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Galaxy NGC 2964 in the Lion - Galaxy NGC 2964 in Leo - NGC 2964 is a barred spiral galaxy located at a distance of about 71 million years - light. In the center of the image is the galaxy NGC 2968 and in the upper right is the galaxy NGC 2970. NGC 2964, a barred spiral galaxy in Leo. In the center of the image is galaxy NGC 2968 and top right is the galaxy NGC 2970
Galaxy NGC 2964 in the Lion - Galaxy NGC 2964 in Leo - NGC 2964 is a barred spiral galaxy located at a distance of about 71 million years - light. In the center of the image is the galaxy NGC 2968 and in the upper right is the galaxy NGC 2970. NGC 2964, a barred spiral galaxy in Leo. In the center of the image is galaxy NGC 2968 and top right is the galaxy NGC 2970

PIX4610256: Galaxy NGC 2964 in the Lion - Galaxy NGC 2964 in Leo - NGC 2964 is a barred spiral galaxy located at a distance of about 71 million years - light. In the center of the image is the galaxy NGC 2968 and in the upper right is the galaxy NGC 2970. NGC 2964, a barred spiral galaxy in Leo. In the center of the image is galaxy NGC 2968 and top right is the galaxy NGC 2970 / Bridgeman Images

ID: PIX4610256

Galaxy NGC 2964 in the Lion - Galaxy NGC 2964 in Leo - NGC 2964 is a barred spiral galaxy located at a distance of about 71 million years - light. In the center of the image is the galaxy NGC 2968 and in the upper right is the galaxy NGC 2970. NGC 2964, a barred spiral galaxy in Leo. In the center of the image is galaxy NGC 2968 and top right is the galaxy NGC 2970

Terre de nuit - Pole Sud - Earth at night - South Pole - The Earth centree on the South Pole observed at night by satellite. The Earth with city lights seen from satellite, centered on south pole
Terre de nuit - Pole Sud - Earth at night - South Pole - The Earth centree on the South Pole observed at night by satellite. The Earth with city lights seen from satellite, centered on south pole

PIX4632507: Terre de nuit - Pole Sud - Earth at night - South Pole - The Earth centree on the South Pole observed at night by satellite. The Earth with city lights seen from satellite, centered on south pole / Bridgeman Images

ID: PIX4632507

Terre de nuit - Pole Sud - Earth at night - South Pole - The Earth centree on the South Pole observed at night by satellite. The Earth with city lights seen from satellite, centered on south pole

Earth by night - Earth by night - Earth by night satellite. Mosaic of hundreds of images obtained by DMSP (Defense Meteorological Satellite Program) satellites in 2003. This image shows Earth's human - generated nighttime lights for the calendar year 2003, based on observations by the Defense Meteorological Satellite Program Operational Line Scanner. In this image, oceans appear black, landmasses appear in varying shades of blue, and lights appear yellow - white. Because these images focus on human impact, they do not include other (natural) light sources. Besides assembling cloud - free images, data visualizers carefully excluded sunlight, moonlight, and light from the Northern Hemisphere aurora
Earth by night - Earth by night - Earth by night satellite. Mosaic of hundreds of images obtained by DMSP (Defense Meteorological Satellite Program) satellites in 2003. This image shows Earth's human - generated nighttime lights for the calendar year 2003, based on observations by the Defense Meteorological Satellite Program Operational Line Scanner. In this image, oceans appear black, landmasses appear in varying shades of blue, and lights appear yellow - white. Because these images focus on human impact, they do not include other (natural) light sources. Besides assembling cloud - free images, data visualizers carefully excluded sunlight, moonlight, and light from the Northern Hemisphere aurora

PIX4632529: Earth by night - Earth by night - Earth by night satellite. Mosaic of hundreds of images obtained by DMSP (Defense Meteorological Satellite Program) satellites in 2003. This image shows Earth's human - generated nighttime lights for the calendar year 2003, based on observations by the Defense Meteorological Satellite Program Operational Line Scanner. In this image, oceans appear black, landmasses appear in varying shades of blue, and lights appear yellow - white. Because these images focus on human impact, they do not include other (natural) light sources. Besides assembling cloud - free images, data visualizers carefully excluded sunlight, moonlight, and light from the Northern Hemisphere aurora / Bridgeman Images

ID: PIX4632529

Earth by night - Earth by night - Earth by night satellite. Mosaic of hundreds of images obtained by DMSP (Defense Meteorological Satellite Program) satellites in 2003. This image shows Earth's human - generated nighttime lights for the calendar year 2003, based on observations by the Defense Meteorological Satellite Program Operational Line Scanner. In this image, oceans appear black, landmasses appear in varying shades of blue, and lights appear yellow - white. Because these images focus on human impact, they do not include other (natural) light sources. Besides assembling cloud - free images, data visualizers carefully excluded sunlight, moonlight, and light from the Northern Hemisphere aurora

Evian les Bains (Haute Savoie).
Evian les Bains (Haute Savoie).

