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&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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�</text>
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                    <text>V H E A S T R O D Y N A M I C I S T ' S R O L E V I S - A - V I S T H E SYSTEMS E N G I N E E R
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REYNOLDS DUNCAN, JR.
NASA Marshall Space Flight Center
Huntsville, Alabama

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AS$RODY&amp;MXCIST'S ROLE VIS-A-VIS THE SYSTgMS ENGINEER

J. Reynolds Duncan, Jr.
Aerospace Engineer
NASA-Marshall Space P l i g h t Center
W u n t s v i l l e , Alabmna

The prablem o f e f f e c t i v e two-way c o m u n i c a t i o n s
is t r e a t e d , w i t h emphasis p l a c e d upon t h e compilat i o n a d p r e s e n t a t i o n of astrodynamical d a m f o r
w e by t h e systems e n g i n e e r i n t h e p r e l i m i n a r y
p h a s e s o f m i s s i o n p l a n n i n g . Such d a t a s h o u l d b e
p r e s e n t e d i n a form which is e a s i l y understood and
v h i c h c a n n o t b e e a s i l y m i s i n t e r p r e t e d by p e r s o n s
w i t h l i t t l e o r no k n o w l e d g e o f a s t r ~ d y ~ r a i c s .
Wherever a s t r o d y n a m i c a l p a r a m e t e r s may b p o s e
c o n s t r a i n t s upon a m i s s i o n , a c l e a r i n d i c a t i o n
s h o u l d be g i v e n o f t h e p o s s i b l e consequences f o r
v i o l a t i o n o f t h e s e c o n s t r a i n t s . When a l t e r n a t i v e s
a r e a v a i l a b l e , they should be indicated, along
w i t h any p e n a l t i e s a s s o c i a t e d w i t h t h e i r u s e . The
r e s u l t of t h e astrodynamicist's e f f o r t should be a
well-informed systems e n g i n e e r who h a s t h e o v e r a l l
p i c t u r e of t h e e f f e c t s o f astrodynamical parameters
upon a m i s s i o n and t h u s w i l l be a b l e t o perform
meaningful t r a d e o f f s t u d i e s w i t h r e g a r d s t o system
d e s i g n a &amp; performance.

I. l n t r o d u c t i o n
The r o l e a n a s t r o d y n a m i c i s t may p l a y i n a
m i s s i o n des.ign s t u d y c a n b e d i v i d e d i n t o two p a r t s :
t h a t o f s u p p l y i n g background o r p r e p l a n n i n g i n f o r mation and t h a t o f p r o v i d i n g additions:, u s u a l l y
more d e t a i l e d , i n f o r m a t i o n f o r u s e d u r i n g t h e s y s tem and subsystem d e s i g n phase. The t y p e and
amount of d a t a s u p p l i e d t o the systems a n a l y s t
d u r i n g t h e l a t t e r p h a s e depends t o a l a r g e e x t e n t
upon t h e completeness and u s e f u l n e s s o f t h e background i n f o r m a t i o n s u p p l i e d t o him e a r l i e r . The
t y p e and method o f p r e s e n t a t i o n of t h i s background
i n f o r m a t i o n i s t h e major t o p i c o f d i s c u s s i o n i n
t h i s paper.
Background i n f o r m a t i o n , a s used h e r e , r e f e r s t o
a s t r o d y n a m i c a l d a t a o f a g e n e r a l n a t u r e which may
c o n t r o l o r i n f l u e n c e t h e d e s i g n o f systems a n d / o r
subsystears. The g e n e r a l f t y o f t h e d a t a i m p l i e s
t h a t t h e d a t a may b e used f o r m i s s i o n p l a n n i n g
p u r p o s e s on a v a r i e t y o f m i s s i o n s . Of c o u r s e , a l l
p o s s i b l e missions? c a n n o t b e covered, b u t by res t r i c t i n g t h e launch, p l a n e t t o b e t h e e a r t h and
s p e c i f y i n g a s i n g l e t a r g e t p l a n e t , a manageable
gr0.q o f c h a r t s and g r a p h s c o u l d b e g e n e r a t e d
c o v e r i n g s u c h p o s s i b i l i t i e s a s d i r e c t and brokenp l a n e t r a n s f e r s f o r a l l r e a l i s t i c launch e n e r g i e s ,
and a r r i v a l c o n f i g u r a t i o n s v a r y i n g from f l y b y t o
low o r b i t a l r e c o n n a i s s a n c e m i s s i o n s . The d a t a
p r e s e n t e d s h o u l d i n d i c a t e t h e e f f e c t o r impact o f
i m p o r t a n t p a r a m e t e r s upon t h e o v e r a l l c l a s s o f
possible missions.
The p r e s e n t a t i o n o f t h e d a t a s h o u l d b&amp; a c m p l i s h e d i n s u c h a way a s t o i n d i c a t e p o s s i b l e
r a n g e s o f v a l u e s o f t h e parablerere. T h i s i s p r e f e r a b l e t o p r e s e n t i n g sample t r a j e c t o r i e s whieh
g i v e only s p e c i f i c values of t h e parameters f o r
Whenever
t h e v a r i ous s e l e c t e d t r a jsc t o r i e s
p o s s i b l e , p a r a m e t e r s which a r e f a m i l i a r t o t h e
u s e r s h o u l d be used and when t h e r e i s any p o s s i b i l i t y o f m i s i n t e r p r e t a t i o n o f t h e meaning o f t h e

.

p a r a m e t e r s , a f u l l e x p l a n a t i o n of t h e i r meaning
should accompany t h e c h a r t s o r g r a p h s . Also, t h e
v a l a e s o f any c o n s t a n t s used i n the g e n e r a t i o n o f
t h e d a t a should b e g i v e n , a l o n g w i t h a n y assumptions
which were made which might a f f e c t t h e a c c u r a c y o f
t h e d a t a . These may seem t o b e s m a l l p o i n t s , b u t
t h e omission o f such items a s t h e s e may c a u s e
problems i n t h e p r o p e r u s e and i n t e r p r e t a t i o n o f t h e
d a t a . One o f t h e primary c a u s e s of t h e s e omissions
i s the f a m i l i a r i t y of the astrodynamicist with the
m a t e r i a l h e i s p r e s e n t i n g . Although t h i n g s may b e
taken f o r g r a n t e d i n a d i a l o g u e between s p e c i a l i s t s
i n t h e same d i s c i p l i n e , making t h e same assumptions
when p r e s e n t i n g d a t a t o p e r s o n s i n a n o t h e r f i e l d
u s u a l l y r e s u l t s i n a c o m u n i c a t i o n problem. Thus,
t h e o b j e c t i v e of t h e a s t r o d y n a m i c i s t s h o u l d b e t o
p r e s e n t t o t h e systems e n g i n e e r d a t a which is e a s y
t o understand, e a s y t o u s e , and which c a n b e
r e g e n e r a t e d w i t h o u t a d d i t i o n a l informa t i o n .
To i l l u s t r a t e t h e s e p o i n t s , some g r a p h s w i l l b e
p r e s e n t e d which would be used i n a m i s s i o n a n a l y s i s
s t u d y o f a n unmanned m i s s i o n t o Mars d u r i n g t h e
1973-74 launch o p p o r t u n i t y . D i s c u s s i o n o f t h e g r a p h s
w i l l c e n t e r around t h e t y p e o f i n f o r m a t i o n which
should accompany each graph i n o r d e r t o make t h e
comunication of t h e information a s e f f e c t i v e a s
p o s s i b l e . Space does n o t p e r m i t t h e d i s p l a y o f a
more complete s e t ' o f c h a r t s and graphs which might
b e used i n such a s t u d y .
If.

