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Jupiter eclipse the Sun - Artist's view. - Artist's view of an eclipse of the Sun seen from Callisto, one of Jupiter's satellites. Jupiter eclipses the sun as seen from Callisto
Jupiter eclipse the Sun - Artist's view. - Artist's view of an eclipse of the Sun seen from Callisto, one of Jupiter's satellites. Jupiter eclipses the sun as seen from Callisto

PIX4574880: Jupiter eclipse the Sun - Artist's view. - Artist's view of an eclipse of the Sun seen from Callisto, one of Jupiter's satellites. Jupiter eclipses the sun as seen from Callisto / Bridgeman Images

ID: PIX4574880

Jupiter eclipse the Sun - Artist's view. - Artist's view of an eclipse of the Sun seen from Callisto, one of Jupiter's satellites. Jupiter eclipses the sun as seen from Callisto

Jupiter by the Cassini - Planisphere of Jupiter obtained by the Cassini probe on 11 and 12 December 2000.Composite of 36 images. The finest details are 120 km
Jupiter by the Cassini - Planisphere of Jupiter obtained by the Cassini probe on 11 and 12 December 2000.Composite of 36 images. The finest details are 120 km

PIX4574899: Jupiter by the Cassini - Planisphere of Jupiter obtained by the Cassini probe on 11 and 12 December 2000.Composite of 36 images. The finest details are 120 km / Bridgeman Images

ID: PIX4574899

Jupiter by the Cassini - Planisphere of Jupiter obtained by the Cassini probe on 11 and 12 December 2000.Composite of 36 images. The finest details are 120 km

Surface de Callisto - Illustration - Spires on Callisto - Illustration - Artist's view of erodes ice peaks on the surface of Callisto. In May 2001 Nasa's Galileo spacecraft took the highest resolution images of any of Jupiter's satellites. The images were of the southeastern perimeter of Callisto's massive Asgard impact basin and what they revealed was unlike anything seen before in the Solar System: bright, icy spires rising from an otherwise relatively flat, cratered terrain. The spires may consist of material thrown outward from a major impact billions of years ago. In this image dozens of knobby spires rise into the airless void to twice the height of the Statue of Liberty. Over the eons the dirty ice in the spires has slowly eroded, leaving the non - ice materials to slide down and collect around the base of the spires. As this location is on the side of Callisto that always faces away from Jupiter (the “anti - Jupiter” side), its jovian host would never appear above the horizon
Surface de Callisto - Illustration - Spires on Callisto - Illustration - Artist's view of erodes ice peaks on the surface of Callisto. In May 2001 Nasa's Galileo spacecraft took the highest resolution images of any of Jupiter's satellites. The images were of the southeastern perimeter of Callisto's massive Asgard impact basin and what they revealed was unlike anything seen before in the Solar System: bright, icy spires rising from an otherwise relatively flat, cratered terrain. The spires may consist of material thrown outward from a major impact billions of years ago. In this image dozens of knobby spires rise into the airless void to twice the height of the Statue of Liberty. Over the eons the dirty ice in the spires has slowly eroded, leaving the non - ice materials to slide down and collect around the base of the spires. As this location is on the side of Callisto that always faces away from Jupiter (the “anti - Jupiter” side), its jovian host would never appear above the horizon

PIX4575211: Surface de Callisto - Illustration - Spires on Callisto - Illustration - Artist's view of erodes ice peaks on the surface of Callisto. In May 2001 Nasa's Galileo spacecraft took the highest resolution images of any of Jupiter's satellites. The images were of the southeastern perimeter of Callisto's massive Asgard impact basin and what they revealed was unlike anything seen before in the Solar System: bright, icy spires rising from an otherwise relatively flat, cratered terrain. The spires may consist of material thrown outward from a major impact billions of years ago. In this image dozens of knobby spires rise into the airless void to twice the height of the Statue of Liberty. Over the eons the dirty ice in the spires has slowly eroded, leaving the non - ice materials to slide down and collect around the base of the spires. As this location is on the side of Callisto that always faces away from Jupiter (the “anti - Jupiter” side), its jovian host would never appear above the horizon / Bridgeman Images

