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'Paranal' Bilder und Clips Suchergebnisse page 181 of 3

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Bilder zu 'Paranal' gefunden, 197

 
The center of our galaxy, the milky way - The center of our galaxy, the milky way - This billion pixel mosaic shows the central region of our galaxy, the Lactee Way. The 52 assembled images cover an area that extends from Sagittarius (with the galactic center and nebulae M8 and M20) on the left, to the Scorpio, with the star Antares and the colored cloud of Rho Ophiuchus on the right. Image obtained with a Takahashi FSQ 106 Ed bezel at Cerro Paranal Observatory in Chile; 200 hours of poses. This image is a 1 billion pixel RGB mosaic of the galactic center region (340 million pixels in each R, V and B color). It shows the region spanning from Sagittarius (with the Milky Way center and M8/M20 area on the left) to Scorpius (with colorful Antares and Rho Ophiuchus region on the right) and cat paw nebula (red nebula at the bottom). This mosaic was assembled from 52 different sky fields made from 1200 individual images and 200 hours total exposure time, final image size is 24000x14000 pixels

Stephane Guisard

PIX4636007

The center of our galaxy, the milky way - The center of our galaxy, the milky way - This billion pixel mosaic shows the central region of our galaxy, the Lactee Way. The 52 assembled images cover an area that extends from Sagittarius (with the galactic center and nebulae M8 and M20) on the left, to the Scorpio, with the star Antares and the colored cloud of Rho Ophiuchus on the right. Image obtained with a Takahashi FSQ 106 Ed bezel at Cerro Paranal Observatory in Chile; 200 hours of poses. This image is a 1 billion pixel RGB mosaic of the galactic center region (340 million pixels in each R, V and B color). It shows the region spanning from Sagittarius (with the Milky Way center and M8/M20 area on the left) to Scorpius (with colorful Antares and Rho Ophiuchus region on the right) and cat paw nebula (red nebula at the bottom). This mosaic was assembled from 52 different sky fields made from 1200 individual images and 200 hours total exposure time, final image size is 24000x14000 pixels

Stephane Guisard

PIX4636007

 
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

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

 
Laser shooting at the Paranal Observatory. - The VLT Laser Guide Star - View of the LGS (Laser Guide Star), a laser beam launches from the Yepun telescope (UT4) 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. 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

PIX4656888

Laser shooting at the Paranal Observatory. - The VLT Laser Guide Star - View of the LGS (Laser Guide Star), a laser beam launches from the Yepun telescope (UT4) 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. 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

PIX4656888

 
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

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

 
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

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

 
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

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

 
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

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

 
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

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

 
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

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

 
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

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

 
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

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

 
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

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

 
Milky way all around the horizon - Panorama of 360 degrees. 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 towards the right middle of the image, the galaxy of Andromede. 360 degrees panorama. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up in the sky. The Large (LMC) and Small (SMC) Magellanic clouds are visible to the left, Orion constellation with Barnard loop to the right, California Nebula and 'tiny' Andromeda galaxy to the right while the Milky Way is visible all aro

Stephane Guisard

PIX4636028

Milky way all around the horizon - Panorama of 360 degrees. 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 towards the right middle of the image, the galaxy of Andromede. 360 degrees panorama. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up in the sky. The Large (LMC) and Small (SMC) Magellanic clouds are visible to the left, Orion constellation with Barnard loop to the right, California Nebula and 'tiny' Andromeda galaxy to the right while the Milky Way is visible all aro

Stephane Guisard

PIX4636028

 
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

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

 
Milky way all around the horizon and Gegenschein - 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 towards the right middle of the image, the galaxy of Andromede. Crossing the image on the right, the gegenschein, the blade glow made up of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. The bright spot near the center of the image is Jupiter Planet. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up i

Stephane Guisard

PIX4636032

Milky way all around the horizon and Gegenschein - 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 towards the right middle of the image, the galaxy of Andromede. Crossing the image on the right, the gegenschein, the blade glow made up of dust reflecting the light of the sun, observable only in a dense sky of any parasite light. The bright spot near the center of the image is Jupiter Planet. The following image was taken at new Moon (No Moon light), middle of the night (minimum zodiacal light effect), in the Atacama desert close to Paranal observatory (no light pollution). The chosen place for this picture has the particularity to be located at a latitude which value is close to the declination of the galactic southern pole. The picture was therefore also taken when the galactic pole passes at zenith, ensuring that there is no Milky Way up i

Stephane Guisard

PIX4636032

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