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View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656706

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656691

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656709

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656712

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656703

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656715

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 39.3 - metre E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 39.3 - metre E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

PIX4653099

Cerro Armazones - Cerro Armazones in the Atacama desert. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. View of Cerro Armazones in the Chilean desert, near Eso's Paranal Observatory, site of the Very Large Telescope (VLT). Cerro Armazones was chosen as the site for the planned European Extremely Large Telescope (E - ELT), which, with its 42 - metre diameter mirror, will be the world's biggest eye on the sky

Cerro Armazones - Cerro Armazones in the Atacama desert. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. View of Cerro Armazones in the Chilean desert, near Eso's Paranal Observatory, site of the Very Large Telescope (VLT). Cerro Armazones was chosen as the site for the planned European Extremely Large Telescope (E - ELT), which, with its 42 - metre diameter mirror, will be the world's biggest eye on the sky

Serge Brunier

PIX4653014

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. A new architectural concept drawing of Eso's planned European Extremely Large Telescope (E - ELT) shows the telescope at work, with its dome open and its record - setting 40 - metre - class primary mirror pointed to the sky. In this illustration, clouds float over the valley overlooked by the E - Elt's summit. The comparatively tiny pickup truck parked at the base of the E - ELT helps to give a sense of the scale of this massive telescope. The E - ELT dome will be similar in size to a football stadium, with a diameter at its base of over 100 m and a height of over 80 m. Scheduled to begin operations early in the next decade, the E - ELT will help tra

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. A new architectural concept drawing of Eso's planned European Extremely Large Telescope (E - ELT) shows the telescope at work, with its dome open and its record - setting 40 - metre - class primary mirror pointed to the sky. In this illustration, clouds float over the valley overlooked by the E - Elt's summit. The comparatively tiny pickup truck parked at the base of the E - ELT helps to give a sense of the scale of this massive telescope. The E - ELT dome will be similar in size to a football stadium, with a diameter at its base of over 100 m and a height of over 80 m. Scheduled to begin operations early in the next decade, the E - ELT will help tra

PIX4653098

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. The construction of this European project is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The E - ELT features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 42 metres in diameter. The construction of this European project is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. With a 42 - m diameter primary mirror, the present baseline, its total rotating mass is 5500 tons. The two platforms on each side of the structure hold large instruments. The E - ELT features a novel, innovative design, based on 5 mirrors. The primary 42 - m mirror is composed of 906 segments, each 1.45 m wide, while the secondary mirror is as large as 6 m in diameter. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 - m mirror supported by 5000 or more actuators so

PIX4653110

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 40 - metre - class E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) in its enclosure on Cerro Armazones, a 3060 - metre mountaintop in Chile's Atacama Desert. The 40 - metre - class E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E - ELT will tackle some of the biggest scientific challenges of our time

PIX4653079

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. A new architectural concept drawing of Eso's planned European Extremely Large Telescope (E - ELT) shows the telescope at work, with its dome open and its record - setting 40 - metre - class primary mirror pointed to the sky. In this illustration, clouds float over the valley overlooked by the E - Elt's summit. The comparatively tiny pickup truck parked at the base of the E - ELT helps to give a sense of the scale of this massive telescope. The E - ELT dome will be similar in size to a football stadium, with a diameter at its base of over 100 m and a height of over 80 m. Scheduled to begin operations early in the next decade, the E - ELT will help tra

Telescope E - ELT - Artist's view - European Extremely Large Telescope - Artwork - Artist's view of the E - ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. A new architectural concept drawing of Eso's planned European Extremely Large Telescope (E - ELT) shows the telescope at work, with its dome open and its record - setting 40 - metre - class primary mirror pointed to the sky. In this illustration, clouds float over the valley overlooked by the E - Elt's summit. The comparatively tiny pickup truck parked at the base of the E - ELT helps to give a sense of the scale of this massive telescope. The E - ELT dome will be similar in size to a football stadium, with a diameter at its base of over 100 m and a height of over 80 m. Scheduled to begin operations early in the next decade, the E - ELT will help tra

PIX4653092

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

PIX4653104

Telescope E - ELT - Artist's View - The E - ELT on Cerro Armazones (artist's printing) - Artist's View of E - ELT (European Extremely Large Telescope), a telescope project measuring 39 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) on Cerro Armazones, at 3060 - metre mountaintop in Chile's Atacama Desert. The E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky

Telescope E - ELT - Artist's View - The E - ELT on Cerro Armazones (artist's printing) - Artist's View of E - ELT (European Extremely Large Telescope), a telescope project measuring 39 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. Artist's impression of the European Extremely Large Telescope (E - ELT) on Cerro Armazones, at 3060 - metre mountaintop in Chile's Atacama Desert. The E - ELT will be the largest optical/infrared telescope in the world - - the world's biggest eye on the sky

PIX4653085

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

Telescope E-ELT -Artist's view - European Extremely Large Telescope - Artwork: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 40 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field - Artist's impression of the European Extremely Large Telescope (E-ELT) in its enclosure on Cerro Armazones, a 3060-metre mountaintop in Chile's Atacama Desert. The 40-meter-class E-ELT will be the largest optical/infrared telescope in the world - the world's biggest eye on the sky. Operations are planned to start early in the next decade, and the E-ELT will tackle some of the biggest scientific challenges of our time - This artist's rendering of the E-ELT is based on the detailed construction design for the telescope

PIX4653094

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656710

Giant telescope

Giant telescope

McConnell, James Edwin (1903-95)

LAL319595

The Sun and Moon on Cerro Armazones - Sun and Moon on Cerro Armazones - 360-degree panorama showing the meteorological station at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. This sunset 360 degree panorama shows the ESO Astronomical Site Monitor on Cerro Armazones in the Chilean desert, near Eso's Paranal Observatory, site of the Very Large Telescope (VLT). Cerro Armazones was chosen as the site for the planned European Extremely Large Telescope (E - ELT), which, with its 42 - metre diameter mirror, will be the world's biggest eye on the sky

The Sun and Moon on Cerro Armazones - Sun and Moon on Cerro Armazones - 360-degree panorama showing the meteorological station at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. This sunset 360 degree panorama shows the ESO Astronomical Site Monitor on Cerro Armazones in the Chilean desert, near Eso's Paranal Observatory, site of the Very Large Telescope (VLT). Cerro Armazones was chosen as the site for the planned European Extremely Large Telescope (E - ELT), which, with its 42 - metre diameter mirror, will be the world's biggest eye on the sky

Serge Brunier

PIX4653005

Sunset on Cerro Armazones - Cerro Armazones at Sunset - Panorama showing the meteorological station at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. 360 - degree panorama of Cerro Armazones in the Chilean desert, near Eso's Paranal Observatory, site of the Very Large Telescope (VLT). Cerro Armazones was chosen as the site for the planned European Extremely Large Telescope (E - ELT), which, with its 42 - metre diameter mirror, will be the world's biggest eye on the sky

Sunset on Cerro Armazones - Cerro Armazones at Sunset - Panorama showing the meteorological station at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. 360 - degree panorama of Cerro Armazones in the Chilean desert, near Eso's Paranal Observatory, site of the Very Large Telescope (VLT). Cerro Armazones was chosen as the site for the planned European Extremely Large Telescope (E - ELT), which, with its 42 - metre diameter mirror, will be the world's biggest eye on the sky

Serge Brunier

PIX4653002

Gazing at the stars - Observation of the sky with a telescope. Star party in Romania. Here we are observing with the 14.5”” telescope. Above the telescope there's Orion, probably the most famous constellation in the winter sky, with its red giant Betelgeuse. Close to the upper edge of the photo you can see the open cluster of the Pleiades. In between Orion and the Pleiades, we have the head of Taurus, the Bull. That is actually another open cluster called the Hyades

Gazing at the stars - Observation of the sky with a telescope. Star party in Romania. Here we are observing with the 14.5”” telescope. Above the telescope there's Orion, probably the most famous constellation in the winter sky, with its red giant Betelgeuse. Close to the upper edge of the photo you can see the open cluster of the Pleiades. In between Orion and the Pleiades, we have the head of Taurus, the Bull. That is actually another open cluster called the Hyades

Alex Conu

PIX4565950

Hypertelescope Carlina - Carlina Hypertelescope concept - This hypertelescope concept is the optical analogue of Arecibo's radiotelescope, but it uses a balloon to carry focal optics. On the ground, several mirrors in a crater or a natural bowl form a virtual giant mirror. Principle of the Carlina hypertelescope. Many small mirrors are distributed on a spherical surface. A helium balloon carries a gondola that contains focal optics

Hypertelescope Carlina - Carlina Hypertelescope concept - This hypertelescope concept is the optical analogue of Arecibo's radiotelescope, but it uses a balloon to carry focal optics. On the ground, several mirrors in a crater or a natural bowl form a virtual giant mirror. Principle of the Carlina hypertelescope. Many small mirrors are distributed on a spherical surface. A helium balloon carries a gondola that contains focal optics

