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Q94190381

star in the constellation Dorado
Thing star Q94190381
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Q94190381

Summary

Q94190381 is a star[1].

Key Facts

  • Q94190381's instance of is recorded as star[2].
  • Q94190381's constellation is recorded as Dorado[3].
  • Q94190381's spectral class is recorded as O9.5IV(n)[4].
  • Q94190381's spectral class is recorded as O9.5 IV(n)[5].
  • Q94190381's catalog code is recorded as 2MASS J05382624-6905019[6].
  • Q94190381's catalog code is recorded as [P93] 83[7].
  • Q94190381's catalog code is recorded as SSTISAGEMC J053826.19-690502.4[8].
  • Q94190381's catalog code is recorded as IRSF J05382622-6905019[9].
  • Q94190381's catalog code is recorded as VFTS 339[10].
  • Q94190381's catalog code is recorded as Gaia DR2 4657686359461747200[11].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.810'}[12].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.826'}[13].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.492'}[14].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.996'}[15].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.992'}[16].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.67'}[17].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.63'}[18].
  • Q94190381's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.4856'}[19].
  • Q94190381's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0311'}[20].
  • Q94190381's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+286.6'}[21].
  • Q94190381's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+275.2'}[22].
  • Q94190381's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+255.6'}[23].
  • Q94190381's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+273.5'}[24].
  • Q94190381's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+294.1'}[25].
  • Q94190381's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+295.2'}[26].

Body

Definition and Type

Q94190381's instance of is recorded as 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] ↑ . The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus. wikidata.org.
  4. [5] ↑ . The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 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] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. wikidata.org.
  12. [13] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  14. [15] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. wikidata.org.
  15. [16] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. wikidata.org.
  16. [17] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  17. [18] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. 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] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  23. [24] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  24. [25] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  25. [26] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. 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). Q94190381. Retrieved May 7, 2026, from https://4ort.xyz/entity/q94190381
MLA “Q94190381.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q94190381.
BibTeX @misc{4ortxyz_q94190381_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q94190381}}, year = {2026}, url = {https://4ort.xyz/entity/q94190381}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q94190381 — https://4ort.xyz/entity/q94190381 (retrieved 2026-05-07)

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