Omega Serpentis b

exoplanet
Place exoplanet Q88863900
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Omega Serpentis b

Summary

Omega Serpentis b is an exoplanet[1].

Key Facts

  • Omega Serpentis b's instance of is recorded as exoplanet[2].
  • Omega Serpentis b's constellation is recorded as Serpens[3].
  • Omega Serpentis b's parent astronomical body is recorded as Omega Serpentis[4].
  • Omega Serpentis b's catalog code is recorded as TIC 272677041b[5].
  • Omega Serpentis b's time of discovery or invention is recorded as +2013-08-00T00:00:00Z[6].
  • Omega Serpentis b's discovery method is recorded as Doppler spectroscopy[7].
  • Omega Serpentis b's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.18'}[8].
  • Omega Serpentis b's M sin i is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+0.736'}[9].
  • Omega Serpentis b's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+1.7'}[10].
  • Omega Serpentis b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+278.59'}[11].
  • Omega Serpentis b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.0020'}[12].
  • Omega Serpentis b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.838'}[13].
  • Omega Serpentis b's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+143.2'}[14].
  • Omega Serpentis b's SIMBAD ID is recorded as * ome Ser b[15].
  • Omega Serpentis b's Wolfram Language entity code is recorded as Entity["Exoplanet", "OmegaSerpentisb"][16].
  • Omega Serpentis b's Extrasolar Planets Encyclopaedia exoplanet ID is recorded as ome_ser_ab--1264[17].
  • Omega Serpentis b's NASA Exoplanet Archive ID is recorded as ome Ser b[18].
  • Omega Serpentis b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+237.57311038624414'}[19].
  • Omega Serpentis b's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+2.19651084789306'}[20].
  • Omega Serpentis b's epoch is recorded as J2000.0[21].
  • Omega Serpentis b's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-48.052'}[22].
  • Omega Serpentis b's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+30.598'}[23].
  • Omega Serpentis b's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2450022'}[24].

Body

Designation and Status

Omega Serpentis b's instance of is recorded as exoplanet[2].

History and Context

Omega Serpentis b's catalog code is recorded as TIC 272677041b[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] . SIMBAD. wikidata.org.
  4. [5] . Exoplanet Archive. wikidata.org.
  5. [6] . Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, and ω Serpentis. wikidata.org.
  6. [7] . Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, and ω Serpentis. 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] . wikidata.org.
  18. [19] . Gaia Data Release 2. wikidata.org.
  19. [20] . Gaia Data Release 2. wikidata.org.
  20. [21] . SIMBAD. wikidata.org.
  21. [22] . Gaia Data Release 2. wikidata.org.
  22. [23] . Gaia Data Release 2. wikidata.org.
  23. [24] . Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, and ω Serpentis. 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). Omega Serpentis b. Retrieved May 3, 2026, from https://4ort.xyz/entity/omega-serpentis-b
MLA “Omega Serpentis b.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/omega-serpentis-b.
BibTeX @misc{4ortxyz_omega-serpentis-b_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Omega Serpentis b}}, year = {2026}, url = {https://4ort.xyz/entity/omega-serpentis-b}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Omega Serpentis b — https://4ort.xyz/entity/omega-serpentis-b (retrieved 2026-05-03)

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