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McNaught Comet McNaught - View of McNaught Comet in January 2007 in Chile. On the left, a laser shot from the Paranal Observatory. Comet McNaught (C/2006 P1) with laser beam from Paranal observatory in Chile. January 2007

McNaught Comet McNaught - View of McNaught Comet in January 2007 in Chile. On the left, a laser shot from the Paranal Observatory. Comet McNaught (C/2006 P1) with laser beam from Paranal observatory in Chile. January 2007

Guillaume Blanchard

PIX4570558

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

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

PIX4656715

La comete Lovejoy - December 2011 - Comet Lovejoy - December 2011 - La comete Lovejoy seen at the Paranal Observatory in Chile on December 23, 2011. Comet Lovejoy seen from Paranal observatory in Chile on Dec. 23, 2011

La comete Lovejoy - December 2011 - Comet Lovejoy - December 2011 - La comete Lovejoy seen at the Paranal Observatory in Chile on December 23, 2011. Comet Lovejoy seen from Paranal observatory in Chile on Dec. 23, 2011

PIX4571224

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

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

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

PIX4656710

Telescope of 8,2m ANTU - The 8,2m telescope Antu.: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

Telescope of 8,2m ANTU - The 8,2m telescope Antu.: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

PIX4656627

Paranal Observatory. - Paranal Observatory, Chile - One of the Auxilliary Telescopes measuring 1.8m in diameter. One of the VLTI auxiliary telescope

Paranal Observatory. - Paranal Observatory, Chile - One of the Auxilliary Telescopes measuring 1.8m in diameter. One of the VLTI auxiliary telescope

Guillaume Blanchard

PIX4656809

The McNaught Comet at the Paranal Observatory - Comet McNaught over Paranal Observatory - View of the McNaught Comet obtained on January 19, 2007 above the VLT in Chile. Comet McNaught (C/2006 P1) as seen over Very Large Telescope, Chile, on January 19 2007

The McNaught Comet at the Paranal Observatory - Comet McNaught over Paranal Observatory - View of the McNaught Comet obtained on January 19, 2007 above the VLT in Chile. Comet McNaught (C/2006 P1) as seen over Very Large Telescope, Chile, on January 19 2007

Guillaume Blanchard

PIX4570574

Paranal Observatory, Chile - Paranal and the Full Moon: The Very Large Telescope (VLT) seen on 11 August 2014 lit by the full moon. The full Moon shines over the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Paranal Observatory, Chile - Paranal and the Full Moon: The Very Large Telescope (VLT) seen on 11 August 2014 lit by the full moon. The full Moon shines over the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657499

The McNaught comet at the Paranal Observatory - Comet McNaught over Paranal observatory - View of the McNaught comet obtained on January 19, 2007 in Chile. In the foreground, one of the auxiliary telescopes of the Paranal Observatory. Comet McNaught (C/2006 P1) as seen over Paranal observatory, Chile, on January 19 2007

The McNaught comet at the Paranal Observatory - Comet McNaught over Paranal observatory - View of the McNaught comet obtained on January 19, 2007 in Chile. In the foreground, one of the auxiliary telescopes of the Paranal Observatory. Comet McNaught (C/2006 P1) as seen over Paranal observatory, Chile, on January 19 2007

Guillaume Blanchard

PIX4570585

Circumpolar - Cerro Paranal - Hemisphere South - Circumpolar above Cerro Paranal observatory - 10h photographic pose around the southern Celeste pole. The glows of twilight on the right and dawn on the left are visible. In the foreground, the domes of the VLT. Cerro Paranal observatory from twilight (right) to dawn (left). 10 hours exposure

Circumpolar - Cerro Paranal - Hemisphere South - Circumpolar above Cerro Paranal observatory - 10h photographic pose around the southern Celeste pole. The glows of twilight on the right and dawn on the left are visible. In the foreground, the domes of the VLT. Cerro Paranal observatory from twilight (right) to dawn (left). 10 hours exposure

Stephane Guisard

PIX4581255

Paranal Observatory, Chile: The Very Large Telescope (VLT) and its auxiliary telescopes seen on August 9, 2014. In the sky the galaxy of Andromede is visible. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Paranal Observatory, Chile: The Very Large Telescope (VLT) and its auxiliary telescopes seen on August 9, 2014. In the sky the galaxy of Andromede is visible. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657492

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Stephane Guisard

PIX4657141

Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657504

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Stephane Guisard

PIX4657134

Chile, Antofagasta Region, Atacama Desert, Paranal Observatory, operated by European Southern Observatory (ESO), view of Very Large Telescope (VLT)

