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Q93431402

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Q93431402

Summary

Q93431402 is a variable star[1].

Key Facts

  • Q93431402's instance of is recorded as variable star[2].
  • Q93431402's constellation is recorded as Sagittarius[3].
  • Q93431402 is part of Q1146456[4].
  • Q93431402's catalog code is recorded as 2MASS J18101766-3145393[5].
  • Q93431402's catalog code is recorded as Cl* NGC 6558 BZO F42[6].
  • Q93431402's catalog code is recorded as [TGB2011] J181017.6622-314539.473[7].
  • Q93431402's catalog code is recorded as [DHM99] BE1198[8].
  • Q93431402's catalog code is recorded as [DBS2015] NGC6558 8[9].
  • Q93431402's catalog code is recorded as Gaia DR2 4048864226831441920[10].
  • Q93431402's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.812'}[11].
  • Q93431402's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.442'}[12].
  • Q93431402's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.054'}[13].
  • Q93431402's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.049'}[14].
  • Q93431402's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9'}[15].
  • Q93431402's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8203'}[16].
  • Q93431402's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-187.89'}[17].
  • Q93431402's metallicity is recorded as {'unit': '1', 'amount': '-0.96'}[18].
  • Q93431402's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+272.57360705880210'}[19].
  • Q93431402's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-31.76092733634770'}[20].
  • Q93431402's epoch is recorded as J2000.0[21].
  • Q93431402's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+3565'}[22].
  • Q93431402's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+11'}[23].
  • Q93431402's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.118'}[24].
  • Q93431402's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.882'}[25].

Body

Definition and Type

Q93431402's instance of is recorded as variable star[2].

Use and Application

Q93431402 is part of Q1146456[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] ↑ . 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  11. [12] ↑ . NGC 6558: a blue horizontal branch moderately metal-poor globular cluster in the bulge. 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] ↑ . Proper motion and densification of the International Celestial Reference Frame in the direction of the Galactic bulge. wikidata.org.
  15. [16] ↑ . Gaia Data Release 2. wikidata.org.
  16. [17] ↑ . The GIRAFFE Inner Bulge Survey (GIBS). III. Metallicity distributions and kinematics of 26 Galactic bulge fields. wikidata.org.
  17. [18] ↑ . The GIRAFFE Inner Bulge Survey (GIBS). III. Metallicity distributions and kinematics of 26 Galactic bulge fields. 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] ↑ . FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. wikidata.org.
  22. [23] ↑ . FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . 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). Q93431402. Retrieved May 7, 2026, from https://4ort.xyz/entity/q93431402
MLA “Q93431402.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q93431402.
BibTeX @misc{4ortxyz_q93431402_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q93431402}}, year = {2026}, url = {https://4ort.xyz/entity/q93431402}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q93431402 — https://4ort.xyz/entity/q93431402 (retrieved 2026-05-07)

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