ESA Document - Emits - ESA
ESA Document - Emits - ESA ESA Document - Emits - ESA
s 2.7.13.3 Baseline design HMM Assessment Study Report: CDF-20(A) February 2004 page 84 of 422 From the analyses presented above, it is evident that it is not possible to meet all of the aerobraking constraints with the current vehicle. If the duration is constrained the loads are unacceptably high. Conversely, if the loads are constrained, the duration is so long that the additional ∆V that would be required to reduce it to meet the constraint would make the aerobraking mass savings negligible. Therefore, an aerobraking manoeuvre was not chosen for the baseline design of this mission case. 2.7.13.4 Manoeuvre budget A typical manoeuvre budget for an aerobraking phase that reduces the apocentre altitude from initially 96 000 km to 500 km is 115 m/s, 15 m/s for pericentre control (initial lowering and subsequent adjustment manoeuvres) and 100 m/s for the perigee raise from the final altitude 2.7.13.5 Options In addition to the more conventional aerobraking manoeuvre considered, “deep aerobraking” is a possible option. This would involve deploying an inflatable heat shield (or using an ablative heat shield), storing the solar arrays, and going deep in the atmosphere to shed the orbital energy in a limited number, of passes. This option has not been analysed in this study. 2.7.14 Artificial gravity One of the biggest problems that must be overcome is the harmful effects of weightlessness on the human body. These effects include loss of bone and muscle mass, loss of red blood cells, fluid shifting from the lower to the upper body, cardiovascular and neurosensory deconditioning, and changes in the immune system. The physiological systems start to change immediately upon launch into microgravity and the time courses of change is different for each of them. For example, the fluid shift and cardiovascular system start immediately within hours while the muscle and bone need some time to adjust to microgravity; deconditioning starts after days (muscle) or weeks (bone). Body fluid and cardiovascular system adapt to new environments in less than 2 weeks. However, cardiac arrhythmia might be a problem in-flight for some individuals during elevated workloads. Muscle loss (muscle volume and power) is maximum within the first 4 weeks, but afterwards the loss rate is reduced (strongly dependent on in-flight countermeasures). Bone loss, however, continues progressively (1% per month) throughout the mission in free space. Figure 2-41 summarizes the reactions to microgravity of each of the physiological systems:
s % of loss from baseline 20 18 16 14 12 10 8 6 4 2 0 % of loss from 1g baseline during flight 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 weeks in microgravity HMM Assessment Study Report: CDF-20(A) February 2004 page 85 of 422 Figure 2-41: Effect of microgravity on physiological systems Currently, some countermeasures for weightlessness such as physical exercise, lower body negative pressure and drugs are used in human spaceflight. However, these countermeasures prevail for the permanent ISS crew but have not proven to be sufficient for longer duration missions on-board MIR. Moreover, these countermeasures currently adopted focus only on stimulating a particular physiological system. Artificial gravity, however, represents a different approach to the problem of microgravity effects because it simulates our natural 1g environment. 2.7.14.1 Trade-offs There are two options for how to approach the implementation of artificial gravity as a way to fight against the negative effects of long exposures to weightlessness. One is by providing artificial gravity through continuous rotation of the entire spacecraft with a large radius of rotation and low angular velocities. The second option is intermittent exposure to artificial gravity enough to overcome the damaging effects of microgravity, using on-board centrifuges with a small radius of rotation and high angular velocities to simulate gravity for certain amounts of time. 2.7.14.1.1 Continuous artificial gravity This option requires that the comfort level for the astronauts is respected (see Figure 2-42 from NASA – Habitability data handbook, Volume 1, MSC-03909, 1971). It implies that the minimum rotation radius must be 17 m, achieving 0.3 g at the maximum spin rate of 4 rpm. bone muscle fluid cardio
- Page 33 and 34: s Figure 2-10: Trajectory Overview
- Page 35 and 36: s 2.4.3.5 TEI and planetary protect
- Page 37 and 38: s HMM Assessment Study Report: CDF-
- Page 39 and 40: s HMM Assessment Study Report: CDF-
- Page 41 and 42: s HMM Assessment Study Report: CDF-
- Page 43 and 44: s HMM Assessment Study Report: CDF-
- Page 45 and 46: s Mars Excursion Vehicle Transfer H
- Page 47 and 48: s 2.7.5.1 Mission elements dry mass
- Page 49 and 50: s 2.7.5.8 MEV release The MEV is re
- Page 51 and 52: s Total mission time (days) 1200 10
- Page 53 and 54: s HMM Assessment Study Report: CDF-
- Page 55 and 56: s HMM Assessment Study Report: CDF-
- Page 57 and 58: s stack 9 Propellant mass of the ne
- Page 59 and 60: s HMM Assessment Study Report: CDF-
- Page 61 and 62: s HMM Assessment Study Report: CDF-
- Page 63 and 64: s HMM Assessment Study Report: CDF-
- Page 65 and 66: s The core supporting structure has
- Page 67 and 68: s 2.7.7.1.3 Mars excursion module S
- Page 69 and 70: s 2.7.7.1.4 Earth return capsule HM
- Page 71 and 72: s Mission Phase Description Event s
- Page 73 and 74: s Mission Phase Description Event s
- Page 75 and 76: s 2.7.10 Mission performance Table
- Page 77 and 78: s Days on Martian surface 450 400 3
- Page 79 and 80: s HMM Assessment Study Report: CDF-
- Page 81 and 82: s HMM Assessment Study Report: CDF-
- Page 83: s Maximum manoeuvre duration 6 mont
- Page 87 and 88: s 2.7.15 Sensitivity analysis HMM A
- Page 89 and 90: s 2.7.15.4 Influence of the mass of
- Page 91 and 92: s HMM Assessment Study Report: CDF-
- Page 93 and 94: s Parameters used: • No Shuttle
- Page 95 and 96: s 2.8.3.3 Launch 3- Front node Figu
- Page 97 and 98: s HMM Assessment Study Report: CDF-
- Page 99 and 100: s HMM Assessment Study Report: CDF-
- Page 101 and 102: s HMM Assessment Study Report: CDF-
- Page 103 and 104: s HMM Assessment Study Report: CDF-
- Page 105 and 106: s HMM Assessment Study Report: CDF-
- Page 107 and 108: s HMM Assessment Study Report: CDF-
- Page 109 and 110: s 2.10.1.4 Communications HMM Asses
- Page 111 and 112: s HMM Assessment Study Report: CDF-
- Page 113 and 114: s 2.10.2.2.2 LEO assembly HMM Asses
- Page 115 and 116: s HMM Assessment Study Report: CDF-
- Page 117 and 118: s Basic RF link Four 70-m Ka-band s
- Page 119 and 120: s HMM Assessment Study Report: CDF-
- Page 121 and 122: s HMM Assessment Study Report: CDF-
- Page 123 and 124: s HMM Assessment Study Report: CDF-
- Page 125 and 126: s 3 TRANSFER VEHICLE 3.1 Systems…
- Page 127 and 128: s Operational Requirements It shall
- Page 129 and 130: s Trans Mars Injection Module Mars
- Page 131 and 132: s Figure 3-2: Parallel configuratio
- Page 133 and 134: s Figure 3-6: Global dimensions com
s<br />
% of loss from baseline<br />
20<br />
18<br />
16<br />
14<br />
12<br />
10<br />
8<br />
6<br />
4<br />
2<br />
0<br />
% of loss from 1g baseline during flight<br />
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34<br />
weeks in microgravity<br />
HMM<br />
Assessment Study<br />
Report: CDF-20(A)<br />
February 2004<br />
page 85 of 422<br />
Figure 2-41: Effect of microgravity on physiological systems<br />
Currently, some countermeasures for weightlessness such as physical exercise, lower body<br />
negative pressure and drugs are used in human spaceflight. However, these countermeasures<br />
prevail for the permanent ISS crew but have not proven to be sufficient for longer duration<br />
missions on-board MIR. Moreover, these countermeasures currently adopted focus only on<br />
stimulating a particular physiological system.<br />
Artificial gravity, however, represents a different approach to the problem of microgravity<br />
effects because it simulates our natural 1g environment.<br />
2.7.14.1 Trade-offs<br />
There are two options for how to approach the implementation of artificial gravity as a way to<br />
fight against the negative effects of long exposures to weightlessness. One is by providing<br />
artificial gravity through continuous rotation of the entire spacecraft with a large radius of<br />
rotation and low angular velocities.<br />
The second option is intermittent exposure to artificial gravity enough to overcome the damaging<br />
effects of microgravity, using on-board centrifuges with a small radius of rotation and high<br />
angular velocities to simulate gravity for certain amounts of time.<br />
2.7.14.1.1 Continuous artificial gravity<br />
This option requires that the comfort level for the astronauts is respected (see Figure 2-42 from<br />
NASA – Habitability data handbook, Volume 1, MSC-03909, 1971). It implies that the<br />
minimum rotation radius must be 17 m, achieving 0.3 g at the maximum spin rate of 4 rpm.<br />
bone<br />
muscle<br />
fluid<br />
cardio