Supplemental I n f o r m a t i o n

A graph such a s t h e one shown i n F i g u r e 1 would
b e one of t h e f i r s t graphs c o n s u l t e d i n a m i s s i o n
a n a l v s i s s t u d y . F i g u r e 1 shows t h e o v e r a l l launch
o p p o r t t i n i t y a s d e f i n e d by t h e launch energy, G.
From t h i s c h a r t , t h e maximum ranges o f t h e launch
d a t e , a r r i v a l d a t e , and time o f f l i g h t c a n b e
o b t a i n e d . accompany in^ t h i s graph s h o u l d be i n f o r mation g i v i n g t h e d e f i n i t i o n s o f Type I, 'llype I f ,
C l a s s 1, and C l a s s 2 t r a j e c t o r i e s a l o n g w i t h a n
explana t t o n o f C, a d a n i n d i c a t i o n o f t h e isccur8cy
o f t h e d a t a . Also, mention s h o u l d b e made o f any
pariameters which may e f f e c t t h e Cg determined launch
o p p o r t u n i t y a l o n g w i t h any p o s s i b l e a l t e r n a t i v e a
such a s broken-plane t r a n e f s r s . The accompanying
i n f o r m a t i o n f o r t h i s f i g u r e might b e p r e s e n t e d a s
follows.

-

Definition of T e r n
Type X t r a j e c t o r i e s a r e t h o s e on which t h e spacec r a f t would t r a v e l l e s s t h a n 180"around t h e s u n
from t h e time t h e s p a c e c r a f t l e a v e s t h e e a r t h u n t i l
i t a r r i v e s a t Mars. Type 11 t r a j e c t o r i e s a r e t h o s e
on which t h e s p a c e c r a f t would t r a v e l b e t w e n 180'
and 360' around t h e s u n . C l a s s 1 and C l a s s 2 t r a j e e t o r i e s a r e s u b c l a s s e s o f Type X: and 'Sypra I1 and
d i f f e r p r i m a r i l y I n t h e f l i g h t times r e q u i r e d ,
C l a s s 2 t r a j e c t o r i e s having l o n g e r f l i g h t times
t h a n C l a s s 1 t r a j e c t o r i e s f o r t h e same launch d a t e
and C3. The parameter, C, , comes from t h e e q u a t i o n
which g i v e s t h e v e l o c i t y of, a n o b j e c t when t r a v e l i n g

�Figure 1

-

1973-74 Launch Opportunity for Mars

�250 days

LAUNCH
Figure 2

-

DATE

1973 Type I Launch Opportunity for Mars

�o n a c o n i c s e c t i o n . The c o n i c e q u a t i o n f o r t h e
v e l o c i t y o f a n o b j e c t is
(I)
where
is the e a r t h ' s gravitational constant, R
i s t h e d i s t a n c e from t h e c e n t e r of t h e e a r t h , and
a i s a measure o f t h e s i t e o f t h e c o n i c s e c t i o n .
Bxpressed i n tenna o f %, Equathon (1) becomes

C, is t h e i n j e c t i o n e n e r g y p r o v i d e d t o the spacec r a f t by t h e l a u n c h v e h i c l e and i s e q u a l t o t w i c e
t h e t o t a l e n e r g y p e r u n i t miss. A s R becomes v e r y
l a r g e , C3 a p p r o a c h e s V?. When t h e s p a c e c r a f t
leaves the g r a v i t a t i o n a l influence of the e a r t h , V
becomes V-, which i s t h e " v e l o c i t y a t i n f i n i t y " o r
t h e "hyperbolic-excess v e l o c i t y . "

-

I n f o r m a t i o n N e c e s s a r y t o U t i l i z e Graph
The C3 l i m i t a t i o n o f t h e l a u n c h v e h i c l e , a s
p r o v i d e d by performance s t u d i e s , i s a l l t h a t i s
needed.
I n f o r m a t i o n O b t a i n a b l e from Graph
Ranges o f l a u n c h d a t e s , a r r i v a l d a t e s , and
f l i g h t t i m e s a s a f u n c t i o n o f t h e C, l i m i t a t i o n s o f
t h e launch v e h i c l e . See F i g u r e 2 f o r a n e n l a r g e d
view o f lower v a l u e s o f
f o r Type I t r a j e c t o r i e s .
See F i g u r e 4 f o r h and a r r i v a l Vm c u r v e s f o r t h e
lower e n e r g y Type I t r a n s f e r s , These p a r a m e t e r s
may l i m i t t h e s i z e o f t h e C, detgrmined launch
opportunity.
A d d i t i o n a l C o n s t r a i n t s t o Consider
'. ( s e e F i g u r e 4 2 ; a r r i v a l V- ( s e e F i g u r e 4 ) ;
ccmmunica t i o n d i s t a n c e r e s t r i c t i o n s ; t r a c k i n g
c o n s t r a i n t s ( b o t h e a r t h o r b i t a l and deep s p a c e ) ;
o p e r a t i o n a l l i m i t a t i o n s on minimum l e n g t h o f launch
period.

Assumptions Made/Accuracy o f , Data/Cons t a n t s Used
Two-body c o n i c s were used i n t h e computation o f
t h e d a t a because t h e c o m p u t a t i o n time r e q u i r e d f o r
c o n i c t r a j e c t o r i e s is much l e s s t h a n t h a t r e q u i r e d
f o r n u m e r i c a l l y i n t e g r a t e d t r a j e c t o r i e s . Accuracy
of the d a t a i s considered adequate f o r mission
a n a l y s i s s t u d i e s . u (sun) = .13271544E12, t h e
a n a l y t i c ephemeris used t o o b t a i n t h e p l a n e t a r y
p o s i t i o n s is d e s c r i b e d i n E n g i n e e r i n g P l a n n i n g
Document No. 406, J e t P r o p u l s i o n L a b o r a t o r y , J u l y ,
1966.
Possible Alternatives
It may b e p o s s i b l e t o e x t e n d t h e launch opportuni'ty w i t h t h e u s e o f b r o k e n - p l a n e t r a n s f e r s .
T h e s ~a r e t r a j e c t o r i e s on which t h e s p a c e c r a f t
t r a v e l s p a r t o f t h e way t o Mars i n one f l i g h t p l a n e
a n d , a f t e r a v e l o c i t y c o r r e c t i o n i s made, t r a v e r s e s
t h e remaining d i s t a n c e i n a d i f f e r e n t f l i g h t p l a n e .
The t o t a l e n e r g y expended (C, + p l a n e change bV +
a r r i v a l Vm) i s l e s s f o r t h i s t y p e of t r a n s f e r t h a n
f o r e i t h e r a Type I o r Type I1 t r a j e c t o r y when t h e
h e l i o c e n t r i c t r a n s f e r angle for a single-plane
On
t r a n s f e r (Type I o r Type T I ) is n e a r 18$.
F i g u r e 1, t h e b r o k e n - p l a n e t r a n s f e r s o f i n t e r e s t
would b r i d g e t h e narrow gap between t h e Type Z and
Type f I c o n t o u r s . U n a t t r a c t i v e f e a t u r e s o f t h e
broken-plane t r a j e c t o r i e s a r e the a d d i t i o n a l