Chile, Antofagasta Region, Atacama Desert, Paranal Observatory, operated by European Southern Observatory (ESO), view of Very Large Telescope (VLT)

UDK844342

Moon and planets above the Paranal Observatory - Paranal Observatory, Venus - Mercury - Mars - Moon conjunction - The Moon with the Venus planets (the brightest at the bottom right of the Moon), Mercury (to the right of the Moon) and Mars (to the top right of the Moon), seen on 1 September 2008 at the Paranal Observatory in Chile. Moon - Venus - Mercury - Mars conjunction in twilight. Paranal Observatory, Chile. Sep 1st 2008

Moon and planets above the Paranal Observatory - Paranal Observatory, Venus - Mercury - Mars - Moon conjunction - The Moon with the Venus planets (the brightest at the bottom right of the Moon), Mercury (to the right of the Moon) and Mars (to the top right of the Moon), seen on 1 September 2008 at the Paranal Observatory in Chile. Moon - Venus - Mercury - Mars conjunction in twilight. Paranal Observatory, Chile. Sep 1st 2008

Stephane Guisard

PIX4657158

Paranal Observatory, Chile - Paranal Observatory, Chile - Yepun, one of the four 8.2m telescopes of the VLT (Very Large Telescope), and two of the four 1.8m auxiliary telescopes. On the horizon, the shadow of the Earth projected on the atmosphere, the belt of Venus (or anticrepuscular arch). January 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. This picture shows at left Yepun, one of the four 8,2m telescopes of the Very Large Telescope (VLT), with two auxiliary telescopes. Visible too, the anticrepuscular arch (or belt of Venus, the shadow of earth projected in the atmosphere) January 2008

Paranal Observatory, Chile - Paranal Observatory, Chile - Yepun, one of the four 8.2m telescopes of the VLT (Very Large Telescope), and two of the four 1.8m auxiliary telescopes. On the horizon, the shadow of the Earth projected on the atmosphere, the belt of Venus (or anticrepuscular arch). January 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. This picture shows at left Yepun, one of the four 8,2m telescopes of the Very Large Telescope (VLT), with two auxiliary telescopes. Visible too, the anticrepuscular arch (or belt of Venus, the shadow of earth projected in the atmosphere) January 2008

Guillaume Blanchard

PIX4657124

8.2 m telescope (VLT) of ESO - Paranal observatory. Very Large Telescope (VLT). - The Cerro Paranal Observatory in Chile has been hosting the European VLT (Very Large Telescope) network since 1998. The European Southern Observatory (ESO) here uses four telescopes measuring 8.2 m in diameter, as well as telescopes measuring 1.8 m to 4 m in diameter: it is the largest observatory in the world. Cerro Paranal is located at 2500 m above sea level, in the Atacama desert. View of one of the 4 8.2m telescopes of the VLT, Very Large Telescope. The european southern observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. Cerro Paranal is 2500 meters in altitude in Atacama desert. Wide - angle view of the structure of one of the 8.2 - m VLT Unit Telescope

8.2 m telescope (VLT) of ESO - Paranal observatory. Very Large Telescope (VLT). - The Cerro Paranal Observatory in Chile has been hosting the European VLT (Very Large Telescope) network since 1998. The European Southern Observatory (ESO) here uses four telescopes measuring 8.2 m in diameter, as well as telescopes measuring 1.8 m to 4 m in diameter: it is the largest observatory in the world. Cerro Paranal is located at 2500 m above sea level, in the Atacama desert. View of one of the 4 8.2m telescopes of the VLT, Very Large Telescope. The european southern observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. Cerro Paranal is 2500 meters in altitude in Atacama desert. Wide - angle view of the structure of one of the 8.2 - m VLT Unit Telescope

Serge Brunier

PIX4657551

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. The Very Large Telescope (VLT) and auxiliary telescopes. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama desert in the northern part of Chile. March 2008

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. The Very Large Telescope (VLT) and auxiliary telescopes. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama desert in the northern part of Chile. March 2008

Stephane Guisard

PIX4657128

Satellite Dish (photo)

Satellite Dish (photo)

UIG2915875

Moon, planets and zodiacal light - Paranal observatory - Paranal observatory, Moon, planets and zodiacal light - Near the horizon, the Moon with Venus planets (the brightest at the bottom right of the Moon), Mercury (on the right of the Moon) and Mars (on the top right of the Moon); above, the zodiacal light. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plan of the Solar System. September 1, 2008 at the Paranal Observatory in Chile. Moon - Venus - Mercury - Mars conjunction near the horizon. Above is zodiacal light. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. Paranal Observatory, Chile. Sep 1st 2008

