Top Results for Scorpius

RCW 127 is the designation given to the massive star-forming region more commonly known as NGC 6334 or the Cat's Paw Nebula, located in the constellation Scorpius. It is cataloged in the RCW (Rodgers, Campbell, Whiteoak) catalogue of H-alpha emission regions in the southern Milky Way. The complex is...

NGC 6357 is an emission nebula located in the constellation Scorpius at a distance of approximately 5,500 to 8,000 light-years from Earth. The nebula is an active star-forming region and contains the open star cluster Pismis 24, which includes some of the most massive stars known, with masses exceed...

The Butterfly Nebula, formally designated NGC 6302, is a stunning bipolar planetary nebula located within the Scorpius constellation. It’s notable for its intricate, butterfly-shaped appearance created by expanding gas and dust ejected from a dying star. This central star, intensely hot and luminous...

The Blue Horsehead Nebula, formally designated IC 4592, is a prominent reflection nebula within the constellation Scorpius. It’s notable for its distinctive blue hue created by light reflecting off interstellar dust particles illuminated by the nearby star Nu Scorpii. Astronomers and amateur observe...

Catalogued as IC 4592, the Blue Horsehead Nebula is a reflection nebula situated in the southern constellation of Scorpius. Its distinctive equine silhouette is formed by a concentrated cloud of interstellar dust that does not emit light of its own. Instead, the dust particles reflect the striking b...

The Blue Horsehead Nebula, officially designated as IC 4592, is an interstellar reflection nebula located in the constellation of Scorpius. The nebula's characteristic shape and brilliant blue coloration are the result of interstellar dust scattering and reflecting the intense light from nearby hot...

The War and Peace Nebula, formally designated NGC 6357, is a star-forming emission nebula located in the Scorpius constellation. Primarily observed through infrared light, it’s notable for its complex structure resembling a painted landscape – hence the name. This region contains abundant hydrogen g...

The Bug Nebula, formally NGC 6302, is a bipolar planetary nebula located in the Scorpius constellation approximately 3,400 light-years from Earth. This notable object displays a distinctive twin lobe shape created by expanding gas ejected from a rapidly dying star. The central star within the nebula...

IC 4592, commonly referred to as the Blue Horsehead Nebula, is a reflection nebula located in the southern constellation of Scorpius. Its distinctive blue hue is generated by interstellar dust grains that scatter and reflect the light of nearby hot stars. The primary source of this illumination is t...

IC 4592, designated as the Blue Horsehead Nebula, is a faint reflection nebula situated in the constellation of Scorpius. The cloud of interstellar dust is illuminated primarily by the bright star system Nu Scorpii, which causes the scattered light to appear distinctly blue to observers. A dark, obs...

The Cat’s Paw Nebula, formally designated NGC 6334, is an emission nebula located in the constellation Scorpius. It exhibits intense hydrogen ionization due to high levels of hot, young stars within a dense star-forming region. Situated approximately 5,500 light years from Earth, this complex provid...

The Lobster Nebula, formally designated NGC 6357, is an emission nebula located within the Scorpius constellation. It’s recognized for its significant star formation activity, particularly centered around the Pismis 24 stellar cluster. Intense ultraviolet radiation from young, hot stars characterize...

Shaula, designated Lambda Scorpii, is the second-brightest star in the constellation Scorpius and marks the tip of the scorpion's tail. The name derives from the Arabic for 'the raised tail.' It is a multiple-star system located approximately 570 light-years from Earth, with the primary component cl...

RCW 120 is a prominent emission nebula located within the constellation Scorpius. Part of the Milky Way’s southern region, it's notable for its distinctive bubble-like structure formed by ionized hydrogen gas (H II). This nebula, first documented in 1960, provides valuable insights into star formati...

The Dragonfish Nebula is a massive star-forming complex located in the constellation Scorpius, heavily obscured by interstellar dust and primarily observable in infrared wavelengths. At its core lies an embedded star cluster containing some of the most massive and luminous stars known in the Milky W...

The Butterfly Nebula, formally NGC 6302, is a bipolar planetary nebula located in the constellation Scorpius. It’s notable for its distinctive butterfly shape formed by expanding gas plumes. At its center lies one of the hottest known stars, reaching approximately 250,000 Kelvin. Astronomers and tho...

The Prawn Nebula, formally designated IC 4628, is an emission nebula located within the Scorpius constellation. It represents a region of intense star formation characterized by hot, young stars ionizing surrounding gas. This nebula, also known as Gum 56, is notable for its distinct shape and vibran...

IC 4628 is a large emission nebula in the constellation Scorpius, commonly called the Prawn Nebula. Ultraviolet radiation from hot young stars ionizes surrounding hydrogen gas, causing the cloud to glow and marking it as an active star-forming region. Located several thousand light-years from Earth,...

NGC 6357, nicknamed the War and Peace Nebula, is a vast star-forming emission nebula located in the constellation Scorpius. It hosts the massive Pismis 24 open star cluster, which contains some of the most massive stars ever discovered. The nebula earned its nickname due to its appearance in infrare...

GJ 667 is a triple star system located approximately 23 light-years away in the constellation Scorpius. The primary components consist of two K-type main-sequence stars orbiting each other, while the third component, GJ 667C, is a distant red dwarf. The M-dwarf companion hosts several confirmed exop...

18 Scorpii is a main-sequence G-type star in the constellation Scorpius, approximately 46 light-years from Earth. It is frequently classified as a solar twin because its temperature, luminosity, chemical composition, mass, and magnetic activity are broadly similar to those of the Sun. The star is ne...

IC 4605 is a yellowish reflection nebula located in the Rho Ophiuchi cloud complex, a vast stellar nursery situated roughly 460 light-years away in the constellation Ophiuchus.

Upsilon Scorpii, traditionally named Lesath, is a hot blue-white subgiant star located in the southern constellation of Scorpius. Positioned approximately 580 light-years from Earth, it marks the southern tip of the scorpion's stinger. Lesath forms a visual pair with the neighboring star Shaula, col...

NGC 6072 is a planetary nebula located in the southern constellation of Scorpius, first documented by astronomer John Herschel in 1837. The structure is characterized by its distinct, slightly asymmetrical, ring-like appearance, which was created by the expulsion of outer layers of gas from an aging...

AH Scorpii is a cool red supergiant in the constellation Scorpius and a variable star whose apparent brightness changes over time. Its extended atmosphere and low surface temperature give it a deep red color, while observations of its variability and surrounding material help astronomers examine the...

NGC 6357, commonly referred to as the Lobster Nebula, is a vast emission nebula situated in the constellation Scorpius roughly 8,000 light-years from Earth. It is an active star-forming region characterized by sprawling clouds of gas and dark dust. At its core lies Pismis 24, an exceptionally young...

IC 4601 is a reflection nebula located in the northern constellation of Ophiuchus. Like other reflection nebulae, it does not emit visible light itself but instead scatters the light from nearby stars. The dense interstellar dust within the nebula is particularly effective at scattering blue wavelen...

An active star-forming emission nebula in Scorpius about 5,500 light-years away, containing numerous protostars and dense molecular clouds making it one of the most productive stellar nurseries nearby.

Paikauhale, formally designated Tau Scorpii, is a hot blue-white main-sequence star located in the constellation Scorpius. The star is scientifically notable for its strong stellar winds, complex magnetic fields, and corresponding X-ray emissions. Its traditional Hawaiian name, meaning "irresponsibl...