Q84218261

Thing t_tauri_type_star Q84218261
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Q84218261

Summary

Q84218261 is a T Tauri-type star[1].

Key Facts

  • Q84218261's instance of is recorded as T Tauri-type star[2].
  • Q84218261's instance of is recorded as eruptive variable star[3].
  • Q84218261's instance of is recorded as near-infrared source[4].
  • Q84218261's instance of is recorded as Orion variable[5].
  • Q84218261's constellation is recorded as Orion[6].
  • Q84218261's spectral class is recorded as M3.3[7].
  • Q84218261's part of is recorded as Q84210325[8].
  • Q84218261's part of is recorded as NAME Orion Nebula Cluster[9].
  • Q84218261's catalog code is recorded as [FKP2017] 397[10].
  • Q84218261's catalog code is recorded as 2MASS J05352792-0609391[11].
  • Q84218261's catalog code is recorded as SDSS J053527.93-060939.1[12].
  • Q84218261's catalog code is recorded as Gaia DR2 3017147562608206976[13].
  • Q84218261's catalog code is recorded as V564 Ori[14].
  • Q84218261's catalog code is recorded as TIC 388918012[15].
  • Q84218261's catalog code is recorded as CVSO 1599[16].
  • Q84218261's catalog code is recorded as Gaia DR3 3017147562608206976[17].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.3'}[18].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.125'}[19].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.12'}[20].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.57'}[21].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.65'}[22].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.974'}[23].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.542'}[24].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.690'}[25].
  • Q84218261's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.567'}[26].

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

  1. [2] . SIMBAD. wikidata.org.
  2. [3] . SIMBAD. wikidata.org.
  3. [4] . SIMBAD. wikidata.org.
  4. [5] . SIMBAD. wikidata.org.
  5. [6] . wikidata.org.
  6. [7] . The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. 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] . SIMBAD. wikidata.org.
  15. [16] . SIMBAD. wikidata.org.
  16. [17] . SIMBAD. wikidata.org.
  17. [18] . SIMBAD. wikidata.org.
  18. [19] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  19. [20] . Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. wikidata.org.
  20. [21] . Kinematics of the Orion Nebula Cluster: velocity substructure and spectroscopic binaries. wikidata.org.
  21. [22] . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  22. [23] . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  23. [24] . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  24. [25] . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
  25. [26] . The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. 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). Q84218261. Retrieved May 7, 2026, from https://4ort.xyz/entity/q84218261
MLA “Q84218261.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q84218261.
BibTeX @misc{4ortxyz_q84218261_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q84218261}}, year = {2026}, url = {https://4ort.xyz/entity/q84218261}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q84218261 — https://4ort.xyz/entity/q84218261 (retrieved 2026-05-07)

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