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Bilder zu 'AT3' gefunden, 13

Amateur astronomer - Amateur astronomer - Amateur astronomer at the Paranal Observatory in Chile. FS128 bezel. Amateur astronomer at Paranal observatory in Chile. Takahashi FS128 refractor

Amateur astronomer - Amateur astronomer - Amateur astronomer at the Paranal Observatory in Chile. FS128 bezel. Amateur astronomer at Paranal observatory in Chile. Takahashi FS128 refractor

Stephane Guisard

PIX4566132

Astronomical bezel - Refracting telescope - Takahashi FS128 - Paranal Observatory in Chile. Takahashi FS128 refractor, Paranal observatory in Chile

Astronomical bezel - Refracting telescope - Takahashi FS128 - Paranal Observatory in Chile. Takahashi FS128 refractor, Paranal observatory in Chile

Stephane Guisard

PIX4566146

Comete 17P/Holmes - Comet 17P/Holmes - View of comete 17P/Holmes beginning November 2007 from the Paranal Observatory in Chile. In the foreground, one of the 1.8m diameter auxilliary telescopes. On October 24, 2007, Comete 17P/Holmes suddenly increased luminosite and became visible to the naked eye. Comet 17P/Holmes is seen here from Paranal observatory in Chile. Foreground is one of the 1,8m auxilliary telescope. Comet 17P/Holmes began a spectacular outburst in brightness on October 24th, brightening from 17th magnitude to 2.5th magnitude, an increase of more than 1 million times brighter to become a unaided - eye object in the constellation of Perseus

Comete 17P/Holmes - Comet 17P/Holmes - View of comete 17P/Holmes beginning November 2007 from the Paranal Observatory in Chile. In the foreground, one of the 1.8m diameter auxilliary telescopes. On October 24, 2007, Comete 17P/Holmes suddenly increased luminosite and became visible to the naked eye. Comet 17P/Holmes is seen here from Paranal observatory in Chile. Foreground is one of the 1,8m auxilliary telescope. Comet 17P/Holmes began a spectacular outburst in brightness on October 24th, brightening from 17th magnitude to 2.5th magnitude, an increase of more than 1 million times brighter to become a unaided - eye object in the constellation of Perseus

Stephane Guisard

PIX4570953

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

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

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

Amateur astronomer - Amateur astronomer - Amateur astronomer at the Paranal Observatory in Chile. FS128 bezel. Amateur astronomer at Paranal observatory in Chile. Takahashi FS128 refractor

Amateur astronomer - Amateur astronomer - Amateur astronomer at the Paranal Observatory in Chile. FS128 bezel. Amateur astronomer at Paranal observatory in Chile. Takahashi FS128 refractor

Stephane Guisard

PIX4566140

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

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

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

Children playing, June 1954 (b/w photo) [2012/001/6/7/AT3]

Children playing, June 1954 (b/w photo) [2012/001/6/7/AT3]

BRV3508945

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

The coaxial helicopter, D'AT3, designed by General Corradino d'Ascanio, an Italian aviation engineer in 1930. The flying machine had two double-bladed, counter-rotating rotors, with control achieved by using auxiliary wings on the trailing edges of the blades

The coaxial helicopter, D'AT3, designed by General Corradino d'Ascanio, an Italian aviation engineer in 1930. The flying machine had two double-bladed, counter-rotating rotors, with control achieved by using auxiliary wings on the trailing edges of the blades

EVB2924094

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