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Q86946602

young stellar object in the constellation Orion
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Q86946602

Summary

Q86946602 is a young stellar object[1].

Key Facts

  • Q86946602's instance of is recorded as young stellar object[2].
  • Q86946602's constellation is recorded as Orion[3].
  • Q86946602's spectral class is recorded as M4.5[4].
  • Q86946602's catalog code is recorded as Mayrit 870187[5].
  • Q86946602's catalog code is recorded as 2MASS J05383745-0250236[6].
  • Q86946602's catalog code is recorded as [HHM2007] 628[7].
  • Q86946602's catalog code is recorded as [SWW2004] J053837.446-025023.71[8].
  • Q86946602's catalog code is recorded as [MJO2008] J053837.4-025023[9].
  • Q86946602's catalog code is recorded as [BNM2013] 93.04 25[10].
  • Q86946602's catalog code is recorded as ESO-HA 1677[11].
  • Q86946602's catalog code is recorded as Gaia DR2 3216059214755240320[12].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.33'}[13].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.809'}[14].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.176'}[15].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.923'}[16].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.431'}[17].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.201'}[18].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.85'}[19].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.43'}[20].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.66'}[21].
  • Q86946602's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.1788'}[22].
  • Q86946602's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.6199'}[23].
  • Q86946602's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+30.92'}[24].
  • Q86946602's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+30.87'}[25].
  • Q86946602's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+31.23'}[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] ↑ . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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] ↑ . A spectroscopic census in young stellar regions: the {sigma} Orionis cluster. 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] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . A survey for low-mass spectroscopic binary stars in the young clusters around {sigma} Orionis and {lambda} Orionis. wikidata.org.
  24. [25] ↑ . A survey for low-mass spectroscopic binary stars in the young clusters around {sigma} Orionis and {lambda} Orionis. wikidata.org.
  25. [26] ↑ . A survey for low-mass spectroscopic binary stars in the young clusters around {sigma} Orionis and {lambda} Orionis. wikidata.org.

Class ancestry

  1. [1] ↑ . Wikidata. wikidata.org.

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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). Q86946602. Retrieved May 7, 2026, from https://4ort.xyz/entity/q86946602
MLA “Q86946602.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q86946602.
BibTeX @misc{4ortxyz_q86946602_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q86946602}}, year = {2026}, url = {https://4ort.xyz/entity/q86946602}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q86946602 — https://4ort.xyz/entity/q86946602 (retrieved 2026-05-07)

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