Best Molecular Cloud
Orion Molecular Cloud 1 is a substantial molecular cloud situated in the Orion constellation. It’s notable as an active star-forming region containing the dense Kleinmann-Low core and the Trapezium cluster of young stars. This nearby nebula provides valuable insights into stellar birth processes and...
The Shark Nebula, designated LDN 1235, is a dark molecular cloud located in the constellation Cepheus. It appears as a silhouette against the background star field, with a shape that resembles a shark, hence its common name. The nebula is included in the Lynds Catalogue of Dark Nebulae, a compilatio...
The Le Gentil 3 nebula resides within the Cygnus constellation a vast dark nebula composed of interstellar dust and gas. It’s notable as one of the largest identified dark nebulae in the Milky Way. Astronomers and researchers studying star formation and the distribution of molecular clouds utilize t...
The Musca Dark Cloud, also known as Musca 1, is a molecular cloud located in the southern constellation Musca. It is notable for its elongated, thread-like morphology, which has made it a subject of study regarding magnetic field structures in star-forming regions. The cloud is a site of ongoing low...
The Aquila Rift is a prominent molecular cloud complex situated in the Milky Way galaxy, located approximately 600 light-years from Earth. It consists of a dense band of cosmic dust and gas that actively obscures the light from background stars, creating a massive, dark rift observable in the night...
The Serpens Molecular Cloud is a nearby star-forming region in the Serpens Cauda constellation, notable for hosting highly active protostellar clusters like Serpens South.
Orion Molecular Cloud 2 (OMC-2) is a dense star-forming region located within the integral-shaped filament of the greater Orion A molecular cloud. Situated roughly 1,500 light-years from Earth, it is recognized by astronomers for hosting one of the richest and most densely packed clusters of protost...
The Lupus Molecular Cloud is a star-forming complex in the Lupus constellation, extensively studied for its dense cores and newly forming low-mass stars.
The Iris Nebula (NGC 7023) is a bright reflection nebula located approximately 1,300 light-years from Earth in the constellation Cepheus. It is illuminated by the hot young star HD 200775, with the star's light reflecting off surrounding dust grains to create the nebula's distinctive blue coloration...
Orion Molecular Cloud 3 (OMC-3) is a dense region within the Orion A molecular cloud complex, part of the integral-shaped filament extending through the constellation Orion. Located approximately 1,344 light-years from Earth, this star-forming region was extensively studied through 850-micron polari...
The Taurus Molecular Cloud is a massive interstellar cloud and star-forming region situated in the constellations Taurus and Auriga. Located approximately 140 parsecs from Earth, it is one of the closest active stellar nurseries to the solar system. The complex contains numerous dense cores, includi...
The Snake Nebula, catalogued as Barnard 72, is a dark nebula in the constellation Ophiuchus that appears as a distinctive S-shaped lane of opaque interstellar dust, silhouetted against the dense background star field of the Milky Way. It was catalogued by astronomer Edward Emerson Barnard in his pho...
The Baby Eagle Nebula is a faint reflection nebula within the Taurus molecular cloud, named for its striking resemblance to a small flying eagle silhouette.
The Perseus Molecular Cloud is a massive, nearby stellar nursery located in the constellation of Perseus, approximately 600 light-years from Earth. It is a highly active star-forming region, distinguished by its dense interstellar dust and gas. The cloud is most notable for harboring the young, embe...
The Lupus I Cloud is a dark molecular cloud in the Lupus complex, notable for an ongoing star-forming event mapped by Herschel in 2012.
The Corona Australis Molecular Cloud is a dark nebula in the southern sky, notable for being one of the closest and most active star-forming regions to our Solar System.
The Chamaeleon II Cloud is a dark cloud in the Chamaeleon complex, notable for ALMA detections of 22 disks around young stars.
The Chamaeleon I Cloud is a dark nebula in the Chamaeleon constellation, distinguished as one of the closest and most active star-forming regions to our own Solar System.
Sandqvist 150 is a dark molecular cloud cataloged by Aage Sandqvist during his pioneering 1970s survey of southern hemisphere dark nebulae.
Sandqvist 157 is a southern dark nebula documented by Aage Sandqvist in his 1976 survey of opaque dust clouds using the ESO Schmidt telescope.
Sandqvist 155 is an obscured dark nebula included in astronomer Aage Sandqvist's 1970s catalog of southern dark clouds in the Milky Way.
Sandqvist 111 is a dark nebula cataloged by Swedish astronomer Aage Sandqvist during his 1970s survey of southern dark clouds at the European Southern Observatory.
Sandqvist 112 is a dark nebula in the southern sky, mapped by astronomer Aage Sandqvist in his 1970s survey of southern galactic dark clouds.
The Lupus 3 dark cloud is an active star-forming region in the Lupus constellation, distinguished as a key component of the nearby Scorpius-Centaurus stellar association.
