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Q80495042

classical Cepheid variable star in the constellation Dorado
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Q80495042

Summary

Q80495042 is a classical Cepheid variable[1].

Key Facts

  • Q80495042's instance of is recorded as classical Cepheid variable[2].
  • Q80495042's constellation is recorded as Dorado[3].
  • Q80495042 is part of Large Magellanic Cloud[4].
  • Q80495042's catalog code is recorded as OGLE LMC-SC7 48548[5].
  • Q80495042's catalog code is recorded as OGLE J051756.59-692803.2[6].
  • Q80495042's catalog code is recorded as OGLE LMC-CEP-1516[7].
  • Q80495042's catalog code is recorded as OGLE LMC100.8 111795[8].
  • Q80495042's catalog code is recorded as Gaia DR2 4658184537046198656[9].
  • Q80495042's type of variable star is recorded as classical Cepheid variable[10].
  • Q80495042's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.275'}[11].
  • Q80495042's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.221'}[12].
  • Q80495042's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.568'}[13].
  • Q80495042's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.36'}[14].
  • Q80495042's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.000'}[15].
  • Q80495042's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.116'}[16].
  • Q80495042's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.8329'}[17].
  • Q80495042's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.4090'}[18].
  • Q80495042's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+225'}[19].
  • Q80495042's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+79.48539473407300'}[20].
  • Q80495042's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-69.46758044677920'}[21].
  • Q80495042's epoch is recorded as J2000.0[22].
  • Q80495042's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.623'}[23].
  • Q80495042's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+5.713'}[24].

Body

Definition and Type

Q80495042's instance of is recorded as classical Cepheid variable[2].

Use and Application

Q80495042 is part of Large Magellanic Cloud[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] ↑ . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. I. Classical Cepheids in the Large Magellanic Cloud. wikidata.org.
  10. [11] ↑ . The panchromatic view of the Magellanic Clouds from classical Cepheids. I. Distance, reddening, and geometry of the Large Magellanic Cloud disk. wikidata.org.
  11. [12] ↑ . The panchromatic view of the Magellanic Clouds from classical Cepheids. I. Distance, reddening, and geometry of the Large Magellanic Cloud disk. wikidata.org.
  12. [13] ↑ . The panchromatic view of the Magellanic Clouds from classical Cepheids. I. Distance, reddening, and geometry of the Large Magellanic Cloud disk. wikidata.org.
  13. [14] ↑ . The Optical Gravitanional Lensing Experiment. Catalog of RR Lyr stars in the Large Magellanic Cloud. wikidata.org.
  14. [15] ↑ . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. I. Classical Cepheids in the Large Magellanic Cloud. wikidata.org.
  15. [16] ↑ . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. I. Classical Cepheids in the Large Magellanic Cloud. wikidata.org.
  16. [17] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . Properties of RR Lyrae stars in the inner regions of the Large Magellanic Cloud. II. The extended sample. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. 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.

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). Q80495042. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80495042
MLA “Q80495042.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80495042.
BibTeX @misc{4ortxyz_q80495042_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80495042}}, year = {2026}, url = {https://4ort.xyz/entity/q80495042}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80495042 — https://4ort.xyz/entity/q80495042 (retrieved 2026-05-07)

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