Hello all...
I've finally completed the first in my series of orbital analyses
for certain battles in SW canon to establish lower bounds on SW
spacecraft propulsion capabilities... first however, thanks to Mike
Wong, for providing me with the impetus to disprove certain claims
regarding the propulsive abilities of SW ships in general, and Curt
Saxon, whose technical commentaries pages were of great benefit,
providing me with the basic astrophysical data on the bodies in
question. I must say it continues to be an interesting challenge, and
hope others will duplicate the excercise for the sake of external
verification.
To provide some background... I am certain that most of you are
aware of the debate that has been raging concerning the comparison of ST
and SW sublight propulsion... lately, the warsies seem to have been
hammering the idea that even the Death Star can accelerate at sizeable
fractions (by Mike Wong's estimate, as much as 10%) of the known rate
for the Galaxy class of starship in ST (which is firmly established as
1000g), and that Star Destroyers can exceed those capabilities by as
much as 3x. As evidence, the warsies have cited the ANH battle of
Yavin, where the original Death Star (hereafter referred to as DS1) was
seen to come into LOS of Yavin 4 (Y4 from now on) after an apparent 30
minute circumnavigation of the Yavin gas giant (YGG or simply GG) --
other scenarios, to include the battle at Endor from ROTJ, and selected
other scenarios from 'official' literature (novels etc.) will be
discussed in other posts -- as an indication that the DS1 must be
capable of substantial acceleration... This particular thread will
definitively illustrate the fallacy of these assumptions wrt the DS1,
and will also serve to establish realistic upper and lower bounds on
the acceleration capabilities of typical fighter craft in the SW
universe, using data gathered from curt's pages, observation of the
available footage, and basic principles of orbital mechanics.
First, let us establish the baseline conditions for this scenario
from the film evidence. We have various external views of DS1 throught
the scenario, verbal cues, and tactical representations shown on
viewscreens in both the DS1's command center and the rebel command
bunker on Y4. The externals are straightforward, allowing us to
determine several facts... first, from the externals:
1. The DS1 was reasonably near to the Yavin GG... perhaps within
three times the GG's radius (which would place the range from DS1 to the
GG at about 1 light second) or closer, as the GG looms quite large in
the background -- it is quite possible that the DS was using its'
repulsorlifts to maintain either an unnaturally slow orbit or a
stationary 'trojan' position at that radius. Also, this position lies
at an acute angle to the GG's terminator (on the sunny side), not
parallel to it, as the terminator is clearly visible with some apparent
curvature.
2. The distance between the DS1 and Yavin does not change
appreciably during the scenario... it will be shown that for reasons of
orbital mechanics, it does not need to.
On to the tactical displays... it should be noted that there are
some important differences in how the two displays present
information... the tactical displays on the DS1 are to scale, showing
the GG, its' major moons and their orbits -- and later Y4's motion as it
moves from behind the GG, all from the DS1's first person point of view
-- this was all necessary information for the DS, and it is
understandable that it was shown... otoh, the display in the rebel
bunker is a 'not to scale' representation of the scenario, from a
third-person, 'god's eye' perspective, for the express (need I say
'obvious'?) purposes of facilitating the presentation of the effective
targeting cone of the DS superlaser, and coordinating the fighter
attack... it is reasonable to assume that, given the circumstances,
no-one on Y4 had any interest whatever in the orbital dynamics of the
situation -- it was more along the lines of 'how much time have we got
to kill that thing before it gets LOS on us????!!!!' now, the facts as
observed from the displays:
1. the DS display clearly establishes that the semi-major axis of
Y4's orbit is at an angle to both the DS1's position vector, shown as it
is in the first person perspective, and the Yavin day/night terminator.
This display also shows that Y4's apogee is to the far left of the
screen, while perigee is on the right, with the GG just to the left of
it.
2. the second display shown on the DS screen shows the GG,
greatly enlarged so that only a small portion of its' curvature is in
view, with Y4 behind it (by approximately 6.5 Y4 radii as measured from
Y4 center to the outermost portion of Yavin's curvature). Yavin is
shown to be moving out from behind the GG at a fairly rapid rate from
left to right -- if this depiction is oriented in the same plane as the
previous display on the screen -- there is no indication otherwise --
then Y4 may be assumed to be nearing, or perhaps has just passed
perigee.
3. when the 30 minute countdown is up, and Y4 is declared to be
in range, its' center as seen from the DS is only 1 radius out from the
GG's curvature. This information, combined with the previous 6.5 radii
observation (a grand total of 7.5 Y4 radii in apparent motion), will
later help to establish the angular motion of Y4 in its' orbit during
the countdown.
4. unfortunately, the rebel's tactical display is of
comparatively little use... the only contribution it makes to these
observations is the apparent acceleration of the DS during the 30 minute
period... I say 'apparent' because it is a misrepresentation -- the DS
is not accelerating wrt the GG... Y4 is...
and now, the verbal cues:
1. at the beginning, when we first see the DS display of the
Yavin group, a sensor operator is heard to say 'orbiting the planet at
maximum velocity... estimated time to firing range 30 minutes'... this
same operator proceeds to give updates almost every time we see the
display from now on. Strangely enough, this appears to be some kind of
mistake, as there is only one possible maximum velocity for a given
orbit with a nonzero eccentricity... velocity at perigee (for orbits
with an eccentricity of zero, there is only orbital velocity... any
slower is suborbital for that radius, while any higher velocity will
result in either a higher orbit or escape from the gravity well). Given
the conflict this velocity statement has with classic orbital mechanics,
there are three possibilites:
a) DS1 is using its' repulsorlifts to alter the apparent
magnitude of the gravity well to allow for a faster orbit
b) the DS1 is itself in an elliptical orbit and is passing
through perigee.
c) the statement does NOT refer to the DS1... rather to the
current velocity of Y4 -- if Y4 was nearing or passing through
perigee in its' orbit of yavin, it would be moving at its'
highest possible velocity.
Of these three possible explanations, the third -- that the
statement refers not to DS1 but to Y4 -- seems most plausible. 'a' is
unlikely, as the DS appears from the observed footage to be moving more
slowly than would be normal for the apparent orbit, contrary to the
proposed theory (a task for which repulsorlifts are commonly used), 'b'
when the statement was made, the DS was obviously farther away from
Yavin than later in the countdown, indicating that maximum relative
velocity was reached later in the scenario.
2. from about the time we first see the rebel display, just after
the fighters launch from the surface, another (rebel this time) sensor
operator is known to call out updates... they dont have any real
bearing on the analysis, serving only as an alternate version of the
countdown clock -- the only time indices of importance are the beginning
of the 30 minute countdown, the 15 minute mark which coincides with the
start of the fighter attack, and the declaration of LOS.
>From the observations above, it is now possible to arrive at a working
theory for the scenario:
DS1 had assumed a station keeping position on the far side
of Yavin from Y4, at a range of about 1 light second from the
GG's center, using its' repulsorlifts to maintain itself in a
stationary trojan-style orbit... thus situated, it had only to
wait for the moon's orbit to bring it into view, which would
happen shortly, as the moon had just reached its' orbital
perigee, and was thus moving out from behind Yavin at the
highest possible real and angular velocites for its' orbit.
We know that the DS holding position was not directly opposite
from Y4's perigee (with the initial vector passing through the
center of Yavin) because, at the time the operator's voice
clearly states '... orbiting the planet at maximum velocity'
the DS tactical display clearly illustrates that Y4's center
is only 6.5 Y4 radii from the outer edge of the GG as seen
from the DS's perspective (not the requisite 10.5 Y4 radii
which would indicate a position directly opposite)-- at the
end of the countdown, Y4's center is 1 radius outside the GG,
making for a total apparent motion of 7.5 radii. This is a
simple of theory to calculate, as it has relatively few
components in motion.
In order to establish the positional relationships for this
scenario, it is helpful to plot the GG, Y4 and its' orbital path around
the GG -- to the proper scale of course -- on a sheet of 17"*22" 10
sq/in graph paper (it helps to visualize the system). The necessary
numbers follow:
known constants from curt's pages, with additions based on my own
calculations (formulae are shown where applicable):
map scale: 2.0E8 m per inch (2.0E5 km/in)
YGG:
mass: 5.299E27 kg
radius: 9.6239E7 m (96239 km)
Y4:
mass: ? (not significant for purposes of this
analysis)
radius: 6.55E6 m (6550 km)
semi-major axis (a): 1.2E9 m (minimum)
semi-minor axis (b): 6.511E8 m (minimum) -- calculated
from the formula e=(1-(b^2/a^2))^.5
eccentricity (e): 0.84 (minimum)
orbital period (P): 122 hours (minimum)
radius of perigee (rp): 1.92E8 m (based on above
data, rp=a(1-e))
radius of apogee (ra): 2.208E9 m (based on above
data, ra=a(1+e))
Using the above data points, in conjunction with the formula for the
polar equation of a conic section, which gives the magnitude of the
position vector for a satellite in orbit,
r=(a(1-e^2))/(1+ecosv)
r and a both must be in same units of distance
v is the polar angle (aka true anomaly) in either degrees or
radians, measured from perigee=0, apogee=180 degrees or 3.142
radians
I proceeded to map out the last 90 degrees of the orbital path of Y4 in
15 degree increments and 'connected the dots', making sure to use an
appropriate curvature. For an approximate representation of my working
diagram, please see the attached .bmp file...
