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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Nov. 11, 1954 - Introducing the” Albatross” - New All-British motor scooter. Does over 80 m.p. Gallon. : The” Albatross” - new All-British motor scooter - the first to compete with the Continental designs has put in its appearance and will be shown to the public for the first time at the Cycle and Motor Cycle Show next week. Built by the Dayton Cycle Company of Park Royal, London - the machine is an ideal runabout and is also a comfortable long-distance two-seat tourer. Powered by a 225 c.c Villiers two - stroke engine it can cruise all day at 55 - 60 m.p.h. has a top speed of over 65 m.p.h. and patrol consumption of more than 80 m.p. gallon. It is fitted with a car-type facia panel complete with speedometer; ammeter; key-operate ignition switch; separate lighting switch and choke control knot - and aldo has a big 7” headlamp. The” Albatross” has almost twice the speed and power plus most of the” extras” of its Italian and German competitors and is priced at KSA95501 182 - 12 - Od. inc

ZUM4944897

Nov. 11, 1954 - Introducing the” Albatross” - New All-British motor scooter. Does over 80 m.p. Gallon. : The” Albatross” - new All-British motor scooter - the first to compete with the Continental designs has put in its appearance and will be shown to the public for the first time at the Cycle and Motor Cycle Show next week. Built by the Dayton Cycle Company of Park Royal, London - the machine is an ideal runabout and is also a comfortable long-distance two-seat tourer. Powered by a 225 c.c Villiers two - stroke engine it can cruise all day at 55 - 60 m.p.h. has a top speed of over 65 m.p.h. and patrol consumption of more than 80 m.p. gallon. It is fitted with a car-type facia panel complete with speedometer; ammeter; key-operate ignition switch; separate lighting switch and choke control knot - and aldo has a big 7” headlamp. The” Albatross” has almost twice the speed and power plus most of the” extras” of its Italian and German competitors and is priced at KSA95501 182 - 12 - Od. inc

ZUM4944897

 
Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

PIX4625061

Saturn rings seen in ultraviolet by Cassini - Saturn's rings in utraviolet - Saturn rings seen in ultraviolet by the Cassini probe. The colours indicate a different distribution of the material within the rings. This false - color image of Saturn's main rings was made by combining data from multiple star occultations using the Cassini ultraviolet imaging spectrograph. During occultations, scientists observe the brightness of a star as the rings pass in front of the star. This provides a measurement of the amount of ring material between the spacecraft and the star. Cassini has given scientists the most detailed view yet of Saturn's densely packed B ring. Cassini found that this part of the rings is densely packed with clumps, called self - gravity wakes, separated by almost empty gaps. These clumps in Saturn's B ring are neatly organized and constantly colliding, which surprised scientists. The clumps in Saturn's B ring, 30 to 50 meters (100 to 160 feet) across, are too small to be see

PIX4625061

 
Chandra Space Telescope - Artist View - Chandra X - Ray Observatory - View of the Chandra Telescope in orbit around Earth. The Chandra space telescope observes the universe in X-ray; it was launched and put into orbit in July 1999. Nasa's Chandra X - ray Observatory as it may appear at about 50,000 miles from the Earth, almost twice as high as Earth - orbiting geosynchronous satellites. Named after the Indian astrophysicist Subrahmanyan Chandrasekhar, the Chandra X - ray Observatory is the world's most powerful X - ray telescope, and at a weight of over 5 tons (10 tons including the detachable booster rocket) was the heaviest payload ever delivered into orbit by the Space Shuttle. Chandra was carried into space by Columbia in July 1999. Originally designed for a 5 year mission dedicated to observing distant celestial objects in the X - ray spectrum, Chandra has been observing for over three times that long and is still going strong. In this image the Chandra X - ray Observatory reveals

Walter B Myers

PIX4645635

Chandra Space Telescope - Artist View - Chandra X - Ray Observatory - View of the Chandra Telescope in orbit around Earth. The Chandra space telescope observes the universe in X-ray; it was launched and put into orbit in July 1999. Nasa's Chandra X - ray Observatory as it may appear at about 50,000 miles from the Earth, almost twice as high as Earth - orbiting geosynchronous satellites. Named after the Indian astrophysicist Subrahmanyan Chandrasekhar, the Chandra X - ray Observatory is the world's most powerful X - ray telescope, and at a weight of over 5 tons (10 tons including the detachable booster rocket) was the heaviest payload ever delivered into orbit by the Space Shuttle. Chandra was carried into space by Columbia in July 1999. Originally designed for a 5 year mission dedicated to observing distant celestial objects in the X - ray spectrum, Chandra has been observing for over three times that long and is still going strong. In this image the Chandra X - ray Observatory reveals

Walter B Myers

PIX4645635

 
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 li

Tom Davis

PIX4564326

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 li

Tom Davis

PIX4564326

 
Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

PIX4626499

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

PIX4626499

 
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

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

 
Venice and its lagoon - satellite view - 09/12/2001 Venice stretches out across numerous small islands in a marshy lagoon along the Adriatic Sea in northeastern Italy. The saltwater lagoon stretches along the shoreline between the mouths of the Po (sth) and Piave (nth) Rivers. This image from the Advanced Spaceborne Thermal Emission and Reflection Radiometer on the Terra satellite shows the watery city in spectacular detail, using false - color image enhancements that bring out the details of water and vegetation. The heart of Venice is on the island known as the Rialto, the largest island in the lagoon, which is just southwest of the center of this scene. The city is somewhat protected from the open sea by a row of sandbanks known as the Lido (east of Rialto), however, the city is continually under threat of flooding and erosion, and has been experimenting with tidal control measures for more than a thousand years. Four hundred bridges cross the labyrinth of canals that form the 120 i

PIX4666419

Venice and its lagoon - satellite view - 09/12/2001 Venice stretches out across numerous small islands in a marshy lagoon along the Adriatic Sea in northeastern Italy. The saltwater lagoon stretches along the shoreline between the mouths of the Po (sth) and Piave (nth) Rivers. This image from the Advanced Spaceborne Thermal Emission and Reflection Radiometer on the Terra satellite shows the watery city in spectacular detail, using false - color image enhancements that bring out the details of water and vegetation. The heart of Venice is on the island known as the Rialto, the largest island in the lagoon, which is just southwest of the center of this scene. The city is somewhat protected from the open sea by a row of sandbanks known as the Lido (east of Rialto), however, the city is continually under threat of flooding and erosion, and has been experimenting with tidal control measures for more than a thousand years. Four hundred bridges cross the labyrinth of canals that form the 120 i

PIX4666419

 
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Moon Formation: Another Hypotheses of Giant Impact - Moon Formation: Hit-and-run Giant Impact Scenario: The hypothesis of giant impact suggests that the Moon was created from material ejected by a collision between the young Earth and a body the size of Mars named Theia 4.5 billion years ago. This scenario is widely accepted, but analyses of lunar samples have shown a major problem with this theory: the Moon should be composed mainly of Theia materials. The elements of the Moon and the Earth show remarkable similarities. Researchers explored a new collision geometry, changing the impact configuration. Their simulation also integrates a more energetic impact (called “hit and run”) that could tear more matter from Earth and make the pre-lunar debris disc dominate by terrestrial matter - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, a

Miller, Ron (b.1947)

PIX4614860

Moon Formation: Another Hypotheses of Giant Impact - Moon Formation: Hit-and-run Giant Impact Scenario: The hypothesis of giant impact suggests that the Moon was created from material ejected by a collision between the young Earth and a body the size of Mars named Theia 4.5 billion years ago. This scenario is widely accepted, but analyses of lunar samples have shown a major problem with this theory: the Moon should be composed mainly of Theia materials. The elements of the Moon and the Earth show remarkable similarities. Researchers explored a new collision geometry, changing the impact configuration. Their simulation also integrates a more energetic impact (called “hit and run”) that could tear more matter from Earth and make the pre-lunar debris disc dominate by terrestrial matter - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, a

Miller, Ron (b.1947)

PIX4614860

 
Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially sch

PIX4615883

Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially sch

PIX4615883

 
Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

 
Colliding galaxy Ngc 6745 in Lyra - Colliding galaxy NGC 6745 in Lyra - The spiral galaxy NGC 6745 is located about 206 million years away - light from Earth. This galaxy is double; a second galaxy at the bottom right of the image collides with it, causing star formation. Image obtained by the Hubble Space Telescope in 1996. A large spiral galaxy, with its nucleus still intact, peers at the smaller passing galaxy (almost out of the field of view at lower right). These galaxies did not merely interact gravitationally as they passed one another, they actually collided. When galaxies collide, the stars that normally comprise the major portion of the luminous mass of each of the two galaxies will almost never collide with each other but will pass rather freely between each other with little damage. This occurs because the physical size of individual stars is tiny compared to their typical separations, making the chance of physical encounter relatively small. In our own Milky Way galaxy, th

PIX4612985

Colliding galaxy Ngc 6745 in Lyra - Colliding galaxy NGC 6745 in Lyra - The spiral galaxy NGC 6745 is located about 206 million years away - light from Earth. This galaxy is double; a second galaxy at the bottom right of the image collides with it, causing star formation. Image obtained by the Hubble Space Telescope in 1996. A large spiral galaxy, with its nucleus still intact, peers at the smaller passing galaxy (almost out of the field of view at lower right). These galaxies did not merely interact gravitationally as they passed one another, they actually collided. When galaxies collide, the stars that normally comprise the major portion of the luminous mass of each of the two galaxies will almost never collide with each other but will pass rather freely between each other with little damage. This occurs because the physical size of individual stars is tiny compared to their typical separations, making the chance of physical encounter relatively small. In our own Milky Way galaxy, th

PIX4612985

 
Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean tha

PIX4615964

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean tha

PIX4615964

 
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Coghlan's Coffin (colour litho)

English School, (20th century)

LAL397767

Coghlan's Coffin (colour litho)

English School, (20th century)

LAL397767

 
Count de Lambert Prince Alexander 1909 (photo)

UIG681946

Count de Lambert Prince Alexander 1909 (photo)

UIG681946

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