Also see:http://forum.nasaspaceflight.com/index.php?topic=31201.0
With such a thin atmosphere and such a large potential crater I wonder if enough debris will be short term thrown into LMO (Low Mars Orbit) to pretty much end the assets in mars orbit. btw. Where is this 500km crater number coming for? Do we have a nucleolus estimate that corresponds to a predicted 500 km crater?
Article says they've measured from the absolute magnitude of the nucleus that the comet is 50km in diameter moving at 56 km/s relative to Mars. That's certainly large enough to leave quite a dent on Mars.
Now, the challenge: get MRO and/or Mars Express in position to watch the flyby/impact!
Quote from: simonbp on 02/26/2013 02:43 pmNow, the challenge: get MRO and/or Mars Express in position to watch the flyby/impact!50km ball, assuming 0.6kg/L density (wiki's opinion for average comet density) at 56km/s gives yield of ... ~15 million gigatons of TNT. Unlikely that any asset in orbit or ground would survive. Might even send very nasty debris cloud crossing Earth orbit too.
It'd still be great for space exploration. Nothing like a dramatic dinosaur-killing impact on Mars to increase funding for doing /something/ about those asteroids...
Aned the effect on Mars' climate would be very significant, because the impact still couldn't dramatically reduce the mass of Mars' atmosphere (it can't blow off anything beyond the horizon) but it would add a heck of a lot of energy and volatiles (more than all of Mars' atmosphere!) to the planet, a combination of out-gassing and such that could dramatically increase the mass of the Martian atmosphere. Perhaps in some places, within half of the Armstrong limit!
Quote from: R7 on 02/26/2013 03:15 pmQuote from: simonbp on 02/26/2013 02:43 pmNow, the challenge: get MRO and/or Mars Express in position to watch the flyby/impact!50km ball, assuming 0.6kg/L density (wiki's opinion for average comet density) at 56km/s gives yield of ... ~15 million gigatons of TNT. Unlikely that any asset in orbit or ground would survive. Might even send very nasty debris cloud crossing Earth orbit too.It'd still be great for space exploration. Nothing like a dramatic dinosaur-killing impact on Mars to increase funding for doing /something/ about those asteroids...Aned the effect on Mars' climate would be very significant, because the impact still couldn't dramatically reduce the mass of Mars' atmosphere (it can't blow off anything beyond the horizon) but it would add a heck of a lot of energy and volatiles (more than all of Mars' atmosphere!) to the planet, a combination of out-gassing and such that could dramatically increase the mass of the Martian atmosphere. Perhaps in some places, within half of the Armstrong limit!
Quote from: Orbiter on 02/26/2013 02:30 pmArticle says they've measured from the absolute magnitude of the nucleus that the comet is 50km in diameter moving at 56 km/s relative to Mars. That's certainly large enough to leave quite a dent on Mars.Yes, that's probably large enough to survive the atmosphere and make it down to the surface.
Unlikely that any asset in orbit or ground would survive.
Might even send very nasty debris cloud crossing Earth orbit too.
Quote from: Robotbeat on 02/26/2013 03:24 pmIt'd still be great for space exploration. Nothing like a dramatic dinosaur-killing impact on Mars to increase funding for doing /something/ about those asteroids...The OP article quotes the upper bound for the energy of a collision as around 200x what Wiki quotes as the energy of the Chixculub impact. [Edit: 2e16 vs 1e14 tons TNT.]That would put it in a different league...
That would be interesting prospect though .. but how long would outer space near Mars be a debris minefield?
Considering the point of impact is inside the atmosphere, that means the Perigees will be pretty low (as inside the thin atmosphere above the impact point), the bulk of the debris will not last very long. An orbit or two.
Quote from: kevin-rf on 02/26/2013 04:15 pmConsidering the point of impact is inside the atmosphere, that means the Perigees will be pretty low (as inside the thin atmosphere above the impact point), the bulk of the debris will not last very long. An orbit or two. This is actually what I keep failing to understand in Moon's giant impact hypothesis. What circularized enough ejecta beyond Roche-limit for Moon to form? What ever an impact throws into what ever (elliptical, hyperbolics would espace, no?) orbit don't those orbits have perigee at (or under) surface? Apparently not, some other effect is in play, would it affect Mars case too, maybe create a ring or something?