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Q92692750

exoplanet in the constellation Lyra
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Q92692750

Summary

Q92692750 is an exoplanet[1].

Key Facts

  • Q92692750's instance of is recorded as exoplanet[2].
  • Q92692750's constellation is recorded as Lyra[3].
  • Q92692750's parent astronomical body is recorded as Q93256282[4].
  • Q92692750's catalog code is recorded as Kepler-1656b[5].
  • Q92692750's catalog code is recorded as KOI-367.01[6].
  • Q92692750's catalog code is recorded as TOI-4584b[7].
  • Q92692750's catalog code is recorded as KOI-367b[8].
  • Q92692750's catalog code is recorded as TOI-4584.01[9].
  • Q92692750's catalog code is recorded as TIC 120255950b[10].
  • Q92692750's time of discovery or invention is recorded as +2018-10-00T00:00:00Z[11].
  • Q92692750's discovery method is recorded as transit method[12].
  • Q92692750's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.838'}[13].
  • Q92692750's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.31'}[14].
  • Q92692750's M sin i is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.15'}[15].
  • Q92692750's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.15'}[16].
  • Q92692750's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+5.02'}[17].
  • Q92692750's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+31.562'}[18].
  • Q92692750's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.3511'}[19].
  • Q92692750's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.197'}[20].
  • Q92692750's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+52.8'}[21].
  • Q92692750's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+57200'}[22].
  • Q92692750's SIMBAD ID is recorded as Kepler-1656b[23].
  • Q92692750's Extrasolar Planets Encyclopaedia exoplanet ID is recorded as kepler_1656_b--6830[24].
  • Q92692750's NASA Exoplanet Archive ID is recorded as Kepler-1656 b[25].
  • Q92692750's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+284.4722473'}[26].

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] ↑ . An abundance of small exoplanets around stars with a wide range of metallicities. wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. 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] ↑ . Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity. wikidata.org.
  11. [12] ↑ . Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity. wikidata.org.
  12. [13] ↑ . Kepler-1656b’s Extreme Eccentricity: Signature of a Gentle Giant. wikidata.org.
  13. [14] ↑ . Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity. wikidata.org.
  14. [15] ↑ . Kepler-1656b’s Extreme Eccentricity: Signature of a Gentle Giant. wikidata.org.
  15. [16] ↑ . Kepler-1656b’s Extreme Eccentricity: Signature of a Gentle Giant. wikidata.org.
  16. [17] ↑ . Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity. wikidata.org.
  17. [18] ↑ . Kepler-1656b’s Extreme Eccentricity: Signature of a Gentle Giant. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity. wikidata.org.
  20. [21] ↑ . Kepler-1656b’s Extreme Eccentricity: Signature of a Gentle Giant. wikidata.org.
  21. [22] ↑ . A statistical reconstruction of the planet population around Kepler solar-type stars. wikidata.org.
  22. [23] ↑ . wikidata.org.
  23. [24] ↑ . wikidata.org.
  24. [25] ↑ . wikidata.org.
  25. [26] ↑ . Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity. 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). Q92692750. Retrieved May 7, 2026, from https://4ort.xyz/entity/q92692750
MLA “Q92692750.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q92692750.
BibTeX @misc{4ortxyz_q92692750_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q92692750}}, year = {2026}, url = {https://4ort.xyz/entity/q92692750}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q92692750 — https://4ort.xyz/entity/q92692750 (retrieved 2026-05-07)

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