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1,365 médias trouvés pour 'Surface View'

The Etang des Soeurs, Osny, near Pontoise, c.1875 (oil on canvas)
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The Colonization of Mars-Illustration - Mars Colony - Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars
View of city M'banza-Kongo, capital of kingdom of Congo, from Description of Africa, by Olfert Dapper (ca 1635-1689), engraving, 1686
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Earth at the end of Permian - Ring arcs over the Permian Earth - A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have either fallen or fallen back to Earth in a meteorite rain. A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today. 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune. Unlike Neptune's rings, the ring arcs around the Earth were of terrestrial origin, debris thrown into orbit by a collision with a large meteorite or comet. The debris consisted of tiny pebbles that were once molten droplets of ejecta, long since cooled in the vacuum of space. The orbit of the ring arc would eventually decay, returning the debris back to Earth as a shower of meteorites. This debris is found on Earth's surface today in the form of dark, glassy objects known as tektites
Painting with Spikes - Composition no. 223, by Wassily Kandinsky, 1919, 20th Century, oil on canvas, 126 x 95 cm
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Telescope E-ELT -Artist's view - E-ELT concept: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 39 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. The Cerro Amazones mountain in the Chilean desert, near Eso's Paranal Observatory, will be the site for the European Extremely Large Telescope (E-ELT), which, with its 39-metre diameter mirror, will be the world's biggest eye on the sky. Here, an artist's rendering shows how the telescope will look on the mountain when it is complete in 2024
Chambord Castle (photo)
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Lighting Interior or Interior with Woman in a Wicker Chair (Intèrieur clair ou Intèrieur avec une femme dans un fauteuil d'osier), by Pierre Bonnard, 1920, 20th Century, oil on canvas, 72 x 51 cm
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Large Composition A with Black, Red, Gray, Yellow and Blue, 1919-1920 (oil on canvas)
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Ice on the Moon - Illustration - Lunar ice - Illustration - Artist's view of ice on the surface of a crater that remains perpetually in the shade of the Sun, near the poles. Water from an encounter with an icy comet has collected in the perpetual shade of a deep crater where the temperature is a constant - 380o F. In 1998, the unmanned Lunar Prospector probe discovered evidence for water ice on the surface of the moon. Some scientists believe that as much as 10 to 300 million tons of ice may reside at the moon's North and South poles. The source of the ice is thought to be from one or more comets that struck the moon's surface four billion years ago. (It is thought that Earth's water may have come from comets as well.) Unfortunately, the moon's small size and lack of an atmosphere caused it to lose almost all of its accumulated water to space. Any water that does remain on the moon would likely be on the poles, hidden in craters and depressions shaded from the Sun
Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet
Temptation on Mount, detail from Episodes from Christ's Passion and Resurrection, reverse surface of Maesta' of Duccio Altarpiece in Cathedral of Siena, by Duccio di Buoninsegna (ca 1255 - pre-1319), tempera on wood, 1308-1311
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Verso: The muscles of the leg, c.1508 (pen & ink over black chalk on paper)
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Lunar base - Illustration - Lunar base - Illustratio
Ms. Andrèe Bonnard with her dogs (Mademoiselle Andrèe Bonnard avec ses chiens), by Pierre Bonnard, 1890, 19th Century, oil on canvas, 188 x 80 cm
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A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have fallen or fallen to Earth in a meteorite rain - A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today - 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune . Unlike Neptune's rings, the ring arcs around the Earth were of terrestrial origin, debris thrown into orbit by a collision with a large meteorite or comet. The debris consisted of tiny pebbles that were once molten droplets of ejecta, long since cooled in the vacuum of space. The orbit of the ring arc would eventually decay, returning the debris back to Earth as a shower of meteorites. This debris is found on Earth's surface today in the form of dark, glassy objects known as tektites.: La Terre à la fin du Permien - Ring arcs over the Permian Earth
View of the port of Sofala, Mozambique, engraving, 18th century
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Misia Godebska and Thadèe Natanson (Misia Godebska et Thadèe Natanson), by Pierre Bonnard, 1902, 20th Century, oil on canvas, 103 x 86 cm
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The Earth 650 million years ago - Artist's view - Snowball Earth - The Earth seen in a period of glaciation (Varanger glaciation), about 650 to 630 million years ago. This is how the Earth may have appeared about 650 million years ago during a period when snow and ice may have covered most, if not all, of the Earth's surface and oceans. This image suggests the Earth's appearance during the Marinoan glaciation from 650 to 630 million years ago. The southern and eastern hemispheres are dominated by glacier - covered land masses while the opposing hemisphere is frozen ocean save for a few areas of exposed liquid water, AKA refugia for the Earth's surviving soft - bodied multicellular organisms. In addition to the Marinoan glaciation there may have been at least two, and possibly three previous Proterozoic glacial periods going back to two billion years ago. The causes of these snowball periods are unknown but may have been due to massive volcanic eruptions, massive meteoritic impacts (both resulting in global sun - reflecting ash clouds), or variance's in the Earth's orbit
Mud Cracks, 1955 (silver gelatin print)
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Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity. Orbiting 14,600 miles above Mars' surface, Deimos completes one revolution every 30 hours
Jupiter seen from its satellite Europe - Illustration - Jupiter & Io from Europa's surface - Illustration - Jupiter and Io seen from the ice surface of the satellite Europe. The surface of Europe is about five times brighter than our Moon. A crescent Jupiter hovers near the horizon along with Jupiter's volcanic satellite Io. In the foreground a meandering crevasse cleaves Europa's icy surface, one of thousands that crisscross this moon's exceedingly flat and bright exterior. The surface of Europa is about five times brighter than our own Moon and is so flat that no feature rises more than 3,000 feet
View of satellites and debris in low orbit around the Earth - Objects in low - Earth orbit - View over Ecuador 80 per cent of recenses are in low orbit up to 2000 km above Earth. Objects in low - Earth orbit (LEO). View over the equator. Eighty percent of all catalogued objects are in low - Earth orbit (LEO), which extends to 2000 km above the Earth's surface. To observe the Earth, spacecraft must orbit at such a low altitude. The spatial density of objects increases at high latitudes
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
Plain of Rephaim from Zion, 1855 (w/c, bodycolour & surface scratching)
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The Gallant Indies (Les Indes galantes), by Frank Stella, 1966, 20th century, acrilic on canvas
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The Earth from space
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Ambroise Vollard with his Cat (Ambroise Vollard avec son chat), by Pierre Bonnard, 1904 - 1905, 20th Century, oil on canvas, 74 x 92.5 cm
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Earth and Moon - Apollo 8 - Dec. 1968 - Earthrise from Apollo 8 spacecraft - Earthrise seen from the control module of Apollo 8 on 22/12/1968. This view of the rising Earth greeted the Apollo 8 astronauts as they came from behind the Moon after the lunar orbit insertion burn. Earth is about five degrees above the horizon in the photo. The unnamed surface features in the foreground are near the eastern limb of the Moon as viewed from Earth. The lunar horizon is approximately 780 kilometers from the spacecraft. Width of the photographed area at the horizon is about 175 kilometers. December 22 1968
Artist's view of a first human crew on Mars - Martian Pioneers - The first human visitors to Mars would face an environment nearly as hostile as the Earth's Moon. While Mars has an atmosphere, it contains no breathable oxygen and is so thin that the surface air pressure is about the same as the Earth's 18 miles above sea level. To venture outside, humans would need hardy suits that would supply pressure, oxygen, moisture, warmth, and insulate them from the fine martian dust that may be both abrasive and caustic. Even with these precautions, humans would still be vulnerable to radiation from solar storms and the continual rain of interstellar cosmic rays
Satellite METOP - A - Artist's view of the European satellite METOP - A in orbit around the Earth. Launch on October 19, 2006, it is the first European meteorological satellite in polar orbit; it includes twelve meteorological instruments. MetOp is a series of three meteorological operational polar orbiting satellites, the first of which, MetOp-1 is the prototype. The instruments on MetOp will produce high - resolution images, vertical temperature and humidity profiles, and temperatures of the land and ocean surface on a global basis. Also on board the satellites will be instruments for monitoring ozone and wind flow over the oceans. The first launch was on October 19 2006
The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Scenario of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere
Nude in Front of the Mantlepiece (Jeune fille nue devant la cheminèe ou Nu devant la cheminèe), by Pierre Bonnard, 1919, 20th Century, oil on canvas, 49 x 118 cm
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Cafè Interior: Afternoon, by Patrick Caulfield, 1973, 29th Century, acrylic on canvas, 213 x 213 cm
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Earth as seen from the Moon - Illustration - Earth as seen from the Moon - Illustration
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Lunar base -Illustration - Lunar base - Illustratio
Belugas in the mouth of the Cunningham Inlet estuary, July 2000 (photo)
Mars Exploration Rover - Mars Exploration Rover is a Martian exploration mission composed of two probes housing two identical rovers, Spirit and Opportunity MER - A, the Spirit robot launched on June 10, 2003, landed on January 3, 2004 in the crater Gusev. MER - B, the Opportunity robot launched on July 8, 2003, landed on January 24, 2004 on Meridiani Planum. The sun rises behind one of the Mars Exploration Rovers as it prepares to analyse a rock with its RAT tool. Mars Exploration Rover (MER) is a robotic mission which aims to explore the Martian surface and geology. The mission began with the sending of two twin rovers: MER - A (Spirit), launched on June 10 2003 and landed on January 03 2004 in Gusev crater; MER - B (Opportunity) launched on July 08 2003 and landed on January 24 2004 at Meridiani Planum
Surface de Mercure - Artist View - Pit-like features on Mercury
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A view of the Apollo 11 lunar module Eagle as it returned from the surface of the moon
View of Basilica of Our Lady of Peace (1985-1989), Yamoussoukro, Lagunes region, Ivory Coast
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Fort Lauderdale Coastline Aerial (photo)
Apollo 16: scientific instruments - Apollo 16: scientific instruments - Partial view of the scientific station (ALSEP) installed on the Moon, with the PSE (Passive Seismic Experiment). 21/04/1972. A partial view of the Apollo 16 Apollo Lunar Surface Experiments Package (ALSEP) in deployed configuration on the lunar surface as photographed during the mission's first extravehicular activity (EVA - 1), on April 21, 1972. The Passive Seismic Experiment (PSE) is in the foreground center; Central Station (C/S) is in center background, with the Radioisotope Thermoelectric Generator (RTG) to the left. One of the anchor flags for the Active Seismic Experiment (ASE) is at right
Saturn above the clouds of Titan - Illustration - Saturn from atop Titan's hydrocarbon haze - Artist's view of the planet Saturn view 80 km above the surface of his satellite Titan. In the plane of the rings of the planet appear from left to right the satellites Enceladus, Dione, Tethys and Rhea. Saturn and its rings would be a majestic sight lording over Titan's hydrocarbon haze. The viewpoint is from 50 miles above Titan's surface and three - quarters of a million miles away from Saturn itself. Four of Saturn's smaller satellites can also be seen along the ring plane: left to right are Enceladus, Dione, Tethys and Rhea. Technically, the orange clouds mark the beginning of Titan's condensate haze, which consists of ethane, methane, nitrogen, and a variety of hydrocarbons known collectively as tholin. These gases and hydrocarbons extend upward another 250 miles, resulting in a bluish, earthlike sky, albeit darker due to Titan's great distance from the Sun. Tholin is created by the interaction of the nitrogen - rich gases with ultraviolet light from the Sun and ultimately precipitates all the way down to Titan's surface. Notwithstanding its flame - like colors, this haze is chilled to minus 330o F
Switzerland Seegfroerni Lake Constance, 1963 (b/w photo)
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Stream of Tenderness, by Piero Dorazio, 1958, 20th Century, oil on canvas, 100.5 ? 180.8 cm
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Astronauts and Geyser on Enceladus - Artist view - Astronauts and Water geyser on Enceladus - Artist view: Two astronauts explore the surface of the Enceladus satellite
Apollo 15: Lunar Jeep - Apollo 15: Lunar Roving Vehicle (LRV) - Lunar Roving Vehicle (LRV). 02/08/1971. The Lunar Roving Vehicle is photographed alone against the lunar background during the third Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley - Apennine landing site. This view is looking north. The west edge of Mount Hadley is at the upper right edge of the picture. Mount Hadley is at the upper right edge of the picture. It rises approximately 4,500 meters (about 14,765 feet) above the plain. The most distant feature visible is approximately 25 kilometers (about 15.5 statute miles) away
Astronauts and Geyser on Enceladus - Artist view - Astronauts and Water geyser on Enceladus - Artist view: Two astronauts explore the surface of the Enceladus satellite
Surface 275 (Superficie 275), by Giuseppe Capogrossi, 1957, 20th Century, oil on canvas, 97 x 145 cm
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Cross-section view of the Earth - Earth cutaway - Internal structure of the Earth. On the surface, the crust forms a bark of about 7 km under the oceans and 30 to 40 km under the continents. Below is the mantle, a 2900 km thick rock belt. The outer core is composed of liquid metal, mainly iron and nickel. The inner core, or seed, is composed of the same alloy but is solid. Art cutaway of Earth showing interior structure. The surface is a crust, a thin layer of solid rock about 7 km thick under the oceans and 30 to 40 km thick where there are continents. Below is the mantle, 2900 km thick layer of molten rock. The outer core consists of liquid metal, mostly iron and nickel. The inner core has a similar composition but is solid
The Dawn probe near Ceres - Artist's view - Dawn approaches Ceres - Artist view of the Dawn probe near the dwarf planet Ceres. In February 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn's three xenon electrostatic ion thrusters can be seen emitting ionized xenon's characteristic blue/magenta glow, gently propelling the probe toward Ceres. While the ion engines have relatively low specific thrust (about equal to the weight of a few sheets of paper), they can operate continuously for long periods making efficient use of the approximately 1,000 pounds of xenon propellant onboard. The wing - like solar arrays produce about 1,300 watts for probe's propulsion and other electrical systems. While no close - up observations of yet been made of Ceres itself, here it is rendered as appearing similar to a much smaller version of the Earth's Moon, heavily cratered with the addition of surface water ice and hypothesized plumes of ice crystals from water geysers on its surface
ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support communications
Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth
Globe of the Moon.
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Apollo 11: Descent of Armstrong on the Moon - Apollo 11: N.Armstrong close to the first moonwalk - Neil A. Armstrong, on the LEM scale, is about to take the first step on the Moon. 20/07/1969. Astronaut Neil A. Armstrong, Apollo 11 commander, descends the ladder of the Apollo 11 Lunar Module prior to making the first step by man on the moon. This view is a black and white reproduction taken from a telecast by the Apollo 11 lunar surface camera during extravehicular activity. The black bar running through the center of the picture is an anamoly in the television ground data system at the Goldstone Tracking Station
Methane lake on Titan - Artist view
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'Earthrise - Apollo 8', 29 December 1968
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The Hunters in the Snow (Jagers in de Sneeuw), by Pieter Bruegel the Elder, 1565, 16th Century, oil on wood, 117 x 162 cm
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Earth - The geoid - Earth's geoid - The Earth's geoid, an image of the inegalites of the Earth's gravitation field. Image centred on Indonesia. Image obtained by the GOCE satellite in 2011. ESA's GOCE mission has delivered the most accurate model of the 'geoid' ever produced, which will be used to further our understanding of how Earth works. A precise model of Earth's geoid is crucial for deriving accurate measurements of ocean circulation, sea - level change and terrestrial ice dynamics. The geoid is also used as a reference surface from which to map the topographical features on the planet. In addition, a better understanding of variations in the gravity field will lead to a deeper understanding of Earth's interior, such as the physics and dynamics associated with volcanic activity and earthquakes
Mine sur un asteroide - Illustration - Mining base on double asteroid 90 Antiope - Illustration - Artist view une base minere installee sur l'asteroid double 90 Antiope. Some day a it may be worthwhile to mine resources from a distant asteroid, whether for raw materials for building an orbiting structure (cheaper than rocketing the materials from Earth's surface) or for some exotic material found only on a particular asteroid. This image is a bird's eye view of a mining settlement on the double asteroid 90 Antiope, located in the main asteroid belt between the orbits of Mars and Jupiter. These two asteroids are about the same size - - 70 miles across - - and orbit around a common center like two ends of a barbell. The gap separating the two bodies is only about 40 miles. The extremely low surface gravity would permit the construction of delicate structures, such as the solar power array silhouetted against the sunny side of the sister asteroid, and would make it relatively easy to transport mined material off the surface