Q93322611

star in the constellation Piscis Austrinus
Thing star Q93322611
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Q93322611

Summary

Q93322611 is a star[1].

Key Facts

  • Q93322611's instance of is recorded as star[2].
  • Q93322611's constellation is recorded as Piscis Austrinus[3].
  • Q93322611's catalog code is recorded as TYC 6977-302-1[4].
  • Q93322611's catalog code is recorded as RAVE J230028.8-284922[5].
  • Q93322611's catalog code is recorded as 2MASS J23002885-2849227[6].
  • Q93322611's catalog code is recorded as Gaia DR2 6606531102868377856[7].
  • Q93322611's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.97'}[8].
  • Q93322611's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.08'}[9].
  • Q93322611's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.981'}[10].
  • Q93322611's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.516'}[11].
  • Q93322611's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.425'}[12].
  • Q93322611's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.4109'}[13].
  • Q93322611's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3290'}[14].
  • Q93322611's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-7.61'}[15].
  • Q93322611's metallicity is recorded as {'unit': '1', 'amount': '-1.58'}[16].
  • Q93322611's metallicity is recorded as {'unit': '1', 'amount': '-1.71'}[17].
  • Q93322611's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2457'}[18].
  • Q93322611's SIMBAD ID is recorded as TYC 6977-302-1[19].
  • Q93322611's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+345.12021743839770'}[20].
  • Q93322611's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-28.82301875238660'}[21].
  • Q93322611's epoch is recorded as J2000.0[22].
  • Q93322611's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4954'}[23].
  • Q93322611's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4828'}[24].
  • Q93322611's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+60'}[25].
  • Q93322611's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+15'}[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] . The Tycho-2 catalogue of the 2.5 million brightest stars. wikidata.org.
  8. [9] . The Tycho-2 catalogue of the 2.5 million brightest stars. wikidata.org.
  9. [10] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  10. [11] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  11. [12] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  12. [13] . Gaia Data Release 2. wikidata.org.
  13. [14] . Gaia Data Release 2. wikidata.org.
  14. [15] . Gaia Data Release 2. wikidata.org.
  15. [16] . 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.
  16. [17] . 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.
  17. [18] . Observational properties of the metal-poor thick disk of the Milky Way and insights into its origins. wikidata.org.
  18. [19] . wikidata.org.
  19. [20] . Gaia Data Release 2. wikidata.org.
  20. [21] . Gaia Data Release 2. wikidata.org.
  21. [22] . Gaia Data Release 2. wikidata.org.
  22. [23] . 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.
  23. [24] . 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.
  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.

📑 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). Q93322611. Retrieved May 7, 2026, from https://4ort.xyz/entity/q93322611
MLA “Q93322611.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q93322611.
BibTeX @misc{4ortxyz_q93322611_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q93322611}}, year = {2026}, url = {https://4ort.xyz/entity/q93322611}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q93322611 — https://4ort.xyz/entity/q93322611 (retrieved 2026-05-07)

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