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Q86183302

red giant branch star in the constellation Hercules
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Q86183302

Summary

Q86183302 is a red giant branch star[1].

Key Facts

  • Q86183302's instance of is recorded as red giant branch star[2].
  • Q86183302's constellation is recorded as Hercules[3].
  • Q86183302 is part of Messier 13[4].
  • Q86183302's catalog code is recorded as Cl* NGC 6205 KAD 438[5].
  • Q86183302's catalog code is recorded as 2MASS J16413806+3618143[6].
  • Q86183302's catalog code is recorded as [LBS2008] 250.4085236+36.303894[7].
  • Q86183302's catalog code is recorded as [LBS2008] 250.4085236+36.303902[8].
  • Q86183302's catalog code is recorded as [SLB2011b] 250.40852+36.30390[9].
  • Q86183302's catalog code is recorded as [SLB2011b] 250.40852+36.30389[10].
  • Q86183302's catalog code is recorded as SDSS J164138.04+361814.0[11].
  • Q86183302's catalog code is recorded as Gaia DR2 1328029623368412672[12].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.32'}[13].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.07'}[14].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.736'}[15].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.276'}[16].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.203'}[17].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.112'}[18].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.047'}[19].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.625'}[20].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.841'}[21].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.691'}[22].
  • Q86183302's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.1303'}[23].
  • Q86183302's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-246.9'}[24].
  • Q86183302's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-243.9'}[25].
  • Q86183302's metallicity is recorded as {'unit': '1', 'amount': '-1.65'}[26].

Body

Definition and Type

Q86183302's instance of is recorded as red giant branch star[2].

Use and Application

Q86183302 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] ↑ . 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] ↑ . Globular and open clusters observed by SDSS/SEGUE: the giant stars. wikidata.org.
  18. [19] ↑ . The SEGUE stellar parameter pipeline. II. Validation with galactic globular and open clusters. wikidata.org.
  19. [20] ↑ . The SEGUE stellar parameter pipeline. II. Validation with galactic globular and open clusters. wikidata.org.
  20. [21] ↑ . The SEGUE stellar parameter pipeline. II. Validation with galactic globular and open clusters. wikidata.org.
  21. [22] ↑ . The SEGUE stellar parameter pipeline. II. Validation with galactic globular and open clusters. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. 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] ↑ . Exploring anticorrelations and light element variations in northern globular clusters observed by the APOGEE survey. 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). Q86183302. Retrieved May 7, 2026, from https://4ort.xyz/entity/q86183302
MLA “Q86183302.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q86183302.
BibTeX @misc{4ortxyz_q86183302_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q86183302}}, year = {2026}, url = {https://4ort.xyz/entity/q86183302}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q86183302 — https://4ort.xyz/entity/q86183302 (retrieved 2026-05-07)

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