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Q85246757

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Q85246757

Summary

Q85246757 is a brown dwarf[1].

Key Facts

  • Q85246757's instance of is recorded as brown dwarf[2].
  • Q85246757's instance of is recorded as exoplanet[3].
  • Q85246757's instance of is recorded as star[4].
  • Q85246757's instance of is recorded as infrared source[5].
  • Q85246757's instance of is recorded as near-infrared source[6].
  • Q85246757's constellation is recorded as Pegasus[7].
  • Q85246757's spectral class is recorded as L2Vpec[8].
  • Q85246757 is part of Beta Pictoris moving group[9].
  • Q85246757's catalog code is recorded as 2MASS J22081363+2921215[10].
  • Q85246757's catalog code is recorded as 2MASSW J2208136+292121[11].
  • Q85246757's time of discovery or invention is recorded as +2000-00-00T00:00:00Z[12].
  • Q85246757's discovery method is recorded as direct imaging[13].
  • Q85246757's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.797'}[14].
  • Q85246757's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.793'}[15].
  • Q85246757's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.148'}[16].
  • Q85246757's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+10'}[17].
  • Q85246757's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.41'}[18].
  • Q85246757's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0251'}[19].
  • Q85246757's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-15.59'}[20].
  • Q85246757's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+50'}[21].
  • Q85246757's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+332.056792'}[22].
  • Q85246757's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+29.355972'}[23].
  • Q85246757's epoch is recorded as J2000.0[24].
  • Q85246757's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.0258'}[25].
  • Q85246757's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.0889'}[26].

Body

Definition and Type

Recorded instance of include brown dwarf[2], exoplanet[3], star[4], infrared source[5], and near-infrared source[6].

Use and Application

Q85246757 is part of Beta Pictoris moving group[9].

References

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

Direct Wikidata claims

  1. [2] ↑ . SIMBAD. wikidata.org.
  2. [3] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  3. [4] ↑ . SIMBAD. wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . wikidata.org.
  7. [8] ↑ . 67 Additional L Dwarfs Discovered by the Two Micron All Sky Survey. wikidata.org.
  8. [9] ↑ . SIMBAD. wikidata.org.
  9. [10] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  12. [13] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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] ↑ . Revealing the Vertical Cloud Structure of a Young Low-mass Brown Dwarf, an Analog to the β-Pictoris b Directly Imaged Exoplanet, through Keck I/MOSFIRE Spectrophotometric Variability. wikidata.org.
  17. [18] ↑ . Fundamental parameters and spectral energy distributions of young and field age objects with masses spanning the stellar to planetary regime. wikidata.org.
  18. [19] ↑ . The Hawaii infrared parallax program. II. Young ultracool field dwarfs. wikidata.org.
  19. [20] ↑ . Population properties of brown dwarf analogs to exoplanets. wikidata.org.
  20. [21] ↑ . The brown dwarf kinematics project I. Proper motions and tangential velocities for a large sample of late-type M, L, and T dwarfs. wikidata.org.
  21. [22] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  22. [23] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  23. [24] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  24. [25] ↑ . The Hawaii infrared parallax program. II. Young ultracool field dwarfs. wikidata.org.
  25. [26] ↑ . The Hawaii infrared parallax program. II. Young ultracool field dwarfs. 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). Q85246757. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85246757
MLA “Q85246757.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85246757.
BibTeX @misc{4ortxyz_q85246757_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85246757}}, year = {2026}, url = {https://4ort.xyz/entity/q85246757}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85246757 — https://4ort.xyz/entity/q85246757 (retrieved 2026-05-07)

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