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Q77870326

young stellar object in the constellation Orion
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Q77870326

Summary

Q77870326 is a young stellar object[1].

Key Facts

  • Q77870326's instance of is recorded as young stellar object[2].
  • Q77870326's constellation is recorded as Orion[3].
  • Q77870326's spectral class is recorded as M4.0[4].
  • Q77870326's catalog code is recorded as 2MASS J05415134-0751483[5].
  • Q77870326's catalog code is recorded as [FKV2013] 226[6].
  • Q77870326's catalog code is recorded as SOXS 866[7].
  • Q77870326's catalog code is recorded as ESO-HA 1774[8].
  • Q77870326's catalog code is recorded as Gaia DR2 3015800729582391296[9].
  • Q77870326's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.416'}[10].
  • Q77870326's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.399'}[11].
  • Q77870326's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.66'}[12].
  • Q77870326's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.940'}[13].
  • Q77870326's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.633'}[14].
  • Q77870326's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.8954'}[15].
  • Q77870326's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.4809'}[16].
  • Q77870326's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+24.647990000'}[17].
  • Q77870326's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+24.189013'}[18].
  • Q77870326's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+24.199696'}[19].
  • Q77870326's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+24.647990'}[20].
  • Q77870326's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+24.658672'}[21].
  • Q77870326's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+403.0795'}[22].
  • Q77870326's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+94.671'}[23].
  • Q77870326's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+85.46395428382090'}[24].
  • Q77870326's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-7.86341456188620'}[25].
  • Q77870326's epoch is recorded as J2000.0[26].

Body

Definition and Type

Q77870326's instance of is recorded as young stellar object[2].

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] ↑ . The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. wikidata.org.
  10. [11] ↑ . The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. wikidata.org.
  11. [12] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  12. [13] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  14. [15] ↑ . Gaia Data Release 2. wikidata.org.
  15. [16] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  17. [18] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  18. [19] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  19. [20] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  20. [21] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . IN-SYNC. IV. The young stellar population in the Orion A molecular cloud. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. 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). Q77870326. Retrieved May 7, 2026, from https://4ort.xyz/entity/q77870326
MLA “Q77870326.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q77870326.
BibTeX @misc{4ortxyz_q77870326_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q77870326}}, year = {2026}, url = {https://4ort.xyz/entity/q77870326}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q77870326 — https://4ort.xyz/entity/q77870326 (retrieved 2026-05-07)

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