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'Lenticular' Bilder und Clips Suchergebnisse page 1 of 1

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Bilder zu 'Lenticular' gefunden, 66

Lenticular clouds - Lenticular clouds - Lenticular clouds above the highest peaks of the Reunio
Lenticular clouds - Lenticular clouds - Lenticular clouds above the highest peaks of the Reunio
LENTICULAR CLOUDS
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Spiral galaxy NGC 536 in Andromede - Hickson 10 group of galaxies in Andromeda - Spiral galaxy NGC 536 (in the center of the picture). With the galaxies NGC 542 (below left), NGC 531 (above NGC 536) and the lenticular galaxy NGC 529 (right), it forms the galaxy group Hickson 10, located about 220 million light years from Earth. This group of four galaxies is around 220 million light years away. The collection of spiral galaxies in the center of the image include: (from top to bottom) NGC 531, NGC 536 and NGC 542. NGC 529 on the right side of the image is a bright lenticular galaxy
Heartbeat 1, 2015, (lenticular print),
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Group of galaxies HCG 61 in Berenice's Hair - Hickson 61 - The Box - The group of galaxies HCG 61 (Hickson 61, the box) consists of three interacting galaxies, and one forward galaxy (NGC 4173, the largest in the image) that is not physically associated. From the top and then clockwise, we find the spiral galaxy NGC 4173, the lenticular galaxy NGC 4169, and the spiral galaxies NGC 4174 and NGC 4175. Hickson 61 (HCG 61) is a group of four galaxies located in Coma Berenices. In foreground is NGC 4173 (top left, the largest spiral galaxy) which is closer than the three other galaxies and not associated to them. At right is the brightest galaxy, NGC 4169, a lenticular galaxy. Bottom right is the spiral galaxy NGC 4174 and bottom left, NGC 4175
Lenticular Galaxy M102 (NGC 5866) in the Dragon - Lenticular galaxy M102 (NGC 5866) in Drac
Lenticular galaxy NGC 4710 in Berenice's Hair - Lenticular galaxy NGC 4710 in Coma Berenices - The galaxy NGC 4710 is located about 60 million years ago - light from Earth, in the galaxy cluster of Our Lady. It's a lenticular galaxy seen from the slice. Image obtained by the Hubble Space Telescope. Edge - on galaxy located at about 60 million light years away. NGC 4710 is a member of the giant Virgo Cluster of galaxies and lies in the northern constellation of Coma Berenices (the Hair of Queen Berenice). It is not one of the brightest members of the cluster, but can easily be seen as a dim elongated smudge on a dark night with a medium - sized amateur telescope. In the 1780s, William Herschel discovered the galaxy and noted it simply as a “” faint nebula””. It is an example of a lenticular or S0 - type galaxy - a type that seems to have some characteristics of both spiral and elliptical galaxies. Image taken by the Hubble Space Telescope
Lenticular Galaxy M102 (NGC 5866) in the Dragon - Edge - on view of M102 (NGC 5866) in Draco - This galaxy from the slice is located 44 million years - light from Earth. Its diameter is 60,000 years - light. Image obtained by the ACS camera of the Hubble space telescope in February 2006. The lenticular galaxy NGC 5866 is about 44 million light - years from Earth in the Northern constellation Draco. Its diameter is approximately 60,000 light - years, two - thirds the diameter of the Milky Way, and its mass is similar to our galaxy. Hubble image taken with the Advanced Camera for Surveys in February 2006
Heartbeat 2, 2015, (lenticular print)
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Transition 3, 2015, (lenticular print)
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Transition 1, 2015, (lenticular print)
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Transition 4, 2015, (lenticular print)
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Lenticular clouds over mountains (photo)
Barree spiral galaxy NGC 6872 in interaction with IC 4970 in the Peacock - Barred spiral interacting galaxy NGC 6872 in Pavo - The barree spiral galaxy NGC 6872 and lenticular IC 4970 are located about 300 million years away - light from Earth. NGC 6872 extends over nearly 750,000 years - light. Image obtained by the ANTU telescope of the VLT on March 29, 1999. View of the spectacular barred spiral galaxy NGC 6872 obtained with FORS1 at ANTU telescope (VLT) in the morning of March 29, 1999. It is of type SBB and is accompanied by a smaller, interacting galaxy, IC 4970 of type S0 (just above the centre). The bright object to the lower right of the galaxies is a star in the Milky Way whose image has been strongly overexposed and exhibits multiple optical reflections in the telescope and instrument. There are also many other, fainter and more distant galaxies of many different forms in the field. The upper left spiral arm of NGC 6872 is significantly disturbed and is populated by a plethora of blueish objects, many of which are star - forming regions. This may have been caused by a recent passage of IC 4970 through it. This interesting system is located in the southern constellation Pavo (The Peacock). It is comparatively distant, almost 300 million light - years away. It extends over more than 7 arcmin in the sky and its real size from tip to tip is thus almost 750,000 light - years. It is in fact one of the largest known, barred spiral galaxies
Transition 2, 2015, (lenticular print)
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Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image made with Siding Spring's 3.9m telescope. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 80 million light years distant
Dimensional Triptych, 2013 (motion lenticular)
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Heartbeat 3, 2015, (lenticular print)
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Peculiar brown actively moving lenticular bodies.
