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Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - Astronauts John Grunsfeld (on the robotic arm of the shuttle) and Andrew Feustel (down) during the fifth and last extravehicular exit to maintain the Hubble space telescope (HST). 18 May 2009. Astronaut John Grunsfeld, STS - 125 mission specialist, positioned on a foot restraint on the end of Atlantis' remote manipulator system (RMS), and astronaut Andrew Feustel (bottom center), mission specialist, participate in the mission's fifth and final session of extravehicular activity (EVA) as work continues to refurbish and upgrade the Hubble Space Telescope. During the seven - hour and two - minute spacewalk, Grunsfeld and Feustel installed a battery group replacement, removed and replaced a Fine Guidance Sensor and three thermal blankets (NOBL) protecting Hubble's electronics. 18 May 2009
Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - Astronauts John Grunsfeld (on the robotic arm of the shuttle) and Andrew Feustel (down) during the fifth and last extravehicular exit to maintain the Hubble space telescope (HST). 18 May 2009. Astronaut John Grunsfeld, STS - 125 mission specialist, positioned on a foot restraint on the end of Atlantis' remote manipulator system (RMS), and astronaut Andrew Feustel (bottom center), mission specialist, participate in the mission's fifth and final session of extravehicular activity (EVA) as work continues to refurbish and upgrade the Hubble Space Telescope. During the seven - hour and two - minute spacewalk, Grunsfeld and Feustel installed a battery group replacement, removed and replaced a Fine Guidance Sensor and three thermal blankets (NOBL) protecting Hubble's electronics. 18 May 2009

PIX4645395: Hubble space telescope: 4th maintenance mission 05/2009 - Hubble space telescope: fourth repair mission 05/2009 - Astronauts John Grunsfeld (on the robotic arm of the shuttle) and Andrew Feustel (down) during the fifth and last extravehicular exit to maintain the Hubble space telescope (HST). 18 May 2009. Astronaut John Grunsfeld, STS - 125 mission specialist, positioned on a foot restraint on the end of Atlantis' remote manipulator system (RMS), and astronaut Andrew Feustel (bottom center), mission specialist, participate in the mission's fifth and final session of extravehicular activity (EVA) as work continues to refurbish and upgrade the Hubble Space Telescope. During the seven - hour and two - minute spacewalk, Grunsfeld and Feustel installed a battery group replacement, removed and replaced a Fine Guidance Sensor and three thermal blankets (NOBL) protecting Hubble's electronics. 18 May 2009 / Bridgeman Images

Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009
Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009

PIX4645452: Hubble space telescope: end of the 4th maintenance mission 05/2009 - Hubble space telescope: end of the fourth repair mission - The Hubble space telescope (HST) seen from space shuttle Atlantis after their separation on 19 May 2009. An STS - 125 crew member aboard the Space Shuttle Atlantis captured this still image of the Hubble Space Telescope as the two spacecraft begin their relative separation on May 19, after having been linked together for the better part of a week. During the week five spacewalks were performed to complete the final servicing. 19 May 2009 / Bridgeman Images

Hubble space telescope - Artist view - Hubble space telescope - Artist view - The Hubble space telescope is a telescope orbiting the Earth at about 600 km altitude. It is 13 metres long, its main mirror has a diameter of 2.4 metres. He is equipped with spectrometer and several cameras observing the Universe in visible and infrared. The Hubble space telescope is in orbit at about 600 km around the Earth. This 13 meters in length telescope with a mirror of 2.4 meters (94.5 inches) in diameter is also equipped of many cameras and a spectrometer to observe the Universe in the visible and infrared light
Hubble space telescope - Artist view - Hubble space telescope - Artist view - The Hubble space telescope is a telescope orbiting the Earth at about 600 km altitude. It is 13 metres long, its main mirror has a diameter of 2.4 metres. He is equipped with spectrometer and several cameras observing the Universe in visible and infrared. The Hubble space telescope is in orbit at about 600 km around the Earth. This 13 meters in length telescope with a mirror of 2.4 meters (94.5 inches) in diameter is also equipped of many cameras and a spectrometer to observe the Universe in the visible and infrared light

PIX4645472: Hubble space telescope - Artist view - Hubble space telescope - Artist view - The Hubble space telescope is a telescope orbiting the Earth at about 600 km altitude. It is 13 metres long, its main mirror has a diameter of 2.4 metres. He is equipped with spectrometer and several cameras observing the Universe in visible and infrared. The Hubble space telescope is in orbit at about 600 km around the Earth. This 13 meters in length telescope with a mirror of 2.4 meters (94.5 inches) in diameter is also equipped of many cameras and a spectrometer to observe the Universe in the visible and infrared light / Bridgeman Images

View on the Sacre Coeur and rue Charles Nodier in Paris 75018. Photograph 10/04/06.
View on the Sacre Coeur and rue Charles Nodier in Paris 75018. Photograph 10/04/06.

TEC4645521: View on the Sacre Coeur and rue Charles Nodier in Paris 75018. Photograph 10/04/06. / Bridgeman Images

Angle boulevard Barbes and rue des Poissonniers in Paris 75018.
Angle boulevard Barbes and rue des Poissonniers in Paris 75018.

TEC4645548: Angle boulevard Barbes and rue des Poissonniers in Paris 75018. / Bridgeman Images

Satellite Kepler - Kepler spacecraft - Kepler satellite in clean room. Kepler is a satellite launched in March 2009, designed to discover inhabitable exoplanets in our galaxy. Nasa's Kepler spacecraft in a clean room at Ball Aerospace & Technologies Corp. in Boulder, Colorado. Kepler is a spaceborne telescope launched in march 2009 and designed to search the nearby region of our galaxy for Earth - size planets orbiting in the habitable zone of stars like our sun
Satellite Kepler - Kepler spacecraft - Kepler satellite in clean room. Kepler is a satellite launched in March 2009, designed to discover inhabitable exoplanets in our galaxy. Nasa's Kepler spacecraft in a clean room at Ball Aerospace & Technologies Corp. in Boulder, Colorado. Kepler is a spaceborne telescope launched in march 2009 and designed to search the nearby region of our galaxy for Earth - size planets orbiting in the habitable zone of stars like our sun

PIX4645650: Satellite Kepler - Kepler spacecraft - Kepler satellite in clean room. Kepler is a satellite launched in March 2009, designed to discover inhabitable exoplanets in our galaxy. Nasa's Kepler spacecraft in a clean room at Ball Aerospace & Technologies Corp. in Boulder, Colorado. Kepler is a spaceborne telescope launched in march 2009 and designed to search the nearby region of our galaxy for Earth - size planets orbiting in the habitable zone of stars like our sun / Bridgeman Images

James Webb Space Telescope (JWST) - Illustration - James Webb Space Telescope (JWST) - Illustration - The JWST Space Telescope will replace the Hubble Space Telescope in 2013. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared
James Webb Space Telescope (JWST) - Illustration - James Webb Space Telescope (JWST) - Illustration - The JWST Space Telescope will replace the Hubble Space Telescope in 2013. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared

PIX4645709: James Webb Space Telescope (JWST) - Illustration - James Webb Space Telescope (JWST) - Illustration - The JWST Space Telescope will replace the Hubble Space Telescope in 2013. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared / Bridgeman Images

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth
James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth

PIX4645744: James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth / Bridgeman Images

Space telescope TPF - Illustration - Space telescope TPF - Illustration - Space telescope project consists of several telescopes measuring 3 to 4m in diameter observing in infrared and operating in interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth. This interferometer will also be supported by a telescope of 4 to 6m diameter equipped with a coronographer (not shown in this illustration)
Space telescope TPF - Illustration - Space telescope TPF - Illustration - Space telescope project consists of several telescopes measuring 3 to 4m in diameter observing in infrared and operating in interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth. This interferometer will also be supported by a telescope of 4 to 6m diameter equipped with a coronographer (not shown in this illustration)

