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Apollo 11: lunar rock - Apollo 11: lunar rock - Close up of lunar rocks contained in the first container of samples brought by astronauts from the Apollo 11 mission. 26 July 1969. A close - up view of the lunar rocks contained in the first Apollo 11 sample return container. The rock box was opened for the first time in the Vacuum Laboratory of the Manned Spacecraft Center's Lunar Receiving Laboratory, Building 37, at 3:55 p.m. (CDT), Saturday, July 26, 1969. The gloved hand gives an indication of size. This box also contained the Solar Wind Composition experiment (not shown) and two core tubes for subsurface samples (not shown). These lunar samples were collected by astronauts Neil A. Armstrong and Edwin E. Aldrin Jr. during their lunar surface extravehicular activity on July 20, 1969. 26 July 1969

Apollo 11: lunar rock - Apollo 11: lunar rock - Close up of lunar rocks contained in the first container of samples brought by astronauts from the Apollo 11 mission. 26 July 1969. A close - up view of the lunar rocks contained in the first Apollo 11 sample return container. The rock box was opened for the first time in the Vacuum Laboratory of the Manned Spacecraft Center's Lunar Receiving Laboratory, Building 37, at 3:55 p.m. (CDT), Saturday, July 26, 1969. The gloved hand gives an indication of size. This box also contained the Solar Wind Composition experiment (not shown) and two core tubes for subsurface samples (not shown). These lunar samples were collected by astronauts Neil A. Armstrong and Edwin E. Aldrin Jr. during their lunar surface extravehicular activity on July 20, 1969. 26 July 1969

PIX4596351

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 return - View of the Houston Control Room when astronauts return to Earth. 17/04/1970. Overall view of the crowded Mission Operations Control Room (MOCR) in the Mission Control Center (MCC) at Manned Spacecraft Center during post - recovery ceremonies aboard the USS Iwo Jima, prime recovery ship for the Apollo 13 mission. The Apollo 13 spacecraft, with astronauts James A. Lovell Jr., John L. Swigert Jr. and Fred W. Haise Jr. aboard, splashed down in the South Pacific Ocean at 12:07:44 p.m. (CST), April 17, 1970. The smooth splashdown and recovery operations brought an end to a perilous space flight for the crewmen and a tiring one for the ground crew in MCC

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 return - View of the Houston Control Room when astronauts return to Earth. 17/04/1970. Overall view of the crowded Mission Operations Control Room (MOCR) in the Mission Control Center (MCC) at Manned Spacecraft Center during post - recovery ceremonies aboard the USS Iwo Jima, prime recovery ship for the Apollo 13 mission. The Apollo 13 spacecraft, with astronauts James A. Lovell Jr., John L. Swigert Jr. and Fred W. Haise Jr. aboard, splashed down in the South Pacific Ocean at 12:07:44 p.m. (CST), April 17, 1970. The smooth splashdown and recovery operations brought an end to a perilous space flight for the crewmen and a tiring one for the ground crew in MCC

PIX4596912

Apollo 13: Alan Shepard in the Control Room - Alan Shepard in Mission Control Center during the Apollo 13 problem - Astronaut Alan Shepard in communication with Apollo 13 astronauts. 14/04/1970. Astronaut Alan B. Shepard Jr., prime crew commander of the Apollo 14 mission, monitors communications between the Apollo 13 spacecraft and Mission Control Center. He is seated at a console in the Mission Operations Control Room of the MCC, Manned Spacecraft Center. The main concern of the moment was action taken by the three Apollo 13 crewmen - astronauts James A. Lovell Jr., John L. Swigert Jr. and Fred W. Haise Jr. - to make corrections inside the spacecraft following discovery of an oxygen cell failure several hours earlier. April 14, 1970

Apollo 13: Alan Shepard in the Control Room - Alan Shepard in Mission Control Center during the Apollo 13 problem - Astronaut Alan Shepard in communication with Apollo 13 astronauts. 14/04/1970. Astronaut Alan B. Shepard Jr., prime crew commander of the Apollo 14 mission, monitors communications between the Apollo 13 spacecraft and Mission Control Center. He is seated at a console in the Mission Operations Control Room of the MCC, Manned Spacecraft Center. The main concern of the moment was action taken by the three Apollo 13 crewmen - astronauts James A. Lovell Jr., John L. Swigert Jr. and Fred W. Haise Jr. - to make corrections inside the spacecraft following discovery of an oxygen cell failure several hours earlier. April 14, 1970

PIX4596889

Apollo 13: Saturn V on his shooting pitch - Apollo 13: Saturn V on launch pad at night - Fusee Saturn V/Apollo 13 on his shooting pitch. 24 March 1970. Nighttime, ground level view of Pad A, Launch Complex 39, Kennedy Space Center (KSC), showing the Apollo 13 (Spacecraft 109/Lunar Module 7/Saturn 508) space vehicle during Countdown Demonstration Test (CDDT). The crew of Nasa's third lunar landing mission includes astronauts James A. Lovell Jr., commander; John L. Swigert Jr., command module pilot; and Fred W. Haise Jr., lunar module pilot. The Apollo 13 launch has been scheduled for 2:13 p.m. (EST), April 11, 1970. 24 March 1970

Apollo 13: Saturn V on his shooting pitch - Apollo 13: Saturn V on launch pad at night - Fusee Saturn V/Apollo 13 on his shooting pitch. 24 March 1970. Nighttime, ground level view of Pad A, Launch Complex 39, Kennedy Space Center (KSC), showing the Apollo 13 (Spacecraft 109/Lunar Module 7/Saturn 508) space vehicle during Countdown Demonstration Test (CDDT). The crew of Nasa's third lunar landing mission includes astronauts James A. Lovell Jr., commander; John L. Swigert Jr., command module pilot; and Fred W. Haise Jr., lunar module pilot. The Apollo 13 launch has been scheduled for 2:13 p.m. (EST), April 11, 1970. 24 March 1970

PIX4596748

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the control room on 15 April 1970 as flight controllers studied the weather forecast in the South Pacific for the landing of the Apollo capsule. A group of flight controllers gather around the console of Glenn S. Lunney (seated, nearest camera), Shift 4 flight director, in the Mission Operations Control Room (MOCR) of Mission Control Center (MCC), located in Building 30 at the Manned Spacecraft Center (MSC). Their attention is drawn to a weather map of the proposed landing site in the South Pacific Ocean. Among those looking on is Dr. Christopher C. Kraft, deputy director, MSC, standing in black suit, on right. When this photograph was taken, the Apollo 13 lunar landing mission had been canceled, and the problem - plagued Apollo 13 crew members were in trans - Earth trajectory attempting to bring their crippled spacecraft back home. April 15, 1970

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the control room on 15 April 1970 as flight controllers studied the weather forecast in the South Pacific for the landing of the Apollo capsule. A group of flight controllers gather around the console of Glenn S. Lunney (seated, nearest camera), Shift 4 flight director, in the Mission Operations Control Room (MOCR) of Mission Control Center (MCC), located in Building 30 at the Manned Spacecraft Center (MSC). Their attention is drawn to a weather map of the proposed landing site in the South Pacific Ocean. Among those looking on is Dr. Christopher C. Kraft, deputy director, MSC, standing in black suit, on right. When this photograph was taken, the Apollo 13 lunar landing mission had been canceled, and the problem - plagued Apollo 13 crew members were in trans - Earth trajectory attempting to bring their crippled spacecraft back home. April 15, 1970

PIX4596874

Apollo 13: Saturn V on his shooting pitch - Apollo 13: Saturn V on launch pad at night - Fusee Saturn V/Apollo 13 on his shooting pitch. 24 March 1970. Nighttime, ground level view of Pad A, Launch Complex 39, Kennedy Space Center (KSC), showing the Apollo 13 (Spacecraft 109/Lunar Module 7/Saturn 508) space vehicle during Countdown Demonstration Test (CDDT). The crew of Nasa's third lunar landing mission includes astronauts James A. Lovell Jr., commander; John L. Swigert Jr., command module pilot; and Fred W. Haise Jr., lunar module pilot. The Apollo 13 launch has been scheduled for 2:13 p.m. (EST), April 11, 1970. 24 March 1970

Apollo 13: Saturn V on his shooting pitch - Apollo 13: Saturn V on launch pad at night - Fusee Saturn V/Apollo 13 on his shooting pitch. 24 March 1970. Nighttime, ground level view of Pad A, Launch Complex 39, Kennedy Space Center (KSC), showing the Apollo 13 (Spacecraft 109/Lunar Module 7/Saturn 508) space vehicle during Countdown Demonstration Test (CDDT). The crew of Nasa's third lunar landing mission includes astronauts James A. Lovell Jr., commander; John L. Swigert Jr., command module pilot; and Fred W. Haise Jr., lunar module pilot. The Apollo 13 launch has been scheduled for 2:13 p.m. (EST), April 11, 1970. 24 March 1970

PIX4596822

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the Houston Control Room during the fourth televised transmission of the Apollo 13 crew. Flight director Eugene F. Kranz (from back to foreground) looks at astronaut Fred W. Haise Jr on screen. 13/04/1970. Overall view of the Mission Operations Control Room (MOCR) in the Mission Control Center (MCC) at Manned Spacecraft Center (MSC), during the fourth television transmission from the Apollo 13 mission in space. Eugene F. Kranz (foreground, back to camera), one of four Apollo 13 flight directors, views the large screen at front of MOCR, astronaut Fred W. Haise Jr., lunar module pilot, is seen on the screen. The fourth TV transmission from the Apollo 13 mission was on the evening of April 13, 1970

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the Houston Control Room during the fourth televised transmission of the Apollo 13 crew. Flight director Eugene F. Kranz (from back to foreground) looks at astronaut Fred W. Haise Jr on screen. 13/04/1970. Overall view of the Mission Operations Control Room (MOCR) in the Mission Control Center (MCC) at Manned Spacecraft Center (MSC), during the fourth television transmission from the Apollo 13 mission in space. Eugene F. Kranz (foreground, back to camera), one of four Apollo 13 flight directors, views the large screen at front of MOCR, astronaut Fred W. Haise Jr., lunar module pilot, is seen on the screen. The fourth TV transmission from the Apollo 13 mission was on the evening of April 13, 1970

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Decollage Apollo 10 - Apollo 10 launch - Decollage of the Saturn V/Apollo 10 rocket, Kennedy Space Center. 18/05/1969. The Apollo 10 (Spacecraft 106/Lunar Module 4/Saturn 505) space vehicle is launched from Pad B, Launch Complex 39, Kennedy Space Center, Florida at 12:49 p.m., May 18, 1969. Aboard the spacecraft are astronauts Thomas P. Stafford, commander; John W. Young, command module pilot; and Eugene A. Cernan, lunar module pilot. The eight - day, lunar orbit mission will mark the first time the complete Apollo spacecraft has operated around the moon and the second manned flight for the Lunar Module (LM). Two Apollo 10 astronauts, Stafford and Cernan, are scheduled to descend to within eight nautical miles of the moon's surface in the LM. 18 May 1969

Decollage Apollo 10 - Apollo 10 launch - Decollage of the Saturn V/Apollo 10 rocket, Kennedy Space Center. 18/05/1969. The Apollo 10 (Spacecraft 106/Lunar Module 4/Saturn 505) space vehicle is launched from Pad B, Launch Complex 39, Kennedy Space Center, Florida at 12:49 p.m., May 18, 1969. Aboard the spacecraft are astronauts Thomas P. Stafford, commander; John W. Young, command module pilot; and Eugene A. Cernan, lunar module pilot. The eight - day, lunar orbit mission will mark the first time the complete Apollo spacecraft has operated around the moon and the second manned flight for the Lunar Module (LM). Two Apollo 10 astronauts, Stafford and Cernan, are scheduled to descend to within eight nautical miles of the moon's surface in the LM. 18 May 1969

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Apollo 11: Decollage of Saturn V - Apollo 11 launch July 16 1969 - Decollage of the Saturn V/Apollo 11 rocket. 16/07/1969. The huge, 363 - feet tall Apollo 11 (Spacecraft 107/Lunar Module 5/Saturn 506) space vehicle is launched from Pad A, Launch Complex 39, Kennedy Space Center (KSC), at 9:32 a.m. (EDT), July 16, 1969. Onboard the Apollo 11 spacecraft were astronauts Neil A. Armstrong, commander; Michael Collins, command module pilot; and Edwin E. Aldrin Jr., lunar module pilot. Apollo 11 is the United States first lunar landing mission. While astronauts Armstrong and Aldrin descend in the Lunar Module (LM) “” Eagle””” to explore the Sea of Tranquility region of the moon, astronaut Collins will remain with the Command and Service Modules (CSM) “” Columbia””” in lunar orbit

Apollo 11: Decollage of Saturn V - Apollo 11 launch July 16 1969 - Decollage of the Saturn V/Apollo 11 rocket. 16/07/1969. The huge, 363 - feet tall Apollo 11 (Spacecraft 107/Lunar Module 5/Saturn 506) space vehicle is launched from Pad A, Launch Complex 39, Kennedy Space Center (KSC), at 9:32 a.m. (EDT), July 16, 1969. Onboard the Apollo 11 spacecraft were astronauts Neil A. Armstrong, commander; Michael Collins, command module pilot; and Edwin E. Aldrin Jr., lunar module pilot. Apollo 11 is the United States first lunar landing mission. While astronauts Armstrong and Aldrin descend in the Lunar Module (LM) “” Eagle””” to explore the Sea of Tranquility region of the moon, astronaut Collins will remain with the Command and Service Modules (CSM) “” Columbia””” in lunar orbit

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Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the control room during the last 24 hours of the Apollo 13 mission as astronauts attempt to return to Earth after an oxygen tank explosion. 16/04/1970. As the problem - plagued Apollo 13 crewmen entered their final 24 hours in space, several persons important to the mission remained attentive at consoles in the Mission Operations Control Room of the Mission Control Center at Manned Spacecraft Center. Among those monitoring communications and serving in supervisory capacities were these four officials from National Aeronautics and Space Administration Headquarters, Washington, D.C.: (from left) Thomas H. McMullen, Office of Manned Space Flight, who served as Shift 1 mission director; Dale Myers, associate administrator, Manned Space Flight; Chester M. Lee of the Apollo Program Directorate, OMSF, Apollo 13 mission director; and Dr. Rocco A. Petrone, Apollo program director, OMSF

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the control room during the last 24 hours of the Apollo 13 mission as astronauts attempt to return to Earth after an oxygen tank explosion. 16/04/1970. As the problem - plagued Apollo 13 crewmen entered their final 24 hours in space, several persons important to the mission remained attentive at consoles in the Mission Operations Control Room of the Mission Control Center at Manned Spacecraft Center. Among those monitoring communications and serving in supervisory capacities were these four officials from National Aeronautics and Space Administration Headquarters, Washington, D.C.: (from left) Thomas H. McMullen, Office of Manned Space Flight, who served as Shift 1 mission director; Dale Myers, associate administrator, Manned Space Flight; Chester M. Lee of the Apollo Program Directorate, OMSF, Apollo 13 mission director; and Dr. Rocco A. Petrone, Apollo program director, OMSF

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Apollo 17: astronauts greet the earth - Apollo 17: astronauts saluting people on Earth - Astronauts Gene Cernan, commander of Apollo 17, (left) and H.Schmitt greet their telespectactors during a television broadcast from the Moon on 13 December 1972. Astronauts Eugene A. Cernan (on left) and Harrison H. Schmitt pay their respects and send their best wishes to the members of the International Youth Science Tour, who were visiting the Manned Spacecraft Center, in brief ceremonies near the close of the third Apollo 17 extravehicular activity (EVA) at the Taurus - Littrow landing site. This picture is a reproduction taken from a color television transmission made by the color RCA TV camera mounted on the lunar roving vehicle. Noting that they had collected a very significant rock composed of many fragments, Schmitt said, “” A portion of a rock will be sent to a representative agency or museum in each of the countries represented by the young people in Houston today...”” 13 Dec 1972

Apollo 17: astronauts greet the earth - Apollo 17: astronauts saluting people on Earth - Astronauts Gene Cernan, commander of Apollo 17, (left) and H.Schmitt greet their telespectactors during a television broadcast from the Moon on 13 December 1972. Astronauts Eugene A. Cernan (on left) and Harrison H. Schmitt pay their respects and send their best wishes to the members of the International Youth Science Tour, who were visiting the Manned Spacecraft Center, in brief ceremonies near the close of the third Apollo 17 extravehicular activity (EVA) at the Taurus - Littrow landing site. This picture is a reproduction taken from a color television transmission made by the color RCA TV camera mounted on the lunar roving vehicle. Noting that they had collected a very significant rock composed of many fragments, Schmitt said, “” A portion of a rock will be sent to a representative agency or museum in each of the countries represented by the young people in Houston today...”” 13 Dec 1972

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Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

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Apollo 11: Decollage of Saturn V - Apollo 11 launch July 16 1969 - Decollage of the Saturn V/Apollo 11 rocket. 16/07/1969. The huge, 363 - feet tall Apollo 11 (Spacecraft 107/Lunar Module 5/Saturn 506) space vehicle is launched from Pad A, Launch Complex 39, Kennedy Space Center (KSC), at 9:32 a.m. (EDT), July 16, 1969. Aboard the Apollo 11 spacecraft were astronauts Neil A. Armstrong, commander; Michael Collins, command module pilot; and Edwin E. Aldrin Jr., lunar module pilot. Apollo 11 is the United States' first lunar landing mission. This view of the liftoff was taken by a camera mounted on the mobile launch tower. While astronauts Armstrong and Aldrin descend in the Lunar Module (LM) “” Eagle””” to explore the Sea of Tranquility region of the moon, astronaut Collins will remain with the Command and Service Modules (CSM) “” Columbia””” in lunar orbit

Apollo 11: Decollage of Saturn V - Apollo 11 launch July 16 1969 - Decollage of the Saturn V/Apollo 11 rocket. 16/07/1969. The huge, 363 - feet tall Apollo 11 (Spacecraft 107/Lunar Module 5/Saturn 506) space vehicle is launched from Pad A, Launch Complex 39, Kennedy Space Center (KSC), at 9:32 a.m. (EDT), July 16, 1969. Aboard the Apollo 11 spacecraft were astronauts Neil A. Armstrong, commander; Michael Collins, command module pilot; and Edwin E. Aldrin Jr., lunar module pilot. Apollo 11 is the United States' first lunar landing mission. This view of the liftoff was taken by a camera mounted on the mobile launch tower. While astronauts Armstrong and Aldrin descend in the Lunar Module (LM) “” Eagle””” to explore the Sea of Tranquility region of the moon, astronaut Collins will remain with the Command and Service Modules (CSM) “” Columbia””” in lunar orbit

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Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - Nasa Administrator Thomas O. Paine in communication with U.S. President Richard Nixon April 14, 1970. Dr. Thomas O. Paine, Administrator, National Aeronautics and Space Administration (NASA), talks on the telephone to President Richard M. Nixon. Dr. Paine is seated at his console in the Mission Operations Control Room (MOCR) at the Mission Control Center (MCC), Manned Spacecraft Center (MSC). Also pictured are Dr. Rocco Petrone, Apollo program director, Office Manned Spaceflight, NASA Headquarters (facing camera); and Chester M. Lee, Apollo mission director, Office of Manned Spaceflight, NASA Headquarters (HQ). Dr. Paine and the President were discussing the revised Apollo 13 flight plan following discovery of an oxygen cell failure in the Apollo 13 spacecraft several hours earlier. April 14, 1970

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - Nasa Administrator Thomas O. Paine in communication with U.S. President Richard Nixon April 14, 1970. Dr. Thomas O. Paine, Administrator, National Aeronautics and Space Administration (NASA), talks on the telephone to President Richard M. Nixon. Dr. Paine is seated at his console in the Mission Operations Control Room (MOCR) at the Mission Control Center (MCC), Manned Spacecraft Center (MSC). Also pictured are Dr. Rocco Petrone, Apollo program director, Office Manned Spaceflight, NASA Headquarters (facing camera); and Chester M. Lee, Apollo mission director, Office of Manned Spaceflight, NASA Headquarters (HQ). Dr. Paine and the President were discussing the revised Apollo 13 flight plan following discovery of an oxygen cell failure in the Apollo 13 spacecraft several hours earlier. April 14, 1970

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Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

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Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 return - View of Houston Control Room as astronauts return to Earth. In the foreground, Gene Kranz, flight manager, savours a cigar. 17/04/1970. Overall view of Mission Operations Control Room in Mission Control Center at the Manned Spacecraft Center (MSC) during the ceremonies aboard the USS Iwo Jima, prime recovery ship for the Apollo 13 mission. Dr. Donald K. Slayton (in black shirt, left of center), director of Flight Crew Operations at MSC, and Chester M. Lee of the Apollo Program Directorate, Office of Manned Space Flight, NASA Headquarters, shake hands, while Dr. Rocco A. Petrone, Apollo program director, Office of Manned Space Flight, NASA Headquarters (standing, near Lee), watches the large screen showing astronaut James A. Lovell Jr., Apollo 13 commander, during the onboard ceremonies. In the foreground, Glynn S. Lunney (extreme left) and Eugene F. Kranz (smoking a cigar), two Apollo 13 flight direc

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 return - View of Houston Control Room as astronauts return to Earth. In the foreground, Gene Kranz, flight manager, savours a cigar. 17/04/1970. Overall view of Mission Operations Control Room in Mission Control Center at the Manned Spacecraft Center (MSC) during the ceremonies aboard the USS Iwo Jima, prime recovery ship for the Apollo 13 mission. Dr. Donald K. Slayton (in black shirt, left of center), director of Flight Crew Operations at MSC, and Chester M. Lee of the Apollo Program Directorate, Office of Manned Space Flight, NASA Headquarters, shake hands, while Dr. Rocco A. Petrone, Apollo program director, Office of Manned Space Flight, NASA Headquarters (standing, near Lee), watches the large screen showing astronaut James A. Lovell Jr., Apollo 13 commander, during the onboard ceremonies. In the foreground, Glynn S. Lunney (extreme left) and Eugene F. Kranz (smoking a cigar), two Apollo 13 flight direc

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Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the control room on 15 April 1970 while the makeshift box (nicknamed “mailbox”) for purging CO2 inside the lunar module is present. Prototype of the “” mail box”” constructed at the Manned Spacecraft Center (MSC) to remove carbon dioxide from the Apollo 13 Command Module (CM) is displayed in the Mission Control Center (MCC). The “” mail box”” was constructed when it became apparent CO2 was prevalent in the CM and the spacecraft's lithium hydroxide system was not removing it sufficiently. A space suit exhaust hose is connected to a lithium hydroxide canister to purge the cabin air. There are 16 such canisters in the CM and each will last approximately 12 hours. Looking at the “” mail box”” are (from the left): Milton L. Windler, shift 1 flight director; Dr. Donald K. (Deke) Slayton, director of flight crew operations, MSC; Howard W. Tindall, deputy director, flight operations, MSC; Sigurd A.

Apollo 13: Control Room - View of Mission Control Center during the Apollo 13 problem - View of the control room on 15 April 1970 while the makeshift box (nicknamed “mailbox”) for purging CO2 inside the lunar module is present. Prototype of the “” mail box”” constructed at the Manned Spacecraft Center (MSC) to remove carbon dioxide from the Apollo 13 Command Module (CM) is displayed in the Mission Control Center (MCC). The “” mail box”” was constructed when it became apparent CO2 was prevalent in the CM and the spacecraft's lithium hydroxide system was not removing it sufficiently. A space suit exhaust hose is connected to a lithium hydroxide canister to purge the cabin air. There are 16 such canisters in the CM and each will last approximately 12 hours. Looking at the “” mail box”” are (from the left): Milton L. Windler, shift 1 flight director; Dr. Donald K. (Deke) Slayton, director of flight crew operations, MSC; Howard W. Tindall, deputy director, flight operations, MSC; Sigurd A.

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Saturn and Mimas seen by the Cassini probe 18/01/2005 - Saturn and Mimas seen by Cassini spacecraft Jan. 18 2005 - The Mimas satellite photographed in front of Saturn by the Cassini probe on 18 January 2005 at a distance of 1.4 million km from the planet. The shadow of Saturn's rings is projected on the planet. Mimas drifts along in its orbit against the azure backdrop of Saturn's northern latitudes in this true color view. The long, dark lines on the atmosphere are shadows cast by the planet's rings. Saturn's northern hemisphere is presently relatively cloud - free, and rays of sunlight take a long path through the atmosphere. This results in sunlight being scattered at shorter (bluer) wavelengths, thus giving the northernmost latitudes their bluish appearance at visible wavelengths. At the bottom, craters on icy Mimas (398 kilometers, or 247 miles across) give the moon a dimpled appearance. Images taken using infrared (930 nanometers), green (568 nanometers) and ultraviolet (338 nano

Saturn and Mimas seen by the Cassini probe 18/01/2005 - Saturn and Mimas seen by Cassini spacecraft Jan. 18 2005 - The Mimas satellite photographed in front of Saturn by the Cassini probe on 18 January 2005 at a distance of 1.4 million km from the planet. The shadow of Saturn's rings is projected on the planet. Mimas drifts along in its orbit against the azure backdrop of Saturn's northern latitudes in this true color view. The long, dark lines on the atmosphere are shadows cast by the planet's rings. Saturn's northern hemisphere is presently relatively cloud - free, and rays of sunlight take a long path through the atmosphere. This results in sunlight being scattered at shorter (bluer) wavelengths, thus giving the northernmost latitudes their bluish appearance at visible wavelengths. At the bottom, craters on icy Mimas (398 kilometers, or 247 miles across) give the moon a dimpled appearance. Images taken using infrared (930 nanometers), green (568 nanometers) and ultraviolet (338 nano

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Futuristic vision of how an interstellar spacecraft

Futuristic vision of how an interstellar spacecraft

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Futuristic vision of how an interstellar spacecraft

Futuristic vision of how an interstellar spacecraft

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Futuristic vision of how an interstellar spacecraft

Futuristic vision of how an interstellar spacecraft

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Futuristic vision of how an interstellar spacecraft

Futuristic vision of how an interstellar spacecraft

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Futuristic vision of how an interstellar spacecraft

Futuristic vision of how an interstellar spacecraft

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Futuristic vision of how an interstellar spacecraft

Futuristic vision of how an interstellar spacecraft

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Futuristic vision of how an interstellar spacecraft might refuel in space

Futuristic vision of how an interstellar spacecraft might refuel in space

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The cracks in Saturns moon, Enceladus

The cracks in Saturns moon, Enceladus

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ISS view of the Strait of Gibraltar with a Russian Soyuz spacecraft and Progress spacecraft, 2016

ISS view of the Strait of Gibraltar with a Russian Soyuz spacecraft and Progress spacecraft, 2016

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Model of the Voyager space probe.

Model of the Voyager space probe.

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Kepler-16

Kepler-16

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NEXT - Ionic Propulsion Engine - NEXT - Ion thruster - NEXT (NASA's Evolutionary Xenon Thruster), new generation ion motor developed by NASA. NASA Glenn has been developing the next generation of ion thrusters for future missions. Nasa's Evolutionary Xenon Thruster (NEXT) Project has developed a 7 - kilowatt ion thruster that can provide the capabilities needed in the future

NEXT - Ionic Propulsion Engine - NEXT - Ion thruster - NEXT (NASA's Evolutionary Xenon Thruster), new generation ion motor developed by NASA. NASA Glenn has been developing the next generation of ion thrusters for future missions. Nasa's Evolutionary Xenon Thruster (NEXT) Project has developed a 7 - kilowatt ion thruster that can provide the capabilities needed in the future

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Rover Curiosity on March, 12 May 2019.

Rover Curiosity on March, 12 May 2019.

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ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

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ATV - artist's view - Anaglyph - The ATV - Anaglyph - Relief view of the European Automated Transfer Vehicle (ATV). Artistic view of the Automated Transfer Vehicle (ATV)

ATV - artist's view - Anaglyph - The ATV - Anaglyph - Relief view of the European Automated Transfer Vehicle (ATV). Artistic view of the Automated Transfer Vehicle (ATV)

D. Ducros

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The Viking probe - The Viking spaceprobe - The Viking 1 and Viking 2 probes, both composed of an orbiter and a lander, explored the planet Mars in 1976. Model of one of the Viking spacecraft, which were made of two parts: an orbiter and a lander. Both Viking 1 and Viking 2 explored March in 1976

The Viking probe - The Viking spaceprobe - The Viking 1 and Viking 2 probes, both composed of an orbiter and a lander, explored the planet Mars in 1976. Model of one of the Viking spacecraft, which were made of two parts: an orbiter and a lander. Both Viking 1 and Viking 2 explored March in 1976

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Retrieving of Shenzhou Spacecraft

Retrieving of Shenzhou Spacecraft

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Core of comet 67P/Churyumov-Gerasimenko seen by Rosetta - Comet 67P/Churyumov-Gerasimenko nucleus from Rosetta: Image of the surface of comet 67P/Churyumov-Gerasimenko taken at an altitude of 16 km during the final descent of the Rosetta probe on 30 September 2016. Rosetta's OSIRIS narrow-angle camera captured this image of Comet 67P/Churyumov-Gerasimenko at 01:20 GMT from an altitude of about 16 km above the surface during the spacecraft's final descent on 30 September. The image scale is about 30 cm/pixel and the image measures about 614 m across

Core of comet 67P/Churyumov-Gerasimenko seen by Rosetta - Comet 67P/Churyumov-Gerasimenko nucleus from Rosetta: Image of the surface of comet 67P/Churyumov-Gerasimenko taken at an altitude of 16 km during the final descent of the Rosetta probe on 30 September 2016. Rosetta's OSIRIS narrow-angle camera captured this image of Comet 67P/Churyumov-Gerasimenko at 01:20 GMT from an altitude of about 16 km above the surface during the spacecraft's final descent on 30 September. The image scale is about 30 cm/pixel and the image measures about 614 m across

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Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

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Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the TGO probe (Trace Gas Orbiter) of the European mission ExoMars 2016. ExoMars Trace Gas Orbiter at Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the TGO probe (Trace Gas Orbiter) of the European mission ExoMars 2016. ExoMars Trace Gas Orbiter at Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

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Voyager space probe: Nasa's Voyager 1 spacecraft entering interstellar space

Voyager space probe: Nasa's Voyager 1 spacecraft entering interstellar space

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Loading up the space Ferry-ship. 1948

Loading up the space Ferry-ship. 1948

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Space Ferry-ship

Space Ferry-ship

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NEXT - Ionic Propulsion Engine - NEXT - Ion thruster - NEXT (NASA's Evolutionary Xenon Thruster), new generation ion motor developed by NASA. NASA Glenn has been developing the next generation of ion thrusters for future missions. Nasa's Evolutionary Xenon Thruster (NEXT) Project has developed a 7 - kilowatt ion thruster that can provide the capabilities needed in the future

NEXT - Ionic Propulsion Engine - NEXT - Ion thruster - NEXT (NASA's Evolutionary Xenon Thruster), new generation ion motor developed by NASA. NASA Glenn has been developing the next generation of ion thrusters for future missions. Nasa's Evolutionary Xenon Thruster (NEXT) Project has developed a 7 - kilowatt ion thruster that can provide the capabilities needed in the future

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The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe above the northern hemisphere of Saturn. This illustration shows Cassini above Saturn's northern hemisphere prior to making one of its Grand Finale dives. During Cassini's Grand Finale, the spacecraft will make 22 orbits around Saturn that carry the spacecraft over the planet's north before diving between Saturn and its rings. At the conclusion of this final set of daring orbits, the spacecraft will plunge into Saturn's atmosphere, ending its mission on Sept. 15, 2017.

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe above the northern hemisphere of Saturn. This illustration shows Cassini above Saturn's northern hemisphere prior to making one of its Grand Finale dives. During Cassini's Grand Finale, the spacecraft will make 22 orbits around Saturn that carry the spacecraft over the planet's north before diving between Saturn and its rings. At the conclusion of this final set of daring orbits, the spacecraft will plunge into Saturn's atmosphere, ending its mission on Sept. 15, 2017.

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La prode Cassini et Saturn - Cassini spacecraft at Saturn - This illustration shows Nasa's Cassini spacecraft about to make one of its dives between Saturn and its innermost rings as part of the mission's Grand Finale. Cassini will make 22 orbits that swoop between the rings and the planet before ending its mission on Sept 15, 2017, with a final plunge into Saturn

La prode Cassini et Saturn - Cassini spacecraft at Saturn - This illustration shows Nasa's Cassini spacecraft about to make one of its dives between Saturn and its innermost rings as part of the mission's Grand Finale. Cassini will make 22 orbits that swoop between the rings and the planet before ending its mission on Sept 15, 2017, with a final plunge into Saturn

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The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe during its final dip into the atmosphere of Saturn on September 15, 2017. As depicted in this illustration, Cassini will plunge into Saturn's atmosphere on Sept 15, 2017. Using its attitude control thrusters, the spacecraft will work to keep its antenna pointed at Earth while it sends its final data, including the composition of Saturn's upper atmosphere. The atmospheric torque will quickly become stronger than what the thrusters can compensate for, and after that point, Cassini will begin to tumble. When this happens, its radio connection to Earth will be severed, ending the mission. Following loss of signal, the spacecraft will burn up like a meteor in Saturn's upper atmosphere.

The Cassini and Saturn probe - Cassini spacecraft at Saturn - Artist's view of the Cassini probe during its final dip into the atmosphere of Saturn on September 15, 2017. As depicted in this illustration, Cassini will plunge into Saturn's atmosphere on Sept 15, 2017. Using its attitude control thrusters, the spacecraft will work to keep its antenna pointed at Earth while it sends its final data, including the composition of Saturn's upper atmosphere. The atmospheric torque will quickly become stronger than what the thrusters can compensate for, and after that point, Cassini will begin to tumble. When this happens, its radio connection to Earth will be severed, ending the mission. Following loss of signal, the spacecraft will burn up like a meteor in Saturn's upper atmosphere.

PIX4643513

The Cassini probe and the rings of Saturn - Cassini spacecraft with Saturn's rings - Artist's view of the Cassini probe near the rings of Saturn. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. Cassini-Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004.

