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'Nebulous' images and/or videos results page 1 of 1

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Images of 'Nebulous' found, 72

Crossbound, 2006 (oil on canvas)
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Morning, 2003 (oil on canvas)
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Yellow Ocean, 2004 (oil on canvas)
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Tibetan Buddhism; central temple; Uetse; Samye Monastery; Himalaya Range; Central Tibet; EU-Tsang; Tibet Autonomous Region; People's Republic of China; Asia
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
Remnants of the Supernova of Sails - The Vela Supernova Remnant - Remnant of the Supernova of Sails. The supernova exploded 12,000 years ago and is approximately 815 light years away from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. About 120 centuries ago an inconspicuous star in what is now the constellation of Vela brightened by about 100 million times to rival the Moon as the brightest object in the night sky. This photograph shows a portion of the north - western quadrant of an expanding nebulous shell, which now surrounds the site of the explosion. Near the centre of the nebula (and not seen here) is the Vela pulsar, a rapidly - spinning neutron star only a few kilometres in diameter, the remnant of the star that exploded. This tiny object spins about 11 times a second and until recently was among the faintest stars ever studied at optical wavelengths, a far cry from its brief glory as one of the brightest stars ever seen
Cradle, 2010 (oil on canvas)
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Flags in front of the snow-covered Eiger Mountain; 3970 m; north wall; the Alps; Grindelwald; Bernese Oberland; Canton of Bern; Switzerland; Europe
Grand Hotel; Karl Johans Gate No. 31; Oslo; Norway; Scandinavia; Northern Europe; Europe
Assembly Hall; Parliament; the Storting building; Storthinget; inner city; Oslo; Norway; Scandinavia; Northern Europe; Europe
Agriculture; tobacco plants in the field; at Thakhek; Khammuan province; Khammouane; Laos; Southeast Asia; Asia
Views of snowy mountain peaks from Mt. Heimgarten; at Ohlstadt; Bavarian Alps; Upper Bavaria; Bavaria; Germany; Europe
Modern architecture; inclined plane; dark clouds reflected in the glass; New Opera House; Operaen; Oslo; Norway; Scandinavia; Northern Europe; Europe
Theravada Buddhism; grey high stupa; Wat Phrabat temple; Bolikhamsai province; Bolikhamxai; Laos; Southeast Asia; Asia
Modern architecture; inclined plane; people walking on the roof; New Opera House; Operaen; Oslo; Norway; Scandinavia; Northern Europe; Europe
Boats bobbing in the bay; Adria; Caorle; Venice Province; Veneto; Italy; Europe
Simple hut in a green rice field; bamboo hut; storm clouds; province of Luang Namtha; Northern Laos; Laos; Southeast Asia; Asia
Nebulae NGC 1973 - 1975 - 1977 in Orion - The reflection nebulae NGC 1973 - 75 - 77 in Orion - Reflection nebulae located just north of the Great Orion Nebula. This group of nebulous stars is just half a degree north of the much brighter Orion Nebula and has largely been ignored because of it. The group of stars here appear as a single star to the unaided eye, the northernmost 'star' in the sword of Orion. Most of the blue nebulosity is starlight scattered by dust, while some of the stars are sufficiently hot to excite the wisps of hydrogen that linger here and create a distinctive red glow
Remnants of the Supernova of Sails - The Vela Supernova Remnant - Remnant of the Supernova of Sails. The supernova exploded 12,000 years ago. The rest of the supernova is approximately 815 years away from Earth. Image obtained with FSQ 106 bezel, 6 hours of installation. About 120 centuries ago an inconspicuous star in what is now the constellation of Vela brightened by about 100 million times to rival the Moon as the brightest object in the night sky. This photograph shows a portion of the north - western quadrant of an expanding nebulous shell, which now surrounds the site of the explosion
Nebulae NGC 1973 - 1975 - 1977 in Orion - The reflection nebulae NGC 1973 - 75 - 77 in Orion - Reflection nebulae located just north of the Great Orion Nebula. This group of nebulous stars is just half a degree north of the much brighter Orion Nebula and has largely been ignored because of it. The group of stars here appear as a single star to the unaided eye, the northernmost 'star' in the sword of Orion. Most of the blue nebulosity is starlight scattered by dust, while some of the stars are sufficiently hot to excite the wisps of hydrogen that linger here and create a distinctive red glow. To the south of the nebula (at the bottom of the picture) faint traces of the yellow reflected light of the Orion nebula can just be detected
Star clusters, 1814
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Plaque de la rue La Caille in Paris - Street Plaque in Paris - Rue du XVIII arrondissement de Paris, in tribute to Nicolas Louis de La Caille (1713 - 1762), astronomer and geodesian. He was responsible for the measurement of a Meridian arc from Cape Town, where he lived from 1751 to 1754, and for the creation of 14 constellations of the southern hemisphere. Rue La Caille, street sign. Abbe Nicolas Louis de Lacaille (March 15, 1713 - March 21, 1762) was a French astronomer. He is noted for his catalogue of nearly 10,000 southern stars, including 42 nebulous objects. This catalogue introduced 14 new constellations which have since become standard
NORTHERN LEAGUE SUPPORTERS GATHER IN VENICE, 1997-09-15 (photo)
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NORTHERN LEAGUE SUPPORTERS GATHERED IN VENICE, 1997-09-15 (photo)
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Sketches for the exterior façade and interior of Sandham Memorial Chapel, 1923 (pencil on paper)
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Sketches for the exterior façade and interior of Sandham Memorial Chapel, 1923 (pencil on paper)
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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 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
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
