NASA’s Dawn Gets Best Look Yet at Ceres

The raw image taken by Dawn while it was 383,000km from Ceres. (PHOTO CREDIT: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

Between the orbits of Mars and Jupiter spins an asteroid belt, and in that asteroid belt is the inner solar system’s dwarf planet. Ceres makes up a third of the asteroid belt’s mass, and, with a diameter of 950 kilometres (590 miles), it was originally thought to have been a planet on its discovery in 1801.

Now, astronomers believe that Ceres is a protoplanet. A protoplanet is a planetary embryo, formed inside a star’s protoplanetary disc during the creation of the solar system. It has a differentiated interior produced by internal melting, but that isn’t big enough to be given full planet status.

NASA believes that studying Ceres — about which relatively little is known, compared to the rest of the solar system — will provide vital information about the formation of our own solar system.

This is the goal of the Dawn probe, launched in 2007 to study the two largest objects in the asteroid belt — the protoplanet Vesta (with a diameter of 525 kilometres, or 326 miles) and Ceres.

Dawn left Vesta’s orbit on September 5, 2012, with over 30,000 images of the protoplanet under its belt, and is due to reach Ceres on March 6, 2015. As it approaches the dwarf planet, it will be snapping a series of better and better images for navigation purposes — but they will also provide early clues about Ceres.

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Michelle Starr