The Cassini probe and the rings of Saturn - Cassini spacecraft with Saturn's rings - Artist's view of the Cassini probe near the rings of Saturn. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. Cassini-Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004.

Steven Hobbs

PIX4643503

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view: Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). TGO has been in orbit around Mars since October 19, 2016. The Schiaparelli module was lost after separation. Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO was launched on March 14 2016 with Schiaparelli. TGO orbits March since October 19 2016. Schiaparelli was lost after separation. TGO searches for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2020

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view: Artist view of the European mission ExoMars 2016 with the separation of the Shiaparelli landing module from the TGO probe (Trace Gas Orbiter). TGO has been in orbit around Mars since October 19, 2016. The Schiaparelli module was lost after separation. Artist's impression depicting the separation of the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, from the Trace Gas Orbiter, and heading for Mars. TGO was launched on March 14 2016 with Schiaparelli. TGO orbits March since October 19 2016. Schiaparelli was lost after separation. TGO searches for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2020

PIX4643703

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

Mission ExoMars 2016 - Artist view - ExoMars Mission - Artist view - Artist view of the European mission ExoMars 2016 with the Shiaparelli landing module embarks on the TGO (Trace Gas Orbiter) probe. Artist's impression depicting the ExoMars 2016 entry, descent and landing demonstrator module, named Schiaparelli, on the Trace Gas Orbiter, and heading for Mars. TGO will be launched in 2016 with Schiaparelli, the entry, descent and landing demonstrator module. It will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars. TGO will also serve as a communications relay for the rover and surface science platform that will be launched in 2018

D. Ducros

PIX4606969

Juno Probe - Artist's View - Juno Artist's Rendering - Artist's View of Juno Probe in orbit around Jupiter. Launch in 2011, the Juno probe will reach Jupiter in 2016. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. Juno will repeatedly dive between the planet and its intense belts of charged particle radiation, coming only 5,000 kilometers (about 3,000 miles) from the cloud tops at closest approach. Juno's primary goal is to improve our understanding of Jupiter's formation and evolution. The spacecraft will spend a year investigating the planet's origins, interior structure, deep atmosphere and magnetosphere. Juno's study of Jupiter will help us to understand the history of our own solar system and provide new insight into how planetary systems form and develop in our galaxy and beyond

Juno Probe - Artist's View - Juno Artist's Rendering - Artist's View of Juno Probe in orbit around Jupiter. Launch in 2011, the Juno probe will reach Jupiter in 2016. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. Juno will repeatedly dive between the planet and its intense belts of charged particle radiation, coming only 5,000 kilometers (about 3,000 miles) from the cloud tops at closest approach. Juno's primary goal is to improve our understanding of Jupiter's formation and evolution. The spacecraft will spend a year investigating the planet's origins, interior structure, deep atmosphere and magnetosphere. Juno's study of Jupiter will help us to understand the history of our own solar system and provide new insight into how planetary systems form and develop in our galaxy and beyond

PIX4605942

Solar Orbiter (photo)

Solar Orbiter (photo)

PIX6039538

Prode Juno and Jupiter - Artist view - Juno Over Jupiter's South Pole -Illustration:

Prode Juno and Jupiter - Artist view - Juno Over Jupiter's South Pole -Illustration:

PIX4605936

Futuristic vision of how a moon bound spacecraft (rocket) might be look. 1936

Futuristic vision of how a moon bound spacecraft (rocket) might be look. 1936

UIG1578665

Replica of the Soviet Space Probe, Venera 3 on Display at the Cosmos Pavilion at the Exhibition of National Economic Achievements (Vdnkh) in Moscow, 1967.

Replica of the Soviet Space Probe, Venera 3 on Display at the Cosmos Pavilion at the Exhibition of National Economic Achievements (Vdnkh) in Moscow, 1967.

UIG3904807

Futuristic vision of how a moon bound spacecraft (rocket) might be look. 1936

Futuristic vision of how a moon bound spacecraft (rocket) might be look. 1936

UIG1578663

New Horizons near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

New Horizons near 2014 MU69 - Artist's view - New Horizons near 2014 MU69 - Artwork - Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Artist's concept of the New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles)

Miller, Ron (b.1947)

PIX4946140

ExoMars rover and orbiter - Artist's view of the TGO probe (Trace Gas Orbiter) of the European ExoMars 2016 mission that will relay the communications of the Exomars 2020 rover. Artist's impression of the ExoMars 2020 rover (foreground), surface science platform (background) and the Trace Gas Orbiter (top). Not to scale

ExoMars rover and orbiter - Artist's view of the TGO probe (Trace Gas Orbiter) of the European ExoMars 2016 mission that will relay the communications of the Exomars 2020 rover. Artist's impression of the ExoMars 2020 rover (foreground), surface science platform (background) and the Trace Gas Orbiter (top). Not to scale

PIX4643654

Juno Probe - Artist's View - Juno Artist's Rendering - Artist's View of Juno Probe in orbit around Jupiter. Launch in 2011, the Juno probe will reach Jupiter in 2016. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. Juno will repeatedly dive between the planet and its intense belts of charged particle radiation, coming only 5,000 kilometers (about 3,000 miles) from the cloud tops at closest approach. Juno's primary goal is to improve our understanding of Jupiter's formation and evolution. The spacecraft will spend a year investigating the planet's origins, interior structure, deep atmosphere and magnetosphere. Juno's study of Jupiter will help us to understand the history of our own solar system and provide new insight into how planetary systems form and develop in our galaxy and beyond

Juno Probe - Artist's View - Juno Artist's Rendering - Artist's View of Juno Probe in orbit around Jupiter. Launch in 2011, the Juno probe will reach Jupiter in 2016. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. Juno will repeatedly dive between the planet and its intense belts of charged particle radiation, coming only 5,000 kilometers (about 3,000 miles) from the cloud tops at closest approach. Juno's primary goal is to improve our understanding of Jupiter's formation and evolution. The spacecraft will spend a year investigating the planet's origins, interior structure, deep atmosphere and magnetosphere. Juno's study of Jupiter will help us to understand the history of our own solar system and provide new insight into how planetary systems form and develop in our galaxy and beyond

PIX4605917

ExoMars 2016 mission - TGO probe in test - ExoMars Trace Gas Orbiter during tests: View of the TGO probe (Trace Gas Orbiter) of the European ExoMars mission, in anechoic chamber test at Thales Alenia, in Cannes on 5 March 2015. ESA's ExoMars Trace Gas Orbiter module is seen here during tests in the anechoic test chamber of Thales Alenia Space, in Cannes, France, on 5 March 2015. The Orbiter itself will remain in Mars orbit to image surface features and study the composition of the atmosphere. The first mission of the ExoMars programme, scheduled to arrive at March in 2016, consists of a Trace Gas Orbiter plus an Entry, Descent and Landing Demonstrator Module (EDM). The main objectives of this mission are to search for evidence of methane and other trace atmospheric gases that could be signatures of active biological or geological processes and to test key technologies in preparation for ESA's contribution to subsequent missions to Mars

