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'Fuzzy' Bilder und Clips Suchergebnisse page 1 of 1

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Girl with Fuzzy Hair, 2004 (etching)
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Werner fuzzy
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Girl with Fuzzy Hair Sitting, 2004 (c-type photo)
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1960s: Fuzzy caterpillar on a leaf.
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1960s: Fuzzy caterpillar sitting on a leaf.
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1960s: Five fuzzy ducklings swim on water.
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Fuzzy silhouette with hood looking through a glass (departure, farewell, regret).
FUZZY ZOELLER FANS HIMSELF WITH WAD OF CASH, 1999-04-07 (photo)
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FUZZY ZOELLER AND JOHN DALY DURING PRACTICE DAY, 1997-06-11 (photo)
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Low angle view of a koala sitting on a branch (b/w photo)
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FUZZY ZOELLER HITS OUT OF SAND TRAP ON SECOND HOLE AT MASTERS, 2000-04-06 (photo)
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A nocturnal view of Chittagong city in Bangladesh. May 5, 2010.  (photo)
FUZZY ZOELLER EXCHANGES HIGH FIVE WITH FAN DURING MASTERS PRACTICE
ROUND, 2002-04-10 (photo)
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GORE RUBS FUZZY TV MICROPHONE ON BABYS FACE IN NEW HAMPSHIRE DINER, 2000-01-06 (photo)
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A nocturnal view of Chittagong city in Bangladesh. May 5, 2010.  (photo)
Lamb's Ear, c.1965 (silver gelatin print)
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Teracotona euprepia, veined tiger, mounted female moth with pale forewings with brown veins and a fuzzy red thorax and pink orange hindwings
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N.B.C.'s ARMY HOUR, Greer Garson, Humphrey Bogart with the Fuzzy Wuzzy Award which was the GI version of the Oscar presented to them, 1944
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The leaders attending the Economic summit in Toronto sit around the table. Mulroney and Reagan are turned and looking at the camera, everyone else is fuzzy, 1988-06-19 (photo)
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Fuzzy still photo form a Pepsi commercial shown on Soviet TV. Pepsi is written in Russian inside the familiar logo and beside the logo it says The new generation chooses Pepsi, 1988-05-18 (photo)
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Oct. 10, 1953 - McCarthy loses at last beaten by Nigerian at Royal Albert hall.: Smiling Sammy McCarthy, chosen contender for the British featherweight title, had his unbeaten certificate taken from his last night at the Royal Albert Hall by fuzzy-haired Nigerian Hogan Bassy
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Two Pounds Of Pomeranian (b/w photo)
Family members of fromer president CHiang Ching-kuo kneel in front of his coffin in Taipei. Facing camera (very fuzzy) are, l-r, his son Chiang Hsiao-wu, brother Chiang Wei-kuo, son Chiang Hsiao-yung.  January 22, 1988 REUTERS/C, 1988-01-22 (photo)
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Comparison of Sun and Betelgeuse sizes - Size comparison: Betelgeuse and Sun - Betelgeuse star is a supergeant red star in the constellation Orion. It's one of the biggest stars known. It appears on this illustration at the scale next to the Sun (at the top). Betelgeuse is a red giant, one of the largest stars known. It forms the left shoulder of the constellation Orion. If Betelgeuse was placed at the center of our solar system, its fuzzy edge would extent out well beyond the orbit of Mars
Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf
Boats and Bay, Los Angeles Bay, Baja California, 1964 (silver gelatin print)
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Cactus, Baja, California, c. 1940 (silver gelatin print)
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Autumn lactee route - Pointe du Raz - Autumn Milky way - Pointe du Raz - The lactee route above Notre Dame des Shipwrecks, Pointe du Raz. Brittany, 27 September 2008. Milky Way above the statue dedicated to “” Our Lady of the Shipwrecks”””. The zodiacal band is visible under the aspect of a fuzzy and pale band extending from the top of the statue to the upper right. A the top of the picture is the powerful lighthouse of the Sein Island. at Pointe du Raz, the western tip of France. Brittany, 27 September 2008
