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Q85930697

Thing exoplanet Q85930697
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Q85930697

Summary

Q85930697 is an exoplanet[1].

Key Facts

  • Q85930697's instance of is recorded as exoplanet[2].
  • Q85930697's constellation is recorded as Cygnus[3].
  • Q85930697's parent astronomical body is recorded as Q90113184[4].
  • Q85930697's parent astronomical body is recorded as Q78174663[5].
  • Q85930697's catalog code is recorded as KOI-2174.02[6].
  • Q85930697's catalog code is recorded as Kepler-1802c[7].
  • Q85930697's catalog code is recorded as Kepler-1802 Bc[8].
  • Q85930697's catalog code is recorded as KOI-2174c[9].
  • Q85930697's time of discovery or invention is recorded as +2017-00-00T00:00:00Z[10].
  • Q85930697's time of discovery or invention is recorded as +2022-02-00T00:00:00Z[11].
  • Q85930697's discovery method is recorded as transit method[12].
  • Q85930697's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.38'}[13].
  • Q85930697's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+2.322'}[14].
  • Q85930697's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+33.13610077'}[15].
  • Q85930697's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.1723'}[16].
  • Q85930697's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+21400'}[17].
  • Q85930697's SIMBAD ID is recorded as Kepler-1802c[18].
  • Q85930697's Extrasolar Planets Encyclopaedia exoplanet ID is recorded as kepler_1802_bc--4434[19].
  • Q85930697's NASA Exoplanet Archive ID is recorded as Kepler-1802 c[20].
  • Q85930697's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+300.2420869'}[21].
  • Q85930697's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.1412854'}[22].
  • Q85930697's epoch is recorded as J2000.0[23].
  • Q85930697's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+6'}[24].
  • Q85930697's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2'}[25].

References

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

Direct Wikidata claims

  1. [2] ↑ . Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. wikidata.org.
  2. [3] ↑ . wikidata.org.
  3. [4] ↑ . Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data. wikidata.org.
  4. [5] ↑ . Exoplanet Archive. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . Exoplanet Archive. wikidata.org.
  7. [8] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  8. [9] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  9. [10] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  10. [11] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  11. [12] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  12. [13] ↑ . Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25. wikidata.org.
  13. [14] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  14. [15] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  15. [16] ↑ . Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25. wikidata.org.
  16. [17] ↑ . Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?. wikidata.org.
  17. [18] ↑ . wikidata.org.
  18. [19] ↑ . wikidata.org.
  19. [20] ↑ . wikidata.org.
  20. [21] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  21. [22] ↑ . ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier that Validates 301 New Exoplanets. wikidata.org.
  22. [23] ↑ . SIMBAD. wikidata.org.
  23. [24] ↑ . SIMBAD. wikidata.org.
  24. [25] ↑ . SIMBAD. 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). Q85930697. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85930697
MLA “Q85930697.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85930697.
BibTeX @misc{4ortxyz_q85930697_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85930697}}, year = {2026}, url = {https://4ort.xyz/entity/q85930697}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85930697 — https://4ort.xyz/entity/q85930697 (retrieved 2026-05-07)

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