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New answer posted

10 months ago

0 Follower 8 Views

P
Payal Gupta

Contributor-Level 10

This is a long answer type question as classified in NCERT Exemplar

When a small element of length dx is considered at x from the load x=0

(a) letT(x) and T(x+dx) are tensions on the two cross sections a distance dx apart then

T(x+dx)+T(x)=dmg= μ dxg

dT= μ gx+C

at x=0 T(0)=mg

C=mg

T(x)= μ gx+Mg

Let length dx at x increases by dr then

Young's modulus Y= stress/strain

T x A d r d x = Y

d r d x = T x Y A

r= 1 Y A 0 L ( μ g x + M g ) d x

= 1 Y A μ g x 2 2 + M g x 0L

r= 1 2 * 10 11 * π * 10 - 6 π * 786 * 10 - 3 * 10 * 10 2 + 25 * 10 * 10

 

so r = 4 * 10 - 3 m

(b) tension will be maximum at x=L

T= μ g L +Mg=(m+M)g

The force = (yield strength) area= 250 * π N

(m+M)g= 250 π

Mg 250 π

M= 25 π 75 k g

New answer posted

10 months ago

0 Follower 4 Views

A
alok kumar singh

Contributor-Level 10

This is a Multiple Choice Questions as classified in NCERT Exemplar

Answer-d

Explanation- We treated that the mass of earth is at centre . in this case a=g=0 at centre but if earth is not uniform then value of g is different at different point.

New answer posted

10 months ago

0 Follower 17 Views

P
Payal Gupta

Contributor-Level 10

This is a long answer type question as classified in NCERT Exemplar

Let the cross sectional area A . consider the equilibrium of the plane aa'. A force F must be acting on this plane making an angle of π 2 - θ with the normal ON. Resolving F into components along the plane (FP) and normal to the plane.

By resolving into components

We get Fp= Fcos θ

And FN= Fsin θ

Let area of the face aa' be A' then

A/A'=sin θ  so A=A'sin θ

The tensile stress = normal force/area=Fsin θ / A '

= F s i n θ A / s i n θ = F A sin2 θ

Shearing stress = parallel foce/Area

= F c o s θ A / s i n θ = F A s i n θ c o s θ

F 2 A ( 2 s i n θ c o s θ = F 2 A s i n 2 θ

a) For stress to be maximum , sin2 θ =1

So θ = π 2

b) Shearing stress to be maximum

sin2 θ = 1

So θ = π 4

New answer posted

10 months ago

0 Follower 2 Views

A
alok kumar singh

Contributor-Level 10

This is a  Short Answer Type Questions as classified in NCERT Exemplar

Explanation- Gravitational force at h height F = G M m h ( r 2 + h 2 ) 3 / 2

When mass is displaced upto distance 2h then

F'= G M m 2 h [ r 2 + ( 2 h ) ] 2 ] 3 2

= 2 G M m h r 2 + 4 h 2 3 2

When h = r then F= G M m h [ r 2 + ( r ) 2 ] 3 / 2

So F = G M m 2 2 r 2

F'= 2 G M m r r 2 + 4 r 2 3 2 = 2 G M m 5 5 r 2

F ' F = 4 2 5 5

F' = 4 2 5 5 F

New answer posted

10 months ago

0 Follower 1 View

A
alok kumar singh

Contributor-Level 10

This is a  Short Answer Type Questions as classified in NCERT Exemplar

Explanation-potential energy of the objects at the surface of the earth is =- G M m R

PE of the object at a height equal to radius of earth = G M m 2 R

Gain in potential energy = G M m 2 R - (- G M m R )= G M m 2 R

= g R 2 m 2 R = 1 2 m g R (GM=gR2)

New answer posted

10 months ago

0 Follower 12 Views

A
alok kumar singh

Contributor-Level 10

This is a  Short Answer Type Questions as classified in NCERT Exemplar

Explanation-The trajectory of a particle under gravitational force of the earth will be in conic section with the centre of the earth as a focus. Only c meets this requirements

New answer posted

10 months ago

0 Follower 4 Views

A
alok kumar singh

Contributor-Level 10

This is a  Short Answer Type Questions as classified in NCERT Exemplar

Explanation- Orbital speed of the satellite vo= G M R

KE of the satellite of mass m, Ek = 1/2mvo2= Gmm/2R              

So kinetic energy is inversely proportional to distance.

b)potential energy of a satellite Ep=-GMm/R

so it is also inversely proportional to R

c)total energy of the satellite E=Ek+Ep = G M m 2 R - G M m R = - G M m 2 R

New answer posted

10 months ago

0 Follower 3 Views

A
alok kumar singh

Contributor-Level 10

This is a  Short Answer Type Questions as classified in NCERT Exemplar

Explanation- Let M be the mass and R be the radius of sphere . an object of mass m be placed at the mid point P of the line joining their centres

Force F1=F2=GMm/ (5R)2

If we displace it through x distance

New force towards sphere A, F1'= GMm/ (5R-x)2

Sphere B F2' = GMm/ (5R+x)2

As F1'>F2' therefore a resultant force (F1'-F2') acts on the objects towards sphere A therefore objects start to move towards A hence equilibrium is unstable.

New answer posted

10 months ago

0 Follower 2 Views

A
alok kumar singh

Contributor-Level 10

This is a  Short Answer Type Questions as classified in NCERT Exemplar

Explanation-Every day the earth advances in the orbit by approximately 10. Then it will have to rotate by 3610 to have the sun at zenith point again. So 3610 corresponds to 24h

So 1o corresponds to 24/361= 0.066h=3.99 min =4min

Hence distant stars would rise 4 min early every successive day.

New answer posted

10 months ago

0 Follower 2 Views

A
alok kumar singh

Contributor-Level 10

This is a  Short Answer Type Questions as classified in NCERT Exemplar

Explanation- Angle between the equatorial plane and orbital plane of a polar satellite is 900 and angle between equatorial plane and orbital plane of a geostationary satellite is 00.

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