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Images from Hubble

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An aesthetic close-up of cosmic clouds and stellar winds featuring LL Orionis, interacting with the Orion Nebula flow. Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun. REUTERS/NASA, ESA and the Hubble Heritage Team

An aesthetic close-up of cosmic clouds and stellar winds featuring LL Orionis, interacting with the Orion Nebula flow. Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun. REUTERS/NASA, ESA and the Hubble Heritage Team

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U Camelopardalis, or U Cam for short, a star nearing the end of its life located in the constellation of Camelopardalis, near the North Celestial Pole. REUTERS/ESA/Hubble, NASA and H. Olofsson

U Camelopardalis, or U Cam for short, a star nearing the end of its life located in the constellation of Camelopardalis, near the North Celestial Pole. REUTERS/ESA/Hubble, NASA and H. Olofsson

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The glowing remains of a dying, sun-like star - of the so-called "ant nebula" (Menzel 3, or Mz3). REUTERS/NASA

The glowing remains of a dying, sun-like star - of the so-called "ant nebula" (Menzel 3, or Mz3). REUTERS/NASA

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The tempestuous stellar nursery called the Carina Nebula, located 7,500 light-years away from Earth in the southern constellation Carina. REUTERS/NASA

The tempestuous stellar nursery called the Carina Nebula, located 7,500 light-years away from Earth in the southern constellation Carina. REUTERS/NASA

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A view of gas pillars in the M16 Eagle Nebula. REUTERS/NASA

A view of gas pillars in the M16 Eagle Nebula. REUTERS/NASA

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Star cluster NGC 2060, a loose collection of stars in 30 Doradus, located in the heart of the Tarantula Nebula 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. REUTERS/NASA/European Southern Observatory/Space Telescope Science Institute/Hubble Space Telescope

Star cluster NGC 2060, a loose collection of stars in 30 Doradus, located in the heart of the Tarantula Nebula 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. REUTERS/NASA/European Southern Observatory/Space Telescope Science Institute/Hubble Space Telescope

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A view of the Whirlpool Galaxy's curving arms where newborn stars reside and its yellowish central core that serves as home for older stars. REUTERS/NASA

A view of the Whirlpool Galaxy's curving arms where newborn stars reside and its yellowish central core that serves as home for older stars. REUTERS/NASA

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Star V838 Monocerotis's (V838 Mon) light echo, which is about six light years in diameter. REUTERS/ NASA, ESA, H. E. Bond (STScI)

Star V838 Monocerotis's (V838 Mon) light echo, which is about six light years in diameter. REUTERS/ NASA, ESA, H. E. Bond (STScI)

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One of the largest mosaics ever assembled from Hubble photos shows several million young stars vying for attention amid a raucous stellar breeding ground in 30 Doradus, a star-forming complex located in the heart of the Tarantula nebula. REUTERS/NASA/ESA

One of the largest mosaics ever assembled from Hubble photos shows several million young stars vying for attention amid a raucous stellar breeding ground in 30 Doradus, a star-forming complex located in the heart of the Tarantula nebula. REUTERS/NASA/ESA

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An image of a small region within a hotbed of star formation M17, also known as the Omega or Swan Nebula, located about 5,500 light-years from Earth in the constellation Sagittarius. REUTERS/NASA/ESA/J. Hester

An image of a small region within a hotbed of star formation M17, also known as the Omega or Swan Nebula, located about 5,500 light-years from Earth in the constellation Sagittarius. REUTERS/NASA/ESA/J. Hester

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A pair of gravitationally interacting galaxies called Arp 147. The left-most galaxy is relatively undisturbed apart from a smooth ring of starlight. It appears nearly on edge to our line of sight. The right- most galaxy, resembling a "zero," exhibits a clumpy, blue ring of intense star formation. REUTERS/NASA/Handout

A pair of gravitationally interacting galaxies called Arp 147. The left-most galaxy is relatively undisturbed apart from a smooth ring of starlight. It appears nearly on edge to our line of sight. The right- most galaxy, resembling a "zero," exhibits a clumpy, blue ring of intense star formation. REUTERS/NASA/Handout

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A panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, revealing the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by dust. REUTERS/NASA/ESA/Hubble Heritage

A panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, revealing the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by dust. REUTERS/NASA/ESA/Hubble Heritage

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An image of the Eagle Nebula reveals a tall, dense tower of gas being sculpted by ultraviolet light from a group of massive, hot stars. REUTERS/NASA/Handout

An image of the Eagle Nebula reveals a tall, dense tower of gas being sculpted by ultraviolet light from a group of massive, hot stars. REUTERS/NASA/Handout

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An image of the Antennae galaxies, as the two galaxies smash together, during which time billions of stars are born, mostly in groups and clusters. The brightest and most compact of these are called super star clusters. REUTERS/NASA, ESA/Hubble/B. Whitmore/Space Telescope Science Institute

An image of the Antennae galaxies, as the two galaxies smash together, during which time billions of stars are born, mostly in groups and clusters. The brightest and most compact of these are called super star clusters. REUTERS/NASA, ESA/Hubble/B. Whitmore/Space Telescope Science Institute

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An image of the Pencil Nebula shows remnants from a star that exploded thousands of years ago. REUTERS/NASA

An image of the Pencil Nebula shows remnants from a star that exploded thousands of years ago. REUTERS/NASA

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Supernova remnant 0509-67.5, located in the Large Magellanic Cloud (LMC), a small galaxy about 170,000 light-years from Earth. REUTERS/NASA, ESA, CXC, SAO, Hubble Heritage Team (STScI/AURA), J. Hughes (Rutgers University)

Supernova remnant 0509-67.5, located in the Large Magellanic Cloud (LMC), a small galaxy about 170,000 light-years from Earth. REUTERS/NASA, ESA, CXC, SAO, Hubble Heritage Team (STScI/AURA), J. Hughes (Rutgers University)

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An image of the Bug Nebula shows impressive walls of compressed gas, laced with trailing strands and bubbling outflows. A dark, dusty torus surrounds the inner nebula (seen at the upper right). At the heart of the turmoil is one of the hottest stars known. REUTERS/HO/ESA/NASA/Albert Zijlstra

An image of the Bug Nebula shows impressive walls of compressed gas, laced with trailing strands and bubbling outflows. A dark, dusty torus surrounds the inner nebula (seen at the upper right). At the heart of the turmoil is one of the hottest stars known. REUTERS/HO/ESA/NASA/Albert Zijlstra

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The "Black Eye" galaxy, so named because an ancient cosmic smashup produced a dark ring and a roiling, conflicted interior. What looks like a black eye in the image is actually a dark band of dust that stands out vividly in front of the galaxy's bright nucleus. REUTERS/NASA and The Hubble Heritage Team

The "Black Eye" galaxy, so named because an ancient cosmic smashup produced a dark ring and a roiling, conflicted interior. What looks like a black eye in the image is actually a dark band of dust that stands out vividly in front of the galaxy's bright nucleus. REUTERS/NASA and The Hubble Heritage Team

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An image of a nebula about 170,000 light-years away. REUTERS/NASA, ESA, Hubble Heritage Team

An image of a nebula about 170,000 light-years away. REUTERS/NASA, ESA, Hubble Heritage Team

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An image shows a giant star-forming nebula with massive young stellar clusters. REUTERS/NASA, ESA, and the Hubble Heritage/Handout

An image shows a giant star-forming nebula with massive young stellar clusters. REUTERS/NASA, ESA, and the Hubble Heritage/Handout

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A pair of interacting galaxies consisting of NGC 5754, the large spiral on the right, and NGC 5752, the smaller companion in the bottom left. NGC 5754's internal structure has hardly been disturbed by the interaction. The outer structure does exhibit tidal features, as does the symmetry of the inner spiral pattern and the kinked arms just beyond its inner ring. In contrast, NGC 5752 has undergone a starburst episode, with a rich...more

A pair of interacting galaxies consisting of NGC 5754, the large spiral on the right, and NGC 5752, the smaller companion in the bottom left. NGC 5754's internal structure has hardly been disturbed by the interaction. The outer structure does exhibit tidal features, as does the symmetry of the inner spiral pattern and the kinked arms just beyond its inner ring. In contrast, NGC 5752 has undergone a starburst episode, with a rich population of massive and luminous star clusters clumping around the core and intertwined with intricate dust lanes. The contrasting reactions of the two galaxies to their interaction are due to their differing masses and sizes. REUTERS/NASA, ESA, the Hubble Heritage Team/ESA/Hubble Collaboration/W. Keel/University of Alabama

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An image of the Orion nebula shows four monstrously massive stars at the center of the cloud. REUTERS/ NASA/JPL-Caltech/T. Megeath/University of Toledo/M. Robberto/STScI

An image of the Orion nebula shows four monstrously massive stars at the center of the cloud. REUTERS/ NASA/JPL-Caltech/T. Megeath/University of Toledo/M. Robberto/STScI

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A massive star known as Eta Carinae in our Milky Way galaxy that experts believe might explode in a supernova in the astronomically near future. REUTERS/NASA/Handout

A massive star known as Eta Carinae in our Milky Way galaxy that experts believe might explode in a supernova in the astronomically near future. REUTERS/NASA/Handout

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An image of Jupiter shows the planet's trademark belts and zones of high- and low-pressure regions in crisp detail. Circular convection cells can be seen at high northern and southern latitudes. REUTERS/NASA, ESA, and the Hubble Heritage Team