o p e r a t i o n a l complexity of t h e m i s s i o n and t h e
p o s s i b i l i t y o f l i t t l e o r no r e t u r n o f s c i e n t i f i c
i n f o r m a t i o n from t h e v i c i n i t y o f t h e t a r g e t p l a n e t
i f t h e plane-change maneuver f a i l s .
The s i x subheadings used above r e p r e s e n t a usea b l e and e f f e c t i v e method o f p r e s e n t i n g t h e supplemental i n f o r m a t i o n which should riccompany F i g u r e 1.
The ma t e r i a 1 p r e s e n t e d under t h e s e subheadings i s ,
t o a s t r o d y n a m i c i s t s , of a v e r y f a m i l i a r n a t u r e , and
might b e c o n s i d e r e d i n f o r m a t i o n which i s n o t worth
i n c l u d i n g s i n c e "everyone knows it." But, a g a i n , it
is t h i s f a m i l i a r i t y o f t h e a s t r o d y n a m i c i s t w i t h h i s
m a t e r i a l t h a t i s o f t e n t h e c a u s e o f comnunication
p r o b l b s . I f t h e above subheadings were used a s a
g u i d e o r c h e c k l i s t i n d e t e r m i n i n g whether t h e i n f o r mation accompanying t h e c h a r t s and graphs s u p p l i e d
t o t h e systems a n a l y s t i s complete, then t h e p o s s i b i l i t y o f misunderstandings and m i s i n t e r p r e t a t i o n s
o f t h e d a t a c o u l d b e reduced.
I n t h e d i s c u s s i o n of the ensuing g r a p h s , t h e
supplemental i n f o r m a t i o n w i l l n o t b e broken down
aad p r e s e n t e d under t h e above subheadings. I n s t e a d ,
t h e s a l i e n t f e a t u r e s o f t h e graphs w i l l be d i s c u s s e d
and t h e terms o r concepts which would b e p r e s e n t e d
i n g r e a t e r depth o r d e t a i l i n a n a c t u a l r e p o r t f o r
u s e i n m i s s i o n d e s i g n s t u d i e s w i l l b e mentioned b u t
not necessarily discussed i n d e t a i l .
It s h o u l d b e noted t h a t t h e supplemental i n f o r mation f o r F i g u r e 1, a s p r e s e n t e d above, c o n t a i n s
not o n l y Lnformation which may b e u s e f u l f o r t h e
c o r r e c t i n t e r p r e t a t i o n o f t h e graph b u t p e r i p h e r a l
i n f o r m a t i o n which p r o v i d e s t h e u s e r w i t h a backdrop
a g a i n s t which t h e d a t a on t h e graph c a n b e viewed.
T h i d p e r m i t s t h e systems a n a l y s t t o i n t e r p r e t t h e
d a t a i n a more e f f e c t i v e and meaningful manner.

The v a l u e o f a graph such a s F i g u r e 1 i s t h a t i t
provides an indication, i n the large, of t h e r e s t r i c t i o n s imposed by t h e launch energy. However, s i n c e
t h e g r e a t e s t i n t e r e s t probably c e n t e r s around t h e
lower v a l u e s o f C,, graphs such a s t h e one shown i n
F i g u r e 2 should a l s o be provided. A complete s e t o f
C3 c u r v e s f o r Mars would i n c l u d e seven o f t h e type
p r e s e n t e d i n F i g u r e 1 and f o u r t e e n o f t h e t y p e p r e s e n t e d i n F i g u r e 2 (seven graphs o f t h e lower C,
v a l u e s f o r t h e Type I t r a n s f e r s p l u s seven graphs o f
Also
t h e lowet C3 v a l u e s f o r Type I1 t r a j e c t o r i e s ) .
i n c l u d e d would be seven graphs showing t h e brokenp l a n e t r a n s f e r s which c o u l d b e used t o b r i d g e t h e
energy r i d g e between t h e Type I and Type I1 c o n t o u r s .
These t w e n t y - e i g h t graphs would r e p r e s e n t t h e
f i f t e e n y e a r p e r i o d r e q u i r e d f o r t h e e a r t h and Mars
t o r e t u r n t o a s i m i l a r s p a c e - f i x e d geometry. S i n c e
t h e supplemental i n f o m t i o n which should accompany
graphs o f t h e type shown i n F i g u r e 2 would b e n e a r l y
i d e n t i c a l t o t h a t which i s provided w i t h t h e F i g u r e 1
type o f g r a p h , t h e e n t i r e group o f l a r g e and s m a l l
s c a l e C3 c u r v e s f o r both 5 p e I and Type 11 could b e
i n c l u d e d under t h e same supplemental informa t i o n
s h e e t . The graphs r e p r e s e n t i n g t h e broken-plane
t r a n s f e r s would d i s p l a y n o t only t h e launch energy
c u r v e s b u t curves r e p r e s e n t i n g t h e AV needed f o r t h e
plane-change maneuver i n o r d e r t h a t a proper a s s e s s ment o f t h e energy requirements can b e made. The
method o f computation o f t h e AV would need t o b e
e x p l a i n e d and a d e t a i l e d i l l u s t r a t i o n o f t h e compari s o n between s i n g l e - p l a n e and broken-plane t r a n s f e r s
should a l s o be provided.

�8 =

DECLINATION

OF

=

INCLINATION

OF

ORBIT

P

:

Figure 3

-

Constraints

It would a p p e a r from F i g u r e 1 t h a t a continuous
o p p o r t u n i t y t o l a u n c h e x i s t s from a b o u t t h e middle
of J u n e , 1973 t o t h e m i d d l e o f
assuming t h a t a C, o f 3 0 &amp; / s e
t h e maximum
launch energy a v a i l a b l e . T h i s
month launch
o p p o r t u n i t y would indeed b e a v a i l a b l e i f t h e o n l y
r e s t r i c t i o n f o r a Mars m i s s i o n was t h e launch
energy. However, t h e r e a r e many o t h e r c o n s t r a i n t s
which need t o b e c o n s i d e r e d and which impose some
r a t h e r s e v e r e r e s t r i c t i o n s on t h i s twenty month
launch o p p o r t u n i t y ,
Consider f i r s t the d e c l i n a t i o n of the outgoing
asymptote,
F i g u r e 3 shows t h a t
i s one of t h e
two a n g l e s which d e f i n e t h e d i r e c t i o n o f t h e o u t going a s y m p t o t e ( t h e o t h e r a n g l e b e i n g t h e r i g h t
ascension).
The o u t g o i n g asymptote i n d i c a t e s t h e
d i r e c t i o n t h e s p a c e c r a f t must b e t r a v e l i n g r e l a t i v e
t o t h e e a r t h when t h e s p a c e c r a f t l e a v e s t h e e a r t h ' s
g r a v i t a t i o n a l i n f l u e n c e . The t h r e e views shown i n
F i g u r e 3 i n d i c a t e t h a t any v a l u e o f i may b e used
t o obtain the d e s i r e d value of 6 a s long a s i 2 h.
T h i s may n o t seem l i k e much o f a r e s t r i c t i o n e x c e p t
t h a t t h e v a l u e s o f i which c a n b e o b t a i n e d
(assuming t h a t t h e n e a r - e a r t h f l i g h t t a k e s p l a c e i n
a pace-fixed p l a n e ) a r e l i m i t e d by t h e l a t i t u d e of
t h e launch s i t e and t h e a v a i l a b l e r a n g e o f launch
a z i m u t h s . The minimum i n c l i n a t i o n o f t h e p a r k i n g
o r b i t which may be o b t a i n e d from a l a u n c h i n g a t
Cape Kennedy i s approximately 21;.28', which c a n be
a c h i e v e d by l a u n c h i n g due E a s t on a launch azimuth

*.

-

THE

ASYMPTOTE

E A R T H ' PARKING

I

HYPElE8OLA

VALUES

ACHIEVE

OF
THE

i MAY
SAME

BE

8,

USED

t i L 81

,

R e l a t i o n s h i p o f t h e Parking O r b i t P l a n e t o
t h e D e c l i n a t i o n o f t h e Outgoing Asyslptote

111. E v a l u a t i o n o f t h e h and

,V

OF

MANY

TO

s

OuttOiNG

PLANE

PERIGEE.

NOTE:

THE

of 90' E a s t of North. The maximum v a l u e o f i i s
determined by t h e range s a f e t y r e s t r i c t i o n s a n d / o r
t r a c k i n g requirements which r e s t r i c t t h e a v a i l a b l e
range o f launch azimuths. Thus, a r a n g e of launch
azimuths such a s 70' t o 110' would r e s u l t i n a
this
maximum a t t a i n a b l e v a l u e of i o f a b o u t 35'
would r e s t r i c t t h e u s a b l e v a l u e s of R t o a r a n g e
o f +3s0. The r e l a t i o n s h i p between launch azimuth
and h w i l l b e d i s c u s s e d i n g r e a t e r d e t a i l i n
Section IV.

-

The h y p e r b o l i c - e x c e s s v e l o c i t y a t a r r i v a l , Vm, is
a n o t h e r parameter which r e q u i r e s c o n s i d e r a t i o n i n a
m i s s i o n d e s i g n s t u d y . It p r o v i d e s a n i n d i c a t i o n o f
t h e minimum amount of veloc'ity which t h e s p a c e c r a f t
must l o s e i n o r d e r t o a t t a i n a n o r b i t a b o u t Mare.
Of c o u r s e , t h e s m a l l e r t h e d e s i r e d o r b i t a b o u t Mau,
(assuming t h e shape of o r b i t , e , i s c o n s t a n t ) t h e
g r e a t e r w i l l be t h e impulse o r AV t h a t t h e spacec r a f t w i l l have t o supply. Thus, knowledge of t h e
range o f v a l u e s o f Vm would p r o v i d e i n f o r m a t i o n f o r
d e t e r m i n i n g t h e s i z e o f r o c k e t motor and amount of
f u e l which would be n e c e s s a r y t o a t t a i n an o r b i t
a b o u t Mars.
Shown i n F i g u r e 4 a r e p l o t s of c o n s t a n t v a l u e s of
t h e s e p a r a m e t e r s . The h o r i z o n t a l and v e r t l c a l s c a l e s
a r e i d e n t i c a l t o t h o s e used i n F i g u r e 2 s o t h a t t h e
e f f e c t af t h e s e two parameters on t h e o v e r a l l Type I
launch o p p o r t u n i t y c a n b e e a s i l y e v a l u a t e d . A more
e f f e c t i v e way o f p r e s e n t i n g t h e combined e f f e c t of
C a r Vm, and h i s t o reproduce t h e c u r v e s o f Vm end h
on t r a n s p a r e n c i e s which would o v e r l a y t h e Cg c u r v e s .
It can b e s e e n from F i g u r e 4 t h a t f o r Type I

�.

-

.

ARRIVAL DATE

-

.-

MAY

APR

1974

JAN

DEC
1973 NOV

21

!

, ,
6 44
JUN 73
1

, , ,
16 21 26

,
I

JUL

Figure 4

-

,
6

./
, ,

,

,

,

,

,

,

,

,

,

10 15 20 25 30 4 9
AUG
SE P
LAUNCH DATE

I 1 16 21 26 31

5

Curves of b n d Vm f o r the 1973
Q p e I Launch Opportunity for Mars

.
I

14

i

�t r a n s f e r s , t h e e a r l i e s t a r r i v a l d a t e a t %rs would
p r o b a b l y b e determined by ,V a n d t h a t e a r l y launch
d a t e s a r e r e s t r i c t e d by h . The r e s t r i c t i o n s imposed
upon t h e launch o p p o r t u n i t y by V- and 6 a r e more
s e v e r e i n o t h e r launch y e a r s than is t h e c a s e i n
1973. For m i s s i o n d e s i g n purposes, c u r v e s o f 6 and
,V would a l s o b e provided f o r use w i t h F i g u r e 1
t y p e g r a p h a s w e l l a s t h e lower enargy Type I1
graphs.
A f t e r imposing upon t h e launch o p p o r t u n i t y t h e
c o n s t r a i n t s which have thus f a r been d i s c u s s e d , i t
m y b e u s e f u l t o i n c l u d e some p i c t u r e s t o i l l u s t r a t e what some o f t h e a v a i l a b l e t r a j e c t o r i e s would
look l i k e . Shown i n F i g u r e s 5 and 6 a r e t h r e e o f
t h e t r a j e c t o r i e s t h a t c o u l d b e used f o r a 1973
mission.
The t r a n s f e r s , and t h e o r b i t s o f e a r t h
and Mars, a r e drawn t o s c a l e and a r e viewed from a
v a n t a g e p o i n t above t h e North E c l i p t i c P o l e , with
t h e s u n a t t h e c e n t e r o f t h e f i g u r e s . An examinat i o n o f t h e t r a j e c t o r i e s would r e v e a l t h a t i n
t r a v e r s i n g t h e d i s t a n c e from e a r t h t o Mars, a l l
three of the transfers require a heliocentric transf e r a n g l e o f l e s s t h a n 180°, and thus a l l t h r e e a r e
Type I t r a n s f e r s . Using t h e p r e v i o u s l y mentioned
r e s t r i c t i o n s on A and f&amp; (6 5 +3s0, C j 5 30 &amp; / s e c 2 )
and p l a c i n g a r e s t r i c t i o n upon VW 5 4.0 laa/sec., i t
can b e s e e n from F i g u r e s 2 and 4 t h a t t h e t h r e e