PIX4645934: Space telescope TPF - Illustration - Space telescope TPF - Illustration - Space telescope project consists of several telescopes measuring 3 to 4m in diameter observing in infrared and operating in interferometry. The objective of this project is to detect planets outside our solar system, similar to Earth. This interferometer will also be supported by a telescope of 4 to 6m diameter equipped with a coronographer (not shown in this illustration) / Bridgeman Images

Henri IV high school in Paris.
Henri IV high school in Paris.

TEC4622737: Henri IV high school in Paris. / Bridgeman Images

Book maker in Paris.
Book maker in Paris.

LBY4622972: Book maker in Paris. / Bridgeman Images

Univeitarian building, laboratory of the Ecole Normale Superieure (1933-1937), Angle de la rue Erasme et la rue Lhomond, Paris 5.
Univeitarian building, laboratory of the Ecole Normale Superieure (1933-1937), Angle de la rue Erasme et la rue Lhomond, Paris 5.

OMG4623045: Univeitarian building, laboratory of the Ecole Normale Superieure (1933-1937), Angle de la rue Erasme et la rue Lhomond, Paris 5. / Bridgeman Images

E.Collins aboard Columbia 07/99 - Astronaut Eileen M. Collins, Commander of Shuttle Columbia, seen aboard the Shuttle on July 24, 1999. Eileen M. Collins, after being the first female pilot of the space shuttle becomes the first female commander of the space shuttle during the STS-93 mission
E.Collins aboard Columbia 07/99 - Astronaut Eileen M. Collins, Commander of Shuttle Columbia, seen aboard the Shuttle on July 24, 1999. Eileen M. Collins, after being the first female pilot of the space shuttle becomes the first female commander of the space shuttle during the STS-93 mission

PIX4647583: E.Collins aboard Columbia 07/99 - Astronaut Eileen M. Collins, Commander of Shuttle Columbia, seen aboard the Shuttle on July 24, 1999. Eileen M. Collins, after being the first female pilot of the space shuttle becomes the first female commander of the space shuttle during the STS-93 mission / Bridgeman Images

Friedrichstrasse to Berlin (Germany).
Friedrichstrasse to Berlin (Germany).

TEC4647645: Friedrichstrasse to Berlin (Germany). / Bridgeman Images

The reconstruction of the Potsdamer Platz in Berlin (Germany).
The reconstruction of the Potsdamer Platz in Berlin (Germany).

TEC4647686: The reconstruction of the Potsdamer Platz in Berlin (Germany). / Bridgeman Images

A construction site in Tiergarten in Berlin (Germany).
A construction site in Tiergarten in Berlin (Germany).

TEC4647780: A construction site in Tiergarten in Berlin (Germany). / Bridgeman Images

Claude Nicollier in the shuttle Discovery STS - 103 1999 - Astronaut Claude Nicollier in Discovery - 1999 - Astronaut Claude Nicollier, mission specialist representing the European Space Agency (ESA), on Discovery's mid deck prior to a space walk in the weightlessness of space
Claude Nicollier in the shuttle Discovery STS - 103 1999 - Astronaut Claude Nicollier in Discovery - 1999 - Astronaut Claude Nicollier, mission specialist representing the European Space Agency (ESA), on Discovery's mid deck prior to a space walk in the weightlessness of space

PIX4647908: Claude Nicollier in the shuttle Discovery STS - 103 1999 - Astronaut Claude Nicollier in Discovery - 1999 - Astronaut Claude Nicollier, mission specialist representing the European Space Agency (ESA), on Discovery's mid deck prior to a space walk in the weightlessness of space / Bridgeman Images

The construction site on the Friedrichstrasse in Berlin (Germany).
The construction site on the Friedrichstrasse in Berlin (Germany).

TEC4647963: The construction site on the Friedrichstrasse in Berlin (Germany). / Bridgeman Images

Depart of astronauts STS - 107 01/2003 - STS - 107 crew is going to launch pad - 16/01/2003. The crew of the STS-107 mission joins firing pad 39A for decolving. Front, from left to right, Ilan Ramon, Kalpana Chawla and William “” Willie”” McCool; behind them, from left to right, Michael Anderson, David Brown, Laurel Clark, and Rick Husband. The STS - 107 crew heads for the Astrovan and a ride to Launch Pad 39A for liftoff. From left to right are Payload Commander Michael Anderson, Mission Specialist David Brown, Payload Specialist Ilan Ramon, Mission Specialists Laurel Clark and Kalpana Chawla, Mission Commandaer Rick Husband and Pilot William “” Willie””” McCool. Ramon is the first astronaut from Israel to fly on a Shuttle. The 16 - day mission is devoted to research and will include more than 80 experiments that will study Earth and space science, advanced technology development, and astronaut health and safety. The payload on Space Shuttle Columbia includes FREESTAR (Fast Reaction Experiments Enabling Science, Technology, Applications and Research) and the SHI Research Double Module (SHI/RDM), known as SPACEHAB. Experiments on the module range from material sciences to life sciences. Liftoff is scheduled for 10:39 a.m. EST
Depart of astronauts STS - 107 01/2003 - STS - 107 crew is going to launch pad - 16/01/2003. The crew of the STS-107 mission joins firing pad 39A for decolving. Front, from left to right, Ilan Ramon, Kalpana Chawla and William “” Willie”” McCool; behind them, from left to right, Michael Anderson, David Brown, Laurel Clark, and Rick Husband. The STS - 107 crew heads for the Astrovan and a ride to Launch Pad 39A for liftoff. From left to right are Payload Commander Michael Anderson, Mission Specialist David Brown, Payload Specialist Ilan Ramon, Mission Specialists Laurel Clark and Kalpana Chawla, Mission Commandaer Rick Husband and Pilot William “” Willie””” McCool. Ramon is the first astronaut from Israel to fly on a Shuttle. The 16 - day mission is devoted to research and will include more than 80 experiments that will study Earth and space science, advanced technology development, and astronaut health and safety. The payload on Space Shuttle Columbia includes FREESTAR (Fast Reaction Experiments Enabling Science, Technology, Applications and Research) and the SHI Research Double Module (SHI/RDM), known as SPACEHAB. Experiments on the module range from material sciences to life sciences. Liftoff is scheduled for 10:39 a.m. EST

PIX4648080: Depart of astronauts STS - 107 01/2003 - STS - 107 crew is going to launch pad - 16/01/2003. The crew of the STS-107 mission joins firing pad 39A for decolving. Front, from left to right, Ilan Ramon, Kalpana Chawla and William “” Willie”” McCool; behind them, from left to right, Michael Anderson, David Brown, Laurel Clark, and Rick Husband. The STS - 107 crew heads for the Astrovan and a ride to Launch Pad 39A for liftoff. From left to right are Payload Commander Michael Anderson, Mission Specialist David Brown, Payload Specialist Ilan Ramon, Mission Specialists Laurel Clark and Kalpana Chawla, Mission Commandaer Rick Husband and Pilot William “” Willie””” McCool. Ramon is the first astronaut from Israel to fly on a Shuttle. The 16 - day mission is devoted to research and will include more than 80 experiments that will study Earth and space science, advanced technology development, and astronaut health and safety. The payload on Space Shuttle Columbia includes FREESTAR (Fast Reaction Experiments Enabling Science, Technology, Applications and Research) and the SHI Research Double Module (SHI/RDM), known as SPACEHAB. Experiments on the module range from material sciences to life sciences. Liftoff is scheduled for 10:39 a.m. EST / Bridgeman Images

