Q83351795

peculiar star in the constellation Indus
Thing peculiar_star Q83351795
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Q83351795

Summary

Q83351795 is a peculiar star[1].

Key Facts

  • Q83351795's instance of is recorded as peculiar star[2].
  • Q83351795's constellation is recorded as Indus[3].
  • Q83351795's spectral class is recorded as CEMP-no[4].
  • Q83351795's catalog code is recorded as BPS CS 22956-0050[5].
  • Q83351795's catalog code is recorded as 2MASS J21580583-6513271[6].
  • Q83351795's catalog code is recorded as SMSS J215805.81-651327.2[7].
  • Q83351795's catalog code is recorded as Gaia DR2 6399358510623784192[8].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.95'}[9].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.597'}[10].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.060'}[11].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.018'}[12].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.745'}[13].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.211'}[14].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.25'}[15].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.854'}[16].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.304'}[17].
  • Q83351795's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.0038'}[18].
  • Q83351795's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1219'}[19].
  • Q83351795's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-36.9'}[20].
  • Q83351795's metallicity is recorded as {'unit': '1', 'amount': '-3.67'}[21].
  • Q83351795's SIMBAD ID is recorded as BPS CS 22956-0050[22].
  • Q83351795's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+329.52430824940610'}[23].
  • Q83351795's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-65.22421136610940'}[24].
  • Q83351795's epoch is recorded as J2000.0[25].
  • Q83351795's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4640'}[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] . 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] . A search for stars of very low metal abundance. VI. Detailed abundances of 313 metal-poor stars. wikidata.org.
  15. [16] . High-resolution spectroscopic study of extremely metal-poor star candidates from the SkyMapper survey. wikidata.org.
  16. [17] . High-resolution spectroscopic study of extremely metal-poor star candidates from the SkyMapper survey. wikidata.org.
  17. [18] . Gaia Data Release 2. wikidata.org.
  18. [19] . Gaia Data Release 2. wikidata.org.
  19. [20] . High-resolution spectroscopic study of extremely metal-poor star candidates from the SkyMapper survey. wikidata.org.
  20. [21] . Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. wikidata.org.
  21. [22] . wikidata.org.
  22. [23] . Gaia Data Release 2. wikidata.org.
  23. [24] . Gaia Data Release 2. wikidata.org.
  24. [25] . Gaia Data Release 2. wikidata.org.
  25. [26] . A search for stars of very low metal abundance. VI. Detailed abundances of 313 metal-poor stars. wikidata.org.

Class ancestry

  1. [1] . Wikidata. wikidata.org.

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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). Q83351795. Retrieved May 7, 2026, from https://4ort.xyz/entity/q83351795
MLA “Q83351795.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q83351795.
BibTeX @misc{4ortxyz_q83351795_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q83351795}}, year = {2026}, url = {https://4ort.xyz/entity/q83351795}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q83351795 — https://4ort.xyz/entity/q83351795 (retrieved 2026-05-07)

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