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Images of 'Four Poster' found, 981

 
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: 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

 
Constellations of the Compsole and the Great Dog - Constellations of Pyxis and Canis Major - Constellation of the Compsole, near the horizon, and constellation of the Great Dog with the brilliant star Sirius. Pyxis, the Mariner's Compasse was originally Pyxis Nauticus and refers to the magnetic compasset. It is a small, insignificant arrangement of faint stars surrounded by much more eyecatching patterns of stars. Pyxis was once part of the very large constellation Argo Navis, the ship Argo, which carried Jason and the Argonauts. Argo Navis is now obsolete, but it was listed in Ptolemy's star catalogue, the Almagest. When the constellation boundaries were defined by the International Astronomical Union in the 1930s it was the only one of Ptolemy's 48 constellations that was not accepted. Instead, it was divided into the four constellations introduced by the French cleric and astronomer Nicolas de Lacaille in the 1750s: Carina, the keel, Puppis the stern, Vela the sails, and Pyxis. La C

PIX4589254

Constellations of the Compsole and the Great Dog - Constellations of Pyxis and Canis Major - Constellation of the Compsole, near the horizon, and constellation of the Great Dog with the brilliant star Sirius. Pyxis, the Mariner's Compasse was originally Pyxis Nauticus and refers to the magnetic compasset. It is a small, insignificant arrangement of faint stars surrounded by much more eyecatching patterns of stars. Pyxis was once part of the very large constellation Argo Navis, the ship Argo, which carried Jason and the Argonauts. Argo Navis is now obsolete, but it was listed in Ptolemy's star catalogue, the Almagest. When the constellation boundaries were defined by the International Astronomical Union in the 1930s it was the only one of Ptolemy's 48 constellations that was not accepted. Instead, it was divided into the four constellations introduced by the French cleric and astronomer Nicolas de Lacaille in the 1750s: Carina, the keel, Puppis the stern, Vela the sails, and Pyxis. La C

PIX4589254

 
Nebula IC 2220 in the Carene - A mass - loss star in IC 2220 - This nebula is illuminated by a giant red star, the star HD 65670. Image obtained by Siding Spring's 3.9m telescope. The bright, supergiant star at the centre of this nebula is known only by its catalog designation, HD 65750. The nebulosity around the star is the result of light reflected by dust surrounding it. The dust is thought to consist mainly of particles of silica condensed from material which the star is losing from its distended surface at a fairly steady rate. The rate of mass loss is much higher than in normal stars and is sufficient to produce the reflection nebula IC 2220. The stellar nature of the central object is revealed by the four diffraction spikes extending from it. These are artifacts due to structures within the telescope. The light from the star has also produced the annular halation ring (a photographic artefact) that ornaments the nebula. These features, real or otherwise, have provoked the name '

PIX4622497

Nebula IC 2220 in the Carene - A mass - loss star in IC 2220 - This nebula is illuminated by a giant red star, the star HD 65670. Image obtained by Siding Spring's 3.9m telescope. The bright, supergiant star at the centre of this nebula is known only by its catalog designation, HD 65750. The nebulosity around the star is the result of light reflected by dust surrounding it. The dust is thought to consist mainly of particles of silica condensed from material which the star is losing from its distended surface at a fairly steady rate. The rate of mass loss is much higher than in normal stars and is sufficient to produce the reflection nebula IC 2220. The stellar nature of the central object is revealed by the four diffraction spikes extending from it. These are artifacts due to structures within the telescope. The light from the star has also produced the annular halation ring (a photographic artefact) that ornaments the nebula. These features, real or otherwise, have provoked the name '

PIX4622497

 
Galaxies cluster Abell 2744 - This image of the galaxy cluster Abell 2744 located in the constellation of the Sculptor, combines images obtained in visible form by the Hubble Space Telescope (HST) and the Very Large Telescope (VLT). This image of galaxy cluster Abell 2744 combines data from the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, with an image taken with the European Southern Observatory's Very Large Telescope (VLT). Hubble provides the central, most detailed part of the image, while the VLT, which has a wider field of view, provides the outer parts of the image. This object has been nicknamed Pandora's Cluster because of the many different and strange phenomena that were unleashed by a huge collision that occurred over a period of 350 million years. A simultaneous pile - up between at least four separate clusters has produced strange effects that have never been seen together before

