I'm reasonably familiar with Sabatier process, all of Zubrin's calculations and so forth, but I'm far less comfortable with launch and landing physics, and Mr Musk's presentation of a few minutes ago got me to wondering:
==>Are there significant astrodynamic reasons for performing Martian escape launches from equatorial latitudes? And, for that matter, Martian landings? Because......
why one earth (oops. Should be writing "Why on Mars") can it make sense to extract the necessary CO2 from the Martian atmosphere? Atmospheric density there ranges from 0.3 mbar at the peak of Olympus Mons up to 11.55 mbar in the depths of Hellas Planitia. Assuming that's atmosphere is pure CO2 (it's about 96%, so close enough), that still is so minuscule an amount of carbon dioxide compared to what occurs at the polar regions that there is effectively no comparison.
The winter polar ice caps are effectively pure carbon dioxide - dry ice - which is 790 times as dense as gaseous CO2 at one atmosphere. Introducing the reduced atmospheric multiplier, and I'm getting 69,300 times more dense than what's present at Hellas Planitia, and 2.637 million times more dense than atop Olympus Mons.
So....why not "shovel in" the polar dry ice rather than create atmospheric scrubbers? Can any low latitude astrodynamics outweigh this advantage?
==>Are there significant astrodynamic reasons for performing Martian escape launches from equatorial latitudes? And, for that matter, Martian landings? Because......
why one earth (oops. Should be writing "Why on Mars") can it make sense to extract the necessary CO2 from the Martian atmosphere? Atmospheric density there ranges from 0.3 mbar at the peak of Olympus Mons up to 11.55 mbar in the depths of Hellas Planitia. Assuming that's atmosphere is pure CO2 (it's about 96%, so close enough), that still is so minuscule an amount of carbon dioxide compared to what occurs at the polar regions that there is effectively no comparison.
The winter polar ice caps are effectively pure carbon dioxide - dry ice - which is 790 times as dense as gaseous CO2 at one atmosphere. Introducing the reduced atmospheric multiplier, and I'm getting 69,300 times more dense than what's present at Hellas Planitia, and 2.637 million times more dense than atop Olympus Mons.
So....why not "shovel in" the polar dry ice rather than create atmospheric scrubbers? Can any low latitude astrodynamics outweigh this advantage?