Chris Peterson wrote:JohnD wrote:Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)
Chris,
But something the size of Ireson Hill?
I went away to calculate, and meanwhile you and neufer talk up a storm! But I think I still have a point to make.
Ireson is 5 x 15m, or about a 10m wide stone. If it is meteoric iron then it will have a mass of about 4,000 tonnes.
Most meteorites seen on Mars, or found on Earth, are much smaller. Why?
The American Meteor Society estimates that meteors encounter the Earth at 11-72 Kilometers/sec- assume that true for Mars, but that's almost irrelevant, due to atmopsherioc drag.
NASA calculates terminal velocity due to atmospheric drag by Vt = SQR[2W/Cd Rho A]
Where W = Mass = 4x10^6 kg
Cd = Coeff drag For a sphere, about 0.6
Rho = atmospheric density At surface, ~0.020 kg/m3. Obviously the higher the lower, but this figure will maximise drag.
A = Fontal area 10m sphere = 78m^2
So Vt = SQR(2 x 4x10^6/0.6 x 0.02 x 78)
= 3000msec = 3kilometers/sec
This is at the lower limit for a "hypervelocity" impact, that would vapourise the meteor and raise a significant crater.
But Ireson Hill is intact and there is no crater.
Therefore Ireson is not a meteorite.
JOhn
[quote="Chris Peterson"][quote="JohnD"]Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?[/quote]
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)[/quote]
Chris,
But something the size of Ireson Hill?
I went away to calculate, and meanwhile you and neufer talk up a storm! But I think I still have a point to make.
Ireson is 5 x 15m, or about a 10m wide stone. If it is meteoric iron then it will have a mass of about 4,000 tonnes.
Most meteorites seen on Mars, or found on Earth, are much smaller. Why?
The American Meteor Society estimates that meteors encounter the Earth at 11-72 Kilometers/sec- assume that true for Mars, but that's almost irrelevant, due to atmopsherioc drag.
NASA calculates terminal velocity due to atmospheric drag by Vt = SQR[2W/Cd Rho A]
Where W = Mass = 4x10^6 kg
Cd = Coeff drag For a sphere, about 0.6
Rho = atmospheric density At surface, ~0.020 kg/m3. Obviously the higher the lower, but this figure will maximise drag.
A = Fontal area 10m sphere = 78m^2
So Vt = SQR(2 x 4x10^6/0.6 x 0.02 x 78)
= 3000msec = 3kilometers/sec
This is at the lower limit for a "hypervelocity" impact, that would vapourise the meteor and raise a significant crater.
But Ireson Hill is intact and there is no crater.
Therefore Ireson is not a meteorite.
JOhn