Foundations of Space Dynamics. Ashish Tewari

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target="_blank" rel="nofollow" href="#fb3_img_img_fa7c2697-38e5-5c94-9d1a-c1778d284edb.png" alt="images"/> km, its altitude decays very rapidly, and it re‐enters the atmosphere after only 3.5 orbits (Fig. 1.2). Hence, the life of the spacecraft is only about 3.5 revolutions in a circular orbit of altitude 180 km above Earth. As Figs. 1.1 and 1.2 indicate, a stable orbit around Earth for this spacecraft should have images km at all times.

Altitude, images (km) Density, images
0 1.2252
1 1.1119
5 0.7366
10 0.4136
20 0.0891
30 0.0185
40 0.0041
50 0.0011
60 images
70 images
80 images
90 images
100 images
110 images
120 images
150 images
200 images
250 images

      Apart from the atmospheric effects, there are other environmental perturbations to a spacecraft's flight around a central body, which is assumed to be spherical as required by Eq. (1.2). These are the gravity of the actual (non‐spherical) shape of the central body, as well as the gravity of other remote large bodies, and the solar radiation pressure. However, such effects are typically small enough to be considered small perturbations when compared to the spherical gravity field of the central body given by Eq. (1.2). Such effects can be regarded as small perturbations applied to the orbit governed by Eq. (1.2), and should be carefully modelled in order to predict the actual motion of the spacecraft.

Charts depicting the decay in the orbit due to atmospheric drag for a spacecraft initially placed in a circular orbit of z = 200 km around Earth. Charts depicting the decay in the orbit due to atmospheric drag for a spacecraft initially placed in a circular orbit of z = 180 km around Earth.

       1.1.2 Gravity as the Governing Force

       1.1.3 Topics in Space Dynamics

      Space dynamics consists of two parts: (a) orbital mechanics, which describes the translation in space of the centre of mass of a rigid body primarily under the influence of gravity, and (b) attitude dynamics, which is the description of the rotation of the rigid body about its own centre of mass. While these two topics are largely studied separately, in some cases orbital mechanics and attitude

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