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Q90188113

Mira variable star in the constellation Perseus
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Q90188113

Summary

Q90188113 is a Mira variable[1].

Key Facts

  • Q90188113's instance of is recorded as Mira variable[2].
  • Q90188113's instance of is recorded as emission-line star[3].
  • Q90188113's instance of is recorded as infrared source[4].
  • Q90188113's instance of is recorded as long-period variable star[5].
  • Q90188113's instance of is recorded as near-infrared source[6].
  • Q90188113's constellation is recorded as Perseus[7].
  • Q90188113's spectral class is recorded as M4[8].
  • Q90188113's catalog code is recorded as GCRV 53679[9].
  • Q90188113's catalog code is recorded as 2MASS J03030282+4816228[10].
  • Q90188113's catalog code is recorded as IRAS 02595+4804[11].
  • Q90188113's catalog code is recorded as Gaia DR2 436111911247769728[12].
  • Q90188113's catalog code is recorded as AM Per[13].
  • Q90188113's catalog code is recorded as TIC 116494652[14].
  • Q90188113's catalog code is recorded as Gaia DR3 436111911247769728[15].
  • Q90188113's type of variable star is recorded as Mira variable[16].
  • Q90188113's type of variable star is recorded as long-period variable star[17].
  • Q90188113's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.869'}[18].
  • Q90188113's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.940'}[19].
  • Q90188113's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.503'}[20].
  • Q90188113's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.858577'}[21].
  • Q90188113's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.92'}[22].
  • Q90188113's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2712'}[23].
  • Q90188113's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-38.46'}[24].
  • Q90188113's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+45.76178401527'}[25].
  • Q90188113's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.2730333634'}[26].

Body

Definition and Type

Recorded instance of include Mira variable[2], emission-line star[3], infrared source[4], long-period variable star[5], and near-infrared source[6].

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

  1. [2] ↑ . SIMBAD. wikidata.org.
  2. [3] ↑ . SIMBAD. wikidata.org.
  3. [4] ↑ . SIMBAD. wikidata.org.
  4. [5] ↑ . SIMBAD. wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . wikidata.org.
  7. [8] ↑ . Recognition of M-type stars in the unclassified spectra of LAMOST DR5 using a hash-learning method. wikidata.org.
  8. [9] ↑ . SIMBAD. wikidata.org.
  9. [10] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . SIMBAD. wikidata.org.
  12. [13] ↑ . SIMBAD. wikidata.org.
  13. [14] ↑ . SIMBAD. wikidata.org.
  14. [15] ↑ . SIMBAD. wikidata.org.
  15. [16] ↑ . General Catalogue of Variable Stars, 3rd ed.. wikidata.org.
  16. [17] ↑ . Long-period High-amplitude Red Variables in the KELT Survey. wikidata.org.
  17. [18] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  18. [19] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  19. [20] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  20. [21] ↑ . Gaia Early Data Release 3. wikidata.org.
  21. [22] ↑ . Long-period High-amplitude Red Variables in the KELT Survey. wikidata.org.
  22. [23] ↑ . Gaia Early Data Release 3. wikidata.org.
  23. [24] ↑ . Recognition of M-type stars in the unclassified spectra of LAMOST DR5 using a hash-learning method. wikidata.org.
  24. [25] ↑ . Gaia Early Data Release 3. wikidata.org.
  25. [26] ↑ . Gaia Early Data Release 3. 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). Q90188113. Retrieved May 7, 2026, from https://4ort.xyz/entity/q90188113
MLA “Q90188113.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q90188113.
BibTeX @misc{4ortxyz_q90188113_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q90188113}}, year = {2026}, url = {https://4ort.xyz/entity/q90188113}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q90188113 — https://4ort.xyz/entity/q90188113 (retrieved 2026-05-07)

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