NGC 5082

from Wikipedia, the free encyclopedia
Galaxy
NGC 5082
{{{Card text}}}
Photo-request.svg
AladinLite
Constellation centaur
Position
equinoxJ2000.0 , epoch : J2000.0
Right ascension 13 h 20 m 39.9 s
declination -43 ° 42 ′ 00 ″
Appearance
Morphological type SB (r) 0 ^ +  
Brightness  (visual) 12.8 mag
Brightness  (B-band) 13.8 mag
Angular expansion 1.5 ′ × 1.0 ′
Position angle 31 °
Surface brightness 13.1 mag / arcmin²
Physical data
Affiliation LGG 348  
Redshift 0.012996 ± 0.000140  
Radial velocity 3896 ± 42 km / s  
Stroke distance
v rad  / H 0
(167 ± 12)  ·  10 6  ly
(51.1 ± 3.6)  Mpc 
history
discovery John Herschel
Discovery date June 3, 1834
Catalog names
NGC  5082 • PGC  46566 • ESO  269-89 • MCG  -07-27-053 • SGC  131745-4326.4 • GC  3490 • h  3485 • LDCE 0916 NED158

NGC 5082 is a 12.8 mag bright, lens-shaped galaxy of the Hubble-type SB0 in the constellation Centaur in the southern sky . It is estimated to be 167 million light years from the Milky Way and about 80,000 light years in diameter.

The supernova SN 1958F was observed here.

The object was discovered on June 3, 1834 by John Herschel with an 18-inch reflector telescope, which "very faint, round; 20 arcseconds. The first of a group of four "noted. The other galaxies in this group are NGC 5086 , NGC 5090, and NGC 5091 .

Web links

Individual evidence

  1. a b c d e NASA / IPAC EXTRAGALACTIC DATABASE
  2. a b c d e SEDS : NGC 5082
  3. ^ VizieR
  4. Simbad
  5. Seligman
  6. Auke Slotegraaf: NGC 5082. Deep Sky Observer's Companion, accessed on May 27, 2015 (English).