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Images of 'Orbits' found, 359

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Planetary orbits, 1660-1 (engraving)

Planetary orbits, 1660-1 (engraving)

Cellarius, Andreas (c.1596-1665) (after)

XCF90197

The Situation of the Earth in the Heavens, plate 74 from 'The Celestial Atlas, or the Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-1 (engraving)

The Situation of the Earth in the Heavens, plate 74 from 'The Celestial Atlas, or the Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-1 (engraving)

Cellarius, Andreas (c.1596-1665) (after)

XCF90198

Map Showing Tycho Brahe's System of Planetary Orbits Around the Earth, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, 1660-61 (hand coloured engraving)

Map Showing Tycho Brahe's System of Planetary Orbits Around the Earth, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, 1660-61 (hand coloured engraving)

Cellarius, Andreas (c.1596-1665)

STC129825

Map showing Tycho Brahe's System of Planetary Orbits, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving) (see 129823 for detail)

Map showing Tycho Brahe's System of Planetary Orbits, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving) (see 129823 for detail)

Cellarius, Andreas (c.1596-1665)

STC129824

Diagram showing the solar system, according to Ptolemy (fl.127-145 AD) from the Nuremberg Chronicle by Hartmann Schedel (1440-1514) 1493 (colour woodcut)

Diagram showing the solar system, according to Ptolemy (fl.127-145 AD) from the Nuremberg Chronicle by Hartmann Schedel (1440-1514) 1493 (colour woodcut)

German School, (15th century)

CHT199607

Tycho Brahe (1546-1601), detail from a map showing his system of planetary orbits, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving) (see 129824)

Tycho Brahe (1546-1601), detail from a map showing his system of planetary orbits, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving) (see 129824)

Cellarius, Andreas (c.1596-1665)

XCF266004

'De Revolutionibus Orbium Coelestium' by Nicolaus Copernicus and 'De Libris Revolutionum Nicolai Copernici Narratio Prima' by Georg Johan Rheticus, two works in one volume, Basel, 1566-67 (see also

'De Revolutionibus Orbium Coelestium' by Nicolaus Copernicus and 'De Libris Revolutionum Nicolai Copernici Narratio Prima' by Georg Johan Rheticus, two works in one volume, Basel, 1566-67 (see also

Swiss School, (16th century)

CH495373

Map of the Christian Constellations as depicted by Julius Schiller, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving)

Map of the Christian Constellations as depicted by Julius Schiller, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving)

Cellarius, Andreas (c.1596-1665)

XCF129833

The Ptolemaic System, from 'Description de l'Univers' by Alain Manesson Mallet (1630-1706) 1683 (engraving) (b/w photo)

The Ptolemaic System, from 'Description de l'Univers' by Alain Manesson Mallet (1630-1706) 1683 (engraving) (b/w photo)

French School, (17th century)

CHT223717

The Copernican System, from 'Description de l'Univers' by Alain Manesson Mallet (1630-1706) 1683 (engraving) (b/w photo)

The Copernican System, from 'Description de l'Univers' by Alain Manesson Mallet (1630-1706) 1683 (engraving) (b/w photo)

French School, (17th century)

CHT223715

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 — 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

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

Walter B Myers

PIX4633164

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

L. Bret

PIX4584034

Diagram showing the Earth at the centre of the Universe, according to Ptolemy (fl.127-145 AD) (coloured engraving)

Diagram showing the Earth at the centre of the Universe, according to Ptolemy (fl.127-145 AD) (coloured engraving)

French School, (17th century)

CHT188842

Ptolemaic System, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving)

Ptolemaic System, from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coelestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving)

Cellarius, Andreas (c.1596-1665)

STC129835

Geocentric System of Ptolemee - Ptolemaic Cosmology - Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1660-1661. The mechanism of the heavenly orbits following the hypothesis of Ptolemy. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1660-1661

Geocentric System of Ptolemee - Ptolemaic Cosmology - Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1660-1661. The mechanism of the heavenly orbits following the hypothesis of Ptolemy. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1660-1661

Sebastien Beaucourt

PIX4629486

A diagram of the Solar system, showing the orbits of some of the minor planets, 19th century

A diagram of the Solar system, showing the orbits of some of the minor planets, 19th century

UIG5311319

Asteroides threaten the Earth - Artist view - Asteroids threatening the Earth - Artist view - Title: Space Situational Awareness - Near Earth Objects Picture caption: The SSA-NEO system is based on syndicating and federating observation and tracking data provided by a large number of European and international sources. The key components include: -Observatories and astronomers with telescopes of various sizes, both professional and amateur -A central SSA-NEO data centre, the 'Small Bodies Data Centre', which uses astrometric measurements collected by the Minor Planet Center (USA) -An analysis capability to predict possible impact locations and assess dangers -Analyses related to risk mitigation, including the possible deflection of an asteroid -A system for issuing warnings and alerts to civil authorities in Europe Data on NeOS are collected from telescopes and radar systems worldwide. Each of these submit observations to the Minor Planet Center (MPC), operated by the International Astronomical Union (IAU) at Cambridge, Massachusetts, USA, which acts as a central clearing house for asteroid and comet observations. The measurements collected there are retrieved by the European Small Bodies Data Centre; orbits and miss distances are computed. In case of high-risk impact predictions, the data will be cross-checked with NASA's SENTRY system, operated by the Jet Propulsion Laboratory (JPL), California, before issuing alerts — Asteroides threaten the Earth - Artist view - Asteroids threatening the Earth - Artist view - Title: Space Situational Awareness - Near Earth Objects Picture caption: The SSA-NEO system is based on syndicating and federating observation and tracking data provided by a large number of European and international sources. The key components include: -Observatories and astronomers with telescopes of various sizes, both professional and amateur -A central SSA-NEO data centre, the 'Small Bodies Data Centre', which uses astrometric measurements collected by the Minor Planet Center (USA) -An analysis capability to predict possible impact locations and assess dangers -Analyses related to risk mitigation, including the possible deflection of an asteroid -A system for issuing warnings and alerts to civil authorities in Europe Data on NeOS are collected from telescopes and radar systems worldwide. Each of these submit observations to the Minor Planet Center (MPC), operated by the International Ast