Moon, planets and zodiacal light - Paranal observatory - Paranal observatory, Moon, planets and zodiacal light - Near the horizon, the Moon with Venus planets (the brightest at the bottom right of the Moon), Mercury (on the right of the Moon) and Mars (on the top right of the Moon); above, the zodiacal light. The zodiacal light comes from the reflection of the Sun's light on the countless interplanetary dust; it draws the plan of the Solar System. September 1, 2008 at the Paranal Observatory in Chile. Moon - Venus - Mercury - Mars conjunction near the horizon. Above is zodiacal light. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. Paranal Observatory, Chile. Sep 1st 2008

Stephane Guisard

PIX4657164

Satellite Dish And European Southern Observatory Vlt Observatory (photo)

Satellite Dish And European Southern Observatory Vlt Observatory (photo)

UIG2915868

Paranal Observatory, Chile - Sunrise at VLT - Paranal Observatory, Chile: The Very Large Telescope (VLT) and an auxiliary telescope seen at the end of the night on August 9, 2014. In the sky the galaxy of Andromede is visible. The morning has arrived at the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode

Paranal Observatory, Chile - Sunrise at VLT - Paranal Observatory, Chile: The Very Large Telescope (VLT) and an auxiliary telescope seen at the end of the night on August 9, 2014. In the sky the galaxy of Andromede is visible. The morning has arrived at the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode

Alex Tudorica

PIX4657511

The zodiacal light and the Paranal observatory - Paranal observatory with zodiacal light - Star sky above the Paranal observatory. On the left, on the horizon, the constellation of Orion. Above a shooting star and the lactee. The glow in the center of the image is the zodiacal light; it comes from the reflection of the Sun's light on the countless interplanetary dust and draws the plane of the Solar System. May 2009. Starry sky above Paranal observatory. Light behind the observatory is the zodiacal light; it comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. A faint meteor is also visible. May 2009

The zodiacal light and the Paranal observatory - Paranal observatory with zodiacal light - Star sky above the Paranal observatory. On the left, on the horizon, the constellation of Orion. Above a shooting star and the lactee. The glow in the center of the image is the zodiacal light; it comes from the reflection of the Sun's light on the countless interplanetary dust and draws the plane of the Solar System. May 2009. Starry sky above Paranal observatory. Light behind the observatory is the zodiacal light; it comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. A faint meteor is also visible. May 2009

Stephane Guisard

PIX4657178

Paranal Observatory - Chile - Paranal Observatory - Chile - The lactee road above the Paranal Observatory in Chile. The road leading to the observatory is equipped with solar energy lighting that preserves the night sky from light pollution. 1 September 2008. Milky way above Paranal observatory, Chile. Sep 1st 2008. The road to the observatory is lightened by solar powered leds to avoid light pollution

Paranal Observatory - Chile - Paranal Observatory - Chile - The lactee road above the Paranal Observatory in Chile. The road leading to the observatory is equipped with solar energy lighting that preserves the night sky from light pollution. 1 September 2008. Milky way above Paranal observatory, Chile. Sep 1st 2008. The road to the observatory is lightened by solar powered leds to avoid light pollution

Stephane Guisard

PIX4657160

Laser shooting at the Paranal Observatory - The VLT Laser Guide Star - View from the LGS (Laser Guide Star), a laser beam launches from the Yepun (UT4) telescope of the VLT. This laser creates an artificial star in the high atmosphere at about 90 km altitude. This repere is analysed and each variation of turbulence in the atmosphere is detected and corrected by the adaptive optics of the telescope. On the left, the two galaxies of the Magellan Cloud, on the right, the dome of the VST (VLT Survey Telescope). A 50 cm wide yellow laser beam is coming out of Yepun, (UT4) of the Very Large Telescope. It is used to create a yellow artificial star at 95 km of altitude which helps the adaptive optics to measure and correct the atmosphere's blurring effect. On the left, the two Magellanic Clouds, on the right, the VST dome

Laser shooting at the Paranal Observatory - The VLT Laser Guide Star - View from the LGS (Laser Guide Star), a laser beam launches from the Yepun (UT4) telescope of the VLT. This laser creates an artificial star in the high atmosphere at about 90 km altitude. This repere is analysed and each variation of turbulence in the atmosphere is detected and corrected by the adaptive optics of the telescope. On the left, the two galaxies of the Magellan Cloud, on the right, the dome of the VST (VLT Survey Telescope). A 50 cm wide yellow laser beam is coming out of Yepun, (UT4) of the Very Large Telescope. It is used to create a yellow artificial star at 95 km of altitude which helps the adaptive optics to measure and correct the atmosphere's blurring effect. On the left, the two Magellanic Clouds, on the right, the VST dome