Autumn lactee route - Pointe du Raz - Autumn Milky way - Pointe du Raz - The lactee route above Notre Dame des Shipwrecks, Pointe du Raz. Brittany, 27 September 2008. Milky Way above the statue dedicated to “” Our Lady of the Shipwrecks”””. The zodiacal band is visible under the aspect of a fuzzy and pale band extending from the top of the statue to the upper right. A the top of the picture is the powerful lighthouse of the Sein Island. at Pointe du Raz, the western tip of France. Brittany, 27 September 2008
Insect: variete of coleoptere staphylinus with a fragrant fuzzy plant or fragrant quackgrass Lithograph by John Curtis (1791-1862) published in “” British Entomology”, collection of 770 illustrations and descriptions of insects from Great Britain, London, England, 1824-1839. Homalota dimidiata, Hygronoma dimidiata, Ochre-banded Staphylinus beetle, with spring grass, Anthoxanthum odoratum. Handcoloured copperplate by John Curtis (1791-1862) for his own “” British Entomology, 770 Illustrations and Descriptions of the Genera of Insects found in Great Britain and Ireland,” London, from 1824 to 1839.
Keenan Wynn, Jane Russell, Ralph Meeker, (on set), 1957 (b/w photo)
The Black Lash, 1952 (print)
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A young woman leaving behind her the images of forgotten men, Italy
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Open cluster M47 in Puppis - Open star cluster M47 in Puppis - M47 (NGC 2422) is a cluster located about 1600 years ago - light that contains about fifty stars. M47 (NGC 2422) is an open cluster in the constellation Puppis, and was known to several observers before being independently discovered by Messier. A coarse bright cluster of some 50 stars, it can be seen by the suitably primed naked eye at a good dark location, as a dim fuzzy spot. About 1600 light - years away, it is spread over an area about that of the full moon (30 arc minutes across), or some 14 light - years linearly
SEA SPOILERS 1936 (film still)
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THE LAST ROUND-UP 1934 (film still)
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TENNIS PIN-UP 1950S
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ZOELLER CELEBRATES SINKING PUTT AT MASTERS, 1998-04-10 (photo)
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Pet shop clerk Hiroko Nagayama holds a pair of rabbits in front of the shop in Tokyo February 9. An .., 1999-02-09 (photo)
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A PET SHOP CLERK HOLDS A PAIR OF RABBITS IN TOKYO, 1999-02-09 (photo)
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Saint Gotthard
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La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne, crossing the Milky Way. Brittany, 27 September 2008
GOLFER DALY TEES OFF AT THE SHARK SHOOTOUT, 1998-11-13 (photo)
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ZOELLER WATCHES TEE SHOT AT TRADITION, 2003-08-28 (photo)
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Hadendoa  Man - Standing on one leg
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Sudan - A group of Hadendoa Warriors
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Former Miss Universe Irene Saez outlines a pro-market, social-minded presidential platform to rid he.., 1998-09-29 (photo)
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La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne, crossing the Milky Way. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. Brittany, 27 September 2008
Sudan - A group of Hadendoa Warriors
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FRED FUNK TEES OFF ON THE 10TH HOLE AT AVENEL, 1998-06-04 (photo)
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THORPE WATCHES TEE SHOT AT TRADITION IN NORTH PLAINS, 2003-08-28 (photo)
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M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is located about 60 million years ago - light from Earth, in the heart of the Virgin's cluster. M87 is the brightest radio source in the constellation, it is also called Virgo A. Image made with Siding Spring's 3.9m telescope. Messier 87 (NGC 4486) lies near the centre of the nearby cluster of galaxies in Virgo at a distance of about 60 million light years. Although the physical boundaries of elliptical galaxies are not well defined, their mass can be, and by any standards M87 is enormous. It contains several thousand billion stars. Associated with this giant galaxy are large numbers of globular clusters, visible in this photograph as the cloud of slightly fuzzy objects around it. Like all ellipticals, M 87 is composed mainly of old stars and is largely devoid of the materials needed to make new ones. The galaxy is not inert however; high energy X - rays have been detected from an extensive outer halo and the galaxy itself is also known as Virgo A, the strongest radio source in the Virgo cluster. The source for this extreme behavior is probably a massive black hole at the center of the galaxy
SAEZ OUTLINES HER PRESIDENTIAL PLATFORM, 1998-09-29 (photo)
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Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in Taurus. However, the Tropic of Cancer is still so names, and is the line of latitude around the northern hemisphere where the Sun is directly overhead at local noon on the day of the summer solstice
Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in Taurus. However, the Tropic of Cancer is still so names, and is the line of latitude around the northern hemisphere where the Sun is directly overhead at local noon on the day of the summer solstice
Third Reich - BDM camp 1938 (photo)
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Self-portrait at the age of 22 (after Rembrandt)
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Galaxy cluster Abell 1689 - Gravitational lenses in Abell 1689 galaxy cluster - Galaxy cluster Abell 1689 is about 2.2 billion years ago - light in the constellation of the Virgin. This image shows, by a gravitational mirage effect, the deformed image of many galaxies located behind the cluster. Near infrared and visible image obtained by the Hubble space telescope. 34 hours of installation. This new Hubble image shows galaxy cluster Abell 1689. It combines both visible and infrared data from Hubble's Advanced Camera for Surveys (ACS) with a combined exposure time of over 34 hours (image on left over 13 hours, image on right over 20 hours) to reveal this patch of sky in greater and striking detail than in previous observations. This image is peppered with glowing golden clumps, bright stars, and distant, ethereal spiral galaxies. Material from some of these galaxies is being stripped away, giving the impression that the galaxy is dripping, or bleeding, into the surrounding space. Also visible are a number of electric blue streaks, circling and arcing around the fuzzy galaxies in the centre. These streaks are the telltale signs of a cosmic phenomenon known as gravitational lensing. Abell 1689 is so massive that it bends and warps the space around it, affecting how light from objects behind the cluster travels through space. These streaks are the distorted forms of galaxies that lie behind the cluster
Barree spiral galaxy NGC 4394 in Berenice's Hair - Barred spiral galaxy NGC 4394 in Coma Berenices: NGC 4394 is a barree spiral galaxy located in the Virgin's cluster about 55 million light years from Earth. Image obtained by the Hubble Space Telescope (HST) - Discovered in 1784 by the German-British astronomer William Herschel, NGC 4394 is a barred spiral galaxy situated about 55 million light-years from Earth. The galaxy lies in the constellation of Coma Berenices (Berenice's Hair), and is considered to be a member of the Virgo Cluster. NGC 4394 is the archetypal barred spiral galaxy, with bright spiral arms emerging from the ends of a bar that cuts through the galaxy's central bulge. These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the centre of NGC 4394 lies a region of ionised gas known as a LINER. Liners are active regions that display a characteristic set of emission lines in their spectra- mostly weakly ionised atoms of oxygen, nitrogen and sulphur. Although LINER galaxies are relatively common, it's still unclear where the energy comes from to ionise the gas. In most cases it is thought to be the influence of a black hole at the centre of the galaxy, but it could also be the result of a high level of star formation. In the case of NGC 4394, it is likely that gravitational interaction with a nearby neighbour has caused gas to flow into the galaxy's central region, providing a new reservoir of material to fuel the black hole or to make new stars
Sunrise - 22 June 2005. - Full moon rising - June 22 - Sunrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevation. Firstly very fuzzy (because of the atmospheric turbulence very strong near the horizon), flatten (because of the atmospheric refraction), dark and red (because of the thicker atmosphere near the horizon), it brightens slowly, get more yellow, as it takes its round shape. That day, many hours were necessary for the Moon to became white. Each picture from this composite had been taken 5 minutes after the previous one. June 22, 2005
Sunrise - 22 June 2005. - Full moon rising - June 22, 2005 - Moonrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevation. Firstly very fuzzy (because of the atmospheric turbulence very strong near the horizon), flatten (because of the atmospheric refraction), dark and red (because of the thicker atmosphere near the horizon), it brightens slowly, get more yellow, as it takes its round shape. That day, many hours were necessary for the Moon to became white. Each picture from this composite had been taken 5 minutes after the previous one. June 22, 2005
Sunrise - 22 June 2005. - Full moon rising - June 22 - Sunrise one day after the summer solstice. The Moon rises very south and remains low in the sky (like the Sun in winter) thus taking longer than usual to rise. It is dark red when it appears discreetly above the sea. At first very blurred (due to the very strong atmospheric turbulence near the horizon), flattened (due to the atmospheric refraction), dark and red (due to the thicker atmosphere near the horizon), it gradually illuminates and yellows, while it regains its very round shape. That day, it will take several hours for her to turn white again. Each image of this montage was taken five minutes after the previous one. June 22, 2005. Full moon is rising on June 22, one day after the summer solstice, so the Moon is rising far to the South. Moreover, it stays low above the horizon (like the Sun in winter) and takes more time than usually to rise. It is dark - red when it appears above the sea, at just one degree of elevation. Firstly very fuzzy (because of the atmospheric turbulence very strong near the horizon), flatten (because of the atmospheric refraction), dark and red (because of the thicker atmosphere near the horizon), it brightens slowly, get more yellow, as it takes its round shape. That day, many hours were necessary for the Moon to became white. Each picture from this composite had been taken 5 minutes after the previous one. June 22, 2005
Spiral galaxy NGC 406 in Toucan - Spiral galaxy NGC 406 in Tucana - NGC 406 is a spiral galaxy located at a distance of about 65 million light years in the southern constellation of Toucan. Image obtained by the Hubble Space Telescope. The spiral galaxy NGC 406 was discovered in 1834 by John Herschel and is here imaged in great detail by the NASA/ESA Hubble Space Telescope. Located some 65 million light - years away, in the southern constellation of Tucana (the Toucan), NGC 406 is about 60 000 light - years across, roughly half the diameter of our galaxy, the Milky Way. In a moderate - sized amateur telescope NGC 406 would appear as a faint hazy blob, like thousands of others across the sky, and none of the spectacular fine detail in the Hubble picture could be made out. In this image the galaxy exhibits spiral arms that are mainly populated by young, massive, bluish stars and crossed by dark dust lanes. As is typically observed in this kind of spiral galaxy, the yellowish central bulge, dominated by an older stellar population, is less prominent and almost totally embedded in the disk structure. The deep image also shows a significant number of more distant galaxies in the background. Some of them are visible as reddish fuzzy spots through the bluish spiral arms of the foreground galaxy. This picture was created from images taken through near - infrared (F814W) and blue (F435W) filters, shown in red and blue respectively, using the Wide Field Channel of Hubble's Advanced Camera for Surveys. The exposure times were twenty minutes per filter and the field of view is 2.7 by 1.6 arcminutes
Double star Gliese 623 - Double star system Gliese 623 in Hercules - Gliese 623 is a double star located about 25 years ago - light in the constellation Hercules. The Hubble space telescope was able for the first time to obtain an image of the two stars that make up this system, in June 1994. The two stars are separated by about twice the distance from Earth to Sun. On the right, 623b, a star 60,000 times less bright than the Sun, and 10 times less massive. Its nature is misidentified, it's a red dwarf or a brown dwarf. A dim double star system cataloged as Gliese 623 lies 25 light - years from Earth, in the constellation of Hercules. The individual stars of this binary system were distinguished for the first time when the Hubble Space Telescope's Faint Object Camera recorded this image in June 1994. They are separated by 200 million miles - about twice the Earth/Sun distance. On the right, the fainter Gliese 623b is 60,000 times less luminous than the Sun and approximately 10 times less massive. The fuzzy rings around its brighter companion, Gliese 623a, are image artifacts. The lowest mass stars are classified as red dwarf stars, but even red dwarfs are massive enough to trigger hydrogen fusion in their cores to sustain their feeble starlight. Slightly less massive objects, known as brown dwarfs, can shine only briefly as their central temperatures are too low to utilize hydrogen as nuclear fuel. The present estimates of the mass of Gliese 623b are right at this red dwarf/brown dwarf border but future observations should help clarify the nature of one of our Galaxy's small stars. Dim and difficult to detect, an abundance of objects like GL623b has been proposed as a possible solution to the mystery of “” Dark Matter”” in the Universe
Detail of the Eagle Nebula (M16) dans le serpent/HST - This eerie, dark structure, resembling an imaginary sea serpent's head, is a column of cool molecular hydrogen gas (two atoms of hydrogen in each molecule) and dust that is an incubator for new stars. The stars are embedded inside finger - like protrusions extending from the top of the nebula. Each “” fingertip”” is somewhat larger than our own solar system. The pillar is slowly eroding away by the ultraviolet light from nearby hot stars, a process called “” photoevaporation””. As it does, small globules of especially dense gas buried within the cloud is uncovered. These globules have been dubbed “” Eggs”” - - an acronym for “” Evaporating Gaseous Globules””. The shadows of the Eggs protect gas behind them, resulting in the finger - like structures at the top of the cloud. Forming inside at least some of the Eggs are embryonic stars - - stars that abruptly stop growing when the Eggs are uncovered and they are separated from the larger reservoir of gas from which they were drawing mass. Eventually the stars emerge, as the Eggs themselves succumb to photoevaporation. The stellar EGGS are found, appropriately enough, in the “” Eagle Nebula”” (also called M16 - - the 16th object in Charles Messier's 18th century catalog of “” fuzzy”” permanent objects in the sky), a nearby star - forming region 6,500 light - years away in the constellation Serpens. The picture was taken on April 1, 1995 with the Hubble Space Telescope Wide Field and Planetary Camera 2. The color image is constructed from three separate images taken in the light of emission from different types of atoms. Red shows emission from singly - ionized sulfur atoms. Green shows emission from hydrogen. Blue shows light emitted by doubly - ionized oxygen atoms
The Eagle Nebula, 1995
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Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated by newborn, massive stars. Andromeda is the closest large galaxy to our Milky Way galaxy, and is located 2.5 million light - years from our sun. It is close enough for telescopes to spy the details of its ringed arms of new stars and hazy blue backbone of older stars. Also seen in the mosaic are two satellite galaxies, known as M32, located just a bit above Andromeda to the left of center, and the fuzzy blue M110, located below the center of the great spiral arms. These satellites are the largest of several that are gravitationally bound to Andromeda. The Andromeda galaxy is larger than our Milky Way and contains more stars, but the Milky Way is thought to perhaps have more mass due to its larger proportion of a mysterious substance called dark matter. Both galaxies belong to our so - called Local Group, a collection of more than 50 galaxies, most of which are tiny dwarf systems. In its quest to map the wh
Quince Fruit on Branch (litho)
Grey squirrel side on crouched over nuts
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Front view of Tarantula
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Side view of a Red Kneed Tarantula
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Red Kneed Tarantula (Brachypelma smithi)
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Bust of a Bishareen or Bisharee woman. Ethiopian Race. From a drawing, taken at the Third Cataract of the Nile, by E. Prisse. Handcoloured steel engraving from Charles Pickering's The Races of Man, London, 1850.
Fuzzles visits the Doctor (colour litho)
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