Best Aquila
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Altair is a brilliant A-type main-sequence star located within the constellation Aquila. Situated just 17 light-years from Earth, it’s notable for its exceptionally fast rotation rate. This rapid spin causes a flattening of the star at its poles. Altair represents a key nearby star system and is par...
The Great Rift is an extensive series of dark molecular dust clouds that obscures a significant portion of the Milky Way galaxy's bright band in Earth's night sky. It stretches from the constellation Cygnus through Aquila and Serpens toward Sagittarius. The dense concentrations of interstellar dust...
W49A is a giant H II region and one of the most massive star-forming complexes in the Milky Way, located approximately 36,000 light-years away in the constellation Aquila. It contains numerous massive O-type stars and is studied as an analog to distant starburst regions because of its extreme lumino...
Vultur volans refers to the ancient Roman designation of the constellation Aquila, meaning “Flying Vulture.” This constellation was identified by Greek astronomers in the 2nd century BC and later adopted by the Romans. It’s notable for its association with a prominent bird figure in classical mythol...
The W51 Nebula is one of the most massive and active star-forming H II regions in the Milky Way galaxy. Located approximately 17,000 light-years away in the constellation Aquila, this stellar nursery is characterized by dense clouds of gas and dust where new stars are actively being born. Astronomer...
NGC 6751 is a glowing planetary nebula in the Aquila constellation, visually estimated to be several thousand years old and discovered by Albert Marth.
W49B represents the expanding debris field of a long-dead star located in the Aquila constellation approximately 33,000 light-years from Earth. This supernova remnant is particularly interesting due to its irregular shape, suggesting a complex explosion mechanism possibly involving jets. Astronomers...
The Manatee Nebula is a supernova remnant in the constellation Aquila that resembles the marine mammal and features unusual jet structures from a microquasar.
The Aquila Rift is a massive dark cloud complex in the Milky Way, notable for containing active star-forming regions situated roughly 600 light-years from Earth.
Barnard 143 is a dark emission nebula located within the Aquila constellation. It’s notable for creating a striking silhouette against the Milky Way due to its dense dust clouds. Astronomers and amateur observers study this region to understand star formation processes and the interaction of gas, du...
The Manatee Nebula, formally designated W50, is a supernova remnant located in the constellation Aquila. Approximately 18,000 light-years from Earth, it’s notable for its distinctive radio emission pattern resembling a manatee and contains the microquasar SS 433 at its core. This nebula originates f...
Barnard 142 is a dark emission nebula located within the Aquila constellation. It’s notable for its distinctive hourglass shape formed by glowing dust and gas ejected from a dying star. Astronomers and amateur observers study it to understand stellar evolution and the processes of planetary nebula f...
The E Nebula is a dark nebula in the constellation Aquila, formed by interstellar dust that obscures the light of stars behind it. Its apparent shape resembles a capital letter E in wide-field photographs and telescopic views, producing the name by which the complex is commonly known. The feature in...
The Glowing Eye Nebula, formally cataloged as NGC 6751, is a planetary nebula located in the northern constellation of Aquila. German astronomer Albert Marth discovered the object in 1863, and modern measurements estimate its diameter at approximately 0.8 light-years. It consists of expanding ionize...
W44 is a mixed-morphology supernova remnant located in the constellation Aquila, estimated to be roughly 20,000 years old. It is characterized by a combination of a radio shell and thermal X-ray emission contained within its boundaries. The remnant is physically associated with the pulsar PSR B1853+...
The E Nebula is a dark absorption cloud in Aquila cataloged by E. E. Barnard, notable for its dark silhouette resembling the letter E.
NGC 6781, informally known as the Snowglobe Nebula, is a planetary nebula situated in the northern constellation of Aquila. It was first documented by the astronomer William Herschel in 1788 during his systematic surveys of the night sky. Astrophotographic studies reveal that the structure consists...
Barnard 335 (B335) is an isolated, dark molecular cloud known as a Bok globule, located in the constellation Aquila. It is recognized as a prototypical environment for low-mass star formation. Inside the opaque cloud, an embedded protostar is actively accreting surrounding gas and dust. Because of i...
Abell 70 (also known as PN A66 70) is a planetary nebula located in the constellation Aquila. It is notable for the presence of a background galaxy that appears superimposed on its rim, creating a distinctive diamond-shaped appearance in telescope images. The nebula contains a binary central star sy...
Sharpless 2-71 is an irregular planetary nebula in Aquila, discovered by Rudolph Minkowski in 1946 and studied for its unusually complex stellar system.
NGC 6781, sometimes called the Snowglobe Nebula, is a planetary nebula in the constellation Aquila. William Herschel discovered it in 1788, and modern observations indicate that its apparently ring-like form is a projection of a more complex, barrel-shaped shell of gas. The nebula was produced when...
A planetary nebula in Aquila approximately 6,500 light-years away, notable for its complex multi-shell structure and high-velocity gas knots visible in Hubble Space Telescope images.
A supernova remnant in Aquila notable for containing the microquasar SS 433, whose relativistic jets have distorted the remnant into its elongated, manatee-like shape.
A compact, high-surface-brightness planetary nebula in Aquila about 7,000 light-years away, notable for its extremely hot central star and dense, rapidly evolving ionized shell.
Sh2-71 is a striking planetary nebula in the constellation Aquila, distinguished by its complex, asymmetric morphology and the highly debated binary nature of its central star system.
A ring-shaped planetary nebula in Aquila discovered by William Herschel in 1791, featuring a bright annular shell surrounded by a faint extended outer halo.