EARLY

LAUMCH

-

EAALY

ARRIVAL

t r a j e c t o r i e s f a l l on t h e boundary of t h e launch
o p p o r t u n i t y d e f i n e d by t h e upper l i m i t s o f V
,
:,
and $ . The t r a j e c t o r y shown i n P i g u r e 5 is
c h a v a c t e r i z e d by v a l u e s o f C3 and
which a r e n e a r
t h e upper l i m i t s of t h e p e r m i s s i b l e r a n g e s o f t h e s e
c o n s t r a i n t s . The two t r a j e c t o r i e s shown i n F i g u r e
6 a r e t h e r e s u l t o f launches which o c c u r l a t e i n
t h e launch o p p o r t u n i t y w i t h t h e s h o r t f l i g h t time
t r a n s f e r having high ,V and C3 v a l u e s , and t h e long
f l i g h t tit r a j e c t o r y r e q u i r i n g t h e maximum a 1 lowa b l e value of &amp;.
P l o t s o f t r a j e c t o r i e s such a s
t h e s e would be o f v a l u e i n h e l p i n g t o visualize t h e
s i m u l a r i t i e s and d i f f e r e n c e s o f t h e t r a n s f e r s which
a r e a v a i l a b l e d u r i n g a launch o p p o r t u n i t y . For
completeness, a group o f t h e s e p l o t s i n t e n d e d f o r
use i n a m i s s i o n d e s i g n s t u d y would a l s o i n c l u d e
i l l u s t r a t i o n s o f a few Type I1 t r a n s f e r s a s w e l l
a s some broken-plane t r a j e c t o r i e s .

IV. Launch Windows
Thus f a r , t h e d i s c u s s i o n of m i s s i o n d e s i g n c h a r t s
h a s c e n t e r e d around t h e launch o p p o r t u n i t y a s
d e f i n e d by 6 , Vm, and C3. T h i s launch o p p o r t u n i t y
( s e e f i g u r e s 2 and 4 ) is a g r i d , w i t h e v e r y p a i r of
launch and a r r i v a l d a t e s r e p r e s e n t i n g a s m a l l s q u a r e
w i t h i n t h e g r i d . The p e r i o d o f time w i t h i n e a c h o f
t h e 24 hour s q u a r e s d u r i n g which a launch c a n o c c u r

*D

LA'E
LATE

. A L ~ I C ~ -I L A ' E A R R I V A L
LAUNCH
E A R L Y ARRIVA!

-

Pigure 6

Figure S
1973 Type I T r a n s f e r s Drawn to S c a l e

�Figure 7

- Launch
Azimuth a s a Function o f Launch
Time w i t h D e c l i n a t i o n a s t h e Parameter

e
i s known a s t h e launch window. Note t h a t w i t h i n
each launch window t h e v a l u e s o f C,, 6 , and Vm
remain r e l a t i v e l y c o n s t a n t . The u s e o f a launch
window is d e s i r a b l e s i n c e t h e a l t e r n a t i v e , t h e
l a u n c h i n g of a v e h i c l e a t a p r e c i s e t i m e , would n o t
p e r m i t a n y unscheduled d e l a y s i n t h e launch prep a r a t i o n s and would n o t a l l o w any h o l d i n g time f o
a w a i t improved w e a t h e r c o n d i t i o n s . The d u r a t i o n of
t h e launch window depends upon t h e r a n g e of a v a i l a b l e launch a z i m u t h s , t h e l a t i t u d e o f t h e launch
s i t e , and t h e d e c l i n a t i o n of t h e o u t g o i n g asymptote,
S i n c e t h e v a l u e o f 6 is e s s e n t i a l l y f i x e d , and t h e
launch s i t e i s r e l a t i v e l y f i x e d ( a t a l a t i t u d e o f
t h e o n l y t h i n g t h a t can b e v a r i e d t o
a b o u t 28.28'),
a c h i e v e a n extended p e r i o d d u r i n g whi,ch t o launch
is t h e launch azimuth. The use o f a v a r i a b l e h u n c h
azimuth implies t h e use of a parking o r b i t s o t h a t
t h e Eirtel b u r n of t h e o r b i t i n g b o o s t v e h i c l e c a n be
properly pos~.rionedw
. t t h r e s p e c t t o t h e outgoing
asymptote. F i g u r e 7 shows t h e s i z e o f t h e launch
window t h a t c a n be o b t a i n e d by v a r y i n g t h e launch
me b f s w i t h the a s t e r i s k s ( * I s ) i n d i c a t e
t h a t t h e y a r e t o b e r e a d a g a i n s t t h e upper launch
t i m e s c a l e , w i t h t h e remaining A ' s t o be r e a d
'
a g a i n s t t h e losJer s c a l e . ~h~ e x c e p t i o n i s 6 = 0'
which i s r e a d a g a i n s t b o t h launch time s c a l e s .
m e d o u b l e v a l u e d n a t u r e of t h e launch time i n d i c a t e s t h a t two s e p a r a t e launch windows may e x i s t
w i t h i n one 24 hour p e r i o d . When t h e a v a i l a b l e
r a n g e o f launch a z i m u t h s is k n a j n and t h e v a l u e o f
8 is known ( t h i s c a n b e o b t a i n e d from graphs such
a s shown i n F i g u r e 4 1 , t h e n t h e l e n g t h o f t h e
a v a i l a b l e launch window(s) c a n be o b t a i n e d i n t h e
f o l l o w i n g manner. A s s m i ng t h e launch azimuth
r e s t r i c t i o n s s t a t e d p r e v i o u s l y (5 110', 2 70') and
R h o f +15',
f i n d t h e i n t e r s e c t i o n of t h e h = 15'*
curve with the horizontal l i n e representing a
lqunch azimuth (LAZ) of 70' and n o t e t h e v a l u e of

