NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the...

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NASA TECHNICAL MEMORANDUM LARGE ANGLE METHOD FOR SPACE VEHICLE ANGULAR MOMENTUM DESATURATION USING GRAVITY GRADIEM~TORQUES NASA https://ntrs.nasa.gov/search.jsp?R=19700010562 2020-03-30T07:11:05+00:00Z

Transcript of NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the...

Page 1: NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems

NASA TECHNICAL MEMORANDUM

LARGE ANGLE METHOD FOR SPACE VEHICLE ANGULAR MOMENTUM DESATURATION USING GRAVITY GRADIEM~TORQUES

NASA

https://ntrs.nasa.gov/search.jsp?R=19700010562 2020-03-30T07:11:05+00:00Z

Page 2: NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems
Page 3: NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems

Sl-:.iAL\!t\- ........................................ 1 -

l s ~ ~ - ~ ~ ~ ~ ~ l ~ ~ ~ ~ ~ ~ l c ~ ~ . ..................... i .............. 2

i J E s \ l - u l L - ~ - ~ - ~ o s CC'?"lJL\X\'. ............................ 10

IEFEiZEWES ....................................... 26

i i i

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Figure

1.

-? -. A-1.

A-2.

-A-3.

A-4,

LIST OF ILLUSTRATIONS

Titlp

Maneuverangles ............................ 8

N o r d z e d .>-torque profile .................... n

ATBi/-LW’CSM d g u r a t i o n .................... 20

The celestial spbem. .......... ............. 20

ATM sun (ecliptic) coordinate system d a t i v e to eq1~1t0ri.d system Xs= ( + z j X E . . . . .............. 21

A-3. ATM reference coordhate system relative to ot%ital -

,426,

Table

1.

Page

system x = [qxl[qylX,. ...................... 22 H ATM flhturbacc C o o k d i n a k system relative to orbital system x = [qt+q IX ................. E

D Y O

LIST OF TABLES

Singlc-Asis Uaneuvers ........................ 7

Xngd.tr Velwity Conmulds for s, y, and z VehicieAxes.. ............................. 9

iv

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i A

C

H -

11s

H --uria

I

k

K. 'I

n li

n. m-1)

p' -

T-conrporwnts of the &saturation momentum (Nms)

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ls,J =

DEFINITION O f SYMBOLS CContinued)

- Lv t

u

*?l

O31

1

c‘

si

GV

0

2

lu general, angular quantities in brackets with a subscript indicate a rotation matrix abut the asis of the subscript. Orher exanrples are [A ’ hZJ 1 ezj

1~ 1, ir 1, IrJ YJ ’

x Y

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DEFINITION OF SYMBOLS (Concluded)

viii

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TEC I" :;LA L MEMORANDUM S-53958

LARGE ANGLE NKTHOD FOR SPACE VEHICLE ANGULAR MOMENTUM DESATURATION USING GWWITY

GRADIENT TORQUES

S UMhlAR Y

An ankwlar momentum desaturation metbod is prese:ited for space vehicles in orbit. This iiirtthod utilims the gravity gradient torques m d - therefom avoids the necessiq fpr iii:LSS espulsion by nhzction jet attitude

. control systems. The desatumtfon mctho(J is based on the assumption that- the iiliniinum moment-of-inertia curis has tn be aligrted with the sun vector during orbital daylight for solar esperinients. It is further assumed that the Wference between the two large nioiiients of inertia is negligible. Large angular inaneuvers of the minimum moment-of-inertia axis during the orbitd night ina9mize the gravity gradient toiqws that are then utilized for desaturation of the angular momentum storcd by a momentum storage device such as control moment gyros.

The basic idea of the desatumtion method is that, icir as long as possible, the vehicle nliniiawu moment-of-inertia axis keeps a consbnt attitude with respect to a rotating coordinate system in which the local vertical is along one of the ases and the orbital angular velocity is along another. The constant attitude. with respect to the rotating coordinaie s_vsttni, is calculated for prupei tmnientuni desaturation.

To keep a constant attitude in a system rutating with constant angular velocity requires. in general. iwrtial angular rates about all body axes ,ciniultancously. These rclte; fire cvnstant and present no probieni for the implenientation of the desaturation method.