Stephane Guisard

PIX4656905

Venus, Jupiter and the zodiacal light - Paranal observatory - Paranal observatory, Venus, Jupiter and zodiacal light - Conjunction Venus Jupiter on November 28, 2008. The lactee path is visible on the horizon. The glow around the two planets is the zodiacal light; it comes from the reflection of the Sun's light on the countless interplanetary dust and draws the plane of the Solar System. Paranal Observatory in Chile. Venus Jupiter conjunction with zodiacal light. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. Milky way is visible near horizon. Paranal Observatory, Chile. November 28 2008

Venus, Jupiter and the zodiacal light - Paranal observatory - Paranal observatory, Venus, Jupiter and zodiacal light - Conjunction Venus Jupiter on November 28, 2008. The lactee path is visible on the horizon. The glow around the two planets is the zodiacal light; it comes from the reflection of the Sun's light on the countless interplanetary dust and draws the plane of the Solar System. Paranal Observatory in Chile. Venus Jupiter conjunction with zodiacal light. Zodiacal light comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. Milky way is visible near horizon. Paranal Observatory, Chile. November 28 2008

Stephane Guisard

PIX4657165

Perseid Meteor above Paranal observatory - A brilliant shooting star (Perseide) passes over the domes of the VLT to the Paranal observatory. Perseid meteor passing above Paranal observatory. The four main (8m diameter mirrors) telescope are opened and observing. Two small (1.8m diameter mirror) auxiliary telescopes are also completely opened and doing interferometric observations. The domes are lit by the Moon that is setting outside the left hand side of the picture

Perseid Meteor above Paranal observatory - A brilliant shooting star (Perseide) passes over the domes of the VLT to the Paranal observatory. Perseid meteor passing above Paranal observatory. The four main (8m diameter mirrors) telescope are opened and observing. Two small (1.8m diameter mirror) auxiliary telescopes are also completely opened and doing interferometric observations. The domes are lit by the Moon that is setting outside the left hand side of the picture

Stephane Guisard

PIX4657228

Paranal Observatory - Chile - Aerienne view of the VLT, Very Large Telescope, consists of 4 main telescopes measuring 8.2m in diameter. This photo obtained in December 1999 also shows the foundations of future 1.8m auxilliary telescopes

Paranal Observatory - Chile - Aerienne view of the VLT, Very Large Telescope, consists of 4 main telescopes measuring 8.2m in diameter. This photo obtained in December 1999 also shows the foundations of future 1.8m auxilliary telescopes

PIX4657505

Paranal Observatory - Chile - Paranal Observatory - Chile - The lactee road above the Paranal Observatory in Chile. The road leading to the observatory is equipped with solar energy lighting that preserves the night sky from light pollution. On the right, the light halo of the city of Antofagasta, 120 km from the. 1 September 2008. Milky way above Paranal observatory, Chile. Sep 1st 2008. The road to the observatory is lightened by solar powered leds to avoid light pollution. At right, light pollution from the city of Antofagasta, 120 km away

Paranal Observatory - Chile - Paranal Observatory - Chile - The lactee road above the Paranal Observatory in Chile. The road leading to the observatory is equipped with solar energy lighting that preserves the night sky from light pollution. On the right, the light halo of the city of Antofagasta, 120 km from the. 1 September 2008. Milky way above Paranal observatory, Chile. Sep 1st 2008. The road to the observatory is lightened by solar powered leds to avoid light pollution. At right, light pollution from the city of Antofagasta, 120 km away

Stephane Guisard

PIX4657167

Lactee route au raz de l'horizon - Paranal horizon in the milky way plane - Fisheye view of the southern sky. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it to the top right of the image, the galaxy of Andromede. A laser shot from one of the domes of the VLT is visible as well as the gegenschein, the blade glow consisting of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. A fish-eye view of southern sky in Chile. Milky way is visible along the 360 degrees of the horizon line. Also visible are Gegenschein at zenith, Paranal observatory with Laser Guide Star, and the three brightest galaxies visible on earth (the large Magellanic clouds and Andromeda galaxy)

Lactee route au raz de l'horizon - Paranal horizon in the milky way plane - Fisheye view of the southern sky. The lactee path blends with the horizon line. In the sky, the three brightest galaxies visible on Earth: the two galaxies of the Magellan Cloud, and opposite it to the top right of the image, the galaxy of Andromede. A laser shot from one of the domes of the VLT is visible as well as the gegenschein, the blade glow consisting of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. A fish-eye view of southern sky in Chile. Milky way is visible along the 360 degrees of the horizon line. Also visible are Gegenschein at zenith, Paranal observatory with Laser Guide Star, and the three brightest galaxies visible on earth (the large Magellanic clouds and Andromeda galaxy)

