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Images of 'Clouds Of Dust' found, 321

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Rape of Proserpine (marble)

Rape of Proserpine (marble)

Bernini, Gian Lorenzo (1598-1680)

FAF283558

A Deluge, c.1517-18 (black chalk on paper)

A Deluge, c.1517-18 (black chalk on paper)

Vinci, Leonardo da (1452-1519)

ROC2628782

Battle of Vicksburg, Mississippi, 19th May, 1863 (colour litho)

Battle of Vicksburg, Mississippi, 19th May, 1863 (colour litho)

McBarron, H. Charles Jr. (1902-92) (after)

PNP269296

Storming of Delhi 1857, from 'The Campaign in India 1857-58 from drawings made during the eventful period of the Great Mutiny, illustrating the military operations before Delhi and its neighbourhood', engraved by George McCulloch, published by Day & Son, c.1857 (colour litho)

Storming of Delhi 1857, from 'The Campaign in India 1857-58 from drawings made during the eventful period of the Great Mutiny, illustrating the military operations before Delhi and its neighbourhood', engraved by George McCulloch, published by Day & Son, c.1857 (colour litho)

Atkinson, George Francklin (1822-59) (after)

NAM261136

American Stuart tank, North Africa, 1942 (b/w photo)

American Stuart tank, North Africa, 1942 (b/w photo)

American Photographer, (20th century)

PNP394790

The Abduction of Proserpina, from 'The Children's Hour: Stories from the Classics', published by the Waverley Book Company (colour litho)

The Abduction of Proserpina, from 'The Children's Hour: Stories from the Classics', published by the Waverley Book Company (colour litho)

Brock, Charles Edmund (1870-1938)

IL262821

Dust Storm on Mars (sillustration)

Dust Storm on Mars (sillustration)

Miller, Ron (b.1947)

PIX4617018

Grand Canyon, 1927 (w/c on paper)

Grand Canyon, 1927 (w/c on paper)

Widforss, Gunnar (1879-1934)

CH429878

A deluge, c.1517-18, (chalk on paper)

A deluge, c.1517-18, (chalk on paper)

Vinci, Leonardo da (1452-1519)

ROC5617343

Gripped in the claw of the constellation Scorpius sits the reflection nebula DG 129, a cloud of gas and dust that reflects light from nearby, bright stars. WISE.

Gripped in the claw of the constellation Scorpius sits the reflection nebula DG 129, a cloud of gas and dust that reflects light from nearby, bright stars. WISE.

UIG867200

Tank Advance, Italy 1944, 1944 (oil on canvas)

Tank Advance, Italy 1944, 1944 (oil on canvas)

Harris, Lawren Philips (1910-1994)

CIV214397

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Mars - Illustration - Mars - Illustration - Artist's view of the planet Mars. The three volcanoes of Tharsis and Olympus Mons are visible on the left. In the centre is the great canyon Valles Marineris. A “” full””” Mars. In this image the massive volcano Olympus Mons is clearly visible upper left of center, while near center are the three Tharsis Montes volcanoes. All these volcanoes are believed to be extinct. To the right of the Tharsis Montes are the deep canyons of Valles Marineris, a meandering network of channels as long as the United States is wide. Mars has been known historically as a bright, reddish “” star”” in Earth's sky. The ruddy hue is due to the presence of iron oxide (i.e., rust) on the martian surface. Mars is often host to white clouds of water - ice crystals (like the high - altitude cirrus clouds on Earth) and experiences seasonal dust storms that can cover the entire planet

Walter B Myers

PIX4616786

The ashes of Joan of Arc and the stake thrown into the Seine, from 'Jeanne d'Arc a Rouen', c.1900 (engraving)

The ashes of Joan of Arc and the stake thrown into the Seine, from 'Jeanne d'Arc a Rouen', c.1900 (engraving)

Deshays, Emile (fl.1890s)

CHT420083

The Veil Nebula, 2010

The Veil Nebula, 2010

UIG1580012

Volcanic ash cloud in Iceland - Volcanic ash cloud from Iceland - The volcanic ash plume caused by the eruption of the Eyjafjoell volcano (Eyjafjallajoekull) in Iceland seen by the Envisat satellite on 11 May 2010. A heavy plume of ash from Iceland's Eyjafjallajoekull volcano is visible travelling over the Atlantic in this Envisat Medium Resolution Imaging Spectrometer image acquired on 11 May 2010. The narrow shape of the ash cloud indicates a lot of wind is blowing in a southerly direction towards the west of Ireland. Also visible, the area around the Hakla volcano (east of Eyjafjallajoekull) now appears black as the snow and ice that surrounded it in April have been completely covered by ash. The volcano has been emitting steam and ash since its recent eruptions began on 20 March

Volcanic ash cloud in Iceland - Volcanic ash cloud from Iceland - The volcanic ash plume caused by the eruption of the Eyjafjoell volcano (Eyjafjallajoekull) in Iceland seen by the Envisat satellite on 11 May 2010. A heavy plume of ash from Iceland's Eyjafjallajoekull volcano is visible travelling over the Atlantic in this Envisat Medium Resolution Imaging Spectrometer image acquired on 11 May 2010. The narrow shape of the ash cloud indicates a lot of wind is blowing in a southerly direction towards the west of Ireland. Also visible, the area around the Hakla volcano (east of Eyjafjallajoekull) now appears black as the snow and ice that surrounded it in April have been completely covered by ash. The volcano has been emitting steam and ash since its recent eruptions began on 20 March

PIX4666212

The Great Volcanic Eruption in New Zealand, I (engraving)

The Great Volcanic Eruption in New Zealand, I (engraving)

English School, (19th century)

LIP1054930

Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Image made with Siding Spring's 3.9m telescope. Our view towards the centre of the Galaxy is obscured by extensive clouds of interstellar dust in the direction of the constellation of Sagittarius. The large - scale, patchy nature of the obscuration can be seen with the unaided eye and it is evident on smaller scales from the uneven distribution of background stars across this picture. Light from bright stars within the dust produces the two blue reflection nebulae (NGC 6589 and 6590), and these stars are members of a loose open cluster of stars, NGC 6595 (Sharpless 37) which is at a distance of about 5,900 light years. A large, almost transparent cloud of hydrogen, mixed with traces of dust, glows with a characteristic magenta hue over most of the field of view. This is known as IC 1283, 1284 and 4700 and is likely at a similar distance to NCC 6595 — Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Image made with Siding Spring's 3.9m telescope. Our view towards the centre of the Galaxy is obscured by extensive clouds of interstellar dust in the direction of the constellation of Sagittarius. The large - scale, patchy nature of the obscuration can be seen with the unaided eye and it is evident on smaller scales from the uneven distribution of background stars across this picture. Light from bright stars within the dust produces the two blue reflection nebulae (NGC 6589 and 6590), and these stars are members of a loose open cluster of stars, NGC 6595 (Sharpless 37) which is at a distance of about 5,900 light years. A large, almost transparent cloud of hydrogen, mixed with traces of dust, glows with a characteristic magenta hue over most of the field of view. This is known as IC 1283, 1284 and

Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Image made with Siding Spring's 3.9m telescope. Our view towards the centre of the Galaxy is obscured by extensive clouds of interstellar dust in the direction of the constellation of Sagittarius. The large - scale, patchy nature of the obscuration can be seen with the unaided eye and it is evident on smaller scales from the uneven distribution of background stars across this picture. Light from bright stars within the dust produces the two blue reflection nebulae (NGC 6589 and 6590), and these stars are members of a loose open cluster of stars, NGC 6595 (Sharpless 37) which is at a distance of about 5,900 light years. A large, almost transparent cloud of hydrogen, mixed with traces of dust, glows with a characteristic magenta hue over most of the field of view. This is known as IC 1283, 1284 and

PIX4619870

Swirling dust clouds and bright newborn stars dominate the view in this image of the Lagoon nebula from NASA's Spitzer Space Telescope.

Swirling dust clouds and bright newborn stars dominate the view in this image of the Lagoon nebula from NASA's Spitzer Space Telescope.

UIG867327

Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present, more isolated home. The infrared image from Spitzer highlights the filaments, colored yellow, green and red in this view, made up of dust associated with the cloud through which the cluster is traveling. The densest portion of the cloud appears in yellow and red, and the more diffuse outskirts are shown in green hues. One of the parent stars, Atlas, can be seen at the bottom left, while six of the sisters are visible at top. Additional stars in the cluster are sprinkled throughout the picture in blue — Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present

PIX4568892

Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon. Each telescope's contribution is presented in a different color: - Yellow represents the near-infrared observations of Hubble. These observations outline the energetic regions where stars are being born as well as reveal hundreds of thousands of stars. - Red represents the infrared observations of Spitzer. The radiation and winds from stars create glowing dust clouds that exhibit complex structures from compact, spherical globules to long, stringy filaments. - Blue and violet represent the X-ray observations of Chandra. X-rays are emitted by gas heated to millions of degrees by stellar explosions and by outflows from the supermassive black hole in the galaxy's center. The bright blue blob on the left side is emission from a double star system containing either a neutron star or a black hole. When these views are brought together, this composite image provides one of the most detailed — Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The ent

Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The ent

PIX4637984

Cowboy riding on a horse shooting with his pistol

Cowboy riding on a horse shooting with his pistol

SSI2167921

Elliptical Galaxy M110 (NGC 205) in Andromede - Elliptical galaxy M110 (NGC 205) in Andromeda - The elliptical galaxy M110, Andromede's satellite galaxy, is about the same distance from us as M31, about 2.9 million years - light. It is of type E6 “special” because it presents some unusual dark structures (probably dust clouds). M110 is the second small companion (along with M32) to our sister galaxy, M31, the Andromeda Nebula. It is classified as type E5 or E6, often with the additional “” p”” for peculiar because of the structure clearly visible in this short exposure image, which is probably due to dust clouds. Because of its small size, it is usually counted as a dwarf spheroidal rather than a normal elliptical

Elliptical Galaxy M110 (NGC 205) in Andromede - Elliptical galaxy M110 (NGC 205) in Andromeda - The elliptical galaxy M110, Andromede's satellite galaxy, is about the same distance from us as M31, about 2.9 million years - light. It is of type E6 “special” because it presents some unusual dark structures (probably dust clouds). M110 is the second small companion (along with M32) to our sister galaxy, M31, the Andromeda Nebula. It is classified as type E5 or E6, often with the additional “” p”” for peculiar because of the structure clearly visible in this short exposure image, which is probably due to dust clouds. Because of its small size, it is usually counted as a dwarf spheroidal rather than a normal elliptical

Jim Misti

PIX4608661

Skirmish During the Hungarian Revolution of 1848-1849, 1881 (oil on canvas)

Skirmish During the Hungarian Revolution of 1848-1849, 1881 (oil on canvas)

Villevalde, Alexander (1857-after 1906)

CH1195776

Martian Landscape - Illustration - Martian landscape - Illustration: Landscape on Mars with “dust devils” - Mars with dust devils

Martian Landscape - Illustration - Martian landscape - Illustration: Landscape on Mars with “dust devils” - Mars with dust devils

Miller, Ron (b.1947)

PIX4617016

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However, unlike the Milky Way, NGC 891 is relatively isolated, undisturbed by neighboring galaxies. If this was a distant view the Milky Way, the dust - lane would probably be distorted by interaction with the Magellanic Clouds, which would be prominent in the picture — Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

PIX4609481

Nebula Omega (M17) in Sagittarius - The Omega Nebula (M17) in the constellation Sagittarius - View of the nebula Omega (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. The Omega Nebula, Messier object 17 (M17), NGC 6618, in the constellation Sagittarius is a bright nebula, criss - crossed by clouds and lanes of opaque dust and gas. It is also known as the Swan Nebula and the Horseshoe Nebula. At a distance of 5700 light - years, M17 is also a source of radio noise

Nebula Omega (M17) in Sagittarius - The Omega Nebula (M17) in the constellation Sagittarius - View of the nebula Omega (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. The Omega Nebula, Messier object 17 (M17), NGC 6618, in the constellation Sagittarius is a bright nebula, criss - crossed by clouds and lanes of opaque dust and gas. It is also known as the Swan Nebula and the Horseshoe Nebula. At a distance of 5700 light - years, M17 is also a source of radio noise

R. Gendler

PIX4620089

The clouds of dust behind US Air Force C-17 Globemaster III at Fort Irwin

The clouds of dust behind US Air Force C-17 Globemaster III at Fort Irwin

UIG2911462

Nebula of the Eagle (IC 4703) in the Snake - detail - Star - birth in the Eagle nebula. - The Pillars of Creation “” is undoubtedly the most famous image realized by the Hubble space telescope, obtained in 1995. 20 years later, the same telescope rephotographed this region with more finesse. These cold gas columns are home to star embryos. The NASA/ESA Hubble Space Telescope has revisited one of its most iconic and popular images: the Eagle Nebula's Pillars of Creation. This image shows the pillars as seen in visible light, capturing the multi - coloured glow of gas clouds, wispy tendrils of dark cosmic dust, and the rust - colored elephants trunks of the nebula's famous pillars. The dust and gas in the pillars is seared by the intense radiation from young stars and eroded by strong winds from massive nearby stars. With these new images comes better contrast and a clearer view for astronomers to study how the structure of the pillars is changing over time.

Nebula of the Eagle (IC 4703) in the Snake - detail - Star - birth in the Eagle nebula. - The Pillars of Creation “” is undoubtedly the most famous image realized by the Hubble space telescope, obtained in 1995. 20 years later, the same telescope rephotographed this region with more finesse. These cold gas columns are home to star embryos. The NASA/ESA Hubble Space Telescope has revisited one of its most iconic and popular images: the Eagle Nebula's Pillars of Creation. This image shows the pillars as seen in visible light, capturing the multi - coloured glow of gas clouds, wispy tendrils of dark cosmic dust, and the rust - colored elephants trunks of the nebula's famous pillars. The dust and gas in the pillars is seared by the intense radiation from young stars and eroded by strong winds from massive nearby stars. With these new images comes better contrast and a clearer view for astronomers to study how the structure of the pillars is changing over time.

PIX4620070

Clouds and dust storm on the Sahara, 2014 (photo)

Clouds and dust storm on the Sahara, 2014 (photo)

PIX6039512

Clouds of dust and ash

Clouds of dust and ash

UTD2842876

Dust Clouds, 1935

Dust Clouds, 1935

UIG1580810

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Image obtained with the 3.9m Anglo - Australian Telescope from Siding Spring. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - Image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Image obtained with the 3.9m Anglo - Australian Telescope from Siding Spring. The Sombrero, named after the broad - brimmed Mexican hat it superficially resembles, is probably the most famous galaxy in the sky. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant

PIX4611674

Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Other wispy nebulae in the western part of the dark cloud betray the presence of young, hidden stars — Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Othe

Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Othe

PIX4620295

A Minute after the Signal declaring the Land Open, Racing across the Boundary amid blinding Clouds of Dust (litho)

A Minute after the Signal declaring the Land Open, Racing across the Boundary amid blinding Clouds of Dust (litho)

English School, (19th century)

LIP1063125

Andromede galaxy (M31) seen in X and infrared - Andromeda galaxy infrared and X - Ray composite - Andromede spiral galaxy seen in X-ray (blue) by the XMM - Newton space telescope and in infrared (orange) by the Herschel space telescope. This mosaic of the Andromeda spiral galaxy highlights explosive stars in its interior, and cooler, dusty stars forming in its many rings. The image is a combination of observations from the Herschel Space Observatory taken in infrared light (seen in orange hues), and the XMM - Newton telescope captured in X - rays (seen in blues). Herschel provides a detailed look at the cool clouds of star birth that line the galaxy's five concentric rings. Massive young stars are heating blankets of dust that surround them, causing them to glow in the longer - wavelength infrared light, known as far - infrared, that Herschel sees. In contrast, XMM - Newton is capturing what happens at the end of the lives of massive stars. It shows the high - energy X - rays that come from, among other objects, supernova explosions and massive dead stars rotating around companions. These X - ray sources are clustered in the center of the galaxy, where the most massive stars tend to form. Andromeda is our Milky Way galaxy's nearest large neighbor. It is located about 2.5 million light - years away and holds up to an estimated trillion stars. Our Milky Way is thought to contain about 200 billion to 400 billion stars — Andromede galaxy (M31) seen in X and infrared - Andromeda galaxy infrared and X - Ray composite - Andromede spiral galaxy seen in X-ray (blue) by the XMM - Newton space telescope and in infrared (orange) by the Herschel space telescope. This mosaic of the Andromeda spiral galaxy highlights explosive stars in its interior, and cooler, dusty stars forming in its many rings. The image is a combination of observations from the Herschel Space Observatory taken in infrared light (seen in orange hues), and the XMM - Newton telescope captured in X - rays (seen in blues). Herschel provides a detailed look at the cool clouds of star birth that line the galaxy's five concentric rings. Massive young stars are heating blankets of dust that surround them, causing them to glow in the longer - wavelength infrared light, known as far - infrared, that Herschel sees. In contrast, XMM - Newton is capturing what happens at the end of the lives of massive stars. It shows the high - energy X - rays that come

Andromede galaxy (M31) seen in X and infrared - Andromeda galaxy infrared and X - Ray composite - Andromede spiral galaxy seen in X-ray (blue) by the XMM - Newton space telescope and in infrared (orange) by the Herschel space telescope. This mosaic of the Andromeda spiral galaxy highlights explosive stars in its interior, and cooler, dusty stars forming in its many rings. The image is a combination of observations from the Herschel Space Observatory taken in infrared light (seen in orange hues), and the XMM - Newton telescope captured in X - rays (seen in blues). Herschel provides a detailed look at the cool clouds of star birth that line the galaxy's five concentric rings. Massive young stars are heating blankets of dust that surround them, causing them to glow in the longer - wavelength infrared light, known as far - infrared, that Herschel sees. In contrast, XMM - Newton is capturing what happens at the end of the lives of massive stars. It shows the high - energy X - rays that come

PIX4609049

Marvels of Motion, The Whirlwind (chromolitho)

Marvels of Motion, The Whirlwind (chromolitho)

English School, (20th century)

LLM5205802

The spiral arms and dust clouds in the nearby Whirlpool galaxy. Hubble Space Telescope (HST).

The spiral arms and dust clouds in the nearby Whirlpool galaxy. Hubble Space Telescope (HST).

UIG867050

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host galaxy. Like a rock tossed into a lake, the collision sent a ripple of energy into space, plowing gas and dust in front of it. Expanding at 200,000 miles per hour, this cosmic tsunami leaves in its wake a firestorm of new star creation. Hubble resolves bright blue knots that are gigantic clusters of newborn stars and immense loops and bubbles blown into space by exploding stars (supernovae) going off like a string of firecrackers. The Cartwheel Galaxy presumably was a normal spiral galaxy like our Milky Way before the collision. This spiral structure is beginning to re - emerge, as seen in the faint arms or spokes between the outer ring and bulls - eye shaped nucleus. The ring contains at least several billion new stars that would not normally have been created in such a short time span and is so large (150,000 light - years across) our entire Milky Way Galaxy would fit inside. Hubble's new view does not solve the mystery as to which of the two small galaxies m — Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host

PIX4613594

The spiral arms and dust clouds in the nearby Whirlpool galaxy. Hubble Space Telescope (HST).

The spiral arms and dust clouds in the nearby Whirlpool galaxy. Hubble Space Telescope (HST).

UIG867052

Volcanic ash cloud in Iceland - Volcanic ash cloud from Iceland - The volcanic ash cloud caused by the eruption of the Eyjafjoell volcano in Iceland seen by the Envisat satellite on 19 April 2010. In this image taken on 19 April 2010 by ESA's Envisat satellite, a heavy plume of ash from the Eyjafjallajoekull Volcano in Iceland is seen travelling in a roughly southeasterly direction. The volcano has been emitting steam and ash since its recent eruptions began on 20 March, and as observable, the emissions continue. The plume, visible in brownish - grey, is approximately 400 km long

Volcanic ash cloud in Iceland - Volcanic ash cloud from Iceland - The volcanic ash cloud caused by the eruption of the Eyjafjoell volcano in Iceland seen by the Envisat satellite on 19 April 2010. In this image taken on 19 April 2010 by ESA's Envisat satellite, a heavy plume of ash from the Eyjafjallajoekull Volcano in Iceland is seen travelling in a roughly southeasterly direction. The volcano has been emitting steam and ash since its recent eruptions began on 20 March, and as observable, the emissions continue. The plume, visible in brownish - grey, is approximately 400 km long

PIX4666194

United States, 1950s: Footage of a column of radioactive particles after nuclear explosion

United States, 1950s: Footage of a column of radioactive particles after nuclear explosion

AVE6327684

Clouds of dust and ash over a volcano

Clouds of dust and ash over a volcano

UTD2842895

United States, 1950s: Drawing showing the movement of particles inside a nuclear cloud column

United States, 1950s: Drawing showing the movement of particles inside a nuclear cloud column

AVE6327680

United States, 1950s: Cloud forming after a nuclear explosion

United States, 1950s: Cloud forming after a nuclear explosion

AVE6327678

A dying star (center) surrounded by a cloud of glowing gas and dust. The star and its cloud halo constitute a "planetary nebula" called NGC 246. Spitzer Space Telescope.

A dying star (center) surrounded by a cloud of glowing gas and dust. The star and its cloud halo constitute a "planetary nebula" called NGC 246. Spitzer Space Telescope.

UIG867065

A dying star (center) surrounded by a cloud of glowing gas and dust. The star and its cloud halo constitute a "planetary nebula" called NGC 246. Spitzer Space Telescope.

A dying star (center) surrounded by a cloud of glowing gas and dust. The star and its cloud halo constitute a "planetary nebula" called NGC 246. Spitzer Space Telescope.

UIG867066

Spitzer Space Telescope comparison views in visible light and infrared of the glowing Trifid Nebula, a giant star-forming cloud of gas and dust located 5,400 light-years away in the Sagittarius. Credit NASA. Science Astronomy

Spitzer Space Telescope comparison views in visible light and infrared of the glowing Trifid Nebula, a giant star-forming cloud of gas and dust located 5,400 light-years away in the Sagittarius. Credit NASA. Science Astronomy

UIG528815

Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. It is one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth.

Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. It is one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth.

UIG867109

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

UIG867150

NASA's WISE captured this image of a hidden star-forming cloud of dust and gas located in the constellation of Cepheus.

NASA's WISE captured this image of a hidden star-forming cloud of dust and gas located in the constellation of Cepheus.

UIG867202

Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. It is one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth.

Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. It is one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth.

UIG867111

Spitzer Space Telescope composite comparison visible-light and infrared views of the glowing Trifid Nebula, a giant star-forming cloud of gas and dust located in the constellation Sagittarius. Credit NASA. Science Astronomy

Spitzer Space Telescope composite comparison visible-light and infrared views of the glowing Trifid Nebula, a giant star-forming cloud of gas and dust located in the constellation Sagittarius. Credit NASA. Science Astronomy

UIG528812

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

UIG867151

NASA's WISE captured this image of a hidden star-forming cloud of dust and gas located in the constellation of Cepheus.

NASA's WISE captured this image of a hidden star-forming cloud of dust and gas located in the constellation of Cepheus.