Extra exit - vehicle of M. Massimino STS - 109 03/2002 - M.Massimino during extravehicular activity. 03/2002 - Astronaut Michael J. Massimino, STS - 109 mission specialist, peers into Columbia's crew cabin during a brief break in work on the Hubble Space Telescope (HST), latched down just a few feet behind in Columbia's cargo bay. Astronauts Massimino and James H. Newman were making their second extravehicular activity (EVA) of the mission. Tue 06 2002
Extra exit - vehicle of M. Massimino STS - 109 03/2002 - M.Massimino during extravehicular activity. 03/2002 - Astronaut Michael J. Massimino, STS - 109 mission specialist, peers into Columbia's crew cabin during a brief break in work on the Hubble Space Telescope (HST), latched down just a few feet behind in Columbia's cargo bay. Astronauts Massimino and James H. Newman were making their second extravehicular activity (EVA) of the mission. Tue 06 2002

PIX4648206: Extra exit - vehicle of M. Massimino STS - 109 03/2002 - M.Massimino during extravehicular activity. 03/2002 - Astronaut Michael J. Massimino, STS - 109 mission specialist, peers into Columbia's crew cabin during a brief break in work on the Hubble Space Telescope (HST), latched down just a few feet behind in Columbia's cargo bay. Astronauts Massimino and James H. Newman were making their second extravehicular activity (EVA) of the mission. Tue 06 2002 / Bridgeman Images

Launch of the shuttle Atlantis STS - 110 04/2002 - Launch of STS - 110 Atlantis. 04/2002 - Launch of STS - 104 Atlantis Carrying the S0 (S - zero) Integrated Truss Structure and Mobile Transporter from Launch Pad 39B. Apr 08 2002
Launch of the shuttle Atlantis STS - 110 04/2002 - Launch of STS - 110 Atlantis. 04/2002 - Launch of STS - 104 Atlantis Carrying the S0 (S - zero) Integrated Truss Structure and Mobile Transporter from Launch Pad 39B. Apr 08 2002

PIX4648232: Launch of the shuttle Atlantis STS - 110 04/2002 - Launch of STS - 110 Atlantis. 04/2002 - Launch of STS - 104 Atlantis Carrying the S0 (S - zero) Integrated Truss Structure and Mobile Transporter from Launch Pad 39B. Apr 08 2002 / Bridgeman Images