The gravity gradieilt torque is perpendicular to both the local vertical :tnd the iiiiniinum ii~oiiient-of-inertra axis for the assumed vehicle configuration.

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I NTR3DUCT I OM

Some niissions for space vehicles in orbit require an itivestigation of a celestial object which in tl\riI rtquires an inertially fixed attitude cluring the time the celestial object is not occ~~tecl by the earth; e. g. , the Apollo Telescope Mount (hThl) and its solar experinients [ I, 21. In the fouowing, ATM rmuenclature and clefititions will be uscd; e, g. , sun instead of celestial object or night i n s t m i of occultation time, etc. The once-considered ATM/LR/CSM configuration wiu also be used, since it had the inoment-of- inertia distrilxtion typicnl for the angular nionientlan desaturation nicthod u d e r discussion.

Gravity gradient, aerodynamic, and other external torques Zcting on the vehicle during the time the vehicle is ineftially fised must be absorbed bv an angular nioinentuiii s toras device, which always has limited capacity. A method Tor iuonientuin desaturation which does not require wass expulsion is desired. The fact that an inertially fixed attitude is not required during night allows tlle utilization of the gravity ~rndicc: ;z cszj*.lnrtion with vehicle attitude nianeuv-c : %=uwate t h ~ monierltuni storage device.

Two typically different cases can be jdentlt'ied for the problein of nionientum desaturation if it is assunied that two of the princilml mommts of inertia of the vehicle are mout the same and the third is .sniaUer. In the first case, the ininiinuni iionlent-of-inertia axis can be D u t into the orbital plme and kept perpendicular to the sun vector. Tllis case is treated in Reference 9 'ulcl does not present ;1 probleni. In the second case, the iiiiniiiiu:u nioiiient-of-iner.tia axis is par: ilel to the sun vector, and 3 c!esiaturation iiietIu1 for this case is treated in Reference 4. Ikwever, si inu1:~tim 4 ~ 1 ~ eci that this nietliod (which worked stitisfDc% ii; iw ihe gravity gradient toxcjucs alone; ivas izot cffcctivz when signsicant aerodyn:uiiic torques were encountc 1'0 i . The Iiiethoct :!*:scribed ia the follo\ving sections increases the effectiveness by mssiiiiizing the gravity gradient torques and the time the.';@ ?orqucs are ayp1ic.d. This rcquircc the iifiiiiiiiuiu iiioiri~nt-of-inerti~ axis to 11:i\~d a ccinstrmt altitude with rtqpect to the grwity gixdient direction, and t!,is attitudtl :nust he mnin- tainccl as long a:: pxsilk.

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GRAVITY GRADIENT I 3RQUE AND MOMENTUM ACCUMULATION

- r = .

&P

or

T -G I'

-r z

-r

0

I J

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with -

A1 = - I - I

1 1 = I - I

S Z Y -

Y s z

where I , I , I s y z are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems are used which are given in Appendis A. Equation (4) can be further siinpIified if the gssunlpticin is nncie that I and I alp identicat:

are principal moments of ine-, and the conqmnents of - r

I Y

Throughout this report, the assumption is &de ihat there is no misalignment between the vehicie- principal moment-of-inertia ais ami tbe geometric axes. Under this condition the coinpineats of the radius vector r ulth respect to the principal ases are

0

%

s -sr)

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e?j (1 + cat) s

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-?S S

by p into thc y - and z -z.t\s, S P 5,

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. - -

. .

. - . S E

Y 0

Z 0

xt:

- -

. -

x, y, Ah'D z VEHICLE XSES

where

- . . I-.

..

.\ .

4 , .

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- - . .

. . . - -_

Page 19: NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems

where 51 is the orbitai rate 3nd 4 about the large 111.oinent-of-int:rtia ask.

is the angular rate limit of the vehicle L

DESATURATION COMMANDS

Each desatur-tion method can be split into two parts. One part is concerned with the wneration of the desaturation comlunnds; the other part is concerned with the schbme to desaturak the coln-mded momentum, These two parts are rather independent of-each other; e. g. , several M e n d niethds for the momentum command generation could use the &uue method for thc maneuver angie geueration.

