Foundations of Space Dynamics. Ashish Tewari
Читать онлайн книгу.target="_blank" rel="nofollow" href="#fb3_img_img_767a0f81-4e24-5ff7-a544-d71b1b23ee83.png" alt="Geometry of an elemental mass, dM, of a body with centre of mass O, and a test mass, m1, located away from the body."/>
Figure 2.4 An elemental mass,
For all the
(2.73)
which results in the following expression for the acceleration of the test mass:
(2.74)
where s is the distance of the test mass,
(2.75)
with
From Fig. 2.4 it follows that
(2.76)
and
(2.77)
the gravitational potential of the mass distribution is given by
and the gravitational acceleration at
(2.79)
2.7.1 Legendre Polynomials
To carry out the integration in Eq. (2.78), it is assumed that the body is entirely contained within the radius
Equation (2.80) is an infinite series expansion in polynomials of
where
(2.82)
with
(2.83)
The first few Legendre polynomials are the following:
(2.84)
Clearly the Legendre polynomials satisfy the condition
By writing
(2.85)
The generating function can be used to establish some of the basic properties of the Legendre polynomials, such as the following: