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Q89123674

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Q89123674

Summary

Q89123674 is a red supergiant[1].

Key Facts

  • Q89123674's instance of is recorded as red supergiant[2].
  • Q89123674's constellation is recorded as Tucana[3].
  • Q89123674's spectral class is recorded as O-rich[4].
  • Q89123674's catalog code is recorded as 2MASS J00533939-7252392[5].
  • Q89123674's catalog code is recorded as SV* HV 11329[6].
  • Q89123674's catalog code is recorded as OGLE SMC-LPV-10459[7].
  • Q89123674's catalog code is recorded as EV* SMC V1022[8].
  • Q89123674's catalog code is recorded as SSTISAGEMA J005339.39-725239.2[9].
  • Q89123674's catalog code is recorded as [GDN2015] SMC250[10].
  • Q89123674's catalog code is recorded as Gaia DR2 4685955696790971264[11].
  • Q89123674's type of variable star is recorded as semiregular variable star[12].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.911'}[13].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.987'}[14].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.647'}[15].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.09'}[16].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.42'}[17].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.01'}[18].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.49'}[19].
  • Q89123674's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9648'}[20].
  • Q89123674's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+140.3'}[21].
  • Q89123674's metallicity is recorded as {'unit': '1', 'amount': '-0.37'}[22].
  • Q89123674's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+13.41419691790030'}[23].
  • Q89123674's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-72.87756888076700'}[24].
  • Q89123674's epoch is recorded as J2000.0[25].
  • Q89123674's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+3600'}[26].

Body

Definition and Type

Q89123674's instance of is recorded as red supergiant[2].

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] ↑ . Spitzerinfrared spectrograph point source classification in the Small Magellanic Cloud. 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] ↑ . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XIII. Long-period variables in the Small Magellanic Cloud. 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] ↑ . Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. wikidata.org.
  16. [17] ↑ . Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. wikidata.org.
  17. [18] ↑ . Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. wikidata.org.
  18. [19] ↑ . Surveying the agents of galaxy evolution in the tidally stripped, low metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool evolved stars. wikidata.org.
  19. [20] ↑ . Gaia Data Release 2. wikidata.org.
  20. [21] ↑ . A new survey of cool supergiants in the Magellanic Clouds. wikidata.org.
  21. [22] ↑ . Lithium abundances and other clues to envelope burning in Small Magellanic Cloud asymptotic giant branch stars. 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] ↑ . Lithium abundances and other clues to envelope burning in Small Magellanic Cloud asymptotic giant branch stars. 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). Q89123674. Retrieved May 7, 2026, from https://4ort.xyz/entity/q89123674
MLA “Q89123674.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q89123674.
BibTeX @misc{4ortxyz_q89123674_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q89123674}}, year = {2026}, url = {https://4ort.xyz/entity/q89123674}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q89123674 — https://4ort.xyz/entity/q89123674 (retrieved 2026-05-07)

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