Best Cygnus
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The Veil Nebula is a vast emission nebula located in Cygnus. It represents the expanding remains of a star explosion, specifically the supernova associated with the Cygnus Loop. This remnant, formed approximately 10,000 to 20,000 years ago, exhibits intricate filament structures and intense radiatio...
NGC 6960 is a filamentary nebula in the constellation Cygnus, constituting the western arc of the larger Veil Nebula. It represents the visible remains of a supernova blast wave that exploded approximately 8,000 years ago. The nebula's filaments appear to cross the foreground star 52 Cygni, though t...
The North America Nebula, formally designated NGC 7000, is a large emission nebula situated within the Cygnus constellation. It’s notable for its distinctive shape resembling a continent, initially identified in a photograph by Max Wolf in 1890. This region contains abundant ionized hydrogen (H II)...
NGC 6888, known as the Crescent Nebula, is an emission nebula located approximately 5,000 light-years away in the constellation Cygnus. It was formed by the powerful stellar winds of the Wolf-Rayet star WR 136 interacting with material the star previously ejected during its red giant phase. The nebu...
NGC 7027 is a vibrant planetary nebula located within the constellation Cygnus. Formed from the ejected material of a dying star, it’s notable for its exceptionally bright and compact central region, a characteristic of young nebulae. Astronomers and amateur observers interested in stellar evolution...
NGC 7000, commonly known as the North America Nebula, is a large emission nebula located in the constellation Cygnus. Its popular name derives from its distinctive shape, which closely resembles the continent of North America. The nebula is situated near Deneb, one of the brightest stars in the nigh...
Sharpless 2-106 is a bipolar emission nebula located within the Cygnus constellation. It’s notable for its distinct twin lobes created by the energetic output of young star S106 IR. This nebula serves as an excellent example of stellar winds sculpting interstellar gas and dust, primarily observed by...
The Egg Nebula, formally CRL 2688, is a stunning bipolar nebula within the Cygnus constellation. It’s notable for its distinctive egg-shaped structure formed by the interaction of stellar winds with a central protostar. This type of nebula provides valuable insights into the early stages of star for...
Pickering's Triangle, designated as NGC 6979, is a portion of the Cygnus Loop, a large supernova remnant in the constellation Cygnus. The filamentary structure was discovered photographically in 1904 by astronomer Williamina Fleming at the Harvard College Observatory under the direction of Edward Ch...
The Pelican Nebula, formally designated IC 5070, is a vibrant emission nebula located within the Cygnus constellation. It’s recognized as an H II region characterized by intense star formation driven by ionization fronts created by hot, young stars. Astronomers and amateur astrophotographers find it...
The Eastern Veil Nebula, catalogued as NGC 6992 and NGC 6995, is a bright filamentary arc of ionized gas forming the eastern section of the Cygnus Loop, a supernova remnant in the constellation Cygnus. The gas was heated by a supernova explosion estimated to have occurred roughly 8,000 years ago. It...
The Crescent Nebula, formally NGC 6888, is a stunning emission nebula within Cygnus. It’s notable for its distinctive crescent shape and the powerful stellar wind emanating from Wolf-Rayet star WR 136. This vibrant structure provides valuable insight into processes of star birth and death observed b...
The Veil Nebula, formally NGC 6960 and NGC 6992, is a vast, filamentary structure within the constellation Cygnus. It represents the aftermath of a supernova event that occurred roughly 8,000 years ago. This ancient nebula’s intricate shapes are formed by expanding gas and dust ejected during the ex...
Sharpless 2-106 is a bipolar emission nebula located approximately 2,000 light-years from Earth in the constellation Cygnus. The nebula's distinctive hourglass shape is created by jets of gas expelled from a central massive star, with the structure visible in both optical and infrared wavelengths. I...
The Gamma Cygni Nebula, cataloged as IC 1318, is an extensive emission-nebula complex in the constellation Cygnus. It appears near Sadr, or Gamma Cygni, in the sky, although the star is in the foreground and is not the nebula's principal source of ionization. Glowing hydrogen regions divided by dark...
Albireo (Beta Cygni) is a double star system in the constellation Cygnus, appearing as the star marking the head of the swan asterism. The brighter primary component is a K-type giant star with a warm amber or golden hue, while the companion is a B-type main-sequence star appearing blue. The pair ca...
The Cocoon Nebula, formally designated IC 5146, is an emission and reflection nebula located within the Cygnus constellation. It’s notable for its distinctive bubble-like structure formed by light reflecting off dust clouds. Barnard 168, a dark lane, is closely associated with this region. Astronome...
The Blinking Eye Nebula is a planetary nebula located in the constellation Cygnus. It is known for an optical illusion where its central star appears to blink when viewed through a telescope using averted vision. As the observer looks away, the central star seems to disappear, making the nebula itse...
IC 1340 is a luminous filamentary structure of ionized gas located in the northern constellation Cygnus. It constitutes the southernmost portion of the Veil Nebula, a large, diffuse supernova remnant resulting from a stellar explosion that occurred roughly 8,000 years ago. The glowing gas filaments...
NGC 6979 is a portion of the Veil Nebula, a large supernova remnant located in the constellation Cygnus. The Veil Nebula is the visible portion of the Cygnus Loop, which was created by the explosion of a massive star thousands of years ago. NGC 6979 appears as a filamentary structure of glowing gas,...
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...
P Cygni is a luminous blue variable star in the constellation Cygnus, estimated to lie several thousand light-years from Earth. It became visible to the naked eye during outbursts around 1600 and again in the mid-17th century, establishing it as one of the earliest recognized variable stars. Its spe...
IC 1318 is a sprawling, diffuse emission nebula complex located in the constellation Cygnus, situated near the bright star Sadr. Often referred to as the Butterfly Nebula due to its visually segmented appearance, the glowing gas clouds are dramatically divided by intervening patches of dark interste...
The Jewel Bug Nebula, officially designated NGC 7027, is a compact emission nebula located within the Cygnus constellation. It was first observed by William Herschel in 1790 and is notable for its intricate structure of gas, primarily ionized nitrogen. This planetary nebula represents the final stag...
The Gamma Cygni Nebula represents an emission nebula formed from ionized hydrogen (HII) gas surrounding the star cluster Sadr in the Cygnus constellation. This expansive region, identified by Edward Barnard in 1893, is notable for its bright pink and red hues produced by energized hydrogen atoms. As...
Kepler-22 is a G-type main-sequence star located approximately 620 light-years away in the constellation Cygnus. It is notable for hosting Kepler-22b, an exoplanet announced in 2011 as the first confirmed planet discovered by the Kepler space telescope to orbit within the habitable zone of a Sun-lik...
NGC 6888, commonly called the Crescent Nebula, is an emission nebula in the constellation Cygnus. It formed as fast stellar wind from the Wolf-Rayet star WR 136 collided with material expelled during an earlier phase of the star's evolution, producing an expanding shell of energized gas. Its curved...
The Soap Bubble Nebula is a delicate planetary nebula located within the constellation Cygnus. Formed from the expelled gases of a dying star, it’s notable for its unusual bubble-like shape resembling a soap bubble. Amateur astronomers like Dave Jurasevich discovered this faint object in 2007. It's...
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