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Q85438137

exoplanet in the constellation Andromeda
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Q85438137

Summary

Q85438137 is an exoplanet[1].

Key Facts

  • Q85438137's instance of is recorded as exoplanet[2].
  • Q85438137's constellation is recorded as Andromeda[3].
  • Q85438137's parent astronomical body is recorded as HAT-P-53[4].
  • Q85438137's catalog code is recorded as TOI-3630.01[5].
  • Q85438137's catalog code is recorded as TIC 189380158b[6].
  • Q85438137's catalog code is recorded as TIC 189380158.01[7].
  • Q85438137's time of discovery or invention is recorded as +2015-12-00T00:00:00Z[8].
  • Q85438137's discovery method is recorded as transit method[9].
  • Q85438137's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.085'}[10].
  • Q85438137's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+86.2'}[11].
  • Q85438137's M sin i is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+1.484'}[12].
  • Q85438137's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+1.477'}[13].
  • Q85438137's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+1.318'}[14].
  • Q85438137's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+1.96162529'}[15].
  • Q85438137's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.4711'}[16].
  • Q85438137's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.0316'}[17].
  • Q85438137's SIMBAD ID is recorded as HAT-P-53b[18].
  • Q85438137's Wolfram Language entity code is recorded as Entity["Exoplanet", "HATMinusPMinus53b"][19].
  • Q85438137's Extrasolar Planets Encyclopaedia exoplanet ID is recorded as hat_p_53_b--2383[20].
  • Q85438137's NASA Exoplanet Archive ID is recorded as HAT-P-53 b[21].
  • Q85438137's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+21.87110220329458'}[22].
  • Q85438137's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+38.96812761735945'}[23].
  • Q85438137's epoch is recorded as J2000.0[24].
  • Q85438137's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.236'}[25].
  • Q85438137's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.176'}[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] ↑ . HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey. wikidata.org.
  4. [5] ↑ . Exoplanet Archive. wikidata.org.
  5. [6] ↑ . Exoplanet Archive. wikidata.org.
  6. [7] ↑ . Exoplanet Archive. wikidata.org.
  7. [8] ↑ . HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey. wikidata.org.
  8. [9] ↑ . HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey. wikidata.org.
  9. [10] ↑ . 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.
  10. [11] ↑ . 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.
  11. [12] ↑ . HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey. wikidata.org.
  12. [13] ↑ . 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.
  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] ↑ . Looking for timing variations in the transits of 16 exoplanets. wikidata.org.
  15. [16] ↑ . Gaia Data Release 2. 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] ↑ . wikidata.org.
  18. [19] ↑ . wikidata.org.
  19. [20] ↑ . wikidata.org.
  20. [21] ↑ . wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . SIMBAD. wikidata.org.
  24. [25] ↑ . Gaia Data Release 2. wikidata.org.
  25. [26] ↑ . Gaia Data Release 2. 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). Q85438137. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85438137
MLA “Q85438137.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85438137.
BibTeX @misc{4ortxyz_q85438137_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85438137}}, year = {2026}, url = {https://4ort.xyz/entity/q85438137}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85438137 — https://4ort.xyz/entity/q85438137 (retrieved 2026-05-07)

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