2019-07-01_neScholar

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planetary formation in the asteroid belt
between Mars and Jupiter.

Structure

Ceres is more similar to the terrestrial
planets (Mercury, Venus, Earth and
Mars) than its asteroid neighbors,
but it is much less dense. One of the
similarities is a layered interior, but
Ceres’ layers aren’t as clearly defined.
Ceres probably has a solid core and a
mantle made of water ice. In fact, Ceres
could be composed of as much as 25
percent water. If that is correct, Ceres
has more water than Earth does. Ceres’
crust is rocky and dusty with large salt
deposits. The salts on Ceres aren’t like
table salt (sodium chloride), but instead
are made of different minerals like
magnesium sulfate.

Surface

Ceres is covered in countless small,
young craters, but none are larger than
175 miles (280 kilometers) in diameter.
This is surprising, given that the dwarf
planet must have been hit by numerous
large asteroids during its 4.5 billion-year
lifetime.

The lack of craters might be due to
layers of ice just below the surface.
The surface features could smooth
out over time if ice or another lower-
density material, such as salt, is just
below the surface. It’s also possible that
past hydrothermal activity, such as ice
volcanoes, erased some large craters.

Within some of Ceres’ craters, there are
regions that are always in shadow. It’s
possible that without direct sunlight,
these “cold traps” could have water ice
in them for long periods of time.

Atmosphere

Ceres has a very thin atmosphere, and
there is evidence it contains water
vapor. The vapor may be produced by
ice volcanoes or by ice near the surface
sublimating (transforming from solid to
gas).

Potential for Life

Ceres is one of the few places in our
solar system where scientists would like
to search for possible signs of life. Ceres
has something a lot of other planets
don’t: water. Here on Earth, water is
essential for life, so it’s possible that
with this ingredient and a few other
conditions met, life could maybe exist
there. Living things on Ceres, if they are
there at all, would likely be very small
microbes similar to bacteria. And while
Ceres might not have living things

Researchers from NASA's Dawn mission have composed the first comprehensive views of the north (left) and south pole regions (right) of
dwarf planet Ceres, using images obtained by the Dawn spacecraft. The images were taken between Aug. 17 and Oct. 23, 2015, from an
altitude of 915 miles (1,470 kilometers).

The region around the south pole appears black in this view because this area has been in shade ever since Dawn's arrival on March 6,
2015, and is therefore not visible. At the north polar region, craters Jarovit, Ghanan and Asari are visible, as well as the mountain Ysolo
Mons. Near the south pole, craters Attis and Zadeni can be seen.

Detailed maps of the polar regions allow researchers to study the craters in this area and compare them to those covering other parts of
Ceres. Variations in shape and complexity can point to different surface compositions. In addition, the bottoms of some craters located close
to the poles receive no sunlight throughout Ceres' orbit around the sun. Scientists want to investigate whether surface ice can be found
there.
Image Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

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