An image of Jupiter shows the planet's trademark belts and zones of high- and low-pressure regions in crisp detail. Circular convection cells can be seen at high northern and southern latitudes. REUTERS/NASA, ESA, and the Hubble Heritage Team

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The staggering aftermath of an encounter between two galaxies, resulting in a ring-shaped galaxy and a long-tailed companion. The collision between the two parent galaxies produced a shockwave effect that first drew matter into the center and then caused it to propagate outwards in a ring. REUTERS/NASA/ESA

The staggering aftermath of an encounter between two galaxies, resulting in a ring-shaped galaxy and a long-tailed companion. The collision between the two parent galaxies produced a shockwave effect that first drew matter into the center and then caused it to propagate outwards in a ring. REUTERS/NASA/ESA

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A view of AM 1316-241, made up of two interacting galaxies - a spiral galaxy in front of an elliptical galaxy. The starlight from the background galaxy is partially obscured by the bands and filaments of dust associated with the foreground spiral galaxy. REUTERS/NASA, ESA, the Hubble Heritage Team/ESA/Hubble Collaboration/W. Keel/University of Alabama

A view of AM 1316-241, made up of two interacting galaxies - a spiral galaxy in front of an elliptical galaxy. The starlight from the background galaxy is partially obscured by the bands and filaments of dust associated with the foreground spiral galaxy. REUTERS/NASA, ESA, the Hubble Heritage Team/ESA/Hubble Collaboration/W. Keel/University of Alabama

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A view of Mars made from a series of exposures taken over a fify-two minute period. REUTERS/J. Bell/Cornell U/and M. Wolff

A view of Mars made from a series of exposures taken over a fify-two minute period. REUTERS/J. Bell/Cornell U/and M. Wolff

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An image of a type 2 Seyfert galaxy that lies 13 million light-years away in the southern constellation Circinus. The galaxy has a compact center and is believed to contain a massive black hole. REUTERS/NASA

An image of a type 2 Seyfert galaxy that lies 13 million light-years away in the southern constellation Circinus. The galaxy has a compact center and is believed to contain a massive black hole. REUTERS/NASA

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An image of galaxy NGC 1512 showing a monster area - 2,400 light-years across - filled with clusters of infant stars. REUTERS/NASA

An image of galaxy NGC 1512 showing a monster area - 2,400 light-years across - filled with clusters of infant stars. REUTERS/NASA

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The Hubble telescope took a close-up look at this heavenly icon, revealing the cloud's intricate structure. This detailed view of the horse's head was released April 24, 2001 to celebrate the orbiting observatory's eleventh anniversary. REUTERS/Handout

The Hubble telescope took a close-up look at this heavenly icon, revealing the cloud's intricate structure. This detailed view of the horse's head was released April 24, 2001 to celebrate the orbiting observatory's eleventh anniversary. REUTERS/Handout

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A new view of the Eagle Nebula, one of the two largest and sharpest images Hubble Space Telescope has ever taken, is released by NASA on Hubble's 15th anniversary April 25, 2005. REUTERS/NASA/Handout

A new view of the Eagle Nebula, one of the two largest and sharpest images Hubble Space Telescope has ever taken, is released by NASA on Hubble's 15th anniversary April 25, 2005. REUTERS/NASA/Handout

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This image, released April 29, 2004, of the Bug Nebula (NGC 6302) taken with the NASA/ESA Hubble Space Telescope, shows impressive walls of compressed gas, laced with trailing strands and bubbling outflows. A dark, dusty torus surrounds the inner nebula (seen at the upper right). At the heart of the turmoil is one of the hottest stars known. Despite a sizzling temperature of at least 250,000 degrees C, the star itself has never...more

This image, released April 29, 2004, of the Bug Nebula (NGC 6302) taken with the NASA/ESA Hubble Space Telescope, shows impressive walls of compressed gas, laced with trailing strands and bubbling outflows. A dark, dusty torus surrounds the inner nebula (seen at the upper right). At the heart of the turmoil is one of the hottest stars known. Despite a sizzling temperature of at least 250,000 degrees C, the star itself has never been seen, as it is hidden by the blanket of dust and shines most brightly in the ultraviolet, making it hard to observe. REUTERS/HO/ESA/NASA and Albert Zijlstra

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Image taken from Hubble space telescope shows a crater on an object called 8405 Asbolus, a 48 mile-wide chuck of ice and dust that lies between Saturn and Uranus. Astronomers using the telescope found what looks like a fresh water crater less than 10 million years old, exposing underlying ice that is apparently unlike any yet seen. REUTERS/Handout