ID: PIX4575211

Surface de Callisto - Illustration - Spires on Callisto - Illustration - Artist's view of erodes ice peaks on the surface of Callisto. In May 2001 Nasa's Galileo spacecraft took the highest resolution images of any of Jupiter's satellites. The images were of the southeastern perimeter of Callisto's massive Asgard impact basin and what they revealed was unlike anything seen before in the Solar System: bright, icy spires rising from an otherwise relatively flat, cratered terrain. The spires may consist of material thrown outward from a major impact billions of years ago. In this image dozens of knobby spires rise into the airless void to twice the height of the Statue of Liberty. Over the eons the dirty ice in the spires has slowly eroded, leaving the non - ice materials to slide down and collect around the base of the spires. As this location is on the side of Callisto that always faces away from Jupiter (the “anti - Jupiter” side), its jovian host would never appear above the horizon

The Moon on 17 April 2005, about 8 days old. - The Moon on 17 April 2005, about 8 days old.
The Moon on 17 April 2005, about 8 days old. - The Moon on 17 April 2005, about 8 days old.

PIX4575489: The Moon on 17 April 2005, about 8 days old. - The Moon on 17 April 2005, about 8 days old. / Bridgeman Images

ID: PIX4575489

The Moon on 17 April 2005, about 8 days old. - The Moon on 17 April 2005, about 8 days old.

Honour staircase of Ca Rezzonico in Venice, Italy.
Honour staircase of Ca Rezzonico in Venice, Italy.

TEC4575561: Honour staircase of Ca Rezzonico in Venice, Italy. / Bridgeman Images

ID: TEC4575561

Honour staircase of Ca Rezzonico in Venice, Italy.

Moon about 13 days - Gibous Moon from November 3, 2006 to 22
Moon about 13 days - Gibous Moon from November 3, 2006 to 22

PIX4575603: Moon about 13 days - Gibous Moon from November 3, 2006 to 22 / Bridgeman Images

ID: PIX4575603

Moon about 13 days - Gibous Moon from November 3, 2006 to 22

Lido Beach in Venice, Italy.
Lido Beach in Venice, Italy.

TEC4575613: Lido Beach in Venice, Italy. / Bridgeman Images

ID: TEC4575613

Lido Beach in Venice, Italy.

11 day gibbous moon
11 day gibbous moon

PIX4575620: 11 day gibbous moon / Bridgeman Images

ID: PIX4575620

11 day gibbous moon

12 day gibbous moon
12 day gibbous moon

PIX4575642: 12 day gibbous moon / Bridgeman Images

ID: PIX4575642

12 day gibbous moon

A few hours after the full moon
A few hours after the full moon

PIX4575674: A few hours after the full moon / Bridgeman Images

ID: PIX4575674

A few hours after the full moon

Color Moon - Colorful Moon - The Moon looks white, even orange or red if it is close to the horizon. In reality different shades exist depending on the composition of the soil. By saturating the colours with a digital treatment, the seas (covered with solidified lava) are mostly blue or rust, while the heavily craterized areas are rosatra. 12 July 2006. The Moon seems to be simply white, or orange/red if it is near the horizon. But in fact some colors appear depending on the nature of its terrains. With a digital process to saturate its color, the seas (covered by solid lavas) are mostly blue or orange, and craterised areas are pinkish
Color Moon - Colorful Moon - The Moon looks white, even orange or red if it is close to the horizon. In reality different shades exist depending on the composition of the soil. By saturating the colours with a digital treatment, the seas (covered with solidified lava) are mostly blue or rust, while the heavily craterized areas are rosatra. 12 July 2006. The Moon seems to be simply white, or orange/red if it is near the horizon. But in fact some colors appear depending on the nature of its terrains. With a digital process to saturate its color, the seas (covered by solid lavas) are mostly blue or orange, and craterised areas are pinkish

PIX4575708: Color Moon - Colorful Moon - The Moon looks white, even orange or red if it is close to the horizon. In reality different shades exist depending on the composition of the soil. By saturating the colours with a digital treatment, the seas (covered with solidified lava) are mostly blue or rust, while the heavily craterized areas are rosatra. 12 July 2006. The Moon seems to be simply white, or orange/red if it is near the horizon. But in fact some colors appear depending on the nature of its terrains. With a digital process to saturate its color, the seas (covered by solid lavas) are mostly blue or orange, and craterised areas are pinkish / Bridgeman Images

ID: PIX4575708

Color Moon - Colorful Moon - The Moon looks white, even orange or red if it is close to the horizon. In reality different shades exist depending on the composition of the soil. By saturating the colours with a digital treatment, the seas (covered with solidified lava) are mostly blue or rust, while the heavily craterized areas are rosatra. 12 July 2006. The Moon seems to be simply white, or orange/red if it is near the horizon. But in fact some colors appear depending on the nature of its terrains. With a digital process to saturate its color, the seas (covered by solid lavas) are mostly blue or orange, and craterised areas are pinkish

View of the Palais du Louvre from the Institut de France, Paris 6th arrondissement.
View of the Palais du Louvre from the Institut de France, Paris 6th arrondissement.

