NGC 1705

from Wikipedia, the free encyclopedia
Galaxy
NGC 1705
{{{Card text}}}
NGC 1705 [1] Hubble Space Telescope
NGC 1705 Hubble Space Telescope
AladinLite
Constellation painter
Position
equinoxJ2000.0 , epoch : J2000.0
Right ascension 04 h 54 m 13.50 s
declination -53 ° 21 ′ 39.8 ″
Appearance
Morphological type SA0- / HII / BCDG  
Brightness  (visual) 11.8 mag
Brightness  (B-band) 12.8 mag
Angular expansion 1.9 ′ × 1.4 ′
Position angle 50 °
Surface brightness 12.9 mag / arcmin²
Physical data
Affiliation isolated  
Redshift 0.002112 ± 0.000019  
Radial velocity 633 ± 6 km / s  
Stroke distance
v rad  / H 0
(20 ± 1)  x  10 6  ly
(6.15 ± 0.45)  Mpc 
diameter 2000 ly
history
discovery John Herschel
Discovery date December 5, 1834
Catalog names
NGC  1705 • PGC  16282 • ESO  158-013 • IRAS  04531-5326 • 2MASX  J04541350-5321398 • SGC  045306-5326.5 • GC  937 • h  2679 • GALEX ASC J045413.62-532138.3 • HIPASS  J0454-53 • 2MIG 638

NGC 1705 is an elliptical dwarf galaxy with extensive star formation regions of the Hubble type E / S0 in the constellation Painter in the southern sky . It is an estimated 28 million light years from the Milky Way and about 15,000 light years across .

In the center of the galaxy is a huge star cluster , which probably formed during a phase of violent star formation, a so-called starburst , about 26 to 31 million years ago. NGC 1705 is particularly suitable as a study object , since some astronomers suspect that dwarf galaxies were among the first star clusters in the early universe .

The object was discovered on December 5, 1834 by the British astronomer John Herschel .

Web links

Individual evidence

  1. ^ Aladin Lite
  2. a b c d e f NASA / IPAC EXTRAGALACTIC DATABASE
  3. a b c d e SEDS : NGC 1705
  4. Seligman