Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Trans-lunar injection
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
== Modeling == [[File:Constellation trans-lunar injection.jpg|thumb |Artist's concept of NASA's [[Constellation program|Constellation]] stack performing the trans-lunar injection burn]] === Patched conics === TLI targeting and lunar transfers are a specific application of the [[N-body problem|n body problem]], which may be approximated in various ways. The simplest way to explore lunar transfer trajectories is by the method of [[Patched Conics|patched conics]]. The spacecraft is assumed to accelerate only under classical 2 body dynamics, being dominated by the Earth until it reaches the Moon's [[Sphere of influence (astrodynamics)|sphere of influence]]. Motion in a patched-conic system is deterministic and simple to calculate, lending itself for rough mission design and "[[Back-of-the-envelope calculation|back of the envelope]]" studies. === Restricted circular three body (RC3B) === More realistically, however, the spacecraft is subject to [[Gravitational force|gravitational forces]] from many bodies. Gravitation from Earth and Moon dominate the spacecraft's acceleration, and since the spacecraft's own mass is negligible in comparison, the spacecraft's trajectory may be better approximated as a [[Euler's three-body problem|restricted three-body problem]]. This model is a closer approximation but lacks an analytic solution,<ref>[[Henri Poincaré]], ''Les Méthodes Nouvelles de Mécanique Céleste'', Paris, Gauthier-Villars et fils, 1892-99.</ref> requiring numerical calculation.<ref>[[Victor Szebehely]], ''Theory of Orbits, The Restricted Problem of Three Bodies'', Yale University, Academic Press, 1967.</ref> === Further accuracy === More detailed simulation involves modeling the Moon's true orbital motion; gravitation from other astronomical bodies; the non-uniformity of the Earth's and Moon's [[Gravitational field|gravity]]; including [[Solar wind|solar radiation pressure]]; and so on. Propagating spacecraft motion in such a model is numerically intensive, but necessary for true mission accuracy.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)