PIX4565849

Galaxies cluster Abell 2744 - This image of the galaxy cluster Abell 2744 located in the constellation of the Sculptor, combines images obtained in visible form by the Hubble Space Telescope (HST) and the Very Large Telescope (VLT). This image of galaxy cluster Abell 2744 combines data from the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, with an image taken with the European Southern Observatory's Very Large Telescope (VLT). Hubble provides the central, most detailed part of the image, while the VLT, which has a wider field of view, provides the outer parts of the image. This object has been nicknamed Pandora's Cluster because of the many different and strange phenomena that were unleashed by a huge collision that occurred over a period of 350 million years. A simultaneous pile - up between at least four separate clusters has produced strange effects that have never been seen together before

PIX4565849

 
Constellations of the Compsole and the Great Dog - Constellations of Pyxis and Canis Major - Constellation of the Compsole, near the horizon, and constellation of the Great Dog with the brilliant star Sirius. Pyxis, the Mariner's Compasse was originally Pyxis Nauticus and refers to the magnetic compasset. It is a small, insignificant arrangement of faint stars surrounded by much more eyecatching patterns of stars. Pyxis was once part of the very large constellation Argo Navis, the ship Argo, which carried Jason and the Argonauts. Argo Navis is now obsolete, but it was listed in Ptolemy's star catalogue, the Almagest. When the constellation boundaries were defined by the International Astronomical Union in the 1930s it was the only one of Ptolemy's 48 constellations that was not accepted. Instead, it was divided into the four constellations introduced by the French cleric and astronomer Nicolas de Lacaille in the 1750s: Carina, the keel, Puppis the stern, Vela the sails, and Pyxis. La C

PIX4589256

Constellations of the Compsole and the Great Dog - Constellations of Pyxis and Canis Major - Constellation of the Compsole, near the horizon, and constellation of the Great Dog with the brilliant star Sirius. Pyxis, the Mariner's Compasse was originally Pyxis Nauticus and refers to the magnetic compasset. It is a small, insignificant arrangement of faint stars surrounded by much more eyecatching patterns of stars. Pyxis was once part of the very large constellation Argo Navis, the ship Argo, which carried Jason and the Argonauts. Argo Navis is now obsolete, but it was listed in Ptolemy's star catalogue, the Almagest. When the constellation boundaries were defined by the International Astronomical Union in the 1930s it was the only one of Ptolemy's 48 constellations that was not accepted. Instead, it was divided into the four constellations introduced by the French cleric and astronomer Nicolas de Lacaille in the 1750s: Carina, the keel, Puppis the stern, Vela the sails, and Pyxis. La C

PIX4589256

 
Lakes of Nayriz, Iran, seen by satellite - Neyriz Lakes, Iran - In southern Iran's Fars province, the lakes of Bakhtegan and Tashk, better known as lakes of Nayriz “” appear on this image taken by ALOS, a four-ton Japanese observation satellite. Lake Bakhtegan (central) and Lake Tashk (upper), located in the Nayriz basin, are dirty lakes in the south-east of the Zagros Mountains, whose water levels fluctuate with rain and snow in the mountains. Lake Bakhtegan, the second largest lake in Iran, is fed mainly by the Kour River, while Lake Tashk receives the overflow from the marecages at its western extremite and from an important permanent north-west source. Although normally separated by narrow strips of land, during the years of heavy rain they can join and form only one lake. Similarly, after several years of low rains, as in 1934 and 1971, the lakes can be completely low except for the points closest to the springs. The two lakes, their delta and the morecages associated with the spr