Stephane Guisard

PIX4635912

Composite image of galaxy cluster Abell 2052 (photo)

Composite image of galaxy cluster Abell 2052 (photo)

SMT1217246

Star sky on the Paranal observatory - Starry Sky above Paranal observatory - Spherical panorama of the star sky above the Paranal observatory in Chile. The lactee route crosses the sky accompanied by zodiacal light. May 2009. Milky Way is crossing Paranal sky and meeting with Zodiacal light to the West behind Paranal Observatory. Three of the most emblematic constellations are visible on the horizon: Orion, Big deeper and Scorpius. The Large and Small magellanic clouds are visible to the South together with Southern Cross, Eta Carina nebula and Coal sack. May 2009

Star sky on the Paranal observatory - Starry Sky above Paranal observatory - Spherical panorama of the star sky above the Paranal observatory in Chile. The lactee route crosses the sky accompanied by zodiacal light. May 2009. Milky Way is crossing Paranal sky and meeting with Zodiacal light to the West behind Paranal Observatory. Three of the most emblematic constellations are visible on the horizon: Orion, Big deeper and Scorpius. The Large and Small magellanic clouds are visible to the South together with Southern Cross, Eta Carina nebula and Coal sack. May 2009

Stephane Guisard

PIX4657215

Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

UIG2915879

Truck Used To Transport Vlt Mirrors (photo)

Truck Used To Transport Vlt Mirrors (photo)

UIG2915867

Paranal Observatory - Chile - Paranal Observatory - Chile - The lactee road above the Paranal Observatory in Chile. 360 degree Panorama of ESO - Paranal Observatory platform. The four 8m (UT) and four 1.8 m (AT) diameter telescopes of the VLT are all observing under the Milky Way arch during this very dark Southern hemisphere spring night. The large (LMC) and small (SMC) Magellanic clouds are visible to the left of the picture while another galaxy, Andromeda Galaxy (M31) is also visible just to the right of UT4. Bright Jupiter is high in the sky. The picture also shows two 'astronomical' lights, the zodiacal light crossing the Milky Way center vertically (just at the left of the middle of the image, above AT3) and the Gegenschein, usually very difficult to observe, below Jupiter on the right hand side of the image

Paranal Observatory - Chile - Paranal Observatory - Chile - The lactee road above the Paranal Observatory in Chile. 360 degree Panorama of ESO - Paranal Observatory platform. The four 8m (UT) and four 1.8 m (AT) diameter telescopes of the VLT are all observing under the Milky Way arch during this very dark Southern hemisphere spring night. The large (LMC) and small (SMC) Magellanic clouds are visible to the left of the picture while another galaxy, Andromeda Galaxy (M31) is also visible just to the right of UT4. Bright Jupiter is high in the sky. The picture also shows two 'astronomical' lights, the zodiacal light crossing the Milky Way center vertically (just at the left of the middle of the image, above AT3) and the Gegenschein, usually very difficult to observe, below Jupiter on the right hand side of the image

Stephane Guisard

PIX4657246

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

UIG2915877

Sun Unit Telescope 1, Moon Unit Telescope 2 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2 (photo)

UIG2915878

Dome From The Inside Of The Paranal Residence (photo)

Dome From The Inside Of The Paranal Residence (photo)

UIG2918449

Star sky on the Paranal observatory - Legendee version - Starry Sky above Paranal observatory - Annotated - Spherical panorama of the star sky above the Paranal observatory in Chile. The lactee route crosses the sky accompanied by zodiacal light. May 2009. The constellations are traced and their names are indicated. Milky Way is crossing Paranal sky and meeting with Zodiacal light to the West behind Paranal Observatory. Three of the most emblematic constellations are visible on the horizon: Orion, Big deeper and Scorpius. The Large and Small magellanic clouds are visible to the South together with Southern Cross, Eta Carina nebula and Coal sack. May 2009. Constellations are drawn with their names written

Star sky on the Paranal observatory - Legendee version - Starry Sky above Paranal observatory - Annotated - Spherical panorama of the star sky above the Paranal observatory in Chile. The lactee route crosses the sky accompanied by zodiacal light. May 2009. The constellations are traced and their names are indicated. Milky Way is crossing Paranal sky and meeting with Zodiacal light to the West behind Paranal Observatory. Three of the most emblematic constellations are visible on the horizon: Orion, Big deeper and Scorpius. The Large and Small magellanic clouds are visible to the South together with Southern Cross, Eta Carina nebula and Coal sack. May 2009. Constellations are drawn with their names written

Stephane Guisard

PIX4657189

The VISTA telescope - Chile - The VISTA telecope - Chile: The dome of the 4.1m VISTA telescope seen from the VLT, in the Atacama desert in Chile. The Vista, 4.1 meter wide-field telescope for Infrared survey seen from VLT in Atacama Desert.

