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Q89076018

long period variable
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Q89076018

Summary

Q89076018 is a long-period variable star[1].

Key Facts

  • Q89076018's instance of is recorded as long-period variable star[2].
  • Q89076018's constellation is recorded as Tucana[3].
  • Q89076018's catalog code is recorded as OGLE SMC-LPV-10151[4].
  • Q89076018's catalog code is recorded as SSTISAGEMA J005311.43-740621.1[5].
  • Q89076018's catalog code is recorded as 2MASS J00531142-7406212[6].
  • Q89076018's catalog code is recorded as SSTISAGEMC J005311.43-740621.1[7].
  • Q89076018's catalog code is recorded as Gaia DR2 4685599317529706880[8].
  • Q89076018's type of variable star is recorded as semiregular variable star[9].
  • Q89076018's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.99'}[10].
  • Q89076018's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.06'}[11].
  • Q89076018's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.64'}[12].
  • Q89076018's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.494'}[13].
  • Q89076018's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.309'}[14].
  • Q89076018's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.857'}[15].
  • Q89076018's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.4310'}[16].
  • Q89076018's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0118'}[17].
  • Q89076018's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+215.3'}[18].
  • Q89076018's metallicity is recorded as {'unit': '1', 'amount': '-0.58'}[19].
  • Q89076018's SIMBAD ID is recorded as OGLE SMC-LPV-10151[20].
  • Q89076018's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+13.29758587771970'}[21].
  • Q89076018's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-74.10589207365190'}[22].
  • Q89076018's epoch is recorded as J2000.0[23].
  • Q89076018's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4209'}[24].
  • Q89076018's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.287'}[25].
  • Q89076018's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.568'}[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] ↑ . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XIII. Long-period variables in the Small Magellanic Cloud. wikidata.org.
  9. [10] ↑ . Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. wikidata.org.
  10. [11] ↑ . Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. wikidata.org.
  11. [12] ↑ . Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. 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. wikidata.org.
  17. [18] ↑ . Optically visible post-AGB/RGB stars and young stellar objects in the Small Magellanic Cloud: candidate selection, spectral energy distributions and spectroscopic examination. wikidata.org.
  18. [19] ↑ . Optically visible post-AGB/RGB stars and young stellar objects in the Small Magellanic Cloud: candidate selection, spectral energy distributions and spectroscopic examination. wikidata.org.
  19. [20] ↑ . 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] ↑ . Optically visible post-AGB/RGB stars and young stellar objects in the Small Magellanic Cloud: candidate selection, spectral energy distributions and spectroscopic examination. wikidata.org.
  24. [25] ↑ . Gaia Data Release 2. wikidata.org.
  25. [26] ↑ . 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). Q89076018. Retrieved May 7, 2026, from https://4ort.xyz/entity/q89076018
MLA “Q89076018.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q89076018.
BibTeX @misc{4ortxyz_q89076018_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q89076018}}, year = {2026}, url = {https://4ort.xyz/entity/q89076018}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q89076018 — https://4ort.xyz/entity/q89076018 (retrieved 2026-05-07)

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