UIG867203

Astronomers have discovered a giant supernova that is smothered in its own dust. In this artist's rendering, an outer shell of gas and dust -- which erupted from the star hundreds of years ago -- obscures the supernova within.

Astronomers have discovered a giant supernova that is smothered in its own dust. In this artist's rendering, an outer shell of gas and dust -- which erupted from the star hundreds of years ago -- obscures the supernova within.

UIG867254

Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. It is one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth.

Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. It is one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth.

UIG867110

The blue star near the center of this image is Zeta Ophiuchi. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. WISE.

The blue star near the center of this image is Zeta Ophiuchi. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. WISE.

UIG867251

Animation of Dust Escaping from a Pipe and Causing Clouds

Animation of Dust Escaping from a Pipe and Causing Clouds

AVE6328521

The blue star near the center of this image is Zeta Ophiuchi. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. WISE.

The blue star near the center of this image is Zeta Ophiuchi. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. WISE.

UIG867249

Gripped in the claw of the constellation Scorpius sits the reflection nebula DG 129, a cloud of gas and dust that reflects light from nearby, bright stars. WISE.

Gripped in the claw of the constellation Scorpius sits the reflection nebula DG 129, a cloud of gas and dust that reflects light from nearby, bright stars. WISE.

UIG867199

1950s: Smoking rocket launch at shore explodes into cloud

1950s: Smoking rocket launch at shore explodes into cloud

AVE6319720

Sandstorm In Chuquicamata (photo)

Sandstorm In Chuquicamata (photo)

UIG2915917

WISE captured this view of a runaway star racing away from its original home. Seen here surrounded by a glowing cloud of gas and dust, the star AE Aurigae appears to be on fire. The cloud is called the Flaming Star nebula.

WISE captured this view of a runaway star racing away from its original home. Seen here surrounded by a glowing cloud of gas and dust, the star AE Aurigae appears to be on fire. The cloud is called the Flaming Star nebula.

UIG867238

WISE captured this view of a runaway star racing away from its original home. Seen here surrounded by a glowing cloud of gas and dust, the star AE Aurigae appears to be on fire. The cloud is called the Flaming Star nebula.

WISE captured this view of a runaway star racing away from its original home. Seen here surrounded by a glowing cloud of gas and dust, the star AE Aurigae appears to be on fire. The cloud is called the Flaming Star nebula.

UIG867237

WISE captured this view of a runaway star racing away from its original home. Seen here surrounded by a glowing cloud of gas and dust, the star AE Aurigae appears to be on fire. The cloud is called the Flaming Star nebula.

WISE captured this view of a runaway star racing away from its original home. Seen here surrounded by a glowing cloud of gas and dust, the star AE Aurigae appears to be on fire. The cloud is called the Flaming Star nebula.

UIG867239

The Cocoon nebula is featured in this image from NASA's WISE. This cloud of dust and gas, cataloged as IC 5146 and located in the constellation Cygnus, is wrapped in a dark cloud of dust called Barnard 168. Within this cocoon of dust and gas, new stars are forming and beginning to emerge into the wild.

The Cocoon nebula is featured in this image from NASA's WISE. This cloud of dust and gas, cataloged as IC 5146 and located in the constellation Cygnus, is wrapped in a dark cloud of dust called Barnard 168. Within this cocoon of dust and gas, new stars are forming and beginning to emerge into the wild.

UIG867227

Sprinting Cheetahs (photo)

Sprinting Cheetahs (photo)

UIG806796

Sprinting Cheetahs (photo)

Sprinting Cheetahs (photo)

UIG806795

The Cocoon nebula is featured in this image from NASA's WISE. This cloud of dust and gas, cataloged as IC 5146 and located in the constellation Cygnus, is wrapped in a dark cloud of dust called Barnard 168. Within this cocoon of dust and gas, new stars are forming and beginning to emerge into the wild.

The Cocoon nebula is featured in this image from NASA's WISE. This cloud of dust and gas, cataloged as IC 5146 and located in the constellation Cygnus, is wrapped in a dark cloud of dust called Barnard 168. Within this cocoon of dust and gas, new stars are forming and beginning to emerge into the wild.

UIG867230

The Cocoon nebula is featured in this image from NASA's WISE. This cloud of dust and gas, cataloged as IC 5146 and located in the constellation Cygnus, is wrapped in a dark cloud of dust called Barnard 168. Within this cocoon of dust and gas, new stars are forming and beginning to emerge into the wild.

The Cocoon nebula is featured in this image from NASA's WISE. This cloud of dust and gas, cataloged as IC 5146 and located in the constellation Cygnus, is wrapped in a dark cloud of dust called Barnard 168. Within this cocoon of dust and gas, new stars are forming and beginning to emerge into the wild.

UIG867229

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

UIG867187

NASA's WISE shows the Rosette nebula located within the constellation Monoceros, or the Unicorn. This nebula, also known as NGC 2237, is a huge star-forming cloud of dust and gas in our Milky Way galaxy. Estimates of the nebula's distance vary from 4,500 to 5,000 light-years away.

NASA's WISE shows the Rosette nebula located within the constellation Monoceros, or the Unicorn. This nebula, also known as NGC 2237, is a huge star-forming cloud of dust and gas in our Milky Way galaxy. Estimates of the nebula's distance vary from 4,500 to 5,000 light-years away.

UIG867198

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

UIG867190

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

UIG867189

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

UIG867188

NASA's WISE shows the Rosette nebula located within the constellation Monoceros, or the Unicorn. This nebula, also known as NGC 2237, is a huge star-forming cloud of dust and gas in our Milky Way galaxy. Estimates of the nebula's distance vary from 4,500 to 5,000 light-years away.

NASA's WISE shows the Rosette nebula located within the constellation Monoceros, or the Unicorn. This nebula, also known as NGC 2237, is a huge star-forming cloud of dust and gas in our Milky Way galaxy. Estimates of the nebula's distance vary from 4,500 to 5,000 light-years away.

UIG867197

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

Sprawling across the constellation Vela is a complex of dark, dense clouds of dust and gas. The complex is called the Vela Molecular Cloud Ridge. This ridge may form part of the edge of the Orion spiral arm spur in our Milky Way galaxy. WISE.

UIG867191

Sprinting Cheetahs (photo)

Sprinting Cheetahs (photo)

UIG806794

Clouds of dust behind US Air Force C-17 Globemaster III

Clouds of dust behind US Air Force C-17 Globemaster III

UIG2626111

Volcanic ash cloud over United Kingdom - Volcanic ash cloud above United Kingdom - Volcanic ash cloud caused by the eruption of Eyjafjoell volcano in Iceland seen by Envisat satellite on 15 April 2010. This image, acquired on 15 April 2010 by Envisat's Medium Resolution Imaging Spectrometer (MERIS), shows the vast cloud of volcanic ash sweeping across the UK from the eruption of Eyjafjallajoekull volcano in Iceland, more than 1000 km away. The ash, which can be seen as the large grey streak in the image, is drifting from west to east at a height of about 11 km above the surface Earth

Volcanic ash cloud over United Kingdom - Volcanic ash cloud above United Kingdom - Volcanic ash cloud caused by the eruption of Eyjafjoell volcano in Iceland seen by Envisat satellite on 15 April 2010. This image, acquired on 15 April 2010 by Envisat's Medium Resolution Imaging Spectrometer (MERIS), shows the vast cloud of volcanic ash sweeping across the UK from the eruption of Eyjafjallajoekull volcano in Iceland, more than 1000 km away. The ash, which can be seen as the large grey streak in the image, is drifting from west to east at a height of about 11 km above the surface Earth

PIX4666179

Jabbah is the name of the bright star right of center, surrounded by a red colored dust cloud. It is a whole system of stars. WISE.

Jabbah is the name of the bright star right of center, surrounded by a red colored dust cloud. It is a whole system of stars. WISE.

UIG867335

Town Of Dalhart Turns Into A Texas Dust Bowl, 1930s

Town Of Dalhart Turns Into A Texas Dust Bowl, 1930s

BOF6284552

Dark stars and nebulae in Sagittarius and Ophiuchus - Dark Nebulae in Sagittarius and Scorpius - Dark nebulae on the edge of the Pipe nebula. This complex of dust clouds that block the light of the stars is located between the Sagittarius and the Scorpio, near the center of our lactee road. Also visible, the nebulae emitted from the Lagoon, Trifide, and Omega. Image obtained with Canon 20Da, 50 mm f/1.4, 6 x 5 min ISO 1600 poses. This amazing complex of dark nebulae and dust in Sagittarius and Ophiuchus lies near the central bulge of our own galaxy, the Milky Way. Dark nebulae are non - luminous clouds of obscuring matter and dust which block the light from stars behind them. Many of the dark nebulae seen here are listed in E.E. Barnard's catalog of dark nebulae and are given a “” B” designation, such as B72, the Snake Nebula. Almost the entire complex of dark nebulae seen on the right hand side of the image make up the “Dark Horse and Rider””. The Pipe Nebula, Lynds Dark Nebula 1773, comprises the hind quarter and back leg of the Dark Horse, which is seen vertically in this image. B63 is the front leg, B270 is the Horse's head, and B276 is the Rider's head. The area is also filled with star clouds, bright emission nebulae such as M8 - the Lagoon Nebula, M20 - the Trifid Nebula, and M17 - the Omega Nebula. The small Sagittarius star cloud, M24, is at the upper left, and the large Sagittarius star cloud at lower left. The center of our galaxy lies near the bottom edge of the image. Image taken with a Canon 20Da DSLR, 50 mm f/1.4, and 6 x 5 min exposures at ISO 1600 — Dark stars and nebulae in Sagittarius and Ophiuchus - Dark Nebulae in Sagittarius and Scorpius - Dark nebulae on the edge of the Pipe nebula. This complex of dust clouds that block the light of the stars is located between the Sagittarius and the Scorpio, near the center of our lactee road. Also visible, the nebulae emitted from the Lagoon, Trifide, and Omega. Image obtained with Canon 20Da, 50 mm f/1.4, 6 x 5 min ISO 1600 poses. This amazing complex of dark nebulae and dust in Sagittarius and Ophiuchus lies near the central bulge of our own galaxy, the Milky Way. Dark nebulae are non - luminous clouds of obscuring matter and dust which block the light from stars behind them. Many of the dark nebulae seen here are listed in E.E. Barnard's catalog of dark nebulae and are given a “” B” designation, such as B72, the Snake Nebula. Almost the entire complex of dark nebulae seen on the right hand side of the image make up the “Dark Horse and Rider””. The Pipe Nebula, Lynds Dark Nebula 1773,

