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Sep. 14, 1954 - Auditions for the new” T.V. Toppers” team: Auditions were held this morning at the T.V. Theatre- for the forming of a new team for the” Television Toppers”. The” Toppers” are being re-formed by their original dance director Leslie Roberts - as the present director Jack Billings is leaving after working with them for 20 months. Keystone Photo shows the producer Richard Afton in front - with behind - dance director Leslie Roberts surrounded by some of the girls awaiting the audition at the Theater this morning

Sep. 14, 1954 - Auditions for the new” T.V. Toppers” team: Auditions were held this morning at the T.V. Theatre- for the forming of a new team for the” Television Toppers”. The” Toppers” are being re-formed by their original dance director Leslie Roberts - as the present director Jack Billings is leaving after working with them for 20 months. Keystone Photo shows the producer Richard Afton in front - with behind - dance director Leslie Roberts surrounded by some of the girls awaiting the audition at the Theater this morning

ZUM4941786

Noctulescent clouds in Alaska, august 2009 (photo)

Noctulescent clouds in Alaska, august 2009 (photo)

Dennis Anderson

PIX4671632

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

C. Carreau

PIX4645746

Aegean Sea from Space - Aegean Sea from Space - The Aegean Sea, with Greece, Cyclades, Crete and Turkey, seen from the International Space Station (ISS) in March 2010. Crete (foreground), the Cyclades Islands, Greece and Turkey lie along the margin of the Eurasian and African tectonic plates; Africa is moving northward and being driven down beneath Eurasia. As a result volcanic islands, such as Santorini, develop and fault - bounded basin such, as the Gulf of Corinth, are formed. In addition, lavas and sediments that were originally deposited on the Mediterranean seafloor are uplifted and deformed. Image taken from the International Space Station (ISS) in March 2010

Aegean Sea from Space - Aegean Sea from Space - The Aegean Sea, with Greece, Cyclades, Crete and Turkey, seen from the International Space Station (ISS) in March 2010. Crete (foreground), the Cyclades Islands, Greece and Turkey lie along the margin of the Eurasian and African tectonic plates; Africa is moving northward and being driven down beneath Eurasia. As a result volcanic islands, such as Santorini, develop and fault - bounded basin such, as the Gulf of Corinth, are formed. In addition, lavas and sediments that were originally deposited on the Mediterranean seafloor are uplifted and deformed. Image taken from the International Space Station (ISS) in March 2010

PIX4665983

Mars - Noctis Labyrinthus - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

Mars - Noctis Labyrinthus - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

PIX4616427

Mar. 03, 1954 - Training For The Indo-China War: The Lasserre Commando of about a hundred man - divided into small group of 4 or 5 are being specially trained to take over the grounds and villages soon after the withdrawal of the Viet Minh Rebels.They are recruited from the former Viet Minh Prisoners. Soon after taking over the ground from the rebels each part of the Village for battlefield is carefully searched for hidden enemy or war material.Photo Shows Scene during the training of the newly formed Lasserre Commandos at Hadong. in India-China

Mar. 03, 1954 - Training For The Indo-China War: The Lasserre Commando of about a hundred man - divided into small group of 4 or 5 are being specially trained to take over the grounds and villages soon after the withdrawal of the Viet Minh Rebels.They are recruited from the former Viet Minh Prisoners. Soon after taking over the ground from the rebels each part of the Village for battlefield is carefully searched for hidden enemy or war material.Photo Shows Scene during the training of the newly formed Lasserre Commandos at Hadong. in India-China

ZUM4920931

Members of Sreda literary circle, formed in the second half of the 1890s by Russian realistic writers - Portraits of Russian intellectuals of the literary group Znanie: from left to right, Andrei Skitalets (Stephan Gabrilovich Petrov), Leonid Nikolaievich Andreiev, Maxim Gorky (Gorki) (1868-1936), Nikolai Fieshev, the singer Ivanovich (Fedor, Feodor) Chaliapine (1873-1938), Ivan Bunin (Bounine) (1870-1953) and Evgeny Nikola Debut of the 20th century - Members of Sreda. Sreda (Wednesday) was a Moscow literary group founded by Russian author Nikolai Teleshov in 1899. Pictured are (left to right); Stepan Skitalets, Leonid Andreyev, Maxim Gorky, Teleshov, Feodor Chaliapin, Ivan Bunin; Evgeny Chirikov.

Members of Sreda literary circle, formed in the second half of the 1890s by Russian realistic writers - Portraits of Russian intellectuals of the literary group Znanie: from left to right, Andrei Skitalets (Stephan Gabrilovich Petrov), Leonid Nikolaievich Andreiev, Maxim Gorky (Gorki) (1868-1936), Nikolai Fieshev, the singer Ivanovich (Fedor, Feodor) Chaliapine (1873-1938), Ivan Bunin (Bounine) (1870-1953) and Evgeny Nikola Debut of the 20th century - Members of Sreda. Sreda (Wednesday) was a Moscow literary group founded by Russian author Nikolai Teleshov in 1899. Pictured are (left to right); Stepan Skitalets, Leonid Andreyev, Maxim Gorky, Teleshov, Feodor Chaliapin, Ivan Bunin; Evgeny Chirikov.

Stefano Bianchetti

XEE4155660

Shuttle Challenger and Himalayas 10/1984 - Himalayas and the Tibetan Plateau with shuttle Challenger - Part of the Himalayas and Tibet Plateau seen by Shuttle Challenger in October 1984. The Himalayas and the Tibetan Plateau (also known as the Qinghai - Xizang Plateau) shown in this photograph were formed and continue to be modified by the convergent collision of two of the world's great continental tectonic plates, the Eurasian and the Indian - Australian. Towards the horizon, hazy and dusty conditions seem to exist on the Indo - Gangetic Plain of northern India (southwest) and the Takla Makan Desert of western China (northwest)

Shuttle Challenger and Himalayas 10/1984 - Himalayas and the Tibetan Plateau with shuttle Challenger - Part of the Himalayas and Tibet Plateau seen by Shuttle Challenger in October 1984. The Himalayas and the Tibetan Plateau (also known as the Qinghai - Xizang Plateau) shown in this photograph were formed and continue to be modified by the convergent collision of two of the world's great continental tectonic plates, the Eurasian and the Indian - Australian. Towards the horizon, hazy and dusty conditions seem to exist on the Indo - Gangetic Plain of northern India (southwest) and the Takla Makan Desert of western China (northwest)

