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Q78378371

horizontal branch star in the constellation Canes Venatici
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Q78378371

Summary

Q78378371 is a horizontal branch star[1].

Key Facts

  • Q78378371's instance of is recorded as horizontal branch star[2].
  • Q78378371's constellation is recorded as Canes Venatici[3].
  • Q78378371's part of is recorded as Messier 3[4].
  • Q78378371's catalog code is recorded as Cl* NGC 5272 S 11007[5].
  • Q78378371's catalog code is recorded as Cl* NGC 5272 SK 21[6].
  • Q78378371's catalog code is recorded as Cl* NGC 5272 SAN 25[7].
  • Q78378371's catalog code is recorded as Cl* NGC 5272 KUST 949[8].
  • Q78378371's catalog code is recorded as NGC 5272 1401[9].
  • Q78378371's catalog code is recorded as 2MASS J13424333+2828158[10].
  • Q78378371's catalog code is recorded as [SLB2011b] 205.68053+28.47108[11].
  • Q78378371's catalog code is recorded as SDSS J134243.32+282815.8[12].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.60'}[13].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.65'}[14].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.096'}[15].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.129'}[16].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.816'}[17].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.722'}[18].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.475'}[19].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.572'}[20].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.657'}[21].
  • Q78378371's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.746'}[22].
  • Q78378371's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-128.8'}[23].
  • Q78378371's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-142.8'}[24].
  • Q78378371's metallicity is recorded as {'unit': '1', 'amount': '-1.37'}[25].
  • Q78378371's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q11929860', 'amount': '+9.8'}[26].

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] ↑ . SIMBAD. 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] ↑ . On the intrinsic widths of the subgiant and horizontal branch sequences in the globular cluster M 3. wikidata.org.
  13. [14] ↑ . On the intrinsic widths of the subgiant and horizontal branch sequences in the globular cluster M 3. 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 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] ↑ . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  22. [23] ↑ . Quantifying kinematic substructure in the Milky Way's stellar halo. 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] ↑ . Quantifying kinematic substructure in the Milky Way's stellar halo. 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). Q78378371. Retrieved May 7, 2026, from https://4ort.xyz/entity/q78378371
MLA “Q78378371.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q78378371.
BibTeX @misc{4ortxyz_q78378371_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q78378371}}, year = {2026}, url = {https://4ort.xyz/entity/q78378371}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q78378371 — https://4ort.xyz/entity/q78378371 (retrieved 2026-05-07)

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