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Q79275779

emission-line star in the constellation Orion
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Q79275779

Summary

Q79275779 is an emission-line star[1].

Key Facts

  • Q79275779's instance of is recorded as emission-line star[2].
  • Q79275779's constellation is recorded as Orion[3].
  • Q79275779's spectral class is recorded as M2.2[4].
  • Q79275779's catalog code is recorded as Haro 4-437[5].
  • Q79275779's catalog code is recorded as PACH 455[6].
  • Q79275779's catalog code is recorded as 2MASS J05375470-0654075[7].
  • Q79275779's catalog code is recorded as Gaia DR2 3016862445497585536[8].
  • Q79275779's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.76'}[9].
  • Q79275779's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.792'}[10].
  • Q79275779's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.277'}[11].
  • Q79275779's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.040'}[12].
  • Q79275779's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.406'}[13].
  • Q79275779's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.191'}[14].
  • Q79275779's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.6727'}[15].
  • Q79275779's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+12.2419'}[16].
  • Q79275779's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+75.320070000'}[17].
  • Q79275779's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+75.374220'}[18].
  • Q79275779's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+75.413280'}[19].
  • Q79275779's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+75.320070'}[20].
  • Q79275779's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+75.359120'}[21].
  • Q79275779's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+81.6867'}[22].
  • Q79275779's SIMBAD ID is recorded as Haro 4-437[23].
  • Q79275779's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+3.395'}[24].
  • Q79275779's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+84.47792820252220'}[25].
  • Q79275779's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-6.90209533273600'}[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] ↑ . 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] ↑ . wikidata.org.
  23. [24] ↑ . IN-SYNC. IV. The young stellar population in the Orion A molecular cloud. 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). Q79275779. Retrieved May 7, 2026, from https://4ort.xyz/entity/q79275779
MLA “Q79275779.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q79275779.
BibTeX @misc{4ortxyz_q79275779_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q79275779}}, year = {2026}, url = {https://4ort.xyz/entity/q79275779}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q79275779 — https://4ort.xyz/entity/q79275779 (retrieved 2026-05-07)

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