PIX4650052

Space shuttle Endeavour over Mauritania - Space shuttle above Richat structure, Mauritania - Space shuttle Endeavour seen above the Richat structure, a geological formation of volcanic origin, in Mauritania. Image obtained from the International Space Station (ISS) in 2002. The space shuttle Endeavour above the Richat Structure, a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the international space station (ISS) in 2002

Space shuttle Endeavour over Mauritania - Space shuttle above Richat structure, Mauritania - Space shuttle Endeavour seen above the Richat structure, a geological formation of volcanic origin, in Mauritania. Image obtained from the International Space Station (ISS) in 2002. The space shuttle Endeavour above the Richat Structure, a geological formation in the Maur Adrar Desert in the African country of Mauritania. Although it resemble an impact crater, the Richat Structure formed when a volcanic dome hardened and gradually eroded, exposing the onion - like layers of rock. Image taken from the international space station (ISS) in 2002

PIX4659122

Cratere Manicouagan - Quebec - March 2001 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station in March 2001. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 200

Cratere Manicouagan - Quebec - March 2001 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station in March 2001. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 200

PIX4630731

Starfield in Sagittarius/Swarms of Young and Older Stars Yield Clues to our Galaxy's Formation: Stars in Sagittarius seen by the Hubble space telescope. Aging red giant stars coexist with their more plentiful younger cousins, the smaller, white, Sun-like stars, in this crowded region of our galaxy's ancient central hub, or bulge. Most of the bright blue stars in the image are probably recently formed stars located in the foreground, in the galaxy's disk. The image is a composite of exposures taken in near-infrared and visible light with Hubble's Wide Field Camera 3

Starfield in Sagittarius/Swarms of Young and Older Stars Yield Clues to our Galaxy's Formation: Stars in Sagittarius seen by the Hubble space telescope. Aging red giant stars coexist with their more plentiful younger cousins, the smaller, white, Sun-like stars, in this crowded region of our galaxy's ancient central hub, or bulge. Most of the bright blue stars in the image are probably recently formed stars located in the foreground, in the galaxy's disk. The image is a composite of exposures taken in near-infrared and visible light with Hubble's Wide Field Camera 3

PIX4607530

Tue 03, 1954 - Training for the Indo-China war.: The last erre commando group of about a hundred men-divided into small groups of 4 or 5 are being specially trained to take over the grounds and villages soon after the withdrawal of the Viet Minh rebels. they are recruited from the former Viet Minh prisoners. soon after taking over the ground from the rebels each part of the village or battlefield is carefully searched for hidden enemy or war material left behind.

Tue 03, 1954 - Training for the Indo-China war.: The last erre commando group of about a hundred men-divided into small groups of 4 or 5 are being specially trained to take over the grounds and villages soon after the withdrawal of the Viet Minh rebels. they are recruited from the former Viet Minh prisoners. soon after taking over the ground from the rebels each part of the village or battlefield is carefully searched for hidden enemy or war material left behind.

ZUM4921265

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

PIX4645724

Mars: Martian face in the region of Cydonia - Mars: cydonia face - Image obtained on 25 July 1976 by the probe Viking 1 at 1873 km from Mars. The picture shows eroded mesa - like landforms. The huge rock formation in the center, which resemble a human head, is formed by shadows giving the illusion of eyes, nose and mouth. The feature is 1.5 kilometers (one mile) across, with the sun angle at approximately 20 degrees. The speckled appearance of the image is due to bit errors, emphasized by enlargement of the photo. The picture was taken by Viking 1 orbiter on July 25 from a range of 1873 kilometers (1162 miles)

Mars: Martian face in the region of Cydonia - Mars: cydonia face - Image obtained on 25 July 1976 by the probe Viking 1 at 1873 km from Mars. The picture shows eroded mesa - like landforms. The huge rock formation in the center, which resemble a human head, is formed by shadows giving the illusion of eyes, nose and mouth. The feature is 1.5 kilometers (one mile) across, with the sun angle at approximately 20 degrees. The speckled appearance of the image is due to bit errors, emphasized by enlargement of the photo. The picture was taken by Viking 1 orbiter on July 25 from a range of 1873 kilometers (1162 miles)

PIX4615174

The Moscow Literary Sreda - Members of Sreda literary circle, formed in the second half of the 1890s by Russian realistic writers - Portraits of Russian intellectuals of the literary group Znanie: from left to right, Andrei Skitalets (Stephan Gabrilovich Petrov), Leonid Nikolaievich Andreiev, Maxim Gorky (Gorki) (1868-1936), Nikolai Teleshev, singer Fiodor (Fedor, Feodor) Ivanovich Shaliapin (1873-1938), Ivan Bunin (Bunin) (1870-1953) and Evgeny Nikola Debut of the 20th century - Members of Sreda. Sreda (Wednesday) was a Moscow literary group founded by Russian author Nikolai Teleshov in 1899. Pictured are (left to right); Stepan Skitalets, Leonid Andreyev, Maxim Gorky, Teleshov, Feodor Chaliapin, Ivan Bunin; Evgeny Chirikov.

The Moscow Literary Sreda - Members of Sreda literary circle, formed in the second half of the 1890s by Russian realistic writers - Portraits of Russian intellectuals of the literary group Znanie: from left to right, Andrei Skitalets (Stephan Gabrilovich Petrov), Leonid Nikolaievich Andreiev, Maxim Gorky (Gorki) (1868-1936), Nikolai Teleshev, singer Fiodor (Fedor, Feodor) Ivanovich Shaliapin (1873-1938), Ivan Bunin (Bunin) (1870-1953) and Evgeny Nikola Debut of the 20th century - Members of Sreda. Sreda (Wednesday) was a Moscow literary group founded by Russian author Nikolai Teleshov in 1899. Pictured are (left to right); Stepan Skitalets, Leonid Andreyev, Maxim Gorky, Teleshov, Feodor Chaliapin, Ivan Bunin; Evgeny Chirikov.

Stefano Bianchetti

XEE4155669

Hurricane Fefa seen by shuttle Atlantis 08/1991 - Hurricane Fefa seen from space 08/1991 - Hurricane Fefa seen over the Pacific by shuttle Atlantis beginning August 1991. This oblique view of Hurricane Fefa shows the full extent of this storm with a cloud gyre several hundred miles in diameter and an elevated segment around the eye. The elevated segment bordering the eye indicates a tightly formed gyre with high internal wind speeds. At the time of this exposure, Fefa was located between the California coast and Hawaii. Fefa eventually dissipated at sea, failing to make landfall and thus did no property damage

Hurricane Fefa seen by shuttle Atlantis 08/1991 - Hurricane Fefa seen from space 08/1991 - Hurricane Fefa seen over the Pacific by shuttle Atlantis beginning August 1991. This oblique view of Hurricane Fefa shows the full extent of this storm with a cloud gyre several hundred miles in diameter and an elevated segment around the eye. The elevated segment bordering the eye indicates a tightly formed gyre with high internal wind speeds. At the time of this exposure, Fefa was located between the California coast and Hawaii. Fefa eventually dissipated at sea, failing to make landfall and thus did no property damage

PIX4673782

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Hot, massive stars which recently formed in M33 give the galaxy its bluish color. The reddish areas are nebulae in the galaxy in which stars are rapidly forming

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Hot, massive stars which recently formed in M33 give the galaxy its bluish color. The reddish areas are nebulae in the galaxy in which stars are rapidly forming

Stephane Guisard

PIX4609326

Cratere Manicouagan - Quebec - March 2008 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) in March 2008. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 2008

Cratere Manicouagan - Quebec - March 2008 - The Manicouagan Impact Crater reservoir in Quebec, Canada - Cratere d'impact Manicouagan, Quebec, seen from the International Space Station (ISS) in March 2008. This 100-kilometre crater formed 212 million years ago, following the fall of an asteroid on Earth. The reservoir, a large annular lake, marks the site of an impact crater 60 miles (100 kilometers) wide. Formed almost 212 million years ago when a large meteorite hit Earth, the crater has been worn down by many advances and retreats of glaciers and other processes of erosion. Seen here from the International Space Station (ISS) in March 2008

PIX4630749

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

James Webb Space Telescope (JWST) - Artist View - The James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

C. Carreau

PIX4645834

March: Iani Chaos - Mars: Iani Chaos - The region of Iani Chaos on Mars. Image obtained by the Mars Express probe. Iani Chaos on Mars, an area where Light Toned Deposits, or LTD, are known to be present. An analysis of data and images from Mars Express suggests that several LTD, some of the least understood structures on Mars, were formed when large amounts of groundwater burst on to the surface. Scientists propose that groundwater had a greater role in shaping the martian surface than previously believed, and may have sheltered primitive life forms as the planet started drying up. This image was obtained with the High Resolution Stereo Camera on board ESA's Mars Express spacecraft

March: Iani Chaos - Mars: Iani Chaos - The region of Iani Chaos on Mars. Image obtained by the Mars Express probe. Iani Chaos on Mars, an area where Light Toned Deposits, or LTD, are known to be present. An analysis of data and images from Mars Express suggests that several LTD, some of the least understood structures on Mars, were formed when large amounts of groundwater burst on to the surface. Scientists propose that groundwater had a greater role in shaping the martian surface than previously believed, and may have sheltered primitive life forms as the planet started drying up. This image was obtained with the High Resolution Stereo Camera on board ESA's Mars Express spacecraft

PIX4616054

Nebula of the cone NGC 2264 in the Unicorn - The Cone Nebula in Monoceros - Region H II located about 2600 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. The Cone nebula is part of an enormous cloud of hydrogen and tiny solid particles associated with the loose open cluster, NGC 2226 in the equatorial constellation of Monoceros. Within and around this cloud are many recently formed stars, some completely hidden within the dense interstellar matter. They can be detected by special infra - red techniques which are able to penetrate the obscuration. The largest of the dust clouds is the curious straight - sided feature which gives this object its name

Nebula of the cone NGC 2264 in the Unicorn - The Cone Nebula in Monoceros - Region H II located about 2600 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. The Cone nebula is part of an enormous cloud of hydrogen and tiny solid particles associated with the loose open cluster, NGC 2226 in the equatorial constellation of Monoceros. Within and around this cloud are many recently formed stars, some completely hidden within the dense interstellar matter. They can be detected by special infra - red techniques which are able to penetrate the obscuration. The largest of the dust clouds is the curious straight - sided feature which gives this object its name

PIX4618601

Nebula N11 in the Great Magellan Cloud - N11 star forming region in Large Magellanic Cloud (LMC) - N11 (Henize 11) is a vast star-forming region located in the Great Magellan Cloud galaxy. It is home to a cluster of hot young stars, NGC 1760. This glowing complex of rings, shells, and powerful young stars lies in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. The overall complex of glowing gas and stars is known as N11 while the central cluster of hot young blue stars is know as NGC 1760. The complex expanding shells of gas have likely formed from multiple generations of hot O and B type stars and their supernovae. N11 spans over 1000 light years across

Nebula N11 in the Great Magellan Cloud - N11 star forming region in Large Magellanic Cloud (LMC) - N11 (Henize 11) is a vast star-forming region located in the Great Magellan Cloud galaxy. It is home to a cluster of hot young stars, NGC 1760. This glowing complex of rings, shells, and powerful young stars lies in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. The overall complex of glowing gas and stars is known as N11 while the central cluster of hot young blue stars is know as NGC 1760. The complex expanding shells of gas have likely formed from multiple generations of hot O and B type stars and their supernovae. N11 spans over 1000 light years across

R. Gendler

PIX4620765

Mars - Atmosphere - View of Mars Planet with Argyre Basin, obtained by the Viking 1 probe in July 1976. Argyre measures 1300 km in diameter and is the second largest impact crater on Mars, after Hellas Planitia. The Argyre impact basin in the southern highlands of Mars. The basin, which is approximately 1,300 kilometers in diameter, was formed about 4 billion years ago during the Heavy Bombardment Period of the early Solar System when an asteroid or comet roughly 50 kilometers across impacted Mars. Argyre is believed to be the second - largest impact basin on Mars after Hellas Planitia and may be one of the best preserved ancient impact basins from the Heavy Bombardment Period

Mars - Atmosphere - View of Mars Planet with Argyre Basin, obtained by the Viking 1 probe in July 1976. Argyre measures 1300 km in diameter and is the second largest impact crater on Mars, after Hellas Planitia. The Argyre impact basin in the southern highlands of Mars. The basin, which is approximately 1,300 kilometers in diameter, was formed about 4 billion years ago during the Heavy Bombardment Period of the early Solar System when an asteroid or comet roughly 50 kilometers across impacted Mars. Argyre is believed to be the second - largest impact basin on Mars after Hellas Planitia and may be one of the best preserved ancient impact basins from the Heavy Bombardment Period

PIX4615099

Onekotan volcanic island seen from space - Onekotan volcanic island seen from space - Onekotan Island is an uninhabited volcanic island north of the Kuril Islands chain (Russia). About 40 kilometres long, this island is home to two stratovolcanoes, on the right (north), the Nemo volcano, on the left (south), the Krenitsyn volcano with the caldera Tao - Rusyr. Image obtained from the International Space Station (ISS) on January 9, 2011. Snow cover highlights the calderas and volcanic cones that form the northern and southern ends of Onekotan Island, part of the Russian Federation in the western Pacific Ocean. Calderas are depressions formed when a volcano empties its magma chamber in an explosive eruption and then the overlaying material collapses into the evacuated space. In this astronaut photograph taken from the International Space Station (ISS) on January 9, 2011, the northern end of the island (image right) is dominated by the Nemo Peak volcano, which began forming within an older

