ACCELERATIONDUETO GRAVITY ANDITSVARIATION
Gravitation

270552 A particle hanging from a massless spring stretches it by \(2 \mathbf{~ c m}\) at earth's surface. How much will the same particle stretch the spring at a height of \(2624 \mathrm{Km}\) from the surface of the earth? (Radius of earth \(=6400 \mathrm{Km})\)

1 \(1 \mathrm{~cm}\)
2 \(2 \mathrm{~cm}\)
3 \(3 \mathrm{~cm}\)
4 \(4 \mathrm{~cm}\)
Gravitation

270553 The value of acceleration due to gravity ' \(g\) ' on the surface of a planet with radius double that of earth and same mean density as that of the earth is \(\left(g_{e}=\right.\) acceleration due to gravity on the surface of earth)

1 \(g_{p}=2 g_{e}\)
2 \(g_{p}=g_{e} / 2\)
3 \(.g_{p}=g_{e} / 4\)
4 \( g_{p}=4 g_{e}\)
Gravitation

270554 If \(\mathbf{g}\) is acceleration due to gravity on the surface of the earth, having radius \(R\), the height at which the acceleration due to gravity reduces to \(\mathrm{g} / 2\) is

1 \(R / 2\)
2 \(\sqrt{2} R\)
3 \(\frac{R}{\sqrt{2}}\)
4 \((\sqrt{2}-1) R\)
Gravitation

270635 The difference in the value of ' \(g\) ' at poles and at a place of latitude \(45^{\circ}\) is

1 \(R \omega^{2}\)
2 \(\frac{R \omega^{2}}{2}\)
3 \(\frac{R \omega^{2}}{4}\)
4 \(\frac{R \omega^{2}}{3}\)
Gravitation

270552 A particle hanging from a massless spring stretches it by \(2 \mathbf{~ c m}\) at earth's surface. How much will the same particle stretch the spring at a height of \(2624 \mathrm{Km}\) from the surface of the earth? (Radius of earth \(=6400 \mathrm{Km})\)

1 \(1 \mathrm{~cm}\)
2 \(2 \mathrm{~cm}\)
3 \(3 \mathrm{~cm}\)
4 \(4 \mathrm{~cm}\)
Gravitation

270553 The value of acceleration due to gravity ' \(g\) ' on the surface of a planet with radius double that of earth and same mean density as that of the earth is \(\left(g_{e}=\right.\) acceleration due to gravity on the surface of earth)

1 \(g_{p}=2 g_{e}\)
2 \(g_{p}=g_{e} / 2\)
3 \(.g_{p}=g_{e} / 4\)
4 \( g_{p}=4 g_{e}\)
Gravitation

270554 If \(\mathbf{g}\) is acceleration due to gravity on the surface of the earth, having radius \(R\), the height at which the acceleration due to gravity reduces to \(\mathrm{g} / 2\) is

1 \(R / 2\)
2 \(\sqrt{2} R\)
3 \(\frac{R}{\sqrt{2}}\)
4 \((\sqrt{2}-1) R\)
Gravitation

270635 The difference in the value of ' \(g\) ' at poles and at a place of latitude \(45^{\circ}\) is

1 \(R \omega^{2}\)
2 \(\frac{R \omega^{2}}{2}\)
3 \(\frac{R \omega^{2}}{4}\)
4 \(\frac{R \omega^{2}}{3}\)
Gravitation

270552 A particle hanging from a massless spring stretches it by \(2 \mathbf{~ c m}\) at earth's surface. How much will the same particle stretch the spring at a height of \(2624 \mathrm{Km}\) from the surface of the earth? (Radius of earth \(=6400 \mathrm{Km})\)

1 \(1 \mathrm{~cm}\)
2 \(2 \mathrm{~cm}\)
3 \(3 \mathrm{~cm}\)
4 \(4 \mathrm{~cm}\)
Gravitation

270553 The value of acceleration due to gravity ' \(g\) ' on the surface of a planet with radius double that of earth and same mean density as that of the earth is \(\left(g_{e}=\right.\) acceleration due to gravity on the surface of earth)

1 \(g_{p}=2 g_{e}\)
2 \(g_{p}=g_{e} / 2\)
3 \(.g_{p}=g_{e} / 4\)
4 \( g_{p}=4 g_{e}\)
Gravitation

270554 If \(\mathbf{g}\) is acceleration due to gravity on the surface of the earth, having radius \(R\), the height at which the acceleration due to gravity reduces to \(\mathrm{g} / 2\) is

1 \(R / 2\)
2 \(\sqrt{2} R\)
3 \(\frac{R}{\sqrt{2}}\)
4 \((\sqrt{2}-1) R\)
Gravitation

270635 The difference in the value of ' \(g\) ' at poles and at a place of latitude \(45^{\circ}\) is

1 \(R \omega^{2}\)
2 \(\frac{R \omega^{2}}{2}\)
3 \(\frac{R \omega^{2}}{4}\)
4 \(\frac{R \omega^{2}}{3}\)
Gravitation

270552 A particle hanging from a massless spring stretches it by \(2 \mathbf{~ c m}\) at earth's surface. How much will the same particle stretch the spring at a height of \(2624 \mathrm{Km}\) from the surface of the earth? (Radius of earth \(=6400 \mathrm{Km})\)

1 \(1 \mathrm{~cm}\)
2 \(2 \mathrm{~cm}\)
3 \(3 \mathrm{~cm}\)
4 \(4 \mathrm{~cm}\)
Gravitation

270553 The value of acceleration due to gravity ' \(g\) ' on the surface of a planet with radius double that of earth and same mean density as that of the earth is \(\left(g_{e}=\right.\) acceleration due to gravity on the surface of earth)

1 \(g_{p}=2 g_{e}\)
2 \(g_{p}=g_{e} / 2\)
3 \(.g_{p}=g_{e} / 4\)
4 \( g_{p}=4 g_{e}\)
Gravitation

270554 If \(\mathbf{g}\) is acceleration due to gravity on the surface of the earth, having radius \(R\), the height at which the acceleration due to gravity reduces to \(\mathrm{g} / 2\) is

1 \(R / 2\)
2 \(\sqrt{2} R\)
3 \(\frac{R}{\sqrt{2}}\)
4 \((\sqrt{2}-1) R\)
Gravitation

270635 The difference in the value of ' \(g\) ' at poles and at a place of latitude \(45^{\circ}\) is

1 \(R \omega^{2}\)
2 \(\frac{R \omega^{2}}{2}\)
3 \(\frac{R \omega^{2}}{4}\)
4 \(\frac{R \omega^{2}}{3}\)