TEC4632561: Evian les Bains (Haute Savoie). / Bridgeman Images

ID: TEC4632561

Evian les Bains (Haute Savoie).

Evian les Bains (Haute Savoie).
Evian les Bains (Haute Savoie).

TEC4632566: Evian les Bains (Haute Savoie). / Bridgeman Images

ID: TEC4632566

Evian les Bains (Haute Savoie).

First plants on Earth - Artist view - First plants - Artist view - Artist view - Artist view of the first plants (Cooksonia caledonica) that appeared on Earth in Silurian more than 400 million years ago. Species of Cooksonia caledonica, the only witness to a spectacular Late Silurian sunset, establish a tenuous foothold on a mound of ancient lava. 600 million years ago the Earth's oceans were teaming with life, however it wasn't until 200 million years later that the first plants emerged from the waters and made the Earth's surface their home. They were simple plants, standing only a few inches tall, consisting of slender stalks with branches and rounded structures called sporangia. The sporangia, common to funguses and non - seed plants, produced and contained the spores required for reproduction
First plants on Earth - Artist view - First plants - Artist view - Artist view - Artist view of the first plants (Cooksonia caledonica) that appeared on Earth in Silurian more than 400 million years ago. Species of Cooksonia caledonica, the only witness to a spectacular Late Silurian sunset, establish a tenuous foothold on a mound of ancient lava. 600 million years ago the Earth's oceans were teaming with life, however it wasn't until 200 million years later that the first plants emerged from the waters and made the Earth's surface their home. They were simple plants, standing only a few inches tall, consisting of slender stalks with branches and rounded structures called sporangia. The sporangia, common to funguses and non - seed plants, produced and contained the spores required for reproduction

PIX4632750: First plants on Earth - Artist view - First plants - Artist view - Artist view - Artist view of the first plants (Cooksonia caledonica) that appeared on Earth in Silurian more than 400 million years ago. Species of Cooksonia caledonica, the only witness to a spectacular Late Silurian sunset, establish a tenuous foothold on a mound of ancient lava. 600 million years ago the Earth's oceans were teaming with life, however it wasn't until 200 million years later that the first plants emerged from the waters and made the Earth's surface their home. They were simple plants, standing only a few inches tall, consisting of slender stalks with branches and rounded structures called sporangia. The sporangia, common to funguses and non - seed plants, produced and contained the spores required for reproduction / Bridgeman Images

ID: PIX4632750

First plants on Earth - Artist view - First plants - Artist view - Artist view - Artist view of the first plants (Cooksonia caledonica) that appeared on Earth in Silurian more than 400 million years ago. Species of Cooksonia caledonica, the only witness to a spectacular Late Silurian sunset, establish a tenuous foothold on a mound of ancient lava. 600 million years ago the Earth's oceans were teaming with life, however it wasn't until 200 million years later that the first plants emerged from the waters and made the Earth's surface their home. They were simple plants, standing only a few inches tall, consisting of slender stalks with branches and rounded structures called sporangia. The sporangia, common to funguses and non - seed plants, produced and contained the spores required for reproduction

Devonian Canopee - Artist's View - Devonian Canopy - Artist's View of an Archaeopteris Forest about 380 million years ago. The fossil record reveals that great forests of Archaeopteris covered much of the Earth 380 million years ago. The large umbrella - like fronds appear to have been optimized for gathering sunlight at the canopy level while still permitting enough light to reach the shorter and younger trees. It was great forests like these that helped to draw much of the carbon dioxide out of the primeval air while releasing the oxygen we breathe today
Devonian Canopee - Artist's View - Devonian Canopy - Artist's View of an Archaeopteris Forest about 380 million years ago. The fossil record reveals that great forests of Archaeopteris covered much of the Earth 380 million years ago. The large umbrella - like fronds appear to have been optimized for gathering sunlight at the canopy level while still permitting enough light to reach the shorter and younger trees. It was great forests like these that helped to draw much of the carbon dioxide out of the primeval air while releasing the oxygen we breathe today

