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Q86260212

star in the constellation Leo Minor
Thing star Q86260212
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Q86260212

Summary

Q86260212 is a star[1].

Key Facts

  • Q86260212's instance of is recorded as star[2].
  • Q86260212's constellation is recorded as Leo Minor[3].
  • Q86260212's spectral class is recorded as B[4].
  • Q86260212's catalog code is recorded as SDSS J102415.42+293145.2[5].
  • Q86260212's catalog code is recorded as [BGK2006] J102415.42+293145.2[6].
  • Q86260212's catalog code is recorded as SDSS J102415.42+293145.1[7].
  • Q86260212's catalog code is recorded as Gaia DR2 741517582439811968[8].
  • Q86260212's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.159'}[9].
  • Q86260212's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.44'}[10].
  • Q86260212's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.505'}[11].
  • Q86260212's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.749'}[12].
  • Q86260212's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.983'}[13].
  • Q86260212's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.6656'}[14].
  • Q86260212's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1296'}[15].
  • Q86260212's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+78'}[16].
  • Q86260212's metallicity is recorded as {'unit': '1', 'amount': '-0.75'}[17].
  • Q86260212's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q11929860', 'amount': '+52.7'}[18].
  • Q86260212's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+156.06426381731500'}[19].
  • Q86260212's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+29.52921558720820'}[20].
  • Q86260212's epoch is recorded as J2000.0[21].
  • Q86260212's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+9477'}[22].
  • Q86260212's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+31600'}[23].
  • Q86260212's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.980'}[24].
  • Q86260212's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.942'}[25].

Body

Definition and Type

Q86260212's instance of is recorded as star[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] ↑ . Hypervelocity Stars. III. The Space Density and Ejection History of Main‐Sequence Stars from the Galactic Center. 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 Sixth Data Release of the Sloan Digital Sky Survey. wikidata.org.
  9. [10] ↑ . The SDSS Photometric Catalog, Release 8. wikidata.org.
  10. [11] ↑ . The SDSS Photometric Catalog, Release 8. wikidata.org.
  11. [12] ↑ . The SDSS Photometric Catalog, Release 8. wikidata.org.
  12. [13] ↑ . The SDSS Photometric Catalog, Release 8. wikidata.org.
  13. [14] ↑ . Gaia Data Release 2. wikidata.org.
  14. [15] ↑ . Gaia Data Release 2. wikidata.org.
  15. [16] ↑ . The SDSS Photometric Catalog, Release 8. wikidata.org.
  16. [17] ↑ . The Milky Way's circular velocity curve to 60 kpc and an estimate of the dark matter halo mass from the kinematics of ~2400 SDSS blue horizontal-branch stars. wikidata.org.
  17. [18] ↑ . The Milky Way's circular velocity curve to 60 kpc and an estimate of the dark matter halo mass from the kinematics of ~2400 SDSS blue horizontal-branch stars. 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] ↑ . The Milky Way's circular velocity curve to 60 kpc and an estimate of the dark matter halo mass from the kinematics of ~2400 SDSS blue horizontal-branch stars. wikidata.org.
  22. [23] ↑ . The Milky Way's circular velocity curve to 60 kpc and an estimate of the dark matter halo mass from the kinematics of ~2400 SDSS blue horizontal-branch stars. 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). Q86260212. Retrieved May 7, 2026, from https://4ort.xyz/entity/q86260212
MLA “Q86260212.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q86260212.
BibTeX @misc{4ortxyz_q86260212_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q86260212}}, year = {2026}, url = {https://4ort.xyz/entity/q86260212}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q86260212 — https://4ort.xyz/entity/q86260212 (retrieved 2026-05-07)

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