https://www.jpl.nasa.gov/news/news.php?feature=6766

Dawn Identifies Age of Ceres' Brightest Area
Jet Propulsion Laboratory
March 8, 2017

The bright central area of Ceres' Occator Crater, known as Cerealia Facula, 
is approximately 30 million years younger than the crater in which it 
lies, according to a new study in the Astronomical Journal. Scientists 
used data from NASA's Dawn spacecraft to analyze Occator's central dome 
in detail, concluding that this intriguing bright feature on the dwarf 
planet is only about 4 million years old -- quite recent in terms of geological 
history.

Researchers led by Andreas Nathues at the Max Planck Institute for Solar 
System Research (MPS) in Gottingen, Germany, analyzed data from two instruments 
on board NASA's Dawn spacecraft: the framing camera, and the visible and 
infrared mapping spectrometer.

The new study supports earlier interpretations from the Dawn team that 
this reflective material -- comprising the brightest area on all of Ceres 
-- is made of carbonate salts, although it did not confirm a particular 
type of carbonate previously identified. The secondary, smaller bright 
areas of Occator, called Vinalia Faculae, are comprised of a mixture of 
carbonates and dark material, the study authors wrote.

New evidence also suggests that Occator's bright dome likely rose in a 
process that took place over a long period of time, rather than forming 
in a single event. They believe the initial trigger was the impact that 
dug out the crater itself, causing briny liquid to rise closer to the 
surface. Water and dissolved gases, such as carbon dioxide and methane, 
came up and created a vent system. These rising gases also could have 
forced carbonate-rich materials to ascend toward the surface. During this 
period, the bright material would have erupted through fractures, eventually 
forming the dome that we see today.

Read more from MPS

The spacecraft is currently on its way to a high-altitude orbit of 12,400 
miles (20,000 kilometers), and to a different orbital plane. In late spring, 
Dawn will view Ceres in "opposition," with the sun directly behind the 
spacecraft. By measuring details of the brightness of the salt deposits 
in this new geometry, scientists may gain even more insights into these 
captivating bright areas.

The Dawn mission is managed by JPL for NASA's Science Mission Directorate 
in Washington. Dawn is a project of the directorate's Discovery Program, 
managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. 
UCLA is responsible for overall Dawn mission science. Orbital ATK Inc., 
in Dulles, Virginia, designed and built the spacecraft. The German Aerospace 
Center, Max Planck Institute for Solar System Research, Italian Space 
Agency and Italian National Astrophysical Institute are international 
partners on the mission team. For a complete list of mission participants, 
visit:

http://dawn.jpl.nasa.gov/mission

More information about Dawn is available at the following sites:

http://www.nasa.gov/dawn

http://dawn.jpl.nasa.gov


News Media Contact
Elizabeth Landau
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6425
elizabeth.lan...@jpl.nasa.gov

2017-059

______________________________________________

Visit our Facebook page https://www.facebook.com/meteoritecentral and the 
Archives at http://www.meteorite-list-archives.com
Meteorite-list mailing list
Meteorite-list@meteoritecentral.com
https://pairlist3.pair.net/mailman/listinfo/meteorite-list

Reply via email to