PIX4632762: Devonian Canopee - Artist's View - Devonian Canopy - Artist's View of an Archaeopteris Forest about 380 million years ago. The fossil record reveals that great forests of Archaeopteris covered much of the Earth 380 million years ago. The large umbrella - like fronds appear to have been optimized for gathering sunlight at the canopy level while still permitting enough light to reach the shorter and younger trees. It was great forests like these that helped to draw much of the carbon dioxide out of the primeval air while releasing the oxygen we breathe today / Bridgeman Images

ID: PIX4632762

Devonian Canopee - Artist's View - Devonian Canopy - Artist's View of an Archaeopteris Forest about 380 million years ago. The fossil record reveals that great forests of Archaeopteris covered much of the Earth 380 million years ago. The large umbrella - like fronds appear to have been optimized for gathering sunlight at the canopy level while still permitting enough light to reach the shorter and younger trees. It was great forests like these that helped to draw much of the carbon dioxide out of the primeval air while releasing the oxygen we breathe today

View of the Burgess Wildlife Artist - View of the Burgess Wildlife Artist - View of the Cambrian Wildlife Artist (- 500 million years) reconstructed from fossils discovered in the early 20th century near Mount Burgess in Canada
View of the Burgess Wildlife Artist - View of the Burgess Wildlife Artist - View of the Cambrian Wildlife Artist (- 500 million years) reconstructed from fossils discovered in the early 20th century near Mount Burgess in Canada

PIX4633194: View of the Burgess Wildlife Artist - View of the Burgess Wildlife Artist - View of the Cambrian Wildlife Artist (- 500 million years) reconstructed from fossils discovered in the early 20th century near Mount Burgess in Canada / Bridgeman Images

ID: PIX4633194

View of the Burgess Wildlife Artist - View of the Burgess Wildlife Artist - View of the Cambrian Wildlife Artist (- 500 million years) reconstructed from fossils discovered in the early 20th century near Mount Burgess in Canada

The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.
The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

TEC4629478: The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007. / Bridgeman Images

ID: TEC4629478

The interurban road station of Brasilia (Brazil). Architect Lucio Costa, 1960. Photography 2007.

The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006
The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006

PIX4629533: The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006 / Bridgeman Images

ID: PIX4629533

The dwarf planet Eris and its satellite Dysnomie - The dwarf planet Eris and its satellite Dysnomie seen by the Hubble space telescope on August 30, 2006

Pilotis of a residential building of a superquadra in Brasilia (Brazil).
Pilotis of a residential building of a superquadra in Brasilia (Brazil).

TEC4629557: Pilotis of a residential building of a superquadra in Brasilia (Brazil). / Bridgeman Images

ID: TEC4629557

Pilotis of a residential building of a superquadra in Brasilia (Brazil).

Building of a superquadra in Brasilia (Brazil). Photography 16/04/07
Building of a superquadra in Brasilia (Brazil). Photography 16/04/07

TEC4629618: Building of a superquadra in Brasilia (Brazil). Photography 16/04/07 / Bridgeman Images

ID: TEC4629618

Building of a superquadra in Brasilia (Brazil). Photography 16/04/07

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

TEC4629731: The southern banking sector in Brasilia (Brazil). / Bridgeman Images

ID: TEC4629731

The southern banking sector in Brasilia (Brazil).

Comparison of Sun Sizes and Jupiter - Sun Diametre: 1,395,000 km Jupiter Diametre: 142,984 k
Comparison of Sun Sizes and Jupiter - Sun Diametre: 1,395,000 km Jupiter Diametre: 142,984 k

PIX4629741: Comparison of Sun Sizes and Jupiter - Sun Diametre: 1,395,000 km Jupiter Diametre: 142,984 k / Bridgeman Images

ID: PIX4629741

Comparison of Sun Sizes and Jupiter - Sun Diametre: 1,395,000 km Jupiter Diametre: 142,984 k

Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's
Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's

PIX4629805: Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's / Bridgeman Images

ID: PIX4629805

Earth and Mars - Earth and Mars - Artist's view of Earth and Mars. The diameter of the planet Mars is half the diameter of the Earth. Artwork showing the Earth and Mars (in foreground). Mars' diameter is half that of the Earth's

Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k
Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k

PIX4629886: Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k / Bridgeman Images

ID: PIX4629886

Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k

Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. Also visible in this photo is the quasar Q0957+561, 9 billion years away - light. The NGC 3079 spiral galaxy is located at about 50 million light years from Earth. Its dics is approximately 70,000 light years wide. The Q0957+561 twin quasar, roughly at 9 billion light years away, is also visible in this image
Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. Also visible in this photo is the quasar Q0957+561, 9 billion years away - light. The NGC 3079 spiral galaxy is located at about 50 million light years from Earth. Its dics is approximately 70,000 light years wide. The Q0957+561 twin quasar, roughly at 9 billion light years away, is also visible in this image

PIX4610486: Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. Also visible in this photo is the quasar Q0957+561, 9 billion years away - light. The NGC 3079 spiral galaxy is located at about 50 million light years from Earth. Its dics is approximately 70,000 light years wide. The Q0957+561 twin quasar, roughly at 9 billion light years away, is also visible in this image / Bridgeman Images

ID: PIX4610486

Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. Also visible in this photo is the quasar Q0957+561, 9 billion years away - light. The NGC 3079 spiral galaxy is located at about 50 million light years from Earth. Its dics is approximately 70,000 light years wide. The Q0957+561 twin quasar, roughly at 9 billion light years away, is also visible in this image

Galaxies M95 and M96 in the Lion - Galaxies M95 and M96 in Leo - M95 (NGC 3351), on the left, is a barree spiral of type SBB, M96 (NGC 3368), on the right, is a spiral galaxy of type Sa. M96 is the brightest member of the Leo I galaxy group, which is also called the M96 group. It also contains M95, M105 and a number of weaker galaxies. Their distance to our Sun was measured with great precision thanks to the discovery of cepheides in these galaxies and the appearance of a supernova of type Ia in M96 in May 1998. These two galaxies are located 37 million light years away from Earth. M95 (NGC 3351, left), is a barred spiral galaxy, M96 (NGC 3368, right), is a spiral galaxy. With M105 (not pictured here), they are dominant members of the Leo I galactic group which also includes several fainter galaxies. Their distance from our Sun has been determinated with great precision thanks to the discovery of Cepheids stars in these galaxies and a type IA supernova in M96 appeared in May 1998. Their distance to our Sun is 37 million light - years
Galaxies M95 and M96 in the Lion - Galaxies M95 and M96 in Leo - M95 (NGC 3351), on the left, is a barree spiral of type SBB, M96 (NGC 3368), on the right, is a spiral galaxy of type Sa. M96 is the brightest member of the Leo I galaxy group, which is also called the M96 group. It also contains M95, M105 and a number of weaker galaxies. Their distance to our Sun was measured with great precision thanks to the discovery of cepheides in these galaxies and the appearance of a supernova of type Ia in M96 in May 1998. These two galaxies are located 37 million light years away from Earth. M95 (NGC 3351, left), is a barred spiral galaxy, M96 (NGC 3368, right), is a spiral galaxy. With M105 (not pictured here), they are dominant members of the Leo I galactic group which also includes several fainter galaxies. Their distance from our Sun has been determinated with great precision thanks to the discovery of Cepheids stars in these galaxies and a type IA supernova in M96 appeared in May 1998. Their distance to our Sun is 37 million light - years

PIX4610672: Galaxies M95 and M96 in the Lion - Galaxies M95 and M96 in Leo - M95 (NGC 3351), on the left, is a barree spiral of type SBB, M96 (NGC 3368), on the right, is a spiral galaxy of type Sa. M96 is the brightest member of the Leo I galaxy group, which is also called the M96 group. It also contains M95, M105 and a number of weaker galaxies. Their distance to our Sun was measured with great precision thanks to the discovery of cepheides in these galaxies and the appearance of a supernova of type Ia in M96 in May 1998. These two galaxies are located 37 million light years away from Earth. M95 (NGC 3351, left), is a barred spiral galaxy, M96 (NGC 3368, right), is a spiral galaxy. With M105 (not pictured here), they are dominant members of the Leo I galactic group which also includes several fainter galaxies. Their distance from our Sun has been determinated with great precision thanks to the discovery of Cepheids stars in these galaxies and a type IA supernova in M96 appeared in May 1998. Their distance to our Sun is 37 million light - years / Bridgeman Images

