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Kepler-74b

extrasolar planet
Thing exoplanet Q21030073
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Kepler-74b

Summary

Kepler-74b is an exoplanet[1].

Key Facts

  • Kepler-74b's instance of is recorded as exoplanet[2].
  • Kepler-74b's constellation is recorded as Cygnus[3].
  • Kepler-74b's parent astronomical body is recorded as Q82201085[4].
  • Kepler-74b's catalog code is recorded as KOI-200b[5].
  • Kepler-74b's catalog code is recorded as Kepler-74b[6].
  • Kepler-74b's catalog code is recorded as TOI-4485b[7].
  • Kepler-74b's catalog code is recorded as KOI-200.01[8].
  • Kepler-74b's catalog code is recorded as TOI-4485.01[9].
  • Kepler-74b's catalog code is recorded as TIC 137903329b[10].
  • Kepler-74b's time of discovery or invention is recorded as +2012-00-00T00:00:00Z[11].
  • Kepler-74b's time of discovery or invention is recorded as +2013-06-00T00:00:00Z[12].
  • Kepler-74b's discovery method is recorded as transit method[13].
  • Kepler-74b's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+87.46'}[14].
  • Kepler-74b's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.604'}[15].
  • Kepler-74b's temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+1078.0'}[16].
  • Kepler-74b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+12.817'}[17].
  • Kepler-74b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+7.340718'}[18].
  • Kepler-74b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+7.340711'}[19].
  • Kepler-74b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+7.34071497'}[20].
  • Kepler-74b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+7.340714746'}[21].
  • Kepler-74b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+7.3407146305'}[22].
  • Kepler-74b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8208'}[23].
  • Kepler-74b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.07813'}[24].
  • Kepler-74b's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+60'}[25].
  • Kepler-74b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.09253632585876'}[26].

Body

Definition and Type

Kepler-74b'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] ↑ . SIMBAD. 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] ↑ . wikidata.org.
  11. [12] ↑ . KOI-200 b and KOI-889 b: two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N. wikidata.org.
  12. [13] ↑ . KOI-200 b and KOI-889 b: two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N. wikidata.org.
  13. [14] ↑ . 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.
  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] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  16. [17] ↑ . Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . KOI-200 b and KOI-889 b: two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N. wikidata.org.
  18. [19] ↑ . 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.
  19. [20] ↑ . Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. wikidata.org.
  20. [21] ↑ . False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. wikidata.org.
  21. [22] ↑ . Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . 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.
  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-74b. Retrieved May 7, 2026, from https://4ort.xyz/entity/q21030073
MLA “Kepler-74b.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q21030073.
BibTeX @misc{4ortxyz_q21030073_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Kepler-74b}}, year = {2026}, url = {https://4ort.xyz/entity/q21030073}, note = {Accessed: 2026-05-07}}
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