Gregoire Cirade

PIX4655341

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

NASA Hubble Space Telescope close-up view of an electric-blue aurora that is eerily glowing one half billion miles away on the giant planet Jupiter

NASA Hubble Space Telescope close-up view of an electric-blue aurora that is eerily glowing one half billion miles away on the giant planet Jupiter

UIG529273

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. 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 by the Hubble Space Telescope and the Large Binocular Telescope. In this composite image, visible - light observations by Nasa's Hubble Space Telescope are combined with infrared data from the ground - based Large Binocular Telescope in Arizona to assemble a dramatic view of the well - known Ring Nebula. Called a planetary nebula, the Ring Nebula is the glowing remains of a Sun - like star. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doug

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. 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 by the Hubble Space Telescope and the Large Binocular Telescope. In this composite image, visible - light observations by Nasa's Hubble Space Telescope are combined with infrared data from the ground - based Large Binocular Telescope in Arizona to assemble a dramatic view of the well - known Ring Nebula. Called a planetary nebula, the Ring Nebula is the glowing remains of a Sun - like star. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doug

PIX4623411

Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with im

Open cluster NGC 4755 - Jewel Box - The Jewel Box star cluster - The NGC 4755 cluster is located in the constellation of the Southern Cross at a distance of 6400 years - light from Earth. The bright orange star on the top right is Kappa Crucis, a supergiant red star. This cluster contains about fifty stars formed about 16 million years ago. This close-up of the center of the cluster was obtained with the Hubble Space Telescope. This image is a “” close - up 'view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue supergiant stars, a solitary ruby - red supergiant and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dimmest stars are less than half the mass of the Sun. This is the first image of an open galactic cluster with im

PIX4568246

Globular cluster NGC 6401 in Ophiuchus - Globular cluster NGC 6401 in Ophiuchus - The NASA/ESA Hubble Space Telescope has used its powerful optics to separate the globular cluster NGC 6401 into its constituent stars. What was once only visible as a ghostly mist in the eyepieces of astronomical instruments has been transformed into a stunning stellar landscape. NGC 6401 can be found within the constellation of Ophiuchus (The Serpent Bearer). The globular cluster itself is relatively faint, so a telescope and some observational experience are required to see it. Globular clusters are very rich, and generally spherical, collections of stars, hence the name. They orbit the cores of galaxies, with the force of gravity also keeping the stars bound as a group. There are around 160 globular clusters associated with our Milky Way, of which NGC 6401 is one. These objects are very old, containing some of the most ancient stars known. However, there are many mysteries surrounding them, with the or

Globular cluster NGC 6401 in Ophiuchus - Globular cluster NGC 6401 in Ophiuchus - The NASA/ESA Hubble Space Telescope has used its powerful optics to separate the globular cluster NGC 6401 into its constituent stars. What was once only visible as a ghostly mist in the eyepieces of astronomical instruments has been transformed into a stunning stellar landscape. NGC 6401 can be found within the constellation of Ophiuchus (The Serpent Bearer). The globular cluster itself is relatively faint, so a telescope and some observational experience are required to see it. Globular clusters are very rich, and generally spherical, collections of stars, hence the name. They orbit the cores of galaxies, with the force of gravity also keeping the stars bound as a group. There are around 160 globular clusters associated with our Milky Way, of which NGC 6401 is one. These objects are very old, containing some of the most ancient stars known. However, there are many mysteries surrounding them, with the or

PIX4564826

Globular cluster M15 in Pegase - Globular cluster M15 in Pegasus - View of the globular cluster M15 by the Hubble space telescope. Located about 35,000 light years away from Earth in the constellation Pegase, M15 is one of 150 known globular clusters forming a vast halo around our galaxy. The bluish object in the middle left of the image is a planetary nebula: Kuestner 648 (Pease 1). Planetary nebulae are gas shells ejected by a star at the end of life, after its phase of red giante; they are very rarely observed in globular clusters or their presence is not yet well understood. The globular cluster Messier 15 is shown in this color image obtained with the NASA Hubble Space Telescope. Lying some 35,000 light - years from Earth in the direction of the constellation Pegasus, M15 is one of almost 150 known globular clusters that form a vast halo surrounding our Milky Way galaxy. The bluish object to the middle left of the image is a gas cloud surrounding a dying star, a planetary nebula k

