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EWS 2012-BLG-26

star in the constellation Ophiuchus
Place star Q88332185
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EWS 2012-BLG-26

Summary

EWS 2012-BLG-26 is a star[1].

Key Facts

  • EWS 2012-BLG-26's instance of is recorded as star[2].
  • EWS 2012-BLG-26's constellation is recorded as Ophiuchus[3].
  • EWS 2012-BLG-26's child astronomical body is recorded as OGLE-2012-BLG-0026Lc[4].
  • EWS 2012-BLG-26's child astronomical body is recorded as OGLE-2012-BLG-0026Lb[5].
  • EWS 2012-BLG-26's catalog code is recorded as Gaia DR2 4061372065008826496[6].
  • EWS 2012-BLG-26's catalog code is recorded as Gaia DR3 4061372065008826496[7].
  • EWS 2012-BLG-26's catalog code is recorded as OGLE-2012-BLG-0026[8].
  • EWS 2012-BLG-26's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.810604'}[9].
  • EWS 2012-BLG-26's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.82'}[10].
  • EWS 2012-BLG-26's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5773'}[11].
  • EWS 2012-BLG-26's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+132.2'}[12].
  • EWS 2012-BLG-26's metallicity is recorded as {'unit': '1', 'amount': '+0.50'}[13].
  • EWS 2012-BLG-26's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+4080'}[14].
  • EWS 2012-BLG-26's SIMBAD ID is recorded as OGLE-2012-BLG-0026[15].
  • EWS 2012-BLG-26's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+263.57791858754'}[16].
  • EWS 2012-BLG-26's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-27.14274086461'}[17].
  • EWS 2012-BLG-26's epoch is recorded as J2000.0[18].
  • EWS 2012-BLG-26's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4815'}[19].
  • EWS 2012-BLG-26's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+2500'}[20].
  • EWS 2012-BLG-26's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.213'}[21].
  • EWS 2012-BLG-26's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.848'}[22].
  • EWS 2012-BLG-26's Gaia ID is recorded as 4061372065008826496[23].

Body

Designation and Status

EWS 2012-BLG-26's instance of is recorded as star[2].

History and Context

Catalog codes include Gaia DR2 4061372065008826496[6], Gaia DR3 4061372065008826496[7], and OGLE-2012-BLG-0026[8].

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] ↑ . wikidata.org.
  5. [6] ↑ . SIMBAD. wikidata.org.
  6. [7] ↑ . SIMBAD. wikidata.org.
  7. [8] ↑ . SIMBAD. wikidata.org.
  8. [9] ↑ . Gaia Early Data Release 3. wikidata.org.
  9. [10] ↑ . Exponential growth of eccentricity in secular theory. wikidata.org.
  10. [11] ↑ . Gaia Early Data Release 3. wikidata.org.
  11. [12] ↑ . Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way. wikidata.org.
  12. [13] ↑ . Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way. wikidata.org.
  13. [14] ↑ . Exponential growth of eccentricity in secular theory. wikidata.org.
  14. [15] ↑ . wikidata.org.
  15. [16] ↑ . Gaia Early Data Release 3. wikidata.org.
  16. [17] ↑ . Gaia Early Data Release 3. wikidata.org.
  17. [18] ↑ . Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way. wikidata.org.
  18. [19] ↑ . Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way. wikidata.org.
  19. [20] ↑ . Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way. wikidata.org.
  20. [21] ↑ . Gaia Early Data Release 3. wikidata.org.
  21. [22] ↑ . Gaia Early Data Release 3. wikidata.org.
  22. [23] ↑ . 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). EWS 2012-BLG-26. Retrieved May 3, 2026, from https://4ort.xyz/entity/ews-2012-blg-26
MLA “EWS 2012-BLG-26.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/ews-2012-blg-26.
BibTeX @misc{4ortxyz_ews-2012-blg-26_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{EWS 2012-BLG-26}}, year = {2026}, url = {https://4ort.xyz/entity/ews-2012-blg-26}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): EWS 2012-BLG-26 — https://4ort.xyz/entity/ews-2012-blg-26 (retrieved 2026-05-03)

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