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Mars Had an Ancient Impact Like Earth

quixote9 writes "The BBC reports on a set of Nature articles showing that Mars had an impact about four billion years ago by a huge asteroid. This was about the same time that a much bigger object slammed into the Earth, throwing material into orbit around our infant planet. This material is thought to have coalesced to form the Moon. 'It happened probably right at the end of the formation of the four terrestrial planets — Mercury, Venus, Earth and Mars,' said Craig Agnor, a co-author on the Francis Nimmo study. 'In terms of the process of the planets sweeping up the last bits of debris, this could have been one of the last big bits of debris.' There's a theory that having a big moon is important to the development of life, because the much bigger tides create a bigger intertidal zone, but people used to think having a huge Moon like ours was a once-in-a-universe event."

8 of 167 comments (clear)

  1. Re:Hopefully. by MBGMorden · · Score: 4, Informative

    Not sure if that was a joke, but Pluto's composition is far too different from Mars for that to have been the case. Besides, singling out Pluto isn't really rational. Pluto was demoted from planetary status precisely because Pluto isn't that special. It's just one of a whole bunch of similar objects out in the Kuiper Belt.

    --
    "People who think they know everything are very annoying to those of us who do."-Mark Twain
  2. Re:Hopefully. by Fox_1 · · Score: 4, Informative

    That bit in the summary about a 'huge' moon like ours and it being a once in a universe event is garbage/FUD added to the real story about an asteroid/small body 's collision with Mars.
    People used to believe the world was flat but we don't need to throw that crap into every story about mapping or GPS.
    IF you RTFA then you'll find no mention of some freaking 'Huge' moon being necessary to life. I suspect whoever wrote the Slashdot summary read too much Issac Asimov from the 60's, and wanted to seem 'SMRT'.
    Check it out here

    --
    The rock, the vulture, and the chain
  3. Re:Impact Scale by Migraineman · · Score: 4, Informative
    A related article over at SpaceFlightNow indicates that the researchers were specifically looking for a scenario that wouldn't vaporize Mars. And I quote:

    "We set out to show that it's possible to make a big hole without melting the majority of the surface of Mars," Aharonson says. The team modeled a range of projectile parameters that could yield a cavity the size and ellipticity of the Mars lowlands without melting the whole planet or making a crater rim.

    After cranking 500 simulations combining various energies, velocities, and impact angles through the GPS division's Beowulf-class computer cluster CITerra, the researchers narrowed in on a "sweet spot"--a range of single-impact parameters that would make exactly the type of crater found on Mars. Although a large impact had been suggested (and discounted) in the past, Aharonson says, computers weren't fast enough to run the models. "The ability to search for parameters that allow an impact compatible with observations is enabled by the dedicated machine at Caltech," he adds.
    So planetary destruction isn't guaranteed, though 10^29 Joules is an incomprehensible amount of energy. Saying it was 100 billion gigatons of TNT might as well be "a gazillion tons" ... though I wonder if that's a metric ton or an imperial ton.
  4. Re:Maybe it was the same collision by MBGMorden · · Score: 5, Informative

    The two colliding bodies generally merge. IE, "Earth" as we know it didn't really collide with some foreign object that went skipping off into space again. "Earth Mark I" was a somewhat different planet whose remains are still here with us, and it collided with a very large object (essentially a planet in it's own right) called Theia (or sometimes aka Orpheus). Those two would have merged and the collision throw up the debris that formed the moon (which is also made up of parts of both)

    So there is no search for the object that hit Earth to form the moon. It's still here with us as part of the new Earth, and Theia/Orpheus is essentially our original planet as well; it's just easier to call the bigger planet involved in that collision "Earth" because, well, it was the bigger of the two.

    The same is likely true of Mars - the object that struck it probably merged with it.

    As an interesting note, it's also thought that a large impact must have struck Venus as well, and must have hit it hard enough to "flip" the planet, as Venus, compared to every other planet in the solar system, rotates "backwards". There were some BIG things floating around and colliding in the early Solar system.

    --
    "People who think they know everything are very annoying to those of us who do."-Mark Twain
  5. Re:Maybe it was the same collision by Bemopolis · · Score: 4, Informative

    Now I wonder tho... just how close would they have to come to each other in order to have mingling gravity completely tear apart the surface of each... Mayhaps a collision isn't necessary after all.
    The Roche limit for an Earth-Mars interaction is about 1.4 Earth radii (by comparison, the Moon is about 60 Earth radii away.) So, pretty damn close.
    --
    "I guess the moral of the story is, don't paint your airship with rocket fuel." -- Addison Bain
  6. Re:Once in a universe? by MBGMorden · · Score: 4, Informative

    Pluto and Charon aren't formed the same way. Charon really isn't even a "moon" at all, since rather than it orbiting Pluto, the center of mass is well between the two of them, and instead they orbit each other. They were almost certain separate bodies that simply became gravitationally bound to each other.

    As well, Charon, in the inner solar system, wouldn't make much of a moon at all. The higher heat would essentially turn it into a comet that would melt away much of it's surface area, and reduce it's already pretty low mass.

    Though I'm not sure about "once in a universe" odds, for 1 very, very large rock to become gravitationally bound in a STABLE orbit around another, without the two impacting (or, this system forming as a result of an impact), does seem like it'd be incredibly rare. Again though, "seeming" incredibly rare is indeed a guess on my part, and our sample size isn't large enough to really determine just how common it is.

    --
    "People who think they know everything are very annoying to those of us who do."-Mark Twain
  7. Re:Once in a universe? by cruachan · · Score: 5, Informative

    I seem to recall that a mechanism had been proposed whereby the material for the colliding body collected at a Trojan point, from which is was dislodged once it reached sufficient size - after which collision with the proto-earth would be just about inevitable. If the mars collider formed in the same way then collision with a large body could be pretty much normal in our sort of system and the incidence of large moons might be very high indeed.

  8. The moon does a lot of different things... by clonan · · Score: 4, Informative

    There are several things that our extremely large moon does for us that make life much more comfortable.

    #1 is of course tides that are more extreme than the sun could generate

    #2 rotational speed. The moon has kept our rotation from slowing as much as it should have. Shorter day/night cycles are important for environmental management.

    #3 atmosphere. The moon helped reduce the density of proto-earth's atmosphere. Without it we probably would resemble Venus.

    #4 plate tectonics. The tidal influence on the crust heats up the mantel and keeps the plates from sealing

    #5 protection. The moon intercepts a large percentage of the impacts destined for earth. This reduces the disruptions caused my meteor impacts. This was more pronounced earlier, when the moon was closer and when it was even more important (more meteors around)

    #6 increased metal content. Since the moon is almost entirely light minerals, most of the metals that were in the original impact were left on earth which artificially increased the concentration of metal in the crust.

    While I can think of other things that could help with one or two of these, I can't think of something that would satisfy all of these consistently for a few billion years.

    What do you suggest as an alternative?