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Kepler-103c

extrasolar planet
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Kepler-103c

Summary

Kepler-103c is an exoplanet[1].

Key Facts

  • Kepler-103c is credited with the discovery of Kepler Space Telescope[2].
  • Kepler-103c's instance of is recorded as exoplanet[3].
  • Kepler-103c's constellation is recorded as Lyra[4].
  • Kepler-103c's parent astronomical body is recorded as Q89740181[5].
  • Kepler-103c's catalog code is recorded as Kepler-103c[6].
  • Kepler-103c's catalog code is recorded as KOI-108.02[7].
  • Kepler-103c's catalog code is recorded as KOI-108c[8].
  • Kepler-103c's catalog code is recorded as TIC 121865656c[9].
  • Kepler-103c's time of discovery or invention is recorded as +2014-02-00T00:00:00Z[10].
  • Kepler-103c's discovery method is recorded as transit method[11].
  • Kepler-103c's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.1'}[12].
  • Kepler-103c's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.704'}[13].
  • Kepler-103c's M sin i is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.09578803277'}[14].
  • Kepler-103c's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.114'}[15].
  • Kepler-103c's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+5.613'}[16].
  • Kepler-103c's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+179.610099357'}[17].
  • Kepler-103c's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.9923'}[18].
  • Kepler-103c's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.6496719336'}[19].
  • Kepler-103c's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+344'}[20].
  • Kepler-103c's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+67400'}[21].
  • Kepler-103c's Google Knowledge Graph ID is recorded as /g/11c3v_tx0n[22].
  • Kepler-103c's SIMBAD ID is recorded as Kepler-103c[23].
  • Kepler-103c's Wolfram Language entity code is recorded as Entity["Exoplanet", "Kepler103c"][24].
  • Kepler-103c's Extrasolar Planets Encyclopaedia exoplanet ID is recorded as kepler_103_c--2475[25].
  • Kepler-103c's NASA Exoplanet Archive ID is recorded as Kepler-103 c[26].

Body

Works and Contributions

Kepler-103c is credited with the discovery of Kepler Space Telescope[2].

References

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

Direct Wikidata claims

  1. [3] ↑ . SIMBAD. wikidata.org.
  2. [4] ↑ . wikidata.org.
  3. [2] ↑ . wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . Exoplanet Archive. wikidata.org.
  8. [9] ↑ . Exoplanet Archive. wikidata.org.
  9. [10] ↑ . Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. wikidata.org.
  10. [11] ↑ . Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. wikidata.org.
  11. [12] ↑ . Using HARPS-N to characterize the long-period planets in the PH-2 and Kepler-103 systems. wikidata.org.
  12. [13] ↑ . Using HARPS-N to characterize the long-period planets in the PH-2 and Kepler-103 systems. wikidata.org.
  13. [14] ↑ . The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. wikidata.org.
  14. [15] ↑ . Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. wikidata.org.
  15. [16] ↑ . The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. wikidata.org.
  16. [17] ↑ . Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. wikidata.org.
  19. [20] ↑ . Using HARPS-N to characterize the long-period planets in the PH-2 and Kepler-103 systems. wikidata.org.
  20. [21] ↑ . Fundamental properties of Kepler planet-candidate host stars using asteroseismology. wikidata.org.
  21. [22] ↑ . wikidata.org.
  22. [23] ↑ . wikidata.org.
  23. [24] ↑ . wikidata.org.
  24. [25] ↑ . wikidata.org.
  25. [26] ↑ . 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). Kepler-103c. Retrieved May 7, 2026, from https://4ort.xyz/entity/q22257075
MLA “Kepler-103c.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q22257075.
BibTeX @misc{4ortxyz_q22257075_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Kepler-103c}}, year = {2026}, url = {https://4ort.xyz/entity/q22257075}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Kepler-103c — https://4ort.xyz/entity/q22257075 (retrieved 2026-05-07)

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