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ASEN 5519: Interplanetary Mission Design

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Vin: The excess velocity when arriving at a planet. ... Basic limitations: 2-body. equations of motion. Practical Implementation: ... Distant Planets ... – PowerPoint PPT presentation

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Title: ASEN 5519: Interplanetary Mission Design


1
ASEN 5519Interplanetary Mission Design
  • Monday, September 25th, 2006
  • Jeffrey S. Parker

2
Lecture Overview
  • Pork Chop Plots
  • Launch Windows
  • Launch Parameters
  • B-Plane Targeting
  • Planetary Quarantine Requirements
  • Mars Odyssey Example
  • Spacecraft observations and Orbit Determination
  • Using the B-Plane to Target a Planetary Arrival
  • Next Week B-Plane Targeting applied to Gravity
    Flybys

3
Interplanetary Mission Design
  • Why do we go?
  • Science, Exploration, Survival
  • What is the cost?
  • Launch energy
  • Excess arrival energy
  • Time of transfer
  • Planetary Quarantine concerns
  • How do we get there?
  • Launch
  • Optional Gravity Assists
  • Optional Resonant Orbits
  • Optional Deep Space Maneuvers
  • Optional Low-thrust
  • Choose an itinerary that optimizes cost vs.
    benefit!

4
Terminology
Outbound
  • Quick review of terminology
  • C3 Launch Energy (km2/s2)
  • V8 Hyberbolic excess velocity (km/s). It
    is the velocity you have arriving/departing a
    planets sphere of influence (SOI) w.r.t. the
    planet.
  • V8 VS/C VPlanet
  • V8in The excess velocity when arriving at a
    planet.
  • V8out The excess velocity when departing from a
    planet.

VSCHelio
V8out
SOI
5
Lamberts Problem
  • Formulation of Lamberts Problem
  • Given t0, R0, tf, Rf
  • Find V0, Vf
  • Basic limitations 2-body equations of motion
  • Practical Implementation
  • Determines an approximate ?V budget for Planet A
    Planet B transfers for many different dates.
  • Pork Chop Plots

6
Application of Lamberts Problem
  • Trajectories that all depart the Earth at the
    same date, but arrive at Mars at different dates

Type I Transfers
7
Application of Lamberts Problem
  • More Mars arrival dates
  • Remember Earth and Mars are not coplanar! Real
    Hohmann transfers rarely exist

8
Application of Lamberts Problem
  • More Mars arrival dates
  • Type II Trajectories

9
Application of Lamberts Problem
  • Summarizing the results
  • Departure date constant
  • Arrival date variable

Type II
Type I
Type I
Type II
Minimum V8
Minimum C3
10
Varying Departure Dates
  • Now, let us allow the Earth-Departure time to vary

TD June 6, 05
TD June 26, 05
TD July 16, 05
TD Aug 5, 05
TD Aug 25, 05
Best Type I TD Aug 5, 2005, C3 16.15
km2/s2 Best Type II TD Aug 25, 2005, C3 15.6
km2/s2
Best Type I TD Aug 25, 2005, V8 2.47
km/s Best Type II TD June 26, 2005, V8 2.47
km/s
11
Pork Chop Plots (PCPs)
  • Add full trade-space of departure/arrival dates
  • Building-block of basic interplanetary mission
    design
  • Example shown is a PCP for Earth-Mars in 2005.

Mars Arrival Dates
Earth Departure Dates
12
Pork Chop Plots (PCPs)
Type II Transfers
180 over-the-top Transfers (The Ridge)
Type I Transfers
C3 Local Minima
V8 Local Minima
13
Pork Chop Plots (PCPs)
Type II Transfer C3 19.5 km2/s2 V8 2.8
km/s TOF 350 days
Type I Transfer C3 18 km2/s2 V8 2.65 km/s TOF
220 days
Nominal Mars Arrival July 14th, 2006
Nominal Mars Arrival March 26th, 2006
Nominal Earth Departure July 31st, 2005
Nominal Earth Departure Aug. 21st, 2005
14
Resulting Trajectories
Type II
Type I
15
What happens if we miss our launch date?
Type I Transfer
Type II Transfer
23.3 day window
24.0 day window
Example The Launch Vehicle can provide a C3 of
21 km2/s2
16
Pork Chop Plots (PCPs)
Acceptable C3 and V8 ranges
17
Distant Planets
  • A single Pork Chop Plot analysis will generally
    be sufficient for a mission to a local planet.
  • For distant planets, it is usually desirable to
    swing by nearby planets enroute to the distant
    planet to save energy.
  • Implications
  • Produce a PCP for each segment in the itinerary!

18
Review The Hyperbola
19
Hyperbola Toolbox(See Handout on Website)
20
Launch Parameters
z
RLA Right-Ascension of Launch Asymptote DLA
Declination of Launch Asymptote C3 Launch
Energy
Ecliptic Axes (NOT Equatorial)
V8
x
y
21
Launching from Earth
  • Earths pole is tilted with respect to the
    ecliptic. This obliquity angle is approximately
    23.45
  • Additionally, launch vehicles have a limited
    available azimuth-range.

22
Definition of the B-Plane
23
B-Plane Toolbox (Handout on Web)
Positions and velocities may be used at periapse
or at the SOI.
24
B-Plane Targeting
  • Advantage of B-Plane targeting well-linearized
    system!
  • Example constructing a TCM enroute to Mars

Well-behaved and very linear relationships
25
Planetary Quarantine Requirements
  • Planetary Quarantine Requirements (PQRs) enforce
    that a spacecraft shall have a very low chance
    of impacting a planet if at any time during its
    mission all of its propulsion capabilities fail.
  • Especially important in the cases of Venus,
    Earth, Mars, Europa, and various other moons in
    the solar system.
  • In some cases, that means there has to be a 99
    chance of missing the planet at any time during a
    trajectory leg.
  • In other cases, e.g., Cassini flying over Earth
    carrying radioactive materials, the chances of
    miss must be better than 99.9999 (literally).

26
On to the Mars Odyssey Example!
  • (Click here to directly link)
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