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Q84000494

peculiar star in the constellation Capricornus
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Q84000494

Summary

Q84000494 is a peculiar star[1].

Key Facts

  • Q84000494's instance of is recorded as peculiar star[2].
  • Q84000494's constellation is recorded as Capricornus[3].
  • Q84000494's spectral class is recorded as CEMP-s[4].
  • Q84000494's catalog code is recorded as BPS CS 22880-0074[5].
  • Q84000494's catalog code is recorded as 2MASS J20460321-2059141[6].
  • Q84000494's catalog code is recorded as Gaia DR2 6857039159217958144[7].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.27'}[8].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.84'}[9].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.990'}[10].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.687'}[11].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.636'}[12].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.770'}[13].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.382'}[14].
  • Q84000494's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.1258'}[15].
  • Q84000494's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0703'}[16].
  • Q84000494's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+97'}[17].
  • Q84000494's metallicity is recorded as {'unit': '1', 'amount': '-2.29'}[18].
  • Q84000494's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+934.3175'}[19].
  • Q84000494's SIMBAD ID is recorded as BPS CS 22880-0074[20].
  • Q84000494's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+311.51340086604640'}[21].
  • Q84000494's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-20.98725308164540'}[22].
  • Q84000494's epoch is recorded as J2000.0[23].
  • Q84000494's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5621'}[24].
  • Q84000494's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+3160'}[25].
  • Q84000494's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-61.977'}[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] ↑ . A search for stars of very low metal abundance. II. 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). Q84000494. Retrieved May 7, 2026, from https://4ort.xyz/entity/q84000494
MLA “Q84000494.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q84000494.
BibTeX @misc{4ortxyz_q84000494_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q84000494}}, year = {2026}, url = {https://4ort.xyz/entity/q84000494}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q84000494 — https://4ort.xyz/entity/q84000494 (retrieved 2026-05-07)

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