ID: PIX4610672

Galaxies M95 and M96 in the Lion - Galaxies M95 and M96 in Leo - M95 (NGC 3351), on the left, is a barree spiral of type SBB, M96 (NGC 3368), on the right, is a spiral galaxy of type Sa. M96 is the brightest member of the Leo I galaxy group, which is also called the M96 group. It also contains M95, M105 and a number of weaker galaxies. Their distance to our Sun was measured with great precision thanks to the discovery of cepheides in these galaxies and the appearance of a supernova of type Ia in M96 in May 1998. These two galaxies are located 37 million light years away from Earth. M95 (NGC 3351, left), is a barred spiral galaxy, M96 (NGC 3368, right), is a spiral galaxy. With M105 (not pictured here), they are dominant members of the Leo I galactic group which also includes several fainter galaxies. Their distance from our Sun has been determinated with great precision thanks to the discovery of Cepheids stars in these galaxies and a type IA supernova in M96 appeared in May 1998. Thei

Spiral galaxy NGC 3628 in the Lion - NGC 3628 spiral galaxy in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with a 400 mm telescope, 2h15mn installation through different filters. NGC 3628 is an edge - on sipral galaxy about 35 Mly away. She forms the remarkable Leo triplet with its neighbors M65 and M66
Spiral galaxy NGC 3628 in the Lion - NGC 3628 spiral galaxy in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with a 400 mm telescope, 2h15mn installation through different filters. NGC 3628 is an edge - on sipral galaxy about 35 Mly away. She forms the remarkable Leo triplet with its neighbors M65 and M66

PIX4610853: Spiral galaxy NGC 3628 in the Lion - NGC 3628 spiral galaxy in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with a 400 mm telescope, 2h15mn installation through different filters. NGC 3628 is an edge - on sipral galaxy about 35 Mly away. She forms the remarkable Leo triplet with its neighbors M65 and M66 / Bridgeman Images

ID: PIX4610853

Spiral galaxy NGC 3628 in the Lion - NGC 3628 spiral galaxy in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with a 400 mm telescope, 2h15mn installation through different filters. NGC 3628 is an edge - on sipral galaxy about 35 Mly away. She forms the remarkable Leo triplet with its neighbors M65 and M66

Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with Siding Spring's 3.9m telescope. This picture has been specially enhanced to reveal NGC 3628, which is seen as an edge - on spiral galaxy, crossed by a dust lane. Galaxies seen edge - on are rare, but this example has other peculiarities. The dust lane is distinctly askew and the ends of the spiral arms are obviously puffed out, with evidence of star formation. The bright bulge of the galaxy also has an unusual 'peanut' shape. This suggests that the galaxies of the Leo group are interacting, gradually pulling each other apart as they orbit each other. Image obtained with the 3.9m telescope of Siding Spring
Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with Siding Spring's 3.9m telescope. This picture has been specially enhanced to reveal NGC 3628, which is seen as an edge - on spiral galaxy, crossed by a dust lane. Galaxies seen edge - on are rare, but this example has other peculiarities. The dust lane is distinctly askew and the ends of the spiral arms are obviously puffed out, with evidence of star formation. The bright bulge of the galaxy also has an unusual 'peanut' shape. This suggests that the galaxies of the Leo group are interacting, gradually pulling each other apart as they orbit each other. Image obtained with the 3.9m telescope of Siding Spring

PIX4610870: Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with Siding Spring's 3.9m telescope. This picture has been specially enhanced to reveal NGC 3628, which is seen as an edge - on spiral galaxy, crossed by a dust lane. Galaxies seen edge - on are rare, but this example has other peculiarities. The dust lane is distinctly askew and the ends of the spiral arms are obviously puffed out, with evidence of star formation. The bright bulge of the galaxy also has an unusual 'peanut' shape. This suggests that the galaxies of the Leo group are interacting, gradually pulling each other apart as they orbit each other. Image obtained with the 3.9m telescope of Siding Spring / Bridgeman Images

ID: PIX4610870

Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. Image obtained with Siding Spring's 3.9m telescope. This picture has been specially enhanced to reveal NGC 3628, which is seen as an edge - on spiral galaxy, crossed by a dust lane. Galaxies seen edge - on are rare, but this example has other peculiarities. The dust lane is distinctly askew and the ends of the spiral arms are obviously puffed out, with evidence of star formation. The bright bulge of the galaxy also has an unusual 'peanut' shape. This suggests that the galaxies of the Leo group are interacting, gradually pulling each other apart as they orbit each other. Image obtained with the 3.9m telescope of Siding Spring

Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. This edge - on galaxy lies about 35 million light years away. It is the fainter member of the Leo triplet, a group of galaxies dominated by M65 and M66
Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. This edge - on galaxy lies about 35 million light years away. It is the fainter member of the Leo triplet, a group of galaxies dominated by M65 and M66

PIX4610901: Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. This edge - on galaxy lies about 35 million light years away. It is the fainter member of the Leo triplet, a group of galaxies dominated by M65 and M66 / Bridgeman Images

ID: PIX4610901

Spiral Galaxy NGC 3628 in the Lion - Spiral galaxy NGC 3628 in Leo - NGC 3628 is a spiral galaxy seen by the slice located at a distance of about 35 million years - light. With its neighbors M65 and M66, it forms a remarkable triplet of galaxies, called the Lion Triplet or the M66 Group. This edge - on galaxy lies about 35 million light years away. It is the fainter member of the Leo triplet, a group of galaxies dominated by M65 and M66

Spiral galaxy NGC 3982 in the Great Bear - Spiral galaxy NGC 3982 in Ursa Major - The spiral galaxy NGC 3982 is located about 68 million years ago - light from Earth. It extends over about 30,000 light years. It is a spiral galaxy that houses a black hole in its heart and large zones of star formation in its arms. This image was taken by the Hubble Space Telescope (HST). This face - on spiral galaxy, called NGC 3982, is striking for its rich tapestry of star birth, along with its winding arms. The arms are lined with pink star - forming regions of glowing hydrogen, newborn blue star clusters, and obscuring dust lanes that provide the raw material for future generations of stars. The bright nucleus is home to an older population of stars, which grow ever more densely packed towards the center. NGC 3982 is located about 68 million light - years away in the constellation Ursa Major. The galaxy spans about 30,000 light - years, one - third of the size of our Milky Way galaxy. This color image is composed of exposures taken by the Hubble Space Telescope's Wide Field Camera 3 (WFC3), the Advanced Camera for Surveys (ACS), and the Wide Field Planetary Camera 2 (WFPC2). The observations were taken between March 2000 and August 2009
Spiral galaxy NGC 3982 in the Great Bear - Spiral galaxy NGC 3982 in Ursa Major - The spiral galaxy NGC 3982 is located about 68 million years ago - light from Earth. It extends over about 30,000 light years. It is a spiral galaxy that houses a black hole in its heart and large zones of star formation in its arms. This image was taken by the Hubble Space Telescope (HST). This face - on spiral galaxy, called NGC 3982, is striking for its rich tapestry of star birth, along with its winding arms. The arms are lined with pink star - forming regions of glowing hydrogen, newborn blue star clusters, and obscuring dust lanes that provide the raw material for future generations of stars. The bright nucleus is home to an older population of stars, which grow ever more densely packed towards the center. NGC 3982 is located about 68 million light - years away in the constellation Ursa Major. The galaxy spans about 30,000 light - years, one - third of the size of our Milky Way galaxy. This color image is composed of exposures taken by the Hubble Space Telescope's Wide Field Camera 3 (WFC3), the Advanced Camera for Surveys (ACS), and the Wide Field Planetary Camera 2 (WFPC2). The observations were taken between March 2000 and August 2009

PIX4610993: Spiral galaxy NGC 3982 in the Great Bear - Spiral galaxy NGC 3982 in Ursa Major - The spiral galaxy NGC 3982 is located about 68 million years ago - light from Earth. It extends over about 30,000 light years. It is a spiral galaxy that houses a black hole in its heart and large zones of star formation in its arms. This image was taken by the Hubble Space Telescope (HST). This face - on spiral galaxy, called NGC 3982, is striking for its rich tapestry of star birth, along with its winding arms. The arms are lined with pink star - forming regions of glowing hydrogen, newborn blue star clusters, and obscuring dust lanes that provide the raw material for future generations of stars. The bright nucleus is home to an older population of stars, which grow ever more densely packed towards the center. NGC 3982 is located about 68 million light - years away in the constellation Ursa Major. The galaxy spans about 30,000 light - years, one - third of the size of our Milky Way galaxy. This color image is composed of exposures taken by the Hubble Space Telescope's Wide Field Camera 3 (WFC3), the Advanced Camera for Surveys (ACS), and the Wide Field Planetary Camera 2 (WFPC2). The observations were taken between March 2000 and August 2009 / Bridgeman Images

