NGC 675

from Wikipedia, the free encyclopedia
Galaxy
NGC 675
{{{Card text}}}
LEDA 1421664, NGC 677 & NGC 675 SDSS mount
LEDA 1421664 , NGC 677 & NGC 675 SDSS image
AladinLite
Constellation Aries
Position
equinoxJ2000.0 , epoch : J2000.0
Right ascension 01 h 49 m 08.6 s
declination + 13 ° 03 ′ 36 ″
Appearance
Morphological type S.  
Brightness  (visual) 14.4 mag
Brightness  (B-band) 14.3 mag
Angular expansion 1 ′ × 0.4 ′
Position angle 99 °
Surface brightness 13.3 mag / arcmin²
Physical data
Redshift 0.017796 ± 0.000100  
Radial velocity 5335 ± 30 km / s  
Stroke distance
v rad  / H 0
(242 ± 17)  x  10 6  ly
(74.2 ± 5.2)  Mpc 
history
discovery Lewis A. Swift
Discovery date September 25, 1886
Catalog names
NGC  675 • UGC  1273 • PGC  6665 • CGCG  437-037 • MCG  + 02-05-41 • IRAS  01464 + 1249 • 2MASX  J01490857 + 1303354 • GALEX ASC J014908.54 + 130335.8 • LDCE 107 NED015

NGC 675 is a spiral galaxy from the Hubble type S in the constellation ram on the ecliptic . It is estimated to be 242 million light years from the Milky Way and about 70,000 light years across.
In the same area of ​​the sky are u. a. the galaxies NGC 671 and NGC 677 .

The object was discovered on September 25, 1886 by the American astronomer Lewis A. Swift .

Web links

Individual evidence

  1. a b c d NASA / IPAC EXTRAGALACTIC DATABASE
  2. a b c d e f SEDS : NGC 675
  3. Seligman