Posts Tagged ‘ED80’
M65 and M66 Imaged by Chris Thayer
M65 (NGC 3623) and M66 (NGC 3627) are two of the galaxies that make up the Leo Triplet (also known as the M66 Group of Galaxies). As its name suggests the Leo Triplet can be found in the constellation of Leo. Charles Messier is generally assumed to have discovered these galaxies but it is possible...
May 14th, 2010 | Chris Thayer, Featured Articles | Read More Pelican Nebula Imaged by Chris Thayer
The Pelican Nebula (also known as IC5070) is a large emission nebula in the constellation Cygnus. It is separated from its larger neighbour, the North America Nebula, by a molecular cloud filled with dark dust.Pelican Nebula – click to enlarge
Imaged using an ED80 and DSI3mono. 9 x 5.5...
October 14th, 2009 | Chris Thayer | Read More Swan Nebula (M17) Imaged by Chris Thayer
M17, the Swan Nebula (also designated NGC 6618) is an emission nebula (HII region) in the constellation of Sagittarius. The radiation of a cluster of stars embedded in nebula is exciting the gass and causing the emission. It is roughly 40 light years in diameter and is over 5,000 ly away. ...
September 23rd, 2009 | Chris Thayer | Read More M81 and M82 Imaged by John Moore
M81 and M82 - click to enlarge
September 5th, 2009 | John Moore | Read More Elephant’s Trunk Nebula (IC1396) Imaged by Chris Thayer
IC 1396 is an emission nebula in the constellation of Cephus. It is a mix of gas and dust clouds; the gas is energised by a bright, central star. This region spannsing over three degrees on the sky and yet is nearly 3,000 light-years away. The winding Elephant’s Trunk nebula seen here is only...
August 28th, 2009 | Chris Thayer | Read More M42 Imaged by Chris Thayer
The Orion Nebula, M42 (also designated NGC 1976) is a diffuse nebula (an HII region) situated south of Orion’s Belt and is one of the brightest nebulae, and is visible to the naked eye. It is approximately1,344±20 light years away and is the closest region of massive star formation to...
August 24th, 2009 | Chris Thayer | Read More Crescent Nebula Imaged by Chris Thayer
The Crescent Nebula (also designated NGC 6888 and Caldwell 27 on Patrick Moore’s Caldwell catalogue) is an emission nebula in the constellation of Cygnus. It was formed by fast stellar winds from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind (ejected by...
August 24th, 2009 | Chris Thayer | Read More The Eagle Nebula (M16) Imaged by Chris Thayer
The Eagle Nebula, M16 is a region of star formation in the constellation Serpens – it has already created an open cluster of stars (the cluster is designated NGC 6611 and the nebula is IC 4703). It was discovered by Jean-Philippe de Cheseaux in 1745-4.
The Eagle Nebula features in one of...
August 23rd, 2009 | Chris Thayer | Read More M42 Imaged by Peter Campbell-Burns
The Orion Nebula (also designated Messier 42, M42, or NGC 1976) is a diffuse nebula situated south of Orion’s Belt and is one of the brightest nebulae, and is visible to the naked eye. It is approximately1,344±20 light years away and is the closest region of massive star formation to Earth. It...
August 13th, 2009 | Peter Campbell-Burns | Read More Veil Nebula Imaged by Peter Campbell-Burns
The Veil Nebula, also known as the Cygnus Loop or the Witch’s Broom Nebula, is a large, relatively faint supernova remnant in the constellation Cygnus. The source supernova exploded some 5,000 to 8,000 years ago, and the remnants have since expanded to cover an area of ~3×3 degrees; about...
August 13th, 2009 | Peter Campbell-Burns | Read More 



