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Armageddon. Earth revolves around the sun in an approximately circular orbit with radius r = a, completing a revolution in the time T=2a3GM12, which is one Earth year; here M is the mass of the sun and G is the universal gravitational constant. The gravitational force of the sun on Earth is given by GMmr2, where m is the mass of Earth. Therefore, if Earth 鈥渟tood still,鈥 losing its orbital velocity, it would fall on a straight line into the sun in accordance with Newton鈥檚 second law: md2rdt2=-GMmr2.

If this calamity occurred, what fraction of the normal year T would it take for Earth to splash into the sun (i.e., achieve r = 0)? [Hint: Use the energy integral lemma and the initial conditionsr0=a,r'0=0 .]

Short Answer

Expert verified

Therefore, the fraction of the normal year T would take for Earth splashing into the sun is t=T42.

Step by step solution

01

General form

The Energy Integral Lemma:

Let y(t) be a solution to the differential equation y=fy, where f(y) is a continuous function that does not depend on y鈥 or the independent variable t. Let F(y) be an indefinite integral offy , that is,fy=ddyFy . Then the quantity Et:=12y't2-Fytis constant; i.e.ddtEt=0

02

Verify the equations

Given that,Newton鈥檚 second law of equation is md2rdt2=-GMmr2 鈥 (1)

Then, r=-GMr2. So, fr=-GMr2

Now find the F(r).

fr=ddrFr-GMr2=ddrGMrFr=GMr

Then, find the quantity.

E=12r't2-Frt=12r't2-GMr

E=12r't2-GMr.......(2)

03

Find the initial conditions

Given that initial conditions are r0=a,r'0=0

Then,

E=12r'02-GMr0=-GMa

Now, substitute the value of E in equation (2).

E=12r't2-GMr-GMa=12r't2-GMr12r't2=GMr-GMa=GM1r-1ar't2=2GM1r-1ar't=2GM1r-1a

04

Find the value of t

Since the Earth is losing its orbital velocity. That is, r is decreasing function. So,

r't=-2GM1r-1a

Then, use the above condition to find the value of t.

drdt=-2GM1r-1a-dt=dr2GM1r-1a=12GMdr1r-1a2GMt=-a1a-a-r-a32arctana1r-1a

Put r = 0,

2GMt=a322t=a3222GM

Given that,

T=2a3GM12

Now find the ratio.

tT=a3222GM2a3GM12=142t=T42

Hence proved.

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