Onekotan volcanic island seen from space - Onekotan volcanic island seen from space - Onekotan Island is an uninhabited volcanic island north of the Kuril Islands chain (Russia). About 40 kilometres long, this island is home to two stratovolcanoes, on the right (north), the Nemo volcano, on the left (south), the Krenitsyn volcano with the caldera Tao - Rusyr. Image obtained from the International Space Station (ISS) on January 9, 2011. Snow cover highlights the calderas and volcanic cones that form the northern and southern ends of Onekotan Island, part of the Russian Federation in the western Pacific Ocean. Calderas are depressions formed when a volcano empties its magma chamber in an explosive eruption and then the overlaying material collapses into the evacuated space. In this astronaut photograph taken from the International Space Station (ISS) on January 9, 2011, the northern end of the island (image right) is dominated by the Nemo Peak volcano, which began forming within an older

PIX4661424

Impact on the Moon - Moon Little splat: 10 million years after the Moon's surface has cooled, an impact with another small body formed from the ring surrounding the Earth probably occurred. This could explain the two very different faces of today's Moon - 10 million years after Moon's cooling: Today's moon was not the only one formed from the ring. There were several others, orbiting at the Lagrange points. The orbit of one was not stable and it eventually drifted into the larger moon in a slow-motion impact that caused the smaller satellite to pancake, spreading itself over an entire hemisphere, creating the mismatched sides the moon has today. An unlucky witness to the “” little splat”” would have seen a tsunami of molten rock roaring up over the horizon

Impact on the Moon - Moon Little splat: 10 million years after the Moon's surface has cooled, an impact with another small body formed from the ring surrounding the Earth probably occurred. This could explain the two very different faces of today's Moon - 10 million years after Moon's cooling: Today's moon was not the only one formed from the ring. There were several others, orbiting at the Lagrange points. The orbit of one was not stable and it eventually drifted into the larger moon in a slow-motion impact that caused the smaller satellite to pancake, spreading itself over an entire hemisphere, creating the mismatched sides the moon has today. An unlucky witness to the “” little splat”” would have seen a tsunami of molten rock roaring up over the horizon

Miller, Ron (b.1947)

PIX4614827

White Sands Desert - New Mexico - White Sands desert - New Mexico - The White Sands desert in New Mexico seen by the EO satellite - 1 on June 27, 2009. The image covers the southeastern part of White Sands National Park. The Advanced Land Imager (ALI) onboard NASA's Earth Observing - 1 (EO-1) satellite captured this image of part of the White Sands National Monument on June 27, 2009. This image shows part of the southeastern portion of the park. The dunes shown in this image are advancing towards the northeast, and the brilliant white sands contrast with darker soils. The sands of White Sands National Monument are formed from gypsum, a soft mineral often left behind when water bodies evaporate

White Sands Desert - New Mexico - White Sands desert - New Mexico - The White Sands desert in New Mexico seen by the EO satellite - 1 on June 27, 2009. The image covers the southeastern part of White Sands National Park. The Advanced Land Imager (ALI) onboard NASA's Earth Observing - 1 (EO-1) satellite captured this image of part of the White Sands National Monument on June 27, 2009. This image shows part of the southeastern portion of the park. The dunes shown in this image are advancing towards the northeast, and the brilliant white sands contrast with darker soils. The sands of White Sands National Monument are formed from gypsum, a soft mineral often left behind when water bodies evaporate

PIX4673346

Sep. 09, 1953 - Egyptian Ex-Premier on Trial in Cairo.. Abdel Hadi accused of Treason: Ibrahim Abdel Hadi, leader of the dissolved Saadist Party appeared before the special Revolutionary Tribunal in Cairo. The first charge of the indictment accuses him “of getting in touch with foreign circles with the object of damaging the present regime and harming the highest interests of the country”. The Tribunal is formed of three members of Gen. Neg ~ ib's military junta all were obscure junior officers in the Egyptian Army when Abdel Hadi was head of the government

Sep. 09, 1953 - Egyptian Ex-Premier on Trial in Cairo.. Abdel Hadi accused of Treason: Ibrahim Abdel Hadi, leader of the dissolved Saadist Party appeared before the special Revolutionary Tribunal in Cairo. The first charge of the indictment accuses him “of getting in touch with foreign circles with the object of damaging the present regime and harming the highest interests of the country”. The Tribunal is formed of three members of Gen. Neg ~ ib's military junta all were obscure junior officers in the Egyptian Army when Abdel Hadi was head of the government

ZUM4879016

Oct. 05, 1954 - Sir Winston Churchill Receives Member of The Ancient and honorable artillery company of Boston. This afternoon Sir Winston Churchill received a deputation from the Ancient and Honourable Artillery company of Boston, Massachusetts, who are now a visit to London, at No. 10, Downing -street today. Their founder, Robert Keayne, was a member of the Hac before he emigrated to America and formed the Boston company in 1637. The prime minister was presented with a suitable engraved, by Photo shows Sir Winston Churchill seen receiving the cigar box from Captain Thomas J. Carty, on the left is Lieut. Mark Bortman, and on right F ~ ed E.Pereira

Oct. 05, 1954 - Sir Winston Churchill Receives Member of The Ancient and honorable artillery company of Boston. This afternoon Sir Winston Churchill received a deputation from the Ancient and Honourable Artillery company of Boston, Massachusetts, who are now a visit to London, at No. 10, Downing -street today. Their founder, Robert Keayne, was a member of the Hac before he emigrated to America and formed the Boston company in 1637. The prime minister was presented with a suitable engraved, by Photo shows Sir Winston Churchill seen receiving the cigar box from Captain Thomas J. Carty, on the left is Lieut. Mark Bortman, and on right F ~ ed E.Pereira

ZUM4942242

Jan. 01, 1954 - Audrey Meets Ramon - After Twenty Eight Years... Star of the Silent Screen - in London... Miss Audrey Roman - first member of the 'Ramon Navarro' fan club - formed in 1922 - achieved a cherished ambition last evening when she met her idol - screen star of the silent days Ramon Navarro - who arrived in London a few days ago. While fans - pressmen - etc... tried to get interviews with the ex screen star at the Savoy Hotel - he was dining with Miss Roman at her home in Stoke Newington... Keystone Photo Shows: Ramon Navarro and Audrey Roman seen as they dined at the latter's Stoke Newington, London home last evening

