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Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water
Voyager and Exoplanets Probe - Voyager entering an alien solar system  Artist's view showing one of the probes approaching another solar system
Artist's view of the 1st discovered exoplanet-51 Peg b - Artwork of 51 Peg b, the first exoplanet discovered: This exoplanet located in the constellation of Pegase, about 48 light years from Earth, is the first discovered exoplanet in 1995. It is a big gas planet very close to its star 51 Pegasi. This type of exoplanet is called a hot Jupiter. Artistic view of 51 Peg b, the first exoplanet discovered in 1995. It is a hot Jupiter type located 48 light-year from the earth in Pegasus constellation
Exoplanete Kepler-64 b: Kepler-64 b or PH1 b (Planet Hunters 1b), is a circumbinary extrasolar planet belonging to the Quadruple Star System Kepler-64 (PH1). PH1b would be a giant gas planet. pH1b (standing for “” Planet Hunters 1””), or by its NASA designation Kepler-64b, is an extrasolar planet found in a circumbinary orbit in the quadruple star system Kepler-64. The giant planet is Neptune-sized, about 20-55 Earth-masses, located 5000 light years from Earth in Cygnus constellation
An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie
Portrait of Sir William Herschel (1738-1822) Astronomer Royal (oil on canvas)
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Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water
Life on a low gravity exoplanet - Life on a low gravity world
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Observation of an exoplanete by interferometry - Observation of an exoplanet with interferometry - Illustration of the principle of direct observation of an exoplanete by interferometry with space telescopes. Places in different places, each telescope observes the light of the star with a slight decay relative to each other. Together these observations would reduce the apparent luminosite of the star and amplify the luminosite of the planet. Optical interferometry combines the light of multiple telescopes to perform the work of a single, much larger telescope. This is possible due to the interaction of light waves, also called interference. Their interaction can be used to cancel out the blinding glare of bright stars or to measure distances and angles precisely
Rover Curiosity on Mars - Curiosity Mars rover selfie - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of images taken by the robot on August 5, 2015. This low-angle self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the site from which it reached down to drill into a rock target called “” Buckskin”” on lower Mount Sharp. The selfie combines several component images taken by Curiosity's Mars Hand Lens Imager (MAHLI) on Aug. 5, 2015, during the 1,065th Martian day, or sol, of the rover's work on Mars. For scale, the rover's wheels are 20 inches (50 centimeters) in diameter and about 16 inches (40 centimeters) wide
Robots envisaged on the red planet
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Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbit around the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three-thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light-years away towards the constellation of Pictor (the Painter) and is one of the best-known examples of a star surrounded by a dusty debris disc. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell-tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 15 times the Earth-Sun separation - or Astronomical Units - which is about the distance Saturn is from the Sun. The planet has a mass of about nine Jupiter masses and is right mass and location to explain the observed warp in the inner parts of the disc
Exoplanete Kepler-70b: Kepler-70b (KOI-55.01) is a confirmed extrasolar planet orbiting the star Kepler-70 (KOI-55), located in the constellation Swan. Kepler-70 b is probably a rocky exoplanet whose surface temperature is one of the warmest known surface temperatures on all exoplanets. Kepler-70b (KOI-55.01) is an exoplanet discovered orbiting the subdwarf B star Kepler-70. It is the hottest exoplanet as of mid-2013, with a surface temperature of 7,143 K (6,870* C)
Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a huge exoplanet with a mass equivalent to 9 times the mass of Jupiter orbit around the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three-thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light-years away towards the constellation of Pictor (the Painter) and is one of the best-known examples of a star surrounded by a dusty debris disc
Detection of an exoplanet by microlens effect - Detection of an exoplanet: Gravitational microlensing - On the left, the observation of a distant star whose light is diluted. On the right, the light of this star is amplified by gravitational lens effect. The gravitational lens effect occurs when the gravitational field of a star acts as a magnifying glass by amplifying the light emitted by a farther star. This amplification is measurable, and when the foreground star is accompanied by a planet, a second peak of intensity in the life rays appears more weakly. Illustration showing at left the observation of faint light emitted by a distant star, at right, the light of the same star magnified by a gravitational lens. Microlensing occurs when the gravitational field of a star acts like a lens, magnifying the light of a distant background star. Possible planets orbiting the foreground star can cause detectable anomalies in the lensing event light curve
Saturn - Illustration - Saturn - Illustration - Artist's view of the planet Saturn. The ring system is composed from the closest to Saturn to the furthest by ring D, then C, B, the division of Cassini, A with the division of Encke, F, G and E. The brightest part of the rings is ring B. This image suggests how Saturn might look from high above the ring plane and at a right angle to the Sun, a perspective that we could never get from the Earth nor from the Hubble Space Telescope
Planet Xena
Exoplanete Kepler-22b: Kepler-22b is an exoplanet orbiting Kepler-22, a star of spectral type G5, similar to the Sun, located about 620 light years (190 pc) from the Solar System in the constellation of Swan. This is the first planet discovered by the Kepler space telescope in the habitable area of a yellow dwarf in December 2011. Kepler-22b is an extrasolar planet orbiting G-type star Kepler-22. It is located 600 light years away from Earth in the constellation of Cygnus. It was discovered by Nasa's Kepler Space Telescope and is the first known transiting planet to orbit within the habitable zone of a Sun-like star
Exoplanete Kepler-186f - Kepler-186f, the first Earth-size Planet in the Habitable Zone: Kepler-186f is the first Earth-size planet in the habitable zone of its star to be discovered. It orbits Kepler-186, a red dwarf located in the constellation of Swan, between 490 and 500 light years of the Earth. Kepler-186f, the first Earth-size Planet in the Habitable Zone. The artist's concept depicts Kepler-186f, the first validated Earth-size planet to orbit a distant star in the habitable zone - a range of distance from a star where liquid water might pool on the planet's surface. The discovery of Kepler-186f confirms that Earth-size planets exist in the habitable zones of other stars and signals a significant step closer to finding a world similar to Earth. The size of Kepler-186f is known to be less than ten percent larger than Earth, but its mass, composition and density are not known. Previous research suggests that a planet the size of Kepler-186f is likely to be rocky. Prior to this discovery, the “” record holder”” for the most “” Earth-like”” planet went to Kepler-62F, which is 40 percent larger than the size of Earth and orbits in its star's habitable zone. Kepler-186f orbits its star once every 130 days and receives one-third the energy that Earth does from the sun, placing it near the outer edge of the habitable zone. If you could stand on the surface of Kepler-186f, the brightness of its star at high noon would appear as bright as our sun is about an hour before sunset on Earth. Kepler-186f resides in the Kepler-186 system about 500 light-years from Earth in the constellation Cygnus. The system is also home to four inner planets, seen lined up in orbit around a host star that is half the size and mass of the sun
Earth 200 million years ago - Artist's view - Early Jurassic Earth - Earth seen at the beginning of the Jurassic, about 200 million years ago. The western hemisphere is representative, the north is up. The Pangee has just split, forming Laurasia to the north and Gondwana to the south. This is how the western hemisphere of the Earth may have appeared 200 million years ago during the Early Jurassic period. North is at the top. During this period continental drift, driven by the massive forces of plate tectonics, had just begun to break the supercontinent of Pangea into Laurasia in the north and Gondwana in the south. In this image the nascent North American continent has just broken away from North Africa while South America and the rest of Africa remain joined as Gondwana. To the west in the global Panthalassa ocean are strips of land corresponding to the Wrangellia Terrane which later merged with western North America
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
Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004
Planetary system around Trappist-1 - Artist's impressions of the TRAPPIST-1 planetary system: Artist's view of extrasolar planets around the red dwarf star TRAPPIST-1. At least seven exoplanets the size of the Earth are orbiting this star 40 light years ago in the constellation Aquarius. All could contain water. This artist's impression shows several of the planets orbiting the ultra-cool red dwarf star TRAPPIST-1. New observations, when combined with very sophisticated analysis, have now yielded good estimates of the densities of all seven of the Earth-sized planets and suggest that they are rich in volatile materials, probably water
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
Exoplanete near a star at the end of life - A dying star sheds its outer layers - An artist's view of a star that, like the Sun at the end of life, turns into a red giant, and expels its upper layers into concentric circles, before becoming a white dwarf. In the foreground, an exoplanet distant from its star that sees its surface reheat. When a star like our sun nears the end of its life, it expands to more than 50 times its original diameter, becoming a red giant. Then over the next several tens of thousands of years the star episodically ejects its outer layers into space, sometimes producing concentric shells. These ejected layers eventually form a planetary nebula. What will subsequently remain of the star is a small, extremely hot core which cools off to become a white dwarf. In this image a red giant star expels its first of many shells of gas into space. In the years to come this spherical shell will grow outward, its circumference eventually expanding far beyond the orbit of this planet. As for this planet, being so far from its parent sun for most of its life has kept it in a deep, dark freeze for the past ten billion years (think Pluto). It has been during only the past 100 million years, when its sun first blossomed into a red giant, that this planet has experienced such light and warmth. This effluence is short - lived, however; in about another million years darkness and cold will again be the norm for this world
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
The Colonization of Mars-Illustration - Mars Colony - Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars
The planet Jupiter, 1880
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Tunguska valley - Artist view (2/3)
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Whole Earth At Night With Country Borders, True Colour Satellite Image
Royal Ms 17 A XLII  ff.68v-69  The Angels of Mars, the Sun and Venus (vellum)
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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
An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration
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Spaceship - Artist's View - Spaceship - Artist vie
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
World map with country borders
Planete extrasolaire - Artist view - Extrasolar planet - Artist vie
Artist's view of an ocean planet - Ocean planet - Artist's view of an exoplanet covered with water on its surface
Artist's view of a hot Jupiter - Exoplanet - Hot Jupiter - Artist's view of a gas giant exoplanet very close to its star. Many of the extra - solar planets which have been discovered in recent years are large, massive, and orbit surprisingly close to their parent stars. These are believed to be gas giant planets similar to Jupiter. Since they're so close to their sun, they're hot. Thus the common term for them has become “” hot Jupiter””. This one is hot enough to glow a dull red even on its night side. The existence of these planets has proven that the arrangement of other solar systems need not closely resemble our own
Exoplanete Kepler - 69c - Kepler - 69c is an exoplanet orbiting Kepler - 69, a star similar to the Sun, located about 2700 light years from the Solar System in the constellation of Swan. Kepler - 69c is a super Earth located in the living area of its star. Artist's concept of planet Kepler - 69c, a super - Earth - size planet (70% larger than Earth). It is the smallest yet found orbiting in the habitable zone of a sun - like star. Its orbit of 242 days resemble that of our neighboring planet Venus
Galaxy in the sky of an exoplanet - Galaxy seen from a rogue planet: Artist's view of a galaxy in the sky of an isolated exoplanet
Artist's View of a Floating Planet - A Floating Planet is a Planet that is not in orbit around an etoil
Exoplanete Trappist-1b - Artist's impression of Trappist-1b: Artist's view of the surface of the extrasolar planet Trappist-1b.
Planete extrasolaire - Artist view - Extrasolar planet - Artist vie
Exoplanete around a binary star - Artist view - Binary Star Exoplanet - Artist rendering
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Exoplanets around a white dwarf - Illustration - White dwarf system - Artwork
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Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering
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Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering
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Exoplanets around Kepler-11: Kepler-11 is a star similar to the Sun, located about 2,000 light years from the Solar System in the constellation Swan. It has a planetary system consisting of at least six exoplanets detected by the Kepler space telescope in 2011. Kepler-11 is a Sun-like star in the constellation Cygnus, located some 2,000 light years from Earth. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size
Exoplanets around a brown dwarf - Artist view - Brown dwarf Exoplanets - Artist rendering
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Exoplanete Tau Bootis b - Tau Booetes b - Artist's view of the extrasolar planet Tau Bootis b view of a hypothetical satellite. Tau Bootis b is located 50 years of light from Earth in the constellation Bovier. It is a gas exoplanet about four times the mass of Jupiter, located very close to its star. The extrasolar planet Tau Booetes b reigns over the airless, baked and battered terrain of a hypothetical moon. Tau Booetes b orbits very close to Tau Booetes, a type F7V star about 50 light years from the Earth. Tau Booetes b is believed to have about four times the mass of the planet Jupiter and orbits around its sun at the astonishing pace of once every 3.3 days. Tau Booetes b is so close to its host sun that the force of the solar wind may be enough to constantly blow off the planet's outer atmosphere
Martian Landscape - Illustration - Martian landscape - Illustration: In the sky the satellites Phobos and Deimos