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Q88422298

red giant branch star in the constellation Hercules
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Q88422298

Summary

Q88422298 is a red giant branch star[1].

Key Facts

  • Q88422298's instance of is recorded as red giant branch star[2].
  • Q88422298's constellation is recorded as Hercules[3].
  • Q88422298 is part of Messier 13[4].
  • Q88422298's catalog code is recorded as Cl* NGC 6205 KAD 621[5].
  • Q88422298's catalog code is recorded as NGC 6205 1097[6].
  • Q88422298's catalog code is recorded as 2MASS J16420340+3630182[7].
  • Q88422298's catalog code is recorded as [SLB2011b] 250.51434+36.50500[8].
  • Q88422298's catalog code is recorded as SDSS J164203.44+363018.0[9].
  • Q88422298's catalog code is recorded as Gaia DR2 1328059142688301056[10].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.32'}[11].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.691'}[12].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.136'}[13].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.061'}[14].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.40'}[15].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.340'}[16].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.741'}[17].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.097'}[18].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.791'}[19].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.653'}[20].
  • Q88422298's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1388'}[21].
  • Q88422298's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0506'}[22].
  • Q88422298's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-256.7'}[23].
  • Q88422298's metallicity is recorded as {'unit': '1', 'amount': '-1.48'}[24].
  • Q88422298's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+250.51415989294130'}[25].
  • Q88422298's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+36.50506179014770'}[26].

Body

Definition and Type

Q88422298's instance of is recorded as red giant branch star[2].

Use and Application

Q88422298 is part of Messier 13[4].

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] ↑ . 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] ↑ . Mass outflow and chromospheric activity of red giant stars in globular clusters. II. M13 and M92. wikidata.org.
  11. [12] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  12. [13] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  14. [15] ↑ . Mass outflow and chromospheric activity of red giant stars in globular clusters. II. M13 and M92. wikidata.org.
  15. [16] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  16. [17] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  17. [18] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  18. [19] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  19. [20] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Differences in the rotational properties of multiple stellar populations in M13: a faster rotation for the ‘extreme’ chemical subpopulation. wikidata.org.
  23. [24] ↑ . Oxygen and sodium abundances in M13 (NGC 6205) giants: linking globular cluster formation scenarios, deep mixing, and post-RGB evolution. 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). Q88422298. Retrieved May 7, 2026, from https://4ort.xyz/entity/q88422298
MLA “Q88422298.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q88422298.
BibTeX @misc{4ortxyz_q88422298_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q88422298}}, year = {2026}, url = {https://4ort.xyz/entity/q88422298}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q88422298 — https://4ort.xyz/entity/q88422298 (retrieved 2026-05-07)

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