AME 30381: Orbital and Space Dynamics


CATALOG DATA:
The one- and two-body problems: geometrical elements and time dependence.  Orbital determination.  Linear orbits and regularization.  Orbital transfer.  The n-body problem: various forms of the three-body problem, including the circular restricted case, its "equilibrium" solutions and their stability.

Prerequisites: AME 20222

TEXTBOOK:
Fundamentals of Astrodynamics; Bake, Mueller and White

COURSE OBJECTIVES :
Upon competion of this course a student should be able to:

TOPICS COVERED:

SCHEDULE:
Course meets three times a week for 50 minutes or twice a week for 75 minute
s

CONTRIBUTION TO THE PROFESSIONAL COMPONENT:
This course represents a balance between engineering science and design, with approximately 67% engineering science and 33% design.

CONTRIBUTION TO PROGRAM LEARNING OUTCOMES AND ASSESSMENT :

Outcome criterion

Topic

Student’s previous
knowledge

Direct measures of
outcome

e

Be able to develop the dynamic model, or equations of motion, which approximate the motion of orbiting bodies using Newton's second law

Newton's second law

Homework \#4 and First Exam

b

Be able to analytically solve the dynamic model for
the classical two-body problem.

Differential equations

Second Exam

b

Be able to numerically solve the dynamic model for
systems with more than two bodies using numerical integration.

Computer programming

Homework \#6 and several homeworks after.

Prepared by: Alan P. Bowling, June 6, 2006

Direct comments, questions, and corrections to amedept@nd.edu