Globular cluster M15 in Pegase - Globular cluster M15 in Pegasus - View of the globular cluster M15 by the Hubble space telescope. Located about 35,000 light years away from Earth in the constellation Pegase, M15 is one of 150 known globular clusters forming a vast halo around our galaxy. The bluish object in the middle left of the image is a planetary nebula: Kuestner 648 (Pease 1). Planetary nebulae are gas shells ejected by a star at the end of life, after its phase of red giante; they are very rarely observed in globular clusters or their presence is not yet well understood. The globular cluster Messier 15 is shown in this color image obtained with the NASA Hubble Space Telescope. Lying some 35,000 light - years from Earth in the direction of the constellation Pegasus, M15 is one of almost 150 known globular clusters that form a vast halo surrounding our Milky Way galaxy. The bluish object to the middle left of the image is a gas cloud surrounding a dying star, a planetary nebula k

PIX4565141

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

PIX4564266

Spiral Galaxy NGC 3810 in the Lion - Spiral galaxy NGC 3810 in Leo - NGC 3810 is a spiral galaxy located at a distance of about 50 million light years in the constellation Lion. Image obtained by the Hubble Space Telescope. The bright galaxy NGC 3810 demonstrates classical spiral structure in this very detailed image from Hubble. The bright central region is thought to be forming many new stars and is outshining the outer areas of the galaxy by some margin. Further out the galaxy displays strikingly rich dust clouds along its spiral arms. A close look shows that Hubble's sharp vision also allows many individual stars to be seen. Hot young blue stars show up in giant clusters far from the center and the arms are also littered with bright red giant stars. NGC 3810 is located about 50 million light - years from Earth in the constellation of Leo (the lion). It was discovered by William Herschel in 1784 and is easily seen as a faint smudge in small telescopes

Spiral Galaxy NGC 3810 in the Lion - Spiral galaxy NGC 3810 in Leo - NGC 3810 is a spiral galaxy located at a distance of about 50 million light years in the constellation Lion. Image obtained by the Hubble Space Telescope. The bright galaxy NGC 3810 demonstrates classical spiral structure in this very detailed image from Hubble. The bright central region is thought to be forming many new stars and is outshining the outer areas of the galaxy by some margin. Further out the galaxy displays strikingly rich dust clouds along its spiral arms. A close look shows that Hubble's sharp vision also allows many individual stars to be seen. Hot young blue stars show up in giant clusters far from the center and the arms are also littered with bright red giant stars. NGC 3810 is located about 50 million light - years from Earth in the constellation of Leo (the lion). It was discovered by William Herschel in 1784 and is easily seen as a faint smudge in small telescopes

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

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

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Lenticular galaxy NGC 4710 in Berenice's Hair - Lenticular galaxy NGC 4710 in Coma Berenices - The galaxy NGC 4710 is located about 60 million years ago - light from Earth, in the galaxy cluster of Our Lady. It's a lenticular galaxy seen from the slice. Image obtained by the Hubble Space Telescope. Edge - on galaxy located at about 60 million light years away. NGC 4710 is a member of the giant Virgo Cluster of galaxies and lies in the northern constellation of Coma Berenices (the Hair of Queen Berenice). It is not one of the brightest members of the cluster, but can easily be seen as a dim elongated smudge on a dark night with a medium - sized amateur telescope. In the 1780s, William Herschel discovered the galaxy and noted it simply as a “” faint nebula””. It is an example of a lenticular or S0 - type galaxy - a type that seems to have some characteristics of both spiral and elliptical galaxies. Image taken by the Hubble Space Telescope

Lenticular galaxy NGC 4710 in Berenice's Hair - Lenticular galaxy NGC 4710 in Coma Berenices - The galaxy NGC 4710 is located about 60 million years ago - light from Earth, in the galaxy cluster of Our Lady. It's a lenticular galaxy seen from the slice. Image obtained by the Hubble Space Telescope. Edge - on galaxy located at about 60 million light years away. NGC 4710 is a member of the giant Virgo Cluster of galaxies and lies in the northern constellation of Coma Berenices (the Hair of Queen Berenice). It is not one of the brightest members of the cluster, but can easily be seen as a dim elongated smudge on a dark night with a medium - sized amateur telescope. In the 1780s, William Herschel discovered the galaxy and noted it simply as a “” faint nebula””. It is an example of a lenticular or S0 - type galaxy - a type that seems to have some characteristics of both spiral and elliptical galaxies. Image taken by the Hubble Space Telescope

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Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

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Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

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Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. This image was obtained by the Hubble Space Telescope in April 2002. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image obtained by the Hubble space telescope in April 2002

Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. This image was obtained by the Hubble Space Telescope in April 2002. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image obtained by the Hubble space telescope in April 2002

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Artist's rendering of the planned Giant Magellan Telescope, 2005 (digital)

Artist's rendering of the planned Giant Magellan Telescope, 2005 (digital)

