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'Carbon Dioxide' images and/or videos results page 1 of 3

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Images of 'Carbon Dioxide' found, 233

Apollo 13 "mail box"
Apollo 13 Lunar Module and the 'mailbox.' The mailbox was a jerry-rigged to use the Command Module lithium hydroxide canisters to purge carbon dioxide from the Lunar Module, the 'lifeboat' where the crew spend return trip to Earth. April 17, 1970
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Sylvie Vartan Records His Issue “Number One” June 17, 1977 (b/w photo)
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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: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a cork from a champagne bottle. Image taken on 1 January 2010 by Mars Reconnaissance Orbiter (MRO) spacecraft
Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future
Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future
Joseph Black (1728 - 1799)
Extinguishing a candle with carbon dioxide
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Space-filling Models showing the Molecules in Decomposition of Sugar to Ethanol and Carbon Dioxide during Fermentation.
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Photosynthesis
Carbon Dioxide Snow Create Static Spark
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The Reaction of Photosynthesis
Dry Ice, 1970, printed 2011 (b/w photo)
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Photosynthesis
USA, 1950s: Diagram showing flow of molecules inside an artificial respiration machine
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Archean stromatolites - Illustration showing the shores of an ancient sea 3 billion years ago. In the foreground, stromatolites, aggregation of sediments and cyanobacteries. Stromatoliths have undoubtedly contributed to our dioxygen-rich atmosphere and the ozone layer that allowed the development of a more complex terrestrial and oceanic life. Dome - shaped stromatolites, averaging three feet high and four feet wide, populate the shallow shore of an ancient sea 3 billion years ago. The Moon looms near the horizon, much closer to the Earth than it is now and therefore appearing considerably larger, but otherwise looking much like the moon we know today. 3 billion years ago the first macro evidence of life on Earth may have appeared in the form of large aggregations of microorganisms and associated sediments known as stromatolites. Cyanobacteria (AKA blue - green algae) were likely one of the primary contributors to these aggregations. During the Archean Eon the Earth's atmosphere contained very little oxygen. Cyanobacteria would have thrived during this time as they employ photosynthesis to combine water, carbon dioxide, and sunlight to create their food, while the byproducts of this process are oxygen and calcium carbonate. Billions of years of photosynthetic processes by cyanobacteria other living organisms are likely the primary source of the oxygen we breathe. They also provided the oxygen that forms the protective ozone layer, filtering the shorter wavelengths of ultraviolet light from the Sun that are harmful to most forms of life. Varieties of stromatolites still flourish to this day with well - known formations in parts of Australia, Brazil, and the Bahamas
Carbon cycle
USA, 1950s: Two glass jars, one containing a lit candle that goes out when oxygen is used up
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The Keeling Curve
Yeast and sugar solution turned into froth of carbon dioxide (anaerobic respiration)
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Carl Wilhelm Scheele
Portrait of Joseph Black
Portrait of Paul Bert, 1886 (engraving)
Animation of Dust Escaping from a Pipe and Causing Clouds
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Sunrise seen from Triton - Artist view - Sunrise on Triton - Artist view - Sunrise seen from Triton, the largest satellite in Neptune. A diminutive sun rises over Triton's hard and glistening landscape of rock, frozen water, carbon dioxide, nitrogen, and methane. The little warmth that reaches Triton's surface induces a nitrogen and methane haze, forming a very tenuous atmosphere. It is very cold on Triton with temperatures falling as low as minus 391o F. While as much as 25% of Triton may be composed of water ice, it is very unlikely that there is any liquid water, or life, on this world
Yeast and sugar solution turned into froth of carbon dioxide (anaerobic respiration) (photo)
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Dog's grotto near Naples - dogs choke on carbon dioxide and man survives
Beer industry, Beer pump in the cellar, powered with carbon dioxide in London restaurant, 
1891
Leigh Valley 607 Locomotive Equipped With The American-La France Foamite Corporation's ALFCO Carbon Dioxide System
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HEALTH WORKERS CULL CHICKENS WITH CARBON DIOXIDE AT A FARM IN HONG KONG
AFTER BIRDFUL OUTBREAK, 2002-02-05 (photo)
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Joseph Priestley (1733-1804), discovered oxygen during his research on the properties of air. He also determined that animals exhale carbon dioxide. 1849 print
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Martian dunes at the end of winter - March: Late Winter view of Dunes: Detail on dunes in the southern hemisphere of Mars. With the end of winter, the Sun melts the carbon dioxide ice present all winter. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on March 21, 2016. HIRISE is a 50 cm telescope that observes visible and near infrared. Sand dunes cover much of this terrain, which has large boulders lying on flat areas between the dunes. It is now late winter here in the Southern hemisphere, and these dunes are just getting enough sunlight to start defrosting their seasonal cover of carbon dioxide. Spots form where pressurized carbon dioxide gas escapes to the surface
Apollo 13: system to purge CO2 - Apollo 13: system to purge carbon dioxide - The makeshift box (nicknamed “mailbox”) built by the crew of Apollo 13 to purge CO2 inside the lunar module after the explosion of an oxygen tank. 04/1970. Interior view of the Apollo 13 Lunar Module (LM) showing the “” mail box””, a jerry - rigged arrangement which the Apollo 13 astronauts built to use the Command Module lithium hydroxide canisters to purge carbon dioxide from the Lunar Module
Artist's view of the Exoplanet HD 189733b - Exoplanet HD 189733b - Artist's view of the transit of the Exoplanet HD 189733b, a hot Jupiter (gas-like planet very close to its star), in front of its star. HD 189733b was discovered in 2005 in the constellation Little Fox. Using the Hubble space telescope, astronomers have detected carbon dioxide and monoxide in the atmosphere of this planet. Previously, methane and water vapour had already been detected in his atmosphere. But with a surface temperature of over 900 degrees, this planet remains too hot to shelter life. This is an artist's impression of the Jupiter - size extrasolar planet, HD 189733b, being eclipsed by its parent star. Astronomers using the Hubble Space Telescope have measured carbon dioxide and carbon monoxide in the planet's atmosphere. The planet is a “” hot Jupiter,””” which is so close to its star that it completes an orbit in only 2.2 days. The planet is too hot for life as we know it. But under the right conditions, on a more Earth - like world, carbon dioxide can indicate the presence of extraterrestrial life. This observation demonstrates that chemical biotracers can be detected by space telescope observations
The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars combined
Mars - View of the north pole - Mars north pole - Image of a portion of the northern polar cap of Mars obtained by the Mars Express probe on May 17, 2010. This image was acquired by the Mars Express High - Resolution Stereo Camera on 17 May 2010 and shows a part of the northern polar region of Mars at the northern hemisphere summer solstice. The polar ice deposits follow the seasonal cycles. Studies made by Mars Express's OMEGA instrument shows that the cap is covered by frozen water and carbon dioxide ice in winter and spring but by this point in the martian year all of the carbon dioxide ice has warmed and evaporated into the planet's atmosphere. Only water ice is left behind, which shows up as bright white areas in this picture. From these layers, large bursts of water vapour are occasionally released into the atmosphere. In winter, part of the atmosphere recondenses as frost and snow on the northern cap. These seasonal deposits can extend as far south as 45* N latitude and be up to a metre thick. Another phenomenon occurs on the curved scarps of the northern polar cap, such as the Rupes Tenuis slope (on the left of this image). During spring, the seasonal carbon dioxide layer is covered by water frost. At certain times, winds remove the millimetre - thick top layer of frozen water, revealing the carbon dioxide ice below. These processes bear witness to a dynamic water cycle on Mars and may lead to the varying accumulation of water ice over the polar cap
Chinon Nuclear Power Plant in Indre-et-Loire, France, 1959, part 4
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Chinon Nuclear Power Plant in Indre-et-Loire, France, 1959, part 5
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Chinon Nuclear Power Plant in Indre-et-Loire, France, 1959, part 3
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Joseph Black, c.1770 (oil on canvas)
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Photosynthesis
Members of the environmental group World Wide Fund for Nature (WWF) prepare a  model house with yell.., 1997-10-16 (photo)
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Joseph Black (1728-99) (oil on panel)
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Max Valier during a record-breaking run with his rocket car on the Avus, 1929 (b/w photo)
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EXC - CHEMISTRY 1700-1799 Nooth's apparatus, c 1775
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Devonian Canopee - Artist's View - Devonian Canopy - Artist's View of an Archaeopteris Forest about 380 million years ago. The fossil record reveals that great forests of Archaeopteris covered much of the Earth 380 million years ago. The large umbrella - like fronds appear to have been optimized for gathering sunlight at the canopy level while still permitting enough light to reach the shorter and younger trees. It was great forests like these that helped to draw much of the carbon dioxide out of the primeval air while releasing the oxygen we breathe today
A Greenpeace activist forms a dinosaurian sculpture out of scrap metal to demonstrate against intern.., 1997-10-22 (photo)
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GREENPEACE DEMONSTRATE AGAINST CLIMATE POLITICS IN BONN, 1997-10-22 (photo)
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Minister of Economics Günter Rexrodt (Germany FDP) - Press conference by Federal Ministers..., 1995 (photo)
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Environment Minister Angela Merkel (Germany CDU) - Press conference of federal ministers and..., 1995 (photo)
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Environment Minister Angela Merkel (Germany CDU) - Press conference of federal ministers and..., 1995 (photo)
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PENGUIN COSTUMED GREENPEACE ACTIVISTS PROTEST IN TOKYO, 1997-10-17 (photo)
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The First Life Forms on Earth - Eoarchean Earth - 3.8 billion years ago, 770 million years after the formation of the Earth, the first life forms appeared as a unicellular organism. Bacteries and archeobacteries (archaea) began to populate the Earth's surface while the atmosphere was still filled with volcanic gases and probably without oxygen. In this illustration, these micro-organisms came out of the ocean to attach themselves to the rock remains of a caldera, bringing colour to this monochrome landscape. 770 million years after the formation of the Earth - - 3.8 billion years ago - - the first life may have appeared in the form of simple, single - celled organisms. Bacteria and archaea may have even found a way to populate the otherwise sterile and inhospitable surface. The atmosphere would likely have consisted solely of gases vented by volcanoes: carbon dioxide, carbon monoxide, sulfur dioxide, nitrogen, methane, hydrogen, methane, ammonia, and water vapor. In this image, a variety of single - celled organisms have ventured out of the ocean and onto the rocky remains of two volcanic calderas, adding color to an otherwise bleak and monochromatic landscape. While the lack of breathable oxygen would be anathema to complex life forms like ourselves, this primitive atmosphere was a rich source of sustenance for these terrestrial vanguards
Minister of Economics Günter Rexrodt (Germany FDP) - Press conference by Federal Ministers..., 1995 (photo)
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TOYOTA MOTOR UNVEILS ITS NEW GREEN PASSENGER CAR IN TOKYO, 1997-10-14 (photo)
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Minister of Economics Günter Rexrodt (Germany FDP) - Press conference by Federal Ministers..., 1995 (photo)
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Environment Minister Angela Merkel (Germany CDU) - Press conference of federal ministers and..., 1995 (photo)
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Dr. Hans-Olaf Henkel (President of the Federation of German Industries) - Press conference of..., 1995 (photo)
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Dr. Hans-Otto Schwarz (President German Gas and Water Management e.V.) - Press conference..., 1995 (photo)
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Apr. 05, 1954 - Survival Training School At Gosport Scrambling Into The Inflatable Life-Rafts: Exercises are being carried out at the Survival Training School H.M.S. Siskin RN. Air Station, Goport to demonstrate the methods of rescue and survival of the crashed air-arm pilots and shipwrecked seamen. One of the items demonstrated is a man life-raft which is rather like an inflates tented dinghy. A container of compressed carbon-dioxide inflates the dinghy ten seconds. A cover of rubberized cotton fabric is then erected on a 54 inch mast - and buttoned down of afford protection from exposure the dinghy is complete with everything needed for survival in the roughest weather
Max Dietrich Kley (Chairman of the Association of Industrial Energy and Power Industries e.V.)..., 1995 (photo)
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