Image taken from Hubble space telescope shows a crater on an object called 8405 Asbolus, a 48 mile-wide chuck of ice and dust that lies between Saturn and Uranus. Astronomers using the telescope found what looks like a fresh water crater less than 10 million years old, exposing underlying ice that is apparently unlike any yet seen. REUTERS/Handout

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Resembling a swirling witch's cauldron of glowing vapors, the black hole-powered core of a nearby active galaxy appears in this colorful NASA Hubble Space Telescope image taken April 10, 1999. The galaxy lies 13 million light-years away in the southern constellation Circinus. This galaxy is designated a type 2 Seyfert, a class of mostly spiral galaxies that have compact centers and are believed to contain massive black holes....more

Resembling a swirling witch's cauldron of glowing vapors, the black hole-powered core of a nearby active galaxy appears in this colorful NASA Hubble Space Telescope image taken April 10, 1999. The galaxy lies 13 million light-years away in the southern constellation Circinus. This galaxy is designated a type 2 Seyfert, a class of mostly spiral galaxies that have compact centers and are believed to contain massive black holes. Seyfert galaxies are themselves part of a larger class of objects called Active Galactic Nuclei or AGN. AGN have the ability to remove gas from the centers of their galaxies by blowing it out into space at phenomenal speeds. Astronomers studying the Circinus galaxy are seeing evidence of a powerful AGN at the center of this galaxy as well. REUTERS/Handout

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A bizarre comet-like X-pattern of filamentary structures circling about 90 million miles from Earth. It is believed the object was created by the collision of two asteroids. REUTERS/NASA/ESA

A bizarre comet-like X-pattern of filamentary structures circling about 90 million miles from Earth. It is believed the object was created by the collision of two asteroids. REUTERS/NASA/ESA

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The first visible-light snapshot of a planet circling another star. Estimated to be no more than three times Jupiter's mass the planet, called Fomalhaut b, orbits the bright southern star Fomalhaut, located 25 light-years away. REUTERS/NASA/ESA

The first visible-light snapshot of a planet circling another star. Estimated to be no more than three times Jupiter's mass the planet, called Fomalhaut b, orbits the bright southern star Fomalhaut, located 25 light-years away. REUTERS/NASA/ESA

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A large rare population of hot, bright stars inside the hub of the neighboring Andromeda galaxy. REUTERS/NASA

A large rare population of hot, bright stars inside the hub of the neighboring Andromeda galaxy. REUTERS/NASA

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An image of a ghostly ring of dark matter in a galaxy cluster designated Cl 0024 17. Astronomers call the ring one of the strongest pieces of evidence to date for the existence of dark matter and suggest the ring was produced from a collision between two gigantic clusters. REUTERS/NASA, ESA, M.J. Jee and H. Ford/Johns Hopkins University/Handout

An image of a ghostly ring of dark matter in a galaxy cluster designated Cl 0024 17. Astronomers call the ring one of the strongest pieces of evidence to date for the existence of dark matter and suggest the ring was produced from a collision between two gigantic clusters. REUTERS/NASA, ESA, M.J. Jee and H. Ford/Johns Hopkins University/Handout

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An image of a coil-shaped Helix Nebula showing a fine web of filamentary "bicycle-spoke" features embedded in the colorful red and blue ring of gas. At 650 light-years away, the Helix is one of the nearest planetary nebulae to Earth. A planetary nebula is the glowing gas around a dying, Sun-like star. REUTERS/NASA

An image of a coil-shaped Helix Nebula showing a fine web of filamentary "bicycle-spoke" features embedded in the colorful red and blue ring of gas. At 650 light-years away, the Helix is one of the nearest planetary nebulae to Earth. A planetary nebula is the glowing gas around a dying, Sun-like star. REUTERS/NASA

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The photo, taken by NASA's Hubble Space Telescope, captures a small region within M17, a hotbed of star formation M17, also known as the Omega or Swan Nebula, is located about 5,500 light-years (1690 parsecs) from Earth in the constellation Sagittarius. The turbulent gases in this photo of Gaseous Nebula in the Milky Way Galaxy shows roughly 1.9.arcminutes (3.1 light-years or 0.95 parsecs) across. The image is being released to...more

The photo, taken by NASA's Hubble Space Telescope, captures a small region within M17, a hotbed of star formation M17, also known as the Omega or Swan Nebula, is located about 5,500 light-years (1690 parsecs) from Earth in the constellation Sagittarius. The turbulent gases in this photo of Gaseous Nebula in the Milky Way Galaxy shows roughly 1.9.arcminutes (3.1 light-years or 0.95 parsecs) across. The image is being released to commemorate the 13th anniversary of Hubble's launch on April 24, 1990. REUTERS/NASA, ESA and J. Hester (ASU)/Handout

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