ID: PIX4610993

Spiral galaxy NGC 3982 in the Great Bear - Spiral galaxy NGC 3982 in Ursa Major - The spiral galaxy NGC 3982 is located about 68 million years ago - light from Earth. It extends over about 30,000 light years. It is a spiral galaxy that houses a black hole in its heart and large zones of star formation in its arms. This image was taken by the Hubble Space Telescope (HST). This face - on spiral galaxy, called NGC 3982, is striking for its rich tapestry of star birth, along with its winding arms. The arms are lined with pink star - forming regions of glowing hydrogen, newborn blue star clusters, and obscuring dust lanes that provide the raw material for future generations of stars. The bright nucleus is home to an older population of stars, which grow ever more densely packed towards the center. NGC 3982 is located about 68 million light - years away in the constellation Ursa Major. The galaxy spans about 30,000 light - years, one - third of the size of our Milky Way galaxy. This color im

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. One of his arms is more extended, probably by the presence of a nearby dwarf galaxy. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting galaxies
Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. One of his arms is more extended, probably by the presence of a nearby dwarf galaxy. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting galaxies

PIX4611054: Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. One of his arms is more extended, probably by the presence of a nearby dwarf galaxy. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting galaxies / Bridgeman Images

ID: PIX4611054

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. One of his arms is more extended, probably by the presence of a nearby dwarf galaxy. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting gala

Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway
Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway

PIX4633623: Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway / Bridgeman Images

ID: PIX4633623

Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway

Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway
Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway

PIX4633631: Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway / Bridgeman Images

ID: PIX4633631

Aurore boreale and photographers - Norway - Aurora borealis and photographers - Norway

Watching an Aurora boreale - Norway - Watching an Aurora borealis - Norway
Watching an Aurora boreale - Norway - Watching an Aurora borealis - Norway

PIX4633680: Watching an Aurora boreale - Norway - Watching an Aurora borealis - Norway / Bridgeman Images

ID: PIX4633680

Watching an Aurora boreale - Norway - Watching an Aurora borealis - Norway

Aurore boreale au clair de Lune - Norway - Aurora borealis with Moonlight - Norway - Aurore boreale a Lofoten, Norway. 21 March 2016
Aurore boreale au clair de Lune - Norway - Aurora borealis with Moonlight - Norway - Aurore boreale a Lofoten, Norway. 21 March 2016

PIX4633868: Aurore boreale au clair de Lune - Norway - Aurora borealis with Moonlight - Norway - Aurore boreale a Lofoten, Norway. 21 March 2016 / Bridgeman Images

ID: PIX4633868

Aurore boreale au clair de Lune - Norway - Aurora borealis with Moonlight - Norway - Aurore boreale a Lofoten, Norway. 21 March 2016

Aurore boreale - Lofoten - Norway - Aurora Borealis above a snow covered traditional village in the Lofoten Islands, Norway
Aurore boreale - Lofoten - Norway - Aurora Borealis above a snow covered traditional village in the Lofoten Islands, Norway

PIX4633928: Aurore boreale - Lofoten - Norway - Aurora Borealis above a snow covered traditional village in the Lofoten Islands, Norway / Bridgeman Images

ID: PIX4633928

Aurore boreale - Lofoten - Norway - Aurora Borealis above a snow covered traditional village in the Lofoten Islands, Norway

Halo around the Moon - Lunar Halo - This halo is due to the light of the full moon reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Moon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter
Halo around the Moon - Lunar Halo - This halo is due to the light of the full moon reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Moon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter

PIX4634038: Halo around the Moon - Lunar Halo - This halo is due to the light of the full moon reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Moon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter / Bridgeman Images

ID: PIX4634038

Halo around the Moon - Lunar Halo - This halo is due to the light of the full moon reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and cause a perfect circle around the Moon. Lunar halos are caused by moonlight being refracted by cirro-stratus clouds. These thin clouds are located very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo that is 44 degrees in diameter

Rays of Light in the Fog - Rays of Light in a foggy night: The light of a floor lamp diffuses into the fog. Spicheren, France. Rays of light from a street lamp in fog. Spicheren, France
Rays of Light in the Fog - Rays of Light in a foggy night: The light of a floor lamp diffuses into the fog. Spicheren, France. Rays of light from a street lamp in fog. Spicheren, France

PIX4634046: Rays of Light in the Fog - Rays of Light in a foggy night: The light of a floor lamp diffuses into the fog. Spicheren, France. Rays of light from a street lamp in fog. Spicheren, France / Bridgeman Images

