Astronomy:NGC 3596
From HandWiki
| NGC 3596 | |
|---|---|
NGC 3596 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 15m 06.2152s[1] |
| Declination | +14° 47′ 13.404″[1] |
| Redshift | 0.003979±0.000002[1] |
| Helio radial velocity | 1,193±1 km/s[1] |
| Distance | 57.24 ± 6.82 Mly (17.550 ± 2.092 Mpc)[1] |
| Apparent magnitude (V) | 12.0[1] |
| Characteristics | |
| Type | SAB(rs)c[1] |
| Size | ~74,900 ly (22.97 kpc) (estimated)[1] |
| Apparent size (V) | 4.0′ × 3.8′[1] |
| Other designations | |
| UGC 6277, MCG+03-29-013, PGC 34298[1] | |
NGC 3596 is an intermediate spiral galaxy in the constellation Leo. It was discovered by German-British astronomer William Herschel on 8 April 1784.[2] It is located below the star Theta Leonis (Chertan).[3] It is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.[4]
Image Gallery
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SDSS image of NGC 3596
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Legacy Surveys image of NGC 3596
See also
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 "Results for object NGC 3596". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=NGC+3596.
- ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 6261". https://cseligman.com/text/atlas/ngc35a.htm#3596.
- ↑ "WikiSky DSS2 image of Chertan and NGC 3596". Wikisky. http://www.wikisky.org/?ra=11.235231682744185&de=15.122766246792818&zoom=8&show_grid=1&show_constellation_lines=1&show_constellation_boundaries=1&show_const_names=0&show_galaxies=1&show_box=1&box_ra=11.237333&box_de=15.429444&box_width=50&box_height=50&img_source=DSS2.
- ↑ "The Leo III Groups". Atlas of the Universe. http://www.atlasoftheuniverse.com/galgrps/leoii.html.
External links
- Galaxy NGC 3596
- NGC 3596 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Coordinates:
11h 15m 06.2152s, +14° 47′ 13.404″
