Kepler-105b

extrasolar planet
Thing exoplanet Q19672616
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Kepler-105b

Summary

Kepler-105b is an exoplanet[1].

Key Facts

  • Kepler-105b's instance of is recorded as exoplanet[2].
  • Kepler-105b's constellation is recorded as Lyra[3].
  • Kepler-105b's parent astronomical body is recorded as Q85834048[4].
  • Kepler-105b's catalog code is recorded as KOI-115.01[5].
  • Kepler-105b's catalog code is recorded as Kepler-105b[6].
  • Kepler-105b's catalog code is recorded as KOI-115b[7].
  • Kepler-105b's catalog code is recorded as TIC 158625964b[8].
  • Kepler-105b's time of discovery or invention is recorded as +2014-00-00T00:00:00Z[9].
  • Kepler-105b's time of discovery or invention is recorded as +2013-00-00T00:00:00Z[10].
  • Kepler-105b's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[11].
  • Kepler-105b's discovery method is recorded as transit method[12].
  • Kepler-105b's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.47'}[13].
  • Kepler-105b's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+85.94'}[14].
  • Kepler-105b's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.016'}[15].
  • Kepler-105b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+2.802'}[16].
  • Kepler-105b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+5.412203'}[17].
  • Kepler-105b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.1490'}[18].
  • Kepler-105b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.0609'}[19].
  • Kepler-105b's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+272.16'}[20].
  • Kepler-105b's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+34600'}[21].
  • Kepler-105b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+287.88729767229006'}[22].
  • Kepler-105b's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+46.27621804218722'}[23].
  • Kepler-105b's epoch is recorded as J2000.0[24].
  • Kepler-105b's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-22.206'}[25].
  • Kepler-105b's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-9.641'}[26].

Body

Definition and Type

Kepler-105b's instance of is recorded as exoplanet[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] . Spectroscopy of faint Kepler mission exoplanet candidate host stars. wikidata.org.
  4. [5] . Extrasolar Planets Encyclopaedia. wikidata.org.
  5. [6] . Extrasolar Planets Encyclopaedia. wikidata.org.
  6. [7] . Extrasolar Planets Encyclopaedia. wikidata.org.
  7. [8] . Exoplanet Archive. wikidata.org.
  8. [9] . wikidata.org.
  9. [10] . Extrasolar Planets Encyclopaedia. wikidata.org.
  10. [11] . Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. wikidata.org.
  11. [12] . Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. wikidata.org.
  12. [13] . Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. wikidata.org.
  13. [14] . Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. wikidata.org.
  14. [15] . Densities and eccentricities of 139 Kepler planets from transit time variations. wikidata.org.
  15. [16] . Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2. wikidata.org.
  16. [17] . ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations. wikidata.org.
  17. [18] . Gaia Data Release 2. wikidata.org.
  18. [19] . High-resolution multi-band imaging for validation and characterization of small Kepler planets. wikidata.org.
  19. [20] . Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. wikidata.org.
  20. [21] . Spectroscopy of faint Kepler mission exoplanet candidate host stars. wikidata.org.
  21. [22] . Gaia Data Release 2. wikidata.org.
  22. [23] . Gaia Data Release 2. wikidata.org.
  23. [24] . SIMBAD. 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.

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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). Kepler-105b. Retrieved May 7, 2026, from https://4ort.xyz/entity/q19672616
MLA “Kepler-105b.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q19672616.
BibTeX @misc{4ortxyz_q19672616_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Kepler-105b}}, year = {2026}, url = {https://4ort.xyz/entity/q19672616}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Kepler-105b — https://4ort.xyz/entity/q19672616 (retrieved 2026-05-07)

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