2001 -
Odyssey to Mars
by William H. Clark
The Earth to Mars trajectory is the subject of my dissertation research. NASA
makes it seem quite simple, but it’s not! Consider a few details.
The Mars missions typically follow an elliptical path and meet the red planet
at the opposite side, at apoapse. (See illustration.) This is the minimum energy
trajectory. At apoapse, the velocity of Mars is 24.13 km/sec and the spacecraft
is going 21.5 km/sec. They are both going about the same direction, but Mars
is going 3 km/sec faster. In practical terms, Mars’ diameter is 6800 km, so
the entire planet will pass by the spacecraft in about half an hour. That’s
a pretty small target, in a 250+ day mission!
These relative speeds mean that, because the s/c is moving slower, it must
wait at the railroad crossing for Mars, as it comes barreling down; then deftly
maneuver into orbit at just the precise moment.
| |
 |
|
| |
The Earth-to-Mars Trajectory
|
|
Folks, there’s only one technology in the universe that I would trust to get
me out of that kind of situation - my own legs! It’s asking a lot for an autonomous
s/c to maneuver its way to safety on its own (timely feedback from Earth is
not available because of the time lag.)
The July 4 landing of Sojourner intersected Mars before apoapse. In this circumstance
the spscrcraft was able to make a proactive approach to Mars, versus reactive.
Their relative velocities weren’t much different, but the geometry is a little
more tractable because the spacecraft is approaching at an acute angle, not
head-on.
It is a very subtle thing that you must experience for yourself. You can do
so with a free computer program available at http://get-me.to/mars
[link inactive]. You input some numbers, then the program
finds an optimum trajectory, and displays all the results - where and when all
five of the Trajectory Correction Maneuvers (TCMs) were done, just like on a
real mission! There is also a free four chapter introduction to orbital mechanics
that describes in laymen’s terms all the facets of the trajectory itself.
You’ll find - just like the mission planners - that it is a very slippery situation.
Change one value by 1% and the s/c might not reach Mars at all, but follow it
around the curve of apoapse, and not catch up for months! Change it the other
way and you might get there, but the total energy requirement doubles - so,
practically speaking, you won’t have the fuel to really get there at all. Other
values will, unexpectedly, add 30 days to the mission!
All of which is not the program’s fault - it’s values are accurate to 14 significant
digits (1/10th of a centimeter!). It’s because it is an extremely
non-linear problem. You’ll see!
|