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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

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

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

Project Mercury: Mastery of Space

Project Mercury: Mastery of Space

BOF745802

An engraving depicting a path of the bright comet of 1556, 16th century

An engraving depicting a path of the bright comet of 1556, 16th century

UIG5311296

Monument to the Conquerors of Space in Moscow, 1971 (b/w photo)

Monument to the Conquerors of Space in Moscow, 1971 (b/w photo)

Alfred Strobel

SZT6305158

An engraving depicting a 36-inch refractor at the Lick Observatory. One of the world's two largest refractors it is on a 'German' style equatorial mounting, with the axis parallel to Earth's polar axis supported on a high pillar. The counterbalance weight for the telescope shows clearly, 20th century

An engraving depicting a 36-inch refractor at the Lick Observatory. One of the world's two largest refractors it is on a 'German' style equatorial mounting, with the axis parallel to Earth's polar axis supported on a high pillar. The counterbalance weight for the telescope shows clearly, 20th century

UIG5311383

An engraving depicting a 36-inch refractor at the Lick Observatory. One of the world's two largest refractors it is on a 'German' style equatorial mounting, with the axis parallel to Earth's polar axis supported on a high pillar. The counterbalance weight for the telescope shows clearly, 19th century

An engraving depicting a 36-inch refractor at the Lick Observatory. One of the world's two largest refractors it is on a 'German' style equatorial mounting, with the axis parallel to Earth's polar axis supported on a high pillar. The counterbalance weight for the telescope shows clearly, 19th century

UIG5311382

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

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

Postcard commemorating 20 years of Soviet space exploration, 1977 (colour litho)

Postcard commemorating 20 years of Soviet space exploration, 1977 (colour litho)

Russian School, (20th century)

LLE5231239

Postage stamps: space exploration:15th anniversary of first manned space mission, 1976, Soviet Union, Columbia mission, 1991, Bulgaria, two astronauts, 1978, Czechoslovakia, 20th century

Postage stamps: space exploration:15th anniversary of first manned space mission, 1976, Soviet Union, Columbia mission, 1991, Bulgaria, two astronauts, 1978, Czechoslovakia, 20th century

DGA2582179

Postage stamps: space exploration: portrait of Yuri Gagarin, 1996, Cuba, Intercosmos program, 1981, Mongolia, Voskhos 2 and Apollo 11 missions, 1982, Hungary, 20th century

Postage stamps: space exploration: portrait of Yuri Gagarin, 1996, Cuba, Intercosmos program, 1981, Mongolia, Voskhos 2 and Apollo 11 missions, 1982, Hungary, 20th century

DGA2582180

Postage stamps: Bicentenary of birth of Alejandro de Humboldt, 1969, 170th anniversary of School of San Alejandro, 1988, card reader by Leopold Romanach, Socialist constitution, 1976, flag, coat of arms, national anthem, Space exploration, Cuba

Postage stamps: Bicentenary of birth of Alejandro de Humboldt, 1969, 170th anniversary of School of San Alejandro, 1988, card reader by Leopold Romanach, Socialist constitution, 1976, flag, coat of arms, national anthem, Space exploration, Cuba

DGA2582184

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316891

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316896

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316894

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316895

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316887

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

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Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316897

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316888

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

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Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316889

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316892

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

premium — Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Echolocation, 2021 (3 channel video projection on Polypropylene Mesh)

Collishaw, Mat (b.1966)

MCW7316890

Genesis, 1969 (colour litho)

Genesis, 1969 (colour litho)

Hepworth, Barbara (1903-75)

WAK3663543

Djorgovski globular cluster 1 in Scorpio - Globular cluster Djorgovski 1 in Scorpius - The Djorgovski globular cluster 1 is a cluster of light stars located near the galactic center, 40,000 years - light from Earth. Its discovery is recent (1987) and studies show that its stars are composed only of hydrogene and helium. The absence of heavier elements that are usually present in stars remains an enigma. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has imaged an area so jam - packed with stars that they almost overwhelm the inky blackness of space. This includes the globular star cluster Djorgovski 1, which was only discovered in 1987 Djorgovski 1 is located close to the centre of our Milky Way Galaxy, within the bulge. If the galaxy is thought of as being like a city, then this bulge is the very busiest district at its centre. Djorgovski 1's proximity to this hub - - within just a few degrees - - explains why the picture is teeming with stars. Globular clusters like Djorgovski 1 formed early in the Milky Way's history, and as such may hold clues about the inner galaxy's early evolution. However, with so much material in the way, obtaining accurate data is problematic. To make matters worse, these stars are faint. Even the most luminous stars in Djorgovski 1 are fainter than the brightest giant stars in the bulge. Another quandary is apparent: how do you know which stars belong to Djorgovski 1, and which are from the bulge? To determine this, astronomers have studied the chemical composition of numerous stars in the area. Stars with a similar composition likely belong in the same group, like siblings in a family. This technique has successfully provided the information to distinguish between stars in Djorgovski 1 and the surrounding bulge. These studies also reveal that Djorgovski 1's stars contain hydrogen and helium, but not much else. In astronomical terms, they — Djorgovski globular cluster 1 in Scorpio - Globular cluster Djorgovski 1 in Scorpius - The Djorgovski globular cluster 1 is a cluster of light stars located near the galactic center, 40,000 years - light from Earth. Its discovery is recent (1987) and studies show that its stars are composed only of hydrogene and helium. The absence of heavier elements that are usually present in stars remains an enigma. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has imaged an area so jam - packed with stars that they almost overwhelm the inky blackness of space. This includes the globular star cluster Djorgovski 1, which was only discovered in 1987 Djorgovski 1 is located close to the centre of our Milky Way Galaxy, within the bulge. If the galaxy is thought of as being like a city, then this bulge is the very busiest district at its centre. Djorgovski 1's proximity to this hub - - within just a few degrees - - explains why the picture is teeming with stars.

Djorgovski globular cluster 1 in Scorpio - Globular cluster Djorgovski 1 in Scorpius - The Djorgovski globular cluster 1 is a cluster of light stars located near the galactic center, 40,000 years - light from Earth. Its discovery is recent (1987) and studies show that its stars are composed only of hydrogene and helium. The absence of heavier elements that are usually present in stars remains an enigma. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has imaged an area so jam - packed with stars that they almost overwhelm the inky blackness of space. This includes the globular star cluster Djorgovski 1, which was only discovered in 1987 Djorgovski 1 is located close to the centre of our Milky Way Galaxy, within the bulge. If the galaxy is thought of as being like a city, then this bulge is the very busiest district at its centre. Djorgovski 1's proximity to this hub - - within just a few degrees - - explains why the picture is teeming with stars.

PIX4565206

Mystery of the 20th century, 1977 (oil on canvas)

Mystery of the 20th century, 1977 (oil on canvas)

Glazunov, Ilya (1930-2017)

FIA5329369

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