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Q88422414

red giant branch star in the constellation Hercules
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Q88422414

Summary

Q88422414 is a red giant branch star[1].

Key Facts

  • Q88422414's instance of is recorded as red giant branch star[2].
  • Q88422414's constellation is recorded as Hercules[3].
  • Q88422414 is part of Messier 13[4].
  • Q88422414's catalog code is recorded as Cl* NGC 6205 KAD 674[5].
  • Q88422414's catalog code is recorded as Cl* NGC 6205 BROWN N27[6].
  • Q88422414's catalog code is recorded as 2MASS J16422126+3633533[7].
  • Q88422414's catalog code is recorded as Pul -3 1330141[8].
  • Q88422414's catalog code is recorded as [SLB2011b] 250.58877+36.56480[9].
  • Q88422414's catalog code is recorded as SDSS J164221.30+363353.2[10].
  • Q88422414's catalog code is recorded as Gaia DR2 1328065121281746560[11].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.06'}[12].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.26'}[13].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.680'}[14].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.230'}[15].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.147'}[16].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.981'}[17].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.521'}[18].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.885'}[19].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.713'}[20].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.600'}[21].
  • Q88422414's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.0235'}[22].
  • Q88422414's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0457'}[23].
  • Q88422414's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-249.4'}[24].
  • Q88422414's metallicity is recorded as {'unit': '1', 'amount': '-1.56'}[25].
  • Q88422414's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+250.58860460728660'}[26].

Body

Definition and Type

Q88422414's instance of is recorded as red giant branch star[2].

Use and Application

Q88422414 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] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . Mass outflow and chromospheric activity of red giant stars in globular clusters. II. M13 and M92. wikidata.org.
  12. [13] ↑ . Mass outflow and chromospheric activity of red giant stars in globular clusters. II. M13 and M92. wikidata.org.
  13. [14] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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] ↑ . 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] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . Differences in the rotational properties of multiple stellar populations in M13: a faster rotation for the ‘extreme’ chemical subpopulation. wikidata.org.
  24. [25] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. 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). Q88422414. Retrieved May 7, 2026, from https://4ort.xyz/entity/q88422414
MLA “Q88422414.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q88422414.
BibTeX @misc{4ortxyz_q88422414_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q88422414}}, year = {2026}, url = {https://4ort.xyz/entity/q88422414}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q88422414 — https://4ort.xyz/entity/q88422414 (retrieved 2026-05-07)

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