PROBLEM 13.104
As a first approximation to the analysis of a space flight from the
earth to Mars, it is assumed that the orbits of the earth and Mars are
circular and coplanar. The mean distances from the sun to the
earth and to Mars are
km and
km,
respectively. To place the spacecraft into an elliptical transfer orbit
at Point A, its speed is increased over a short interval of time to
which is faster than the earth’s orbital speed. When the spacecraft
reaches Point B on the elliptical transfer orbit, its speed
is
increased to the orbital speed of Mars. Knowing that the mass of
the sun is
times the mass of the earth, determine the
increase in velocity required (a) at A, (b) at B.
SOLUTION
3 2 6 2 20 3 2
332.8(10) (9.81 m/s )(6.37 10 m) 1.3247(10) m /sGM = ×=
Circular orbits
9
Earth 29.758 m/s
149.6(10)
E
GM
v= =
9
Mars 24.115 m/s
227.8(10)
M
GM
v= =
Conservation of angular momentum
Elliptical orbit
Conservation of energy
22
99
11
22
149.6(10) 227.8(10)
AB
GM GM
vv−=−
(227.8) 1.52273
(149.6)
AB B
vv v= =
20 20
22 2
99
1 1.3247(10) 1 1.3247(10)
(1.52273)
22
149.6(10) 227.8(10)
BB
vv−=−
28
0.65935 3.0398(10)
B
v=
21, 471 m/s, 32,695 m/s
BA
vv= =
(a) Increase at A,
32.695 29.758 2.94 km/s
AE
vv−= − =
(b) Increase at B,
24.115 21.471 2.64 km/s
BM
vv−= − =