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'Limb' Bilder und Clips Suchergebnisse page 8911 of 100

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Bilder zu 'Limb' gefunden, 8,941

 
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The Big picture: The Army's First - WWI And WWII Combat

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The Big picture: The Army's First - WWI And WWII Combat

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Huge Filaprom, 2015 (digital photo)

Corban, Gabriel Octavian (21st century)

MMM7340354

Huge Filaprom, 2015 (digital photo)

Corban, Gabriel Octavian (21st century)

MMM7340354

 
Earth's atmosphere and night clouds - Earth's atmosphere, noctilucent clouds and Moon - View of the Earth's atmosphere and a crescent moon photographs from the International Space Station on July 27, 2003. Night clouds are also visible. These clouds look like cirrus but are much higher, between 75 and 90 km from the Earth's surface. Noctilucent clouds are very high clouds that look like cirrus clouds, but are much higher (75 - 90 km above the Earth's surface) than clouds that we observe every day. They are optically thin and can only be observed during twilight hours, when the sun is just below the horizon and only shines on the uppermost atmosphere. In this image, the limb of the Earth at the bottom transitions into the orange - colored troposphere, the lowest and most dense portion of the Earth's atmosphere. The troposphere ends abruptly at the tropopause, which appears in the image as the sharp boundary between the orange - and blue - colored atmosphere. The silvery - blue noctiluce

PIX4675194

Earth's atmosphere and night clouds - Earth's atmosphere, noctilucent clouds and Moon - View of the Earth's atmosphere and a crescent moon photographs from the International Space Station on July 27, 2003. Night clouds are also visible. These clouds look like cirrus but are much higher, between 75 and 90 km from the Earth's surface. Noctilucent clouds are very high clouds that look like cirrus clouds, but are much higher (75 - 90 km above the Earth's surface) than clouds that we observe every day. They are optically thin and can only be observed during twilight hours, when the sun is just below the horizon and only shines on the uppermost atmosphere. In this image, the limb of the Earth at the bottom transitions into the orange - colored troposphere, the lowest and most dense portion of the Earth's atmosphere. The troposphere ends abruptly at the tropopause, which appears in the image as the sharp boundary between the orange - and blue - colored atmosphere. The silvery - blue noctiluce

PIX4675194

 
Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

PIX4625303

Saturn seen by the Cassin probe - Saturn seen by Cassini spacecraft on october 10 2013: Saturn seen by the Cassini probe on October 10, 2013. - A swing high above Saturn by Nasa's Cassini spacecraft revealed this stately view of the golden-hued planet and its main rings. The view is in natural color, as human eyes would have seen it. This mosaic was made from 36 images in three color filters obtained by Cassini's imaging science subsystem on Oct. 10, 2013 - A bright, narrow wave of clouds around 42 degrees north latitude appears to be some of the turbulent aftermath of a giant storm that reached its violent peak in early 2011. The mysterious six-sided weather pattern known as the hexagon is visible around Saturn's north pole - The rings shown here include Saturn's main rings. The rings known as the C, B and A rings - listed here in order of closeness to Saturn - are easily seen. The F ring is also there, but not easily seen without enhancing the contrast of the image. (Rings were named

PIX4625303

 
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Garden Centipede (Lithobius variegatus) (photo)

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Garden Centipede (Lithobius variegatus) (photo)

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Neptune - Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 14, 1989 at 14.8 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the right, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. This contrast enhanced color photograph of Neptune was produced from images taken through the orange, green, and violet filters of the narrow angle camera. As Voyager 2 approaches Neptune, rapidly increasing image resolution is revealing striking new details in the planet's atmosphere, and this picture shows features as small as a few hundred kilometers in extent. Bright, wispy “” cirrus - type”” clouds are seen overlying the Great Dark Spot (GDS) at its southern (lower) margin and over its northwest (upper left) boundary. This is the fi

PIX4622776

Neptune - Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 14, 1989 at 14.8 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the right, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. This contrast enhanced color photograph of Neptune was produced from images taken through the orange, green, and violet filters of the narrow angle camera. As Voyager 2 approaches Neptune, rapidly increasing image resolution is revealing striking new details in the planet's atmosphere, and this picture shows features as small as a few hundred kilometers in extent. Bright, wispy “” cirrus - type”” clouds are seen overlying the Great Dark Spot (GDS) at its southern (lower) margin and over its northwest (upper left) boundary. This is the fi

PIX4622776

 
Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

PIX4622787

Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

PIX4622787

 
Solar eruption seen by SOHO 02/04/2001 - Large solar flare seen by SOHO on april 2 2001 - Solar eruption seen by SOHO satellite; the Sun is masked by a coronographer. An image of the Sun taken at the same time by another satellite instrument was superimposed. A large solar flare occurred at 4:51 p.m. EDT, on Monday, April 2, 2001. as Observed by the Solar and Heliospheric Observatory (SOHO) satellite. Solar flares, among the solar systems mightiest eruptions, are tremendous explosions in the atmosphere of the Sun capable of releasing as much energy as a billion megatons of TNT. Caused by the sudden release of magnetic energy, in just a few seconds, solar flares can accelerate solar particles to very high velocities, almost to the speed of light, and heat solar material to tens of millions of degrees. The recent explosion from the active region near the sun's northwest limb hurled a coronal mass ejection into space at a whopping speed of roughly 7.2 million kilometers per hour. Luckily,

PIX4627092

Solar eruption seen by SOHO 02/04/2001 - Large solar flare seen by SOHO on april 2 2001 - Solar eruption seen by SOHO satellite; the Sun is masked by a coronographer. An image of the Sun taken at the same time by another satellite instrument was superimposed. A large solar flare occurred at 4:51 p.m. EDT, on Monday, April 2, 2001. as Observed by the Solar and Heliospheric Observatory (SOHO) satellite. Solar flares, among the solar systems mightiest eruptions, are tremendous explosions in the atmosphere of the Sun capable of releasing as much energy as a billion megatons of TNT. Caused by the sudden release of magnetic energy, in just a few seconds, solar flares can accelerate solar particles to very high velocities, almost to the speed of light, and heat solar material to tens of millions of degrees. The recent explosion from the active region near the sun's northwest limb hurled a coronal mass ejection into space at a whopping speed of roughly 7.2 million kilometers per hour. Luckily,

PIX4627092

 
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Magnified mosquito wing

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Magnified mosquito wing

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Booted Raquet-Tail (Ocreatus underwoodii) (photo)

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Booted Raquet-Tail (Ocreatus underwoodii) (photo)

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False whip scorpion (Amblypygi), view from above

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False whip scorpion (Amblypygi), view from above

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Longhorn beetle (Cerambycidae), front view (photo)

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Longhorn beetle (Cerambycidae), front view (photo)

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False Whip Scorpion (Amblypygi), close-up

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False Whip Scorpion (Amblypygi), close-up

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False Whip Scorpion (Amblypygi), close-up

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False Whip Scorpion (Amblypygi), close-up

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Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

PIX4624891

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

PIX4624891

 
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Longitudinal sections of the femur 1,2 and of the tibia 3. Copperplate engraving by Edward Mitchell after an anatomical illustration by Jean-Joseph Sue from John Barclay's A Series of Engravings of the Human Skeleton, MacLachlan and Stewart, Edinburgh, 1824.

FLO4565745

Longitudinal sections of the femur 1,2 and of the tibia 3. Copperplate engraving by Edward Mitchell after an anatomical illustration by Jean-Joseph Sue from John Barclay's A Series of Engravings of the Human Skeleton, MacLachlan and Stewart, Edinburgh, 1824.

FLO4565745

 
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Dissected Jewel beetle (Euchroma gigantea), view from above

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Dissected Jewel beetle (Euchroma gigantea), view from above

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Wing of male Antirrhea butterfly (Antirrhea philoctetes), close-up

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Wing of male Antirrhea butterfly (Antirrhea philoctetes), close-up

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Patte de Harfang des neiges, chouette harfang (Bubo scandiacus) - Snowy owl leg bones, femur, knee joint, tibiotarsus, trsometatarsus, toes and sharp talons, side view.-Photo by Philip Dowell, Courtesy of The Natural History Museum, London

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Patte de Harfang des neiges, chouette harfang (Bubo scandiacus) - Snowy owl leg bones, femur, knee joint, tibiotarsus, trsometatarsus, toes and sharp talons, side view.-Photo by Philip Dowell, Courtesy of The Natural History Museum, London

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Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

PIX4582251

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

PIX4582251

 
Earthrise and Moon seen since LRO. 10/2015 - Earthrise and Moon as seen from LRO. 10/2015 - Earthrise above the Moon seen from Lunar Reconnaissance Orbiter (LRO). Composite of images obtained on October 12, 2015. Nasa's Lunar Reconnaissance Orbiter (LRO) captured a unique view of Earth from the spacecraft's vantage point in orbit around the moon. In this composite image we see Earth appear to rise over the lunar horizon from the viewpoint of the spacecraft, with the center of the Earth just off the coast of Liberia (at 4.04 degrees North, 12.44 degrees West). The large tan area in the upper right is the Sahara Desert, and just beyond is Saudi Arabia. The Atlantic and Pacific coasts of South America are visible to the left. On the moon, we get a glimpse of the crater Compton, which is located just beyond the eastern limb of the moon, on the lunar farside. LRO was launched on June 18, 2009, and has collected a treasure trove of data with its seven powerful instruments, making an invaluab

PIX4577425

Earthrise and Moon seen since LRO. 10/2015 - Earthrise and Moon as seen from LRO. 10/2015 - Earthrise above the Moon seen from Lunar Reconnaissance Orbiter (LRO). Composite of images obtained on October 12, 2015. Nasa's Lunar Reconnaissance Orbiter (LRO) captured a unique view of Earth from the spacecraft's vantage point in orbit around the moon. In this composite image we see Earth appear to rise over the lunar horizon from the viewpoint of the spacecraft, with the center of the Earth just off the coast of Liberia (at 4.04 degrees North, 12.44 degrees West). The large tan area in the upper right is the Sahara Desert, and just beyond is Saudi Arabia. The Atlantic and Pacific coasts of South America are visible to the left. On the moon, we get a glimpse of the crater Compton, which is located just beyond the eastern limb of the moon, on the lunar farside. LRO was launched on June 18, 2009, and has collected a treasure trove of data with its seven powerful instruments, making an invaluab

PIX4577425

 
Saturn seen by the Cassini probe on 10 - 09 - 2007 - Saturn seen by Cassini spacecraft Sept. 10 2007. - Saturn seen by the Cassini probe on 10 - 09 - 2007 at a distance of 3.3 million km from the planet shortly before it flew over the Japet satellite. Mosaic of 45 images. Several satellites are visible in this image; from right to left: Titan, Tethys, Rhea, Mimas, Enceladus and Dione. While on final approach for its Sept. 2007 close encounter with Saturn's moon Iapetus, Cassini spun around to take in a sweeping view of the Saturn System. Iapetus (1,468 kilometers, or 912 miles across) is the only major moon of Saturn with a significant inclination to its orbit. From the other major satellites, the rings would appear almost edge - on, but from Iapetus, the rings usually appear at a tilt, as seen here. This natural color mosaic consists of 15 red, green and blue spectral filter images acquired in five wide - angle camera footprints that swept across the scene. Moons visible in this image

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Saturn seen by the Cassini probe on 10 - 09 - 2007 - Saturn seen by Cassini spacecraft Sept. 10 2007. - Saturn seen by the Cassini probe on 10 - 09 - 2007 at a distance of 3.3 million km from the planet shortly before it flew over the Japet satellite. Mosaic of 45 images. Several satellites are visible in this image; from right to left: Titan, Tethys, Rhea, Mimas, Enceladus and Dione. While on final approach for its Sept. 2007 close encounter with Saturn's moon Iapetus, Cassini spun around to take in a sweeping view of the Saturn System. Iapetus (1,468 kilometers, or 912 miles across) is the only major moon of Saturn with a significant inclination to its orbit. From the other major satellites, the rings would appear almost edge - on, but from Iapetus, the rings usually appear at a tilt, as seen here. This natural color mosaic consists of 15 red, green and blue spectral filter images acquired in five wide - angle camera footprints that swept across the scene. Moons visible in this image

PIX4625105

 
Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

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Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

PIX4625361

 
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Cats, lions, and a dragon, c.1517-18 (black chalk, pen & ink and wash on paper)

Vinci, Leonardo da (1452-1519)

ROC5907191

Cats, lions, and a dragon, c.1517-18 (black chalk, pen & ink and wash on paper)

Vinci, Leonardo da (1452-1519)

ROC5907191

 
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  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Pirate code or piratical articles. A list as drawn up by John Phillips, captain of the Revenge, who set a code for his men in 1724: I. Every Man Shall obey civil Command; the Captain shall have one full Share and a half of all Prizes; the Master, Carpenter, Boatswain and Gunner shall have one Share and quarter. II. If any Man shall offer to run away, or keep any Secret from the Company, he shall be marooned with one Bottle of Powder, one Bottle of Water, one small Arm, and Shot. III. If any Man shall steal any Thing in the Company, or game, to the Value of a Piece of Eight, he shall be marooned or shot. IV. If any time we shall meet another Marooner that Man shall sign his Articles without the Consent of our Company, shall suffer such Punishment as the Captain and Company shall think fit. V. That Man that shall strike another whilst these Articles are in force, shall receive Moses's Law (that is, 40 Stripes lacking one) on the bare Back. VI. That Man that shall snap his Arms, or smoke

BL3288596

Pirate code or piratical articles. A list as drawn up by John Phillips, captain of the Revenge, who set a code for his men in 1724: I. Every Man Shall obey civil Command; the Captain shall have one full Share and a half of all Prizes; the Master, Carpenter, Boatswain and Gunner shall have one Share and quarter. II. If any Man shall offer to run away, or keep any Secret from the Company, he shall be marooned with one Bottle of Powder, one Bottle of Water, one small Arm, and Shot. III. If any Man shall steal any Thing in the Company, or game, to the Value of a Piece of Eight, he shall be marooned or shot. IV. If any time we shall meet another Marooner that Man shall sign his Articles without the Consent of our Company, shall suffer such Punishment as the Captain and Company shall think fit. V. That Man that shall strike another whilst these Articles are in force, shall receive Moses's Law (that is, 40 Stripes lacking one) on the bare Back. VI. That Man that shall snap his Arms, or smoke

BL3288596

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