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A physics exercise exploring the concept of escape velocity and its relationship to the conservation of energy. It includes calculations and explanations of key principles, such as gravitational potential energy and kinetic energy. The document also demonstrates the application of these concepts in a practical scenario, providing a clear understanding of escape velocity and its significance in space exploration.
Typology: Assignments
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tmosphe rit^ resistonce^ So^ he^ Sy^ ste^ is^ Con^ Servative^.
Scme
ot sofce^ far^ bjeet^ mass(m)^ = -^ GMm
Re
At r> o,o .'. At Y>,V2 0.
2GMRe
Re
6371 x1o3 =nl.^ || 2o8.52kms :.D^ ms trovee
(X,YYoCenter d Posim masses : Take (^) dtd to
2
I
2
X,=(acos8 coso, a sino tsind
2
2
2
Lot he centev he yod on he civele
2
and (^) let the (^) rod make (^) amg le a (^) win he
Ttal ke CT)^ =^ Lmvt^ +^ Lm^ =^ Jnlvv$).
whele the t sig tels abot bo macsey. Ohe has t, Sne has -.
4
2
4
2
(^2) al Sinb Sin o e d
( The^ t^ tevwms^ cemad^ ot^ ahen^ you^ add^ ) T6telCoor dnatey kinehc energy in hen
.8= k
M
dt
Sd
dfalt
Let M mitmz CTstal mass)
m,
Since he Lagrngian doent des end n tme explicty: 4:-L = Const =
2d (^) ovder
wheve k DDis a cnst
Enrgy Stem (E)
2
M
Since g =^ k
2
for fe atlng body
2
2
2
23 Far^ d'ssipetive^ foces^ :CvNf^ to)
2
2- m,
2
k
whee (^) Si is^ General:ed^ fce^ S=-SE
-V=
nomjevotive,
T= Lm (knehc Cnerg)
2