Nomenclature and applicable formulas:
A. Constants and variables:
G Universal gravitational constant 6.67E-17
N*km^2/kg^2
e! specific mechanical energy -- values less than
zero define closed orbits, while equal to or greater
than zero define open, ie escape trajectories
V velocity
m' gravitational constant for a given mass
m1 primary mass
m2 secondary mass
r radius
a semi-major axis of a given objects' orbit
e eccentricity
v true anomaly, the angular component of the
satellites current orbital position, where 0 degrees
or radians = perigee(depending on the equation, will
be in either degrees or radians)
rp radius of perigee
ra radius of apogee
P orbital period
n mean motion (in radians/second)
E eccentric anomaly (radians)
M mean anomaly (radians)
t-t0 time of flight from one angular position in
orbit to another in seconds
B. equations
1. attractive force F between two bodies of known
mass and separation distance d:
F (in newtons) =(-Gm1m2)/d^2
2. polar equation of a conic section (gives the
magnitude of the position vector in terms of the
vector's location in the orbit):
r (in km) =a(1-e^2)/(1+ecosv)
3. e! (energy) for a given orbit. can also
determine Vescape for any given distance r by
setting e! to zero and solving for V, or the
circular velocity for a e=0 orbit by setting a equal
to r, and solving for V
e!=(V^2/2)-(m'/r)=(-m')/2a
4. a (semi-major axis in km)
a=-m'/(2e!)=(ra+rp)/2
5. e (eccentricity)
e=1-(rp/a)=(ra/a)-1
6. rp (radius of perigee in km) =a(1-e)
7. ra (radius of apogee in km) =a(1+e)
8. P (orbital period) =2pi(a^3/m')^-2 P in
minutes
9. n (mean orbital motion in rad/sec)
=(m'/a^3)^-2
10. E (eccentric anomaly in radians): cos
E=(e+cosv)/(1+ecosv)
11. M (mean anomaly in radians)
=E-esinE=M0+n(t-t0)
12. t-t0 (elapsed time) =(M-M0)/n
As ti happens, there is at least one solution for this theory which
works out perfectly... if the major axis of Y4's orbit lies 30 degrees
off the line of the terminator on Yavin, such that Y4's perigee is on
the sunny side of the GG, and DS1's position lies at 200000km from
Yavin, at an angle of +19 degrees on the sunny side of the GG
terminator, Y4 comes into LOS with DS1 just as it reaches perigee...
thus, the line from Yavin's center to Y4 at the beginning of the
scenario defines a true orbital motion of 30 degrees for Y4... From the
above calculations, we know that Y4 takes 30 minutes and 2 seconds to
travel through the last 30 degrees of its orbit to perigee, which fits
quite nicely within the parameters set in the film. It should also be
noted that this solution is fairly independent of the range of the DS to
Yavin, as changing that variable has no effect on the true anomaly.
on to the fighter performance analysis (based on the above scenario of
course)...
Since we are extremely time limited for the fighter transit from Y4
to the DS -- the absolute minimum range between the two at the initial
time for the scenario is at least 400kkm -- any normal intercept orbit
approach is out, as the fastest conventional transfer orbit would take
just under 2 hours to complete. This necessitates the argument that the
fighters were under heavy acceleration for the entire transit, using
their repulsorlifts to ignore the gravity well of Yavin. If the
fighters launched at the 30 minute mark, they would have only 15 minutes
to complete the transit, as combat is known to begin at roughly the 15
minute mark. To accomplish the transit in the necessary timeframe, the
fighters would have had to accelerate at a minimum rate of 211g to the
halfway point (covering ~200kkm in 7.5 minutes or less, at an average
velocity of 466.67km/sec, although this could be slightly less as they
benefit from Y4's initial orbital velocity at the time, on the order of
42 km/sec), with a subsequent deceleration at the same rate to arrive at
rest relative to the DS. Later launch times serve to compress the time
window (although the range does not substantially change until after the
15 minute mark due to the orbital motion of Y4), necessitating higher
acceleration. While it can be argued that the fighters were wasting no
time in getting to the DS, thus accelerating at their maximum rate, the
scenes in the rebel hangar following the 30 minute mark serve to cast
some uncertainty on the exact timing of the fighter launch, leaving the
211g rate as a reasonable lower bound on the fighter's maximum g
rating. Note that under the orbital scenario described, even if the
fighters did not launch until the 20 minute mark, they would not have
had to accelerate at a rate beyond 2000g to cover the distance in time,
so this figure can serve as an upper bound. Such performance, wether it
be the lower or higher figure, can be considered to be a typical
expectation of fighter performance in the SW universe, with larger ship
types being comparatively sluggish (increasingly so as size increases),
although larger types would probably be able to maintain their maximum
rates for much longer periods and to higher relativistic velocities, due
to increases in engine specific impulse with size, as well as much
larger reaction mass reserves.
Please forgive any typos or apparent grogginess... I had to piece this
together over the course of the last 2 months, squeezing it into the
temporal cauldron that passes for my life at the moment (doing the math
was easy -- writing this analysis of my results was a royal pain in the
@$$)... but please feel free to comment on any items that seem seriously
mistaken. The analysis of the Battle for Endor is coming, but it might
be another 2 months... I will make every effort to reply to responses
to this post in the meantime.
aaaahhhh... done... except for my references...
1. _Space_Propulsion_Analysis_and_Design_, by Humble, Henry and
Larson, ISBN 0-07-031320-2, McGraw Hill space technology series.
2. _Introduction_to_Space_Dynamics_, by Thomson, ISBN 0-486-65113-4,
Dover.
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