The dark nebula predominant at the lower left of the above photograph is known as the Pipe Nebula. The dark clouds, suggestively shaped like smoke rising from a pipe, are caused by absorption of background starlight by dust [
http://antwrp.gsfc.
]. These dust clouds can be traced all the way to the Rho Ophiuchi nebular clouds [
http://antwrp.gsfc.
] on the right. The brightest star in the field is Antares [
http://antwrp.gsfc.
]. Many types of nebula are highlighted here: the red are emission nebula [
http://antwrp.gsfc.
], the blue are reflection nebula [
http://antwrp.gsfc.
], and the dark are absorption nebula [
http://antwrp.gsfc.
]. This picture has been digitally enhanced [
http://www.astropix
].
Explanation
The dark nebula predominant at the lower left of the above photograph is known as the Pipe Nebula. The dark clouds, suggestively shaped like smoke rising from a pipe, are caused by absorption of background starlight by dust [
http://antwrp.gsfc.
]. These dust clouds can be traced all the way to the Rho Ophiuchi nebular clouds [
http://antwrp.gsfc.
] on the right. The brightest star in the field is Antares [
http://antwrp.gsfc.
]. Many types of nebula are highlighted here: the red are emission nebula [
http://antwrp.gsfc.
], the blue are reflection nebula [
http://antwrp.gsfc.
], and the dark are absorption nebula [
http://antwrp.gsfc.
]. This picture has been digitally enhanced [
http://www.astropix
].
Explanation