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Bilder zu 'Messungen' gefunden, 436

 
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Map of the moon by H Percy Wilkins, third edition, 1952 (technical drawing, paper)

Wilkins, H. Percy (1896-1960)

MMM7340725

Map of the moon by H Percy Wilkins, third edition, 1952 (technical drawing, paper)

Wilkins, H. Percy (1896-1960)

MMM7340725

 
Polaris - Illustration - Polaris System - Illustration - Polaris is a triple system composed of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This illustration shows the triple system of this star, Polaris A and Polaris Ab, and further on, his companion Polaris B. This is a view from within the Polaris triple star system. The North Star, Polaris A is a bright supergiant variable star.Just above Polaris is a small companion, Polaris Ab, which is 2 billion miles from Polaris. Much farther away, near the top of the illustration, is the wide companion Polaris B. Polaris B is located approximately 240 billion miles from Polaris A. The two companion stars are the same temperature as Polaris A, but are dwarf stars. The wide companion star is visible in small telescopes. It was first noticed by William Herschel in 1780. The close companion, Polaris Ab was known to exist from measurements of a wobble in Polaris, caused by the gravitational tu

PIX4572039

Polaris - Illustration - Polaris System - Illustration - Polaris is a triple system composed of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This illustration shows the triple system of this star, Polaris A and Polaris Ab, and further on, his companion Polaris B. This is a view from within the Polaris triple star system. The North Star, Polaris A is a bright supergiant variable star.Just above Polaris is a small companion, Polaris Ab, which is 2 billion miles from Polaris. Much farther away, near the top of the illustration, is the wide companion Polaris B. Polaris B is located approximately 240 billion miles from Polaris A. The two companion stars are the same temperature as Polaris A, but are dwarf stars. The wide companion star is visible in small telescopes. It was first noticed by William Herschel in 1780. The close companion, Polaris Ab was known to exist from measurements of a wobble in Polaris, caused by the gravitational tu

PIX4572039

 
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A plan of a weir and embankment on the Arno east of Florence, 1504 (pen & ink with brown and blue wash, over black chalk on paper)

Vinci, Leonardo da (1452-1519)

ROC3930012

A plan of a weir and embankment on the Arno east of Florence, 1504 (pen & ink with brown and blue wash, over black chalk on paper)

Vinci, Leonardo da (1452-1519)

ROC3930012

 
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An architectural drawing of the large railway bridge over the river Wear at Sunderland, Durham

BL3286648

An architectural drawing of the large railway bridge over the river Wear at Sunderland, Durham

BL3286648

 
James Webb Space Telescope (JWST) - JWST in clean room: Curvature measurements of the JWST Space Telescope (James Webb Space Telescope) at Nasa's Goddard Space Center. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Engineers and technicians working on the James Webb Space Telescope successfully completed the first important optical measurement of Webb's fully assembled primary mirror, called a Center of Curvature test. Taking a “” before””” optical measurement of the telescope's deployed mirror is crucial before the telescope goes into several stages of rigorous mechanical testing. These tests will simulate the violent sound and vibration environments the telescope will experience inside its rocket on its way out into space. This environment is one of the most stressful structurally and could alter the shape and alignment of Webb's primary mirror, which could degrade or, in the worst case, ruin it

PIX4645835

James Webb Space Telescope (JWST) - JWST in clean room: Curvature measurements of the JWST Space Telescope (James Webb Space Telescope) at Nasa's Goddard Space Center. The JWST will replace the Hubble Space Telescope in 2018. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Engineers and technicians working on the James Webb Space Telescope successfully completed the first important optical measurement of Webb's fully assembled primary mirror, called a Center of Curvature test. Taking a “” before””” optical measurement of the telescope's deployed mirror is crucial before the telescope goes into several stages of rigorous mechanical testing. These tests will simulate the violent sound and vibration environments the telescope will experience inside its rocket on its way out into space. This environment is one of the most stressful structurally and could alter the shape and alignment of Webb's primary mirror, which could degrade or, in the worst case, ruin it

