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Q89574675

Algol variable in the constellation Capricornus
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Q89574675

Summary

Q89574675 is an Algol variable[1].

Key Facts

  • Q89574675's instance of is recorded as Algol variable[2].
  • Q89574675's constellation is recorded as Capricornus[3].
  • Q89574675's spectral class is recorded as G1.5V[4].
  • Q89574675's catalog code is recorded as BD-10 5791[5].
  • Q89574675's catalog code is recorded as GSC 05793-00603[6].
  • Q89574675's catalog code is recorded as PPM 205755[7].
  • Q89574675's catalog code is recorded as TYC 5793-603-1[8].
  • Q89574675's catalog code is recorded as 2MASS J21550720-0947572[9].
  • Q89574675's catalog code is recorded as 1RXS J215507.4-094807[10].
  • Q89574675's catalog code is recorded as ASAS J215507-0947.9[11].
  • Q89574675's catalog code is recorded as ASAS J215507-0948.1[12].
  • Q89574675's catalog code is recorded as Gaia DR1 2617895679171636736[13].
  • Q89574675's catalog code is recorded as Gaia DR2 2617895679171636736[14].
  • Q89574675's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.942'}[15].
  • Q89574675's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.655'}[16].
  • Q89574675's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.505'}[17].
  • Q89574675's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.91'}[18].
  • Q89574675's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.534'}[19].
  • Q89574675's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.298'}[20].
  • Q89574675's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.0757'}[21].
  • Q89574675's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.0152'}[22].
  • Q89574675's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-34.35'}[23].
  • Q89574675's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+166.2455'}[24].
  • Q89574675's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+46.8'}[25].
  • Q89574675's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+44.4'}[26].

Body

Definition and Type

Q89574675's instance of is recorded as Algol variable[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] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . SIMBAD. wikidata.org.
  8. [9] ↑ . SIMBAD. wikidata.org.
  9. [10] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . SIMBAD. wikidata.org.
  12. [13] ↑ . SIMBAD. wikidata.org.
  13. [14] ↑ . SIMBAD. wikidata.org.
  14. [15] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  15. [16] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  16. [17] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  17. [18] ↑ . The Tycho-2 catalogue of the 2.5 million brightest stars. wikidata.org.
  18. [19] ↑ . ASAS photometry of ROSAT sources. I. Periodic variable stars coincident with bright sources from the ROSAT All Sky Survey. wikidata.org.
  19. [20] ↑ . ASAS photometry of ROSAT sources. I. Periodic variable stars coincident with bright sources from the ROSAT All Sky Survey. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. wikidata.org.
  25. [26] ↑ . A spectroscopic survey of the youngest field stars in the solar neighborhood . II. The optically faint sample. 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). Q89574675. Retrieved May 7, 2026, from https://4ort.xyz/entity/q89574675
MLA “Q89574675.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q89574675.
BibTeX @misc{4ortxyz_q89574675_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q89574675}}, year = {2026}, url = {https://4ort.xyz/entity/q89574675}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q89574675 — https://4ort.xyz/entity/q89574675 (retrieved 2026-05-07)

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