Physics Gravitation

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2 months ago

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A
alok kumar singh

Contributor-Level 10

E A E B = G M m A 2 * 3 r G M m B 2 * 4 r = m A m B * 4 3 = 4 3 * 4 3 = 1 6 9

New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

g 1 = G M ( R + h ) 2

g 1 = g ( 1 + h R ) 2

Given h = D = 2R

g 1 = g ( 1 + 2 R R ) 2

g 1 = g 9

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2 months ago

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A
alok kumar singh

Contributor-Level 10

M1 ->Mass of satellite (1)

M2 -> Mass of satellite (2)

MP -> Mass of planet    

Now NLM (2) on S1

G M 1 M P R 1 2 = m 1 v 1 2 R 1

Similarly v2 =   G M P R 2

v 1 v 2 = R 2 R 1 = 8 0 0 3 2 0 0 = 1 2 = 1 x                

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Payal Gupta

Contributor-Level 10

m = 1kg ; ΔU=Gmem (R+h) (GmemR)

ΔU=GMmRGMmR+h

=mg0Rmg0R (1+hR)=mg0 {11 (1+3RR)}

=mg0R (34)

=34*1*10*6400km

=48000*103J.

=48MJ.

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2 months ago

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Vishal Baghel

Contributor-Level 10

The law of gravitation holds good for any pair of bodies in the universe.

This is correct statement.

The weight of any person becomes zero when the person is at the centre of the Earth.

Weight = mg

= m * 0 [g = 0 at the centre of the Earth]

= 0

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alok kumar singh

Contributor-Level 10

W equator   = W pole   - m ω 2 R

= 196 - 19.6 * 2 π 24 * 60 * 60 2 * 6400 * 10 3 = 195.33 N

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2 months ago

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Vishal Baghel

Contributor-Level 10

F on P =  G M M r 2 + 2 G M M ( 2 r ) 2

F o n P = G * 1 0 4 1 3 2 ( 1 + 1 2 ) 1 0 0 G

New answer posted

2 months ago

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alok kumar singh

Contributor-Level 10

 

E A E B = G M m A 2 * 3 r G M m B 2 * 4 r = m A m B * 4 3 = 4 3 * 4 3 = 1 6 9

New answer posted

2 months ago

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Payal Gupta

Contributor-Level 10

As we know that gP=g (RR+h)2=g (R54R)2=16g25

Δg=ggP=9g25

The percentage decrease in the weight of the object = Δgg*100=36%

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2 months ago

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Vishal Baghel

Contributor-Level 10

g = G M r 2

d g = 2 G M r 3 d r

d g * 1 0 0 = 2 ( G M r 2 ) d r r * 1 0 0

d g g * 1 0 0 = 2 * 2 ? = 4 %

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