NGC 3612

galaxy
Thing infrared_source Q1105596
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NGC 3612

Summary

NGC 3612 is an infrared source[1]. It has Wikipedia articles in 10 language editions, a strong signal of global cultural recognition.[2]

Key Facts

  • NGC 3612 is credited with the discovery of Otto Wilhelm von Struve[3].
  • NGC 3612's image is recorded as NGC3612 - SDSS DR14.jpg[4].
  • NGC 3612's instance of is recorded as infrared source[5].
  • NGC 3612's instance of is recorded as emission-line galaxy[6].
  • NGC 3612's instance of is recorded as spiral galaxy[7].
  • NGC 3612's constellation is recorded as Leo[8].
  • NGC 3612's galaxy morphological type is recorded as Scd[9].
  • NGC 3612's galaxy morphological type is recorded as S/I[10].
  • NGC 3612's part of is recorded as Coma Cluster[11].
  • NGC 3612's Commons category is recorded as NGC 3612[12].
  • NGC 3612's catalog code is recorded as NGC 3612[13].
  • NGC 3612's catalog code is recorded as 2MASX J11181468+2637143[14].
  • NGC 3612's catalog code is recorded as MCG+05-27-051[15].
  • NGC 3612's catalog code is recorded as UGC 6321[16].
  • NGC 3612's catalog code is recorded as PGC 34546[17].
  • NGC 3612's catalog code is recorded as Z 156-56[18].
  • NGC 3612's catalog code is recorded as Z 1115.6+2654[19].
  • NGC 3612's catalog code is recorded as UZC J111814.7+263714[20].
  • NGC 3612's catalog code is recorded as SDSS J111814.71+263714.0[21].
  • NGC 3612's catalog code is recorded as SDSS J111814.70+263713.9[22].
  • NGC 3612's catalog code is recorded as CAIRNS J111814.75+263714.1[23].
  • NGC 3612's catalog code is recorded as LEDA 34546[24].
  • NGC 3612's catalog code is recorded as 2MASS J11181468+2637143[25].
  • NGC 3612's time of discovery or invention is recorded as +1869-03-16T00:00:00Z[26].
  • NGC 3612's redshift is recorded as {'amount': '+0.02783'}[27].

Body

Works and Contributions

NGC 3612 is credited with the discovery of Otto Wilhelm von Struve[3].

Why It Matters

NGC 3612 has Wikipedia articles in 10 language editions, a strong signal of global cultural recognition.[2]

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

  1. [4] . wikidata.org.
  2. [5] . SIMBAD. wikidata.org.
  3. [6] . SIMBAD. wikidata.org.
  4. [7] . wikidata.org.
  5. [8] . VizieR. wikidata.org.
  6. [3] . wikidata.org.
  7. [9] . wikidata.org.
  8. [10] . SIMBAD. wikidata.org.
  9. [11] . SIMBAD. wikidata.org.
  10. [12] . wikidata.org.
  11. [13] . SIMBAD. wikidata.org.
  12. [14] . SIMBAD. wikidata.org.
  13. [15] . SIMBAD. wikidata.org.
  14. [16] . SIMBAD. wikidata.org.
  15. [17] . SIMBAD. wikidata.org.
  16. [18] . SIMBAD. wikidata.org.
  17. [19] . SIMBAD. wikidata.org.
  18. [20] . SIMBAD. wikidata.org.
  19. [21] . SIMBAD. wikidata.org.
  20. [22] . SIMBAD. wikidata.org.
  21. [23] . SIMBAD. wikidata.org.
  22. [24] . SIMBAD. wikidata.org.
  23. [25] . SIMBAD. wikidata.org.
  24. [26] . wikidata.org.
  25. [27] . The SDSS Photometric Catalog, Release 9. wikidata.org.

Class ancestry

  1. [1] . Wikidata. wikidata.org.

Aggregate / graph-position facts

  1. [2] . Wikidata sitelinks. 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). NGC 3612. Retrieved May 3, 2026, from https://4ort.xyz/entity/ngc-3612
MLA “NGC 3612.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/ngc-3612.
BibTeX @misc{4ortxyz_ngc-3612_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{NGC 3612}}, year = {2026}, url = {https://4ort.xyz/entity/ngc-3612}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): NGC 3612 — https://4ort.xyz/entity/ngc-3612 (retrieved 2026-05-03)

Canonical URL: https://4ort.xyz/entity/ngc-3612 · Last refreshed: