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Bilder zu 'Single-object' gefunden, 29,605

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Future Concepts Skylon spaceplane, 1990s

Future Concepts Skylon spaceplane, 1990s

UIS5082902

Launch Vehicles, USA Rocketdyne J-2 rocket motor, 1960s

Launch Vehicles, USA Rocketdyne J-2 rocket motor, 1960s

UIS5065244

Telegraphy, Cooke & Wheatstone Wheatstone bridge, c 1843

Telegraphy, Cooke & Wheatstone Wheatstone bridge, c 1843

UIS5060835

Microscopes, 18th Century Modified Marshall type compound microscope, 1720

Microscopes, 18th Century Modified Marshall type compound microscope, 1720

UIS5086894

Watches, Pocket Two pocket watches (montre gousset), c 1705 and c 1660

Watches, Pocket Two pocket watches (montre gousset), c 1705 and c 1660

UIS5061428

Austin Seven motor car, 1922

Austin Seven motor car, 1922

UIS5061088

Farm Equipment, Tractors Lanz 'Bulldog' tractor, c 1930

Farm Equipment, Tractors Lanz 'Bulldog' tractor, c 1930

UIS5063807

Clocks, Domestic, General Bracket clock (pendule cartel), English, c 1706

Clocks, Domestic, General Bracket clock (pendule cartel), English, c 1706

UIS5068840

Clocks, Domestic, General Bracket clock, English, c 1706

Clocks, Domestic, General Bracket clock, English, c 1706

UIS5063614

Spinning Wheels, Manual Silk twister's wheel, cross and reeler for twisting silk by hand, c 1770

Spinning Wheels, Manual Silk twister's wheel, cross and reeler for twisting silk by hand, c 1770

UIS5061183

Launch Vehicles, USA Saturn V rocket, 1967

Launch Vehicles, USA Saturn V rocket, 1967

UIS5065187

Electric filament lamps made by Swan (left) and Edison (right : lampe electrique a incandescence), 1878-1879

Electric filament lamps made by Swan (left) and Edison (right : lampe electrique a incandescence), 1878-1879

UIS5062575

Launch Vehicles, British Black Arrow flight sequence programmer, c 1968

Launch Vehicles, British Black Arrow flight sequence programmer, c 1968

UIS5069878

Launch Vehicles, USA Saturn V rocket, 1967

Launch Vehicles, USA Saturn V rocket, 1967

UIS5065301

Launch Vehicles, British Black Arrow flight sequence programmer, c 1968

Launch Vehicles, British Black Arrow flight sequence programmer, c 1968

UIS5069881

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30

PIX4618255

Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer

Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer

PIX4618266

Distant galaxies in the Fornax constellation - Distant galaxies in the Fornax constellation - Image of distant galaxies obtained by the Hubble space telescope in the constellation Forneau in September 2003. This image represents a typical view of our distant universe. In taking this picture, Hubble is looking down a long corridor of galaxies stretching billions of light - years distant in space, corresponding to looking billions of years back in time. The field shown in this picture covers a relatively small patch of sky, a fraction of the area of the full moon, yet it is richly populated with a variety of galaxy types. A handful of large fully formed galaxies are scattered throughout the image. These galaxies are easy to see because they are relatively close to us. Several of the galaxies are spirals with flat disks that are oriented edge - on or face - on to our line of sight, or somewhere in between. Elliptical galaxies and more exotic galaxies with bars or tidal tails are also visi

Distant galaxies in the Fornax constellation - Distant galaxies in the Fornax constellation - Image of distant galaxies obtained by the Hubble space telescope in the constellation Forneau in September 2003. This image represents a typical view of our distant universe. In taking this picture, Hubble is looking down a long corridor of galaxies stretching billions of light - years distant in space, corresponding to looking billions of years back in time. The field shown in this picture covers a relatively small patch of sky, a fraction of the area of the full moon, yet it is richly populated with a variety of galaxy types. A handful of large fully formed galaxies are scattered throughout the image. These galaxies are easy to see because they are relatively close to us. Several of the galaxies are spirals with flat disks that are oriented edge - on or face - on to our line of sight, or somewhere in between. Elliptical galaxies and more exotic galaxies with bars or tidal tails are also visi

PIX4613828

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

PIX4583169

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

Planetary nebula NGC 6369 in Ophiuchus/HST - NGC 6369 is known to amateur astronomers as the “” Little Ghost Nebula,”” because it appears as a small, ghostly cloud surrounding the faint, dying central star. NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light - years from Earth. When a star with a mass similar to that of our own Sun nears the end of its lifetime, it expands in size to become a red giant. The red - giant stage ends when the star expels its outer layers into space, producing a faintly glowing nebula. Astronomers call such an object a planetary nebula, because its round shape resembles that of a planet when viewed with a small telescope. The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground - based telescopes because of the blurring produced by the Earth's atmo

PIX4623194

Mahogany secretary stamped by Lemarchand, belonged to Prince Murat, open, France, 19th century

Mahogany secretary stamped by Lemarchand, belonged to Prince Murat, open, France, 19th century

Lemarchand, Charles-Joseph (1859-1926) & Louis-Edouard (1795-1872)

DGA1082384

Mahogany secretary stamped by Lemarchand, belonged to Prince Murat, France, 19th century

Mahogany secretary stamped by Lemarchand, belonged to Prince Murat, France, 19th century

Lemarchand, Charles-Joseph (1859-1926) & Louis-Edouard (1795-1872)

DGA1082383

A Staffordshire saltglaze tartan-ground royalist teapot and cover with a bust length portrait of Prince Charles Edward Stuart (1720-1788), c.1750 (ceramic)

A Staffordshire saltglaze tartan-ground royalist teapot and cover with a bust length portrait of Prince Charles Edward Stuart (1720-1788), c.1750 (ceramic)

English School, (18th century)

CH1766854

A bronze figure of H.R.H. The Prince of Wales, later Edward VIII, dressed for tennis, c.1920s-1930s (bronze, light brown patina)

A bronze figure of H.R.H. The Prince of Wales, later Edward VIII, dressed for tennis, c.1920s-1930s (bronze, light brown patina)

Jagger, Charles Sergeant (1885-1934)

CH991009

H.R.H. Prince of Wales, 1921-2 ; 1935 (bronze with a light brown patina)

H.R.H. Prince of Wales, 1921-2 ; 1935 (bronze with a light brown patina)

Jagger, Charles Sergeant (1885-1934)

CH1197090

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