ID: PIX4634046

Rays of Light in the Fog - Rays of Light in a foggy night: The light of a floor lamp diffuses into the fog. Spicheren, France. Rays of light from a street lamp in fog. Spicheren, France

Hurricane Irma seen by satellite 09/2017 - Hurricane Irma 09/2017: Hurricane Irma on September 7, 2017. Image obtained by the American satellite Terra. Terra satellite image of the Hurricane Irma on September 7 2017
Hurricane Irma seen by satellite 09/2017 - Hurricane Irma 09/2017: Hurricane Irma on September 7, 2017. Image obtained by the American satellite Terra. Terra satellite image of the Hurricane Irma on September 7 2017

PIX4634067: Hurricane Irma seen by satellite 09/2017 - Hurricane Irma 09/2017: Hurricane Irma on September 7, 2017. Image obtained by the American satellite Terra. Terra satellite image of the Hurricane Irma on September 7 2017 / Bridgeman Images

ID: PIX4634067

Hurricane Irma seen by satellite 09/2017 - Hurricane Irma 09/2017: Hurricane Irma on September 7, 2017. Image obtained by the American satellite Terra. Terra satellite image of the Hurricane Irma on September 7 2017

The city of Benodet in Brittany.
The city of Benodet in Brittany.

TEC4634167: The city of Benodet in Brittany. / Bridgeman Images

ID: TEC4634167

The city of Benodet in Brittany.

From Big Bang to Today - Evolution of the Universe - Artist's view showing the stages of formation of the universe. This image represents the evolution of the Universe, starting with the Big Bang. The red arrow marks the flow of time
From Big Bang to Today - Evolution of the Universe - Artist's view showing the stages of formation of the universe. This image represents the evolution of the Universe, starting with the Big Bang. The red arrow marks the flow of time

PIX4634267: From Big Bang to Today - Evolution of the Universe - Artist's view showing the stages of formation of the universe. This image represents the evolution of the Universe, starting with the Big Bang. The red arrow marks the flow of time / Bridgeman Images

ID: PIX4634267

From Big Bang to Today - Evolution of the Universe - Artist's view showing the stages of formation of the universe. This image represents the evolution of the Universe, starting with the Big Bang. The red arrow marks the flow of time

The Earth Universe at the Big Bang - Artist's view of the Universe, from its first moments at the top left, to the solar system and the Earth at the right
The Earth Universe at the Big Bang - Artist's view of the Universe, from its first moments at the top left, to the solar system and the Earth at the right

PIX4634281: The Earth Universe at the Big Bang - Artist's view of the Universe, from its first moments at the top left, to the solar system and the Earth at the right / Bridgeman Images

ID: PIX4634281

The Earth Universe at the Big Bang - Artist's view of the Universe, from its first moments at the top left, to the solar system and the Earth at the right

The entrance to the Parc du Centre d'art contemporain, Domaine de Kerguehennec, in Bignan (Morbihan, Brittany). Photography 13/08/09.
The entrance to the Parc du Centre d'art contemporain, Domaine de Kerguehennec, in Bignan (Morbihan, Brittany). Photography 13/08/09.

TEC4634287: The entrance to the Parc du Centre d'art contemporain, Domaine de Kerguehennec, in Bignan (Morbihan, Brittany). Photography 13/08/09. / Bridgeman Images

ID: TEC4634287

The entrance to the Parc du Centre d'art contemporain, Domaine de Kerguehennec, in Bignan (Morbihan, Brittany). Photography 13/08/09.

The contemporary art centre, Domaine de Kerguehennec, in Bignan, Brittany (Morbihan). 1000 concrete pots for an old greenhouse by Jean Pierre Reynaud, 1986, Sculpture Park. Photography 13/08/09
The contemporary art centre, Domaine de Kerguehennec, in Bignan, Brittany (Morbihan). 1000 concrete pots for an old greenhouse by Jean Pierre Reynaud, 1986, Sculpture Park. Photography 13/08/09

TEC4634294: The contemporary art centre, Domaine de Kerguehennec, in Bignan, Brittany (Morbihan). 1000 concrete pots for an old greenhouse by Jean Pierre Reynaud, 1986, Sculpture Park. Photography 13/08/09 / Bridgeman Images

ID: TEC4634294

The contemporary art centre, Domaine de Kerguehennec, in Bignan, Brittany (Morbihan). 1000 concrete pots for an old greenhouse by Jean Pierre Reynaud, 1986, Sculpture Park. Photography 13/08/09


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