Q84209174

emission-line star in the constellation Orion
Thing emission_line_star Q84209174
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Q84209174

Summary

Q84209174 is an emission-line star[1].

Key Facts

  • Q84209174's instance of is recorded as emission-line star[2].
  • Q84209174's constellation is recorded as Orion[3].
  • Q84209174's spectral class is recorded as M8.0[4].
  • Q84209174's part of is recorded as NAME Orion Nebula Cluster[5].
  • Q84209174's catalog code is recorded as [BAB2014] 364118[6].
  • Q84209174's catalog code is recorded as 2MASS J05345368-0545111[7].
  • Q84209174's catalog code is recorded as [R2001] 1561[8].
  • Q84209174's catalog code is recorded as [RHS2000] 1-934[9].
  • Q84209174's catalog code is recorded as [RRS2004] SOFF W068[10].
  • Q84209174's catalog code is recorded as CXORRS J053453.6-054511[11].
  • Q84209174's catalog code is recorded as [FHM2008] F22-ap215[12].
  • Q84209174's catalog code is recorded as ESO-HA 1057[13].
  • Q84209174's catalog code is recorded as Gaia DR2 3017243185759909504[14].
  • Q84209174's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.377'}[15].
  • Q84209174's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.429'}[16].
  • Q84209174's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.71'}[17].
  • Q84209174's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.33'}[18].
  • Q84209174's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.20'}[19].
  • Q84209174's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.7566'}[20].
  • Q84209174's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.5401'}[21].
  • Q84209174's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+23.1'}[22].
  • Q84209174's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+25.90'}[23].
  • Q84209174's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+26.52'}[24].
  • Q84209174's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+29.13'}[25].
  • Q84209174's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+393.6853'}[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] . SIMBAD. 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] . 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] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  17. [18] . Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. wikidata.org.
  18. [19] . Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. wikidata.org.
  19. [20] . Gaia Data Release 2. wikidata.org.
  20. [21] . Gaia Data Release 2. wikidata.org.
  21. [22] . Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. wikidata.org.
  22. [23] . Spectroscopic binaries in the Orion nebula cluster and NGC 2264. wikidata.org.
  23. [24] . Spectroscopic binaries in the Orion nebula cluster and NGC 2264. wikidata.org.
  24. [25] . Spectroscopic binaries in the Orion nebula cluster and NGC 2264. 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). Q84209174. Retrieved May 7, 2026, from https://4ort.xyz/entity/q84209174
MLA “Q84209174.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q84209174.
BibTeX @misc{4ortxyz_q84209174_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q84209174}}, year = {2026}, url = {https://4ort.xyz/entity/q84209174}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q84209174 — https://4ort.xyz/entity/q84209174 (retrieved 2026-05-07)

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