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Q81424077

spectroscopic binary in the constellation Monoceros
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Q81424077

Summary

Q81424077 is a spectroscopic binary[1].

Key Facts

  • Q81424077's instance of is recorded as spectroscopic binary[2].
  • Q81424077's constellation is recorded as Monoceros[3].
  • Q81424077 is part of NGC 2324[4].
  • Q81424077's catalog code is recorded as 2MASS J07040821+0105184[5].
  • Q81424077's catalog code is recorded as Cl* NGC 2324 MMU 1006[6].
  • Q81424077's catalog code is recorded as Cl* NGC 2324 BSV 10797[7].
  • Q81424077's catalog code is recorded as Cl* NGC 2324 BSF 79[8].
  • Q81424077's catalog code is recorded as Cl* NGC 2324 PCA 1-1006[9].
  • Q81424077's catalog code is recorded as NGC 2324 91[10].
  • Q81424077's catalog code is recorded as SBC9 2887[11].
  • Q81424077's catalog code is recorded as Gaia DR2 3114600336198020096[12].
  • Q81424077's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.294'}[13].
  • Q81424077's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.766'}[14].
  • Q81424077's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.633'}[15].
  • Q81424077's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.312'}[16].
  • Q81424077's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.291'}[17].
  • Q81424077's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.144'}[18].
  • Q81424077's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.9662'}[19].
  • Q81424077's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2693'}[20].
  • Q81424077's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+33.87'}[21].
  • Q81424077's metallicity is recorded as {'unit': '1', 'amount': '-0.17'}[22].
  • Q81424077's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+106.03426177407090'}[23].
  • Q81424077's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+1.08845628628140'}[24].
  • Q81424077's epoch is recorded as J2000.0[25].
  • Q81424077's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5040'}[26].

Body

Definition and Type

Q81424077's instance of is recorded as spectroscopic binary[2].

Use and Application

Q81424077 is part of NGC 2324[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] ↑ . 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] ↑ . 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] ↑ . 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.
  16. [17] ↑ . 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.
  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] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . 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.
  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] ↑ . 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). Q81424077. Retrieved May 7, 2026, from https://4ort.xyz/entity/q81424077
MLA “Q81424077.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q81424077.
BibTeX @misc{4ortxyz_q81424077_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q81424077}}, year = {2026}, url = {https://4ort.xyz/entity/q81424077}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q81424077 — https://4ort.xyz/entity/q81424077 (retrieved 2026-05-07)

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