The VISTA telescope - Chile - The VISTA telecope - Chile: The dome of the 4.1m VISTA telescope seen from the VLT, in the Atacama desert in Chile. The Vista, 4.1 meter wide-field telescope for Infrared survey seen from VLT in Atacama Desert.

Alex Tudorica

PIX4657630

La comete Lovejoy - December 2011 - Comet Lovejoy - December 2011 - La comete Lovejoy seen at the Paranal Observatory in Chile on December 23, 2011. Comet Lovejoy seen from Paranal observatory in Chile on Dec. 23, 2011

La comete Lovejoy - December 2011 - Comet Lovejoy - December 2011 - La comete Lovejoy seen at the Paranal Observatory in Chile on December 23, 2011. Comet Lovejoy seen from Paranal observatory in Chile on Dec. 23, 2011

PIX4571209

Barred spiral galaxy NGC 1398 in the Furnace: The galaxy NGC 1398 is located at a distance of about 65 million light years. Image obtained by the VLT telescope. This galaxy is located in the constellation of Fornax (The Furnace), approximately 65 million light-years away. This image comprises data gathered by the Focal Reducer/low dispersion Spectrograph 2 (FORS2) instrument, mounted on Eso's Very Large Telescope (VLT) at Paranal Observatory, Chile. It shows NGC 1398 in striking detail, from the dark lanes of dust mottling its spiral arms, through to the pin-hued star-forming regions sprinkled throughout its outer regions.

Barred spiral galaxy NGC 1398 in the Furnace: The galaxy NGC 1398 is located at a distance of about 65 million light years. Image obtained by the VLT telescope. This galaxy is located in the constellation of Fornax (The Furnace), approximately 65 million light-years away. This image comprises data gathered by the Focal Reducer/low dispersion Spectrograph 2 (FORS2) instrument, mounted on Eso's Very Large Telescope (VLT) at Paranal Observatory, Chile. It shows NGC 1398 in striking detail, from the dark lanes of dust mottling its spiral arms, through to the pin-hued star-forming regions sprinkled throughout its outer regions.

PIX4609909

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. Image obtained with the VLT in Chile. This picture of the nearby galaxy NGC 3521 was taken using the FORS1 instrument on Eso's Very Large Telescope, at the Paranal Observatory in Chile. The large spiral galaxy lies in the constellation of Leo (The Lion), and is only 35 million light - years distant. This picture was created from exposures taken through three different filters that passed blue light, yellow/green light, and near - infrared light. These are shown in this picture as blue, green, and red, respectively

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. Image obtained with the VLT in Chile. This picture of the nearby galaxy NGC 3521 was taken using the FORS1 instrument on Eso's Very Large Telescope, at the Paranal Observatory in Chile. The large spiral galaxy lies in the constellation of Leo (The Lion), and is only 35 million light - years distant. This picture was created from exposures taken through three different filters that passed blue light, yellow/green light, and near - infrared light. These are shown in this picture as blue, green, and red, respectively

PIX4610741

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

PIX4574313

Spiral Galaxy NGC 253 - NGC 253 is the brightest galaxy in the Sculptor's group, the closest galaxy group to the Local Group. It is about 13 million light years away. Composite image obtained from the Hubble sptial telescope, the Subaru, VLT and the 1.5m Danish telescopes. NGC 253 is a large, almost edge - on spiral galaxy, and is one of the nearest galaxies beyond our local neighborhood of galaxies. In this image taken by Hubble space telescope thousands of individual stars are resolved in this galaxy located 13 million light years away.Multipanel Mosaic and Composite from Four Data Sources 8.2 Meter Subaru Telescope, Hubble Space Telescope European Southern Observatory (VLT and Danish 1.5M

Spiral Galaxy NGC 253 - NGC 253 is the brightest galaxy in the Sculptor's group, the closest galaxy group to the Local Group. It is about 13 million light years away. Composite image obtained from the Hubble sptial telescope, the Subaru, VLT and the 1.5m Danish telescopes. NGC 253 is a large, almost edge - on spiral galaxy, and is one of the nearest galaxies beyond our local neighborhood of galaxies. In this image taken by Hubble space telescope thousands of individual stars are resolved in this galaxy located 13 million light years away.Multipanel Mosaic and Composite from Four Data Sources 8.2 Meter Subaru Telescope, Hubble Space Telescope European Southern Observatory (VLT and Danish 1.5M