Jan. 01, 1954 - Audrey Meets Ramon - After Twenty Eight Years... Star of the Silent Screen - in London... Miss Audrey Roman - first member of the 'Ramon Navarro' fan club - formed in 1922 - achieved a cherished ambition last evening when she met her idol - screen star of the silent days Ramon Navarro - who arrived in London a few days ago. While fans - pressmen - etc... tried to get interviews with the ex screen star at the Savoy Hotel - he was dining with Miss Roman at her home in Stoke Newington... Keystone Photo Shows: Ramon Navarro and Audrey Roman seen as they dined at the latter's Stoke Newington, London home last evening

ZUM4904048

Spiral galaxy M81 seen by the Hubble space telescope - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions, while its core is surrounded by much older yellow stars and a black hole. Image obtained by the Hubble space telescope with the ACS camera in 2006. Although the M81 galaxy is 11.6 million light - years away, this image taken by the Hubble space telescope is so sharp that it can resolve individual stars, along with open star clusters, globular star clusters, and even glowing regions of fluorescent gas. The spiral arms, which wind all the way down into the nucleus, are made up of young, bluish, hot stars formed in the past few million years. They also host a population of stars formed in an episode of star formation that started about 600 million years ago. The greenish regions are dense areas of bright star formation. The ultraviolet light from hot young stars are fluorescing the surr

Spiral galaxy M81 seen by the Hubble space telescope - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions, while its core is surrounded by much older yellow stars and a black hole. Image obtained by the Hubble space telescope with the ACS camera in 2006. Although the M81 galaxy is 11.6 million light - years away, this image taken by the Hubble space telescope is so sharp that it can resolve individual stars, along with open star clusters, globular star clusters, and even glowing regions of fluorescent gas. The spiral arms, which wind all the way down into the nucleus, are made up of young, bluish, hot stars formed in the past few million years. They also host a population of stars formed in an episode of star formation that started about 600 million years ago. The greenish regions are dense areas of bright star formation. The ultraviolet light from hot young stars are fluorescing the surr

PIX4610340

Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

Christchurch and the Peninsula of Banks (New Zealand) from space - Christchurch and Banks Peninsula, New Zealand - The Peninsula of Banks and the City of Christchurch seen from the International Space Station (ISS) on August 15, 2006. The Banks Peninsula is an ancient erode volcano forming a peninsula on the east coast of the South Island. Oblique view (the photograph was taken from a side angle) of the city of Christchurch, New Zealand. Snow highlights the peaks of the Banks Peninsula to the southeast of the city. The peninsula has a radically different landscape compared to the adjoining, flat Canterbury Plains, where Christchurch (gray patch to the north) is located. The Banks Peninsula is formed from the overlapping cones of the extinct Lyttelton and Akaroa volcanoes. Subsequent erosion of the cones formed the heavily dissected terrain visible in the image, and sea level rise led to the creation of several harbors around the Peninsula. Erosion continues unabated today, as evidenced

PIX4675641

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

R. Gendler

PIX4618379

Cocoon Nebula (IC 5146) in the Swan - Cocoon Nebula (IC 5146) in Cygnus - The Cocon Nebula, IC 5146, is an emission nebula located about 4000 years from Earth in the constellation of Swan. This star-forming region is illuminated by massive young stars. This complex mass of molecular hydrogen and dust, located 4,000 light years from earth, glows red by emitting light, shines blue by reflecting light and exhibits a pattern of dark lanes that result when dust absorbs light. Much of the light seen in the main part of this nebula is generated by the massive bright star near it's center. The Cocoon is a stellar nursery containing a relatively young open cluster of stars with several individual constituents that are newly formed

Cocoon Nebula (IC 5146) in the Swan - Cocoon Nebula (IC 5146) in Cygnus - The Cocon Nebula, IC 5146, is an emission nebula located about 4000 years from Earth in the constellation of Swan. This star-forming region is illuminated by massive young stars. This complex mass of molecular hydrogen and dust, located 4,000 light years from earth, glows red by emitting light, shines blue by reflecting light and exhibits a pattern of dark lanes that result when dust absorbs light. Much of the light seen in the main part of this nebula is generated by the massive bright star near it's center. The Cocoon is a stellar nursery containing a relatively young open cluster of stars with several individual constituents that are newly formed

Adam Block

PIX4622748

Cocon Nebula (IC 5146) in the Swan - Cocoon Nebula IC5146 - The Cocon Nebula, IC 5146, is an emission nebula located about 4000 years from Earth in the constellation of Swan. This star-forming region is illuminated by massive young stars. This complex mass of molecular hydrogen and dust, located 4,000 light years from earth, glows red by emitting light, shines blue by reflecting light and exhibits a pattern of dark lanes that result when dust absorbs light. Much of the light seen in the main part of this nebula is generated by the massive bright star near it's center. The Cocoon is a stellar nursery containing a relatively young open cluster of stars with several individual constituents that are newly formed

Cocon Nebula (IC 5146) in the Swan - Cocoon Nebula IC5146 - The Cocon Nebula, IC 5146, is an emission nebula located about 4000 years from Earth in the constellation of Swan. This star-forming region is illuminated by massive young stars. This complex mass of molecular hydrogen and dust, located 4,000 light years from earth, glows red by emitting light, shines blue by reflecting light and exhibits a pattern of dark lanes that result when dust absorbs light. Much of the light seen in the main part of this nebula is generated by the massive bright star near it's center. The Cocoon is a stellar nursery containing a relatively young open cluster of stars with several individual constituents that are newly formed

PIX4622764

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

R. Gendler

PIX4618356

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Through an extraordinary chance alignment, a face - on spiral galaxy lies precisely in front of another larger spiral. This line - up provides us with the rare chance to visualize dark material within the front galaxy, seen only because it is silhouetted against the object behind it. NGC 3314 lies about 140 million light - years from Earth, in the direction of the southern hemisphere constellation Hydra. The bright blue stars forming a pinwheel shape near the center of the front galaxy have formed recently from interstellar gas and dust. In many galaxies, interstellar dust lies only in the same regions as recently formed blue stars. However, in the foreground galaxy, NGC 3314a, there are numerous additional dark dust lanes that are

