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Q90199718

peculiar star in the constellation Pegasus
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Q90199718

Summary

Q90199718 is a peculiar star[1].

Key Facts

  • Q90199718's instance of is recorded as peculiar star[2].
  • Q90199718's constellation is recorded as Pegasus[3].
  • Q90199718's catalog code is recorded as BPS CS 29516-0024[4].
  • Q90199718's catalog code is recorded as 2MASS J22261535+0251462[5].
  • Q90199718's catalog code is recorded as Gaia DR2 2703747063191473536[6].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.57'}[7].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.43'}[8].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.636'}[9].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.061'}[10].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.973'}[11].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.011'}[12].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.416'}[13].
  • Q90199718's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2645'}[14].
  • Q90199718's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2842'}[15].
  • Q90199718's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-84.27'}[16].
  • Q90199718's metallicity is recorded as {'unit': '1', 'amount': '-3.06'}[17].
  • Q90199718's metallicity is recorded as {'unit': '1', 'amount': '-2.88'}[18].
  • Q90199718's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+336.56398974971320'}[19].
  • Q90199718's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+2.86286812206930'}[20].
  • Q90199718's epoch is recorded as J2000.0[21].
  • Q90199718's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4650'}[22].
  • Q90199718's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+16'}[23].
  • Q90199718's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+55'}[24].
  • Q90199718's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-38.707'}[25].
  • Q90199718's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.999'}[26].

Body

Definition and Type

Q90199718's instance of is recorded as peculiar star[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] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. wikidata.org.
  7. [8] ↑ . Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. wikidata.org.
  8. [9] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  9. [10] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  10. [11] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  11. [12] ↑ . Broadband UBVRCIC Photometry of Horizontal‐Branch and Metal‐poor Candidates from the HK and Hamburg/ESO Surveys. I. wikidata.org.
  12. [13] ↑ . Broadband UBVRCIC Photometry of Horizontal‐Branch and Metal‐poor Candidates from the HK and Hamburg/ESO Surveys. I. wikidata.org.
  13. [14] ↑ . Gaia Data Release 2. wikidata.org.
  14. [15] ↑ . Gaia Data Release 2. wikidata.org.
  15. [16] ↑ . First stars XII. Abundances in extremely metal-poor turnoff stars, and comparison with the giants. wikidata.org.
  16. [17] ↑ . LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. wikidata.org.
  17. [18] ↑ . LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. wikidata.org.
  22. [23] ↑ . LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. wikidata.org.
  23. [24] ↑ . LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. 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). Q90199718. Retrieved May 7, 2026, from https://4ort.xyz/entity/q90199718
MLA “Q90199718.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q90199718.
BibTeX @misc{4ortxyz_q90199718_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q90199718}}, year = {2026}, url = {https://4ort.xyz/entity/q90199718}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q90199718 — https://4ort.xyz/entity/q90199718 (retrieved 2026-05-07)

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