This is the set of images |
New Horizons’ location in the Kuiper Belt gives the spacecraft a uniquely oblique view of the small planets like Quaoar orbiting so far from the sun. When these images were taken, Quaoar was approximately 4 billion miles (6.4 billion kilometers) from the sun and 1.3 billion miles (2.1 billion kilometers) from New Horizons. With the oblique view available from New Horizons, LORRI sees only a portion of Quaoar’s illuminated surface, which is very different from the nearly fully illuminated view of the dwarf planet from Earth. Comparing Quaoar from the two very different perspectives gives mission scientists a valuable opportunity to study the light-scattering properties of Quaoar’s surface.
In addition to many background stars, two far away galaxies – IC 1048 and UGC 09485, each about 370 billion times farther from New Horizons than Quaoar – are also visible in these images. Unlike the galaxies and stars, Quaoar appears to move across the background scene due to its much closer distance. Other objects which appear to move in these images are camera artifacts.
In June the New Horizons mission received the go-ahead to fly onward to 2014 MU69 -- considered one of the early building blocks of the solar system -- with a planned rendezvous of Jan. 1, 2019.
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