Q76836950

low-mass star in the constellation Orion
Thing low_mass_star Q76836950
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Q76836950

Summary

Q76836950 is a low-mass star[1].

Key Facts

  • Q76836950's instance of is recorded as low-mass star[2].
  • Q76836950's constellation is recorded as Orion[3].
  • Q76836950's spectral class is recorded as M2.0[4].
  • Q76836950's catalog code is recorded as 2MASS J05392435-0234013[5].
  • Q76836950's catalog code is recorded as [SFR2008] S59[6].
  • Q76836950's catalog code is recorded as [HHM2007] 1027[7].
  • Q76836950's catalog code is recorded as [SWW2004] J053924.358-023401.25[8].
  • Q76836950's catalog code is recorded as Mayrit 605079[9].
  • Q76836950's catalog code is recorded as [MJO2008] J053924.3-023401[10].
  • Q76836950's catalog code is recorded as [BNM2013] 90.02 83[11].
  • Q76836950's catalog code is recorded as Gaia DR2 3216487680692797568[12].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.98'}[13].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.272'}[14].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.058'}[15].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.394'}[16].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.251'}[17].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.015'}[18].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.833'}[19].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.19'}[20].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.62'}[21].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.53'}[22].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.28'}[23].
  • Q76836950's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.6200'}[24].
  • Q76836950's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.4181'}[25].
  • Q76836950's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+33.18'}[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] . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. 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] . SIMBAD. 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] . Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
  16. [17] . Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
  17. [18] . Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
  18. [19] . Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
  19. [20] . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. wikidata.org.
  20. [21] . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. wikidata.org.
  21. [22] . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. wikidata.org.
  22. [23] . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. wikidata.org.
  23. [24] . Gaia Data Release 2. wikidata.org.
  24. [25] . Gaia Data Release 2. wikidata.org.
  25. [26] . FLAMES spectroscopy of low-mass stars in the young clusters σ Ori and λ Ori. 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). Q76836950. Retrieved May 7, 2026, from https://4ort.xyz/entity/q76836950
MLA “Q76836950.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q76836950.
BibTeX @misc{4ortxyz_q76836950_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q76836950}}, year = {2026}, url = {https://4ort.xyz/entity/q76836950}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q76836950 — https://4ort.xyz/entity/q76836950 (retrieved 2026-05-07)

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