Mason, Todd (20th-21st century)

SMT1217095

Star field in the constellation Sagittarius - Scattered stars in Sagittarius: Stars in Sagittarius seen by the space telescope Hubble. This stunning image, captured by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys (ACS), shows part of the sky in the constellation of Sagittarius (The Archer). The region is rendered in exquisite detail - deep red and bright blue stars are scattered across the frame, set against a background of thousands of more distant stars and galaxies. Two features are particularly striking: the colours of the stars, and the dramatic crosses that burst from the centres of the brightest bodies. While some of the colours in this frame have been enhanced and tweaked during the process of creating the image from the observational data, different stars do indeed glow in different colours. Stars differ in colour according to their surface temperature: very hot stars are blue or white, while cooler stars are redder. They may be cooler because they are sma

Star field in the constellation Sagittarius - Scattered stars in Sagittarius: Stars in Sagittarius seen by the space telescope Hubble. This stunning image, captured by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys (ACS), shows part of the sky in the constellation of Sagittarius (The Archer). The region is rendered in exquisite detail - deep red and bright blue stars are scattered across the frame, set against a background of thousands of more distant stars and galaxies. Two features are particularly striking: the colours of the stars, and the dramatic crosses that burst from the centres of the brightest bodies. While some of the colours in this frame have been enhanced and tweaked during the process of creating the image from the observational data, different stars do indeed glow in different colours. Stars differ in colour according to their surface temperature: very hot stars are blue or white, while cooler stars are redder. They may be cooler because they are sma

PIX4572253

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

PIX4572109

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

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Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

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Giant Telescope (litho)

Giant Telescope (litho)

English School, (20th century)

LLM2812593

Asteroides Ceres and Vesta seen by the Hubble space telescope - Asteroids Ceres and Vesta seen by the Hubble space telescope - Ceres and Vesta are the two largest bodies of the asteroid belt, a region located between Mars and Jupiter. Since August 2006, Ceres is considered a dwarf planet. Ceres (left) has a diameter of about 950 km. Image obtained in January 2004. The image on the right, obtained on 14 and 16 May 2007, shows the asteroid Vesta. Its diameter is about 530 km. These Hubble Space Telescope images of Vesta and Ceres show two of the most massive asteroids in the asteroid belt, a region between Mars and Jupiter. At least 100,000 asteroids inhabit the asteroid belt, a reservoir of leftover material from the formation of our solar-system planets 4.6 billion years ago. The International Astronomical Union named Ceres one of three dwarf planets in 2006. Ceres is round like planets in our solar system, but it does not clear debris out of its orbit as our planets do. The image at r

Asteroides Ceres and Vesta seen by the Hubble space telescope - Asteroids Ceres and Vesta seen by the Hubble space telescope - Ceres and Vesta are the two largest bodies of the asteroid belt, a region located between Mars and Jupiter. Since August 2006, Ceres is considered a dwarf planet. Ceres (left) has a diameter of about 950 km. Image obtained in January 2004. The image on the right, obtained on 14 and 16 May 2007, shows the asteroid Vesta. Its diameter is about 530 km. These Hubble Space Telescope images of Vesta and Ceres show two of the most massive asteroids in the asteroid belt, a region between Mars and Jupiter. At least 100,000 asteroids inhabit the asteroid belt, a reservoir of leftover material from the formation of our solar-system planets 4.6 billion years ago. The International Astronomical Union named Ceres one of three dwarf planets in 2006. Ceres is round like planets in our solar system, but it does not clear debris out of its orbit as our planets do. The image at r

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Telescope E-ELT -Artist's view - E-ELT concept: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 39 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. The Cerro Amazones mountain in the Chilean desert, near Eso's Paranal Observatory, will be the site for the European Extremely Large Telescope (E-ELT), which, with its 39-metre diameter mirror, will be the world's biggest eye on the sky. Here, an artist's rendering shows how the telescope will look on the mountain when it is complete in 2024

Telescope E-ELT -Artist's view - E-ELT concept: Artist's view of the E-ELT (European Extremely Large Telescope), a telescope project measuring 39 metres in diameter. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. The Cerro Amazones mountain in the Chilean desert, near Eso's Paranal Observatory, will be the site for the European Extremely Large Telescope (E-ELT), which, with its 39-metre diameter mirror, will be the world's biggest eye on the sky. Here, an artist's rendering shows how the telescope will look on the mountain when it is complete in 2024

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Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