Asteroides threaten the Earth - Artist view - Asteroids threatening the Earth - Artist view - Title: Space Situational Awareness - Near Earth Objects Picture caption: The SSA-NEO system is based on syndicating and federating observation and tracking data provided by a large number of European and international sources. The key components include: -Observatories and astronomers with telescopes of various sizes, both professional and amateur -A central SSA-NEO data centre, the 'Small Bodies Data Centre', which uses astrometric measurements collected by the Minor Planet Center (USA) -An analysis capability to predict possible impact locations and assess dangers -Analyses related to risk mitigation, including the possible deflection of an asteroid -A system for issuing warnings and alerts to civil authorities in Europe Data on NeOS are collected from telescopes and radar systems worldwide. Each of these submit observations to the Minor Planet Center (MPC), operated by the International Ast

P. Carril

PIX4583884

Planisphere. Copernican system, with the Sun, not the Earth at the centre of the solar system. The observed motions of the planets are described in terms of a complex set of circular orbits around the sun, this explaination later being replaced with the more elegant system of eliptical orbits.

Planisphere. Copernican system, with the Sun, not the Earth at the centre of the solar system. The observed motions of the planets are described in terms of a complex set of circular orbits around the sun, this explaination later being replaced with the more elegant system of eliptical orbits.

BL3261850

The Kuiper Belt - Illustration - The Kuiper Belt is an area beyond the orbit of Neptune with small ice bodies. The orbits of planets Jupiter, Saturn, Uranus, Neptune and Pluto are represented

The Kuiper Belt - Illustration - The Kuiper Belt is an area beyond the orbit of Neptune with small ice bodies. The orbits of planets Jupiter, Saturn, Uranus, Neptune and Pluto are represented

P. Carril

PIX4630360

In the asteroid belt: Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

In the asteroid belt: Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

Miller, Ron (b.1947)

PIX4584131

Kepler's concept of an attractive force from the sun - a 'virtue'. His idea of 'gravity' by which he hoped to account for his elliptical planetary orbits was to some extent analogous to magnetism. From Johannnes Kepler Epitome Astronomiae Copernicanae

Kepler's concept of an attractive force from the sun - a 'virtue'. His idea of 'gravity' by which he hoped to account for his elliptical planetary orbits was to some extent analogous to magnetism. From Johannnes Kepler Epitome Astronomiae Copernicanae

UIG541700

Satellite Planck. Illustration - Artist's view of the European satellite Planck separating from the upper floor of the Ariane V rocket, 30 minutes after its launch. This satellite measures temperature fluctuations in the fossil radiation of the primordial universe. Planck separates from upper stage. Planck separated from the launcher about 30 minutes after launch, a couple of minutes after Herschel. The two spacecraft independently headed towards their respective orbits around the second Lagrange point of the Sun - Earth system (L2), some 1.5 million km from Earth in the direction opposite to the Sun. Planck is the first european mission to study the relic radiation from the Big Bang. Ever since the detection of small fluctuations in the temperature of this radiation, called Cosmic Microwave Background, astronomers have used the fluctuations to understand both the origin of the Universe and the formation of galaxies

Satellite Planck. Illustration - Artist's view of the European satellite Planck separating from the upper floor of the Ariane V rocket, 30 minutes after its launch. This satellite measures temperature fluctuations in the fossil radiation of the primordial universe. Planck separates from upper stage. Planck separated from the launcher about 30 minutes after launch, a couple of minutes after Herschel. The two spacecraft independently headed towards their respective orbits around the second Lagrange point of the Sun - Earth system (L2), some 1.5 million km from Earth in the direction opposite to the Sun. Planck is the first european mission to study the relic radiation from the Big Bang. Ever since the detection of small fluctuations in the temperature of this radiation, called Cosmic Microwave Background, astronomers have used the fluctuations to understand both the origin of the Universe and the formation of galaxies

D. Ducros

PIX4646038

Box with Objects (mixed media)

Box with Objects (mixed media)

Cornell, Joseph (1903-72)

JGG117610

European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in the CSG for Soyuz vehicles. Ariane 5 ES, another version of the Ariane 5E featuring a restartable version of Ariane 5G's storable propellant upper stage. One of its primary payloads is the Autonomous Transfer Vehicle (ATV) for resupply and reboost missions to the International Space Station. Ariane 5 ECA, the most powerful version of the Ariane 5E, an evolution of the generic Ariane 5 launcher with an increased propellant load in its solid booster stages and an improved capacity for the liquid oxygen tank of its cryogenic core stage to feed its new Vulcain 2 main engine. The Ariane 5 ECA was first launched on December 11, 2002. Its payload capacity to geostationary transfer orbit reaches 10 metric tons — European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in th

European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in th

D. Ducros

PIX4604567

The Copernican system of the sun, from the 'Harmonia Macrocosmica', published in Amsterdam, 1660 (engraving)d

The Copernican system of the sun, from the 'Harmonia Macrocosmica', published in Amsterdam, 1660 (engraving)d

Cellarius, Andreas (c.1596-1665)

EDI42129

Copernican, Heliocentric, Sun-centred, system of universe showing Jupiter and Saturn with the orbits of their moons. Hand-coloured engraving Paris, 1761

Copernican, Heliocentric, Sun-centred, system of universe showing Jupiter and Saturn with the orbits of their moons. Hand-coloured engraving Paris, 1761

UIG532189

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 — 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 rin

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 rin

Walter B Myers

PIX4669572

Ptolemee Geocentric System - Ptolemaic Cosmology - The orbits of planets around the Earth. Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1708. Planetary orbits around the Earth. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1708

Ptolemee Geocentric System - Ptolemaic Cosmology - The orbits of planets around the Earth. Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1708. Planetary orbits around the Earth. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1708

Sebastien Beaucourt

PIX4629437

Asteroides - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

Asteroides - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

PIX4584096

Geocentric System of Ptolemee - Ptolemaic Cosmology - Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1660-1661. The planisphere of Ptolemy, or the mechanism of the heavenly orbits following the hypothesis of Ptolemy laid out in a planar view. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1660-1661

Geocentric System of Ptolemee - Ptolemaic Cosmology - Engraving from “Harmonia Macrocosmica” by Andreas Cellarius, 1660-1661. The planisphere of Ptolemy, or the mechanism of the heavenly orbits following the hypothesis of Ptolemy laid out in a planar view. Plate of the Harmonia Macrocosmica of Andreas Cellarius, 1660-1661

Sebastien Beaucourt

PIX4629481

Eclipse totale de Soleil 02/1998 - Composite Image, Total Eclipse of the Sun - 1998 - The different phases of the total eclipse of the Sun of 26 February 1998. February 26, 1998 Total Eclipse of the Sun. Partial phases and corona during mid totality. A total eclipse of the Sun occurs when the orbits of the Sun and Moon line up and the Moon moves in front to the Sun, totally blocking its light from reaching a narrow path on the Earth

Eclipse totale de Soleil 02/1998 - Composite Image, Total Eclipse of the Sun - 1998 - The different phases of the total eclipse of the Sun of 26 February 1998. February 26, 1998 Total Eclipse of the Sun. Partial phases and corona during mid totality. A total eclipse of the Sun occurs when the orbits of the Sun and Moon line up and the Moon moves in front to the Sun, totally blocking its light from reaching a narrow path on the Earth

Jerry Lodriguss

PIX4627431

A Day on Io - 5/6 - Illustration - A Day on Io - 5/6 - Artwork: Io always points the same face towards Jupiter during his orbit and like the Moon from Earth, Jupiter presents different phases to him. This series of images shows the landscape changing in a day from a point in the northern hemisphere of Io-5. Ten and a half hours later, the sun set on the horizon of Io. Jupiter is in his last quarter phase. In the distance, a volcano erupts and the gases emitted into the thin atmosphere of Io illuminate in the magnetic field surrounding Jupiter and Io - Io keeps the same face towards Jupiter as it orbits the planet. For this reason, Jupiter appears to hang motionless in Io's sky. Just as the Earth's Moon does, Jupiter goes through phases as Io orbits it. Here's a gallery showing the view from a location in the northern hemisphere during the course of a single day - 5. Ten and a half hours later and the sun has now set below Io's horizon. Jupiter is in its last quarter phase. A distant volcano has begun erupting and the gasse it is releasing into IO's thin atmosphere are glowing in the dense radiation field that surrounds Jupiter and Io — A Day on Io - 5/6 - Illustration - A Day on Io - 5/6 - Artwork: Io always points the same face towards Jupiter during his orbit and like the Moon from Earth, Jupiter presents different phases to him. This series of images shows the landscape changing in a day from a point in the northern hemisphere of Io-5. Ten and a half hours later, the sun set on the horizon of Io. Jupiter is in his last quarter phase. In the distance, a volcano erupts and the gases emitted into the thin atmosphere of Io illuminate in the magnetic field surrounding Jupiter and Io - Io keeps the same face towards Jupiter as it orbits the planet. For this reason, Jupiter appears to hang motionless in Io's sky. Just as the Earth's Moon does, Jupiter goes through phases as Io orbits it. Here's a gallery showing the view from a location in the northern hemisphere during the course of a single day - 5. Ten and a half hours later and the sun has now set below Io's horizon. Jupiter is in its last quarter phase. A distant vo

A Day on Io - 5/6 - Illustration - A Day on Io - 5/6 - Artwork: Io always points the same face towards Jupiter during his orbit and like the Moon from Earth, Jupiter presents different phases to him. This series of images shows the landscape changing in a day from a point in the northern hemisphere of Io-5. Ten and a half hours later, the sun set on the horizon of Io. Jupiter is in his last quarter phase. In the distance, a volcano erupts and the gases emitted into the thin atmosphere of Io illuminate in the magnetic field surrounding Jupiter and Io - Io keeps the same face towards Jupiter as it orbits the planet. For this reason, Jupiter appears to hang motionless in Io's sky. Just as the Earth's Moon does, Jupiter goes through phases as Io orbits it. Here's a gallery showing the view from a location in the northern hemisphere during the course of a single day - 5. Ten and a half hours later and the sun has now set below Io's horizon. Jupiter is in its last quarter phase. A distant vo

Miller, Ron (b.1947)

PIX4614156

London, England: c.1920 An astronomical model for higher education in the New County Hall in Westminster showing the motions of the earth, moon and sun. (b/w photo)

London, England: c.1920 An astronomical model for higher education in the New County Hall in Westminster showing the motions of the earth, moon and sun. (b/w photo)

UIG3274322

Project Mercury: members of the Mercury Seven in training

Project Mercury: members of the Mercury Seven in training

BOF745803

The solar system - Our solar system. Artwork - Planet orbits around the Sun. Orbits of planets around the Sun

The solar system - Our solar system. Artwork - Planet orbits around the Sun. Orbits of planets around the Sun

Sebastian Voltmer

PIX4630165

The asteroid belt - The asteroid belt- Artwork - View of the main asteroid belt, from planetary orbits to jupiter, with Trojan asteroids. Artist view of the asteroid belt located between Mars and Jupiter orbits plus the trojan asteroids

The asteroid belt - The asteroid belt- Artwork - View of the main asteroid belt, from planetary orbits to jupiter, with Trojan asteroids. Artist view of the asteroid belt located between Mars and Jupiter orbits plus the trojan asteroids

L. Bret

PIX4584064

Bohr atomic model

Bohr atomic model

UIG558150

Portrait of Nicolas Copernicus (1473-1543) (engraving) (b/w photo)

Portrait of Nicolas Copernicus (1473-1543) (engraving) (b/w photo)

French School, (16th century)

XIR166573

Halley's Comet

Green, Harry (b.1920)

LAL453420

Harmonia Macrocosmica, 17th (engraving)

Harmonia Macrocosmica, 17th (engraving)

Cellarius, Andreas (c.1596-1665)

Gianni Cigolini

MEV5048664

Orbits of Earth and Jupiter around Sun and zodiac, drawing taken from Dialogue Concerning Two Chief World Systems, 3th day, by Galileo Galilei (1564-1641), 1632

Orbits of Earth and Jupiter around Sun and zodiac, drawing taken from Dialogue Concerning Two Chief World Systems, 3th day, by Galileo Galilei (1564-1641), 1632

Galilei, Galileo (1564-1642)

DGA3074198

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

L. Bret

PIX4584062

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

S. Numazawa

PIX4584061

The asteroid belt - The asteroid belt- Artwork: Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

The asteroid belt - The asteroid belt- Artwork: Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits

Miller, Ron (b.1947)

PIX4584118

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe above the northern hemisphere of Saturn. This illustration shows Cassini above Saturn's northern hemisphere prior to making one of its Grand Finale dives. During Cassini's Grand Finale, the spacecraft will make 22 orbits around Saturn that carry the spacecraft over the planet's north before diving between Saturn and its rings. At the conclusion of this final set of daring orbits, the spacecraft will plunge into Saturn's atmosphere, ending its mission on Sept. 15, 2017.

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe above the northern hemisphere of Saturn. This illustration shows Cassini above Saturn's northern hemisphere prior to making one of its Grand Finale dives. During Cassini's Grand Finale, the spacecraft will make 22 orbits around Saturn that carry the spacecraft over the planet's north before diving between Saturn and its rings. At the conclusion of this final set of daring orbits, the spacecraft will plunge into Saturn's atmosphere, ending its mission on Sept. 15, 2017.

PIX4643494

Space tourism - Artist's view - Cruise shuttle in low earth orbit - Artist's view of a space shuttle of the future in orbit around the Earth. A reusable space tourism “” cruise””” shuttle orbits the earth at an altitude of approximately 250 miles. This spacecraft is 75 feet long by 55 feet wide.

Space tourism - Artist's view - Cruise shuttle in low earth orbit - Artist's view of a space shuttle of the future in orbit around the Earth. A reusable space tourism “” cruise””” shuttle orbits the earth at an altitude of approximately 250 miles. This spacecraft is 75 feet long by 55 feet wide.

Walter B Myers

PIX4640616

Halley's Comet (gouache on paper)

Halley's Comet (gouache on paper)

Green, Harry (b.1920)

LAL278481

India: Jantar Mantar, Maharaja Jai Singhs 1724 astronomical observatory, near Connaught Place, New Delhi

India: Jantar Mantar, Maharaja Jai Singhs 1724 astronomical observatory, near Connaught Place, New Delhi

David Henley

PFH1189572

La planete Neuf - Illustration - Planet Nine - Artwork: Vue d'artiste de la planete Neuf. The Ninth Planet is a hypothetical planet of the Solar System indirectly recorded, the existence of which is suggested by observing the orbits of several transneptunian objects. This planet would be gaseous, similar to Uranus or Neptune. A hypothetical planet in the outer reaches of the solar system orbits more than 700 times farther from the sun than earth does. A Super-earth, with an estimated mass of 10 Earths (approximately 5,000 times the mass of Pluto), a diameter two to four times that of Earth, and a highly elliptical orbit with an orbital period of approximately 15,000 years, the planet is shown as a ringed ice giant whose night side is illuminated by lightning and aurorae powered by galactic cosmic rays.

La planete Neuf - Illustration - Planet Nine - Artwork: Vue d'artiste de la planete Neuf. The Ninth Planet is a hypothetical planet of the Solar System indirectly recorded, the existence of which is suggested by observing the orbits of several transneptunian objects. This planet would be gaseous, similar to Uranus or Neptune. A hypothetical planet in the outer reaches of the solar system orbits more than 700 times farther from the sun than earth does. A Super-earth, with an estimated mass of 10 Earths (approximately 5,000 times the mass of Pluto), a diameter two to four times that of Earth, and a highly elliptical orbit with an orbital period of approximately 15,000 years, the planet is shown as a ringed ice giant whose night side is illuminated by lightning and aurorae powered by galactic cosmic rays.

Dixon, Don (b.1951)

PIX4629665

Titan - Illustration - Saturn's satellite Titan - Artist's view of Titan, Saturn's largest satellite. Titan is Saturn's largest satellite and the second - largest satellite in the Solar System (just slightly smaller than Jupiter's Ganymede). Although Titan orbits Saturn, it is still larger than the planet Mercury and has the most substantial atmosphere of any satellite in the Solar System

Titan - Illustration - Saturn's satellite Titan - Artist's view of Titan, Saturn's largest satellite. Titan is Saturn's largest satellite and the second - largest satellite in the Solar System (just slightly smaller than Jupiter's Ganymede). Although Titan orbits Saturn, it is still larger than the planet Mercury and has the most substantial atmosphere of any satellite in the Solar System

Walter B Myers

PIX4626072

Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006

Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006

Steven Hobbs

PIX4606256

Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006

Venus Express Probe - Artist's View - Venus Express spacecraft - Artwork - The European Venus Express probe was launched on 9 November 2005 and has been placed in orbit around Venus since 11 April 2006. The european spacecraft Venus Express has been launched from Baikonur in november 2005 and orbits the planet Venus since april 11 2006

D. Ducros

PIX4606222

Nicolaus Copernicus (1473-1543), detail from a Map showing the Copernican System of Planetary Orbits, 'Planisphaerium Copernicanum', from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coeslestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving) (detail of 22556)

Nicolaus Copernicus (1473-1543), detail from a Map showing the Copernican System of Planetary Orbits, 'Planisphaerium Copernicanum', from 'The Celestial Atlas, or The Harmony of the Universe' (Atlas coeslestis seu harmonia macrocosmica) pub. by Joannes Janssonius, Amsterdam, 1660-61 (hand coloured engraving) (detail of 22556)

Cellarius, Andreas (c.1596-1665)

STC129826

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 — 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 dis

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 dis

Miller, Ron (b.1947)

PIX4608153

Fusee Ariane 5 ECA - 08/2008 - Ariane 5 ECA liftoff - 08/2008 - Decolving the Ariane 5 ECA rocket with on board, two communication satellites, the AMC-21 satellite and the Superbird 7 satellite. Flight V185 was launched on August 14, 2008. Ariane 5 ECA, V185 launcher lifts off from Europe's Spaceport at Kourou, in English Guiana, on its mission to place two telecommunications satellites into geostationary transfer orbits. Lift - off of flight V185 took place at 22:44 CEST/Paris on 14 August 2008 (20:44 UTC/GMT; 17:44 UTC - 3/Kourou).The satellites were accurately injected into the correct transfer orbits about 30 minutes later. The payload comprised AMC-21, which will provide will provide 24 Ku - band channels of television and enterprise data distribution services over the USA, the Gulf of Mexico, Central America and the Caribbean, and Superbird 7, which will provide 28 Ku - band channels of broadcast services and mobile terminal links over Japan, eastern Asia and the Pacific Ocean. The payload mass was 8068 kg; the satellite masses totalled 7229 kg, with payload adapters and dispensers making up the additional 839 kg — Fusee Ariane 5 ECA - 08/2008 - Ariane 5 ECA liftoff - 08/2008 - Decolving the Ariane 5 ECA rocket with on board, two communication satellites, the AMC-21 satellite and the Superbird 7 satellite. Flight V185 was launched on August 14, 2008. Ariane 5 ECA, V185 launcher lifts off from Europe's Spaceport at Kourou, in English Guiana, on its mission to place two telecommunications satellites into geostationary transfer orbits. Lift - off of flight V185 took place at 22:44 CEST/Paris on 14 August 2008 (20:44 UTC/GMT; 17:44 UTC - 3/Kourou).The satellites were accurately injected into the correct transfer orbits about 30 minutes later. The payload comprised AMC-21, which will provide will provide 24 Ku - band channels of television and enterprise data distribution services over the USA, the Gulf of Mexico, Central America and the Caribbean, and Superbird 7, which will provide 28 Ku - band channels of broadcast services and mobile terminal links over Japan, eastern Asia and the Pacific Ocean. T

Fusee Ariane 5 ECA - 08/2008 - Ariane 5 ECA liftoff - 08/2008 - Decolving the Ariane 5 ECA rocket with on board, two communication satellites, the AMC-21 satellite and the Superbird 7 satellite. Flight V185 was launched on August 14, 2008. Ariane 5 ECA, V185 launcher lifts off from Europe's Spaceport at Kourou, in English Guiana, on its mission to place two telecommunications satellites into geostationary transfer orbits. Lift - off of flight V185 took place at 22:44 CEST/Paris on 14 August 2008 (20:44 UTC/GMT; 17:44 UTC - 3/Kourou).The satellites were accurately injected into the correct transfer orbits about 30 minutes later. The payload comprised AMC-21, which will provide will provide 24 Ku - band channels of television and enterprise data distribution services over the USA, the Gulf of Mexico, Central America and the Caribbean, and Superbird 7, which will provide 28 Ku - band channels of broadcast services and mobile terminal links over Japan, eastern Asia and the Pacific Ocean. T