*

launch time on t h e
s c a l e -1.93 h o u r s . Now move
a l o n g t h e 6 = 15'* c u r v e towards t h e upper r i g h t
(always move a l o n g t h e c u r v e s o f S i n t h e d i r e c t i o n
o f i n c r e a s i n g time on t h e launch time s c a l e ) u n t i l
t h e i n t e r s e c t i o n w i t h LAZ = 110' i s reached and n o t e
t h i s time on t h e
s c a l e below -6.93 h o u r s . Take
t h e d i f f e r e n c e between t h e s e two times and f i n d t h a t
t h e launch window d u r a t i o n i s f i v e hours. Now t r a c e
a l o n g t h e 6 = 15' c u r v e i n a s i m i l a r mannet from
LAZ = 70' t o LAZ = 110' and, r e a d i n g a g a i n s t t h e
lower launch time s c a l e , t h e d u r a t i o n o f t h e launch
window w i l l be found t o b e 22.07 h o u r s minus 17.07
h o u r s , o r f i v e hours. When t h e ran$e of launch
azimuths i s s w e t r i c a l a b o u t 90' ( a s i s t h e c a s e
w i t h 70°and 110' ) t h e l e n g t h o f t h e two launch
wir~dowsw i l l b e i d e n t i c a l . Assume now t h a t t h e
launch azimuth r e s t r i c t i o n s a r e 6 8 _&lt; LA2 5 loo0
and t h e v a l u e of 6 is +30°.
Tracing along t h e
= 30°* c u r v e shows t h a t i t never r e a c h e s t h e r a n g e
o f al1o;able launch azimuths and t h u s does n o t prov i d e any launch window. However, t r a c i n g a l o n g t h e
= 30' does p r o v i d e a launch window o f 23.77 h o u r s
minus 17.50 h o u r s , o r 6.27 h o u r s . The launch times
shown on F i g u r e 7 do n o t correspond t o t h e S a s t e r n
Standard o r Greenwich Mean times o f launch
the
time shown on t h e s c a l e s is a r e l a t i v e and n o t a n
a b s o l u t e time. S e v e r a l o t h e r s e t s o f c u r v e s , used
i n c o n j u n c t i o n w i t h F i g u r e 7 , would be n e c e s s a r y t o
supply t h e a c t u a l launch times. The primary r e a sons f o r p r o v i d i n g a f o l d e d launch time w a l e on
F i g u r e 7 were t o make i t e a s y t o compute t h e l e n g t h
o f time between t h e end o f t h e f i r s t launch window
and t h e beginning o f t h e second and t o h e l p r e l a t e
t h i s i n f o r m a t i o n t o t h a t on F i g u r e 8. The p r o c e d u r e
whieh has been o u t l i n e d above f o r u s i n g F i g u r e 7 i s
v a l i d only f o r p o s i t i v e v a l u e s of 6 . When n e g a t i v e
v a l u e s o f A a r e ueed i t i s n e c e s s a r y t o move t h e
a s t e r i s k s (*IS) from t h e top launch t i m e s c a l e t o

*

-

�thi? bottom launch time s c a l e and then proceed a s
before.
I n a d d i t i o n t o the d u r a t i o n of t h e launch window,
t h e time t h e boost v e h i c l e must spend c o a s t i n g i n
t h e parking o r b i t can a l s o be expressed a s a funct i o n of t h e launch azimuth and 6. The use of a
c o a s t a r c provides an e f f i c i e n t method f o r t h e prop e r p o s i t i o n i n g of t h e f i n a l burn a r c of t h e boost
vehicle
t h i s is . t h e burn which removes t h e spacec r a f t from i t s e a r t h parking o r b i t and p l a c e s it
o n t o t h e d e s i r e d i n t e r p l a n e t a r y t r a j e c t o r y . Figure
8 and Figure 9 provide a means f o r determining what
t h e l e n g t h o f t h e c o a s t time ( o r c o a s t a r c ) must be
i n o r d e r t o a c h i e v e t h e proper e a r t h d e p a r t u r e
geometry. The i n t e r p r e t a t i o n of Figure 8 i s accomp l i s h e d i n a manner very s i m i l a r t o t h a t used i n
Figure 7. Knowing t h e v a l u e of fi needed and t h e
range of launch azimuths which can b e used, t h e
range of c o a s t a r c s ( c o a s t times) which a r e required
can be found on t h e s c a l e s a c r o s s t h e bottom o f t h e
graph. The a s t e r i s k s (*'s) have t h e same meaning on
Figure 8 a s they d i d on F i g u r e 7 , including t h e
switching of s c a l e s f o r n e g a t i v e values o f h . The
primary d i f f e r e n c e i n t h e i n t e r p r e t a t i o n of Figure 8
a s opposed t o Figure 7 is t h a t t h e s c a l e s f o r t h e
c o a s t time and c o a s t a r c on Figure 8 a r e a b s o l u t e ,
and t h e r e f o r e i n d i v i d u a l values of c o a s t time (coast
a r c ) can be read from t h e graph (on Figure 7 i t was
only p o s s i b l e t o read time spans, a s t h e i n d i v i d u a l
times on t h e graph were r e l a t i v e ) . For example,
assuming a launch azimuth range o f 70' 5 LAZ _&lt; 110'
and a 6 of +IS', i t can be seen from Figure 8 t h a t
t h e c o a s t a r c - r e q u i r e d f o r one launch window ranges

-

"

from about 85' t o 150°, while a range £ran a b o u t
210' t o 275' is necessary f o r the o t h e r launch
window. Since t h e values of t h e c o a s t s r c a r e
a b s o l u t e , then i t can a l s o be s a i d t h a t i f a launch
azimuth of 70' i s used t o achieve a 6 o f +15',
it
would be necessary f o r t h e l e n g t h o f t h e earth
o r b i t a l c o a s t i n g a r c to* be e i t h e r 1 5 6 o r 275'.
*By
using Figures 7-and 8 t o g e t h e r , t h e behavior of t h e
c o a s t a r c a c r o s s t h e launch wtn%ow(s) can be observed. From t h e above example i t i s h n n n t b d t
t h e c o a s t a r c s f o r t h e two launch windavs r a n g e
To determine
from 85O t o 150' and 210' t o 275'.
which is t h e i n i t i a l and which L s t h e f i n a l v a l u e
of the c o a s t a r c s it i s necessary to r e f e r back t o
Figure 7. Using Figure 7, t r a c e a l o n g t h e curves
= +15' i n t h e sense of i n c r e a s i n g launch time.
of
Notice t h a t both launch windows open using a launch
azimuth o f 60' and both c l o s e , f i v e hours l a t e r ,
with a launch azimuth o f 118. Now, using F i g u r e 8 ,
t r a c e along t h e 6 = +15' curves and n o t e t h a t t h e
only way t h e behavior of t h e launch a z i m t h , a s
noted on Figure 7, can be d u p l i c a t e d , i s t o t r a c e
along t h e curves o f d e c l i n a t i o n from r i g h t t o l e f t .
This method o f nro\reprent alpng t h e l i n e s of c o n s t a n t
-%a -&amp;be d e c l i n a t i o n , always moving t o t h e
c o r r e c t procedure f o r u t i l i z i n g Figure 8, i.e.,
within a launch window, a s t h e launch t i m e i n c r e a s e s ,
t h e c o a s t time (coast a r c ) decreases. 2he ranges of
c o a s t a r c s (and c o a s t times) obtained from F i g u r e 8
can be matched t o t h e launch windows o b t a i n e d from
Figure 7 by combining t h e values from t h e a s t e r i s k
(*) s c a l e s t o d e f i n e one launch window and combining t h e values from t h e unmarked s c a l e s to form
t h e o t h e r launch window. ' K e r e f o r e froan the range

LAUNCH AZIMUTH (dep)

