Physics Gravitation

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New answer posted

a month ago

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A
alok kumar singh

Contributor-Level 10

m ω 2 . 2 d 3 = G . m . 2 m d 2 ω = 3 G m d 3  

T = 2 π ω = 2 π d 3 3 G m

 

             

New answer posted

a month ago

0 Follower 2 Views

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

a month 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

a month ago

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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

a month 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

a month ago

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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

a month 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

a month ago

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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

a month ago

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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

a month ago

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V
Vishal Baghel

Contributor-Level 10

( v e ) A = ( v e ) B M 1 R 1 = M 2 R 2

R is not correct.

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