PIX4660585

Lakes of Nayriz, Iran, seen by satellite - Neyriz Lakes, Iran - In southern Iran's Fars province, the lakes of Bakhtegan and Tashk, better known as lakes of Nayriz “” appear on this image taken by ALOS, a four-ton Japanese observation satellite. Lake Bakhtegan (central) and Lake Tashk (upper), located in the Nayriz basin, are dirty lakes in the south-east of the Zagros Mountains, whose water levels fluctuate with rain and snow in the mountains. Lake Bakhtegan, the second largest lake in Iran, is fed mainly by the Kour River, while Lake Tashk receives the overflow from the marecages at its western extremite and from an important permanent north-west source. Although normally separated by narrow strips of land, during the years of heavy rain they can join and form only one lake. Similarly, after several years of low rains, as in 1934 and 1971, the lakes can be completely low except for the points closest to the springs. The two lakes, their delta and the morecages associated with the spr

PIX4660585

 
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621160

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621160

 
Space exploration: MPCV module - Artist view - The MPCV spacecraft in space - The Multi-Purpose Crew Vehicle (MPCV) above Earth. This capsule should be able to take a crew of six astronauts to an asteroid, the Moon or to take men to Mars. Here, the vehcule is connected to an additional housing module for a mission of more than three months. The Multi-Purpose Crew Vehicle (MPCV) is a spacecraft project currently being developed by Lockheed Martin for NASA. Based on specifications and tests already performed for the Orion spacecraft. It was announced by NASA on 24 May 2011. For even longer missions the Deep Space Vehicle (DSV) could be mated with an Extended Stay Module (ESM). The ESM would offer additional life support and accommodations for a crew of three or four for deep space missions lasting 90 days or longer

Walter B Myers

PIX4639046

Space exploration: MPCV module - Artist view - The MPCV spacecraft in space - The Multi-Purpose Crew Vehicle (MPCV) above Earth. This capsule should be able to take a crew of six astronauts to an asteroid, the Moon or to take men to Mars. Here, the vehcule is connected to an additional housing module for a mission of more than three months. The Multi-Purpose Crew Vehicle (MPCV) is a spacecraft project currently being developed by Lockheed Martin for NASA. Based on specifications and tests already performed for the Orion spacecraft. It was announced by NASA on 24 May 2011. For even longer missions the Deep Space Vehicle (DSV) could be mated with an Extended Stay Module (ESM). The ESM would offer additional life support and accommodations for a crew of three or four for deep space missions lasting 90 days or longer

Walter B Myers

PIX4639046

 
Chandra Space Telescope - Artist View - Chandra X - Ray Observatory - View of the Chandra Telescope in orbit around Earth. The Chandra space telescope observes the universe in X-ray; it was launched and put into orbit in July 1999. Nasa's Chandra X - ray Observatory as it may appear at about 50,000 miles from the Earth, almost twice as high as Earth - orbiting geosynchronous satellites. Named after the Indian astrophysicist Subrahmanyan Chandrasekhar, the Chandra X - ray Observatory is the world's most powerful X - ray telescope, and at a weight of over 5 tons (10 tons including the detachable booster rocket) was the heaviest payload ever delivered into orbit by the Space Shuttle. Chandra was carried into space by Columbia in July 1999. Originally designed for a 5 year mission dedicated to observing distant celestial objects in the X - ray spectrum, Chandra has been observing for over three times that long and is still going strong. In this image the Chandra X - ray Observatory reveals

Walter B Myers

PIX4645635

Chandra Space Telescope - Artist View - Chandra X - Ray Observatory - View of the Chandra Telescope in orbit around Earth. The Chandra space telescope observes the universe in X-ray; it was launched and put into orbit in July 1999. Nasa's Chandra X - ray Observatory as it may appear at about 50,000 miles from the Earth, almost twice as high as Earth - orbiting geosynchronous satellites. Named after the Indian astrophysicist Subrahmanyan Chandrasekhar, the Chandra X - ray Observatory is the world's most powerful X - ray telescope, and at a weight of over 5 tons (10 tons including the detachable booster rocket) was the heaviest payload ever delivered into orbit by the Space Shuttle. Chandra was carried into space by Columbia in July 1999. Originally designed for a 5 year mission dedicated to observing distant celestial objects in the X - ray spectrum, Chandra has been observing for over three times that long and is still going strong. In this image the Chandra X - ray Observatory reveals

