MAE 180A – Spacecraft Guidance I
Winter 2008
ANNOUNCEMENTS:
There will be no lecture on
Tuesday March 4th.
One more question has been
added to HW #3 (Problem 2.13 a)
Office Hours for Wednesday 2/13 and 2/20 have been
cancelled due to room conflicts.
If there are any questions on the homework due Tuesday feel free to send
me an email.
Midterm will be on Tuesday of Week 6 (2/12)
Office Hours for 1/23 will be from 3-4pm, EBU-II 305
Instructor: Professor M. Yousef Bahadori
Email: mbahadori@ucsd.edu
Office: EBU-II 562
Cell: (310) 480-2930
Office Hours: Tuesday 2:30-3:30pm, or by appointment
TA: Garrett Uyema
Email: guyema@ucsd.edu
Office Hours: Wednesday 2-3pm, EBU-II 305
Reader: Peng Liem
Email: peliem@ucsd.edu
Lectures: Tuesday and Thursday 3:30-4:50pm, U413-2
Textbook (required):
Fundamental of Astrodynamics” Bate, Mueller, and White, Dover Publications, Inc.,
1971.
Recommended Text (not required):
Space Mission Analysis and Design, 3rd ed., J.R. Wertz & W.J. Larson
(Eds.), Microcosm Press,
Grading:
Homework – 20%
Midterm – 35% (Tuesday, 2/12) Solutions
Final – 45%
(Tuesday, March 18, 2008, 3:00-6:00pm)
ALL EXAMS ARE OPEN BOOK, BUT CLOSED NOTES/SOLUTIONS
Homework #1(due 1/24): 1.1, 1.2, 1.3, 1.5 (a,b,c,d), 1.8 (a,c,e), 1.9 Solutions
Homework #2 (due 2/7): 2.1, 2.2, 2.5 (c), 2.7, 2.8 (a) Solutions
Homework #3 (due 2/19): 2.8(b), 2.10,
2.12, 2.13 (a) and 2.14 Solutions
For Problem 2.8(b), you will need the answer from Part (a)
of the problem for the following vectors:
r = - 1.177 P - 0.208 Q (DU);
v = 0.362 P - 0.344 Q
(DU/TU)
For Problem 2.13 (a), find e, p, unit vectors P, Q, and W, and
velocity vector v2.
Homework #4 (due 2/28): Solutions
3.1 (but use
westward movement of the orbit at a rate of 5 degrees/day), 3.2, 3.6 (prove for
each part whether the orbit is possible or impossible), 3.8
3.9 (for notation consistency, use r1 = 1 DU,
r2 = 15 DU, and r3 = infinite);
Homework #5 (due 3/6): Solutions
Problem 1:
The orbit of
an Earth satellite has r(perigee) = 1.5 DU, and its parameter is p = 2.5
DU. At point A on the
orbit, its
true anomaly is 75 degrees. Calculate the time of flight to apogee (point B)
after the satellite
passes three
times through the perigee. Provide
the answer in "days-hours-minutes" for example: "5 days, 3
hours, 27 minutes."
Problem 2:
Using the
data and results from Problem 1, show the following on a separate sheet
(to-scale and detailed):
Earth
(assumed spherical), satellite orbit, auxiliary circle, true anomaly for points
A and B, perigee,
apogee,
prime focus, vacant focus, and eccentric anomaly for points A and B. Calculating the semi-minor
axis, b (in
units of DU), helps in the drawing.
You can fit everything on a single 8.5"x11" sheet if you use
a scale of 2
cm = 1 DU for the drawing.
Problem 3:
A space
probe is approaching the sun on a parabolic path (i.e., a one-time encounter),
with perihelion
distance of
0.8 AU. How many days is the probe
closer than 1.1 AU to the sun?
Homework
#6 (due 3/13): 8.10, 8.11,
8.12, 8.13, 8.14 Solutions