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Q80895200

star in the constellation Dorado
Thing star Q80895200
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Q80895200

Summary

Q80895200 is a star[1].

Key Facts

  • Q80895200's instance of is recorded as star[2].
  • Q80895200's constellation is recorded as Dorado[3].
  • Q80895200's spectral class is recorded as O9V[4].
  • Q80895200's spectral class is recorded as O9[5].
  • Q80895200's part of is recorded as NGC 2070[6].
  • Q80895200's catalog code is recorded as Cl* NGC 2070 SMB 309[7].
  • Q80895200's catalog code is recorded as VFTS 483[8].
  • Q80895200's catalog code is recorded as IRSF J05384025-6905311[9].
  • Q80895200's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.38'}[10].
  • Q80895200's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.5'}[11].
  • Q80895200's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.36'}[12].
  • Q80895200's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.79'}[13].
  • Q80895200's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.44'}[14].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+273.4'}[15].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+276.8'}[16].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+274.8'}[17].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+260.1'}[18].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+282.6'}[19].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+267.3'}[20].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+292.4'}[21].
  • Q80895200's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+276.0'}[22].
  • Q80895200's SIMBAD ID is recorded as Cl* NGC 2070 SMB 309[23].
  • Q80895200's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+40'}[24].
  • Q80895200's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+84.6676667'}[25].
  • Q80895200's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-69.0918833'}[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] ↑ . The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus. wikidata.org.
  4. [5] ↑ . The VLT-FLAMES Tarantula Survey. XIII: On the nature of O Vz stars in 30 Doradus. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . SIMBAD. wikidata.org.
  8. [9] ↑ . SIMBAD. wikidata.org.
  9. [10] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  10. [11] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  11. [12] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  12. [13] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  13. [14] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  14. [15] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  15. [16] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  16. [17] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  17. [18] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  18. [19] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  19. [20] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  20. [21] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  21. [22] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  22. [23] ↑ . wikidata.org.
  23. [24] ↑ . The VLT-FLAMES Tarantula Survey. XIII: On the nature of O Vz stars in 30 Doradus. wikidata.org.
  24. [25] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  25. [26] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. 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). Q80895200. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80895200
MLA “Q80895200.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80895200.
BibTeX @misc{4ortxyz_q80895200_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80895200}}, year = {2026}, url = {https://4ort.xyz/entity/q80895200}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80895200 — https://4ort.xyz/entity/q80895200 (retrieved 2026-05-07)

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