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Q85262429

peculiar star in the constellation Capricornus
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Q85262429

Summary

Q85262429 is a peculiar star[1].

Key Facts

  • Q85262429's instance of is recorded as peculiar star[2].
  • Q85262429's constellation is recorded as Capricornus[3].
  • Q85262429's spectral class is recorded as CEMP-s[4].
  • Q85262429's spectral class is recorded as CEMP-no[5].
  • Q85262429's catalog code is recorded as HE 2133-1426[6].
  • Q85262429's catalog code is recorded as 2MASS J21360722-1412353[7].
  • Q85262429's catalog code is recorded as UCAC4 379-163127[8].
  • Q85262429's catalog code is recorded as Gaia DR2 6841937882405108352[9].
  • Q85262429's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.380'}[10].
  • Q85262429's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.139'}[11].
  • Q85262429's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.111'}[12].
  • Q85262429's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.698'}[13].
  • Q85262429's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.845'}[14].
  • Q85262429's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.48'}[15].
  • Q85262429's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.3659'}[16].
  • Q85262429's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8451'}[17].
  • Q85262429's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.6'}[18].
  • Q85262429's metallicity is recorded as {'unit': '1', 'amount': '-3.37'}[19].
  • Q85262429's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1183.2919'}[20].
  • Q85262429's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+324.03010662005720'}[21].
  • Q85262429's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-14.20982768721710'}[22].
  • Q85262429's epoch is recorded as J2000.0[23].
  • Q85262429's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+6300'}[24].
  • Q85262429's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+12600'}[25].
  • Q85262429's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.954'}[26].

Body

Definition and Type

Q85262429'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] ↑ . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . SIMBAD. wikidata.org.
  8. [9] ↑ . SIMBAD. 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] ↑ . Normal and outlying populations of the Milky Way stellar halo at [Fe/H] <-2. wikidata.org.
  15. [16] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . Normal and outlying populations of the Milky Way stellar halo at [Fe/H] <-2. 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] ↑ . Normal and outlying populations of the Milky Way stellar halo at [Fe/H] <-2. wikidata.org.
  24. [25] ↑ . Normal and outlying populations of the Milky Way stellar halo at [Fe/H] <-2. 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). Q85262429. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85262429
MLA “Q85262429.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85262429.
BibTeX @misc{4ortxyz_q85262429_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85262429}}, year = {2026}, url = {https://4ort.xyz/entity/q85262429}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85262429 — https://4ort.xyz/entity/q85262429 (retrieved 2026-05-07)

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