Did a Giant Impact Make the Martian Moons?

In summary, the moons of Mars may have been captured asteroids or may have formed after the planet was formed from the debris of a large impactor.
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CygnusX-1
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by Ken Croswell

The Martian moons look like asteroids—dark, crater-pocked, and potato-shaped—suggesting Mars had snatched them from the nearby asteroid belt. But now planetary scientists have conducted the first computer simulations that bolster a controversial alternative idea: The satellites formed as our own moon did, after a big object smashed into the planet and kicked up debris.

Full story: ScienceNOW
 
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CygnusX-1 said:
by Ken Croswell

The Martian moons look like asteroids—dark, crater-pocked, and potato-shaped—suggesting Mars had snatched them from the nearby asteroid belt. But now planetary scientists have conducted the first computer simulations that bolster a controversial alternative idea: The satellites formed as our own moon did, after a big object smashed into the planet and kicked up debris.

Full story: ScienceNOW
There are four different hypotheses being proposed:
  1. Phobos and Deimos were captured asteroids; or
  2. Phobos and Deimos formed during the accretion process that created Mars; or
  3. Phobos and Deimos are second-generation Solar System objects that coalesced in orbit after Mars formed, rather than forming concurrently out of the same birth cloud as Mars; or
  4. Phobos and Deimos are debris from a large impactor on Mars (similar to the Terra/Theia impact that created our moon).
The near-circular orbits of the two moons are very near to Mars' equator, which makes it difficult to reconcile in the capture theory. The problem with option #2 is that both Phobos and Deimos are spectroscopically different from Mars. Furthermore, Phobos is spectroscopically different from the asteroids in the asteroid belt. Deimos is spectroscopically similar to D-Class asteroids in the asteroid belt. If Phobos and Deimos were the debris from a large impactor on Mars, then they should both be chemically similar, but they are not. With regard to the second-generation object theory, I was not able to find a paper on the subject, just a quotation from Dr. Martin Pätzold, from the University of Cologne, Germany, and Principal Investigator of the Mars Radio Science (MaRS) experiment: http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Phobos_flyby_success

See also:
Capture of Phobos and Deimos by Photoatmospheric Drag - Icarus, Volume 37, Issue 1, January 1979, Pages 113–123 (paid subscription)
http://[URL ']Formation of Phobos and Deimos via a Giant Impact[/URL] - Icarus, Volume 252, May 2015, Pages 334-338 (paid subscription) (arXiv free reprint)
 
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1. What evidence supports the theory that a giant impact created the Martian moons?

Scientists have found that Phobos and Deimos, the two moons of Mars, have a composition similar to that of C-type asteroids. This supports the theory that they were formed from debris left over from a giant impact on Mars.

2. How long ago did the giant impact occur on Mars?

Based on the age of the Martian surface, it is estimated that the giant impact occurred around 4.3 billion years ago. This is consistent with the formation of other planetary bodies in our solar system.

3. What would have happened to Mars after the giant impact?

The impact would have caused a significant amount of material to be ejected from Mars, which could have potentially formed a ring around the planet. This material could have also contributed to the formation of other moons or smaller satellites around Mars.

4. Could the Martian moons eventually crash back into the planet?

Yes, it is possible that Phobos and Deimos could eventually crash back into Mars. In fact, Phobos is gradually moving closer to Mars and is expected to crash into the planet in around 50 million years.

5. How does the giant impact theory explain the unusual orbit and shape of the Martian moons?

The giant impact theory suggests that the debris from the impact would have formed a disk around Mars, which eventually coalesced into the Martian moons. This could explain why the moons have an irregular shape and orbit close to the planet.

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