Several facts that affect the moi.ientum conimaml generation must be born in mind.: The first is that approximations will haye to be made for the calculation of the angular moixentum desatumted by a given set-of nsrneuvers, or the mathematical treatment becomes unmanageable. Semndly,

~ the stored anguhr tuouientuni is the difference between the accumulation mc! the desaturation and does not indicate the desaturation itself. Furthermore, the assumptions bvere made that the large inertias are equal and that there is no misalignment between the principal moment-of-inertia ases and the %eo- metric vehicle axes. It is therefore impossible to generate an esact coiiiiirana, aixi the &saturation command h s to be uplated by a suninration process such th:it t i = s, y,z)

Di = H 7 AH

Di II Di (n-l) )1

u1ier.c H is thc present des:tturation coiiiiiiand, H is that of the Din Ditn-1) +st orbit. ana AH is the desircd change. The latter has to Ix. chosen

Di sc:!’. that H will honie in on llie csnc! solulion. Smiiplc data system

consideratimi shows the f d i G i \ ing iirrrn to bc aclcquatc 3.4 J : Di

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= Z H + K H AH Din n Ain (R-1) Aiiti-1)

Le.. it is necessa~y to also consitler the past orbit. H

an ,dr moiuentuni dependent on the stot-ed iiioirientuiu of the- following form:

is an average Ai

This form averages the peak inoinenta (during the ciay~hdf of the orbit only) and provides a selectable offset through H- which allows the conversion, on

the average, to any point in the nioaientum space, B-

or ease of initiaGzation (initial values for the snglcs are knoivn, and the oiies for the nioiiienturn cot~i~nmds are not) equation (12) is replaced by - equations U€ the form

The summation of the desatumtion co&iand changes; cf. equation (12).

is now in the past nuncuver coiiiiiiands rathcr than in the

DESATURATION MANEUVER EFFECTIVENESS

11

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u I'

1117)

Transforination of the gravity gradient toiqiie to the I-sjsteul rcsults in

1'

i ;1

(1s)

1 ' . -b 1'

Evaluation of eqlxiion (IS) \\-it11 the use of cqclatims ( 6 ) and (17) results in ( seconld-or:;er terins are neglected: details are in Appendix B)

r 7

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Espressions of the iiixneuver tingles as ;L funcrion of the coniiwndcd iiioi’iientuin .&re fieecied FUC!I thtrt the :icturd iiimientuin of equations ( 2 0 ) . (21) . rind ( 2 2 ) equ;ds or nppr’oric.lies the coiiiixmndcc! iiionientuin. -Aciclitional con- straints w e needed since there ;ire iiwre nianeuver angles th:m equ:itionc.

Equations (12) and (15) show that there is interest in the @is

connected ivith the change c! the i~imeuver coiiinialids. Partial c1iffercnti:ition will supply the oiie for X i :

S

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14

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(3-5 j

The angular ~uomcnh am measured abut the vehicle LX~S (whrcu, under the assuuq~tir?r! G: no uusslignment, is the P-sy-steml u-hilc king sun-oriented, but for the development so far, 3!1 momenta eompnents were assumed tu k in the I-system, and a resokution is ncxxssary:

.bsuiue an orbital angle fi.om -p to +p (us~mlly equivalent to the night i n t e i w i j with respect to midnight is available for desaturaticn: then i p is

Page 26: NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems

CONCLUS ICN AND 2fCOMMENDATIONS

.- I *

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APPENDIX A

OEFlNITlONS OF ATM COORDINATE SYSEMS AND ANGLES

s,, i..!S, A

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S

-S

S z

I S

S

v

k;

5

Page 29: NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems
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APPENDIX B

DESATURATfON TORQUE AND ANGULAR MOMENTUM COMPONENTS

The conipunents of the desaturstion torue s - d d be in an inertial frame for etrse of integration to obtain the angpiar desatumiir:n mwneentuni. The components of the &saturation torque in the T - S ~ S ~ I U are [see

or, with equation (17) and neglecting second-order terms.

Integration of the s-coniponcnt of T froin --GT

23

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Page 36: NASA TECHNICAL MEMORANDUM · with - A1 =-I -I 11 = I -I S ZY - Y sz where I , I I syz are in the P-system Fur convenience and comparison, the definitions for ATM coordinate systems