Tempete sur Saturn seen by the Cassini probe - Huge Storm on Saturn seen by Cassini spacecraft - Evolution of a huge tempete on Saturn seen by the Cassini probe from December 5, 2010 to August 12, 2011. This series of images from Nasa's Cassini spacecraft shows the development of the largest storm seen on the planet since 1990. These true - color and composite near - true - color views chronicle the storm from its start in late 2010 through mid - 2011, showing how the distinct head of the storm quickly grew large but eventually became engulfed by the storm's tail. The earliest image of the storm, taken Dec. 5, 2010, is in the top left of the panel. The storm appears only as a small, white cloud on the terminator between the day side and night side of the planet. The next view, in the top middle of the panel and taken Jan. 2, 2011, shows that the head quickly grew much larger and a tail began to trail a great distance eastward. Some of the clouds moved south and got caught up in a current that flows to the east (to the right) relative to the storm head. In the top right of the panel, this tail, which appears as slightly blue clouds south and now west (left) of the storm head, can be seen encountering the storm in the Feb. 25 image.The April 22 image, in the bottom left of the panel, is one of Cassini's last views of the storm when it still had a recognizable head. In this view, the tail is south of the head and is well established by this time.The May 18 view, in the bottom middle, shows only the storm's tail. The head still existed at this time, but it is beyond the horizon and out of the field of view here.Between the time of the May 18 image and the next image shown here (from Aug. 12), the head of the storm was engulfed by the part of the storm's tail that spread eastward at the same latitude as the head. The Aug. 12 image, in the bottom right, shows that the head has lost its distinct identity and is now just part of the jumble of the storm. Also visible in these
Tempete sur Saturn seen by the Cassini probe - Huge Storm on Saturn seen by Cassini spacecraft - Evolution of a huge tempete on Saturn seen by the Cassini probe from December 5, 2010 to August 12, 2011. This series of images from Nasa's Cassini spacecraft shows the development of the largest storm seen on the planet since 1990. These true - color and composite near - true - color views chronicle the storm from its start in late 2010 through mid - 2011, showing how the distinct head of the storm quickly grew large but eventually became engulfed by the storm's tail. The earliest image of the storm, taken Dec. 5, 2010, is in the top left of the panel. The storm appears only as a small, white cloud on the terminator between the day side and night side of the planet. The next view, in the top middle of the panel and taken Jan. 2, 2011, shows that the head quickly grew much larger and a tail began to trail a great distance eastward. Some of the clouds moved south and got caught up in a current that flows to the east (to the right) relative to the storm head. In the top right of the panel, this tail, which appears as slightly blue clouds south and now west (left) of the storm head, can be seen encountering the storm in the Feb. 25 image.The April 22 image, in the bottom left of the panel, is one of Cassini's last views of the storm when it still had a recognizable head. In this view, the tail is south of the head and is well established by this time.The May 18 view, in the bottom middle, shows only the storm's tail. The head still existed at this time, but it is beyond the horizon and out of the field of view here.Between the time of the May 18 image and the next image shown here (from Aug. 12), the head of the storm was engulfed by the part of the storm's tail that spread eastward at the same latitude as the head. The Aug. 12 image, in the bottom right, shows that the head has lost its distinct identity and is now just part of the jumble of the storm. Also visible in these

PIX4625230: Tempete sur Saturn seen by the Cassini probe - Huge Storm on Saturn seen by Cassini spacecraft - Evolution of a huge tempete on Saturn seen by the Cassini probe from December 5, 2010 to August 12, 2011. This series of images from Nasa's Cassini spacecraft shows the development of the largest storm seen on the planet since 1990. These true - color and composite near - true - color views chronicle the storm from its start in late 2010 through mid - 2011, showing how the distinct head of the storm quickly grew large but eventually became engulfed by the storm's tail. The earliest image of the storm, taken Dec. 5, 2010, is in the top left of the panel. The storm appears only as a small, white cloud on the terminator between the day side and night side of the planet. The next view, in the top middle of the panel and taken Jan. 2, 2011, shows that the head quickly grew much larger and a tail began to trail a great distance eastward. Some of the clouds moved south and got caught up in a current that flows to the east (to the right) relative to the storm head. In the top right of the panel, this tail, which appears as slightly blue clouds south and now west (left) of the storm head, can be seen encountering the storm in the Feb. 25 image.The April 22 image, in the bottom left of the panel, is one of Cassini's last views of the storm when it still had a recognizable head. In this view, the tail is south of the head and is well established by this time.The May 18 view, in the bottom middle, shows only the storm's tail. The head still existed at this time, but it is beyond the horizon and out of the field of view here.Between the time of the May 18 image and the next image shown here (from Aug. 12), the head of the storm was engulfed by the part of the storm's tail that spread eastward at the same latitude as the head. The Aug. 12 image, in the bottom right, shows that the head has lost its distinct identity and is now just part of the jumble of the storm. Also visible in these / Bridgeman Images

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - which indicates that the sea was larger at some point in the past and has become smaller due to evaporation. The deposits are material left behind after the methane & ethane liquid evaporates, somewhat akin to the saline crust on a salt flat
Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - which indicates that the sea was larger at some point in the past and has become smaller due to evaporation. The deposits are material left behind after the methane & ethane liquid evaporates, somewhat akin to the saline crust on a salt flat

PIX4625340: Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - which indicates that the sea was larger at some point in the past and has become smaller due to evaporation. The deposits are material left behind after the methane & ethane liquid evaporates, somewhat akin to the saline crust on a salt flat / Bridgeman Images

