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Q85263267

white dwarf in the constellation Lyra
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Q85263267

Summary

Q85263267 is a white dwarf[1].

Key Facts

  • Q85263267's instance of is recorded as white dwarf[2].
  • Q85263267's constellation is recorded as Lyra[3].
  • Q85263267's spectral class is recorded as DA[4].
  • Q85263267's catalog code is recorded as Gaia DR2 2101020107679847552[5].
  • Q85263267's catalog code is recorded as SDSS J191719.16+392718.8[6].
  • Q85263267's catalog code is recorded as KIC 4357037[7].
  • Q85263267's catalog code is recorded as KIS J191719.17+392718.2[8].
  • Q85263267's catalog code is recorded as EQ J1917+3927[9].
  • Q85263267's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.91'}[10].
  • Q85263267's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.2720'}[11].
  • Q85263267's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.70'}[12].
  • Q85263267's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.51'}[13].
  • Q85263267's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.39'}[14].
  • Q85263267's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.21'}[15].
  • Q85263267's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.56'}[16].
  • Q85263267's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.0847'}[17].
  • Q85263267's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+196.668'}[18].
  • Q85263267's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+289.32988609316294'}[19].
  • Q85263267's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+39.45536918823473'}[20].
  • Q85263267's epoch is recorded as J2000.0[21].
  • Q85263267's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+12650'}[22].
  • Q85263267's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+12750'}[23].
  • Q85263267's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+103000000'}[24].
  • Q85263267's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+104700000'}[25].
  • Q85263267's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-99.597'}[26].

Body

Definition and Type

Q85263267's instance of is recorded as white dwarf[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 search for ZZ Ceti stars in the original Kepler mission. 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 search for ZZ Ceti stars in the original Kepler mission. wikidata.org.
  10. [11] ↑ . Gaia Data Release 2. wikidata.org.
  11. [12] ↑ . DA white dwarfs in Sloan Digital Sky Survey Data Release 7 and a search for infrared excess emission. wikidata.org.
  12. [13] ↑ . DA white dwarfs in Sloan Digital Sky Survey Data Release 7 and a search for infrared excess emission. wikidata.org.
  13. [14] ↑ . DA white dwarfs in Sloan Digital Sky Survey Data Release 7 and a search for infrared excess emission. wikidata.org.
  14. [15] ↑ . DA white dwarfs in Sloan Digital Sky Survey Data Release 7 and a search for infrared excess emission. wikidata.org.
  15. [16] ↑ . DA white dwarfs in Sloan Digital Sky Survey Data Release 7 and a search for infrared excess emission. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Line Widths: Kepler Observations of 27 Pulsating DA White Dwarfs through K2 Campaign 8. wikidata.org.
  22. [23] ↑ . White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Line Widths: Kepler Observations of 27 Pulsating DA White Dwarfs through K2 Campaign 8. wikidata.org.
  23. [24] ↑ . White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Line Widths: Kepler Observations of 27 Pulsating DA White Dwarfs through K2 Campaign 8. wikidata.org.
  24. [25] ↑ . White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Line Widths: Kepler Observations of 27 Pulsating DA White Dwarfs through K2 Campaign 8. 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). Q85263267. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85263267
MLA “Q85263267.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85263267.
BibTeX @misc{4ortxyz_q85263267_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85263267}}, year = {2026}, url = {https://4ort.xyz/entity/q85263267}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85263267 — https://4ort.xyz/entity/q85263267 (retrieved 2026-05-07)

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