Kepler-51 b

extrasolar planet
Place super_puff Q19758286
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Kepler-51 b

Summary

Kepler-51 b is a super-puff[1]. It draws 3 Wikipedia views per month (super_puff category, ranking #2 of 2).[2]

Key Facts

  • Kepler-51 b's image is recorded as Kepler 51 planets compared to some of the planets in our Solar system.png[3].
  • Kepler-51 b's instance of is recorded as super-puff[4].
  • Kepler-51 b's instance of is recorded as exoplanet[5].
  • Kepler-51 b's constellation is recorded as Cygnus[6].
  • Kepler-51 b's Commons category is recorded as Kepler-51 b[7].
  • Kepler-51 b's parent astronomical body is recorded as Kepler-51[8].
  • Kepler-51 b's catalog code is recorded as Kepler-51b[9].
  • Kepler-51 b's catalog code is recorded as KOI-620.01[10].
  • Kepler-51 b's catalog code is recorded as KOI-620b[11].
  • Kepler-51 b's catalog code is recorded as TIC 27846348b[12].
  • Kepler-51 b's time of discovery or invention is recorded as +2012-00-00T00:00:00Z[13].
  • Kepler-51 b's time of discovery or invention is recorded as +2013-01-00T00:00:00Z[14].
  • Kepler-51 b's discovery method is recorded as transit method[15].
  • Kepler-51 b's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.03'}[16].
  • Kepler-51 b's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.78'}[17].
  • Kepler-51 b's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q681996', 'amount': '+3.69'}[18].
  • Kepler-51 b's temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+543.0'}[19].
  • Kepler-51 b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+6.89'}[20].
  • Kepler-51 b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+45.1555023'}[21].
  • Kepler-51 b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+45.1542'}[22].
  • Kepler-51 b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+45.15529288'}[23].
  • Kepler-51 b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+45.15530074'}[24].
  • Kepler-51 b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+45.1553095644'}[25].
  • Kepler-51 b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+45.154'}[26].
  • Kepler-51 b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2473'}[27].

Body

Designation and Status

Recorded instance of include super-puff[4] and exoplanet[5].

History and Context

Catalog codes include Kepler-51b[9], KOI-620.01[10], KOI-620b[11], and TIC 27846348b[12].

Why It Matters

Kepler-51 b draws 3 Wikipedia views per month (super_puff category, ranking #2 of 2).[2]

References

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

Direct Wikidata claims

  1. [3] . wikidata.org.
  2. [4] . The Featureless Transmission Spectra of Two Super-puff Planets. wikidata.org.
  3. [5] . SIMBAD. wikidata.org.
  4. [6] . wikidata.org.
  5. [7] . wikidata.org.
  6. [8] . SIMBAD. wikidata.org.
  7. [9] . SIMBAD. wikidata.org.
  8. [10] . SIMBAD. wikidata.org.
  9. [11] . Exoplanet Archive. wikidata.org.
  10. [12] . Exoplanet Archive. wikidata.org.
  11. [13] . Extrasolar Planets Encyclopaedia. wikidata.org.
  12. [14] . Transit timing observations from Kepler – VII. Confirmation of 27 planets in 13 multiplanet systems via transit timing variations and orbital stability. wikidata.org.
  13. [15] . Transit timing observations from Kepler – VII. Confirmation of 27 planets in 13 multiplanet systems via transit timing variations and orbital stability. wikidata.org.
  14. [16] . The Featureless Transmission Spectra of Two Super-puff Planets. wikidata.org.
  15. [17] . The Featureless Transmission Spectra of Two Super-puff Planets. wikidata.org.
  16. [18] . The Featureless Transmission Spectra of Two Super-puff Planets. wikidata.org.
  17. [19] . Extrasolar Planets Encyclopaedia. wikidata.org.
  18. [20] . The Featureless Transmission Spectra of Two Super-puff Planets. wikidata.org.
  19. [21] . Transit timing observations from Kepler – VII. Confirmation of 27 planets in 13 multiplanet systems via transit timing variations and orbital stability. wikidata.org.
  20. [22] . The Featureless Transmission Spectra of Two Super-puff Planets. wikidata.org.
  21. [23] . Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. wikidata.org.
  22. [24] . False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. wikidata.org.
  23. [25] . Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets. wikidata.org.
  24. [26] . Very low density planets around Kepler-51 revealed with transit timing variations and an anomaly similar to a planet-planet eclipse event. wikidata.org.
  25. [27] . Gaia Data Release 2. 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-51 b. Retrieved May 3, 2026, from https://4ort.xyz/entity/kepler-51-b
MLA “Kepler-51 b.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/kepler-51-b.
BibTeX @misc{4ortxyz_kepler-51-b_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Kepler-51 b}}, year = {2026}, url = {https://4ort.xyz/entity/kepler-51-b}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Kepler-51 b — https://4ort.xyz/entity/kepler-51-b (retrieved 2026-05-03)

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