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Q81792391

possible red giant branch star in the constellation Puppis
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Q81792391

Summary

Q81792391 is a possible red giant branch star[1].

Key Facts

  • Q81792391's instance of is recorded as possible red giant branch star[2].
  • Q81792391's constellation is recorded as Puppis[3].
  • Q81792391's part of is recorded as Q840003[4].
  • Q81792391's catalog code is recorded as 2MASS J07524183-3832129[5].
  • Q81792391's catalog code is recorded as Cl* NGC 2477 KVI 1019[6].
  • Q81792391's catalog code is recorded as Cl* NGC 2477 MMU 2061[7].
  • Q81792391's catalog code is recorded as Cl* NGC 2477 BSV 36385[8].
  • Q81792391's catalog code is recorded as Cl* NGC 2477 HART 2061[9].
  • Q81792391's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.3091'}[10].
  • Q81792391's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.714'}[11].
  • Q81792391's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.909'}[12].
  • Q81792391's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.382'}[13].
  • Q81792391's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.858'}[14].
  • Q81792391's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.747'}[15].
  • Q81792391's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6694'}[16].
  • Q81792391's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+8.926'}[17].
  • Q81792391's metallicity is recorded as {'unit': '1', 'amount': '+0.07'}[18].
  • Q81792391's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1493.88'}[19].
  • Q81792391's SIMBAD ID is recorded as Cl* NGC 2477 KVI 1019[20].
  • Q81792391's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+2.3'}[21].
  • Q81792391's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+118.17429398585709'}[22].
  • Q81792391's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-38.53693217832555'}[23].
  • Q81792391's epoch is recorded as J2000.0[24].
  • Q81792391's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5030'}[25].
  • Q81792391's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+500'}[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] ↑ . Gaia Data Release 2. wikidata.org.
  10. [11] ↑ . Red giants in open clusters. wikidata.org.
  11. [12] ↑ . Red giants in open clusters. 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] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. The catalogue of radial velocity standard stars. wikidata.org.
  17. [18] ↑ . Old open clusters as key tracers of Galactic chemical evolution. II. Iron and elemental abundances in NGC 2324, NGC 2477, NGC 2660, NGC 3960, and Berkeley 32. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. wikidata.org.
  19. [20] ↑ . wikidata.org.
  20. [21] ↑ . Rotational and radial velocities of 1.3-2.2 M_{sun}_ red giants in open clusters. 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] ↑ . Old open clusters as key tracers of Galactic chemical evolution. II. Iron and elemental abundances in NGC 2324, NGC 2477, NGC 2660, NGC 3960, and Berkeley 32. wikidata.org.
  25. [26] ↑ . Old open clusters as key tracers of Galactic chemical evolution. II. Iron and elemental abundances in NGC 2324, NGC 2477, NGC 2660, NGC 3960, and Berkeley 32. 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). Q81792391. Retrieved May 7, 2026, from https://4ort.xyz/entity/q81792391
MLA “Q81792391.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q81792391.
BibTeX @misc{4ortxyz_q81792391_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q81792391}}, year = {2026}, url = {https://4ort.xyz/entity/q81792391}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q81792391 — https://4ort.xyz/entity/q81792391 (retrieved 2026-05-07)

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