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Q80946210

star in the constellation Canis Major
Thing star Q80946210
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Q80946210

Summary

Q80946210 is a star[1].

Key Facts

  • Q80946210's instance of is recorded as star[2].
  • Q80946210's constellation is recorded as Canis Major[3].
  • Q80946210's part of is recorded as Q67857053[4].
  • Q80946210's catalog code is recorded as GES J06411368-1629164[5].
  • Q80946210's catalog code is recorded as GES J06411363-1629172[6].
  • Q80946210's catalog code is recorded as Cl* Berkeley 25 CGM 13[7].
  • Q80946210's catalog code is recorded as 2MASS J06411367-1629164[8].
  • Q80946210's catalog code is recorded as Gaia DR2 2946940584079996160[9].
  • Q80946210's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.36'}[10].
  • Q80946210's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.33'}[11].
  • Q80946210's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.97'}[12].
  • Q80946210's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.130'}[13].
  • Q80946210's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.424'}[14].
  • Q80946210's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.281'}[15].
  • Q80946210's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.3941'}[16].
  • Q80946210's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0548'}[17].
  • Q80946210's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+135.3'}[18].
  • Q80946210's metallicity is recorded as {'unit': '1', 'amount': '-0.28'}[19].
  • Q80946210's metallicity is recorded as {'unit': '1', 'amount': '-0.20'}[20].
  • Q80946210's SIMBAD ID is recorded as Cl* Berkeley 25 CGM 13[21].
  • Q80946210's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+100.30698049726540'}[22].
  • Q80946210's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-16.48791102838670'}[23].
  • Q80946210's epoch is recorded as J2000.0[24].
  • Q80946210's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4620'}[25].
  • Q80946210's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4710'}[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] ↑ . SIMBAD. 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] ↑ . Old open clusters in the outer Galactic disk. wikidata.org.
  10. [11] ↑ . Old open clusters in the outer Galactic disk. wikidata.org.
  11. [12] ↑ . Old open clusters in the outer Galactic disk. wikidata.org.
  12. [13] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  14. [15] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  15. [16] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young-field stars. wikidata.org.
  18. [19] ↑ . The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young-field stars. wikidata.org.
  19. [20] ↑ . The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young-field stars. 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] ↑ . The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young-field stars. wikidata.org.
  25. [26] ↑ . The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young-field 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). Q80946210. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80946210
MLA “Q80946210.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80946210.
BibTeX @misc{4ortxyz_q80946210_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80946210}}, year = {2026}, url = {https://4ort.xyz/entity/q80946210}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80946210 — https://4ort.xyz/entity/q80946210 (retrieved 2026-05-07)

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