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Asteroide Vesta seen by the Hubble Space Telescope - Asteroid Vesta - Photo obtained in visible view of the Vesta asteroid in May 1996 by the Hubble Space Telescope. The images reveal a huge impact crater 450 km in diameter south of the asteroid; the original image is at the top left, modeled in 3D on the right. Astronomers have used the Hubble Space telescope to discover a giant impact crater on the asteroid Vesta. <BR>Left is a Hubble Space Telescope image of the asteroid Vesta, taken in May 1996 when the asteroid was 110 million miles from Earth. The asymmetry of the asteroid and “” nub”” and the south pole is suggestive that it suffered a large impact event. Center is a color-encoded elevation map of Vesta that clearly shows the giant 285- mile diameter impact basin and “” bull 's-eye”” central peak. Right is a 3-D computer model of the asteroid Vesta synthesized from Hubble topographic data. The crater's 8-mile high central peak can clearly be seen near the pole. At the bottom an

Asteroide Vesta seen by the Hubble Space Telescope - Asteroid Vesta - Photo obtained in visible view of the Vesta asteroid in May 1996 by the Hubble Space Telescope. The images reveal a huge impact crater 450 km in diameter south of the asteroid; the original image is at the top left, modeled in 3D on the right. Astronomers have used the Hubble Space telescope to discover a giant impact crater on the asteroid Vesta. <BR>Left is a Hubble Space Telescope image of the asteroid Vesta, taken in May 1996 when the asteroid was 110 million miles from Earth. The asymmetry of the asteroid and “” nub”” and the south pole is suggestive that it suffered a large impact event. Center is a color-encoded elevation map of Vesta that clearly shows the giant 285- mile diameter impact basin and “” bull 's-eye”” central peak. Right is a 3-D computer model of the asteroid Vesta synthesized from Hubble topographic data. The crater's 8-mile high central peak can clearly be seen near the pole. At the bottom an

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Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. This image was obtained by the Hubble Space Telescope in April 2002. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image obtained by the Hubble space telescope in April 2002

Colliding galaxies NGC 4676 in Berenice's Hair - Colliding galaxies NGC 4676 - The galaxy NGC 4676 is located about 300 million years away - light from Earth. It is a system of two spiral galaxies that collide and eventually become one galaxy. This image was obtained by the Hubble Space Telescope in April 2002. Located 300 million light - years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed “” The Mice”” because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. Image obtained by the Hubble space telescope in April 2002

PIX4611830

Centre of the nebula of the Lagoon (M8) seen by the Hubble space telescope. The Lagoon Nebula is a star-forming region located about 4000 light years from Earth.

Centre of the nebula of the Lagoon (M8) seen by the Hubble space telescope. The Lagoon Nebula is a star-forming region located about 4000 light years from Earth.

PIX4619950

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

PIX4612940

Detail of the Cone nebula in the Unicorn - The Cone Nebula (NGC 2264) - Detail - Image obtained by the Hubble space telescope of the upper part of the Cone nebula (NGC 2264), a star-forming region located about 2500 years ago - light from Earth. The Cone Nebula (NGC 2264) - - so named because, in ground - based images, it has a conical shape - - this giant pillar resides in a turbulent star - forming region. This picture, taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope, shows the upper 2.5 light - years of the nebula, a height that equals 23 million roundtrips to the Moon. The entire nebula is 7 light - years long. The Cone Nebula resides 2,500 light - years away in the constellation Monoceros. ACS made this observation on April 2, 2002. The color image is constructed from three separate images taken in blue, near - infrared, and hydrogen - alpha filters

Detail of the Cone nebula in the Unicorn - The Cone Nebula (NGC 2264) - Detail - Image obtained by the Hubble space telescope of the upper part of the Cone nebula (NGC 2264), a star-forming region located about 2500 years ago - light from Earth. The Cone Nebula (NGC 2264) - - so named because, in ground - based images, it has a conical shape - - this giant pillar resides in a turbulent star - forming region. This picture, taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope, shows the upper 2.5 light - years of the nebula, a height that equals 23 million roundtrips to the Moon. The entire nebula is 7 light - years long. The Cone Nebula resides 2,500 light - years away in the constellation Monoceros. ACS made this observation on April 2, 2002. The color image is constructed from three separate images taken in blue, near - infrared, and hydrogen - alpha filters

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Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