ExoMars 2016 mission - TGO probe in test - ExoMars Trace Gas Orbiter during tests: View of the TGO probe (Trace Gas Orbiter) of the European ExoMars mission, in anechoic chamber test at Thales Alenia, in Cannes on 5 March 2015. ESA's ExoMars Trace Gas Orbiter module is seen here during tests in the anechoic test chamber of Thales Alenia Space, in Cannes, France, on 5 March 2015. The Orbiter itself will remain in Mars orbit to image surface features and study the composition of the atmosphere. The first mission of the ExoMars programme, scheduled to arrive at March in 2016, consists of a Trace Gas Orbiter plus an Entry, Descent and Landing Demonstrator Module (EDM). The main objectives of this mission are to search for evidence of methane and other trace atmospheric gases that could be signatures of active biological or geological processes and to test key technologies in preparation for ESA's contribution to subsequent missions to Mars

S. Corvaja

PIX4643641

Stardust probe and comet Wild 2 - Artist view - The Stardust probe and comet Wild 2 - Artist view - The Stardust probe was launched on February 7, 1999 with the primary objective of studying the comet Wild 2 and taking samples during a passage through the comet's hair. Stardust was the first probe to collect and bring back to Earth interstellar and cometary dust. The return capsule landed on Earth on 15 January 2006 with the samples. Stardust is an interplanetary spacecraft, whose primary purpose was to investigate the makeup of the comet Wild 2 and its coma. It was launched on February 07 1999 and returned to Earth on January 15 2006. It is the first sample return mission to collect cosmic dust and return the sample to Earth; the capsule contains cometary and interstellar samples gathered by the Stardust spacecraft

Stardust probe and comet Wild 2 - Artist view - The Stardust probe and comet Wild 2 - Artist view - The Stardust probe was launched on February 7, 1999 with the primary objective of studying the comet Wild 2 and taking samples during a passage through the comet's hair. Stardust was the first probe to collect and bring back to Earth interstellar and cometary dust. The return capsule landed on Earth on 15 January 2006 with the samples. Stardust is an interplanetary spacecraft, whose primary purpose was to investigate the makeup of the comet Wild 2 and its coma. It was launched on February 07 1999 and returned to Earth on January 15 2006. It is the first sample return mission to collect cosmic dust and return the sample to Earth; the capsule contains cometary and interstellar samples gathered by the Stardust spacecraft

PIX4607214

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

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NASA's Juno spacecraft provides a never-before-seen perspective on Jupiter's south pole, 2016

NASA's Juno spacecraft provides a never-before-seen perspective on Jupiter's south pole, 2016

UIG3508055

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643784

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643799

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69.

Miller, Ron (b.1947)

PIX4643810

Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars approaching the planet Mars, 2016. Artist view of the european spacecraft ExoMars approaching planet March in 2016

Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars approaching the planet Mars, 2016. Artist view of the european spacecraft ExoMars approaching planet March in 2016

D. Ducros

PIX4606971

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Artist view of the sovietic probe Mars 96 observing the planet Mars. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the soviet March 96 spacecraft above planet Mars. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Artist view of the sovietic probe Mars 96 observing the planet Mars. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the soviet March 96 spacecraft above planet Mars. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606422

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

PIX4605637

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

Pioneer 10 and Jupiter - Artist's View - Pioneer 10 probe and Jupiter - Artist view - Pioneer 10 was launched on March 3, 1972 with as its first destination, the Planet Jupiter, which it flew over on December 3, 1973; it was the first space probe to approach this planet; it was also the first space probe to leave the solar system. The Pioneer 10 and Pioneer 11 probes have embarked on a plate, called the Pioneer plate, containing a message intended for potential aliens. Artist rendition of the Pioneer F (Pioneer 10) spacecraft shown in orbit around Jupiter

PIX4605645

Comet 67P/Churyumov-Gerasimenko and Philae - Comet 67P/Churyumov-Gerasimenko nucleus with Philae: Detail of the surface of the nucleus of Comet 67P/Churyumov-Gerasimenko as seen on September 2, 2016 by the Rosetta probe. The Philae lander appears pose on the comet - Rosetta's lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel - Philae's 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae's orientation - A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked

Comet 67P/Churyumov-Gerasimenko and Philae - Comet 67P/Churyumov-Gerasimenko nucleus with Philae: Detail of the surface of the nucleus of Comet 67P/Churyumov-Gerasimenko as seen on September 2, 2016 by the Rosetta probe. The Philae lander appears pose on the comet - Rosetta's lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel - Philae's 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae's orientation - A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked

PIX4588652

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

Cassini - Huygens and Saturn - Cassini spacecraft at Saturn - Artist's view of the Cassini probe around Saturn. The Huygens European module is attached to the probe. The Cassini-Huygens probe was launched on 15 October 1997 and has been placed in orbit around Saturn since 1 July 2004. The great Cassini orbiter, with the Huygens probe still in place, prepares to slip through the ring plane of Saturn. Cassini - Huygens was launched from the earth on october 15 1997 and is orbiting Saturn system from july 1st 2004

PIX4606016

Diagram of the Soviet Space Probe Venera 1 Which Was Launched Towards Venus on February 12, 1961.

Diagram of the Soviet Space Probe Venera 1 Which Was Launched Towards Venus on February 12, 1961.

UIG3904364

how a moon bound spacecraft (rocket) would take off to return from the Moon to the Earth

how a moon bound spacecraft (rocket) would take off to return from the Moon to the Earth

UIG1578664

Artist's view of the New Horizons probe near Pluto - New Horizons over Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft approaches dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 15,000 miles from Pluto (upper right), 27,000 miles from its largest moon Charon (lower left) and 2.97 billion miles from the Earth. This side of the spacecraft on the left can be seen the Visibl

Artist's view of the New Horizons probe near Pluto - New Horizons over Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft approaches dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 15,000 miles from Pluto (upper right), 27,000 miles from its largest moon Charon (lower left) and 2.97 billion miles from the Earth. This side of the spacecraft on the left can be seen the Visibl

Walter B Myers

PIX4607323

Artist's view of the New Horizons probe near Pluto - New Horizons over Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft over dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 10,000 miles from Pluto (upper right), 22,000 miles from its largest moon Charon (upper left) and 2.97 billion miles from the Earth. Dominating this side of the spacecraft with an 8 inch aperture is th

Artist's view of the New Horizons probe near Pluto - New Horizons over Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft over dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 10,000 miles from Pluto (upper right), 22,000 miles from its largest moon Charon (upper left) and 2.97 billion miles from the Earth. Dominating this side of the spacecraft with an 8 inch aperture is th

Walter B Myers

PIX4607329

Le trou noir THE BLACK HOLE de Gary Nelson 1979

Le trou noir THE BLACK HOLE de Gary Nelson 1979

XRD1724706

Infrared image of the southern aurora of Jupiter, as captured by NASA's Juno spacecraft, 2016

Infrared image of the southern aurora of Jupiter, as captured by NASA's Juno spacecraft, 2016

UIG3508065

The Cassini and Saturn probe - Cassini spacecraft at Saturn: Artist's view of the Cassini probe around Saturn. - Artist's concept of Cassini orbiter crossing Saturn's ring plane

The Cassini and Saturn probe - Cassini spacecraft at Saturn: Artist's view of the Cassini probe around Saturn. - Artist's concept of Cassini orbiter crossing Saturn's ring plane

PIX4643481

Solar Sails - Artist View - Solar sails - Artist view - Artist view of probes using solar wind and photons emitted by the Sun as a means of propulsion. The spacecraft deploys a large membrane mirror which reflects light from the Sun, or some other source. The radiation pressure on the mirror provides a tiny amount of thrust by reflecting photons

Solar Sails - Artist View - Solar sails - Artist view - Artist view of probes using solar wind and photons emitted by the Sun as a means of propulsion. The spacecraft deploys a large membrane mirror which reflects light from the Sun, or some other source. The radiation pressure on the mirror provides a tiny amount of thrust by reflecting photons

P. Carril

PIX4640409

Mars Recognition Orbiter and the Comet, Artist view (photo)

Mars Recognition Orbiter and the Comet, Artist view (photo)

Steven Hobbs

PIX6039537

Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Artist impression of Solar Orbiter in front of the Sun (not to scale). Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. Solar Orbiter's over-arching mission goals are to examine how the Sun creates and controls the heliosphere, the extended atmosphere of the Sun in which we reside, and the effects of solar activity on it. Solar Orbiter is an ESA-led mission wit

Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Artist impression of Solar Orbiter in front of the Sun (not to scale). Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. Solar Orbiter's over-arching mission goals are to examine how the Sun creates and controls the heliosphere, the extended atmosphere of the Sun in which we reside, and the effects of solar activity on it. Solar Orbiter is an ESA-led mission wit

PIX4643802

Jupiter Icy Moon Explorer (JUICE) Probe - Artist's view - Jupiter Icy Moon Explorer or JUICE (formerly JGO and EJSM/Laplace) is a space mission of the European Space Agency to be launched in 2022 towards the moons of Jupiter by an Ariane 5 rocket. This space probe is to study by flying over them several times three of the ice moons of Jupiter - Callisto, Europe and Ganymede. The Jupiter iY moons Explorer (JUICE) is an interplanetary spacecraft in development by the European Space Agency (ESA). The mission is being developed to visit the Jovian system focused on studying three of Jupiter's Galilean moons: Ganymede, Callisto, and Europa all of which are thought to have significant bodies of liquid water beneath their surfaces, making them potentially habitable environments.The spacecraft is set for launch in 2022 and would reach Jupiter in 2030

Jupiter Icy Moon Explorer (JUICE) Probe - Artist's view - Jupiter Icy Moon Explorer or JUICE (formerly JGO and EJSM/Laplace) is a space mission of the European Space Agency to be launched in 2022 towards the moons of Jupiter by an Ariane 5 rocket. This space probe is to study by flying over them several times three of the ice moons of Jupiter - Callisto, Europe and Ganymede. The Jupiter iY moons Explorer (JUICE) is an interplanetary spacecraft in development by the European Space Agency (ESA). The mission is being developed to visit the Jovian system focused on studying three of Jupiter's Galilean moons: Ganymede, Callisto, and Europa all of which are thought to have significant bodies of liquid water beneath their surfaces, making them potentially habitable environments.The spacecraft is set for launch in 2022 and would reach Jupiter in 2030

PIX4605908

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

PIX4606652

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

PIX4607314

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

PIX4607330

Pioneer Venus orbiter - Artist view - Pioneer Venus orbiter - Artist view - The Pioneer Venus Project was a NASA space exploration mission to Venus launched in 1978. It consisted of two separate probes, one to study Venus from its orbit (Pioneer Venus Orbiter) and the other to analyze the atmosphere of the planet through 4 atmospheric probes (Pioneer Venus Multiprobe). An artist concept of the orbiter approaching Venus is shown here

Pioneer Venus orbiter - Artist view - Pioneer Venus orbiter - Artist view - The Pioneer Venus Project was a NASA space exploration mission to Venus launched in 1978. It consisted of two separate probes, one to study Venus from its orbit (Pioneer Venus Orbiter) and the other to analyze the atmosphere of the planet through 4 atmospheric probes (Pioneer Venus Multiprobe). An artist concept of the orbiter approaching Venus is shown here

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Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

Mars Express - Artist's View - Mars Express artist's view - The European Mars Express probe was launched on June 2, 2003 and began its observations in March early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004

D. Ducros

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Trajectory of the Ulysses probe, launched by Europeans to study the Sun.: The Ulysses probe - Ulysses spacecraft trajectory- Artwork

Trajectory of the Ulysses probe, launched by Europeans to study the Sun.: The Ulysses probe - Ulysses spacecraft trajectory- Artwork

L. Bret

PIX4643812

Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Esa's Solar Orbiter is set to provide new views of our star, in particular providing close-up observations of the Sun's poles. Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. An artist's impression of Solar Orbiter in front of the stormy Sun is depicted here

Solar Orbiter - Solar Orbiter is a solar observation satellite of the European Space Agency (ESA) developed with the participation of NASA, which is scheduled to launch in February 2019 and begin observations around 2022. The main objective of this scientific mission is to study the processes behind the solar wind, the heliospheric magnetic field, the energetic solar particles and the magnetic field of the Sun. Esa's Solar Orbiter is set to provide new views of our star, in particular providing close-up observations of the Sun's poles. Following its launch in February 2019 and three-year journey using gravity swingbys at Earth and Venus, Solar Orbiter will operate from an elliptical orbit around the Sun. At its closest it will approach our star within 42 million kilometers, closer than planet Mercury. An artist's impression of Solar Orbiter in front of the stormy Sun is depicted here

PIX4643821

Solar Probe Plus: Solar Probe Plus is a NASA space mission to study the solar crown. The Solar Probe Plus spacecraft with solar panels folded into the shadows of its protective shield, gathers data on its approach to the Sun - NASA has begun development of a mission to visit and study the sun closer than ever before. The unprecedented project, named Solar Probe Plus, is slated to launch no later than 2018

Solar Probe Plus: Solar Probe Plus is a NASA space mission to study the solar crown. The Solar Probe Plus spacecraft with solar panels folded into the shadows of its protective shield, gathers data on its approach to the Sun - NASA has begun development of a mission to visit and study the sun closer than ever before. The unprecedented project, named Solar Probe Plus, is slated to launch no later than 2018

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European astronaut on Mars - Illustration - European female astronaut on Mars - Illustration - A European astronaut finds the Rover Pasteur of the EXOMARS mission. Artist's view. An european astronaut finds the Rover Pasteur of the EXOMARS mission

European astronaut on Mars - Illustration - European female astronaut on Mars - Illustration - A European astronaut finds the Rover Pasteur of the EXOMARS mission. Artist's view. An european astronaut finds the Rover Pasteur of the EXOMARS mission

P. Carril

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