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Images of 'Methane' found, 199

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Penitent, or Fireman

Penitent, or Fireman

UIG863766

Gas explosion in a coal mine (colour litho)

Gas explosion in a coal mine (colour litho)

French School, (19th century)

LLM2818279

Firedamp Explosion in the Mines at Saint-Etienne, from 'Le Petit Parisien', 20th December 1891 (litho)

Firedamp Explosion in the Mines at Saint-Etienne, from 'Le Petit Parisien', 20th December 1891 (litho)

Dete, Beltrand and Clair-Guyot, E. (fl. 1884)

STC373776

Exploration of Titan - Illustration - Looking for life on Titan - An automatic probe explores a hydrocarbon marsh in search of traces of life. A robotic probe explores a frigid ethane lake on Titan. Like the European Space Agency's Huygens probe, this probe carries its own light source as the surface of Titan is only 0.1 percent as bright as the Earth's. Titan is host to a plethora of organic (carbon - based) compounds, hence this is one of the few places in the Solar System where life outside of the Earth may have evolved. In many ways, Titan resemble a frozen primordial Earth, though the greatest obstacle to Titan harboring life - - as we know it - - is the extreme cold. Even though all the chemical ingredients are present, Titan simply may not be warm enough to initiate the chemical reactions required for life. Perhaps sometime in the next decades such a mission to Titan will be a reality

Exploration of Titan - Illustration - Looking for life on Titan - An automatic probe explores a hydrocarbon marsh in search of traces of life. A robotic probe explores a frigid ethane lake on Titan. Like the European Space Agency's Huygens probe, this probe carries its own light source as the surface of Titan is only 0.1 percent as bright as the Earth's. Titan is host to a plethora of organic (carbon - based) compounds, hence this is one of the few places in the Solar System where life outside of the Earth may have evolved. In many ways, Titan resemble a frozen primordial Earth, though the greatest obstacle to Titan harboring life - - as we know it - - is the extreme cold. Even though all the chemical ingredients are present, Titan simply may not be warm enough to initiate the chemical reactions required for life. Perhaps sometime in the next decades such a mission to Titan will be a reality

Walter B Myers

PIX4626138

Methane (CH4) also called Marsh Gas or Ignis Fatuus, causing a dancing light in swampy ground known as Will-o-the-Wisp or Jack-o-Lantern. Observed 1811.

Methane (CH4) also called Marsh Gas or Ignis Fatuus, causing a dancing light in swampy ground known as Will-o-the-Wisp or Jack-o-Lantern. Observed 1811.

UIG865303

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

PIX4606969

Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Earth. Unlike cirrus clouds on Earth however, which are composed of crystals of water ice, Neptune's cirrus clouds are made up of crystals of frozen methane. Neptune's clouds are driven by winds of 1,200 mph, the fastest winds of any planet in the Solar System — Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Ear

Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Ear

Walter B Myers

PIX4624042

Methane lake on Titan - Artist view

Methane lake on Titan - Artist view

Miller, Ron (b.1947)

PIX7223439

The electric gun of Alessandro (Alexandre) Volta used to ignite methane. Museum of Science and Technology, Milan.

The electric gun of Alessandro (Alexandre) Volta used to ignite methane. Museum of Science and Technology, Milan.

Volta, Alessandro (1745-1827)

Giancarlo Costa

GIA4744271

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

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

Walter B Myers

PIX4624014

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the TGO probe (Trace Gas Orbiter) of the European mission ExoMars 2016. ExoMars Trace Gas Orbiter at Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the TGO probe (Trace Gas Orbiter) of the European mission ExoMars 2016. ExoMars Trace Gas Orbiter at Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

PIX4606979

Pluto's Atmosphere - Artist's View - Pluto's Atmosphere - Pluto's Artist's View surrounded by its thin atmosphere. In 1985 it was discovered that Pluto has an atmosphere, albeit a very tenuous one. Pluto's atmosphere arises only when it approaches closer to the Sun during its highly eccentric, 248 earth years long orbit. The atmosphere likely consists of nitrogen, methane, and carbon monoxide, which sublimate directly from Pluto's frozen surface. As Pluto's orbit moves it away from the Sun, these gases are believed to slowly precipitate back to Pluto's surface

Pluto's Atmosphere - Artist's View - Pluto's Atmosphere - Pluto's Artist's View surrounded by its thin atmosphere. In 1985 it was discovered that Pluto has an atmosphere, albeit a very tenuous one. Pluto's atmosphere arises only when it approaches closer to the Sun during its highly eccentric, 248 earth years long orbit. The atmosphere likely consists of nitrogen, methane, and carbon monoxide, which sublimate directly from Pluto's frozen surface. As Pluto's orbit moves it away from the Sun, these gases are believed to slowly precipitate back to Pluto's surface

Walter B Myers

PIX4624547

Neptune seen by Voyager 2 1989 - Image of Neptune obtained by the Voyager 2 probe at 16 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, a small shiny cloud of irregular shape moving very quickly, nicknames the scooter

Neptune seen by Voyager 2 1989 - Image of Neptune obtained by the Voyager 2 probe at 16 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, a small shiny cloud of irregular shape moving very quickly, nicknames the scooter

PIX4622792

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view: Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). TGO has been in orbit around Mars since October 19, 2016. The Schiaparelli module was lost after separation. Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO was launched on March 14 2016 with Schiaparelli. TGO orbits March since October 19 2016. Schiaparelli was lost after separation. TGO searches for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2020

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view: Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). TGO has been in orbit around Mars since October 19, 2016. The Schiaparelli module was lost after separation. Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO was launched on March 14 2016 with Schiaparelli. TGO orbits March since October 19 2016. Schiaparelli was lost after separation. TGO searches for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2020

PIX4643703

Yagua tribe located near Iquitos, Amazonian, Peru, 2022 (photography)

Yagua tribe located near Iquitos, Amazonian, Peru, 2022 (photography)

Sergi Reboredo

SRB7333185

Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The bright clouds immediately to the south and east of this oval are seen to substantially change their appearances in periods as short as four hours. The second dark spot, at 54 degrees south latitude near the terminator (lower right edge), Neptune circuits every 16.1 hours. This image has been processed to enchance the visibility of small features, at some sacrifice of color fidelity — Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

PIX4622787

Artist's view of the New Horizons probe near Pluto - New Horizons over Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft over dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 10,000 miles from Pluto (upper right), 22,000 miles from its largest moon Charon (upper left) and 2.97 billion miles from the Earth. Dominating this side of the spacecraft with an 8 inch aperture is the Long - Range Reconnaissance Imager (LORRI), a digital camera with a large telephoto telescope fortified to operate in the cold, hostile environs of deep space. At 90 days before closest approach to Pluto, Lorri's images will surpass the quality of the best Hubble Space Telescope images of Pluto. While little is known about Pluto's appearance, here this Kuiper belt dwarf planet is realized as a frozen world covered with various ices, hosting a thin atmosphere of nitrogen, methane and other hydrocarbons too possibly, with a significantly weathered surface as Pluto's 248 - year orbit alternately brings it closer then further from the warmth of the sun — Artist's view of the New Horizons probe near Pluto - New Horizons over Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft over dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 10,000 miles from Pluto (upper right), 22,000 miles from its largest moon Charon (upper left) and 2.97 billion miles from the Earth. Dominating this side of the spacecraft with an 8 inch aperture is th

Artist's view of the New Horizons probe near Pluto - New Horizons over Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft over dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 10,000 miles from Pluto (upper right), 22,000 miles from its largest moon Charon (upper left) and 2.97 billion miles from the Earth. Dominating this side of the spacecraft with an 8 inch aperture is th

Walter B Myers

PIX4607329

Alexander Volta (engraving)

Alexander Volta (engraving)

Italian School, (19th century)

LLE815838

Clouds on the south pole of Titan - Illustration - Clouds over Titan's south pole - Artist's view of methane clouds observed over the south pole of Titan by the Cassini probe in October 2004. In October 2004 the Cassini orbiter revealed for the first time what may be highly reflective (in the infrared at least) methane clouds over Titan's south pole. This image suggests how those clouds may appear from within the cloud deck itself. The Sun is visible immediately above, though from this great distance the Sun appears to be only 1/10th its diameter from Earth

Clouds on the south pole of Titan - Illustration - Clouds over Titan's south pole - Artist's view of methane clouds observed over the south pole of Titan by the Cassini probe in October 2004. In October 2004 the Cassini orbiter revealed for the first time what may be highly reflective (in the infrared at least) methane clouds over Titan's south pole. This image suggests how those clouds may appear from within the cloud deck itself. The Sun is visible immediately above, though from this great distance the Sun appears to be only 1/10th its diameter from Earth

Walter B Myers

PIX4626063

Safety lamps designed by Humphry Davy for use by miners

Safety lamps designed by Humphry Davy for use by miners

Basire, James, the younger (1769-1822)

XOS1766096

Methane Canyon and River on Titan - Artist View - Titan canyon and methane river: Artist view of the surface of the Titan satellite. The Cassini probe confirmed that lakes and rivers of methane or ethane exist on its surface

Methane Canyon and River on Titan - Artist View - Titan canyon and methane river: Artist view of the surface of the Titan satellite. The Cassini probe confirmed that lakes and rivers of methane or ethane exist on its surface

Miller, Ron (b.1947)

PIX4626163

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange areas are thought to be evaporite - the Titan equivalent of salt flats on Earth. The evaporated material is thought to be organic chemicals originally from Titan's haze particles that once dissolved in liquid methane. They appear orange in this image against the greenish backdrop of Titan's typical bedrock of water ice - In this mosaic, Kraken Mare, which is Titan's largest sea and covers about the same area as Earth's Caspian Sea and Lake Superior combined, can be seen spreading out with many tendrils on the upper right,. The big dark zone up and left of Kraken is Ligeia Mare, the second largest sea. Below Ligeia, shaped similar to a sports fan's foam finger that points just up from left, is Punga Mare, the third largest Titan Sea. Numerous other smaller lakes dot the area. Titan's north pole is located in the geographic location just above the end of the “” finger”” of Punga Mare. The data shown here were obtained by Cassini's visual and infrared mapping spectrometer during — Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

PIX4625336

Oil Lake on Titan - Titan's ethane ocean - Artist's view of a hydrocarbon lake (methane - ethane) on the surface of Titan. Compared to the Earth, Titan is very far from the Sun's warming rays - - about ten times further - - and this leaves Titan a very cold world. Titan has an average surface temperature of minus 290o F. If there is any water on Titan it is frozen hard as steel, yet Titan may be the only body in the Solar System besides the Earth that harbors a liquid ocean. Titan's ocean would not be one of water, rather it would probably be composed of (very cold) liquid ethane. (On the Earth we know ethane as a colorless, odorless, nontoxic, flammable gas, a constituent of natural gas and petroleum.) If this werenn't exotic enough, immediately beneath this ocean may lie hundreds of feet of frozen acetylene (a common component of welder's torches)

Oil Lake on Titan - Titan's ethane ocean - Artist's view of a hydrocarbon lake (methane - ethane) on the surface of Titan. Compared to the Earth, Titan is very far from the Sun's warming rays - - about ten times further - - and this leaves Titan a very cold world. Titan has an average surface temperature of minus 290o F. If there is any water on Titan it is frozen hard as steel, yet Titan may be the only body in the Solar System besides the Earth that harbors a liquid ocean. Titan's ocean would not be one of water, rather it would probably be composed of (very cold) liquid ethane. (On the Earth we know ethane as a colorless, odorless, nontoxic, flammable gas, a constituent of natural gas and petroleum.) If this werenn't exotic enough, immediately beneath this ocean may lie hundreds of feet of frozen acetylene (a common component of welder's torches)

Walter B Myers

PIX4626096

Oil Marsh on Titan - Ethane swamp on Titan - Artist's view of an ethane marsh on the surface of Titan. Initially astronomers thought that Titan's entire surface may be covered by a liquid hydrocarbon ocean. More recent observations in infrared wavelengths suggest otherwise. In this image the artist is suggesting that Titan may be host to extremely cold ethane - methane swamps

Oil Marsh on Titan - Ethane swamp on Titan - Artist's view of an ethane marsh on the surface of Titan. Initially astronomers thought that Titan's entire surface may be covered by a liquid hydrocarbon ocean. More recent observations in infrared wavelengths suggest otherwise. In this image the artist is suggesting that Titan may be host to extremely cold ethane - methane swamps

Walter B Myers

PIX4626110

Methane lake in effervescence on Titan - Artist's view - Effervescent Sea on Titan - Artist's view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Gas bubbles emanating from the depths could form there.

Methane lake in effervescence on Titan - Artist's view - Effervescent Sea on Titan - Artist's view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Gas bubbles emanating from the depths could form there.

Miller, Ron (b.1947)

PIX4626240

Surface of Titan seen by Huygens - Illustration - Titan Emerges - Artist's view of the surface of Titan as it appeared at the European probe Huygens on January 14, 2005 when it descended, about 20 km from the ground. This is how the surface of Titan may have appeared to the European Space Agency's Huygens probe when it emerged from the satellite's ubiquitous hydrocarbon haze about 12 miles above Titan's surface. Huygens made its historic decent on 14 January 2005, making it the first man - made object to reach the surface of the satellite of another planet

Surface of Titan seen by Huygens - Illustration - Titan Emerges - Artist's view of the surface of Titan as it appeared at the European probe Huygens on January 14, 2005 when it descended, about 20 km from the ground. This is how the surface of Titan may have appeared to the European Space Agency's Huygens probe when it emerged from the satellite's ubiquitous hydrocarbon haze about 12 miles above Titan's surface. Huygens made its historic decent on 14 January 2005, making it the first man - made object to reach the surface of the satellite of another planet

Walter B Myers

PIX4626018

Riviere de Methane sur Titan - Artist's view - Titan methane river delta: Artist's view of the surface of the Titan satellite. The Cassini probe confirmed that lakes and rivers of methane or ethane exist on its surface

Riviere de Methane sur Titan - Artist's view - Titan methane river delta: Artist's view of the surface of the Titan satellite. The Cassini probe confirmed that lakes and rivers of methane or ethane exist on its surface

Miller, Ron (b.1947)

PIX4626180

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - which indicates that the sea was larger at some point in the past and has become smaller due to evaporation. The deposits are material left behind after the methane & ethane liquid evaporates, somewhat akin to the saline crust on a salt flat — Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - whi

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - whi

PIX4625340

Geyser on Titan - Artist view - Cryogeyser on Titan - Artist view - Artist view of geyser on the surface of Titan, Saturn's largest satellite

Geyser on Titan - Artist view - Cryogeyser on Titan - Artist view - Artist view of geyser on the surface of Titan, Saturn's largest satellite

Miller, Ron (b.1947)

PIX4974163

Riviere de Methane sur Titan - Artist's view - Titan methane river delta: Artist's view of the surface of the Titan satellite. The Cassini probe confirmed that lakes and rivers of methane or ethane exist on its surface

Riviere de Methane sur Titan - Artist's view - Titan methane river delta: Artist's view of the surface of the Titan satellite. The Cassini probe confirmed that lakes and rivers of methane or ethane exist on its surface

Miller, Ron (b.1947)

PIX4626183

Ice volcano on Titan - Artist view - Titan Ice Volcano

Ice volcano on Titan - Artist view - Titan Ice Volcano

Miller, Ron (b.1947)

PIX4626243

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Miller, Ron (b.1947)

PIX4626037

Titan Exploration - Illustration - Exploring a hydrocarbon swamp on Titan - Automatic balloons fly over an oil marsh on the surface of Titan. A pair of balloon - borne probes leisurely survey a methane - ethane “” swamp”” on Titan. Each probe carries its own spot light illuminating the terrain below, augmenting the haze - filtered sunlight. Scientists have long speculated that methane and ethane may exist as liquids on Titan's extremely cold surface, but it wasn't until 2005 that the Cassini spacecraft's radar imager detected what indeed may be large hydrocarbon lakes on Titan's northern latitudes. While it is believed that the liquid in these lakes would be primarily methane and ethane, this won't be confirmed until the lakes - - if that's indeed what they are - - are actually sampled. Whatever lies on Titan's surface, there is the possibility that the ancient and exotic environment has given rise to compounds heretofore unknown on Earth. Large quantities of Methane and ethane exist in Earth's relatively warm environment as components of natural gas — Titan Exploration - Illustration - Exploring a hydrocarbon swamp on Titan - Automatic balloons fly over an oil marsh on the surface of Titan. A pair of balloon - borne probes leisurely survey a methane - ethane “” swamp”” on Titan. Each probe carries its own spot light illuminating the terrain below, augmenting the haze - filtered sunlight. Scientists have long speculated that methane and ethane may exist as liquids on Titan's extremely cold surface, but it wasn't until 2005 that the Cassini spacecraft's radar imager detected what indeed may be large hydrocarbon lakes on Titan's northern latitudes. While it is believed that the liquid in these lakes would be primarily methane and ethane, this won't be confirmed until the lakes - - if that's indeed what they are - - are actually sampled. Whatever lies on Titan's surface, there is the possibility that the ancient and exotic environment has given rise to compounds heretofore unknown on Earth. Large quantities of Methane and ethane exist i

Titan Exploration - Illustration - Exploring a hydrocarbon swamp on Titan - Automatic balloons fly over an oil marsh on the surface of Titan. A pair of balloon - borne probes leisurely survey a methane - ethane “” swamp”” on Titan. Each probe carries its own spot light illuminating the terrain below, augmenting the haze - filtered sunlight. Scientists have long speculated that methane and ethane may exist as liquids on Titan's extremely cold surface, but it wasn't until 2005 that the Cassini spacecraft's radar imager detected what indeed may be large hydrocarbon lakes on Titan's northern latitudes. While it is believed that the liquid in these lakes would be primarily methane and ethane, this won't be confirmed until the lakes - - if that's indeed what they are - - are actually sampled. Whatever lies on Titan's surface, there is the possibility that the ancient and exotic environment has given rise to compounds heretofore unknown on Earth. Large quantities of Methane and ethane exist i

Walter B Myers

PIX4626117

Titan Radar Map - Titan Surface: The surface of Titan seen on the radar of the Cassini probe. Image centred on the north pole. In blue the lakes and seas of methane and ethane - Radar image of Titan's north polar regions. The regions marked as blue indicate seas (largest areas) and lakes (smaller features). All lakes observed to date lie above 70o latitude

Titan Radar Map - Titan Surface: The surface of Titan seen on the radar of the Cassini probe. Image centred on the north pole. In blue the lakes and seas of methane and ethane - Radar image of Titan's north polar regions. The regions marked as blue indicate seas (largest areas) and lakes (smaller features). All lakes observed to date lie above 70o latitude

PIX4625385

Methane lake on Titan - Artist view - Titan lake - Artist view: Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Methane lake on Titan - Artist view - Titan lake - Artist view: Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Miller, Ron (b.1947)

PIX4626115

Flood on Titan - Artist's view - Titan flash flood: Artist's view of the surface of the Titan satellite. Heavy methane rains can cause sudden flooding. Monsoon-like storms of methane rain have created a flash flood churning through a river channel on Saturn's moon Titan

Flood on Titan - Artist's view - Titan flash flood: Artist's view of the surface of the Titan satellite. Heavy methane rains can cause sudden flooding. Monsoon-like storms of methane rain have created a flash flood churning through a river channel on Saturn's moon Titan

Miller, Ron (b.1947)

PIX4626244

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Methane lake on Titan - Artist view - Titan lake - Artist view - Artist view from the surface of the Titan satellite. The Cassini probe confirmed that methane or ethane lakes exist on its surface. Lakes of liquid methane or exotic hydrocarbons cover the surface of Titan

Steven Hobbs

PIX4626030

Diagram of Plutos interior structure showing rocky and icy core, thin icy water and methane outer layer

Diagram of Plutos interior structure showing rocky and icy core, thin icy water and methane outer layer

DGA572736

Penitent, or Fireman

Penitent, or Fireman

UIG863777

Diagram of Neptunes interior structure showing solid core, icy methane, ammonia and water mantle

Diagram of Neptunes interior structure showing solid core, icy methane, ammonia and water mantle

DGA572735

Titan's south pole - Illustration - At Titan's south pole - Artist's view of Titan's surface near the south pole. Artwork

Titan's south pole - Illustration - At Titan's south pole - Artist's view of Titan's surface near the south pole. Artwork

Miller, Ron (b.1947)

PIX4626050

VOLTA, Alessandro, Count (1745-1827).

VOLTA, Alessandro, Count (1745-1827).

TRK560622

Switzerland Company Emigration (b/w photo)

Switzerland Company Emigration (b/w photo)

Stringer (STR)

KES6253437

Table Showing Flammable Limits of Different Vapors and Gases

Table Showing Flammable Limits of Different Vapors and Gases

AVE6328430

Penitent, or Fireman

Penitent, or Fireman

UIG863790

Laying of the Marsh Gas Tubes, Italy 1956 (b/w photo)

Laying of the Marsh Gas Tubes, Italy 1956 (b/w photo)

UIT6190235

South Staffordshire Coal Field, England

South Staffordshire Coal Field, England

UIG863796

The Senghenydd Colliery disaster, Wales (colour litho)

The Senghenydd Colliery disaster, Wales (colour litho)

Italian School, (20th century)

LLM3097760

Explosion of Fire-damp (methane) in mine

Explosion of Fire-damp (methane) in mine

UIG863771

Explosion of Fire-damp (methane) in mine

Explosion of Fire-damp (methane) in mine

UIG863770

Seaham Colliery, County Durham, England, showing the head gear above the shaft, and work in an active coal seam. The central vignettes show two models of miner's lamp, the Davy, left, which was the more popular, and the Clanny. Below, a boy is operating the ventillating furnace which created a draught in the workings, so preventing a build up of fire-damp (methane). On the right a pit pony pulling wagons has just passed through a trap door, another device to control ventillation. Engraving from The Graphic (London, 28 January 1871).

Seaham Colliery, County Durham, England, showing the head gear above the shaft, and work in an active coal seam. The central vignettes show two models of miner's lamp, the Davy, left, which was the more popular, and the Clanny. Below, a boy is operating the ventillating furnace which created a draught in the workings, so preventing a build up of fire-damp (methane). On the right a pit pony pulling wagons has just passed through a trap door, another device to control ventillation. Engraving from The Graphic (London, 28 January 1871).

UIG526813

Methane lake on Titan - Artist view - Methane lake on Titan - Artist view

Methane lake on Titan - Artist view - Methane lake on Titan - Artist view

Dixon, Don (b.1951)

PIX4626017

Methane lakes on Titan seen by Cassini - Methane lakes on Titan seen by Cassin

Methane lakes on Titan seen by Cassini - Methane lakes on Titan seen by Cassin

PIX4625380

Geyser de methane sur Titan - Artist view - Geyser de methane sur Titan - Vue d'artiste

Geyser de methane sur Titan - Artist view - Geyser de methane sur Titan - Vue d'artiste

Dixon, Don (b.1951)

PIX4625963

A man transporting methane on his bicycle

A man transporting methane on his bicycle

MEP2344752

Tue. 09, 1953 - Blast of a ship in Duisburg - Ruhrort: One methane-gas bottle exploded on the Dutch ship” Rupel” from Rotterdan. The foreship was completely torn open and destroyed by the heavy explosion. The 18-years-old son of the ship-owner Willem Koopmans, Rotterdam, was killed. Until now they do not know why it came to the explosion of the methane-gas.

Tue. 09, 1953 - Blast of a ship in Duisburg - Ruhrort: One methane-gas bottle exploded on the Dutch ship” Rupel” from Rotterdan. The foreship was completely torn open and destroyed by the heavy explosion. The 18-years-old son of the ship-owner Willem Koopmans, Rotterdam, was killed. Until now they do not know why it came to the explosion of the methane-gas.

ZUM4830364

A researcher checks a sealed pot of methane in the electrical generator developed by Kajima Corporat.., 1999-10-14 (photo)

A researcher checks a sealed pot of methane in the electrical generator developed by Kajima Corporat.., 1999-10-14 (photo)

Toshiyuki Aizawa

REU7584121

KAJIMA RESEARCHER CHECKS SEALED POT OF METHANE IN LAST ELECTRICAL GENERATOR IN TOKYO, 1999-10-14 (photo)

KAJIMA RESEARCHER CHECKS SEALED POT OF METHANE IN LAST ELECTRICAL GENERATOR IN TOKYO, 1999-10-14 (photo)

Toshiyuki Aizawa

REU8350148

MINE WORKERS CARRY BODY OF ONE OF EIGHTEEN MEN KILLED IN A METHANE GAS EXPLOSION, 1999-07-30 (photo)

MINE WORKERS CARRY BODY OF ONE OF EIGHTEEN MEN KILLED IN A METHANE GAS EXPLOSION, 1999-07-30 (photo)

Juda Ngwenya

REU8509761

Portrait of Italian physicist Alessandro Volta (1745-1827) credited as the inventor of the electrical battery and the discoverer of methane. 19th century (chromolithograph)

Portrait of Italian physicist Alessandro Volta (1745-1827) credited as the inventor of the electrical battery and the discoverer of methane. 19th century (chromolithograph)

ELD4949736

RESCUE WORKERS ARRIVE AT THE MINE AFTER EIGHTEEN MEN WERE KILLED IN A METHANE GAS EXPLOSION IN ..., 1999-07-30 (photo)

RESCUE WORKERS ARRIVE AT THE MINE AFTER EIGHTEEN MEN WERE KILLED IN A METHANE GAS EXPLOSION IN ..., 1999-07-30 (photo)

Juda Ngwenya

REU8493709

RESCUE WORKERS ARRIVE AT MINE AFTER 18 MEN WERE KILLED IN METHANE GAS EXPLOSION, 1999-07-30 (photo)

RESCUE WORKERS ARRIVE AT MINE AFTER 18 MEN WERE KILLED IN METHANE GAS EXPLOSION, 1999-07-30 (photo)

Juda Ngwenya

REU8475539

Portrait of Alessandro Volta (1745-1827) inventor of the first electric battery (Portrait of italian physicist Alessandro Volta credited as the inventor of the electrical battery and the discoverer of methane) chromolithograph of the beginning of the 20th century

Portrait of Alessandro Volta (1745-1827) inventor of the first electric battery (Portrait of italian physicist Alessandro Volta credited as the inventor of the electrical battery and the discoverer of methane) chromolithograph of the beginning of the 20th century

Unknown Artist, (20th century)

ELD4949644

A fuel highbred concept Jeep, Commander 2, uses methane and fuel cell technology to power it, as Dai.., 2000-10-24 (photo)

A fuel highbred concept Jeep, Commander 2, uses methane and fuel cell technology to power it, as Dai.., 2000-10-24 (photo)

Brendan McDermid

REU8493777

A fuel highbred concept Jeep, Commander 2, uses methane and fuel cell technology to power it, as Dai.., 2000-10-24 (photo)

A fuel highbred concept Jeep, Commander 2, uses methane and fuel cell technology to power it, as Dai.., 2000-10-24 (photo)

Brendan McDermid

REU7558867

Rice terraces plantation near Luang Prabang, Laos, 2022 (photography)

Rice terraces plantation near Luang Prabang, Laos, 2022 (photography)

Sergi Reboredo

SRB7333244

Woman working in the ricefield plantation near Kiet Ngong, Laos, 2022 (photography)

Woman working in the ricefield plantation near Kiet Ngong, Laos, 2022 (photography)

Sergi Reboredo

SRB7333225

Artist's view of the Exoplanet HD 189733b - Artist's impression of exoplanet HD 189733b - Artist's view 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. We discovered water vapor and methane in his atmosphere. Artist's impression of the extrasolar planet HD 189733b, now known to have methane and water. Astronomers used the Hubble Space Telescope to detect methane - - the first organic molecule found on an extrasolar planet. Hubble also confirmed the presence of water vapour in the Jupiter - size planet's atmosphere, a discovery made in 2007 with the help of the Spitzer Space Telescope. They made the finding by studying how light from the host star filters through the planet's atmosphere

Artist's view of the Exoplanet HD 189733b - Artist's impression of exoplanet HD 189733b - Artist's view 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. We discovered water vapor and methane in his atmosphere. Artist's impression of the extrasolar planet HD 189733b, now known to have methane and water. Astronomers used the Hubble Space Telescope to detect methane - - the first organic molecule found on an extrasolar planet. Hubble also confirmed the presence of water vapour in the Jupiter - size planet's atmosphere, a discovery made in 2007 with the help of the Spitzer Space Telescope. They made the finding by studying how light from the host star filters through the planet's atmosphere

PIX4573412

Primitive Earth - Artist's View - Primitive Earth - Artist's View of Earth about 4 billion years ago. Methane was probably abundant in the atmosphere creating persistent fog. The Moon at the time was much closer to Earth than today

Primitive Earth - Artist's View - Primitive Earth - Artist's View of Earth about 4 billion years ago. Methane was probably abundant in the atmosphere creating persistent fog. The Moon at the time was much closer to Earth than today

Dixon, Don (b.1951)

PIX4632682

WORKERS UNLOAD COFFINS FROM A TRUCK IN NOVOKUZNETSK, 1997-12-04 (photo)

WORKERS UNLOAD COFFINS FROM A TRUCK IN NOVOKUZNETSK, 1997-12-04 (photo)

Dima Korotayev

REU8196453

Ice Volcano on Triton - Illustration - Ice volcano on Triton - Cryovolcanoes and geysers of nitrogen and methane have been observed on the surface of the Triton satellite. There is evidence that the south pole of Neptune's satellite Triton is host to dozens of ice volcanoes, or geysers. One such eruption was observed to shoot a towering jet of material to a height of five miles, while the tenuous nitrogen atmosphere carried the smoky plume over 80 miles “” downwind.” The eruptive material is believed to be a combination of liquid nitrogen, dust, and methane compounds driven by seasonal heating from the Sun

Ice Volcano on Triton - Illustration - Ice volcano on Triton - Cryovolcanoes and geysers of nitrogen and methane have been observed on the surface of the Triton satellite. There is evidence that the south pole of Neptune's satellite Triton is host to dozens of ice volcanoes, or geysers. One such eruption was observed to shoot a towering jet of material to a height of five miles, while the tenuous nitrogen atmosphere carried the smoky plume over 80 miles “” downwind.” The eruptive material is believed to be a combination of liquid nitrogen, dust, and methane compounds driven by seasonal heating from the Sun

Walter B Myers

PIX4624061

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-17 (photo)

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-17 (photo)

Tomislav Peternek

REU8257674

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-17 (photo)

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-17 (photo)

Tomislav Peternek

REU8272978

Rice fields near Banteay Srei. Cambodia, 2022 (photography)

Rice fields near Banteay Srei. Cambodia, 2022 (photography)

Sergi Reboredo

SRB7333179

A relative of a dead miner cries over his coffin during the funerals December 5. Sixty-seven Russian.., 1997-12-05 (photo)

A relative of a dead miner cries over his coffin during the funerals December 5. Sixty-seven Russian.., 1997-12-05 (photo)

Dima Korotayev

REU7645726

Rescue workers carry the body of a miner from the Zyryanovskaya mine, in the city of Novokuznetsk De.., 1997-12-03 (photo)

Rescue workers carry the body of a miner from the Zyryanovskaya mine, in the city of Novokuznetsk De.., 1997-12-03 (photo)

Dima Korotayev

REU7567481

Artist's view of the volcano Ganesa Macula on Titan - This formation with a diameter of 180 km, seems to be a cryovolcano, an ice volcano. The surface temperature of Titan is about - 180* C, so the “lava” (a mixture of methane, ammonia and water) flows from it is icy.

Artist's view of the volcano Ganesa Macula on Titan - This formation with a diameter of 180 km, seems to be a cryovolcano, an ice volcano. The surface temperature of Titan is about - 180* C, so the “lava” (a mixture of methane, ammonia and water) flows from it is icy.

M. Carroll

PIX4625925

FUEL HIGHBRED CONCEPT TRUCK MANUFACTURED BY JEEP, 2000-10-24 (photo)

FUEL HIGHBRED CONCEPT TRUCK MANUFACTURED BY JEEP, 2000-10-24 (photo)

Brendan McDermid

REU7896983

UKRAINIAN MINERS IN DONETSK, 1999-05-25 (photo)

UKRAINIAN MINERS IN DONETSK, 1999-05-25 (photo)

Gleb Garanich

REU8379832

Rescue workers load the body of a miner from Zyryanovskaya mine, in the city of Novokuznetsk on a tr.., 1997-12-03 (photo)

Rescue workers load the body of a miner from Zyryanovskaya mine, in the city of Novokuznetsk on a tr.., 1997-12-03 (photo)

Dima Korotayev

REU7645857

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-18 (photo)

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-18 (photo)

Emil Vas

REU8240608

YUGOSLAV MINERS MOURN THE DEATH OF THEIR COLLEAGUES, 1998-01-18 (photo)

YUGOSLAV MINERS MOURN THE DEATH OF THEIR COLLEAGUES, 1998-01-18 (photo)

Emil Vas

REU8271987

MEMBERS OF A RESCUE TEAM CARRY THE BODY OF ONE MINER, 2001-04-26 (photo)

MEMBERS OF A RESCUE TEAM CARRY THE BODY OF ONE MINER, 2001-04-26 (photo)

REU8382567

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-18 (photo)

RELATIVES MOURN THE DEATH OF A MINER KILLED IN YUGOSLAVIA, 1998-01-18 (photo)

Emil Vas

REU8352124

PEOPLE GATHER TO REMEMBER MINERS KILLED IN WESTRAY DISASTER, 2002-05-09 (photo)

PEOPLE GATHER TO REMEMBER MINERS KILLED IN WESTRAY DISASTER, 2002-05-09 (photo)

Jim Young

REU7874284

Biogas: Nepali woman mixing cow urine and manure to make slurry in anaerobic digestion tank to ferment into methane gas, Kahare, Chalnakhel, Kathmandu Valley, Nepal (photo)

Biogas: Nepali woman mixing cow urine and manure to make slurry in anaerobic digestion tank to ferment into methane gas, Kahare, Chalnakhel, Kathmandu Valley, Nepal (photo)

Chinch Gryniewicz

POV3594884

A NURSE FEEDS AN INJURED COAL MINER AT A HOSPITAL IN DONETSK, 2001-01-22 (photo)

A NURSE FEEDS AN INJURED COAL MINER AT A HOSPITAL IN DONETSK, 2001-01-22 (photo)

REU8184774

10/06/2005 Transport public : autobus a methane (ecologique) dans une rue de Rome. Photo Campanini ©AGF/Leemage

FOTO SERENA CAMPANINI/AGF — 10/06/2005 Transport public : autobus a methane (ecologique) dans une rue de Rome. Photo Campanini ©AGF/Leemage FOTO SERENA CAMPANINI/AGF

10/06/2005 Transport public : autobus a methane (ecologique) dans une rue de Rome. Photo Campanini ©AGF/Leemage FOTO SERENA CAMPANINI/AGF

AGF5484785

A UKRAINIAN MINER SITS IN SHUTTLE BUS, 1999-05-25 (photo)

A UKRAINIAN MINER SITS IN SHUTTLE BUS, 1999-05-25 (photo)

Gleb Garanich

REU8296734

FUEL CELLS FROM A HIGHBRED CONCEPT MANUFACTURED BY JEEP, 2000-10-24 (photo)

FUEL CELLS FROM A HIGHBRED CONCEPT MANUFACTURED BY JEEP, 2000-10-24 (photo)

Brendan McDermid

REU7812679

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