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New answer posted

3 months ago

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A
alok kumar singh

Contributor-Level 10

  F 1 c o s 4 5 ° + F 2 c o s 4 5 ° + F 3 = m v 2 r

G m 2 ( 2 r ) 2 . 1 2 + G m 2 ( 2 r ) 2 . 1 2 + G m 2 ( 2 r ) 2 = m v 2 r            

  v = G m 4 r ( 2 2 + 1 )          

Putting m = 1 kg and r = 1 m,

v = 1 2 G ( 1 + 2 2 )        

 

New answer posted

3 months ago

0 Follower 2 Views

A
alok kumar singh

Contributor-Level 10

  ω = 2 π T ω 1 ω 2 = T 2 T 1 = 8

New answer posted

3 months ago

0 Follower 2 Views

V
Vishal Baghel

Contributor-Level 10

G M ( 3 R / 2 ) 2 = G M R 3 * r

O A = 4 R 9 = r

A B = R 4 R 9 = 5 R 9 O A : A B = 4 : 5 = x : y x = 4

New answer posted

3 months ago

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P
Payal Gupta

Contributor-Level 10

F = m E cos θ

 =m (GMR3*r)*xr ma=mgR*a=gRx

T = 2 π R g

 

New answer posted

3 months ago

0 Follower 3 Views

P
Payal Gupta

Contributor-Level 10

Method – I:

F=MsphereEring=M*Gmx (R2+x2)32=M*Gmx8R (R2+8R2)32=8GMm27R2

Method – II:

F=dFcosθ=cosθ (dm)GM (R2+8R2)=8GMm27R2

New answer posted

3 months ago

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V
Vishal Baghel

Contributor-Level 10

As we go pole to equator, acceleration due to gravity decreases. So, weight of the body will also reduces. Thus, weight on equator will be slightly smaller than 49 N.

New answer posted

3 months ago

0 Follower 5 Views

V
Vishal Baghel

Contributor-Level 10

Image is virtual, when an object is placed at distance 10 cm from the lens and image is real when object is placed at 20 cm from the lens.

Thus, m1 = -m2 => f f 1 0 = f f 2 0 f = 1 5 c m  

New answer posted

3 months ago

0 Follower 2 Views

V
Vishal Baghel

Contributor-Level 10

T = 2 π r 3 G M e

T B T A = 2 π G M e ( r B 3 / 2 r A 3 / 2 ) = 2 * 3 . 1 4 6 . 6 7 * 1 0 1 1 * 6 * 1 0 2 4 [ ( 8 * 1 0 6 ) 3 2 ( 7 * 1 0 6 ) 3 2 ]

New answer posted

3 months ago

0 Follower 4 Views

P
Payal Gupta

Contributor-Level 10

Using conservation of energy :

12mvi2GmmR=0Gmm11R

vi2=2011GmR

Escape velocity is defined as 2GMR

v i = 1 0 1 1 v e

New answer posted

3 months ago

0 Follower 2 Views

V
Vishal Baghel

Contributor-Level 10

Acceleration due to gravity at r distance above the surface = G M ( R + r ) 2  

Acceleration due to gravity at r distance below the surface = G M R 3 ( R r )

So, ratio = ( R r ) ( R + r ) 2 R 3 = ( R r ) ( R 2 + r 2 + 2 R r ) R 3 = 1 + r R r 2 R 2 r 3 R 3

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