TEC4598098: View of the Palais du Louvre from the Institut de France, Paris 6th arrondissement. / Bridgeman Images

ID: TEC4598098

View of the Palais du Louvre from the Institut de France, Paris 6th arrondissement.

Institut de France, College des Quatre Nations, Paris 6th arrondissement. Architect Louis Le Vau (1612-1670).
Institut de France, College des Quatre Nations, Paris 6th arrondissement. Architect Louis Le Vau (1612-1670).

TEC4598155: Institut de France, College des Quatre Nations, Paris 6th arrondissement. Architect Louis Le Vau (1612-1670). / Bridgeman Images

ID: TEC4598155

Institut de France, College des Quatre Nations, Paris 6th arrondissement. Architect Louis Le Vau (1612-1670).

Apollo 17: E. Cernan on the Moon - Apollo 17: E. Cernan at the Lunar Rover Vehicle - E.Cernan and the lunar jeep near Lem. 13/12/1972. Cernan at the Rover prior to EVA - 3 geology traverse. Dec 13 1972
Apollo 17: E. Cernan on the Moon - Apollo 17: E. Cernan at the Lunar Rover Vehicle - E.Cernan and the lunar jeep near Lem. 13/12/1972. Cernan at the Rover prior to EVA - 3 geology traverse. Dec 13 1972

PIX4598217: Apollo 17: E. Cernan on the Moon - Apollo 17: E. Cernan at the Lunar Rover Vehicle - E.Cernan and the lunar jeep near Lem. 13/12/1972. Cernan at the Rover prior to EVA - 3 geology traverse. Dec 13 1972 / Bridgeman Images

ID: PIX4598217

Apollo 17: E. Cernan on the Moon - Apollo 17: E. Cernan at the Lunar Rover Vehicle - E.Cernan and the lunar jeep near Lem. 13/12/1972. Cernan at the Rover prior to EVA - 3 geology traverse. Dec 13 1972

Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. Astronaut Eugene A. Cernan, Apollo 17 commander, is photographed inside the lunar module on the lunar surface following the third extravehicular activity (EVA - 3) of his mission. Note lunar dust on his suit
Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. Astronaut Eugene A. Cernan, Apollo 17 commander, is photographed inside the lunar module on the lunar surface following the third extravehicular activity (EVA - 3) of his mission. Note lunar dust on his suit

PIX4598221: Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. Astronaut Eugene A. Cernan, Apollo 17 commander, is photographed inside the lunar module on the lunar surface following the third extravehicular activity (EVA - 3) of his mission. Note lunar dust on his suit / Bridgeman Images

ID: PIX4598221

Apollo 17: E. Cernan in LEM - Apollo 17: E. Cernan inside the LM after EVA. Dec 13 1972 - Eugene Cernan in the LEM after his third extravehicular release. 13/12/1972. Astronaut Eugene A. Cernan, Apollo 17 commander, is photographed inside the lunar module on the lunar surface following the third extravehicular activity (EVA - 3) of his mission. Note lunar dust on his suit

Aerial view of Badwater Basin, endorheic basin (1988 - Photography)
Aerial view of Badwater Basin, endorheic basin (1988 - Photography)

LRI4598238: Aerial view of Badwater Basin, endorheic basin (1988 - Photography) / Bridgeman Images

ID: LRI4598238

Aerial view of Badwater Basin, endorheic basin (1988 - Photography)

The Ecole Nationale Superieure des Beaux Arts in Paris. Architects Felix Duban (1797-1872) and Francois Debret (1777-1850), reconstructions 1816. The building occupies what remains of the convent of the Petites Augustins (17th century) and the hotel de Chimay (1635), to which buildings were assistant in the 19th century.
The Ecole Nationale Superieure des Beaux Arts in Paris. Architects Felix Duban (1797-1872) and Francois Debret (1777-1850), reconstructions 1816. The building occupies what remains of the convent of the Petites Augustins (17th century) and the hotel de Chimay (1635), to which buildings were assistant in the 19th century.