Remnants of the Supernova of Sails - Part of the Vela Supernova Remnant - Rest of the Supernova of Sails. The supernova exploded 12,000 years ago and is approximately 815 light years away from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. About 120 centuries ago an inconspicuous star in what is now the constellation of Vela brightened by about 100 million times to rival the Moon as the brightest object in the night sky. This photograph shows a portion of the north - western quadrant of an expanding nebulous shell, which now surrounds the site of the explosion. Near the centre of the nebula (and not seen here) is the Vela pulsar, a rapidly - spinning neutron star only a few kilometres in diameter, the remnant of the star that exploded. This tiny object spins about 11 times a second and until recently was among the faintest stars ever studied at optical wavelengths, a far cry from its brief glory as one of the brightest stars ever seen
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 - 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
Nebula NGC 6334 in the Scorpion - The 'reddened' nebulosity of NGC 6334 - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebula NGC 6334 shows no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. This nebula is quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour of stars associated with the nebula indicate that they are dimmed by a factor of about 10 in the green part of the spectrum, much more in the blue, but relatively little at red wavelengths. Some care has been taken to ensure that these images are as close to true - colour as possible
Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius - These nebulae are located approximately 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebulae NGC 6334 and NGC 6357 show no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. These nebulae are quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Careful measurement of the colour of stars associated with the nebulae indicate that they are dimmed by a factor of about 10 in the green part of the spectrum, much more in the blue, but relatively little at red wavelengths. Some care has been taken to ensure that these images are as close to true - colour as possible
Barree spiral galaxy NGC 1483 in Dorado - Barred spiral galaxy NGC 1483 in Dorado - NGC 1483 is a barree spiral galaxy located about 60 million years ago - light in the southern constellation of Dorado. Image obtained by the Hubble Space Telescope (HST). NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star - forming regions. In the background, many other distant galaxies can be seen. The constellation Dorado is home to the Dorado Group of galaxies, a loose group comprising an estimated 70 galaxies and located some 62 million light - years away. The Dorado group is much larger than the Local Group that includes the Milky Way (and which contains around 30 galaxies) and approaches the size of a galaxy cluster. Galaxy clusters are the largest groupings of galaxies (and indeed the largest structures of any type) in the Universe to be held together by their gravity. Barred spiral galaxies are so named because of the prominent bar - shaped structures found in their center. They form about two thirds of all spiral galaxies, including the Milky Way. Recent studies suggest that bars may be a common stage in the formation of spiral galaxies, and may indicate that a galaxy has reached full maturity. Image taken with the Hubble space telescope (HST)
Academy of Fine Arts, Munich, 1999 (photo)
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Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the brim with stars. This image is formed from data gathered by the Focal Reducer and low dispersion Spectrograph (FORS) instrument, installed on Eso's Very Large Telescope at Paranal Observatory. An array of distant galaxies are also visible throughout the frame, the most prominent being the small, edge-on, spiral galaxy visible to the left of NGC 7098, known as ESO 048-G007
Astrid Giers, 1999 (photo)
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The End of Innocence, 2009 (Screen, projector and hard drive)
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Globular cluster 47 Toucan - The globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. At the top right of the image, part of the galaxy of the Little Magellan Cloud; under NGC 104, a small globular cluster, NGC 121. Discovered by Abbe Nicholas Louis de Lacaille on September 14, 1751. NGC 104, better known as 47 Tucanae, is the second largest and second brightest globular cluster in the skies, outshone only by another southern globular, Omega Centauri (NGC 5139). As its name “” 47 Tucanae”” indicates, this object was first cataloged as a star and numbered the 47th in Tucana. Although a conspicuous naked - eye object, it is situated so much south at its declination of - 72 deg, that it was not discovered as a deepsky object before 1751, when Abbe Lacaille cataloged it in his list of southern nebulous objects. Next to observe and catalog it were James Dunlop in 1826, and John Herschel in 1834. The stars of 47 Tucanae are spread over a volume almost 120 light years across. At their distance of 13,400 light years, they still cover an area of the sky of about the same apparent diameter as the full moon, about 30 minutes of arc. Globular cluster 47 Tucanae is approaching us at roughly 19 km/s. NGC104 has a tight core, making it difficult to resolve. The Small Magellanic Cloud (NGC292) can be seen just entering the field in the top right corner. A small globular cluster NGC121 is seen just “” below”” NGC104. This globular cluster actually belongs to the Small Magellanic Cloud, while NGC104 belongs to the Milky Way Galaxy. They just happen to line up conveniently
Old open cluster NGC 2818 and planetary nebula NGC 2818A - Old Open cluster NGC 2818 and planetary nebula in Pyxis - The open cluster NGC 2818 in the southern constellation of the Compsole is distinguished by the fact that most of its bright stars have already become supernovae; this indicates that this cluster must be very old, perhaps a billion years. It has a planetary nebula, NGC 2818A, a star at the end of life. These objects are located approximately 10,000 light years away from Earth. The open cluster NGC 2818 is not very conspicuous because most of the brilliant, massive stars that normally distinguish such groupings have vanished as supernovae, indicating that the cluster is quite mature. The massive stars dominating the scene in young clusters leaving the fainter, long - lived stars behind. Eventually, they too come to the end of their lives, throwing off their outer layers as planetary nebulae. This one, identified as NGC 2818A, is particularly graceful, and its existence suggests that the cluster to which it belongs is unusually old, at least a billion years. Most such clusters have lost their identity after a few hundred million years. The cluster and its planetary nebula are about 10,000 light years distant