COAST TIME (rnlnl

Figure 8

- Launch Azimuth a s a Function of

Coast Arc and
Coast Time with Declination a s t h e Paradleter

�o f launch azimuths and t h e v a l u e o f b used i n t h e
example above, t h e following information i s obtaina b l e front Figures 7 and 8. Two launch witidows a r e
a v a i l a b l e , both o f f i v e hours d u r a t i o n . The f g r s t
launch w i d o w opens w i t h a launch azimuth o f 7@ and
a c o a s t time o f d m u t 37 minutes. As t h e launch
tZme *ncreases, the launch azimuth slowly i n c r e a s e s
and t h e c o a s t time slowly d e c r e a s e s u n t i l , a t t h e
end of t h e f i r s t window, t h e launch a z i m t % has
reached 110' and t h e c o a s t time h a s d e c l i n e d to
about 21 d n u t e s . About 1 0 hours l a t e r the second
launch window opens w i t h a launch azimuth of 70'
and a c o a s t time o f about 67 minutes. Acxoss t h e
window, t h e launch azimuth and c o a s t time v a r y
slowly, a s b e f o r e , u n t i l a t t h e end o f tIy f i v e
hour wendow, t h e launch azimuth a t t a i n s 110' and t h e
c o a s t t i m e reaches 51 minutes.
I n a d d i t i o n t o t h e launch azimuth and 6, t h e
c o a s t a r c 19 a l s o a f u n c t i o n of such t h i n g s a s t h e
parking o r b i t r a d i u s , t h e i n j e c t i o n energy (C,) t h e
t&amp;e aneomely of' t h e iWje.ction. i t i W a t h e escape hyperb o l a , t h e l e n g t h o f t h e f i r s t and second burn a r c s
of t h e b o o s t v e h i c l e , t h e r a d i u s o f c l o s e approach
of t h e escape hypefbola, and t h e l a t i t u d e of t h e
launch s i t e . Constant values were assumed f o r a l l
of t h e s e parameters and t h e values t h a t were used
should c e r t a i n l y b e included w i t h thh supplemental
information provided w i t h t h e graph. It may n o t be
necessary t o i n c l u d e a f u l l e x p l a n a t i o n of t h e meani n g of t h e s e parameters, b u t t h e aystems a n a l y s t
should be provided w i t h t h e knowledge t h a t assumpt i o n s were made and should be given t h e values of .
t h e c o n s t a n t s t h a t were used. The values o f t h e
c o n s t a n t s used i n t h e g e n e r a t i o n o f t h e d a t a o f
Figure 8 a r e , i n t h e o r d e r given above and beginning
= 6583 km (a 100
w i t h t h e parking o r b i t r a d i u s :
12.125
n a u t i c a l m i l e a l t i t u d e parking o r b i t ) ; C,
k d ? s e c 2 ; u = 16.2'; 4 = 20.47'~ I)1 = 29.0';
RCA = 6583 km; m = 28.28'.
Since Pigure 8 could be
expected t o be used w i t h a wide range of Cj '8, and
a change i n t h e C3 does a f f e c t t h e v a l u e of t h e
c o a s t time ( c o a s t a r c ) , t h e e f f e c t o f a v a r i a t i o n i n
C, upon t h e launch window w i l l be discussed b r i e f l y .
A s f o r t h e e f f e c t of t h e o t h e r parameters upon t h e
c o a s t time, s u f f i c e i t t o say t h a t i f a launch i s
made from Cape Kennedy w i t h a S a t u r n V c l a s s v e h i c l e ,
t h e information obtained from Figure 8 would be
completely adequate f o r use i n mission design
s t u d i e s . I f t h e launch window information obtained
from Figure 8 i s a s s o c i a t e d w i t h a n i n t e r p l a n e t a r y
t r a j e c t o r y which r e q u i r e s a n i n j e c t i o n energy (C,)
t h a t i s d i f f e r e n t from 12 .I25 I&amp;
/sec2, then a
c o r r e c t i o n should be made t o t h e c o a s t times ( c o a s t
a r c s ) provided by Figure 8. Figure 9 shows t h e
amount of t h e c o a s t time c o r r e c t i o n a s a f u n c t i o n of
Simply combine t h e a p p r o p r i a t e c o a s t time
C,.
c o r r e c t i o n from Figure 9 w i t h t h e values of t h e
c o a s t time obtained from Figure 6.

+

COAST TIME ( m i n l

,

%

-

To complete t h e supplemental informatioh which
would accompany Figures 7 and 8 i n a mission design
document, mention should be made of t h e use of
"dog- leg" maneuvers which could be used t o extend
t h e launch window. Of course, t h e p e n a l t i e s i n c u r r e d from t h e use of a "dog-leg" maneuver should
a l s o be d i s c u s s e d . A s mentioned previously, i f t h e
s i x subheadings l i s t e d under S e c t i o n I1 a r e used a s
a c h e c k l i s t i n t h e p r e p a r a t i o n of t h e supplemental
information which should accompany each c h a r t o r
graph, then t h e l i k e l i h o o d of misunderstandings and
m i s i n t e r p r e t a t i o n s can be reduced, and t h e systems
engineer can u t i l i z e t h e d a t a with f u l l knowledge of
t h e options which a r e a v a i l a b l e t o him.

Figure 9
..
.

V.

- Parking-Orbit

Coast Time
Correction a s a Function of

C,

-

&lt; ~t eal l i t e O r b i t a l Considera t i o n s

The f i n a l phase t o be considered i n a mission
design study i s t h e a r r i v a l of t h e s p a c e c r a f t a t
t h e trjirget p l a n e t . The a s trodynamica 1 d a t a supplied
t o the' systems a n a l y s t i n support of t M s phase of
t h e study i s c h i e f l y concerned with t h e r e p r e s e n t s t i o n and c l a s s i f i c a t i o n of t h e c h a r a c t e r i s t i c s o f
a l l a v a i l a b l e o r b i t s about Mars, and t h e method by
which these o r b i t s can be a t t a i n e d . It i s n o t
f e a s i b l e , w i t h i n t h e l i m i t e d space a v a i l a b l e i n t h i s
paper, t o p r e s e n t and d i s c e s s the c h a r t s and graphs
which would b e used t o c l a s s i f y and l o c a t e s p e c i f i c
o r b i t s of i n t e r e s t . The d i s c u s s i o n w i l l d e a l p r i marily with the major s c i e n t i f i c and engineering
c o n s t r a i n t s which must be considered i n the course
of t h e o r b i t s e l e c t i o n process.
Since t h e primary reason f o r an o r b i t a l reconnaissance mission t o Mars i s the s c i e n t i f i c invest i g a t i o n of t h e p l a n e t , i t would seem reasonable t o
c o n s i d e r f i r s t t h e s c i e n t i f i c c o n s t r a i n t s upon t h e
o r b i t . These requirements might i n c l u d e r e s t r i c t i o n s on, o r s p e c i f i c a t i o n s o f , t h e o r b i t ' s s i Z e ,
shape, i n c l i n a t i o n and o r i e n t a t i o n f o r such purposes
a s photography, W photometry, meteorology, f i e l d s
and p e r t i c l e s measurements, S-band o c c u l t a t i o n s ,
magnerometer measurements, o r r e l e a s e of a lander
capsule. When a l l of t h e r e s t r i c t i o n s which r e s u l t
from experiments such a s these a r e imposed upon t h e
o r b i t , t h e r e s u l t i n g number of p o s s i b l e o r b i t s which
could be used i s , a t b e s t , s e v e r e l y reduced. Nat,
consider t h e engineering c o n s t r a i n t s upon t h e o r b i t .
These c o n s t r a i n t s a r e imposed s o t h a t t h e various
s p a c e c r a f t systems and subsystems w i l l o p e r a t e
e f f e c t i v e l y and e f f i c i e n t l y , and thus permit t h e
s c i e n t i f i c i n v e s t i g a t i o n s mentioned above t o proceed normally. The engineering c o n s t r a i n t s may
p l a c e requirements on the o r b i t f o r such things a s
power generation ( s p a c e c r a f t must remain i n s u n l i g h t

