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'Trapez' images and/or videos results page 1 of 4

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Images of 'Trapez' found, 274

Love Flight of a Pink Candy Heart, 1930 (oil on canvas)
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Circus Heights, 2002 (oil on canvas)
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Women of Paris: The Circus Lover, 1885 (oil on canvas)
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Moscow State Circus, 1988
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Circus Acrobats
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The Flying Codomas, illustration from the portfolio 'Jazz', 1947 (colour stencil print)
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Acrobat on the Trapeze, 1979 (pastel on paper)
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The Rockefeller Emerald
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Circus Scene I, 1994 (w/c on paper)
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Tony Curtis, Gina Lollobrigida And Burt Lancaster, Trapeze 1956 Directed By Carol Reed
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The Rockefeller Emerald
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Orion Nebula - the trapeze - The Trapezium region in M42 - Located 1500 years - light, Orion Nebula is the closest region of formation of stars of the Sun. In the center of the picture, the Trapeze of Orion. The Trapeze is among the youngest known open clusters, it is made up of 4 massive stars that make the nebula shine. The central 'star' of the three groups forming the asterism of Orion's sword is in reality a nebula, and is clearly nebulous to the unaided eye. At the heart of the most luminous nebulosity shimmer a handful of stars known as the Trapezium cluster, visible in binoculars. These are the brightest members of a substantial cluster of stars, most of which are still hidden in the dusty recesses of the Orion nebula against which they are seen. The stars of the Trapezium provide much of the energy which makes the brilliant Orion Nebula visible and are at a distance of about 1500 light years
Acrobats, c.1933 (linocut)
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Mural for Cruise Liner, 1995 (w/c on paper)
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The Flying Trapeze, 1899 (pencil on paper)
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Two Trapeze Artists (b/w photo)
The Arc Maker I & II (acrylic on canvas with collage)
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Lancaster House, built 1825-40, London, UK (photo)
The Circus (oil on panel)
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W.C. Coup's New United Monster Shows: Bebe the Flying Lady, 1892 (colour litho)
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The Human Cannonball ''Loyal'' Fired from the cannon., 1879 (poster)
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On a Blue Ceiling, Eight Geometric Figures: Circle, Trapezoid, Parallelogram, Rectangle, Square, Triangle, Right Triangle, X (Wall Drawing No. 35), 1981 (chalk & latex paint on plaster)
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On a Blue Ceiling, Eight Geometric Figures: Circle, Trapezoid, Parallelogram, Rectangle, Square, Triangle, Right Triangle, X (Wall Drawing No. 35), 1981 (chalk & latex paint on plaster)
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Trapeze Artist On The Swing (b/w photo)
Drawing for 'The Very Clumsy Click Beetle', 1977 (w/c on paper)
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12345-1, 1979 (graphite, pen and black ink on paper)
Jean-Paul Belmondo (b/w photo)
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Orion Nebula - the trapper
Weights on a brown field, 1969 (ink on paper)
Trapeze artists in the 19th century, from The Century Magazine, published 1887 (engraving)
Trapeze, 1956 (film still)
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The Acrobats, published 1925 (drypoint)
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Orion Nebula - the trapeze - The Trapezium region in M42 - Located 1500 years - light, Orion Nebula is the closest region of formation of stars of the Sun. In the center of the picture, the Trapeze of Orion. The Trapeze is among the youngest known open clusters, it is made up of 4 massive stars that make the nebula shine. Image obtained with Siding Spring's 3.9m telescope. The central 'star' of the three groups forming the asterism of Orion's sword is in reality a nebula, and is clearly nebulous to the unaided eye. At the heart of the most luminous nebulosity shimmer a handful of stars known as the Trapezium cluster, visible in binoculars. These are the brightest members of a substantial cluster of stars, most of which are still hidden in the dusty recesses of the Orion nebula against which they are seen. The stars of the Trapezium provide much of the energy which makes the brilliant Orion Nebula visible and are at a distance of about 1500 light years. This image was made at the prime focus of the Anglo - Australian Telescope