PIX4645835

 
Uranus and three satellites seen by Voyager 2 - Image obtained by the Voyager 2 probe in January 1986 showing the planet Uranus accompanied by the satellites Ariel (top right), Miranda (closest to the planet) and Umbriel (bottom left). This Voyager photograph of Uranus taken in january 1986 is a composite of for images taken by the narrow angle camera. At this range, clouds and other features in the atmosphere as small as 1,370 km. could be detected by Voyager 2. Yet, no such features are visible. This view is toward the illuminated south pole of Uranus. The predominant blue color is the result of atmospheric methane, which absorbs the red wavelengths from incoming sunlight. The spot at the upper left edge of the planet's disk reulted from the removal of a network mark used in making measurments on the photograph. Three of Uranus' five known satellites are visible; Miranda (at far right, closest to the planet), Ariel (next out, at top), and Umbriel (lower left). Titania and Oberon are

PIX4634712

Uranus and three satellites seen by Voyager 2 - Image obtained by the Voyager 2 probe in January 1986 showing the planet Uranus accompanied by the satellites Ariel (top right), Miranda (closest to the planet) and Umbriel (bottom left). This Voyager photograph of Uranus taken in january 1986 is a composite of for images taken by the narrow angle camera. At this range, clouds and other features in the atmosphere as small as 1,370 km. could be detected by Voyager 2. Yet, no such features are visible. This view is toward the illuminated south pole of Uranus. The predominant blue color is the result of atmospheric methane, which absorbs the red wavelengths from incoming sunlight. The spot at the upper left edge of the planet's disk reulted from the removal of a network mark used in making measurments on the photograph. Three of Uranus' five known satellites are visible; Miranda (at far right, closest to the planet), Ariel (next out, at top), and Umbriel (lower left). Titania and Oberon are

PIX4634712

 
The cluster of stars Pismis 24 in the Scorpio - Pismis 24 star cluster in Scorpius - This image obtained by the Hubble space telescope shows the cluster of young stars Pismis 24, located about 8000 years - light in the nebula NGC 6357 of the Scorpio. This cluster houses a star that was thought to be the most massive star in our galaxy, between 200 and 300 solar masses (the brightest star in the top center of the image). The measurements obtained by the Hubble telescope showed that this star, Pismis 24 - 1, was actually a double star and that its mass was actually only about 100 solar masses. The small open star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 in Scorpius, about 8,000 light - years away from Earth. Some of the stars in this cluster are extremely massive and emit intense ultraviolet radiation. The brightest object in the picture is designated Pismis 24 - 1. It was once thought to weigh as much as 200 to 300 solar masses. This would not only have m

PIX4569076

The cluster of stars Pismis 24 in the Scorpio - Pismis 24 star cluster in Scorpius - This image obtained by the Hubble space telescope shows the cluster of young stars Pismis 24, located about 8000 years - light in the nebula NGC 6357 of the Scorpio. This cluster houses a star that was thought to be the most massive star in our galaxy, between 200 and 300 solar masses (the brightest star in the top center of the image). The measurements obtained by the Hubble telescope showed that this star, Pismis 24 - 1, was actually a double star and that its mass was actually only about 100 solar masses. The small open star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 in Scorpius, about 8,000 light - years away from Earth. Some of the stars in this cluster are extremely massive and emit intense ultraviolet radiation. The brightest object in the picture is designated Pismis 24 - 1. It was once thought to weigh as much as 200 to 300 solar masses. This would not only have m

PIX4569076

 
Swan Lace - detail - This delicate Hubble Space Telescope image shows a tiny portion of the Cygnus loop, a supernova remnant in the constellation of Cygnus, the Swan. Measurements on this super - detailed image of a cosmic veil shows that the original supernova explosion took place only 5000 years ago. The Cygnus loop, also known as the Veil Nebula, is well - known to amateur astronomers as a challenging target for larger telescopes. It has a diameter of about 3 degrees (corresponding to 6 full moons). This spectacular nebula was created when a massive star ended its days in an immense supernova explosion. A bubble of dust and gas was expelled into space and has continued to expand outwards ever since. The Cygnus Loop consists of two main arcs, designated NGC 6992/95 for the Eastern arc and NGC 6960 for the Western arc (also called the Witch's Broom Nebula). The tiny area of the Hubble image is seen in the upper left - hand corner of the nebula, at the outer edge of one of the large fi

