Home › Entities › exoplanet › 24 Boötis b

24 Boötis b

extrasolar planet
Place exoplanet Q77929709
Press Enter · cited answer in seconds

24 Boötis b

Summary

24 Boötis b is an exoplanet[1].

Key Facts

  • 24 Boötis b's instance of is recorded as exoplanet[2].
  • 24 Boötis b's constellation is recorded as Boötes[3].
  • 24 Boötis b's parent astronomical body is recorded as 24 Boötis[4].
  • 24 Boötis b's catalog code is recorded as TIC 441712711b[5].
  • 24 Boötis b's time of discovery or invention is recorded as +2018-08-00T00:00:00Z[6].
  • 24 Boötis b's discovery method is recorded as Doppler spectroscopy[7].
  • 24 Boötis b's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.032'}[8].
  • 24 Boötis b's M sin i is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.883'}[9].
  • 24 Boötis b's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.91'}[10].
  • 24 Boötis b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+30.33'}[11].
  • 24 Boötis b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.3900'}[12].
  • 24 Boötis b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.194'}[13].
  • 24 Boötis b's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-179.2'}[14].
  • 24 Boötis b's SIMBAD ID is recorded as * 24 Boo b[15].
  • 24 Boötis b's Extrasolar Planets Encyclopaedia exoplanet ID is recorded as 24_boo_b--6733[16].
  • 24 Boötis b's NASA Exoplanet Archive ID is recorded as 24 Boo b[17].
  • 24 Boötis b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+217.1555242'}[18].
  • 24 Boötis b's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.8446488'}[19].
  • 24 Boötis b's epoch is recorded as J2000.0[20].
  • 24 Boötis b's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-46.816'}[21].
  • 24 Boötis b's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-304.064'}[22].
  • 24 Boötis b's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2450008.6'}[23].

Body

Designation and Status

24 Boötis b's instance of is recorded as exoplanet[2].

History and Context

24 Boötis b's catalog code is recorded as TIC 441712711b[5].

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] ↑ . Planets around the evolved stars 24 Boötis and γ Libra: A 30 d-period planet and a double giant-planet system in possible 7:3 MMR. wikidata.org.
  4. [5] ↑ . Exoplanet Archive. wikidata.org.
  5. [6] ↑ . Planets around the evolved stars 24 Boötis and γ Libra: A 30 d-period planet and a double giant-planet system in possible 7:3 MMR. wikidata.org.
  6. [7] ↑ . Planets around the evolved stars 24 Boötis and γ Libra: A 30 d-period planet and a double giant-planet system in possible 7:3 MMR. wikidata.org.
  7. [8] ↑ . Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars. wikidata.org.
  8. [9] ↑ . Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars. wikidata.org.
  9. [10] ↑ . Extrasolar Planets Encyclopaedia. wikidata.org.
  10. [11] ↑ . Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars. wikidata.org.
  11. [12] ↑ . Gaia Data Release 2. wikidata.org.
  12. [13] ↑ . Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars. wikidata.org.
  13. [14] ↑ . Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars. wikidata.org.
  14. [15] ↑ . wikidata.org.
  15. [16] ↑ . wikidata.org.
  16. [17] ↑ . wikidata.org.
  17. [18] ↑ . Planets around the evolved stars 24 Boötis and γ Libra: A 30 d-period planet and a double giant-planet system in possible 7:3 MMR. wikidata.org.
  18. [19] ↑ . Planets around the evolved stars 24 Boötis and γ Libra: A 30 d-period planet and a double giant-planet system in possible 7:3 MMR. wikidata.org.
  19. [20] ↑ . SIMBAD. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Planets around the evolved stars 24 Boötis and γ Libra: A 30 d-period planet and a double giant-planet system in possible 7:3 MMR. 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). 24 Boötis b. Retrieved May 3, 2026, from https://4ort.xyz/entity/24-bo-tis-b
MLA “24 Boötis b.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/24-bo-tis-b.
BibTeX @misc{4ortxyz_24-bo-tis-b_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{24 Boötis b}}, year = {2026}, url = {https://4ort.xyz/entity/24-bo-tis-b}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): 24 Boötis b — https://4ort.xyz/entity/24-bo-tis-b (retrieved 2026-05-03)

Canonical URL: https://4ort.xyz/entity/24-bo-tis-b · Last refreshed: