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Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems
Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems

PIX4572541: Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems / Bridgeman Images

ID: PIX4572541

Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems

Brown dwarf star Gliese 229 b - Brown dwarf Gliese 229 b - Artist view of the brown dwarf star Gliese 229B. Discovered in 1995 in the constellation Lievre at 18 years - light from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and is estimated to be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a distance of about a half million miles. Glowing like a charcoal ember, Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun. Gliese 229 b is believed to be 30 to 40 times more massive than the planet Jupiter, which is massive enough for Gliese 229 b to sustain deuterium fusion, but not enough mass to initiate hydrogen fusion like our Sun. As a result, Gliese 229 b radiates a temperature of only 1,300o F. It is believed to be two to four billion years old. Despite being so much more massive than the planet Jupiter, the diameter of this brown dwarf is believed to be actually slightly less than Jupiter's; Gliese 229 b's greater mass results in its overcoming the internal pressures that sustain Jupiter's greater volume
Brown dwarf star Gliese 229 b - Brown dwarf Gliese 229 b - Artist view of the brown dwarf star Gliese 229B. Discovered in 1995 in the constellation Lievre at 18 years - light from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and is estimated to be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a distance of about a half million miles. Glowing like a charcoal ember, Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun. Gliese 229 b is believed to be 30 to 40 times more massive than the planet Jupiter, which is massive enough for Gliese 229 b to sustain deuterium fusion, but not enough mass to initiate hydrogen fusion like our Sun. As a result, Gliese 229 b radiates a temperature of only 1,300o F. It is believed to be two to four billion years old. Despite being so much more massive than the planet Jupiter, the diameter of this brown dwarf is believed to be actually slightly less than Jupiter's; Gliese 229 b's greater mass results in its overcoming the internal pressures that sustain Jupiter's greater volume

PIX4572553: Brown dwarf star Gliese 229 b - Brown dwarf Gliese 229 b - Artist view of the brown dwarf star Gliese 229B. Discovered in 1995 in the constellation Lievre at 18 years - light from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and is estimated to be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a distance of about a half million miles. Glowing like a charcoal ember, Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun. Gliese 229 b is believed to be 30 to 40 times more massive than the planet Jupiter, which is massive enough for Gliese 229 b to sustain deuterium fusion, but not enough mass to initiate hydrogen fusion like our Sun. As a result, Gliese 229 b radiates a temperature of only 1,300o F. It is believed to be two to four billion years old. Despite being so much more massive than the planet Jupiter, the diameter of this brown dwarf is believed to be actually slightly less than Jupiter's; Gliese 229 b's greater mass results in its overcoming the internal pressures that sustain Jupiter's greater volume / Bridgeman Images

ID: PIX4572553

Brown dwarf star Gliese 229 b - Brown dwarf Gliese 229 b - Artist view of the brown dwarf star Gliese 229B. Discovered in 1995 in the constellation Lievre at 18 years - light from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and is estimated to be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a distance of about a half million miles. Glowing like a charcoal ember, Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun. Gliese 229 b is believed to be 30 to 40 times more massive than the planet Jupiter, which is massive enough for Gliese 229 b to sustain deuterium fusion, but not enough mass to initiate hydrogen fusion like our Sun. As

The Montparnasse Tower in Paris. Construction 1969-1975, architect Roger Saubot. Photography 30/05/09.
The Montparnasse Tower in Paris. Construction 1969-1975, architect Roger Saubot. Photography 30/05/09.

LBY4572783: The Montparnasse Tower in Paris. Construction 1969-1975, architect Roger Saubot. Photography 30/05/09. / Bridgeman Images

ID: LBY4572783

The Montparnasse Tower in Paris. Construction 1969-1975, architect Roger Saubot. Photography 30/05/09.

The tomb of Jean Paul Sartre (1905-1980) and Simone de Beauvoir (1908-1986) at the cemetery of Montparnasse, Paris. Photography 30/05/09.
The tomb of Jean Paul Sartre (1905-1980) and Simone de Beauvoir (1908-1986) at the cemetery of Montparnasse, Paris. Photography 30/05/09.

LBY4572798: The tomb of Jean Paul Sartre (1905-1980) and Simone de Beauvoir (1908-1986) at the cemetery of Montparnasse, Paris. Photography 30/05/09. / Bridgeman Images

ID: LBY4572798

The tomb of Jean Paul Sartre (1905-1980) and Simone de Beauvoir (1908-1986) at the cemetery of Montparnasse, Paris. Photography 30/05/09.

The Good Lord Illustration of a series of proverbs, 18th century (w/c)
The Good Lord Illustration of a series of proverbs, 18th century (w/c)

JLJ4572839: The Good Lord Illustration of a series of proverbs, 18th century (w/c), Carmontelle, Louis Carrogis (1717-1806) / Bridgeman Images

ID: JLJ4572839

The Good Lord Illustration of a series of proverbs, 18th century (w/c)

Carmontelle, Louis Carrogis (1717-1806)

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.
Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

TEC4573152: Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat., Andrault, Michel (1926-2020) & Parat, Pierre (b.1928) / Bridgeman Images

ID: TEC4573152

Tour of the Societe Generale à la Defense (Hauts de Seine). Construction 1995, architects Michel Andrault and Pierre Parat.

Andrault, Michel (1926-2020) & Parat, Pierre (b.1928)

Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets
Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets

PIX4573201: Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets / Bridgeman Images

ID: PIX4573201

Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets

Venus and Adonis, 17th century (oil on canvas)
Venus and Adonis, 17th century (oil on canvas)

JLJ4573239: Venus and Adonis, 17th century (oil on canvas), Cornelisz. van Haarlem, Cornelis (1562-1638) / Bridgeman Images

ID: JLJ4573239

Venus and Adonis, 17th century (oil on canvas)

Cornelisz. van Haarlem, Cornelis (1562-1638)

Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets
Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets

PIX4573338: Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets / Bridgeman Images

ID: PIX4573338

Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie
Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

PIX4573359: Planete extrasolaire - Artist view - Extrasolar planet - Artist vie / Bridgeman Images

ID: PIX4573359

Planete extrasolaire - Artist view - Extrasolar planet - Artist vie

The life of the Virgin: the birth of Mary, detail (Fresco, 1365)
The life of the Virgin: the birth of Mary, detail (Fresco, 1365)

LRI4572561: The life of the Virgin: the birth of Mary, detail (Fresco, 1365), Giovanni da Milano (fl.1350-70) / Bridgeman Images

ID: LRI4572561

The life of the Virgin: the birth of Mary, detail (Fresco, 1365)

Giovanni da Milano (fl.1350-70)

Japanese art: women in spring, 19th century (print)
Japanese art: women in spring, 19th century (print)

JLJ4572647: Japanese art: women in spring, 19th century (print), Japanese School, (19th century) / Bridgeman Images

ID: JLJ4572647

Japanese art: women in spring, 19th century (print)

Japanese School, (19th century)

The morning prayer (oil on canvas, 18th century)
The morning prayer (oil on canvas, 18th century)

LRI4572665: The morning prayer (oil on canvas, 18th century), Greuze, Jean Baptiste (1725-1805) / Bridgeman Images

ID: LRI4572665

The morning prayer (oil on canvas, 18th century)

Greuze, Jean Baptiste (1725-1805)

Portrait of Tieleman Roosterman, Dutch trader (Painting, 1634)
Portrait of Tieleman Roosterman, Dutch trader (Painting, 1634)

LRI4572710: Portrait of Tieleman Roosterman, Dutch trader (Painting, 1634), Hals, Frans (1582/3-1666) / Bridgeman Images

ID: LRI4572710

Portrait of Tieleman Roosterman, Dutch trader (Painting, 1634)

Hals, Frans (1582/3-1666)

Young Woman Walking, 18th century (pencil)
Young Woman Walking, 18th century (pencil)

JLJ4572761: Young Woman Walking, 18th century (pencil), Fragonard, Jean-Honore (1732-1806) / Bridgeman Images

ID: JLJ4572761

Young Woman Walking, 18th century (pencil)

Fragonard, Jean-Honore (1732-1806)

An Indian princess has her miniature toilet from the Mughole School of 1740 (miniature)
An Indian princess has her miniature toilet from the Mughole School of 1740 (miniature)

JLJ4572823: An Indian princess has her miniature toilet from the Mughole School of 1740 (miniature), Mughal School (18th century) / Bridgeman Images

ID: JLJ4572823

An Indian princess has her miniature toilet from the Mughole School of 1740 (miniature)

Mughal School (18th century)

The Boulevard Raspail to Paris Boulevard Raspail - Paris -
The Boulevard Raspail to Paris Boulevard Raspail - Paris -

LBY4572841: The Boulevard Raspail to Paris Boulevard Raspail - Paris - / Bridgeman Images

ID: LBY4572841

The Boulevard Raspail to Paris Boulevard Raspail - Paris -

Scenario of the formation of a star - Scenario of the formation of a star. From left to right: 1. Interstellar gas and dust cloud, zooming on a blood cell. 2. Contraction and warming of the blood cell. 3. The blood cell flattened around the young star. 4. young star. Left is a cloud of gaz and interstellar dust. Inside is a dark globule which will contract to create a rotating disk flattening, at the center of this disk, the stars ingnites
Scenario of the formation of a star - Scenario of the formation of a star. From left to right: 1. Interstellar gas and dust cloud, zooming on a blood cell. 2. Contraction and warming of the blood cell. 3. The blood cell flattened around the young star. 4. young star. Left is a cloud of gaz and interstellar dust. Inside is a dark globule which will contract to create a rotating disk flattening, at the center of this disk, the stars ingnites

PIX4572917: Scenario of the formation of a star - Scenario of the formation of a star. From left to right: 1. Interstellar gas and dust cloud, zooming on a blood cell. 2. Contraction and warming of the blood cell. 3. The blood cell flattened around the young star. 4. young star. Left is a cloud of gaz and interstellar dust. Inside is a dark globule which will contract to create a rotating disk flattening, at the center of this disk, the stars ingnites / Bridgeman Images

ID: PIX4572917

Scenario of the formation of a star - Scenario of the formation of a star. From left to right: 1. Interstellar gas and dust cloud, zooming on a blood cell. 2. Contraction and warming of the blood cell. 3. The blood cell flattened around the young star. 4. young star. Left is a cloud of gaz and interstellar dust. Inside is a dark globule which will contract to create a rotating disk flattening, at the center of this disk, the stars ingnites

La Defense in the Hauts de Seine.
La Defense in the Hauts de Seine.

TEC4573491: La Defense in the Hauts de Seine. / Bridgeman Images

ID: TEC4573491

La Defense in the Hauts de Seine.

Quartier de la Defense (Hauts de Seine).
Quartier de la Defense (Hauts de Seine).

TEC4573554: Quartier de la Defense (Hauts de Seine). / Bridgeman Images

ID: TEC4573554

Quartier de la Defense (Hauts de Seine).

Quartier de la Defense (Hauts de Seine).
Quartier de la Defense (Hauts de Seine).

TEC4573563: Quartier de la Defense (Hauts de Seine). / Bridgeman Images

ID: TEC4573563

Quartier de la Defense (Hauts de Seine).

Portrait of Charles d'Amboise, 16th century (oil on canvas)
Portrait of Charles d'Amboise, 16th century (oil on canvas)

JLJ4573604: Portrait of Charles d'Amboise, 16th century (oil on canvas), Solario, Andrea (c.1466-1524) / Bridgeman Images

ID: JLJ4573604

Portrait of Charles d'Amboise, 16th century (oil on canvas)

Solario, Andrea (c.1466-1524)

Still life (oil on canvas, 19th century)
Still life (oil on canvas, 19th century)

LRI4573655: Still life (oil on canvas, 19th century), Neugebauer, Josef (1810-1895) / Bridgeman Images

ID: LRI4573655

Still life (oil on canvas, 19th century)

Neugebauer, Josef (1810-1895)

Campaign of Italy (1796-1797): 'The outside of a military hospital or the French in Italy' (oil on canvas)
Campaign of Italy (1796-1797): 'The outside of a military hospital or the French in Italy' (oil on canvas)

JLJ4573709: Campaign of Italy (1796-1797): 'The outside of a military hospital or the French in Italy' (oil on canvas), Taunay, Nicolas Antoine (1755-1830) / Bridgeman Images

ID: JLJ4573709

Campaign of Italy (1796-1797): 'The outside of a military hospital or the French in Italy' (oil on canvas)

Taunay, Nicolas Antoine (1755-1830)

Planet Jupiter - Planet Jupiter - Jupiter (the brightest spot in the sky) seen on December 30, 2010. Jupiter (the brightest dot in the sky) seen on December 30, 2010
Planet Jupiter - Planet Jupiter - Jupiter (the brightest spot in the sky) seen on December 30, 2010. Jupiter (the brightest dot in the sky) seen on December 30, 2010

PIX4574408: Planet Jupiter - Planet Jupiter - Jupiter (the brightest spot in the sky) seen on December 30, 2010. Jupiter (the brightest dot in the sky) seen on December 30, 2010 / Bridgeman Images

ID: PIX4574408

Planet Jupiter - Planet Jupiter - Jupiter (the brightest spot in the sky) seen on December 30, 2010. Jupiter (the brightest dot in the sky) seen on December 30, 2010

Esther chosen by King Assuerus (oil on canvas, 17th century)
Esther chosen by King Assuerus (oil on canvas, 17th century)

LRI4574487: Esther chosen by King Assuerus (oil on canvas, 17th century), Rubens, Peter Paul (1577-1640) / Bridgeman Images

ID: LRI4574487

Esther chosen by King Assuerus (oil on canvas, 17th century)

Rubens, Peter Paul (1577-1640)

Impacts comete SL - 9 on Jupiter/HST 18/07/1994 - Photo obtained by the Hubble space telescope on 18 July 1994. Traces of impacts left by fragments D and G. The comet Shoemaker - Levy 9 fragmented and then hit Jupiter during the month of July 1994
Impacts comete SL - 9 on Jupiter/HST 18/07/1994 - Photo obtained by the Hubble space telescope on 18 July 1994. Traces of impacts left by fragments D and G. The comet Shoemaker - Levy 9 fragmented and then hit Jupiter during the month of July 1994

PIX4574551: Impacts comete SL - 9 on Jupiter/HST 18/07/1994 - Photo obtained by the Hubble space telescope on 18 July 1994. Traces of impacts left by fragments D and G. The comet Shoemaker - Levy 9 fragmented and then hit Jupiter during the month of July 1994 / Bridgeman Images

ID: PIX4574551

Impacts comete SL - 9 on Jupiter/HST 18/07/1994 - Photo obtained by the Hubble space telescope on 18 July 1994. Traces of impacts left by fragments D and G. The comet Shoemaker - Levy 9 fragmented and then hit Jupiter during the month of July 1994

Jupiter seen by Pioneer 10 - Jupiter seen by Pioneer 10 - The planet Jupiter seen by Pioneer 10 on 2 December 1973, at a distance of 2,584,000 km from the planet. Jupiter seen by Pioneer 10 spacecraft at a range of 2,584,000 km on december 2 1973
Jupiter seen by Pioneer 10 - Jupiter seen by Pioneer 10 - The planet Jupiter seen by Pioneer 10 on 2 December 1973, at a distance of 2,584,000 km from the planet. Jupiter seen by Pioneer 10 spacecraft at a range of 2,584,000 km on december 2 1973

PIX4574580: Jupiter seen by Pioneer 10 - Jupiter seen by Pioneer 10 - The planet Jupiter seen by Pioneer 10 on 2 December 1973, at a distance of 2,584,000 km from the planet. Jupiter seen by Pioneer 10 spacecraft at a range of 2,584,000 km on december 2 1973 / Bridgeman Images

ID: PIX4574580

Jupiter seen by Pioneer 10 - Jupiter seen by Pioneer 10 - The planet Jupiter seen by Pioneer 10 on 2 December 1973, at a distance of 2,584,000 km from the planet. Jupiter seen by Pioneer 10 spacecraft at a range of 2,584,000 km on december 2 1973

The business district of Defense La Defense (c) Luc Boegly/Artedia/Leemage
The business district of Defense La Defense (c) Luc Boegly/Artedia/Leemage

LBY4574632: The business district of Defense La Defense (c) Luc Boegly/Artedia/Leemage / Bridgeman Images

ID: LBY4574632

The business district of Defense La Defense (c) Luc Boegly/Artedia/Leemage

Jupiter seen from its satellite Europe - Illustration - Jupiter from Europa's surface - Illustration - Jupiter seen from the icy surface of the satellite Europe. Europa is Jupiter's fourth largest satellite and is slightly smaller than the Earth's Moon. Europa is believed to be composed of silicate rocks with a layer of water ice covering the entire surface. This image is inspired by recent discoveries on Europa of regions that look very much like pack - ice on Earth's polar seas during spring thaws. The perspective is from an altitude of several thousand feet. The large crater in the foreground is about a half - mile in diameter. It may be that beneath Europa's surface ice there is a layer of liquid water, perhaps as much as 30 miles deep. This subsurface “” ocean”” would be kept liquid by tidally generated heat
Jupiter seen from its satellite Europe - Illustration - Jupiter from Europa's surface - Illustration - Jupiter seen from the icy surface of the satellite Europe. Europa is Jupiter's fourth largest satellite and is slightly smaller than the Earth's Moon. Europa is believed to be composed of silicate rocks with a layer of water ice covering the entire surface. This image is inspired by recent discoveries on Europa of regions that look very much like pack - ice on Earth's polar seas during spring thaws. The perspective is from an altitude of several thousand feet. The large crater in the foreground is about a half - mile in diameter. It may be that beneath Europa's surface ice there is a layer of liquid water, perhaps as much as 30 miles deep. This subsurface “” ocean”” would be kept liquid by tidally generated heat

PIX4575161: Jupiter seen from its satellite Europe - Illustration - Jupiter from Europa's surface - Illustration - Jupiter seen from the icy surface of the satellite Europe. Europa is Jupiter's fourth largest satellite and is slightly smaller than the Earth's Moon. Europa is believed to be composed of silicate rocks with a layer of water ice covering the entire surface. This image is inspired by recent discoveries on Europa of regions that look very much like pack - ice on Earth's polar seas during spring thaws. The perspective is from an altitude of several thousand feet. The large crater in the foreground is about a half - mile in diameter. It may be that beneath Europa's surface ice there is a layer of liquid water, perhaps as much as 30 miles deep. This subsurface “” ocean”” would be kept liquid by tidally generated heat / Bridgeman Images

ID: PIX4575161

Jupiter seen from its satellite Europe - Illustration - Jupiter from Europa's surface - Illustration - Jupiter seen from the icy surface of the satellite Europe. Europa is Jupiter's fourth largest satellite and is slightly smaller than the Earth's Moon. Europa is believed to be composed of silicate rocks with a layer of water ice covering the entire surface. This image is inspired by recent discoveries on Europa of regions that look very much like pack - ice on Earth's polar seas during spring thaws. The perspective is from an altitude of several thousand feet. The large crater in the foreground is about a half - mile in diameter. It may be that beneath Europa's surface ice there is a layer of liquid water, perhaps as much as 30 miles deep. This subsurface “” ocean”” would be kept liquid by tidally generated heat

Mazars Exlatis a Courbevoie, 61, rue Henri Regnault, Courbevoie, 2006 - Arquitectonia (Bernardo Fort- brescia), Agence d'architecture Bridot-Willerval (Bruno Willerval)
Mazars Exlatis a Courbevoie, 61, rue Henri Regnault, Courbevoie, 2006 - Arquitectonia (Bernardo Fort- brescia), Agence d'architecture Bridot-Willerval (Bruno Willerval)

LBY4575251: Mazars Exlatis a Courbevoie, 61, rue Henri Regnault, Courbevoie, 2006 - Arquitectonia (Bernardo Fort- brescia), Agence d'architecture Bridot-Willerval (Bruno Willerval) / Bridgeman Images

ID: LBY4575251

Mazars Exlatis a Courbevoie, 61, rue Henri Regnault, Courbevoie, 2006 - Arquitectonia (Bernardo Fort- brescia), Agence d'architecture Bridot-Willerval (Bruno Willerval)

Clouds on Jupiter seen by Voyager 2 - Jupiter clouds seen by Voyager 2 - Clouds on Jupiter seen by the Voyager 2 probe on July 6, 1979. Jupiter clouds seen by Voyager 2 on July 6, 1979
Clouds on Jupiter seen by Voyager 2 - Jupiter clouds seen by Voyager 2 - Clouds on Jupiter seen by the Voyager 2 probe on July 6, 1979. Jupiter clouds seen by Voyager 2 on July 6, 1979

PIX4574690: Clouds on Jupiter seen by Voyager 2 - Jupiter clouds seen by Voyager 2 - Clouds on Jupiter seen by the Voyager 2 probe on July 6, 1979. Jupiter clouds seen by Voyager 2 on July 6, 1979 / Bridgeman Images

ID: PIX4574690

Clouds on Jupiter seen by Voyager 2 - Jupiter clouds seen by Voyager 2 - Clouds on Jupiter seen by the Voyager 2 probe on July 6, 1979. Jupiter clouds seen by Voyager 2 on July 6, 1979

Portrait of Archduke Leopold Wilhelm of Austria, in front of siege of Gravelines in 1652. (Painting, c.1655)
Portrait of Archduke Leopold Wilhelm of Austria, in front of siege of Gravelines in 1652. (Painting, c.1655)

LRI4574712: Portrait of Archduke Leopold Wilhelm of Austria, in front of siege of Gravelines in 1652. (Painting, c.1655), Teniers, David the Younger (1610-90) / Bridgeman Images

ID: LRI4574712

Portrait of Archduke Leopold Wilhelm of Austria, in front of siege of Gravelines in 1652. (Painting, c.1655)

Teniers, David the Younger (1610-90)

Io satellite of Jupiter seen in section - Probable structure of the interior of satellite Io. A metallic core (grey) of iron or nickel surrounds a shell of rocks to the surface
Io satellite of Jupiter seen in section - Probable structure of the interior of satellite Io. A metallic core (grey) of iron or nickel surrounds a shell of rocks to the surface

PIX4574797: Io satellite of Jupiter seen in section - Probable structure of the interior of satellite Io. A metallic core (grey) of iron or nickel surrounds a shell of rocks to the surface / Bridgeman Images

ID: PIX4574797

Io satellite of Jupiter seen in section - Probable structure of the interior of satellite Io. A metallic core (grey) of iron or nickel surrounds a shell of rocks to the surface

The Actions of Louis II Prince of Bourbon Conde known as the Grand Conde, Battle of Brie Count Robert Detail, 17th century (oil on canvas)
The Actions of Louis II Prince of Bourbon Conde known as the Grand Conde, Battle of Brie Count Robert Detail, 17th century (oil on canvas)

JLJ4574923: The Actions of Louis II Prince of Bourbon Conde known as the Grand Conde, Battle of Brie Count Robert Detail, 17th century (oil on canvas), Le Conte, Sauveur (1659-94) / Bridgeman Images

ID: JLJ4574923

The Actions of Louis II Prince of Bourbon Conde known as the Grand Conde, Battle of Brie Count Robert Detail, 17th century (oil on canvas)

Le Conte, Sauveur (1659-94)

Ganymede - Jupiter Satellite 02 - 2007 - The Jupiter satellite, Ganymede, seen on 27 February 2007 by the New Horizons probe has a distance of 3.5 million km. The image is a composite of visible and infrared data
Ganymede - Jupiter Satellite 02 - 2007 - The Jupiter satellite, Ganymede, seen on 27 February 2007 by the New Horizons probe has a distance of 3.5 million km. The image is a composite of visible and infrared data

PIX4574947: Ganymede - Jupiter Satellite 02 - 2007 - The Jupiter satellite, Ganymede, seen on 27 February 2007 by the New Horizons probe has a distance of 3.5 million km. The image is a composite of visible and infrared data / Bridgeman Images

ID: PIX4574947

Ganymede - Jupiter Satellite 02 - 2007 - The Jupiter satellite, Ganymede, seen on 27 February 2007 by the New Horizons probe has a distance of 3.5 million km. The image is a composite of visible and infrared data


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