TEC4598269: The Ecole Nationale Superieure des Beaux Arts in Paris. Architects Felix Duban (1797-1872) and Francois Debret (1777-1850), reconstructions 1816. The building occupies what remains of the convent of the Petites Augustins (17th century) and the hotel de Chimay (1635), to which buildings were assistant in the 19th century. / Bridgeman Images

ID: TEC4598269

The Ecole Nationale Superieure des Beaux Arts in Paris. Architects Felix Duban (1797-1872) and Francois Debret (1777-1850), reconstructions 1816. The building occupies what remains of the convent of the Petites Augustins (17th century) and the hotel de Chimay (1635), to which buildings were assistant in the 19th century.

Aerial view of residential suburbs (1988 - Photography)
Aerial view of residential suburbs (1988 - Photography)

LRI4598280: Aerial view of residential suburbs (1988 - Photography) / Bridgeman Images

ID: LRI4598280

Aerial view of residential suburbs (1988 - Photography)

Pont des Arts, Paris 6th arrondissement. Reconstruction in 1981 by Louis Arretche. The Passerelle des Arts, the first iron bridge in Paris, had the mission of joining the Institut de France and the Louvre, which was then called the Palais des Arts. Reserved for pawns, it was built from 1801 to 1804. It initially consisted of nine arches. Following numerous river accidents, its reconstruction was decided in 1981 but two arches were removed to line them up on the Pont Neuf.
Pont des Arts, Paris 6th arrondissement. Reconstruction in 1981 by Louis Arretche. The Passerelle des Arts, the first iron bridge in Paris, had the mission of joining the Institut de France and the Louvre, which was then called the Palais des Arts. Reserved for pawns, it was built from 1801 to 1804. It initially consisted of nine arches. Following numerous river accidents, its reconstruction was decided in 1981 but two arches were removed to line them up on the Pont Neuf.

TEC4598304: Pont des Arts, Paris 6th arrondissement. Reconstruction in 1981 by Louis Arretche. The Passerelle des Arts, the first iron bridge in Paris, had the mission of joining the Institut de France and the Louvre, which was then called the Palais des Arts. Reserved for pawns, it was built from 1801 to 1804. It initially consisted of nine arches. Following numerous river accidents, its reconstruction was decided in 1981 but two arches were removed to line them up on the Pont Neuf. / Bridgeman Images

ID: TEC4598304

Pont des Arts, Paris 6th arrondissement. Reconstruction in 1981 by Louis Arretche. The Passerelle des Arts, the first iron bridge in Paris, had the mission of joining the Institut de France and the Louvre, which was then called the Palais des Arts. Reserved for pawns, it was built from 1801 to 1804. It initially consisted of nine arches. Following numerous river accidents, its reconstruction was decided in 1981 but two arches were removed to line them up on the Pont Neuf.

La Fontaine Medicis in the Luxembourg Gardens in Paris. Presumably a work by Solomon de Brush 1571-1626) built in the taste of Italian caves with sculptures by Augustus Ottin (1811-1890) made in 1866.
La Fontaine Medicis in the Luxembourg Gardens in Paris. Presumably a work by Solomon de Brush 1571-1626) built in the taste of Italian caves with sculptures by Augustus Ottin (1811-1890) made in 1866.

TEC4598345: La Fontaine Medicis in the Luxembourg Gardens in Paris. Presumably a work by Solomon de Brush 1571-1626) built in the taste of Italian caves with sculptures by Augustus Ottin (1811-1890) made in 1866. / Bridgeman Images

ID: TEC4598345

La Fontaine Medicis in the Luxembourg Gardens in Paris. Presumably a work by Solomon de Brush 1571-1626) built in the taste of Italian caves with sculptures by Augustus Ottin (1811-1890) made in 1866.

Building Felix Potin, 140 bis rue de Rennes Paris 6th arrondissement. Architect Paul Auscher (1866-1932), construction 1904.
Building Felix Potin, 140 bis rue de Rennes Paris 6th arrondissement. Architect Paul Auscher (1866-1932), construction 1904.