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Through an extraordinary chance alignment, a face - on spiral galaxy lies precisely in front of another larger spiral. This line - up provides us with the rare chance to visualize dark material within the front galaxy, seen only because it is silhouetted against the object behind it. NGC 3314 lies about 140 million light - years from Earth, in the direction of the southern hemisphere constellation Hydra. The bright blue stars forming a pinwheel shape near the center of the front galaxy have formed recently from interstellar gas and dust. In many galaxies, interstellar dust lies only in the same regions as recently formed blue stars. However, in the foreground galaxy, NGC 3314a, there are numerous additional dark dust lanes that are

PIX4610557

Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila

Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila

PIX4594003

Cocoon Nebula (IC 5146) in Swan - Cocoon Nebula - IC 5146 - in Cygnus - The Cocon Nebula, IC 5146, is an emission nebula located about 4000 years from Earth in the constellation of Swan. This complex mass of molecular hydrogen and dust, located 4,000 light years from earth, glows red by emitting light, shines blue by reflecting light and exhibits a pattern of dark lanes that result when dust absorbs light. Much of the light seen in the main part of this nebula is generated by the massive bright star near it's center. The Cocoon is a stellar nursery containing a relatively young open cluster of stars with several individual constituents that are newly formed. Wide angle, long exposure photographs reveals the nebula to be very extensive - essentially a vast river of interstellar dust

Cocoon Nebula (IC 5146) in Swan - Cocoon Nebula - IC 5146 - in Cygnus - The Cocon Nebula, IC 5146, is an emission nebula located about 4000 years from Earth in the constellation of Swan. This complex mass of molecular hydrogen and dust, located 4,000 light years from earth, glows red by emitting light, shines blue by reflecting light and exhibits a pattern of dark lanes that result when dust absorbs light. Much of the light seen in the main part of this nebula is generated by the massive bright star near it's center. The Cocoon is a stellar nursery containing a relatively young open cluster of stars with several individual constituents that are newly formed. Wide angle, long exposure photographs reveals the nebula to be very extensive - essentially a vast river of interstellar dust

R. Gendler

PIX4622743

Akimiski Island, Canada, seen by Landsat - 7 - Akimiski Island, Canada, seen by satellite - Akimiski Island is a 3000 km island of James Bay, Canada. Uninhabited, it belongs to the territory of Nunavut. Image obtained by Landsat-7 satellite on 9 August 2000. Scraped clean and weighted down for thousands of years by Pleistocene ice sheets, Akimiski Island in James Bay provides a case study of how Earth's land surfaces evolve following glaciation. During the last ice age, this small island was buried under several thousand meters ice, but since its retreat, the island has rebounded (risen in elevation) and new beach areas have emerged, streams and lakes have formed, and trees and other vegetation have colonized the new territory. This image of Akimiski Island was captured by the Landsat 7 satellite on August 9, 2000

Akimiski Island, Canada, seen by Landsat - 7 - Akimiski Island, Canada, seen by satellite - Akimiski Island is a 3000 km island of James Bay, Canada. Uninhabited, it belongs to the territory of Nunavut. Image obtained by Landsat-7 satellite on 9 August 2000. Scraped clean and weighted down for thousands of years by Pleistocene ice sheets, Akimiski Island in James Bay provides a case study of how Earth's land surfaces evolve following glaciation. During the last ice age, this small island was buried under several thousand meters ice, but since its retreat, the island has rebounded (risen in elevation) and new beach areas have emerged, streams and lakes have formed, and trees and other vegetation have colonized the new territory. This image of Akimiski Island was captured by the Landsat 7 satellite on August 9, 2000

PIX4672935

Feb. 22, 1954 - Socialites at party? A group of? Social? this afternoon attended a party at the Caf? of Paris, sponsored by the British Travel Association. The party formed part of a film which is being made for the British Travel Association, to be called? Where Do We Go From Here? It will show London? s? gaiety and night life? to foreigners. Keystone Photo Shows: A general view at the party this afternoon as the scene is photographed. The film camera in centre moves in for a close-up of a table at which are seated, from left: Loella, Duchess of Westminster; Mr. Peter Coats; Mrs. Gerald Legge; Lady Rendlesham; Hon. John Sideley and Mrs. John Ward. H/Keystone

Feb. 22, 1954 - Socialites at party? A group of? Social? this afternoon attended a party at the Caf? of Paris, sponsored by the British Travel Association. The party formed part of a film which is being made for the British Travel Association, to be called? Where Do We Go From Here? It will show London? s? gaiety and night life? to foreigners. Keystone Photo Shows: A general view at the party this afternoon as the scene is photographed. The film camera in centre moves in for a close-up of a table at which are seated, from left: Loella, Duchess of Westminster; Mr. Peter Coats; Mrs. Gerald Legge; Lady Rendlesham; Hon. John Sideley and Mrs. John Ward. H/Keystone

ZUM4916070

Ho Chi Minh in France, c. 1920 (b/w photo)

Ho Chi Minh in France, c. 1920 (b/w photo)

PFH1773970

Tarantula nebula before the appearance of supernova 1987A - The Tarantula Nebula, before supernova SN1987A - Tarantula Nebula photographed in 1984. Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. By great good fortune, the star (Sanduleak - 69* 202) which exploded as the supernova, had been observed some years previously and was found to be a typical young, bluish star, much hotter and brighter than stars like the Sun. There are many similar stars in this part of the LMC which is dominated by the spectacular red cloud of the Tarantula Nebula. It in such nebulae that stars are formed, often in compact groups such as those scattered across this photograph, which was taken in 1984

Tarantula nebula before the appearance of supernova 1987A - The Tarantula Nebula, before supernova SN1987A - Tarantula Nebula photographed in 1984. Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. By great good fortune, the star (Sanduleak - 69* 202) which exploded as the supernova, had been observed some years previously and was found to be a typical young, bluish star, much hotter and brighter than stars like the Sun. There are many similar stars in this part of the LMC which is dominated by the spectacular red cloud of the Tarantula Nebula. It in such nebulae that stars are formed, often in compact groups such as those scattered across this photograph, which was taken in 1984

PIX4582367

Mars surface seen by the rover Curiosity 03/2014: The formation “” Kimberley “” seen by Curiosity on March 25, 2014. The strata indicate a flow of water towards Mount Sharp (in the background). A view from the “” Kimberley”” formation on Mars taken by Nasa's Curiosity rover. The strata in the foreground dip towards the base of Mount Sharp, indicating flow of water toward a basin that existed before the larger bulk of the mountain formed. The colors are adjusted so that rocks look approximately as they would if they were on Earth, to help geologists interpret the rocks. This “” white balancing”” to adjust for the lighting on Mars overly compensates for the absence of blue on Mars, making the sky appear light blue and sometimes giving dark, black rocks a blue cast.

Mars surface seen by the rover Curiosity 03/2014: The formation “” Kimberley “” seen by Curiosity on March 25, 2014. The strata indicate a flow of water towards Mount Sharp (in the background). A view from the “” Kimberley”” formation on Mars taken by Nasa's Curiosity rover. The strata in the foreground dip towards the base of Mount Sharp, indicating flow of water toward a basin that existed before the larger bulk of the mountain formed. The colors are adjusted so that rocks look approximately as they would if they were on Earth, to help geologists interpret the rocks. This “” white balancing”” to adjust for the lighting on Mars overly compensates for the absence of blue on Mars, making the sky appear light blue and sometimes giving dark, black rocks a blue cast.

PIX4616687

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Adam Block

PIX4618377

Jupiter seen from his satellite Ganymede - Illustration - Ridges, grooves, and craters on Ganymede - Artist's view of the surface of Ganymede, Jupiter's largest satellite. An impact crater about 15 km in diameter differs from the striated surface of the satellite. In the sky are represented Jupiter, the Europe satellite on the top right, and Io on the left of Jupiter. Jupiter's largest satellite Ganymede has a varying surface, some of which is characterized by rumpled bundles of ridges and grooves that run for hundreds of miles over a frozen surface of water - ice. They probably formed long ago when tectonic forces pulled apart Ganymede's upper crust; similar sets of faults occur in rift zones on Earth, as in eastern Africa. Subsequent meteoritic impacts have peppered - - and broken in places - - the continuity of the running formations. In this image an impact crater about 10 miles in diameter dominates a scene otherwise defined by a dozen long ridges. In the middle of the crater is a

Jupiter seen from his satellite Ganymede - Illustration - Ridges, grooves, and craters on Ganymede - Artist's view of the surface of Ganymede, Jupiter's largest satellite. An impact crater about 15 km in diameter differs from the striated surface of the satellite. In the sky are represented Jupiter, the Europe satellite on the top right, and Io on the left of Jupiter. Jupiter's largest satellite Ganymede has a varying surface, some of which is characterized by rumpled bundles of ridges and grooves that run for hundreds of miles over a frozen surface of water - ice. They probably formed long ago when tectonic forces pulled apart Ganymede's upper crust; similar sets of faults occur in rift zones on Earth, as in eastern Africa. Subsequent meteoritic impacts have peppered - - and broken in places - - the continuity of the running formations. In this image an impact crater about 10 miles in diameter dominates a scene otherwise defined by a dozen long ridges. In the middle of the crater is a

Walter B Myers

PIX4575196

Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila

Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila

PIX4594009

Open cluster NGC 4755 - Jewel box - The Jewel Box cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 7800 years - light from Earth. The bright orange star is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 14 million years ago. NGC4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster

Open cluster NGC 4755 - Jewel box - The Jewel Box cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 7800 years - light from Earth. The bright orange star is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 14 million years ago. NGC4755 (Caldwell 94) is called the Jewel Box, based on John Herschel's comment in the 1830's that it looked like a superb piece of jewelry. There are about 50 stars in this cluster which formed some 14 million years ago. Most of the cluster members are blue giants which in a few million years will exhaust their hydrogen fuel and become red giants on their way to a cataclysmic end as supernovae. One red giant can already be seen at the center of the cluster

R. Gendler

PIX4568254

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained with a 90 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained with a 90 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

PIX4623489

Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years

Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years

PIX4618685

Dunes near the north pole on Mars - Dunes at North Polar Cap on Mars: Image obtained on March 26, 2014 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. Formative down-slope winds descending on Mars' North Polar ice cap likely play an important role in transporting sediment from the base of the ice cap into the dune fields that sit beyond the ice cap. The deep chasm that formed on the polar cap edge is identified as an area of strong down-slope winds and has a clear connection to Mars' largest dune field, Olympia Undae. Repeat HiRise images from this chasm that specifically targets the dunes, provides the basis to evaluate the sand fluxes which are associated with the dune and ripple movement in this area

Dunes near the north pole on Mars - Dunes at North Polar Cap on Mars: Image obtained on March 26, 2014 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. Formative down-slope winds descending on Mars' North Polar ice cap likely play an important role in transporting sediment from the base of the ice cap into the dune fields that sit beyond the ice cap. The deep chasm that formed on the polar cap edge is identified as an area of strong down-slope winds and has a clear connection to Mars' largest dune field, Olympia Undae. Repeat HiRise images from this chasm that specifically targets the dunes, provides the basis to evaluate the sand fluxes which are associated with the dune and ripple movement in this area

PIX4580075

Glacier Viedma, Argentina - Viedma Glacier in Argentina - The Viedma Glacier in Argentina, observed from the International Space Station on January 10, 2004. This detailed view was taken with an 800 mm lens from the International Space Station on 10 January, 2004. The image shows the lower end of the Viedma Glacier that flows into Lake Viedma, one of three major glacially formed lakes on the Patagonian side of the southern Andean ice sheet, at 50 degrees South. The image reveals the slender dark lines of rock material (moraine) which is carried in the slowly flowing ice. Lighter lines at right angles are patterns of crevasse. The glacier diverges into two lakes where calved icebergs can be seen floating in the lakes. The glacier here is about 1.8 km wide

Glacier Viedma, Argentina - Viedma Glacier in Argentina - The Viedma Glacier in Argentina, observed from the International Space Station on January 10, 2004. This detailed view was taken with an 800 mm lens from the International Space Station on 10 January, 2004. The image shows the lower end of the Viedma Glacier that flows into Lake Viedma, one of three major glacially formed lakes on the Patagonian side of the southern Andean ice sheet, at 50 degrees South. The image reveals the slender dark lines of rock material (moraine) which is carried in the slowly flowing ice. Lighter lines at right angles are patterns of crevasse. The glacier diverges into two lakes where calved icebergs can be seen floating in the lakes. The glacier here is about 1.8 km wide

PIX4675760

Nebula RCW38 in the constellation of sails seen in infrared by the VLT - Three - colour composite image of RCW38, obtained through three near - infrared filters. This is a region in the Milky Way at a distance of about 5,000 light years, where stars which have recently formed in clouds of gas and dust are still heavily obscured and cannot be observed in the visible part of the spectrum. Contrarily, as this image shows, they are very well seen at infrared wavelengths where the obscuration is substantially lower. The diffuse radiation is a mixture of starlight scattered by the dust and gas in the area, and atomic and molecular hydrogen line emission. RCW 38 is at a distance of ~ 1.7 kpc (~ 5500 light years) from us, near the famous Vela supernova remnant and the Gum nebul

