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New answer posted

10 months ago

0 Follower 3 Views

V
Vishal Baghel

Contributor-Level 10

Mass of the Earth, M = 6.0 * 1024 kg

Mass of the satellite, m = 200 kg

Radius of the Earth, Re = 6.4 *106 m

Universal gravitational constant, G = 6.67 * 10–11 N m2 kg2

Height of the satellite, h = 400 km = 0.4 *106 m

Total energy of the satellite at height h = 12mv2 + ( -GMemRe+h )

Orbital velocity of the satellite, v = GMeRe+h

Total energy of the satellite at height h = m2 ( GMeRe+h) - ( GMemRe+h ) = - 12(GMemRe+h)

The negative sign indicates that the satellite is bound to the Earth. This is called bound energy of the satellite Typee quationhere.

Energy require to send the satellite out of its orbit = - (bound energy) = 12(GMemRe+h)

=&nb

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New answer posted

10 months ago

0 Follower 11 Views

V
Vishal Baghel

Contributor-Level 10

Escape velocity of the projectile on the Earth's surface, vesc = 11.2 km/s = 11.2 *103 m/s

Projection velocity of the projectile = 3 vesc

Mass of the projectile = m

Velocity of the projectile far away from the Earth = vf

Total energy of the projectile on the Earth = 12 m vp2 - 12 m vesc2

Gravitational potential energy of the projectile far away from the Earth is zero.

Total energy of the projectile far away from the Earth = 12 m vf2

From the law of conservation of energy

12 m vp2  12 m vesc2 = 12 m vf2

vp2-vesc2=vf2

vf = vp2-vesc2 = (3vesc)2-vesc2 = 8* 11.2= 31.68 km/s

New answer posted

10 months ago

0 Follower 6 Views

V
Vishal Baghel

Contributor-Level 10

Velocity of the rocket, v = 5 km/s = 5 *103 m/s

Mass of the Earth, Me = 6.0 * 1024 kg

Radius of the Earth, Re = 6.4 * 106 m

Height reached by rocket mass, m = h

At the Earth's surface

Total energy of the rocket = Kinetic energy + Potential energy = 12 m v2 + ( -GmMeRe )

At highest point h, v = 0, and potential energy = -GmMeRe+h

Total energy of the rocket at height h = -GmMeRe+h

From the law of conservation of energy, we have,

Total energy of the rocket at Earth surface = Total energy at height h

12 m v2 + ( -GmMeRe ) = -GmMeRe+h or 12v2 = GMe(1Re-1Re+h)

12v2 = GMe(1Re-1Re+h) = GMehRe(Re+h) = GMeRe2*Reh(Re+h) = gReh(Re+h) 

...more

New answer posted

10 months ago

0 Follower 1 View

V
Vishal Baghel

Contributor-Level 10

Weight of a body of mass m at Earth's surface, W = mg = 250 N

Body of mass m is located at depth, d = 12Re , where Re is radius of the Earth

Acceleration due to gravity at depth g (d) is given by : g' = (1 - dRe )g = (1/2)g

Weight of the body at depth d

W' = mg' = (1/2) mg = (1/2)W = (1/2) x 250 N = 125 N

New answer posted

10 months ago

0 Follower 2 Views

V
Vishal Baghel

Contributor-Level 10

Weight of the body, W = 63 N

Acceleration due to gravity at h from the Earth's surface is given by

g' = g (1+hRe)2 where g = acceleration due to gravity on the Earth's surface,  Re = Radius of the Earth. h = Re2

g' = g (1+Re/2Re)2 = g (1+h2h)2 = (4/9)g

Weight of the body of mass m at a height h is given by

W' = m X g' = (4/9) mg = (4/9) x w = (4/9) x 63 N = 28 N

New answer posted

10 months ago

0 Follower 4 Views

V
Vishal Baghel

Contributor-Level 10

Distance of the Earth from the Sun, re = 1.50 * 108 km = 1.5 * 1011 m

Time period of the Earth = Te , Time period of the Saturn Ts = 29.5Te

Distance of Saturn from the Sun = rs

From Kepler's 3rd law of planetary motion, we have T =( 4π2r3GM)1/2

For Saturn and Sun, we can write, rs3re3 = Ts2Te3

rs = re(29.5TeTe)2/3 = 1.5 * 1011*(29.51)2/3 = 1.4 X 1012 m

New answer posted

10 months ago

0 Follower 2 Views

V
Vishal Baghel

Contributor-Level 10

Orbital radius of the Earth around the Sun, r = 1.5 * 108 km = 1.5 * 1011 m

Time taken by the Earth to complete 1 revolution around the Sun, T = 1 year = 365.25 days = 365.25 * 24 *24*60*60s

Universal gravitational constant, G = 6.67 *10-11 N m2/kg2

Thus, mass of the Sun can be calculated as,

M = 4π2r3GT2 = 4* (3.1416)2* (1.5*1011)36.67*10-11* (365.25*24*60*60)2 = 2.0 *1030 kg

New answer posted

10 months ago

0 Follower 1 View

V
Vishal Baghel

Contributor-Level 10

If the upper half of the spherical shell is cut out, then the net gravitational force acting on a particle at an arbitrary point P will be in the downward direction. Since gravitational intensity at a point is defined as the gravitational force per unit mass at that point, it will also act in the downward direction. Thus, the gravitational intensity at an arbitrary point P of the hemispherical shell has the direction as indicated by arrow e.

New answer posted

10 months ago

0 Follower 7 Views

V
Vishal Baghel

Contributor-Level 10

Gravitational potential (V) is constant at all points in a spherical shell. Hence the gravitational gradient ( dVdr) is zero everywhere inside the spherical shell. The gravitational potential gradient is equal to the negative of gravitational intensity. Hence intensity is also zero at all points inside the spherical shell. This indicates that gravitational forces acting at a point in a spherical shell are symmetric

If the upper half of a spherical shell is cut out then the net gravitational force acting on a particle located at the centre O will be in the downward direction

Since gravitational intensity at a point is defined as the gravi

...more

New answer posted

10 months ago

0 Follower 2 Views

V
Vishal Baghel

Contributor-Level 10

(a) Legs hold the entire mass of a body in standing position due to gravitational pull. In space, an astronaut feels weightlessness because of the absence of gravity. Therefore swollen feet of an astronaut do not affect him/her in space

 

(b) A swollen face is caused generally because of apparent weightlessness in space. Sense organs such as eyes, ears, nose and mouth constitute a person's face. These symptoms can affect astronaut in space

 

(c) Headaches are caused because of mental strain. It can affect the working of an astronaut in space

 

(d) Space has different orientations. Therefore, orientational problem can affec

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