Walter B Myers

PIX4645635

 
Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

PIX4608987

Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

PIX4608987

 
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

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

 
Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

PIX4609752

Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

PIX4609752

 
Satellite MSG - 1 - Meteosat 8 - Anaglyph - Satellite MSG - 1 - Meteosat 8 - Anaglyph - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Meteosat Second Generation (MSG), is equipped with an extremely sophisticated imaging radiometer that can separate the incoming radiation into 12 (3 with the current Meteosat) different spectral bands. Each section, four of them in the visible and eight in the thermal infrared, delivers different information. They vary from visible images of weather systems during the day to cloud temperature at night; from surface temperature and water vapour to trace gas concentrations and dust particles in the atmosphere. MSG will deliver about twenty times as much information as its predecessor Meteosat, resulting in much more acc

D. Ducros

PIX4644648

Satellite MSG - 1 - Meteosat 8 - Anaglyph - Satellite MSG - 1 - Meteosat 8 - Anaglyph - Artist's view of the European satellite MSG - 1 (Meteosat Second Generation) or Meteosat 8, in orbit around the Earth. Launched on August 28, 2002, it is a geostationary satellite located 35 600 km from Earth; dedicated to meteorology, it observes the Earth in visible, and in infrared. Meteosat Second Generation (MSG), is equipped with an extremely sophisticated imaging radiometer that can separate the incoming radiation into 12 (3 with the current Meteosat) different spectral bands. Each section, four of them in the visible and eight in the thermal infrared, delivers different information. They vary from visible images of weather systems during the day to cloud temperature at night; from surface temperature and water vapour to trace gas concentrations and dust particles in the atmosphere. MSG will deliver about twenty times as much information as its predecessor Meteosat, resulting in much more acc

D. Ducros

PIX4644648

 
Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

PIX4625315

Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

PIX4625315

 
Space exploration: MPCV module - Artist view - The MPCV spacecraft in space - The Multi-Purpose Crew Vehicle (MPCV) above Earth. This capsule should be able to take a crew of six astronauts to an asteroid, the Moon or to take men to Mars. Here, the vehcule is connected to an additional housing module for a mission of more than three months. The Multi-Purpose Crew Vehicle (MPCV) is a spacecraft project currently being developed by Lockheed Martin for NASA. Based on specifications and tests already performed for the Orion spacecraft. It was announced by NASA on 24 May 2011. For even longer missions the Deep Space Vehicle (DSV) could be mated with an Extended Stay Module (ESM). The ESM would offer additional life support and accommodations for a crew of three or four for deep space missions lasting 90 days or longer

Walter B Myers

PIX4639090

Space exploration: MPCV module - Artist view - The MPCV spacecraft in space - The Multi-Purpose Crew Vehicle (MPCV) above Earth. This capsule should be able to take a crew of six astronauts to an asteroid, the Moon or to take men to Mars. Here, the vehcule is connected to an additional housing module for a mission of more than three months. The Multi-Purpose Crew Vehicle (MPCV) is a spacecraft project currently being developed by Lockheed Martin for NASA. Based on specifications and tests already performed for the Orion spacecraft. It was announced by NASA on 24 May 2011. For even longer missions the Deep Space Vehicle (DSV) could be mated with an Extended Stay Module (ESM). The ESM would offer additional life support and accommodations for a crew of three or four for deep space missions lasting 90 days or longer

Walter B Myers

PIX4639090

 
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

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

 
Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the is

PIX4672476

Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the is

PIX4672476

 
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Advert for Rising Sun, stove polish, reverse side, 1887 (colour litho)

English School, (19th century)

BL5901690

Advert for Rising Sun, stove polish, reverse side, 1887 (colour litho)

English School, (19th century)

BL5901690

 
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Advert for Rising Sun, stove polish, 1887 (colour litho)

English School, (19th century)

BL5901689

Advert for Rising Sun, stove polish, 1887 (colour litho)

English School, (19th century)

BL5901689

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