Q79288858

young stellar object in the constellation Orion
Thing young_stellar_object Q79288858
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Q79288858

Summary

Q79288858 is a young stellar object[1].

Key Facts

  • Q79288858's instance of is recorded as young stellar object[2].
  • Q79288858's constellation is recorded as Orion[3].
  • Q79288858's spectral class is recorded as M4.5[4].
  • Q79288858's part of is recorded as sigma Orionis Cluster[5].
  • Q79288858's catalog code is recorded as 2MASS J05375206-0236046[6].
  • Q79288858's catalog code is recorded as Mayrit 790270[7].
  • Q79288858's catalog code is recorded as [KJN2005] 62[8].
  • Q79288858's catalog code is recorded as [HHM2007] 219[9].
  • Q79288858's catalog code is recorded as [MJO2008] J053752.0-023604[10].
  • Q79288858's catalog code is recorded as [BZR2011] S Ori J053752.07-023604.6[11].
  • Q79288858's catalog code is recorded as UGCS J053752.06-023604.6[12].
  • Q79288858's catalog code is recorded as [BNM2013] 92.01 377[13].
  • Q79288858's catalog code is recorded as Gaia DR2 3216126486827855744[14].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.34'}[15].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+21.624'}[16].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.249'}[17].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.003'}[18].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.14'}[19].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.55'}[20].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.20'}[21].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+22.41'}[22].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.91'}[23].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.20'}[24].
  • Q79288858's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.8763'}[25].
  • Q79288858's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.3649'}[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] . SIMBAD. wikidata.org.
  13. [14] . SIMBAD. wikidata.org.
  14. [15] . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. 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] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  19. [20] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  20. [21] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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] . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. wikidata.org.
  24. [25] . Gaia Data Release 2. wikidata.org.
  25. [26] . Gaia Data Release 2. 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). Q79288858. Retrieved May 7, 2026, from https://4ort.xyz/entity/q79288858
MLA “Q79288858.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q79288858.
BibTeX @misc{4ortxyz_q79288858_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q79288858}}, year = {2026}, url = {https://4ort.xyz/entity/q79288858}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q79288858 — https://4ort.xyz/entity/q79288858 (retrieved 2026-05-07)

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