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Central part of the Virgin galaxy cluster - Heart of the Virgo cluster of galaxies - The two elliptic galaxies are at the center M86 (NGC 4406), right M84 (NGC 4374). Image obtained with a 130 mm bezel. 1h pose M86 and M84 are two giant lenticular galaxies at the heart of the Virgo cluster of galaxies. NGC 4438, a spiral galaxy at the left of the photo, appears to be distorted by an interaction with nearby NGC 4435. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe
Ideal Boys, Francesco, 1997 (3D Lenticular transparency, lightbox)
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Central part of the Virgin galaxy cluster - Heart of the Virgo cluster of galaxies - The Virgin cluster contains about 2000 galaxies. The two elliptical galaxies are: at the center, M86 (NGC 4406), and M84 (NGC 4374), at the top. M86 and M84 are two giant lenticular galaxies at the heart of the Virgo cluster of galaxies. NGC 4438, a spiral galaxy at the bottom left of the photo, appears to be distorted by an interaction with nearby NGC 4435. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe
Central part of the Virgin galaxy cluster - Heart of the Virgo cluster of galaxies - On the right are the M84 (NGC 4374) and M86 (NGC 4406) (to its left). Lower left is the elliptical galaxy M87. The Virgin's cluster is located about 70 million light years away from Earth and contains nearly 2000 galaxies. This photo shows the heart of the Virgo cluster of galaxies. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. It is the center of our local supercluster of galaxies which includes members of our local group, the Milky Way (our own galaxy), M31, M32, M110, M33, the Magellanic clouds, and others. Markarian's Chain of galaxies is to the upper right, including giant elliptical galaxies M86 and M84. M87 is another giant elliptical galaxy at lower left in the photo. Also called Virgo A, this galaxy contains nearly 3 trillion solar masses. It lies at a distance of 60 million light years and may be as large, physically, in space, as 1/2 million light years in diameter
Photograph of Lenticular clouds over the South Georgia Island
Central part of the Virgo cluster of galaxies - Central part of the Virgo cluster of galaxies - On the left the M84 (NGC 4374) and M86 (NGC 4406) (to its right) dominate the image. To the right is the elliptical galaxy M87. The Virgin's cluster is located about 70 million light years away from Earth and contains nearly 2000 galaxies. Galaxies M84 (NGC 4374) and M86 (NGC 4406), upper left corner of this image and the elliptical galaxy M87, center right. The Virgo cluster is at about 70 million light years from Earth and contains approximately 2000 galaxies
Central part of the Virgo cluster - Central part of the Virgo cluster - The Virgin cluster contains several thousand galaxies. It is located about 70 million light years from Earth. To the right are the galaxies M84 (NGC 4374) and M86 (NGC 4406) (to the left) dominate the image. Lower left is the elliptical galaxy M87. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. Markarian's Chain of galaxies is in the center, including giant elliptical galaxies M86 and M84. M87 is another giant elliptical galaxy at lower left in the photo
Ideal Boys, Roberto, 1997 (3D Lenticular transparency, lightbox)
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Central part of the Virgo cluster of galaxies - Central part of the Virgo cluster of galaxies - On the right the M84 (NGC 4374) and M86 (NGC 4406) (to its left) dominate the image. Lower left is the elliptical galaxy M87. The nearest moderately rich cluster of galaxies lies in the direction of Virgo. The richest part of the cluster is centred on the giant elliptical - lenticular galaxies M84 (NGC 4374) (right) and M86 (NGC 4406) (left) which dominate this picture. However, the dynamical centre of the cluster is M87, to the lower left (south east) of this picture
Ideal Boys, Johnluca and Paco, 1997 (3D Lenticular transparency, lightbox)
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Burnt Almonds, Rudolph & Gisela, 2000 (3D Lenticular transparency, steel, lightbox)
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Burnt Almonds, Wilhelm & Ingrid, 2000 (3D Lenticular transparency, steel, lightbox)
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The Virgo cluster of galaxies - The Virgo cluster of galaxies - The Virgin cluster contains about 2000 galaxies. In the middle of the picture, the giant elliptical galaxy M87. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Image of the central portion of the great Virgo/Coma cluster including Markarians chain. Located about 70 million light years away, The Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. Image taken with the Palomar Observatory 48 - inch Schmidt telescope as part of the Digitized Sky Survey
Chalcosine (photo)
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Lenticular clouds hovering above snowy mountain peaks under calm twilight sky scenery.
