Q76843492

Thing t_tauri_type_star Q76843492
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Q76843492

Summary

Q76843492 is a T Tauri-type star[1].

Key Facts

  • Q76843492's instance of is recorded as T Tauri-type star[2].
  • Q76843492's constellation is recorded as Cepheus[3].
  • Q76843492's spectral class is recorded as K6.5[4].
  • Q76843492's catalog code is recorded as [SHB2004] Trumpler 37 91-506[5].
  • Q76843492's catalog code is recorded as 2MASS J21385807+5743343[6].
  • Q76843492's catalog code is recorded as IPHAS J213858.08+574334.4[7].
  • Q76843492's catalog code is recorded as [BVD2011] 77[8].
  • Q76843492's catalog code is recorded as [NSW2012] 298[9].
  • Q76843492's catalog code is recorded as Gaia DR2 2178404633705020544[10].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.39'}[11].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.52'}[12].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.040'}[13].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.777'}[14].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.141'}[15].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.732'}[16].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.546'}[17].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.26'}[18].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.14'}[19].
  • Q76843492's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.9883'}[20].
  • Q76843492's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0117'}[21].
  • Q76843492's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-15.8'}[22].
  • Q76843492's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+988.4353'}[23].
  • Q76843492's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+8.4'}[24].
  • Q76843492's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+324.74199599313660'}[25].
  • Q76843492's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+57.72622785764970'}[26].

Body

Definition and Type

Q76843492's instance of is recorded as T Tauri-type 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] . High-Resolution Spectroscopy in Tr 37: Gas Accretion Evolution in Evolved Dusty Disks. 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] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  12. [13] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  13. [14] . Accretion in evolved and transitional disks in Cep OB2: looking for the origin of the inner holes. wikidata.org.
  14. [15] . Accretion in evolved and transitional disks in Cep OB2: looking for the origin of the inner holes. wikidata.org.
  15. [16] . Accretion in evolved and transitional disks in Cep OB2: looking for the origin of the inner holes. wikidata.org.
  16. [17] . Accretion in evolved and transitional disks in Cep OB2: looking for the origin of the inner holes. wikidata.org.
  17. [18] . T Tauri candidates and accretion rates using IPHAS: method and application to IC 1396. wikidata.org.
  18. [19] . T Tauri candidates and accretion rates using IPHAS: method and application to IC 1396. wikidata.org.
  19. [20] . Gaia Data Release 2. wikidata.org.
  20. [21] . Gaia Data Release 2. wikidata.org.
  21. [22] . High-Resolution Spectroscopy in Tr 37: Gas Accretion Evolution in Evolved Dusty Disks. wikidata.org.
  22. [23] . Gaia Data Release 2. wikidata.org.
  23. [24] . High-Resolution Spectroscopy in Tr 37: Gas Accretion Evolution in Evolved Dusty Disks. wikidata.org.
  24. [25] . Gaia Data Release 2. wikidata.org.
  25. [26] . 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). Q76843492. Retrieved May 7, 2026, from https://4ort.xyz/entity/q76843492
MLA “Q76843492.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q76843492.
BibTeX @misc{4ortxyz_q76843492_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q76843492}}, year = {2026}, url = {https://4ort.xyz/entity/q76843492}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q76843492 — https://4ort.xyz/entity/q76843492 (retrieved 2026-05-07)

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