J
JonClarke
Guest
Thanks for the feedback, much appreciated. <br /><br /><i>At first glance your plan looks very similar to the NASA DRM 1.0 except it's even more conservative, no nuclear power or nuclear propulsion. </i> <br /><br />The similarities are due to the common semi-direct architecture.<br /><br />We opted against nuclear power for three reasons. 1) the study was to be used for public outreach and we did not want to fight too many issues at once. 2) We wanted to examine the common assumption that nuclear power was necessary. 3) We wanted to minimise the amount of technology development required.<br /><br /><i>While your MTV reminds me of the MTV from the ESAS plan for Mars. Combining the MTV with Earth Return propulsion preserves certain abort options the DRM 1.0 lacks. </i><br /><br />Once again the similarities are due to the semi-direct architecture of the two studies.<br /><br /><i>I have two principle questions regarding your plan. The first is about crew size. Your payload masses appear very similar to those from the NASA DRM 1.0, but your mission is for only 4 crew while the NASA mission supports 6. The even smaller payloads of the NASA DRM 3.0 still supports a crew of 6. Are you being overly conservative with your estimates? Couldn't you easily accomodate a crew of 6? (Or alternatively cut your mass estimates by 1/3?) </i><br /><br />The size (and shape) or our lander modules were fixed, we sized the crew to what modules of this dimension could support. The landers mass ~60 tonnes in LEO and scale quite well to the ~80 tonne DRM 3.0 landers. <br /><br />The real difference is in the MTV. The DRM’s ERV massed 80 or so tonnes, ours 130. Even the difference in flight profile (we ferry the crew both ways) and design (we include an earth entry capsule) cannot account for this. We agonised over this but could find no way of reducing the mass any further using realistic numbers and margins from Larson and Pranke. Even then we cut a few corners in things like medical equipment an <div class="Discussion_UserSignature"> <p><em>Whether we become a multi-planet species with unlimited horizons, or are forever confined to Earth will be decided in the twenty-first century amid the vast plains, rugged canyons and lofty mountains of Mars</em> Arthur Clarke</p> </div>