TEC4598446: Building Felix Potin, 140 bis rue de Rennes Paris 6th arrondissement. Architect Paul Auscher (1866-1932), construction 1904. / Bridgeman Images

ID: TEC4598446

Building Felix Potin, 140 bis rue de Rennes Paris 6th arrondissement. Architect Paul Auscher (1866-1932), construction 1904.

Building of a superquadra in Brasilia (Brazil).
Building of a superquadra in Brasilia (Brazil).

TEC4629523: Building of a superquadra in Brasilia (Brazil). / Bridgeman Images

ID: TEC4629523

Building of a superquadra in Brasilia (Brazil).

Housing building of a superquadra in Brasilia (Brazil).
Housing building of a superquadra in Brasilia (Brazil).

TEC4629547: Housing building of a superquadra in Brasilia (Brazil). / Bridgeman Images

ID: TEC4629547

Housing building of a superquadra in Brasilia (Brazil).

The curvature of the space-vue d'artiste - The curvature of the space-vue d'artist
The curvature of the space-vue d'artiste - The curvature of the space-vue d'artist

PIX4629695: The curvature of the space-vue d'artiste - The curvature of the space-vue d'artist / Bridgeman Images

ID: PIX4629695

The curvature of the space-vue d'artiste - The curvature of the space-vue d'artist

Comparison of Earth and gas giants planets - Planetary-size comparison: Earth and gas giants planets - Comparison of Earth and Jupiter sizes. Earth diameter: 12 756,28 km Diametre of Jupiter: 142 984 km Diametre of Saturn: 120 000 km Diametre of Uranus: 50 800 km Diametre of Neptune: 49 500 km Size comparison in diametric values: Earth: 12,756.28 km Jupiter: 142,984 km Saturn: 120 000 km Uranus: 50 800 km Neptune: 49 500 k
Comparison of Earth and gas giants planets - Planetary-size comparison: Earth and gas giants planets - Comparison of Earth and Jupiter sizes. Earth diameter: 12 756,28 km Diametre of Jupiter: 142 984 km Diametre of Saturn: 120 000 km Diametre of Uranus: 50 800 km Diametre of Neptune: 49 500 km Size comparison in diametric values: Earth: 12,756.28 km Jupiter: 142,984 km Saturn: 120 000 km Uranus: 50 800 km Neptune: 49 500 k

PIX4629700: Comparison of Earth and gas giants planets - Planetary-size comparison: Earth and gas giants planets - Comparison of Earth and Jupiter sizes. Earth diameter: 12 756,28 km Diametre of Jupiter: 142 984 km Diametre of Saturn: 120 000 km Diametre of Uranus: 50 800 km Diametre of Neptune: 49 500 km Size comparison in diametric values: Earth: 12,756.28 km Jupiter: 142,984 km Saturn: 120 000 km Uranus: 50 800 km Neptune: 49 500 k / Bridgeman Images

ID: PIX4629700

Comparison of Earth and gas giants planets - Planetary-size comparison: Earth and gas giants planets - Comparison of Earth and Jupiter sizes. Earth diameter: 12 756,28 km Diametre of Jupiter: 142 984 km Diametre of Saturn: 120 000 km Diametre of Uranus: 50 800 km Diametre of Neptune: 49 500 km Size comparison in diametric values: Earth: 12,756.28 km Jupiter: 142,984 km Saturn: 120 000 km Uranus: 50 800 km Neptune: 49 500 k

The southern banking sector in Brasilia (Brazil).
The southern banking sector in Brasilia (Brazil).

TEC4629742: The southern banking sector in Brasilia (Brazil). / Bridgeman Images

ID: TEC4629742

The southern banking sector in Brasilia (Brazil).

