A mathematical model is developed for the assessment of the launch mass of
a vehicle designed for a human mission to Mars. The mission involves six st
ages: (i) ascent from Earth surface to low Earth orbit, (ii) outgoing trip
from low Earth orbit to low Mars orbit., (iii) descent and landing on Mars,
(iv) ascent from Mars surface to low Mars orbit, (v) return trip from low
Mars orbit to low Earth orbit, (vi) descent and landing on Earth. The basic
objective is to minimize the launch mass while containing the total flight
time.
The mathematical model includes two parts: interplanetary flight and planet
ary flight. The interplanetary flight model is based on the restricted four
-body scheme and covers the spacecraft transfer from a low Earth orbit to a
low Mars orbit and back. The planetary flight model concerns the spacecraf
t ascent from Earth surface to low Earth orbit and from Mars surface to low
Mars orbit. The sequential gradient-restoration algorithm is employed to s
olve optimal trajectory problems of interplanetary flight in mathematical p
rogramming format and optimal trajectory problems of planetary Right in opt
imal control format.
The planetary flight study shows that, due to the large gravitational const
ant of Earth, it is best to assemble the spacecraft in low Earth orbit and
launch it from there, rather than from the Earth surface. To reduce the rat
io of outgoing LEO mass to return LEO mass, it is best to design the spacec
raft as consisting of three modules: Earth return module, habitation module
, Mars excursion module.
The interplanetary flight study shows that, for minimum energy LEO-LMO-LEO
transfer, the total characteristic velocity is 11.30 km/s. The round-trip t
ime is 970 days, including a stay of 454 days on Mars while waiting for an
optimal return date. For a fast transfer mission with a stay of 30 days on
Mars, the round-trip time can be reduced to less than half at the cost of n
early doubling the characteristic velocity, thereby resulting into a mass r
atio 10 times higher than that of a minimum energy mission, if chemical pro
pellants are used.
To decrease the total mass ratio, use of advanced techniques is indispensab
le. First, aerobraking techniques can contribute considerably to the reduct
ion of mass ratios: excess velocity on arrival to Mars (outgoing trip) and
excess velocity on arrival to Earth (return trip) can be depleted via aerob
raking maneuvers instead of propulsive maneuvers. Second, the development o
f engine/propellant combinations with high specific impulse can be another
key factor for reducing the mass ratio. Third, cargo transportation can be
used: equipment and propellant not required for the outgoing trip can be se
nt before the crew leaves Earth via a cargo spacecraft using a low-thrust e
ngine having high specific impulse. Numerical computation shows that, if bo
th aerobraking techniques and cargo transportation techniques are employed,
the mass ratio for a minimum energy mission can be brought down by a facto
r of 5, while the mass ratio for a fast transfer mission can be brought dow
n by a factor of 20.
To sum up, the mathematical model developed for a launch vehicle can help t
he engineer to assess proper development directions. Numerical results are
highly dependent on certain factors characterizing hardware and propellant
such as engine specific impulse, spacecraft structural factor and aerobraki
ng structural factor. At this time, we must look at a round trip Earth-Mars
-Earth by humans as a formidable undertaking. This paper merely indicates s
ome useful directions. (C) 2001 Elsevier Science Ltd. All rights reserved.