Dark stars and nebulae in Sagittarius and Ophiuchus - Dark Nebulae in Sagittarius and Scorpius - Dark nebulae on the edge of the Pipe nebula. This complex of dust clouds that block the light of the stars is located between the Sagittarius and the Scorpio, near the center of our lactee road. Also visible, the nebulae emitted from the Lagoon, Trifide, and Omega. Image obtained with Canon 20Da, 50 mm f/1.4, 6 x 5 min ISO 1600 poses. This amazing complex of dark nebulae and dust in Sagittarius and Ophiuchus lies near the central bulge of our own galaxy, the Milky Way. Dark nebulae are non - luminous clouds of obscuring matter and dust which block the light from stars behind them. Many of the dark nebulae seen here are listed in E.E. Barnard's catalog of dark nebulae and are given a “” B” designation, such as B72, the Snake Nebula. Almost the entire complex of dark nebulae seen on the right hand side of the image make up the “Dark Horse and Rider””. The Pipe Nebula, Lynds Dark Nebula 1773,

Jerry Lodriguss

PIX4621393

Jabbah is the name of the bright star right of center, surrounded by a red colored dust cloud. It is a whole system of stars. WISE.

Jabbah is the name of the bright star right of center, surrounded by a red colored dust cloud. It is a whole system of stars. WISE.

UIG867336

Earth seen from space: California and Mexico - Dust storm in Baja California seen from space - Dust Tempete on Baja California. Image obtained by Aqua satellite on 27 November 2011. Dust clouds blowing out of Mexico across an otherwise cloud - free view of Baja California. Late November 2011 offered mostly cloud - free skies and a compelling view of the entire length of Baja California and the Pacific coast of Mexico. In the midst of the clarity, strong northeasterly winds stirred up dust storms on the mainland and the peninsula. The natural - color images required to make this oblique view were acquired on November 27, 2011, by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua satellite

Earth seen from space: California and Mexico - Dust storm in Baja California seen from space - Dust Tempete on Baja California. Image obtained by Aqua satellite on 27 November 2011. Dust clouds blowing out of Mexico across an otherwise cloud - free view of Baja California. Late November 2011 offered mostly cloud - free skies and a compelling view of the entire length of Baja California and the Pacific coast of Mexico. In the midst of the clarity, strong northeasterly winds stirred up dust storms on the mainland and the peninsula. The natural - color images required to make this oblique view were acquired on November 27, 2011, by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua satellite

PIX4673273

United States, 1950s: A race car is photographed as it speeds and leaves the audience in its dust

United States, 1950s: A race car is photographed as it speeds and leaves the audience in its dust

AVE6327718

Piles of pebbles, mining waste from the Roman era, Special Nature Reserve of Bessa, Piedmont, Italy

Piles of pebbles, mining waste from the Roman era, Special Nature Reserve of Bessa, Piedmont, Italy

DGA2570773

Piles of pebbles, mining waste from the Roman era, Special Nature Reserve of Bessa, Piedmont, Italy

Piles of pebbles, mining waste from the Roman era, Special Nature Reserve of Bessa, Piedmont, Italy

DGA2570771

This image of the Elephant's Trunk nebula from NASA's WISE, shows clouds of dust and gas being pushed and eroded by a massive star.

This image of the Elephant's Trunk nebula from NASA's WISE, shows clouds of dust and gas being pushed and eroded by a massive star.

UIG867293

USA, Alaska, Eastern Interior, Chitina, dust clouds rolling off Copper River

USA, Alaska, Eastern Interior, Chitina, dust clouds rolling off Copper River

UDK842251

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