Nebula RCW38 in the constellation of sails seen in infrared by the VLT - Three - colour composite image of RCW38, obtained through three near - infrared filters. This is a region in the Milky Way at a distance of about 5,000 light years, where stars which have recently formed in clouds of gas and dust are still heavily obscured and cannot be observed in the visible part of the spectrum. Contrarily, as this image shows, they are very well seen at infrared wavelengths where the obscuration is substantially lower. The diffuse radiation is a mixture of starlight scattered by the dust and gas in the area, and atomic and molecular hydrogen line emission. RCW 38 is at a distance of ~ 1.7 kpc (~ 5500 light years) from us, near the famous Vela supernova remnant and the Gum nebul

PIX4621658

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained with a 50 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC 6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained with a 50 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC 6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

R. Jay GaBany

PIX4623523

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained with a 90 cm telescope, and the Hubble and Subaru telescopes. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. Image Composite

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained with a 90 cm telescope, and the Hubble and Subaru telescopes. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. Image Composite

PIX4623530

Volcano Llullaillaco - Volcano Llullaillaco - Llullaillaco or Llullay - Yacu is an active stratovolcano located in the Andes on the border between Argentina and Chile. This image obtained from the International Space Station on 9 December 2009 shows a vast flow of lava that extends from the volcanic cone. The summit of South America's Llullaillaco Volcano has an elevation of 6,739 meters (22,110 feet) above sea level, making it the highest historically active volcano in the world. The current stratovolcano - - a cone - shaped volcano built from successive layers of thick lava flows and eruption products like ash and rock fragments - - is built on top of an older stratovolcano. This detailed astronaut photograph of Llullaillaco illustrates an interesting volcanic feature known as a coulee (image top right). Coulees are formed from highly viscous, thick lavas that flow onto a steep surface. Image taken on December 9, 2009 from the International space station (ISS)

Volcano Llullaillaco - Volcano Llullaillaco - Llullaillaco or Llullay - Yacu is an active stratovolcano located in the Andes on the border between Argentina and Chile. This image obtained from the International Space Station on 9 December 2009 shows a vast flow of lava that extends from the volcanic cone. The summit of South America's Llullaillaco Volcano has an elevation of 6,739 meters (22,110 feet) above sea level, making it the highest historically active volcano in the world. The current stratovolcano - - a cone - shaped volcano built from successive layers of thick lava flows and eruption products like ash and rock fragments - - is built on top of an older stratovolcano. This detailed astronaut photograph of Llullaillaco illustrates an interesting volcanic feature known as a coulee (image top right). Coulees are formed from highly viscous, thick lavas that flow onto a steep surface. Image taken on December 9, 2009 from the International space station (ISS)

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Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away

R. Jay GaBany

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La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne, crossing the Milky Way. Brittany, 27 September 2008

La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne, crossing the Milky Way. Brittany, 27 September 2008

Laurent Laveder

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Spiral Galaxy NGC 4522 - Galaxy Spiral NGC 4522 - Moving at a speed of 10 million km/h in the Virgin's galaxy cluster, this spiral galaxy loses some of its gas. NGC 4522 is located about 60 million light years away from Earth. Image obtained by the Hubble Space Telescope. NGC 4522 is a spectacular example of a spiral galaxy that is currently being stripped of its gas content. The galaxy is part of the Virgo galaxy cluster and its rapid motion within the cluster results in strong winds across the galaxy as the gas within is left behind. Scientists estimate that the galaxy is moving at more than 10 million kilometers per hour. A number of newly formed star clusters that developed in the stripped gas can be seen in the Hubble image. The stripped spiral galaxy is located some 60 million light - years away from Earth

Spiral Galaxy NGC 4522 - Galaxy Spiral NGC 4522 - Moving at a speed of 10 million km/h in the Virgin's galaxy cluster, this spiral galaxy loses some of its gas. NGC 4522 is located about 60 million light years away from Earth. Image obtained by the Hubble Space Telescope. NGC 4522 is a spectacular example of a spiral galaxy that is currently being stripped of its gas content. The galaxy is part of the Virgo galaxy cluster and its rapid motion within the cluster results in strong winds across the galaxy as the gas within is left behind. Scientists estimate that the galaxy is moving at more than 10 million kilometers per hour. A number of newly formed star clusters that developed in the stripped gas can be seen in the Hubble image. The stripped spiral galaxy is located some 60 million light - years away from Earth

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Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red the star-forming regions appear. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. The data in this image show the many stars within the galaxy as well as reddish star forming regions that are filled with hot hydrogen gas. Hot, massive stars which recently formed in M33 give the galaxy its bluish color. The reddish areas are nebulae in the galaxy in which stars are rapidly forming

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red the star-forming regions appear. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. The data in this image show the many stars within the galaxy as well as reddish star forming regions that are filled with hot hydrogen gas. Hot, massive stars which recently formed in M33 give the galaxy its bluish color. The reddish areas are nebulae in the galaxy in which stars are rapidly forming

R. Gendler

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Mercury by Messenger. 14/01/2008 - Mercury by Messenger - Jan 14 2008 - Image of the surface of Mercury obtained at a distance of 11,588 km by the Messenger probe on January 14, 2008. The large impact crater at the bottom left of the image is about 230 km in diameter. This image of Mercury's surface was acquired during Messenger's first flyby of the planet on January 14, 2008 when the spacecraft was 11,588 km (7,200 miles) from Mercury's surface. This scene shows at least five different events in Mercury's surface history. The large crater to the lower left of the image measures ~ 230 km (143 miles) in diameter and has a prominent crater, about 85 km (53 miles) across, nestled inside it, south of its center. Both of these craters were subsequently filled with a material that appears to have been emplaced in a relatively fluid form, as evidenced by the fact that the material “” embays”” or onlaps the ejecta blanket surrounding the rim of the smaller crater. The larger crater is filled a

Mercury by Messenger. 14/01/2008 - Mercury by Messenger - Jan 14 2008 - Image of the surface of Mercury obtained at a distance of 11,588 km by the Messenger probe on January 14, 2008. The large impact crater at the bottom left of the image is about 230 km in diameter. This image of Mercury's surface was acquired during Messenger's first flyby of the planet on January 14, 2008 when the spacecraft was 11,588 km (7,200 miles) from Mercury's surface. This scene shows at least five different events in Mercury's surface history. The large crater to the lower left of the image measures ~ 230 km (143 miles) in diameter and has a prominent crater, about 85 km (53 miles) across, nestled inside it, south of its center. Both of these craters were subsequently filled with a material that appears to have been emplaced in a relatively fluid form, as evidenced by the fact that the material “” embays”” or onlaps the ejecta blanket surrounding the rim of the smaller crater. The larger crater is filled a

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