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HERE IS THE EXAMPLE We next calculate the eccentricity. We have 2(-1.3792 107)(6.0797 1010)2 (3.986 x 1014)2 2Eh2 0.64172 [el = so that from Eq.
HERE IS THE EXAMPLE
We next calculate the eccentricity. We have 2(-1.3792 107)(6.0797 1010)2 (3.986 x 1014)2 2Eh2 0.64172 [el = so that from Eq. [3.8.15] -./1-0.64172-0.59857 From Eq. [3.8.18, the semimajor axis is 14.450 in [el d2E2-1.3972 X 10 and from Eq. [3.8.19b], the distance to perigee is 2(-1.3972 x 106) ry-a(I-e)-14.45 xi 06(1-0.59857) 5.8008 x 106m which, unfortunately, is smaller than the radius of the earth. The rocket crashes into the earth I1 on its way back We next calculate the eccentricity. We have 2(-1.3792 107)(6.0797 1010)2 (3.986 x 1014)2 2Eh2 0.64172 [el = so that from Eq. [3.8.15] -./1-0.64172-0.59857 From Eq. [3.8.18, the semimajor axis is 14.450 in [el d2E2-1.3972 X 10 and from Eq. [3.8.19b], the distance to perigee is 2(-1.3972 x 106) ry-a(I-e)-14.45 xi 06(1-0.59857) 5.8008 x 106m which, unfortunately, is smaller than the radius of the earth. The rocket crashes into the earth I1 on its way back
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