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Vapor Drawing #15, 2003 (aluminum and silicon monoxide on paper)

premium — Vapor Drawing #15, 2003 (aluminum and silicon monoxide on paper)

Vapor Drawing #15, 2003 (aluminum and silicon monoxide on paper)

Bell, Larry (b.1939)

HST2908725

Vapor Drawing #2, 2003 (aluminum and silicon monoxide on paper)

premium — Vapor Drawing #2, 2003 (aluminum and silicon monoxide on paper)

Vapor Drawing #2, 2003 (aluminum and silicon monoxide on paper)

Bell, Larry (b.1939)

HST2908724

United States, 1950s: Liquid evaporates on hot surface

United States, 1950s: Liquid evaporates on hot surface

AVE6326059

An ice making machine

An ice making machine

UIG5312025

The Salt Industries of Cheshire (litho)

The Salt Industries of Cheshire (litho)

English School, (19th century)

LIP1056596

An engraving depicting Carre's apparatus for the artificial production of ice. A vessel containing concentrated ammonia is heated. The vaporised ammonia liquefies. Subsequent cooling vaporises ammonia producing cold, 19th century

An engraving depicting Carre's apparatus for the artificial production of ice. A vessel containing concentrated ammonia is heated. The vaporised ammonia liquefies. Subsequent cooling vaporises ammonia producing cold, 19th century

UIG5311430

Illustration showing Cyrano de Bergerac flying using lifting energy provided by bottles of dew, evaporated by sunlight.

Illustration showing Cyrano de Bergerac flying using lifting energy provided by bottles of dew, evaporated by sunlight.

UIG5311119

La corde sensible, 1960 (oil on canvas)

La corde sensible, 1960 (oil on canvas)

Magritte, Rene (1898-1967)

CH6295527

Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates

Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates

L. Bret

PIX4573389

Plant for the production of evaporated salt pans

Plant for the production of evaporated salt pans

TRK879647

Mars with water - Artist's view - Wet Mars - Artwork: More than three billion years ago, water flowed on Mars. The water is now evaporated. This illustration can also illustrate the terraformation of Mars. 3.5 billion years ago Mars had water.

Mars with water - Artist's view - Wet Mars - Artwork: More than three billion years ago, water flowed on Mars. The water is now evaporated. This illustration can also illustrate the terraformation of Mars. 3.5 billion years ago Mars had water.

PIX4616947

Gamma Cassiopeia, IC 59 and IC 63 - The bright bluish star shown here is Gamma Cassiopeiae. It is currently evaporating two nearby clouds of gas - IC 59 and IC 63

Gamma Cassiopeia, IC 59 and IC 63 - The bright bluish star shown here is Gamma Cassiopeiae. It is currently evaporating two nearby clouds of gas - IC 59 and IC 63

R. Gendler

PIX4621810

The Dissolution, or the Alchymist producing an Aetherial Representation, published by Hannah Humphrey in 1796 (hand-coloured etching)

The Dissolution, or the Alchymist producing an Aetherial Representation, published by Hannah Humphrey in 1796 (hand-coloured etching)

Gillray, James (1757-1815)

NCO190413

Poster advertising Franck Perfume, Paris, France, c.1925

Poster advertising Franck Perfume, Paris, France, c.1925

French School, (20th century)

FGL2967457

High speed strobe photograph of a cloud of droplets 'stopped' in full flight during a sneeze. Most of the moisture in the droplets quickly evaporates, leaving thousands of germ laden particles from the nose and throat floating in the air. 1940 photo by Prof. Marshall W. Jennison, of Massachusetts Institute of Technology

High speed strobe photograph of a cloud of droplets 'stopped' in full flight during a sneeze. Most of the moisture in the droplets quickly evaporates, leaving thousands of germ laden particles from the nose and throat floating in the air. 1940 photo by Prof. Marshall W. Jennison, of Massachusetts Institute of Technology

EVB2925640

The Dissolution or The Alchymist producing an Aetherial Representation, pub. 1796 (hand coloured engraving)

The Dissolution or The Alchymist producing an Aetherial Representation, pub. 1796 (hand coloured engraving)

Gillray, James (1757-1815)

STC2966808

Mars with water - Artist's view - Martian Waterfall - Artwork: More than three billion years ago, water flowed on Mars. The water is now evaporated. This illustration can also illustrate the terraformation of Mars - 3.5 billion years ago Mars had water. This artwork could also show terraforming of a future March

Mars with water - Artist's view - Martian Waterfall - Artwork: More than three billion years ago, water flowed on Mars. The water is now evaporated. This illustration can also illustrate the terraformation of Mars - 3.5 billion years ago Mars had water. This artwork could also show terraforming of a future March

Miller, Ron (b.1947)

PIX4616893

Astronauts explore Callisto - Illustration: Astronauts explore the erodes peaks of Callisto - Astronauts among eroded peaks of its moon Callisto - Several square miles of the surface is dominated by towering spires of ice, 260 to 330 feet (80 to 100 m) tall. While composed mostly of ice, the spires also contain some darker dust, which absorbs heat from the Sun. As the ice erodes, the dark material apparently slides down and collects in low-lying areas. As the ice continues to vaporize, the dark material accumulates and the erosion process accelerates

Astronauts explore Callisto - Illustration: Astronauts explore the erodes peaks of Callisto - Astronauts among eroded peaks of its moon Callisto - Several square miles of the surface is dominated by towering spires of ice, 260 to 330 feet (80 to 100 m) tall. While composed mostly of ice, the spires also contain some darker dust, which absorbs heat from the Sun. As the ice erodes, the dark material apparently slides down and collects in low-lying areas. As the ice continues to vaporize, the dark material accumulates and the erosion process accelerates

Miller, Ron (b.1947)

PIX4614107

Salt pans, 1995 (photo)

Salt pans, 1995 (photo)

SZT11769007

Soyer's 'Magic Stove', c 1850

Soyer's 'Magic Stove', c 1850

UIS5082415

Mars Science Laboratory - Artist View - Mars Science Laboratory - Artist view - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover that will explore the surface of Mars from 2012 onwards. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for stereo color viewing of surrounding terrain and material collected by the arm; and, the ChemCam instrument, which is a laser that vaporizes material from rocks up to about 9 meters (30 feet) away and determines what elements the rocks are made of

Mars Science Laboratory - Artist View - Mars Science Laboratory - Artist view - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover that will explore the surface of Mars from 2012 onwards. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for stereo color viewing of surrounding terrain and material collected by the arm; and, the ChemCam instrument, which is a laser that vaporizes material from rocks up to about 9 meters (30 feet) away and determines what elements the rocks are made of

PIX4606945

Potash evaporation ponds in Lop Nur, Xinjiang, China (photo)

Potash evaporation ponds in Lop Nur, Xinjiang, China (photo)

UIG3272371

Distillation Glass retort, Italian, 1650-1800

Distillation Glass retort, Italian, 1650-1800

UIS5067095

Engraving depicting a young lady gilding buttons

Engraving depicting a young lady gilding buttons

UIG5308936

Kief (Hashish / Maruijana / Cannabis) Smoker - Algeria

Kief (Hashish / Maruijana / Cannabis) Smoker - Algeria

EPL7049070

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in this subimage are polygonal cracks in the ice on the dunes (the cracks disappear when the ice is gone). Image taken on 07 April 2008 by Mars Reconnaissance Orbiter (MRO) spacecraft — Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

PIX4616482

Distillation Glass retort, Italian, 1650-1800

Distillation Glass retort, Italian, 1650-1800

UIS5068830

Producing salt by evaporating sea water in salt pans, 1556 (engraving)

Producing salt by evaporating sea water in salt pans, 1556 (engraving)

Unknown Artist, (16th century)

Bianchetti, Stefano

XEE4162943

Lake Yamma, Queensland, Australia, True Colour Satellite Image

Lake Yamma, Queensland, Australia, True Colour Satellite Image

UIG601917

Mars Science Laboratory - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the rover examines a rock on Mars with a set of tools at the end of the rover's arm, which extends about 2 meters (7 feet). Two instruments on the arm can study rocks up close. Also, a drill can collect sample material from inside of rocks and a scoop can pick up samples of soil. The arm can sieve the samples and deliver fine powder to instruments inside the rover for thorough analysis. The mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for stereo color viewing of surrounding terrain and material collected by the arm; and, the ChemCam instrument, which is a laser that vaporizes material from rocks up to about 9 meters (30 feet) away and determines what elements the rocks are made of — Mars Science Laboratory - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the rover examines a rock on Mars with a set of tools at the end of the rover's arm, which extends about 2 meters (7 feet). Two instruments on the arm can study rocks up close. Also, a drill can collect sample material from inside of rocks and a scoop can pick up samples of soil. The arm can sieve the samples and deliver fine powder to instruments inside the rover for thorough analysis. The mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for

Mars Science Laboratory - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the rover examines a rock on Mars with a set of tools at the end of the rover's arm, which extends about 2 meters (7 feet). Two instruments on the arm can study rocks up close. Also, a drill can collect sample material from inside of rocks and a scoop can pick up samples of soil. The arm can sieve the samples and deliver fine powder to instruments inside the rover for thorough analysis. The mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for

PIX4606810

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shine primarily in the blue, green, and red light emitted by excited atoms of hydrogen, nitrogen, oxygen, and sulfur. Particularly striking is the rose - like feature, seen to the right of center, which glows in the red light emitted by hydrogen and sulfur. ACS made this observation on April 1 and 2, 2002. The color image is constructed from four separate images taken in these filters: blue, near infrared, hydrogen alpha, and doubly ionized oxygen — Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

PIX4620193

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shine primarily in the blue, green, and red light emitted by excited atoms of hydrogen, nitrogen, oxygen, and sulfur. Particularly striking is the rose - like feature, seen to the right of center, which glows in the red light emitted by hydrogen and sulfur. ACS made this observation on April 1 and 2, 2002. The color image is constructed from four separate images taken in these filters: blue, near infrared, hydrogen alpha, and doubly ionized oxygen — Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

PIX4620159

HEA - THERMOMETERS 'Double' barometer and thermometer, c 1740

HEA - THERMOMETERS 'Double' barometer and thermometer, c 1740

UIS5063062

Instruments, Spectroscopes Grating spectrometer, 1882-1905

Instruments, Spectroscopes Grating spectrometer, 1882-1905

UIS5069441

HEA - THERMOMETERS 'Double' barometer and thermometer, c 1740

HEA - THERMOMETERS 'Double' barometer and thermometer, c 1740

UIS5061425

Instruments, Spectroscopes Hilger wavelength spectrometer (spectrometre) with camera, c 1919

Instruments, Spectroscopes Hilger wavelength spectrometer (spectrometre) with camera, c 1919

UIS5067044

Exoplanet Kelt-9b - Illustration

Exoplanet Kelt-9b - Illustration

Miller, Ron (b.1947)

PIX7223407

Halley Comete - Halley's Comet on December 9, 1985 - Halley Comete December 9, 1985

Halley Comete - Halley's Comet on December 9, 1985 - Halley Comete December 9, 1985

PIX4569993

Comet Holmes, 2009 (digital photo)

Comet Holmes, 2009 (digital photo)

Howes, Nick (21st century)

MMM7341110

View from Travertine Plateau

View from Travertine Plateau

SAP703408

Travertine Plateau

Travertine Plateau

SAP703410

Travertine Plateau

Travertine Plateau

SAP703406

View from Travertine Plateau

View from Travertine Plateau

SAP703409

Comete of Halley - Halley's comet - View on April 10, 1986

Comete of Halley - Halley's comet - View on April 10, 1986

PIX4569954

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Reboredo, Sergi

SRB3585211

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Reboredo, Sergi

SRB3585210

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Reboredo, Sergi

SRB3585209

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