PIX4604257

Fusee Ariane 5 ECA -11/2010 - Ariane 5 ECA liftoff- 11/2010 - Decolving the Ariane 5 ECA rocket with the telecommunications satellites Hylas1 and Intelsat 17 on board. Flight V198 was launched on November 26, 2010. On 26 November 2010, an Ariane 5 launcher lifted off from Europe's Spaceport in English Guiana on its mission to place two telecommunications satellites, Hylas-1 and Intelsat 17, into their planned transfer orbits. Liftoff of V198, the 54th Ariane 5 flight, came at 19:39 CET (18:39 GMT; 15:39 English Guiana)

Fusee Ariane 5 ECA -11/2010 - Ariane 5 ECA liftoff- 11/2010 - Decolving the Ariane 5 ECA rocket with the telecommunications satellites Hylas1 and Intelsat 17 on board. Flight V198 was launched on November 26, 2010. On 26 November 2010, an Ariane 5 launcher lifted off from Europe's Spaceport in English Guiana on its mission to place two telecommunications satellites, Hylas-1 and Intelsat 17, into their planned transfer orbits. Liftoff of V198, the 54th Ariane 5 flight, came at 19:39 CET (18:39 GMT; 15:39 English Guiana)

PIX4641308

The star Fomalhaut - Star Fomalhaut - The star Fomalhaut is located 25 years - light from Earth in the constellation Southern Fish. An extrasolar planet, called Fomalhaut b, with a mass close to Jupiter, is in orbit around it. This image shows Fomalhaut, the star around which the discovered planet Fomalhaut b orbits. Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. It is blazing through hydrogen at such a furious rate that it will burn out in only one billion years, 10% the lifespan of our star. The field of view is 2.7 x 2.9 degrees

The star Fomalhaut - Star Fomalhaut - The star Fomalhaut is located 25 years - light from Earth in the constellation Southern Fish. An extrasolar planet, called Fomalhaut b, with a mass close to Jupiter, is in orbit around it. This image shows Fomalhaut, the star around which the discovered planet Fomalhaut b orbits. Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. It is blazing through hydrogen at such a furious rate that it will burn out in only one billion years, 10% the lifespan of our star. The field of view is 2.7 x 2.9 degrees

PIX4571995

Fusee Ariane 5 ECA - 05/2011 - Ariane 5 ECA liftoff - 05/2011 - Decolving the Ariane 5 ECA rocket with the telecommunications satellites GSAT - 8 and ST - 2 on board. The launch of flight VA202 took place on May 20, 2011. On 20 May 2011, an Ariane 5 launcher lifted off from Europe's Spaceport in English Guiana on its mission to place two telecommunications satellites, GSAT - 8 and ST - 2, into their planned transfer orbits. Flight VA202 was the third Ariane 5 launch of 2011. Liftoff of the 58th Ariane 5 mission came at 22:38 CEST (20:38 GMT; 17:38 English Guiana)

Fusee Ariane 5 ECA - 05/2011 - Ariane 5 ECA liftoff - 05/2011 - Decolving the Ariane 5 ECA rocket with the telecommunications satellites GSAT - 8 and ST - 2 on board. The launch of flight VA202 took place on May 20, 2011. On 20 May 2011, an Ariane 5 launcher lifted off from Europe's Spaceport in English Guiana on its mission to place two telecommunications satellites, GSAT - 8 and ST - 2, into their planned transfer orbits. Flight VA202 was the third Ariane 5 launch of 2011. Liftoff of the 58th Ariane 5 mission came at 22:38 CEST (20:38 GMT; 17:38 English Guiana)

PIX4604391

August 24, 2016: Artist's view of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible between the planet and the star Proxima. Proxima b is a little more massive than Earth, orbit in habitable area or temperature would allow the presence of liquid water on its surface - This artist's impression shows the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image between the planet and Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

August 24, 2016: Artist's view of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible between the planet and the star Proxima. Proxima b is a little more massive than Earth, orbit in habitable area or temperature would allow the presence of liquid water on its surface - This artist's impression shows the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image between the planet and Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

PIX4650952

Futuristic advertising poster for tourism on Kepler-16 b - Illustration - Futuristic Advert for tourism on Kepler-16 b - Illustration: Advertising promoting tourism on Kepler-16 b. This exoplanet is orbiting in the habitable area of the Starsystem Kepler-16 (AB), an Algol-type binary star located at a distance of about 200 light years from the Sun in the constellation of Swan. An astronaut could contemplate a double sunset. Like Luke Skywalker's planet “” Tatooine””” in Star Wars, Kepler-16b orbits a pair of stars. Described here as a terrestrial planet, Kepler-16b might also be a gas giant like Saturn. Prospects for life on this unusual world aren't good, as it has a temperature similar to that of dry ice. But the discovery indicates that the movie's iconic double-sunset is anything but science fiction.

Futuristic advertising poster for tourism on Kepler-16 b - Illustration - Futuristic Advert for tourism on Kepler-16 b - Illustration: Advertising promoting tourism on Kepler-16 b. This exoplanet is orbiting in the habitable area of the Starsystem Kepler-16 (AB), an Algol-type binary star located at a distance of about 200 light years from the Sun in the constellation of Swan. An astronaut could contemplate a double sunset. Like Luke Skywalker's planet “” Tatooine””” in Star Wars, Kepler-16b orbits a pair of stars. Described here as a terrestrial planet, Kepler-16b might also be a gas giant like Saturn. Prospects for life on this unusual world aren't good, as it has a temperature similar to that of dry ice. But the discovery indicates that the movie's iconic double-sunset is anything but science fiction.

PIX4608238

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

August 24, 2016: Artist's view of the surface of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the star Proxima. Proxima b is a little more massive than the Earth, orbit in habitable area where the temperature would allow the presence of liquid water on its surface - This artist's impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right of Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

August 24, 2016: Artist's view of the surface of Planet Proxima b orbiting the red dwarf star Proxima of Centaur, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the star Proxima. Proxima b is a little more massive than the Earth, orbit in habitable area where the temperature would allow the presence of liquid water on its surface - This artist's impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right of Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

PIX4650935

Earth-type exoplanete around Centauri Proxima - Artist's impression of the planet orbiting Proxima Centauri: Artist's view of Planet Proxima b orbiting around the red dwarf star Proxima of Centauri, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the image. Proxima b is slightly more massive than the Earth, orbit in habitable areas where the temperature would allow the presence of liquid water on its surface. This artist's impression shows a view of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

Earth-type exoplanete around Centauri Proxima - Artist's impression of the planet orbiting Proxima Centauri: Artist's view of Planet Proxima b orbiting around the red dwarf star Proxima of Centauri, the closest star to the solar system. The double star Alpha Centauri AB is visible at the top right of the image. Proxima b is slightly more massive than the Earth, orbit in habitable areas where the temperature would allow the presence of liquid water on its surface. This artist's impression shows a view of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface

Miller, Ron (b.1947)

PIX4608073

EDRS Relay Satellite Network - Artist's view - The European Data Relay Satellite System - EDRS - The European Data Relay Satellites (EDRS) programme is a geostationary orbit satellite network project enabling faster and better data transmission between satellites and ground stations using new communication technologies. EDRS will replace ESA's Artemis data relay satellite, which has been in operation since 2003 and will reach the end of life in the first half of the next decade. December 2008. Artist impression of European Data Relay Satellite (EDRS) system. EDRS is a network of satellites that will use geostationary satellites to communicate with both ground stations and other satellites - whose lower orbits restrict the time that they can 'see' any one ground station. Allowing low - Earth orbit satellites to deliver data continuously, instead of storing it on board for transmission while overflying a ground station, will increase the timeliness with which we receive data improving global communications, navigation and Earth observation — EDRS Relay Satellite Network - Artist's view - The European Data Relay Satellite System - EDRS - The European Data Relay Satellites (EDRS) programme is a geostationary orbit satellite network project enabling faster and better data transmission between satellites and ground stations using new communication technologies. EDRS will replace ESA's Artemis data relay satellite, which has been in operation since 2003 and will reach the end of life in the first half of the next decade. December 2008. Artist impression of European Data Relay Satellite (EDRS) system. EDRS is a network of satellites that will use geostationary satellites to communicate with both ground stations and other satellites - whose lower orbits restrict the time that they can 'see' any one ground station. Allowing low - Earth orbit satellites to deliver data continuously, instead of storing it on board for transmission while overflying a ground station, will increase the timeliness with which we receive data improving gl

EDRS Relay Satellite Network - Artist's view - The European Data Relay Satellite System - EDRS - The European Data Relay Satellites (EDRS) programme is a geostationary orbit satellite network project enabling faster and better data transmission between satellites and ground stations using new communication technologies. EDRS will replace ESA's Artemis data relay satellite, which has been in operation since 2003 and will reach the end of life in the first half of the next decade. December 2008. Artist impression of European Data Relay Satellite (EDRS) system. EDRS is a network of satellites that will use geostationary satellites to communicate with both ground stations and other satellites - whose lower orbits restrict the time that they can 'see' any one ground station. Allowing low - Earth orbit satellites to deliver data continuously, instead of storing it on board for transmission while overflying a ground station, will increase the timeliness with which we receive data improving gl

P. Carril

PIX4642966

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 — 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 tran

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 tran

Walter B Myers

PIX4640726

Hubble ultra deep field - In the southern constellation of the furnace, the Hubble space telescope posed 270h to obtain this image of the distant universe. Approximately 10,000 galaxies distant from 5 to 13 billion light years are visible in this image. This view of nearly 10,000 galaxies is the deepest visible - light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy - studded view represents a “” deep”” core sample of the universe, cutting across billions of light - years. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well - defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. In ground - based photographs, the patch of sky in which the galaxies reside (just one - tenth the diameter of the full Moon) is largely empty. Located in the constellation Fornax, the region is so empty that only a handful of stars within the Milky Way galaxy can be seen in the image. In this image, blue and green correspond to colors that can be seen by the human eye, such as hot, young, blue stars and the glow of Sun - like stars in the disks of galaxies. Red represents near - infrared light, which is invisible to the human eye, such as the red glow of dust - enshrouded galaxies.The image required 800 exposures taken over the course of 400 Hubble orbits around Earth. The total amount of exposure time was 11.3 days, taken between Sept. 24, 2003 and Jan. 16, 2004 — Hubble ultra deep field - In the southern constellation of the furnace, the Hubble space telescope posed 270h to obtain this image of the distant universe. Approximately 10,000 galaxies distant from 5 to 13 billion light years are visible in this image. This view of nearly 10,000 galaxies is the deepest visible - light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy - studded view represents a “” deep”” core sample of the universe, cutting across billions of light - years. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well - defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. In ground - based photographs, the patch of sky in which the galaxies reside (just one - tenth the diameter of the full Moon

Hubble ultra deep field - In the southern constellation of the furnace, the Hubble space telescope posed 270h to obtain this image of the distant universe. Approximately 10,000 galaxies distant from 5 to 13 billion light years are visible in this image. This view of nearly 10,000 galaxies is the deepest visible - light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy - studded view represents a “” deep”” core sample of the universe, cutting across billions of light - years. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well - defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. In ground - based photographs, the patch of sky in which the galaxies reside (just one - tenth the diameter of the full Moon

PIX4613783

European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in the CSG for Soyuz vehicles. Ariane 5 ES, another version of the Ariane 5E featuring a restartable version of Ariane 5G's storable propellant upper stage. One of its primary payloads is the Autonomous Transfer Vehicle (ATV) for resupply and reboost missions to the International Space Station. Ariane 5 ECA, the most powerful version of the Ariane 5E, an evolution of the generic Ariane 5 launcher with an increased propellant load in its solid booster stages and an improved capacity for the liquid oxygen tank of its cryogenic core stage to feed its new Vulcain 2 main engine. The Ariane 5 ECA was first launched on December 11, 2002. Its payload capacity to geostationary transfer orbit reaches 10 metric tons — European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in th

European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in th

D. Ducros

PIX4604563

1970s lunar module orbits over moon surface

1970s lunar module orbits over moon surface

AVE6319843

1970s intrepid lunar module descends onto moon surface

1970s intrepid lunar module descends onto moon surface

AVE6319826

1970s intrepid lunar module descends onto moon surface

1970s intrepid lunar module descends onto moon surface

AVE6319827

1970s intrepid lunar module descends onto moon surface

1970s intrepid lunar module descends onto moon surface

AVE6319830

1970s lunar module descends onto moon surface

1970s lunar module descends onto moon surface

AVE6319828

The Solar System (colour litho)

The Solar System (colour litho)

German School, (19th century)

LLM3630293

1970s intrepid lunar module descends onto moon surface

1970s intrepid lunar module descends onto moon surface

AVE6319825

A diagram of the Solar system, showing the orbits of some of the minor planets, 19th century

A diagram of the Solar system, showing the orbits of some of the minor planets, 19th century

UIG5311318

1970s lunar module orbits over the surface of the moon

1970s lunar module orbits over the surface of the moon

AVE6319823

1970s lunar module descends onto moon surface

1970s lunar module descends onto moon surface

AVE6319829

A diagram of the Solar system, showing the orbits of some of the minor planets, 19th century

A diagram of the Solar system, showing the orbits of some of the minor planets, 19th century

UIG5311394

Television screen displaying a simulation of John Glenn in the Friendship 7 space capsule. There were no publicly broadcast images of Glenn during the first US orbital space flight. February 20, 1962

Television screen displaying a simulation of John Glenn in the Friendship 7 space capsule. There were no publicly broadcast images of Glenn during the first US orbital space flight. February 20, 1962

EVB2942025

Television screen animation of John Glenn's Friendship 7 space capsule approaching North America, during his three orbit space flight on Feb. 20, 1962

Television screen animation of John Glenn's Friendship 7 space capsule approaching North America, during his three orbit space flight on Feb. 20, 1962

EVB2942026

The Compleat Orrery, pub. London 1780 (coloured engraving)

The Compleat Orrery, pub. London 1780 (coloured engraving)

English School, (18th century)

STC984703

A Comet (chromolitho)

A Comet (chromolitho)

English School, (20th century)

LLM5205133

Frontispiece to 'Theoria motuum planetarium et cometarum', 1744 (litho)

Frontispiece to 'Theoria motuum planetarium et cometarum', 1744 (litho)

Swiss School (18th century)

BL3704223

Page from The Pictorial Museum of Animated Nature (engraving)

Page from The Pictorial Museum of Animated Nature (engraving)

English School, (19th century)

LLP980211

Urbain Le Verrier, French mathematician and astronomer (chromolitho)

Urbain Le Verrier, French mathematician and astronomer (chromolitho)

French School, (20th century)

LLM977497

1950s: Animated electrons swirl and spin around the nucleus of an atom

1950s: Animated electrons swirl and spin around the nucleus of an atom

AVE6329332

A diagram of the solar system, showing the orbits of four asteroids (planetoids) by Thomas Burnet. Thomas Burnet (1635-1715) an English theologian and writer on cosmogony, 19th century

A diagram of the solar system, showing the orbits of four asteroids (planetoids) by Thomas Burnet. Thomas Burnet (1635-1715) an English theologian and writer on cosmogony, 19th century

UIG5311305

The Solar System (coloured engraving)

The Solar System (coloured engraving)

American School, (19th century)

LLM6014054

George Biddell Airy (engraving)

George Biddell Airy (engraving)

English School, (19th century)

LLE815677

Astronomical Clock, North Transept, Exeter Cathedral (photo)

Astronomical Clock, North Transept, Exeter Cathedral (photo)

John Bethell

JB3243610

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