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Images of 'Spaceprobe' found, 236

The probes Osiris-Rex and Hayabusa 2 - Artist's view - Osiris-rex and Hayabusa 2 - Artwork: Artist's view of the probe Osiris-Rex near the asteroid Bennu (right) and the probe Hayabusa 2 near the asteroid (162173) Ryugu (upper left). OSIRIS-REX was launched on 8 September 2016 to reach the asteroid Bennu in 2018 and bring a sample back to Earth in 2023. Hayabusa 2 is a space probe of JAXA, the Japanese space agency, launched in December 2014, which will study the asteroid (162173) Ryugu from July 2018 to February 2019 and bring a sample to Earth in December 2020. Osiris-rex will travel to a near-earth asteroid called Bennu and bring a small sample back to Earth for study. It was launched on Sep 8, 2016. As planned, the spacecraft will reach its asteroid target in 2018 and return a sample to Earth in 2023. Hayabusa2 is an asteroid sample return mission operated by the Japanese space agency, JAXA. Launched in December 2014 Hayabusa 2 is expected to arrive at the asteroid 162173 Ryugu in July 2018, survey the asteroid for a year and a half, depart in December 2019, and return to Earth in December 2020
Voyager and Exoplanets Probe - Voyager entering an alien solar system  Artist's view showing one of the probes approaching another solar system
Rover Curiosity on Mars - Curiosity Mars rover selfie - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of images taken by the robot on August 5, 2015. This low-angle self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the site from which it reached down to drill into a rock target called “” Buckskin”” on lower Mount Sharp. The selfie combines several component images taken by Curiosity's Mars Hand Lens Imager (MAHLI) on Aug. 5, 2015, during the 1,065th Martian day, or sol, of the rover's work on Mars. For scale, the rover's wheels are 20 inches (50 centimeters) in diameter and about 16 inches (40 centimeters) wide
Mars Express probe - Artist's View - Mars Express artist's view - The European probe Mars Express leaves the Earth propelled by the upper floor Fregat. This probe was launched on 2 June 2003 and began its observations in 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 was mounted on the Fregat upper stage. Most of the energy needed to propel Mars Express from Earth to Mars is provided by the four - stage Soyuz/Fregat launcher. The Fregat upper stage separated from the spacecraft after placed it on a Mars - bound trajectory
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
The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected, the probe measures 32 meters with its panels deployed, the core of the comet about 4 km. Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko. The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays, while the comet nucleus is thought to be about 4 km wide
Solar Orbiter (photo)
Mars Exploration Rover - Mars Exploration Rover is a Martian exploration mission composed of two probes housing two identical rovers, Spirit and Opportunity MER - A, the Spirit robot launched on June 10, 2003, landed on January 3, 2004 in the crater Gusev. MER - B, the Opportunity robot launched on July 8, 2003, landed on January 24, 2004 on Meridiani Planum. The sun rises behind one of the Mars Exploration Rovers as it prepares to analyse a rock with its RAT tool. Mars Exploration Rover (MER) is a robotic mission which aims to explore the Martian surface and geology. The mission began with the sending of two twin rovers: MER - A (Spirit), launched on June 10 2003 and landed on January 03 2004 in Gusev crater; MER - B (Opportunity) launched on July 08 2003 and landed on January 24 2004 at Meridiani Planum
Artist's view of the New Horizons probe and a Kuiper object - The New Horizons spacecraft near Kuiper Belt Object - Artist's view of the New Horizons probe approaching a Kuiper object. The Sun shines more than 6 billion km surrounded by a disc of dust. Jupiter and Neptune appear as two stars to the right of the Sun. 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. Artist's impression of the New Horizons spacecraft encountering a Kuiper Belt object. The Sun, more than 4.1 billion miles (6.7 billion kilometers) away, shines as a bright star embedded in the glow of the zodiacal dust cloud. Jupiter and Neptune are visible as orange and blue “” stars””” to the right of the Sun. Although you would not actually see the myriad other objects that make up the Kuiper Belt because they are so far apart, they are shown here to give the impression of an extensive disk of icy worlds beyond Neptune
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
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - 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. 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
Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory
The Osiris-Rex probe and the Bennu asteroid - Artist's view - OSIRIS-REx near asteroid Bennu - Artwork: Artist's view of the Osiris-Rex probe near the Asteroid Bennu - OSIRIS-REx is to be launched on September 8, 2016 to reach the Asteroid Bennu in 2018 and bring a sample back to Earth in 2023 - OSiRIS-Osiris-Osiris-Osiris-Osiris-Rex in 2023 Ris-rex will travel to a near-earth asteroid called Bennu and bring a small sample back to Earth for study. The mission is scheduled to launch Sep 8, 2016. As planned, the spacecraft will reach its asteroid target in 2018 and return a sample to Earth in 2023
The Dawn probe near Ceres - Artist's view - Dawn approaches Ceres - Artist view of the Dawn probe near the dwarf planet Ceres. In February 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn's three xenon electrostatic ion thrusters can be seen emitting ionized xenon's characteristic blue/magenta glow, gently propelling the probe toward Ceres. While the ion engines have relatively low specific thrust (about equal to the weight of a few sheets of paper), they can operate continuously for long periods making efficient use of the approximately 1,000 pounds of xenon propellant onboard. The wing - like solar arrays produce about 1,300 watts for probe's propulsion and other electrical systems. While no close - up observations of yet been made of Ceres itself, here it is rendered as appearing similar to a much smaller version of the Earth's Moon, heavily cratered with the addition of surface water ice and hypothesized plumes of ice crystals from water geysers on its surface
Model of the Voyager space probe.
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
Rover Curiosity on Mars - Curiosity Mars rover selfie: Mars Science Laboratory (MSL), named Curiosity, is a NASA rover exploring the surface of Mars. This self-portrait is a composite of a dozen images taken by the robot on October 6, 2015. This self-portrait of Nasa's Curiosity Mars rover shows the vehicle at the “” Big Sky”” site, where its drill collected the mission's fifth taste of Mount Sharp. The scene combines dozens of images taken during the 1,126th Martian day, or sol, of Curiosity's work on Mars (Oct. 6, 2015, PDT), by the Mars Hand Lens Imager (MAHLI) camera at the end of the rover's robotic arm. The rock drilled at this site is sandstone in the Stimson geological unit inside Gale Crater. The view is centered toward the west-northwest. It does not include the rover's robotic arm, though the shadow of the arm is visible on the ground. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot in the images, or portions of images, that were used in this mosaic. This portrait of the rover was designed to show the Chemistry and Camera (ChemCam) instrument atop the rover appearing level. This causes the horizon to appear to tilt toward the left, but in reality it is fairly flat. For scale, the rod's wheels are 20 inches (50 centimeters) in diameter and about 16 inches (40 centimeters) wide. The drilled hole in the rock, appearing grey near the lower left corner of the image, is 0.63 inch (1.6 centimeters) in diameter
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
Voyager space probe: Nasa's Voyager 1 spacecraft entering interstellar space
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 communications
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
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.
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 the Long - Range Reconnaissance Imager (LORRI), a digital camera with a large telephoto telescope fortified to operate in the cold, hostile environs of deep space. At 90 days before closest approach to Pluto, Lorri's images will surpass the quality of the best Hubble Space Telescope images of Pluto. While little is known about Pluto's appearance, here this Kuiper belt dwarf planet is realized as a frozen world covered with various ices, hosting a thin atmosphere of nitrogen, methane and other hydrocarbons too possibly, with a significantly weathered surface as Pluto's 248 - year orbit alternately brings it closer then further from the warmth of the sun
Exploration of Titan - Illustration - Looking for life on Titan - An automatic probe explores a hydrocarbon marsh in search of traces of life. A robotic probe explores a frigid ethane lake on Titan. Like the European Space Agency's Huygens probe, this probe carries its own light source as the surface of Titan is only 0.1 percent as bright as the Earth's. Titan is host to a plethora of organic (carbon - based) compounds, hence this is one of the few places in the Solar System where life outside of the Earth may have evolved. In many ways, Titan resemble a frozen primordial Earth, though the greatest obstacle to Titan harboring life - - as we know it - - is the extreme cold. Even though all the chemical ingredients are present, Titan simply may not be warm enough to initiate the chemical reactions required for life. Perhaps sometime in the next decades such a mission to Titan will be a reality
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)
The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Scenario of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere
Europa Jupiter System Mission (EJSM) - Artist view - Europa Jupiter System Mission (EJSM) - Artist view - Artist view of the EJSM (Europa Jupiter System Mission) mission, with Nasa's Jupiter Europa Orbiter (JEO) probe and ESA's Jupiter Ganymede Orbiter (JGO) probe. This mission proposes an in-depth exploration of Jupiter's system and its moons to study the emergence of habitable worlds around giant planets. JEO will explore Jupiter and the Io satellite, then further study Europe; JGO will explore Jupiter and the Callisto moon and will enter into orbit around Ganymede for a comprehensive and detailed study. Launch planned around 2020. Artist's concept of the two Europa Jupiter System Mission spacecraft - Nasa's Jupiter Europa Orbiter (JEO) and the European Space Agency's Jupiter Ganymede Orbiter (JGO) exploring the Jupiter system. Possible launch in 2020
The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (back view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory