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Q84215220

young stellar object in the constellation Orion
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Q84215220

Summary

Q84215220 is a young stellar object[1].

Key Facts

  • Q84215220's instance of is recorded as young stellar object[2].
  • Q84215220's constellation is recorded as Orion[3].
  • Q84215220's spectral class is recorded as M0.9[4].
  • Q84215220 is part of Q84210325[5].
  • Q84215220 is part of NAME Orion Nebula Cluster[6].
  • Q84215220's catalog code is recorded as 2MASS J05354684-0605075[7].
  • Q84215220's catalog code is recorded as [RHS2000] 1-1420[8].
  • Q84215220's catalog code is recorded as [FHM2008] F31-ap155[9].
  • Q84215220's catalog code is recorded as [FKV2013] 966[10].
  • Q84215220's catalog code is recorded as SDSS J053546.85-060507.4[11].
  • Q84215220's catalog code is recorded as SOXS 347[12].
  • Q84215220's catalog code is recorded as Gaia DR2 3017171717504263296[13].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.82'}[14].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.78'}[15].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.20'}[16].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.664'}[17].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.192'}[18].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.328'}[19].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.859'}[20].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.627'}[21].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.89'}[22].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.637'}[23].
  • Q84215220's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.9988'}[24].
  • Q84215220's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.5026'}[25].
  • Q84215220's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+26.819052'}[26].

Body

Definition and Type

Q84215220's instance of is recorded as young stellar object[2].

Use and Application

Part of include Q84210325[5], a molecular cloud[27] and NAME Orion Nebula Cluster[6], an open cluster[28].

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 low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. 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] ↑ . Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. wikidata.org.
  14. [15] ↑ . Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. wikidata.org.
  15. [16] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  16. [17] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  17. [18] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  18. [19] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  19. [20] ↑ . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  20. [21] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  21. [22] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  22. [23] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . Gaia Data Release 2. wikidata.org.
  25. [26] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.

Inline context (facts about related entities)

  1. [27] ↑ . Wikidata. wikidata.org. → on this site
  2. [28] ↑ . Wikidata. wikidata.org. → on this site

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). Q84215220. Retrieved May 7, 2026, from https://4ort.xyz/entity/q84215220
MLA “Q84215220.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q84215220.
BibTeX @misc{4ortxyz_q84215220_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q84215220}}, year = {2026}, url = {https://4ort.xyz/entity/q84215220}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q84215220 — https://4ort.xyz/entity/q84215220 (retrieved 2026-05-07)

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