PIX4609126

Spiral galaxy NGC 7793 in the Sculptor - Spiral galaxy NGC 7793 in Sculptor - The spiral galaxy NGC 7793 is located 12 million years ago - light from Earth and resides in a grouping of several galaxies called the Sculptor's group. Image obtained with one of the telescopes of the VLT in Chile. NGC 7793 is at a distance of about 12 million light years; it is a member of the Sculptor group, where the galaxies are few in number and well separated in space. Image taken with one of the workhorses of the ESO Paranal Observatory, the FORS instrument, attached to the Very Large Telescope

Spiral galaxy NGC 7793 in the Sculptor - Spiral galaxy NGC 7793 in Sculptor - The spiral galaxy NGC 7793 is located 12 million years ago - light from Earth and resides in a grouping of several galaxies called the Sculptor's group. Image obtained with one of the telescopes of the VLT in Chile. NGC 7793 is at a distance of about 12 million light years; it is a member of the Sculptor group, where the galaxies are few in number and well separated in space. Image taken with one of the workhorses of the ESO Paranal Observatory, the FORS instrument, attached to the Very Large Telescope

PIX4613237

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Image obtained with the ANTU telescope of the VLT on January 30, 2000. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant. This image was obtained with FORS1 instrument on ANTU telescope at Paranal observatory on January 30 2000

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Image obtained with the ANTU telescope of the VLT on January 30, 2000. The light from this remarkable spiral system is dominated by the billions of old, faint stars that form the vast 'bulge' around its tiny hidden nucleus. Most spirals, including the Milky Way, have clouds of old, faint stars around their nuclei, but in M104 the galaxy's light is dominated by them. This effect is enhanced because disk of the galaxy is seen nearly edge - on and dust in its outer parts is in silhouette as it crosses the picture. The galaxy is about 28 million light years distant. This image was obtained with FORS1 instrument on ANTU telescope at Paranal observatory on January 30 2000

PIX4611598

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

Unit Telescopes And Auxiliary Telescopes (photo)

Unit Telescopes And Auxiliary Telescopes (photo)

UIG2915874

Unit Telescopes And Auxiliary Telescopes (photo)

Unit Telescopes And Auxiliary Telescopes (photo)

UIG2915873

Mechanical Structure Of Moon Unit Telescope 2 (photo)

Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915887

Mechanical Structure Of Moon Unit Telescope 2 (photo)

Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915886

Mechanical Structure Of Moon Unit Telescope 2 (photo)

Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915895

Moon Unit Telescope 2 (photo)

Moon Unit Telescope 2 (photo)

UIG2915904

Unit Telescopes And Auxiliary Telescopes (photo)

Unit Telescopes And Auxiliary Telescopes (photo)

UIG2915872

Mechanical Structure Of Moon Unit Telescope 2 (photo)

Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915885

Moon Unit Telescope 2 (photo)

Moon Unit Telescope 2 (photo)

UIG2915906

Mechanical Structure Of Moon Unit Telescope 2 (photo)

Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915890

Mechanical Structure Containing The 82 Meter Mirror Of Moon Unit Telescope 2 (photo)

Mechanical Structure Containing The 82 Meter Mirror Of Moon Unit Telescope 2 (photo)

UIG2915889

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

Mechanical Structure Of Moon Unit Telescope 2 (photo)

Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915898

Southern Cross Unit Telescope 3 (photo)

Southern Cross Unit Telescope 3 (photo)

UIG2915900

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

Mechanical Structure Of Moon Unit Telescope 2 (photo)

Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915888

Mechanical Structure Containing The 82 Meter Mirror Of Moon Unit Telescope 2 (photo)

Mechanical Structure Containing The 82 Meter Mirror Of Moon Unit Telescope 2 (photo)

UIG2915891

Center of the Orion Nebula - Trapeze - Orion nebula center - Mosaic of infrared images showing the center of the Orion Nebula, the Trapeze region. 4 massive stars form the Trapeze but the image also shows the cluster of stars associated with it, constitutes a thousand stars of about 1 million years old. Mosaic of 81 infrared images obtained by the ISAAC instrument at the VLT. Colour composite mosaic image of the central part of the Orion Nebula, based on 81 images obtained with the infrared multi - mode ISAAC instrument on the ESO Very Large Telescope (VLT) at the Paranal Observatory. The famous Trapezium stars are seen near the centre and the photo also shows the associated cluster of about one thousand stars, about a million years old

