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This assignment is for Classical Mechanics. It was assigned by Miss Sangita Singh at Anna University of Technology. It includes: Optimum, Hubble, CourseWare, Synchronization, Gravitaional, Space, Surface, Equator, Orbit, Inclination
Typology: Exercises
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Consider the design and optimization of a 2 stage rocket. We desire to determine the optimum mass ratio between the first and second stages of a rocket. The payload is 10% of the total mass of the rocket M. The mass of the first and second stages together is then 90% of the total mass M. 90% of the mass of each stage is fuel. The mass of the first stage is R times the combined mass of the two stages, (m 1 =. 9 ∗ R ∗ M ), leaving (1 − R) times the combined mass of the two stages for the mass of the second stage (m 2 =. 9 ∗ (1 − R)M ). (R is a number less than 1, say .55 as a typical value.) Now let’s launch. Take c = 4500 and for convenience take the total mass M equal to 1 (payload plus both stages; M = 1). Ignore gravity and use the expression for the ”ideal” Δv from a rocket firing from Lecture 14, Δ(v)ideal = −cln( mmf 0 ) = −cln(μ). Calculate the velocity after the first stage is fired to comple tion and about to be thrown away. Then calculate the additional velocity from the firing of the upper stage after the first stage has been discarded.( Using (v 0 )ideal ignores the effect of gravity and gives the most optimistic prediction of final velocity.)
1-a) Now fire the first stage and fly it to completion. For a general value of R, and the specified masses of the payload, fuel and second stage, what is the final velocity of the rocket after the first firing? What is μ for this part of the calculation?
1-b Now fire the second stage, and fly it to completion. What is the final velocity of the rocket vf after this firing. Express this final velocity as a function of R, the mass ratio of the first stage m 1 to the total rocket mass m 1 + m 2 (excluding payload). What is μ for this part of the calculation?
1-c Find the optimum value of R that maximizes the final velocity. You may do this by either plotting vf inal(R) vs. R, or by taking ( (^) dRdv^ )f inal, setting it equal to zero, and solving for R.
1-d Compare this ”optimum” velocity to the final velocity for a single stage rocket. (What would R be for a single stage rocket?)
Consider the elliptical orbit of a satellite about the earth. At the point of closest approach, the distance from the center of the earth is 5 earth radii. At the furthest approach, the distance is 20 earth radii. Ignore the moon, although it is out there somewhere. The radius of the earth is 6. 37 × 106 m; the mass of the earth is 5. 97 × 1024 kg; the universal gravitational constant G = 6. 67 × 10 −^11 m^3 /kgsec^2
a) What is the total period of the satellite about the earth?
b) What is the time of flight from the point of closest approach, to a point located at an angle of 160 o^ as sketched?
c) What is the velocity of the satellite at the point of closest approach. What is the velocity of the satellite at the farthest point.
Consider two bodies of mass M = 5. 97 × 1024 kg and m = 7. 36 × 1022. Non-dimensionalize distances by the radius of the earth (Re = 6. 36 × 106 m and time by 1 day = 24 hours = 3600 ∗ 24 sec. The masses are separated by a non-dimensional distance of 60.25. They orbit about their common center of mass. Formulate and solve the ”Kepler problem” for the orbital motion of each body about their common center of mass. The universal gravitational constant is G = 6. 67 × 10 −^11 m^3 /kgsec^2.
4-1 Where is the center of mass of the system. How do the bodies move about this center of mass.
4-2 What non-dimensional velocities v 1 and v 2 will produce circular orbits for both bodies?
4-3 What is the non-dimensional radius r 1 of the orbit of M?
4-4 What is the non-dimensional radius r 2 of the orbit of m?