Home › Entities › eclipsing_binary_star › Q88927051

Q88927051

eclipsing binary star
Thing eclipsing_binary_star Q88927051
Press Enter · cited answer in seconds

Q88927051

Summary

Q88927051 is an eclipsing binary star[1].

Key Facts

  • Q88927051's instance of is recorded as eclipsing binary star[2].
  • Q88927051's constellation is recorded as Dorado[3].
  • Q88927051's spectral class is recorded as B1III-II[4].
  • Q88927051's catalog code is recorded as OGLE LMC175.6 41894[5].
  • Q88927051's catalog code is recorded as OGLE LMC517.01.031002[6].
  • Q88927051's catalog code is recorded as VFTS 27[7].
  • Q88927051's catalog code is recorded as IRSF J05371736-6907481[8].
  • Q88927051's catalog code is recorded as 2MASS J05371734-6907479[9].
  • Q88927051's catalog code is recorded as OGLE LMC-ECL-20808[10].
  • Q88927051's catalog code is recorded as Gaia DR2 4657690551351243392[11].
  • Q88927051's type of variable star is recorded as eclipsing binary star[12].
  • Q88927051's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.611'}[13].
  • Q88927051's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.575'}[14].
  • Q88927051's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.754'}[15].
  • Q88927051's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.71'}[16].
  • Q88927051's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.8'}[17].
  • Q88927051's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.639'}[18].
  • Q88927051's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.7606'}[19].
  • Q88927051's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+273.1'}[20].
  • Q88927051's SIMBAD ID is recorded as VFTS 27[21].
  • Q88927051's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+91'}[22].
  • Q88927051's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+84.32234851228100'}[23].
  • Q88927051's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-69.13001776841960'}[24].
  • Q88927051's epoch is recorded as J2000.0[25].
  • Q88927051's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+20500'}[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. XVIII. Classifications and radial velocities of the B-type 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] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XII. Eclipsing binary stars in the Large Magellanic Cloud. 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] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  16. [17] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  17. [18] ↑ . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XII. Eclipsing binary stars in the Large Magellanic Cloud. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . The VLT-FLAMES Tarantula Survey. XVIII. Classifications and radial velocities of the B-type stars. wikidata.org.
  20. [21] ↑ . wikidata.org.
  21. [22] ↑ . The VLT-FLAMES Tarantula Survey. XIX. B-type supergiants: Atmospheric parameters and nitrogen abundances to investigate the role of binarity and the width of the main sequence. 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] ↑ . The VLT-FLAMES Tarantula Survey. XIX. B-type supergiants: Atmospheric parameters and nitrogen abundances to investigate the role of binarity and the width of the main sequence. 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). Q88927051. Retrieved May 7, 2026, from https://4ort.xyz/entity/q88927051
MLA “Q88927051.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q88927051.
BibTeX @misc{4ortxyz_q88927051_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q88927051}}, year = {2026}, url = {https://4ort.xyz/entity/q88927051}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q88927051 — https://4ort.xyz/entity/q88927051 (retrieved 2026-05-07)

Canonical URL: https://4ort.xyz/entity/q88927051 · Last refreshed: