Kepler-43b

extrasolar planet
Place exoplanet Q18812303
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Kepler-43b

Summary

Kepler-43b is an exoplanet[1].

Key Facts

  • Kepler-43b is credited with the discovery of Kepler Space Telescope[2].
  • Kepler-43b's instance of is recorded as exoplanet[3].
  • Kepler-43b's constellation is recorded as Lyra[4].
  • Kepler-43b's parent astronomical body is recorded as Q4041996[5].
  • Kepler-43b's catalog code is recorded as KOI-135.01[6].
  • Kepler-43b's catalog code is recorded as Kepler-43b[7].
  • Kepler-43b's catalog code is recorded as TOI-2178b[8].
  • Kepler-43b's catalog code is recorded as KOI-135b[9].
  • Kepler-43b's catalog code is recorded as TOI-2178.01[10].
  • Kepler-43b's catalog code is recorded as TIC 164892194b[11].
  • Kepler-43b's time of discovery or invention is recorded as +2011-00-00T00:00:00Z[12].
  • Kepler-43b's time of discovery or invention is recorded as +2012-02-00T00:00:00Z[13].
  • Kepler-43b's discovery method is recorded as transit method[14].
  • Kepler-43b's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.028'}[15].
  • Kepler-43b's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+84.57'}[16].
  • Kepler-43b's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+3.14'}[17].
  • Kepler-43b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.2'}[18].
  • Kepler-43b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.115'}[19].
  • Kepler-43b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+12.425'}[20].
  • Kepler-43b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.16'}[21].
  • Kepler-43b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+11.67'}[22].
  • Kepler-43b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.12'}[23].
  • Kepler-43b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.219'}[24].
  • Kepler-43b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+3.02409309'}[25].
  • Kepler-43b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9653'}[26].

Body

Designation and Status

Kepler-43b's instance of is recorded as exoplanet[3].

History and Context

Catalog codes include KOI-135.01[6], Kepler-43b[7], TOI-2178b[8], KOI-135b[9], TOI-2178.01[10], and TIC 164892194b[11].

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] . Exoplanet Archive. wikidata.org.
  6. [7] . Exoplanet Archive. wikidata.org.
  7. [8] . Exoplanet Archive. wikidata.org.
  8. [9] . Exoplanet Archive. wikidata.org.
  9. [10] . Exoplanet Archive. wikidata.org.
  10. [11] . Exoplanet Archive. wikidata.org.
  11. [12] . Extrasolar Planets Encyclopaedia. wikidata.org.
  12. [13] . SOPHIE velocimetry of Kepler transit candidates. V. The three hot Jupiters KOI-135b, KOI-204b and KOI-203b (alias Kepler-17b). wikidata.org.
  13. [14] . SOPHIE velocimetry of Kepler transit candidates. V. The three hot Jupiters KOI-135b, KOI-204b and KOI-203b (alias Kepler-17b). wikidata.org.
  14. [15] . The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. wikidata.org.
  15. [16] . The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. wikidata.org.
  16. [17] . The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. wikidata.org.
  17. [18] . SOPHIE velocimetry of Kepler transit candidates. V. The three hot Jupiters KOI-135b, KOI-204b and KOI-203b (alias Kepler-17b). wikidata.org.
  18. [19] . Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets. wikidata.org.
  19. [20] . Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2. wikidata.org.
  20. [21] . The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. wikidata.org.
  21. [22] . False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. wikidata.org.
  22. [23] . Kepler-424 b: A "Lonely" Hot Jupiter That Found A Companion. wikidata.org.
  23. [24] . Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry. wikidata.org.
  24. [25] . The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. 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-43b. Retrieved May 3, 2026, from https://4ort.xyz/entity/kepler-43b
MLA “Kepler-43b.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/kepler-43b.
BibTeX @misc{4ortxyz_kepler-43b_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Kepler-43b}}, year = {2026}, url = {https://4ort.xyz/entity/kepler-43b}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Kepler-43b — https://4ort.xyz/entity/kepler-43b (retrieved 2026-05-03)

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