Serge Brunier

PIX4652988

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

Galaxy clusters LCDCS - 0829 - Galaxy cluster LCDCS - 0829 - Gravitational lenses in the galaxy cluster LCDCS - 0829. Image obtained by the Hubble Space Telescope. The NASA/ESA Hubble Space Telescope usually works as a solo artist to capture awe - inspiring images of the distant Universe. For this picture, though, Hubble had a helping hand from the subject of the image, a galaxy cluster called LCDCS - 0829, as the huge mass of the galaxies in the cluster acted like a giant magnifying glass. This strange effect is called gravitational lensing. The object was discovered during the Las Campanas Distant Clusters Survey, which explains the cluster's unusual name. This survey was carried out in March 1995 using a 1 - metre telescope at the Las Campanas Observatory in Chile. More than one thousand clusters of galaxies, most of them previously unknown, were found in a dedicated survey of a long, but narrow, section of the southern sky. The bizarre phenomenon of gravitational lensing is a conse

Galaxy clusters LCDCS - 0829 - Galaxy cluster LCDCS - 0829 - Gravitational lenses in the galaxy cluster LCDCS - 0829. Image obtained by the Hubble Space Telescope. The NASA/ESA Hubble Space Telescope usually works as a solo artist to capture awe - inspiring images of the distant Universe. For this picture, though, Hubble had a helping hand from the subject of the image, a galaxy cluster called LCDCS - 0829, as the huge mass of the galaxies in the cluster acted like a giant magnifying glass. This strange effect is called gravitational lensing. The object was discovered during the Las Campanas Distant Clusters Survey, which explains the cluster's unusual name. This survey was carried out in March 1995 using a 1 - metre telescope at the Las Campanas Observatory in Chile. More than one thousand clusters of galaxies, most of them previously unknown, were found in a dedicated survey of a long, but narrow, section of the southern sky. The bizarre phenomenon of gravitational lensing is a conse

PIX4565707

Liquid mirror telescope on the Moon - Lunar liquid mirror telescope - Illustration of an astronomical observatory on the Moon. Installs near the southern pole of the Moon, a giant telescope with liquid mirror, one kilometre in diameter. A giant liquid mirror telescope 1 kilometer wide (6 tenths of a mile) and 1 kilometer tall lies nestled in an approximately 1 kilometer wide crater near the Moon's south pole. In the foreground is a kind of lunar city for human habitation composed of pressurized and radiation-hardened living units. On the upper right are landing pads for transports arriving to and departing from the lunar surface. A liquid mirror telescope is a Newtonian reflecting type telescope that employs a reflecting liquid as the primary mirror. A concept first identified 300 years ago by Isaac Newton himself, the reflecting liquid assumes the proper paraboloidal shape by rotating the container the liquid is in. On Earth working liquid mirror telescopes have been created with diam

Liquid mirror telescope on the Moon - Lunar liquid mirror telescope - Illustration of an astronomical observatory on the Moon. Installs near the southern pole of the Moon, a giant telescope with liquid mirror, one kilometre in diameter. A giant liquid mirror telescope 1 kilometer wide (6 tenths of a mile) and 1 kilometer tall lies nestled in an approximately 1 kilometer wide crater near the Moon's south pole. In the foreground is a kind of lunar city for human habitation composed of pressurized and radiation-hardened living units. On the upper right are landing pads for transports arriving to and departing from the lunar surface. A liquid mirror telescope is a Newtonian reflecting type telescope that employs a reflecting liquid as the primary mirror. A concept first identified 300 years ago by Isaac Newton himself, the reflecting liquid assumes the proper paraboloidal shape by rotating the container the liquid is in. On Earth working liquid mirror telescopes have been created with diam

Walter B Myers

PIX4639385

Detail of the nebula NGC 3324 in the Carene - Detail of nebula NGC 3324 in Carina - Detail of the nebula NGC 3324 obtained by the Hubble space telescope. This nebula is located in the southern hemisphere, close to the great Carene nebula about 7200 light years from Earth. The image obtained by the Hubble Space Telescope shows a gas wall at the edge of a cavite created by the radiation and stellar winds blown by young warm stars. Hubble space telescope image shows the edge of a giant gaseous cavity within the star - forming region called NGC 3324. The glowing nebula has been carved out by intense ultraviolet radiation and stellar winds from several hot, young stars. A cluster of extremely massive stars, located well outside this image in the center of the nebula, is responsible for the ionization of the nebula and excavation of the cavity. The image also reveals dramatic dark towers of cool gas and dust that rise above the glowing wall of gas. The dense gas at the top resists the bliste

