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Q84217597

high proper-motion star in the constellation Orion
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Q84217597

Summary

Q84217597 is a high proper-motion star[1].

Key Facts

  • Q84217597's instance of is recorded as high proper-motion star[2].
  • Q84217597's constellation is recorded as Orion[3].
  • Q84217597's spectral class is recorded as M1.4[4].
  • Q84217597's catalog code is recorded as [RHS2000] 1-1064[5].
  • Q84217597's catalog code is recorded as 2MASS J05350651-0600008[6].
  • Q84217597's catalog code is recorded as Gaia DR2 3017187900941041152[7].
  • Q84217597's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.928'}[8].
  • Q84217597's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.756'}[9].
  • Q84217597's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.158'}[10].
  • Q84217597's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.20'}[11].
  • Q84217597's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.958'}[12].
  • Q84217597's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.6653'}[13].
  • Q84217597's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+15.2498'}[14].
  • Q84217597's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+29.491034000'}[15].
  • Q84217597's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-57.522640'}[16].
  • Q84217597's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-54.450512'}[17].
  • Q84217597's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+29.491034'}[18].
  • Q84217597's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+32.563164'}[19].
  • Q84217597's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+65.5746'}[20].
  • Q84217597's SIMBAD ID is recorded as 2MASS J05350651-0600008[21].
  • Q84217597's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+11.953'}[22].
  • Q84217597's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+83.77714640472020'}[23].
  • Q84217597's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-6.00020678086410'}[24].
  • Q84217597's epoch is recorded as J2000.0[25].
  • Q84217597's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+3153'}[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] ↑ . The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. wikidata.org.
  8. [9] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  11. [12] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  12. [13] ↑ . Gaia Data Release 2. wikidata.org.
  13. [14] ↑ . Gaia Data Release 2. wikidata.org.
  14. [15] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  15. [16] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. 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] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . wikidata.org.
  21. [22] ↑ . IN-SYNC. IV. The young stellar population in the Orion A molecular cloud. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . Gaia Data Release 2. wikidata.org.
  25. [26] ↑ . IN-SYNC. IV. The young stellar population in the Orion A molecular cloud. 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). Q84217597. Retrieved May 7, 2026, from https://4ort.xyz/entity/q84217597
MLA “Q84217597.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q84217597.
BibTeX @misc{4ortxyz_q84217597_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q84217597}}, year = {2026}, url = {https://4ort.xyz/entity/q84217597}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q84217597 — https://4ort.xyz/entity/q84217597 (retrieved 2026-05-07)

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