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AA 4362 Astrodynamics

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from a planet? Escape Velocity. Escape Velocity: Where is the. best place. in an elliptical ... from a planet? Minimum DV. Is always! at. perigee. Which leads ... – PowerPoint PPT presentation

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Title: AA 4362 Astrodynamics


1
AA 4362Astrodynamics
Maneuvering in Space I In-Plane Orbital
Maneuvering
Week 5 Vallado Chapter 6, Sections 6.1, 6.2, 6.3
2
The Vis-ViVa Equation (revisited)
Total (Mechanical) Energy of the Satellite For
a satellite orbiting in a gravity field outside
of the atmosphere (no external drag) there are
no dissipative forces acting, thus the total
energy of the satellite is constant throughout
the orbit
3
Total (Specific) Mechanical Energy
4
Total (Specific) Mechanical Energy
5
Vis-Viva Equation
6
Vis-Viva Equationfor all of the conic sections
7
Applications of the Vis-Viva equation
Escape Velocity Where is the best place
in an elliptical orbit to escape from a planet?
8
Escape Velocity
Escape Velocity Where is the best place
in an elliptical orbit to escape from a planet?
9
Escape Velocity
Escape Velocity Where is the best place
in an elliptical orbit to escape from a planet?
Minimum DV Is always! at perigee
10
Which leads us to In-Plane Orbital Transfer
11
Feasible Transfer Orbits
Transfer Orbit MUST Intersect BOTH Inner and
Outer Orbits
12
Feasible Transfer Orbits (contd)
13
Excess-energy transfer orbit
Wasted DV
Shaded region of aT, eT phase plot
14
Optimal-energy transfer Orbit
Two curves Are tangential In space
Intersection of the Curves on the aT, eT phase
plot
Why, well it is a Constrained
optimization Problem and the answer Is a bit
subtle but here goes
Target Orbit
15
Why is Hohmann Transfer Optimal For DV
DV2
DV1
Burn 1
Burn 2
16
Why is Hohmann Transfer Optimal For DV (contd)
Velocity Of target Orbit
Velocity Of initial Orbit
Velocity Vector after burn 1
Velocity Vector after burn 2
17
Why is Hohmann Transfer Optimal For DV (contd)
18
Why is Hohmann Transfer Optimal For DV (contd)
19
Why is Hohmann Transfer Optimal For DV (contd)
Recall that from the Keplers Third law
derivation
20
Why is Hohmann Transfer Optimal For DV (contd)
Or plugging in the Vis Visa equation
21
Why is Hohmann Transfer Optimal For DV (contd)
Since e lt 1 . Is always positive
Thus for a given aT, the minimum DVT occurs at
the minimum Allowable eccentricity
22
Why is Hohmann Transfer Optimal For DV (contd)
Optimal Solution Occurs Along the feasible region
boundary
Thus For Optimal Transfer The equalities hold
23
Why is Hohmann Transfer Optimal For DV (contd)
Now Look at Orbital Energies
1
2
3
24
Why is Hohmann Transfer Optimal For DV (contd)
Substituting in from the Vis-Viva equation
Boundary Value _at_ Burn 1 Curve
Boundary Value _at_ Burn 2 Curve
25
Why is Hohmann Transfer Optimal For DV (contd)
Substituting in from the Vis-Viva equation
Minimum transfer energy will be at
minimum Eccentricity value along the
feasibility boundary
26
Why is Hohmann Transfer Optimal For DV (contd)
Optimal Solution Occurs Along the feasible region
boundary
Intersection of the boundary curves
Thus For Optimal Transfer The equalities hold
27
Why is Hohmann Transfer Optimal For DV (contd)
Solving for aT, eT
28
Why is Hohmann Transfer Optimal For DV (contd)
Solving for aT, eT
29
The Hohmann Transfer
30
The Hohmann transfer
  • Most fuel efficient method
  • All velocity changes are tangential
  • (change velocity magnitude but not direction)
  • Between circular or (aligned elliptical orbits)
  • Takes longer than other less efficient transfers
  • Tangential elliptical transfer orbit
  • (example Geosynchronous Transfer Orbit GTO)

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32
Hohmann Transfer Calculating the DVs
33
Hohmann Transfer Calculating the DVs
34
Hohmann Transfer Calculating the DVs
35
Hohmann Transfer Calculating the DVs
36
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Hohmann TransferTotal DV
-1
38
Hohmann Transfer Problem Solved!
39
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40
ExampleDV required for Hohmann Transfer from
GEO to LEO
41
ExampleDV required for Hohmann Transfer from
GEO to LEO (contd)
Compute Orbit ratio
Compute Normalized DV
42
ExampleDV required for Hohmann Transfer from
GEO to LEO (contd)
Compute Initial Orbit Velocity
Compute Required DV
43
Example Problem 2
Orbital Rendezvous
44
Transfer Orbit parameters
45
Transfer Orbit period
46
Angular Velocity
47
Angular Velocities (within initial orbits)
48
Lead angle
49
Interceptor Wait time
50
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