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Q91099406

red giant branch star in the constellation Sagitta
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Q91099406

Summary

Q91099406 is a red giant branch star[1].

Key Facts

  • Q91099406's instance of is recorded as red giant branch star[2].
  • Q91099406's constellation is recorded as Sagitta[3].
  • Q91099406 is part of Messier 71[4].
  • Q91099406's catalog code is recorded as Cl* NGC 6838 AH C[5].
  • Q91099406's catalog code is recorded as GEN# +2.68380171[6].
  • Q91099406's catalog code is recorded as UBV M 37365[7].
  • Q91099406's catalog code is recorded as [CBG2009] NGC 6838 508232[8].
  • Q91099406's catalog code is recorded as 2MASS J19534854+1844491[9].
  • Q91099406's catalog code is recorded as [DBS2015] M71 15[10].
  • Q91099406's catalog code is recorded as Gaia DR2 1821608334516635648[11].
  • Q91099406's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.65'}[12].
  • Q91099406's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.60'}[13].
  • Q91099406's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.32'}[14].
  • Q91099406's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.73'}[15].
  • Q91099406's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.580'}[16].
  • Q91099406's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.371'}[17].
  • Q91099406's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1829'}[18].
  • Q91099406's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4622'}[19].
  • Q91099406's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-41.62'}[20].
  • Q91099406's metallicity is recorded as {'unit': '1', 'amount': '-0.54'}[21].
  • Q91099406's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2163.5656'}[22].
  • Q91099406's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+298.45228147409090'}[23].
  • Q91099406's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+18.74698576533040'}[24].
  • Q91099406's epoch is recorded as J2000.0[25].
  • Q91099406's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5025'}[26].

Body

Definition and Type

Q91099406's instance of is recorded as red giant branch star[2].

Use and Application

Q91099406 is part of Messier 71[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] ↑ . 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  15. [16] ↑ . FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. wikidata.org.
  16. [17] ↑ . FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. wikidata.org.
  20. [21] ↑ . FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . Gaia Data Release 2. wikidata.org.
  25. [26] ↑ . FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. 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). Q91099406. Retrieved May 7, 2026, from https://4ort.xyz/entity/q91099406
MLA “Q91099406.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q91099406.
BibTeX @misc{4ortxyz_q91099406_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q91099406}}, year = {2026}, url = {https://4ort.xyz/entity/q91099406}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q91099406 — https://4ort.xyz/entity/q91099406 (retrieved 2026-05-07)

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