Artist's view of the ice fountains on Enceladus - Artist's view of the ice jets on the surface of the Encelade satellite observed by the Cassini probe. It would appear that these particles feed the E ring of Saturn, which was previously unknown
Artist's view of the ice fountains on Enceladus - Artist's view of the ice jets on the surface of the Encelade satellite observed by the Cassini probe. It would appear that these particles feed the E ring of Saturn, which was previously unknown

PIX4625788: Artist's view of the ice fountains on Enceladus - Artist's view of the ice jets on the surface of the Encelade satellite observed by the Cassini probe. It would appear that these particles feed the E ring of Saturn, which was previously unknown / Bridgeman Images

Concert area from Bercy to Paris.
Concert area from Bercy to Paris.

TEC4627935: Concert area from Bercy to Paris. / Bridgeman Images

LHC: work on the ATLAS detector - LHC: Work on the ATLAS semiconductor tracker barrel - Work performed on the ATLAS semiconductor trajectory (SCT) - one of the main elements of the ATLAS internal detector Precision work is performed on the semiconductor tracker barrel of the ATLAS experiment. All work on these delicate components must be performed in a clean room so that impurities in the air, such as dust, do not contaminate the detector. The semiconductor tracker will be mounted in the barrel close to the heart of the ATLAS experiment to detect the path of particles produced in proton-proton collisions
LHC: work on the ATLAS detector - LHC: Work on the ATLAS semiconductor tracker barrel - Work performed on the ATLAS semiconductor trajectory (SCT) - one of the main elements of the ATLAS internal detector Precision work is performed on the semiconductor tracker barrel of the ATLAS experiment. All work on these delicate components must be performed in a clean room so that impurities in the air, such as dust, do not contaminate the detector. The semiconductor tracker will be mounted in the barrel close to the heart of the ATLAS experiment to detect the path of particles produced in proton-proton collisions

PIX4650506: LHC: work on the ATLAS detector - LHC: Work on the ATLAS semiconductor tracker barrel - Work performed on the ATLAS semiconductor trajectory (SCT) - one of the main elements of the ATLAS internal detector Precision work is performed on the semiconductor tracker barrel of the ATLAS experiment. All work on these delicate components must be performed in a clean room so that impurities in the air, such as dust, do not contaminate the detector. The semiconductor tracker will be mounted in the barrel close to the heart of the ATLAS experiment to detect the path of particles produced in proton-proton collisions / Bridgeman Images

Green Coulee. Promenade planted above the Viaduc des Arts, Paris 12th. It crosses the 12th arrondissement in its full length, for 4.5 km. The railway tracks are replaced by hanging gardens, designed by Philippe Mathieux and baptises Promenade Plante.
Green Coulee. Promenade planted above the Viaduc des Arts, Paris 12th. It crosses the 12th arrondissement in its full length, for 4.5 km. The railway tracks are replaced by hanging gardens, designed by Philippe Mathieux and baptises Promenade Plante.

TEC4628006: Green Coulee. Promenade planted above the Viaduc des Arts, Paris 12th. It crosses the 12th arrondissement in its full length, for 4.5 km. The railway tracks are replaced by hanging gardens, designed by Philippe Mathieux and baptises Promenade Plante. / Bridgeman Images

Marche d'Aligre in Paris.
Marche d'Aligre in Paris.

TEC4628074: Marche d'Aligre in Paris. / Bridgeman Images

Place de la Bastille in Paris.
Place de la Bastille in Paris.

