\n\tAfter traveling 1.7 billion miles over four years, NASA’s Dawn spacecraft has begun sending images of the asteroid Vesta back to Earth. NASA will begin the investigation of Vesta in more detail after it maneuvers the spacecraft into an orbit about 1,700 miles from the asteroid.
\n
\n\tHere is the first full-frame photo of Vesta taken on July 24 from a distance of about 3,200 miles. Vesta is abou 114 million miles from Earth.
\n
\n\t”We have been calling Vesta the smallest terrestrial planet,” said Chris Russell, Dawn’s principal investigator at UCLA. “The latest imagery provides much justification for our expectations. They show that a variety of processes were once at work on the surface of Vesta and provide extensive evidence for Vesta’s planetary aspirations.”
\n
\n\tNASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tThis view of the dark side of Vesta was taken from a distance of about 3,200 miles.
\n
\n\tNASA describes the instruments brought aboard Dawn:
\n
\n\t”In addition to the framing camera, Dawn’s instruments include the gamma ray and neutron detector and the visible and infrared mapping spectrometer. The gamma ray and neutron detector uses 21 sensors with a very wide field of view to measure the energy of subatomic particles emitted by the elements in the upper yard (meter) of the asteroid’s surface. The visible and infrared mapping spectrometer will measure the surface mineralogy of both Vesta and Dawn’s next target, the dwarf planet Ceres.”
\n
\n\tImage credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tHere’s an image of the south pole of Vesta.
\n
\n\tImage credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tThis set of three craters is in the northern hemisphere of Vesta. They’ve been nicknamed “Snowman.”
\n
\n\tImage credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tThe south equatorial region shows some interesting craters.
\n
\n\tImage credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tThe south polar region and its large bump is shown by Dawn days before it arrived at Vesta.
\n
\n\tImage credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tHere’s the size of Vesta compared to the 8 other asteroids that humans have made close contact with.
\n\tOne of Dawn’s first images of Vesta on its approach shows the large bump on its surface.
\n
\n\tImage credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tVesta’s equatorial region is marked by grooves.
\n
\n\tImage credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
\n\tThis is what Vesta looks like from Earth courtesy of the Hubble Space Telescope.
\n\tThis should give you an indication of the size of the Dawn spacecraft as scientists prepared it for launch.
\n\tHere is the Dawn spacecraft with its ion propulsion system installed.
\n\tThe ion propulsion system goes through a test on Earth. Dawn has three 30-centimeter-diameter (12-inch) ion thrust units. It produces an electrical charge to accelerate ions from xenon fuel that will be 10 times faster than chemical fuel.
\n
\n\tThe spacecraft uses only 10 ounces of fuel per day and would accelerate on an Earth highway from 0 to 60 miles per hour in 4 days. But without gravity in space, its got speed to burn.
\n\tHere’s what the Dawn spacecraft must look like with its solar panels fully extended as it orbits Vesta.
\n\tDawn’s next target will be the dwarf planet Ceres – seen here through the Hubble.
