Best Vulpecula

HD 189733 is a K-type main-sequence star located approximately 64 light-years away in the constellation Vulpecula. The star hosts a hot Jupiter exoplanet, HD 189733 b, discovered in 2005, which became the first exoplanet to have its atmospheric composition directly characterized through transmission...

The Dumbbell Nebula (Messier 27) is a large planetary nebula formed from the ejected remains of a white dwarf star. Discovered by Charles Messier in 1764, it’s notable for its substantial size and brightness within this type of celestial object. Located approximately 1,360 light-years away in the co...

NGC 6820 is an emission nebula in Vulpecula surrounding cluster NGC 6823, notable for pillars of gas shaped by radiation from young massive stars.

Sh2-86 is an H II emission nebula located in the constellation Vulpecula. It is closely associated with the young open star cluster NGC 6823 and serves as a primary site of active star formation within the Vulpecula OB1 stellar association. The region is cataloged within the Sharpless catalog of neb...

NGC 6823 is an open star cluster situated in Vulpecula, notable for its surrounding emission nebula and formation shaped by stellar winds.

Sh2-88 is a Vulpecula H II complex tied to Vulpecula OB1, notable for compact knots Sh2-88B1 and the ultracompact region Sh2-88B2.

Sh2-90 is a small Vulpecula H II region, notable for a hollow shell structure and embedded infrared sources linked to ongoing star formation.

Abell 74 is an ancient planetary nebula distinguished by its large, faint, and highly evolved ring of ionized gas surrounding a central binary star.