Distance between Earth and Moon - Earth-Moon system at correct distance - Scale illustration showing distance between Earth and Moon. Planet Saturn has been added for comparison. Earth-Moon system at the correct distance with Saturn for comparison in the middle
Distance between Earth and Moon - Earth-Moon system at correct distance - Scale illustration showing distance between Earth and Moon. Planet Saturn has been added for comparison. Earth-Moon system at the correct distance with Saturn for comparison in the middle

PIX4629750: Distance between Earth and Moon - Earth-Moon system at correct distance - Scale illustration showing distance between Earth and Moon. Planet Saturn has been added for comparison. Earth-Moon system at the correct distance with Saturn for comparison in the middle / Bridgeman Images

ID: PIX4629750

Distance between Earth and Moon - Earth-Moon system at correct distance - Scale illustration showing distance between Earth and Moon. Planet Saturn has been added for comparison. Earth-Moon system at the correct distance with Saturn for comparison in the middle

Comparison of sizes: Objects by Kuiper and France - Planetary-size comparison: Kuiper objects with France - Des objets de Kuiper compares à la France. The planetoides represented are in the background, Eris, then Charon, and Ceres, in the foreground. Some planetoids compared to Earth. The bodies above are, from back to front, Eris, Charon and Ceres
Comparison of sizes: Objects by Kuiper and France - Planetary-size comparison: Kuiper objects with France - Des objets de Kuiper compares à la France. The planetoides represented are in the background, Eris, then Charon, and Ceres, in the foreground. Some planetoids compared to Earth. The bodies above are, from back to front, Eris, Charon and Ceres

PIX4629955: Comparison of sizes: Objects by Kuiper and France - Planetary-size comparison: Kuiper objects with France - Des objets de Kuiper compares à la France. The planetoides represented are in the background, Eris, then Charon, and Ceres, in the foreground. Some planetoids compared to Earth. The bodies above are, from back to front, Eris, Charon and Ceres / Bridgeman Images

ID: PIX4629955

Comparison of sizes: Objects by Kuiper and France - Planetary-size comparison: Kuiper objects with France - Des objets de Kuiper compares à la France. The planetoides represented are in the background, Eris, then Charon, and Ceres, in the foreground. Some planetoids compared to Earth. The bodies above are, from back to front, Eris, Charon and Ceres

Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet
Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet

PIX4630042: Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet / Bridgeman Images

ID: PIX4630042

Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet

Moon about 18 days - Moon 11 - 09 - 2006 Mosaic of 62 images obtained with a telescope and webcam
Moon about 18 days - Moon 11 - 09 - 2006 Mosaic of 62 images obtained with a telescope and webcam

PIX4575775: Moon about 18 days - Moon 11 - 09 - 2006 Mosaic of 62 images obtained with a telescope and webcam / Bridgeman Images

ID: PIX4575775

Moon about 18 days - Moon 11 - 09 - 2006 Mosaic of 62 images obtained with a telescope and webcam

Moon of about 25 days - A 25 day moon - Mosaic of 11 images. 15 August 2009. A 25 day moon, waning crescent. Mosaic of 11 images. August 15, 2009
Moon of about 25 days - A 25 day moon - Mosaic of 11 images. 15 August 2009. A 25 day moon, waning crescent. Mosaic of 11 images. August 15, 2009

PIX4575839: Moon of about 25 days - A 25 day moon - Mosaic of 11 images. 15 August 2009. A 25 day moon, waning crescent. Mosaic of 11 images. August 15, 2009 / Bridgeman Images

ID: PIX4575839

Moon of about 25 days - A 25 day moon - Mosaic of 11 images. 15 August 2009. A 25 day moon, waning crescent. Mosaic of 11 images. August 15, 2009

19 day gibbous moon
19 day gibbous moon

PIX4575846: 19 day gibbous moon / Bridgeman Images

ID: PIX4575846

19 day gibbous moon

Roman roofs, Rome, Italy. Photo 25/01/98.
Roman roofs, Rome, Italy. Photo 25/01/98.

TEC4575925: Roman roofs, Rome, Italy. Photo 25/01/98. / Bridgeman Images

ID: TEC4575925

Roman roofs, Rome, Italy. Photo 25/01/98.

Planted Roman terrace, Rome, Italy.
Planted Roman terrace, Rome, Italy.

TEC4575959: Planted Roman terrace, Rome, Italy. / Bridgeman Images

ID: TEC4575959

Planted Roman terrace, Rome, Italy.

Moon of 26 day
Moon of 26 day

PIX4575964: Moon of 26 day / Bridgeman Images

ID: PIX4575964

Moon of 26 day

The Tiber in Rome, Italy. Photography 25/01/98.
The Tiber in Rome, Italy. Photography 25/01/98.

TEC4575975: The Tiber in Rome, Italy. Photography 25/01/98. / Bridgeman Images

ID: TEC4575975

The Tiber in Rome, Italy. Photography 25/01/98.


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