PIX4582633

Swan Lace - detail - This delicate Hubble Space Telescope image shows a tiny portion of the Cygnus loop, a supernova remnant in the constellation of Cygnus, the Swan. Measurements on this super - detailed image of a cosmic veil shows that the original supernova explosion took place only 5000 years ago. The Cygnus loop, also known as the Veil Nebula, is well - known to amateur astronomers as a challenging target for larger telescopes. It has a diameter of about 3 degrees (corresponding to 6 full moons). This spectacular nebula was created when a massive star ended its days in an immense supernova explosion. A bubble of dust and gas was expelled into space and has continued to expand outwards ever since. The Cygnus Loop consists of two main arcs, designated NGC 6992/95 for the Eastern arc and NGC 6960 for the Western arc (also called the Witch's Broom Nebula). The tiny area of the Hubble image is seen in the upper left - hand corner of the nebula, at the outer edge of one of the large fi

PIX4582633

 
Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 450 years - light from Earth. Image obtained by a 50 cm telescope, 42 poses of 15 minutes accumulated. Located in the constellation of Aquarius, the Helix is our closest planetary nebula at only 450 light years distance. It is so close that it can be telescopically seen shifting one side to the other in front of the more distant background stars as the earth moves around the sun - a phenomenon called parallax. Parallax measurements are used to trigonometrically deduce distance between an object in space and the earth. A planetary nebula results when a red giant star, near the ends of it's productive life, sheds its outer layers into space and creates a breathtaking shell of surrounding gas that early visual astronomers likened to the disks of planets. This planetary spans approximately 1.5 light years and is still expanding. The name associated with the Helix is derived from the c

R. Jay GaBany

PIX4623639

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 450 years - light from Earth. Image obtained by a 50 cm telescope, 42 poses of 15 minutes accumulated. Located in the constellation of Aquarius, the Helix is our closest planetary nebula at only 450 light years distance. It is so close that it can be telescopically seen shifting one side to the other in front of the more distant background stars as the earth moves around the sun - a phenomenon called parallax. Parallax measurements are used to trigonometrically deduce distance between an object in space and the earth. A planetary nebula results when a red giant star, near the ends of it's productive life, sheds its outer layers into space and creates a breathtaking shell of surrounding gas that early visual astronomers likened to the disks of planets. This planetary spans approximately 1.5 light years and is still expanding. The name associated with the Helix is derived from the c

R. Jay GaBany

PIX4623639

 
Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

PIX4675989

Tyndall Glacier, Chile - Tyndall Glacier, Chile - The Tyndall Glacier in Torres del Paine National Park in Chile, observed from the International Space Station in November 2007. Tyndall Glacier is located in the Torres del Paine National Park in Chile. This glacier, which has a total area of 331 square kilometers and a length of 32 kilometers (based on 1996 measurements), begins in the Patagonian Andes Mountains to the west and terminates in Lago Geikie. The digital astronaut photograph taken in november 2007 records visible light in red, green, and blue wavelengths (true color). The Tyndall Glacier terminus has retreated significantly during the past 17 years. Significant ice loss was also observed earlier this year at Grey Glacier, about 30 kilometers to the north - northeast, suggesting both glaciers are responding similarly to regional changes in temperature and precipitation. A medial moraine is visible in the center of the glacier, extending along its length (top image, center le

PIX4675989

 
Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

PIX4616544

Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

PIX4616544

 
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Nutzungsbeschränkungen von unseren Content-Partnern
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  • Web download not available - Please contact your account manager for access
Standing male nude, c.1515-20 (chalk on paper) (verso of 3715476)

Buonarroti, Michelangelo (1475-1564)

ROC3715629

Standing male nude, c.1515-20 (chalk on paper) (verso of 3715476)

Buonarroti, Michelangelo (1475-1564)

ROC3715629

 
Zusätzliche Genehmigungen
  • Permission required for all uses - Please contact us
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  • Web download not available - Please contact your account manager for access
Male nude with proportions indicated, c.1515-20 (chalk on paper)

Buonarroti, Michelangelo (1475-1564)

ROC3715476

Male nude with proportions indicated, c.1515-20 (chalk on paper)

Buonarroti, Michelangelo (1475-1564)

ROC3715476

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