This is an 16.5 minute exposure with
an ST-9E CCD camera thru Kopernik's 20-inch F/8.1 Ritchey Chretien Cassegrain
telescope taken on September 19, 2004 at 4:00 UT. The field of view is
9x9 arc minutes with North at the top.
NGC 799 and NGC 800 are a close pair of Spiral Galaxies in the Constellation of Cetus. They have nearly identical red shifts and therefore they are probably very close to each other. NGC 799 has a small bright nucleus and a short bar that appears to be the location of Supernova 2004dt. There are two very dim and broad spiral arms that start at the ends of the bar and wrap nearly completely around this galaxy forming a pseudo outer ring. NGC 800 has a bright nucleus and three bright knotty arms.
The Sloan Digital Sky Survey has tentatively identified the 20th magnitude star-like object labeled 'QSO' in our image as a very distant Quasar: SDSS J020202.64-001009.2. They conclude that this object has a red shift of roughly 2.89. After adjusting for the effects of Relativity, this implies that this Quasar is receding from us that the astounding speed of 88% of the speed of light, and a distance of 14 billion light years.
Classification: (R')SB(s)a: Dreyer description in the NGC: |
Classification: : SA(rs)c: Dreyer description in the NGC:
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George Normandin, KAS
September 22nd, 2004