Detail of the nebula NGC 3324 in the Carene - Detail of nebula NGC 3324 in Carina - Detail of the nebula NGC 3324 obtained by the Hubble space telescope. This nebula is located in the southern hemisphere, close to the great Carene nebula about 7200 light years from Earth. The image obtained by the Hubble Space Telescope shows a gas wall at the edge of a cavite created by the radiation and stellar winds blown by young warm stars. Hubble space telescope image shows the edge of a giant gaseous cavity within the star - forming region called NGC 3324. The glowing nebula has been carved out by intense ultraviolet radiation and stellar winds from several hot, young stars. A cluster of extremely massive stars, located well outside this image in the center of the nebula, is responsible for the ionization of the nebula and excavation of the cavity. The image also reveals dramatic dark towers of cool gas and dust that rise above the glowing wall of gas. The dense gas at the top resists the bliste

PIX4618883

Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

Milky Way above Cerro Armazones - Star sky at the top of Cerro Armazones. This 3060-metre mountain in Chile will host the giant telescope E - ELT (European Extremely Large Telescope). The construction of this 42-metre telescope is expected to start at the end of 2010 and will be inaugurated around 2018. Its main mirror will consist of 906 hexagonal mirrors assembled together, and its total surface will be equal to that of a football field. On 26 April 2010, the ESO Council selected Cerro Armazones as the baseline site for the planned 42 - metre European Extremely Large Telescope (E - ELT). Cerro Armazones is a mountain at an altitude of 3060 metres in the central part of Child's Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of Eso's Very Large Telescope

Serge Brunier

PIX4652987

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

Elliptical galaxy NGC 1316 in the Furnace - Giant elliptical galaxy NGC 1316 - By studying the clusters of stars and clouds of dust visible in this photo taken by the Hubble space telescope in March 2003, it is believed that the giant elliptical galaxy NGC 1316 is the result of a collision of two spiral galaxies that occurred some billions of years ago. This galaxy resides about 75 million light years ago in the cluster of galaxies of the Furnace. Also called Fornax A, it is one of the strongest radio sources in the sky. This image made from data obtained with the NASA Hubble Space Telescope reveals the dust lanes and star clusters of this giant galaxy that give evidence that it was formed from a past merger of two gas - rich galaxies. NGC 1316 is on the outskirts of a nearby cluster of galaxies in the southern constellation of Fornax, at a distance of about 75 million light - years. It is one of the brightest ellipticals in the Fornax galaxy cluster. NGC 1316, also known as Fornax A,

Elliptical galaxy NGC 1316 in the Furnace - Giant elliptical galaxy NGC 1316 - By studying the clusters of stars and clouds of dust visible in this photo taken by the Hubble space telescope in March 2003, it is believed that the giant elliptical galaxy NGC 1316 is the result of a collision of two spiral galaxies that occurred some billions of years ago. This galaxy resides about 75 million light years ago in the cluster of galaxies of the Furnace. Also called Fornax A, it is one of the strongest radio sources in the sky. This image made from data obtained with the NASA Hubble Space Telescope reveals the dust lanes and star clusters of this giant galaxy that give evidence that it was formed from a past merger of two gas - rich galaxies. NGC 1316 is on the outskirts of a nearby cluster of galaxies in the southern constellation of Fornax, at a distance of about 75 million light - years. It is one of the brightest ellipticals in the Fornax galaxy cluster. NGC 1316, also known as Fornax A,

PIX4609803

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

PIX4564265

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. On the top image, the largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Saturn's left blade, on the left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. The image in the center shows the satellites Enceladus and Dione that cast their shadow on the west (left) side of Saturn, Titan in the upper right, and Mimas on the eastern edge of Saturn. In the image below, Dione and his shadow pass to the center of Saturn, above Enceladus and its shadow. Titan is on Saturn's eastern blade, Mimas is right above the rings. This sequence of images captures the parade of several of Saturn's moons trans

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. On the top image, the largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Saturn's left blade, on the left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. The image in the center shows the satellites Enceladus and Dione that cast their shadow on the west (left) side of Saturn, Titan in the upper right, and Mimas on the eastern edge of Saturn. In the image below, Dione and his shadow pass to the center of Saturn, above Enceladus and its shadow. Titan is on Saturn's eastern blade, Mimas is right above the rings. This sequence of images captures the parade of several of Saturn's moons trans

PIX4624877

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

PIX4624891

Large Binocular Telescope - The Large Binocular Telescope (LBT) consists of two large mirrors measuring 8.4m in diameter. Mount Graham, Arizona. The Large Binocular Telescope (LBT) combines two side - by - side 8 - meter telescopes. Mt. Graham in Arizona, USA

Large Binocular Telescope - The Large Binocular Telescope (LBT) consists of two large mirrors measuring 8.4m in diameter. Mount Graham, Arizona. The Large Binocular Telescope (LBT) combines two side - by - side 8 - meter telescopes. Mt. Graham in Arizona, USA

Stefan Seip

PIX4654734

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