TEC4628080: Place de la Bastille in Paris. / Bridgeman Images

Total Eclipse of Sun 22/07/2009 - Total Solar Eclipse - July 22 2009 - Total Sun Eclipse of 22 July 2009 seen in China, about fifty kilometers from Hangzhou city. Total Solar Eclipse seen from China near Hangzhou
Total Eclipse of Sun 22/07/2009 - Total Solar Eclipse - July 22 2009 - Total Sun Eclipse of 22 July 2009 seen in China, about fifty kilometers from Hangzhou city. Total Solar Eclipse seen from China near Hangzhou

PIX4628150: Total Eclipse of Sun 22/07/2009 - Total Solar Eclipse - July 22 2009 - Total Sun Eclipse of 22 July 2009 seen in China, about fifty kilometers from Hangzhou city. Total Solar Eclipse seen from China near Hangzhou / Bridgeman Images

Total Eclipse of Sun - 11/07/2010 - Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun of 11 July 2010 seen in French Polynesia (Tatakoto atoll). High resolution image, composite of 120 images. The total solar eclipse of 11 July 2010 seen in Tatakoto Atoll, French Polynesia. Composition of 120 images
Total Eclipse of Sun - 11/07/2010 - Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun of 11 July 2010 seen in French Polynesia (Tatakoto atoll). High resolution image, composite of 120 images. The total solar eclipse of 11 July 2010 seen in Tatakoto Atoll, French Polynesia. Composition of 120 images

PIX4628258: Total Eclipse of Sun - 11/07/2010 - Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun of 11 July 2010 seen in French Polynesia (Tatakoto atoll). High resolution image, composite of 120 images. The total solar eclipse of 11 July 2010 seen in Tatakoto Atoll, French Polynesia. Composition of 120 images / Bridgeman Images

Annular Eclipse of Sun 15 January 2010 - Myanmar Annular Solar Eclipse - Annular Eclipse of Sun 15 January 2010 seen from Bagan in Burma. Annular Solar Eclipse sequence wide - angle taken in Bagan, Myanmar on Jan. 15, 2010
Annular Eclipse of Sun 15 January 2010 - Myanmar Annular Solar Eclipse - Annular Eclipse of Sun 15 January 2010 seen from Bagan in Burma. Annular Solar Eclipse sequence wide - angle taken in Bagan, Myanmar on Jan. 15, 2010

PIX4628296: Annular Eclipse of Sun 15 January 2010 - Myanmar Annular Solar Eclipse - Annular Eclipse of Sun 15 January 2010 seen from Bagan in Burma. Annular Solar Eclipse sequence wide - angle taken in Bagan, Myanmar on Jan. 15, 2010 / Bridgeman Images

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Diamond effect at the end of the total eclipse. Ocean Lake, Wyoming, USA. Total solar eclipse on 2017 August 21 from Ocean Lake, Wyoming, USA
Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Diamond effect at the end of the total eclipse. Ocean Lake, Wyoming, USA. Total solar eclipse on 2017 August 21 from Ocean Lake, Wyoming, USA

PIX4628479: Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Diamond effect at the end of the total eclipse. Ocean Lake, Wyoming, USA. Total solar eclipse on 2017 August 21 from Ocean Lake, Wyoming, USA / Bridgeman Images

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse in Wyoming - Total Eclipse of Sun from August 21, 2017 seen in Wyoming, USA. Wide angle view of the sky during the total solar eclipse of August 21 2017
Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse in Wyoming - Total Eclipse of Sun from August 21, 2017 seen in Wyoming, USA. Wide angle view of the sky during the total solar eclipse of August 21 2017

PIX4628500: Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse in Wyoming - Total Eclipse of Sun from August 21, 2017 seen in Wyoming, USA. Wide angle view of the sky during the total solar eclipse of August 21 2017 / Bridgeman Images

Artist's view of an eclipse of Solei
Artist's view of an eclipse of Solei

PIX4628526: Artist's view of an eclipse of Solei / Bridgeman Images

Pious image: The Virgin in Heaven with the Child Jesus, 20th century (engraving)
Pious image: The Virgin in Heaven with the Child Jesus, 20th century (engraving)

LRI4629015: Pious image: The Virgin in Heaven with the Child Jesus, 20th century (engraving) / Bridgeman Images


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