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Q87992042

high proper-motion star in the constellation Cetus
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Q87992042

Summary

Q87992042 is a high proper-motion star[1].

Key Facts

  • Q87992042's instance of is recorded as high proper-motion star[2].
  • Q87992042's constellation is recorded as Cetus[3].
  • Q87992042's catalog code is recorded as BD-16 179[4].
  • Q87992042's catalog code is recorded as G 268-118[5].
  • Q87992042's catalog code is recorded as NLTT 3698[6].
  • Q87992042's catalog code is recorded as PPM 209750[7].
  • Q87992042's catalog code is recorded as TYC 5851-2090-1[8].
  • Q87992042's catalog code is recorded as 2MASS J01070029-1602239[9].
  • Q87992042's catalog code is recorded as RAVE J010700.3-160223[10].
  • Q87992042's catalog code is recorded as RAVE J010700.3-160224[11].
  • Q87992042's catalog code is recorded as Gaia DR1 2359449732986083200[12].
  • Q87992042's catalog code is recorded as Gaia DR2 2359449737281529984[13].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.843'}[14].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.516'}[15].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.458'}[16].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.542'}[17].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.994'}[18].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.209'}[19].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.837'}[20].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.702'}[21].
  • Q87992042's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.8324'}[22].
  • Q87992042's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.3579'}[23].
  • Q87992042's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-38.01'}[24].
  • Q87992042's metallicity is recorded as {'unit': '1', 'amount': '-0.94'}[25].
  • Q87992042's metallicity is recorded as {'unit': '1', 'amount': '-0.95'}[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] ↑ . SIMBAD. wikidata.org.
  9. [10] ↑ . SIMBAD. wikidata.org.
  10. [11] ↑ . SIMBAD. wikidata.org.
  11. [12] ↑ . SIMBAD. wikidata.org.
  12. [13] ↑ . SIMBAD. 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  16. [17] ↑ . APASS Landolt-Sloan BVgri photometry of RAVE stars. I. Data, effective temperatures, and reddenings. wikidata.org.
  17. [18] ↑ . APASS Landolt-Sloan BVgri photometry of RAVE stars. I. Data, effective temperatures, and reddenings. wikidata.org.
  18. [19] ↑ . APASS Landolt-Sloan BVgri photometry of RAVE stars. I. Data, effective temperatures, and reddenings. wikidata.org.
  19. [20] ↑ . APASS Landolt-Sloan BVgri photometry of RAVE stars. I. Data, effective temperatures, and reddenings. wikidata.org.
  20. [21] ↑ . APASS Landolt-Sloan BVgri photometry of RAVE stars. I. Data, effective temperatures, and reddenings. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . Gaia Data Release 2. wikidata.org.
  24. [25] ↑ . Unveiling systematic biases in the 1D LTE excitation-ionization balance of Fe for FGK stars: a novel approach to determination of stellar parameters. wikidata.org.
  25. [26] ↑ . Unveiling systematic biases in the 1D LTE excitation-ionization balance of Fe for FGK stars: a novel approach to determination of stellar parameters. wikidata.org.

Class ancestry

  1. [1] ↑ . Wikidata. wikidata.org.

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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). Q87992042. Retrieved May 7, 2026, from https://4ort.xyz/entity/q87992042
MLA “Q87992042.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q87992042.
BibTeX @misc{4ortxyz_q87992042_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q87992042}}, year = {2026}, url = {https://4ort.xyz/entity/q87992042}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q87992042 — https://4ort.xyz/entity/q87992042 (retrieved 2026-05-07)

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