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Q113595459

exoplanet in the constellation Draco
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Q113595459

Summary

Q113595459 is an exoplanet[1].

Key Facts

  • Q113595459's instance of is recorded as exoplanet[2].
  • Q113595459's constellation is recorded as Draco[3].
  • Q113595459's parent astronomical body is recorded as Q85185054[4].
  • Q113595459's catalog code is recorded as TOI-1670c[5].
  • Q113595459's catalog code is recorded as TOI-1670.01[6].
  • Q113595459's catalog code is recorded as TIC 441739020c[7].
  • Q113595459's catalog code is recorded as TIC 441739020.01[8].
  • Q113595459's time of discovery or invention is recorded as +2022-03-00T00:00:00Z[9].
  • Q113595459's discovery method is recorded as transit method[10].
  • Q113595459's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.09'}[11].
  • Q113595459's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+88.84'}[12].
  • Q113595459's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.63'}[13].
  • Q113595459's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q3421309', 'amount': '+0.987'}[14].
  • Q113595459's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+40.74976'}[15].
  • Q113595459's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.0224'}[16].
  • Q113595459's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.249'}[17].
  • Q113595459's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+105.5'}[18].
  • Q113595459's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+259.0172522'}[19].
  • Q113595459's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+72.1611806'}[20].
  • Q113595459's epoch is recorded as J2000.0[21].
  • Q113595459's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.923'}[22].
  • Q113595459's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.007'}[23].

Body

Definition and Type

Q113595459'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] ↑ . Exoplanet Archive. wikidata.org.
  5. [6] ↑ . Exoplanet Archive. wikidata.org.
  6. [7] ↑ . Exoplanet Archive. wikidata.org.
  7. [8] ↑ . Exoplanet Archive. wikidata.org.
  8. [9] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  9. [10] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  10. [11] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  11. [12] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  12. [13] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  13. [14] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  14. [15] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  15. [16] ↑ . Gaia Early Data Release 3. wikidata.org.
  16. [17] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  17. [18] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  18. [19] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  19. [20] ↑ . TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration. wikidata.org.
  20. [21] ↑ . SIMBAD. wikidata.org.
  21. [22] ↑ . Gaia Early Data Release 3. wikidata.org.
  22. [23] ↑ . Gaia Early Data Release 3. 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). Q113595459. Retrieved May 7, 2026, from https://4ort.xyz/entity/q113595459
MLA “Q113595459.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q113595459.
BibTeX @misc{4ortxyz_q113595459_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q113595459}}, year = {2026}, url = {https://4ort.xyz/entity/q113595459}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q113595459 — https://4ort.xyz/entity/q113595459 (retrieved 2026-05-07)

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