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Kepler-102e

extrasolar planet
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Kepler-102e

Summary

Kepler-102e is an exoplanet[1]. Kepler-102e draws 2 Wikipedia views per month (exoplanet category, ranking #96 of 578).[2]

Key Facts

  • Kepler-102e's instance of is recorded as exoplanet[3].
  • Kepler-102e's constellation is recorded as Lyra[4].
  • Kepler-102e's parent astronomical body is recorded as Q16852002[5].
  • Kepler-102e's catalog code is recorded as Kepler-102e[6].
  • Kepler-102e's catalog code is recorded as KOI-82.01[7].
  • Kepler-102e's catalog code is recorded as TOI-6005.01[8].
  • Kepler-102e's catalog code is recorded as KOI-82e[9].
  • Kepler-102e's catalog code is recorded as TOI-6005e[10].
  • Kepler-102e's catalog code is recorded as TIC 123357864e[11].
  • Kepler-102e's time of discovery or invention is recorded as +2014-00-00T00:00:00Z[12].
  • Kepler-102e's time of discovery or invention is recorded as +2013-00-00T00:00:00Z[13].
  • Kepler-102e's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[14].
  • Kepler-102e's discovery method is recorded as transit method[15].
  • Kepler-102e's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.0'}[16].
  • Kepler-102e's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.56'}[17].
  • Kepler-102e's M sin i is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.01491646276'}[18].
  • Kepler-102e's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.028'}[19].
  • Kepler-102e's temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+579.0'}[20].
  • Kepler-102e's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+2.414'}[21].
  • Kepler-102e's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+16.1456994111'}[22].
  • Kepler-102e's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.2478'}[23].
  • Kepler-102e's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.1162026732'}[24].
  • Kepler-102e's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+360'}[25].
  • Kepler-102e's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+33000'}[26].
  • Kepler-102e's Google Knowledge Graph ID is recorded as /g/11b7kggvly[27].

Body

Designation and Status

Kepler-102e's instance of is recorded as exoplanet[3].

History and Context

Catalog codes include Kepler-102e[6], KOI-82.01[7], TOI-6005.01[8], KOI-82e[9], TOI-6005e[10], and TIC 123357864e[11].

Why It Matters

Kepler-102e draws 2 Wikipedia views per month (exoplanet category, ranking #96 of 578).[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. [5] ↑ . SIMBAD. wikidata.org.
  4. [6] ↑ . SIMBAD. wikidata.org.
  5. [7] ↑ . SIMBAD. wikidata.org.
  6. [8] ↑ . Exoplanet Archive. wikidata.org.
  7. [9] ↑ . Exoplanet Archive. wikidata.org.
  8. [10] ↑ . Exoplanet Archive. wikidata.org.
  9. [11] ↑ . Exoplanet Archive. wikidata.org.
  10. [12] ↑ . wikidata.org.
  11. [13] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  12. [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.
  13. [15] ↑ . 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. [16] ↑ . 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.
  15. [17] ↑ . 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.
  16. [18] ↑ . The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. wikidata.org.
  17. [19] ↑ . Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. wikidata.org.
  18. [20] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  19. [21] ↑ . The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. wikidata.org.
  20. [22] ↑ . Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets. wikidata.org.
  21. [23] ↑ . Gaia Data Release 2. wikidata.org.
  22. [24] ↑ . The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. wikidata.org.
  23. [25] ↑ . 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.
  24. [26] ↑ . A statistical reconstruction of the planet population around Kepler solar-type stars. wikidata.org.
  25. [27] ↑ . wikidata.org.

Class ancestry

  1. [1] ↑ . Wikidata. wikidata.org.

Aggregate / graph-position facts

  1. [2] ↑ . Wikimedia Foundation. dumps.wikimedia.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-102e. Retrieved May 3, 2026, from https://4ort.xyz/entity/kepler-102e
MLA “Kepler-102e.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/kepler-102e.
BibTeX @misc{4ortxyz_kepler-102e_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Kepler-102e}}, year = {2026}, url = {https://4ort.xyz/entity/kepler-102e}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Kepler-102e — https://4ort.xyz/entity/kepler-102e (retrieved 2026-05-03)

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