Burnt Almonds, Heinrich & Eva, 2000 (3D Lenticular transparency, steel, lightbox)
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Burnt Almonds, Gustav & Helga, 2000 (3D Lenticular transparency, steel, lightbox)
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Burnt Almonds, Georg & Rosa, 2000 (3D Lenticular transparency, steel, lightbox)
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Time lapse of lenticular clouds and a mountain pasture landscape, Emilia Romagna, Italy, Europe
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Lenticular clouds hovering above snowy mountain peaks under calm twilight sky scenery.
General perspective of the Royal Albert Bridge looking across the River Tamar, Saltash, Cornwall, 1954 (b/w photo)
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Lenticular flask by the Pilgrim Flask Painter, side depicting two komasts and a brazier. Etrusco-Corinthian pottery from Cerveteri (Lazio). Etruscan civilization, 7th Century BC.
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Altocumulus clouds over mountain, Mount Rainier, Mount Rainier National Park, Washington, USA
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Surgical trepanning instruments including spring forceps, Savigny's trephines, scalpel, elevator, Mr. Hey's saws, lenticular, raspatory, brush, and trephine from the 19th century. Copperplate engraving by Wilson Lowry after an illustration by J. Farey from Abraham Rees' “” Cyclopedia or Universal Dictionary,” London, 1819.
Virgo constellation nebula, illustration
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Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, on its left, is probably interacting with it. Image obtained with a 35 cm telescope, 6 hours of poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The galaxies are about 95 million light years distant. Image taken with 14.5”” RCOS telescope, 6 Hours of exposure
Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image obtained with a 50 cm telescope, composite of several poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 95 million light years distant
Galaxy NGC 4650A in Centaurus - Galaxy NGC 4650A in Centaurus - The polar ring galaxy NGC 4650A is located about 130 million years away from Earth. The host galaxy is surrounded by a polar ring shaped like gas and stars. This type of galaxy is rarely observed. This image was obtained by the ANTU telescope of the VLT in 1998. This is a colour photo from the VLT that shows NGC 4650A, a member of the so - called Centaurus chain of galaxies in the southern constellation of that name. NGC 4650A is a complex system that is located at a distance of about 130 million light - years. There are two main components, a lenticular - shaped galaxy (of type S0), surrounded by a knotty extended ring - like distribution of stars, dust and gas, almost perpendicular to each other. The stars in the central, structureless region and the material (stars, gas, and dust) in the outer disk rotate in two different planes that are almost perpendicular to each other. The observed motions indicate the presence of a significant halo of dark matter within the system, although it is still unclear to which of the two components this matter belongs. Because the velocities of stars and gas can be measured in two independent planes, NGC 4650A serves as a prototype for detailed studies of the shape of dark matter halos. The origin of this strange spatial configuration is not known with certainty. It is likely, however, that an encounter between two galaxies may have played a significant role. The photo is based on a series of seven exposures through three different optical filters, obtained under mediocre observing conditions during a small break in the technical work. They have been combined to produce the present photo
Advertisement for Kodacolor cine film (Kodak), 1929 Advertisement for Kodacolor cine film, 1929
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Central part of the Virgo cluster of galaxies - The Virgin's cluster contains several thousand galaxies. It is located about 70 million light years away from Earth. To the right are the galaxies M84 (NGC 4374) and M86 (NGC 4406) (to the left) dominate the image. Lower left is the elliptical galaxy M87. Located about 70 million light years away, the Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. Markarian's Chain of galaxies is in the center, including giant elliptical galaxies M86 and M84. M87 is another giant elliptical galaxy at lower left in the photo