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New answer posted•a year ago
New answer posted•a year ago
S
a year ago

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

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New answer posted•a year ago
New answer posted•a year ago
New answer posted•a year ago
S
a year ago

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.

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New answer posted•a year ago
S
a year ago

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  

...Read more

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New answer posted•a year ago
S
a year ago

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 ]

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New answer posted•a year ago
New answer posted•a year ago
S
a year ago

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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New answer posted•a year ago
S
a year ago

at point P,

= K E P + P E P

= 1 2 m v P 2 + { − G M 1 m ( r / 2 ) − G M 2 m r / 2 }

at infinity (ie for escaping from both masses)

⇒ v P = 4 G ( M 1 + M 2 ) r

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