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SPACETRACK REPORT NO. 3
Models for Propagation of
NORAD Element Sets
Felix R. Hoots
Ronald L. Roehrich
December 1980
Package Compiled by
TS Kelso
31 December 1988
General perturbations element sets generated by NORAD can be used to predict position and ve-
locity of Earth-orbiting objects. To do this one must be careful to use a prediction method which
is compatible with the way in whic h the elements were generated. Equations for five compatible
models are given here along with corresponding FO RTRAN IV computer code. With this informa-
tion a user will be able to make satellite predictions which are completely compatible with NORAD
predictions.
i
Contents
ABSTRACT i
CONTENTS ii
1INTRODUCTION 1
2 The Propagation Models 1
3 Compatibility with NORAD Element Sets 2
4 General Program Description 2
5 The SGP Model 3
6 The SGP4 Model 10
7 The SDP4 Model 21
8 The SGP8 Model 31
9 The SDP8 Model 47
10 The Deep-Space Subroutine 58
11 Driver and Function Subroutines 69
12 Users Guide, Constants, and Symbols 76
13 Sample Test Cases 79
14 Sampl e Implementation 85
ACKNOWLEDGEMENTS 86
REFERENCES 87
ii
APPROVED FOR PUBLIC RELEASE; DISTRIBUTION UNLIMITED
Requests for additional copies by agencies of the Department of Defense, their contractors, and
other go vernment agencies should be directed to the:
1
Defense Documentation Center
Cameron Station
Alexandria VA 22314
All other persons and organizations should apply to the:
Department of Commerce
National Technical Information Service
5285 Port Royal Road
Springfield VA 22161
Address special inquiries to:
Project Spacetrack Reports
Office of Astrodynamics
Aerospace Defense Center
ADC/DO6
Peterson AFB CO 80914
1
Editor’s note: These are the addresses from the original document and may no longer be valid.
iii
1INTRODUCTION
NORAD maintains general perturbation element sets on all resident space objects. These element
sets are periodically refined so as to main tain a reasonable prediction capability on all space objects.
In turn, these element sets are provided to users. The purpose of this report is to provide the user
with a means of propagating these element sets in time to obtain a position and velocit y of the
space object.
The most i mp ortant
point to be noted is that not just any prediction model will suffice. The
NORAD element sets are “mean” values obtained by removing periodic variations in a particular
way. In order to obtain goo d predictions, these p erio dic variations must be reconstructed (by
the prediction mo del) in exactly the same way they were removed by NORAD. Hence, inputting
NORAD element sets into a different model (even though the model may be more accurate or even
a numerical integrator) will result in degraded predictions. The NORAD element sets must
be used
with one of the models described in this report in order to retain maximum prediction accuracy.
All space objects are classified by NORAD as near-Earth (period less than 225 minutes) or
deep-space (period greater than or equal 225 minutes). Depending on the period, the NORAD
element sets are automatically generated with the near-Earth or deep-space model. The user can
then calculate the satellite period and know which prediction model to use.
2 THE PROPAGATION MODELS
Five mathematical models for prediction of satellite position and velocity are available. The first
of these, SGP, was dev eloped by Hilton & Kuhlman (1966) and is used for near-Earth satellites.
This model uses a simplification of the work of Kozai (1959) for its gravitational model and it takes
the drag effect on mean motion as linear in time. This assumption dictates a quadratic variation
of mean anomaly with time. The drag effect on eccentricity is modeled in such a way that perigee
height remains constant.
The second model, SGP4, w as developed by Ken Cranford in 1970 (see Lane and Hoots 1979)
and is used for near-Earth satellites. This model was obtained by simplification of the more
extensive analytical theory of Lane and Cranford (1969) which uses the solution of Brouwer (1959)
for its gravitational model and a power density function for its atmospheric model (see Lane, et al.
1962).
The next model, SDP4, is an extension of SGP4 to be used for deep-space satellites. The
deep-space equations were developed by Hujsak (1979) and model the gravitational effects of the
moon and sun as well as certain sectoral and tesseral Earth harmonics whic h are of particular
importance for half-day and one-day period orbits.
The SGP8 model (see Hoots 1980) is used for near-Earth satellites and is obtained by simpli-
fication of an extensive analytical theory of Hoots (to appear) which uses the same gravitational
and atmospheric models as Lane and Cranford did but integrates the differential equations in a
much different manner.
1
Finally, the SDP8 model is an extension of SGP8 to be used for deep-space satellites. The
deep-space effects are modeled in SDP8 with the same equations used in SDP4.
3 COMPATIBILITY WITH NORAD ELEMENT SETS
The NORAD element sets are currently generated with either SGP4 or SDP4 depending on whether
the satellite is near-Earth or deep-space. For element sets sent to external users, the value of mean
motion is altered sligh tly and a pseudo-drag term ( ˙n/2) is generated. These changes allow an SGP
user to make compatible predictions in the following manner. If the satellite is near-Earth, then
the pseudo-drag term used in SGP sim ulates the drag effect of the SGP4 model. If the satellite
is deep-space, then the pseudo-drag term used in SGP sim ulates the deep-space secular effects of
SDP4.
For SGP4 and SDP4 users, the mean motion is first recovered from its altered form and the
drag effect is obtained from the SGP4 drag term (B
∗
) with the pseudo-drag term being ignored.
The value of the mean motion can be used to determine whether the satellite is near-Earth or
deep-space (and hence whether SGP4 or SDP4 was used to generate the element set). From this
information the user can decide whether to use SGP4 or SDP4 for propagation and hence be assured
of agreement with NORAD predictions.
The SGP8 and SDP8 models have the same gravitational and atmospheric models as SGP4
and SDP4, although the form of the solution equations is quite differen t. Additionally, SGP8 and
SDP8 use a ballistic coefficient (B term) in the drag equations rather than the B
∗
drag term.
Ho wever, compatible predictions can be made with NORAD elemen t sets b y first calculating a B
term from the SGP4 B
∗
drag term.
At the present time consideration is being given to replacing SGP4 and SDP4 by SGP8 and
SDP8 as the NORAD satellite models. In such a case the new NORAD element sets would still
give compatible predictions for SGP, SGP4, and SDP4 users and, for SGP8 and SDP8 users, would
give agreement with NORAD predictions.
4 GENERAL PROGRAM DESCRIPTION
The five ephemeris packages cited in Section Two have each been programmed in FORTRAN IV
as stand-alone subroutines. They each access the two function subroutines ACTAN and FMOD2P
and the deep-space equations access the function subroutine THETAG. The function subroutine
ACTAN is a two argument (quadrant preserving) arctangen t subroutine which has been specifically
designed to return the angle within the range of 0 to 2π. The function subroutine FMOD2P takes
an angle and returns the modulo by 2π of that angle. The function subroutine THETA G calculates
the epoch time in days since 1950 Jan 0.0 UTC, stores this in COMMON, and returns the right
ascension of Greenwich at epoch.
One additional subroutine DEEP is accessed by SDP4 and SDP8 to obtain the deep-space
perturbations to b e added to the main equations of motion.
2
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