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p

5

-.
a s much a s p o s s i b l e ) , navigation ( s p a c e c r a f t must
maintain f i x on n a v i g a t i o n a l s t a r t s ) ) , and commun i c e t i o n s (spacpcraf t must maintain c o n t a c t with
e a r t h f o r t h e transmission of d e w ) . I n a d d i t i o n
t o these c o n s t r a i n t s t h e l i m i t a t i o n imposed by t h e
performance of t h e s p a c e c r a f t retro-propulsion
system must be conaiderad. This performance ca2ab i l i t y p l a c e s a lower bound on t h e s i t e and shaoe
of t h e o r b i t s which can be a t t a i n e d about Mars.
The l i m i t a t i o n s imposed by t h i s c o n s t r a i n t a r e
represented on t h e i n t e r p l a n e t a r y launch opportunity
c h a r t s by t h e parameter VW (see Figure 4). When a l l
o f t h e s c i e n t i f i c and engineering c o n s t r a t n t s which
have thus f a r been discussed a r e imposed, i n t o t a l ,
a s requirements upon t h e o r b i t , t h e number of o r b i t s
which can provide t h e d e s i r e d c h a r a c t e r i s t i c s is
o f e n zero. Thus, s i n c e i t w i l l very l i k e l y be t h e
c a s e t h a t everything which i s required o r d e s i r e d
cannot be achieved, i t w i l l be necessary f o r t h e
systems a n a l y s t t o perform t r a d e o f f s t u d i e s i h
o r d e r t o maximize t h e t o t a l s c i e n t i f i c r e t u r n from
t h e mission. The arrtrodpnamicist should t h e r e f o r e
supply d a t a which would r e p r e s e n t , i n an e f f e c t i v e
manner, t h e impact of each of t h e c o n s t r a i n t s upon
t h e s i z e , shape, i n c l i n a t i o n , and o r i e n t a t i o n of
t h e a v a i l a b l e o r b i t s , and which would i n d i c a t e t o
t h e a n a l y s t t h e a v a i l a b l e ranges of t h e q r b i t a i
parameters s o t h a t t h e s t u d i e s can be perfomed i n
a n e f f i c i m t and m n i n g f u l manner.

,

The e f f e c t i v e t r a n s f e r of d a t a from t h e a s t r o dynamicist t o t h e systems engineer can be accomp l i s h e d r a t h e r e a s i l y i f e l i t t l e c a r e i s taken i n
t h e p r e p a r a t i o n of t h e supplemenU1 information
which should aceompany each of t h e c h a r t s and graphs.
The use of a c h e c k l i s t i n t h e p r e p a r a t i o n of t h e
supplemental i n f o m t i o n may help t o e l i m i n a t e
omissions which may occur because of t h e a s t r u dynamicist's f a m i l i a r i t y w i t h h i s own m a t e r i a l .
The o b j e c t i v e of the astrodynamicist should be t o
p r e s e n t t o t h e systems engineer material'whicF can
be used e s s i l y and e f f e c t i v e l y , and which w i l l cont a i n a l l of t h e supplemental information necessary
t o enable t h e system a n a l y s t t o perform meaningful
tradeof f s t u d i e s atid make knowledgeable d e c i s i o n s

.

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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
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                <text>Duncan, J. Reynolds, Jr.</text>
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            <name>Date</name>
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                <text>1969-01-22</text>
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                <text>Astrodynamics</text>
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                <text>Box 30, Folder 14</text>
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                  <text>&lt;a href="http://libarchstor2.uah.edu/digitalcollections/items/show/3332" target="_blank" rel="noreferrer noopener"&gt;View Edwin D. Burwell's World War II service timeline, 1943-1944&lt;/a&gt;</text>
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                  <text>&lt;a href="http://libarchstor.uah.edu:8081/repositories/2/resources/60" target="_blank" rel="noreferrer noopener"&gt;View the Saturn V Collection finding aid in ArchivesSpace&lt;/a&gt;</text>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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                <text>"The Case for Compatibility" is a paper by Robert L. Smith, Jr., who worked in Quality and Reliability Assurance Laboratory at George C. Marshall Space Flight Center. The summary states, "Ever since the use of missiles and space launch vehicles began, questions have existed in every program regarding the similarity between upstream (e.g., manufacturing, static firing ) and launch site checkout equipment. Programs have existed which utilized nearly identical equipment for both uses; other programs have existed in which any resemblance of the equipment was probably coincidental. Many factors have entered the final decisions, not the least of which were economic and schedule considerations, and, in some instances, the organizational structure of the developer."</text>
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                <text>Saturn V Collection</text>
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                <text>Box 17, Folder 61</text>
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                <text>University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabama</text>
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                <text>This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections.</text>
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                  <text>&lt;a href="http://libarchstor.uah.edu:8081/repositories/2/resources/60" target="_blank" rel="noreferrer noopener"&gt;View the Saturn V Collection finding aid in ArchivesSpace&lt;/a&gt;</text>
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                  <text>Saturn V Collection</text>
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              <description>An account of the resource</description>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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                <text>"The Challenge of Change vs the Control of the Process."</text>
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            <description>An account of the resource</description>
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                <text>The introduction states, "This paper is designed to present the Rocketdyne engine program as it applies to the Saturn launch vehicles and will apply to the Apollo program of manned flight to the moon (Fig. 1). The vehicle that will launch this flight is the Saturn V, the largest and most powerful of the Saturn family. This vehicle, 362 feet tall and 33 feet in diameter, will be capable of sending a 45-ton payload to the moon or placing a 120-ton payload in earth orbit. Five F-1 engines power the first stage of the Saturn V; five J-2 engines, the second stage; and one J-2 engine, the third stage. The thrust of the first-stage engines alone will be equivalent to 160 million horsepower. Both of these engines, the F-1 and the J-2, were designed at, and are currently being produced by Rocketdyne."</text>
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                <text>Clark, Ross</text>
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                <text>1964-12-01</text>
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                <text>1960-1969</text>
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            <name>Subject</name>
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                <text>Saturn V</text>
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              <elementText elementTextId="33564">
                <text>Saturn Project (U.S.)</text>
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                <text>Saturn launch vehicles--Design and construction</text>
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                <text>Liquid propellant rockets</text>
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                <text>Liquid propellant rocket engines</text>
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                <text>North American Aviation. Rocketdyne Division</text>
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            <elementTextContainer>
              <elementText elementTextId="33570">
                <text>Saturn V Collection</text>
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              <elementText elementTextId="33571">
                <text>Box 12, Folder 42</text>
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              <elementText elementTextId="206303">
                <text>University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabama</text>
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            <name>Rights</name>
            <description>Information about rights held in and over the resource</description>
            <elementTextContainer>
              <elementText elementTextId="33574">
                <text>This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections.</text>
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