Orion's Trapeze - Trapezium Multiple Star System in Orion - Orion's Trapeze is one of the youngest open clusters known, with new stars still forming in this region. The Trapezium is the most famous multiple star system in the entire night sky. Located at the very heart of M42, the Orion Nebula, it is one of the youngest star clusters known. The four brightest stars in the Trapezium (A, B, C and D) are easily visible in a four inch telescope with decent optical quality under good seeing conditions. They range in brightness from magnitude 5 to magnitude 8. They can be seen merged together as one star to the unaided eye as the middle star in the sword of Orion. The image above shows the four brightest stars of the Trapezium at the center of the photo. The core of M42 surrounding the Trapezium is a blue - green color from the predominantly green spectral emission line of Oxygen III, with a smaller amount of blue - green mixed in from the hydrogen - beta emission line. These particular wavelengths also happen to be the wavelengths to which the human visual system is most sensitive for color vision. Much of the rest of the Orion Nebula has a lot of red hydrogen - alpha emission, but the eye is not very sensitive to this wavelength. Some red can be seen in the brightest parts of the nebula that emit hydrogen - alpha light by observers with sensitive color vision. For most people however, if they see any color at all, it will be a very pale green, or blue - green, from the Oxygen III spectral lines
Orion Nebula - the trapeze - The Trapezium region in M42 - Located 1500 years - light, Orion Nebula is the closest region of formation of stars of the Sun. In the center of the picture, the Trapeze of Orion. The Trapeze is among the youngest known open clusters, it is made up of 4 massive stars that make the nebula shine. Image obtained with Siding Spring's 3.9m telescope. 30-sec poses. The central 'star' of the three groups forming the asterism of Orion's sword is in reality a nebula, and is clearly nebulous to the unaided eye. At the heart of the most luminous nebulosity shimmer a handful of stars known as the Trapezium cluster, visible in binoculars. These are the brightest members of a substantial cluster of stars, most of which are still hidden in the dusty recesses of the Orion nebula against which they are seen. The stars of the Trapezium provide much of the energy which makes the brilliant Orion Nebula visible and are at a distance of about 1500 light years. This image was made with three, 30 - second exposures at the prime focus of the Anglo - Australian Telescope
Orion Nebula - the trapeze - The Trapezium region in M42 - Located 1500 years - light, Orion Nebula is the closest region of formation of stars of the Sun. In the center of the picture, the Trapeze of Orion. The Trapeze is among the youngest known open clusters, it is made up of 4 massive stars that make the nebula shine. Image obtained with Siding Spring's 3.9m telescope. The central 'star' of the three groups forming the asterism of Orion's sword is in reality a nebula, and is clearly nebulous to the unaided eye. At the heart of the most luminous nebulosity shimmer a handful of stars known as the Trapezium cluster, visible in binoculars. These are the brightest members of a substantial cluster of stars, most of which are still hidden in the dusty recesses of the Orion nebula against which they are seen. The stars of the Trapezium provide much of the energy which makes the brilliant Orion Nebula visible and are at a distance of about 1500 light years. This image was made at the prime focus of the Anglo - Australian Telescope
Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun
Orion Nebula - the trapeze - The Trapezium region in M42 - Located 1500 years - light, Orion Nebula is the closest region of formation of stars of the Sun. In the center of the picture, the Trapeze of Orion. The Trapeze is among the youngest known open clusters, it is made up of 4 massive stars that make the nebula shine. Image obtained from the 1.5m Danish telescope of La Silla in Chile. The central 'star' of the three groups forming the asterism of Orion's sword is in reality a nebula, and is clearly nebulous to the unaided eye. At the heart of the most luminous nebulosity shimmer a handful of stars known as the Trapezium cluster, visible in binoculars. These are the brightest members of a substantial cluster of stars, most of which are still hidden in the dusty recesses of the Orion nebula against which they are seen. The stars of the Trapezium provide much of the energy which makes the brilliant Orion Nebula visible and are at a distance of about 1500 light years. This image was made at the danish 1.5 meter telescope in La Silla, Chile
Cirque D'Hiver, 1814 (colour litho)
Trapeze, 1956 (film still)
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Trapeze, 1956 (film still)
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Trapeze, 1956 (film still)
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Trapeze artists practicing
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Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained from the 2.2 meter MPG/ESO telescope of the La Silla Observatory. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun. This new image of the Orion Nebula was captured using the Wide Field Imager camera on the MPG/ESO 2.2 - metre telescope at the La Silla Observatory, Chile. This image is a composite of several exposures taken through a total of five different filters. Light that passed through a red filter, as well as light from a filter that shows the glowing hydrogen gas, is colored red. Light in the yellow - green part of the spectrum is colored green, blue light is colored blue and light that passed through an ultraviolet filter has been colored purple. The exposure times were about 52 minutes through each filter
Trapeze, 1956 (film still)
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Trapeze, 1956 (film still)
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Woman in the trapeze, 1930
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Orion's Nebula - The Great Nebula in Orion - Located 1500 years ago - the light of the Earth, Orion's Nebula is the closest region to the formation of stars of the Sun. In its heart, a group of young stars called Orion's Trapeze. To the eye, the nebula appears as a misty patch around the central star of the line of three which form Orion's sword. The central group of stars is the Trapezium cluster and these stars are responsible for producing the nebula. It is the high concentration of dust and gas in this part of the sky which has resulted in the formation of the stars, so the Orion nebula is no random association of bright stars and dusty gas. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun
Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained from the 2.2 meter MPG/ESO telescope of the La Silla Observatory. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun. This new image of the Orion Nebula was captured using the Wide Field Imager camera on the MPG/ESO 2.2 - metre telescope at the La Silla Observatory, Chile. This image is a composite of several exposures taken through a total of five different filters. Light that passed through a red filter, as well as light from a filter that shows the glowing hydrogen gas, is colored red. Light in the yellow - green part of the spectrum is colored green, blue light is colored blue and light that passed through an ultraviolet filter has been colored purple. The exposure times were about 52 minutes through each filter
Orion nebula centre - Trapeze - Orion nebula center - Mosaic of images obtained by the space telescope in 1994 and 1995 showing the center of Orion nebula, the region around the Trapeze, a cluster of 4 very young and massive stars that make this nebula shine. The picture shows a churning turbulent star factory set within a maelstrom of flowing, luminescent gas. Although this 2.5 light - years wide view is still a small portion of the entire Orion nebula, it includes almost all of the light from the bright glowing clouds of gas and a star cluster associated with the nebula. Hubble reveals details as small as 4.1 billion miles across. Hubble Space Telescope observing time was devoted to making this panorama because the nebula is a vast laboratory for studying the processes which gave birth to our own Sun and solar system 4.5 billion years ago. Gas are illuminated and heated by a torrent of energetic ultraviolet light from its four hottest and most massive stars, called the Trapezium, which lie near the center of the image. In addition to the Trapezium, this stellar cavern contains 700 hundred other young stars at various stages of formation. High - speed jets of hot gas spewed by some of the infant stars send supersonic shock waves tearing into the nebula at 100,000 miles per hour. These shock waves appear as thin curved loops, sometimes with bright knots on their end (the brightest examples are near the bright star at the lower left). The mosaic reveals at least 153 glowing protoplanetary disks (first discovered with the Hubble in 1992, and dubbed “” proplyds”) that are believed to be embryonic solar systems that will eventually form planets. (Our solar system has long been considered the relic of just such a disk that formed around the newborn Sun). The abundance of such objects in the Orion nebula strengthens the argument that planet formation is a common occurrence in the universe. The proplyds that are closest to the Trapezium stars (image c
'Appy 'Ampstead, c.1933 (linocut)
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Center of the Orion Nebula - Trapeze - Orion nebula center - Mosaic of infrared images showing the center of the Orion Nebula, the Trapeze region. 4 massive stars form the Trapeze but the image also shows the cluster of stars associated with it, constitutes a thousand stars of about 1 million years old. Mosaic of 81 infrared images obtained by the ISAAC instrument at the VLT. Colour composite mosaic image of the central part of the Orion Nebula, based on 81 images obtained with the infrared multi - mode ISAAC instrument on the ESO Very Large Telescope (VLT) at the Paranal Observatory. The famous Trapezium stars are seen near the centre and the photo also shows the associated cluster of about one thousand stars, about a million years old
The Acrobat, 1983 (oil on canvas)
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Harold Langdon, silent comedian, in The Strong Man
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Orion M43 Nebula and the Trapeze - The Orion Nebula, M43 and Trapezium - The M43 Nebula (NGC 1982) is part of the large Orion Nebula (M42), the central part of which can be seen at the bottom right. The Trapeze d'Orion is a very young cluster of stars nestled in the heart of the nebula. Located 1500 years - light, Orion's Nebula is the closest region of formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. Nebula M43 (NGC 1982) belongs to the great Orion nebula (M42), seen at bottom. This image also reveals the Orion Trapezium, a group of stars (bottom right) that makes the Orion nebula shine. Orion Nebula is located at a distance of about 1500 light years
Composition with trapezium (colour litho)
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Five male trapeze artists performing at a circus c1890.
Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this picture using the Anglo - Australian Telescope at Siding Spring