Center of the Orion Nebula - Trapeze - Orion nebula center - Mosaic of infrared images showing the center of the Orion Nebula, the Trapeze region. 4 massive stars form the Trapeze but the image also shows the cluster of stars associated with it, constitutes a thousand stars of about 1 million years old. Mosaic of 81 infrared images obtained by the ISAAC instrument at the VLT. Colour composite mosaic image of the central part of the Orion Nebula, based on 81 images obtained with the infrared multi - mode ISAAC instrument on the ESO Very Large Telescope (VLT) at the Paranal Observatory. The famous Trapezium stars are seen near the centre and the photo also shows the associated cluster of about one thousand stars, about a million years old

PIX4617863

The Last Rays Of The Sun Illuminate Part Of The Mechanical Structure Of Moon Unit Telescope 2 (photo)

The Last Rays Of The Sun Illuminate Part Of The Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915892

The Last Rays Of The Sun Illuminate Part Of The Mechanical Structure Of Moon Unit Telescope 2 (photo)

The Last Rays Of The Sun Illuminate Part Of The Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915893

The Last Rays Of The Sun Illuminate Part Of The Mechanical Structure Of Moon Unit Telescope 2 (photo)

The Last Rays Of The Sun Illuminate Part Of The Mechanical Structure Of Moon Unit Telescope 2 (photo)

UIG2915894

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

UIG2915905

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

UIG2915903

Southern Cross Unit Telescope 3 & Moon Unit Telescope 2 (photo)

Southern Cross Unit Telescope 3 & Moon Unit Telescope 2 (photo)

UIG2915884

Auxiliary Telescopes, Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

Auxiliary Telescopes, Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

UIG2915882

Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

UIG2915902

Antu (Sun) Unit Telescope 1 (photo)

Antu (Sun) Unit Telescope 1 (photo)

UIG2915899

Control Center & Antu (Sun) Unit Telescope 1 (photo)

Control Center & Antu (Sun) Unit Telescope 1 (photo)

UIG2915869

Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

UIG2915883

Auxiliary Telescope, Sun Unit Telescope 1, Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

Auxiliary Telescope, Sun Unit Telescope 1, Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

UIG2915910

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

UIG2915897

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

UIG2915896

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

UIG2915909

Paranal Observatory - The VLT - Paranal Observatory - The VLT - View of the 4 8.2m telescopes of the VLT, Very Large Telescope, at the top of Cerro Paranal in Chile

Paranal Observatory - The VLT - Paranal Observatory - The VLT - View of the 4 8.2m telescopes of the VLT, Very Large Telescope, at the top of Cerro Paranal in Chile

E. Perrin

PIX4656668

Paranal Observatory - The VLT - Paranal Observatory - The VLT - View of the 4 8.2m telescopes of the VLT, Very Large Telescope, at the top of Cerro Paranal in Chile

Paranal Observatory - The VLT - Paranal Observatory - The VLT - View of the 4 8.2m telescopes of the VLT, Very Large Telescope, at the top of Cerro Paranal in Chile

E. Perrin

PIX4656669

European 8.2 m telescope (VLT) - Paranal observatory. Very Large Telescope (VLT). - The Cerro Paranal Observatory in Chile has been hosting the European VLT (Very Large Telescope) network since 1998. The European Southern Observatory (ESO) here uses four telescopes measuring 8.2 m in diameter, as well as telescopes measuring 1.8 m to 4 m in diameter: it is the largest observatory in the world. Cerro Paranal is located at 2500 m above sea level, in the Atacama.View of one of the 4 8.2m telescopes of the VLT, Very Large Telescope. The european southern observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. Cerro Paranal is 2500 meters in altitude in Atacama desert. Wide - angle view of the structure of one of the 8.2 - m VLT Unit Telescope

European 8.2 m telescope (VLT) - Paranal observatory. Very Large Telescope (VLT). - The Cerro Paranal Observatory in Chile has been hosting the European VLT (Very Large Telescope) network since 1998. The European Southern Observatory (ESO) here uses four telescopes measuring 8.2 m in diameter, as well as telescopes measuring 1.8 m to 4 m in diameter: it is the largest observatory in the world. Cerro Paranal is located at 2500 m above sea level, in the Atacama.View of one of the 4 8.2m telescopes of the VLT, Very Large Telescope. The european southern observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. Cerro Paranal is 2500 meters in altitude in Atacama desert. Wide - angle view of the structure of one of the 8.2 - m VLT Unit Telescope

Serge Brunier

PIX4657539

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