}, url = {https://4ort.xyz/entity/q86086722}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q86086722 — https://4ort.xyz/entity/q86086722 (retrieved 2026-05-07)

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