Top Results for Orion

The Orion Molecular Cloud Complex is a large collection of molecular clouds and associated nebulae in the constellation Orion. It includes Orion A and Orion B, with the Orion Nebula, or M42, embedded in Orion A. Dense, cold gas and dust in the complex provide the material from which stars and young...

The Horsehead Nebula, formally known as Barnard 33, is an emission nebula located within the Orion constellation. It’s a dark cloud of interstellar gas and dust notable for its distinctive equine shape. Astronomer Williamina Fleming first photographed this iconic structure in 1888. The nebula is act...

Barnard 33, widely known as the Horsehead Nebula, is a small, dark nebula located in the constellation Orion. It was first recorded in 1888 by astronomer Williamina Fleming on a photographic plate taken at the Harvard College Observatory. The nebula is a dense cloud of dust and gas that obscures the...

Betelgeuse is a massive red supergiant star located within the constellation Orion. It’s notable due to its immense size and status as a pre-supernova object, making it a key subject for astronomers studying stellar evolution and potential catastrophic events. Scientists investigate Betelgeuse to un...

Rigel is a brilliant blue supergiant star located within the constellation Orion. It’s notable for its extreme luminosity, making it readily visible and historically important for navigation. As one of the brightest stars in our sky, Rigel is observed by astronomers studying stellar evolution and th...

IC 434 is a bright emission nebula located within the Orion constellation. Discovered by William Herschel in 1786, it’s notable for its prominent glow and position adjacent to the Horsehead Nebula. Astronomers and amateur astrophotographers study IC 434 to observe stellar nurseries and understand pr...

The Orion Nebula, designated M42, is an emission nebula located approximately 1,344 light-years from Earth within the Orion constellation. It’s notable as one of the brightest nebulae visible to the naked eye and a prime location for star formation. Astronomers and amateur stargazers alike study thi...

The 1991 U.S. one-sheet for Jonathan Demme's The Silence of the Lambs, depicting Jodie Foster's face with a death's-head moth over her mouth, a design that won wide recognition for its unsettling artistry.

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...

Herbig-Haro objects 1 and 2 (HH 1-2) are bright nebulosities resulting from the collision of high-velocity jets of gas ejected by a young protostar with surrounding interstellar material. Located in the constellation Orion, they were among the first such objects to be identified and studied in detai...

Sh2-276, also known as Barnard’s Loop, is a vast emission nebula situated within the Orion constellation. Observed by E.E. Barnard in 1894, it represents a prominent arc of glowing gas linked to the larger Orion-Eridanus superbubble. The nebula's structure—particularly the Barnards loop—is notable f...

The Horsehead Nebula, also known as Barnard 33, is a dark nebula within the Orion constellation. Its distinctive silhouette against the brighter emission nebula IC 434 makes it an iconic astronomical object. Discovered by Williamina Fleming in 1888, it’s notable for its complex structure and provide...

Messier 78 (M78 or NGC 2068) is a reflection nebula located in the constellation Orion, situated roughly 1,600 light-years from Earth. It was discovered by the French astronomer Pierre Méchain in 1780 and later added to Charles Messier's catalog. The nebula is illuminated by the light of several you...

NGC 2068, better known as Messier 78, is the brightest diffuse reflection nebula in the Earth's night sky. Located within the constellation Orion, it appears distinctly blue because interstellar dust scatters the light from embedded, hot young stars. French astronomer Pierre Méchain first recorded t...

Alnitak is a multiple star system positioned as the easternmost star in Orion's Belt. The system is dominated by Alnitak Aa, a hot, blue O-type supergiant, and includes at least two smaller companion stars. It is located approximately 800 light-years from Earth and is highly luminous in the night sk...

NGC 2024, commonly known as the Flame Nebula, is an emission nebula located in the Orion Molecular Cloud Complex. It is situated in close proximity to Alnitak, one of the three bright stars forming Orion's Belt, whose intense ultraviolet light ionizes the hydrogen gas within the nebula. The nebula a...

The Flame Nebula, formally designated NGC 2024, is a vibrant emission nebula located within the Orion constellation. It’s recognized for its intense star-forming activity obscured by dense dust clouds. The nebula's bright emission arises from ionized hydrogen gas, primarily fueled by the powerful ra...

Mintaka, designated Delta Orionis, is the westernmost star in Orion's Belt and is situated almost directly on the celestial equator. It is a complex multiple-star system located roughly 1,200 light-years from Earth, with the primary component being a massive, hot blue O-type giant. Mintaka can be id...

The Orion-Eridanus Superbubble is an immense cavity of ionized hydrogen gas in the Milky Way, spanning approximately 40 degrees of the night sky. It was formed by stellar winds and supernova explosions from massive stars in the Orion OB1 association. Astronomers study this superbubble to better unde...

Theta1 Orionis C is the most massive and luminous member of the Trapezium cluster, a group of young stars at the centre of the Orion Nebula (M42). The primary component is an O-type star with an estimated mass of approximately 40 solar masses and a surface temperature exceeding 39,000 kelvin. It is...

NGC 2174 is an emission nebula within the Orion constellation. It’s notable for its distinctive resemblance to a primate's head, created by dense clouds of hydrogen gas ionized by young, hot stars. This region is actively forming new stars and is primarily observed by astronomers studying star forma...

NGC 1999 is a bright reflection nebula located in the southern part of the Orion constellation, illuminated by the variable star V380 Orionis. It is situated roughly 1,500 light-years away from Earth and lies close to the Orion Nebula. Historically, the nebula was noted for a puzzling, dark, T-shape...

Sharpless 2-276, commonly called Barnard's Loop, is a large emission nebula forming a broad arc around much of the Orion constellation. The glowing structure consists primarily of ionized hydrogen and spans roughly ten degrees of the sky, making it far larger in apparent extent than the Orion Nebula...

The Orion StarBlast 6 is a portable telescope designed for beginner astronomers and students. This compact, tabletop Dobsonian offers a straightforward path to observing celestial objects like the Moon, planets, and brighter deep-sky phenomena. Its integrated rocker box simplifies aiming and setup,...

Messier 43 is an emission nebula located within the Orion constellation. It’s notable for being a relatively isolated star-forming region, distinct from the larger Orion Nebula. The nebula contains abundant hydrogen-II gas, indicating active star formation. Astronomers and amateur observers study it...

The Running Man Nebula is a complex reflection nebula within the Orion constellation. It’s notable for its distinctive dark cloud shape resembling a sprinting figure. This emission nebula forms as starlight reflects off dust and gas, actively contributing to star formation regions. Astronomers and a...

FU Orionis is a variable star in the constellation Orion and the prototype of the FU Orionis class of pre-main-sequence stars. In 1936, it underwent a dramatic increase in brightness of several magnitudes and has remained luminous since. FU Orionis objects are young T Tauri-like stars observed to un...

Sh2-264 represents the Lambda Orionis Ring, a prominent emission nebula within the Orion constellation. This vast structure is driven by ionization from the blue giant star Meissa, creating vibrant colors. Astronomers study it to understand regions of active star formation and the interaction betwee...

NGC 2175, commonly referred to as the Monkey Head Nebula, is an H II emission nebula and open star cluster located in the constellation Orion. The massive star-forming region is composed of glowing hydrogen gas and cosmic dust energized by hot, young stars at its center, which carve out distinctive...