Emily LakdawallaDec 05, 2014

Ceres is round!

Okay, so the fact that Ceres is round is not news. It's still thrilling to see Ceres begin to come into focus as a round world. This first image shows the full size of Dawn's Framing Camera photo, with Ceres just a speck in the center:

Dawn's view of Ceres on December 1, 2014
Dawn's view of Ceres on December 1, 2014 Dawn took this photo of Ceres from a distance of 1.2 million kilometers as it approached for its 2015 rendezvous. NASA / JPL / UCLA / MPS / DLR / IDA

Let's zoom in, enlarging but keeping the original pixels. Ceres spans just 8 or 9 pixels, but that's enough to show a gibbous phase of a round world.

Dawn's view of Ceres on December 1, 2014 (detail)
Dawn's view of Ceres on December 1, 2014 (detail) NASA / JPL / UCLA / MPS / DLR / IDA

Round is so important to geologists. Round means that the force of gravity has overcome the strength of the materials that make up Ceres, squishing it together and forcing its surface to be approximately flat, according to the local force of gravity; over time, that makes a world round, not quite spherical, but bulging slightly at the equator. This reshaping by gravity generates heat in a couple of different ways, and heat encourages planetary materials to flow faster, sometimes even melting. Ceres will have tectonic features, maybe even an internal ocean. Or there were such features, once. Ceres' surface will have recorded those changes. It remains for Dawn to see whether those recordings have been preserved across geologic time, leaving a record that we, back on Earth, can decipher.

Dawn took the photo on December 1 from a distance of 1.2 million kilometers. That is actually not very far away, as deep-space distances go; for context, Titan orbits Saturn at a distance of 1.2 million kilometers. Dawn is really, really close, and getting closer every day. For more on its approach to Ceres, read Marc Rayman's most recent Dawn Journal. For more photos of Ceres, just stay tuned!

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