359598 A star suddenly shrinks and its density becomes \(10^{9}\) times the original value. The value of acceleration due to gravity on its surface will increase by a factor of

359599 In order to simulate different values of \(g\), aspiring astronauts are put on a plane which dives in a parabola given by the equation:
\(x^{2}=500 y\)
Where \(x\) is horizontal, \(y\) is vertically upwards; both being measured of the velocity of the plane is constant throughout, and has the value of 360 \(km/h\). The effective \(g\) experienced by an astronaut on the plane equals

359600 The diameters of two planets are in the ratio \(4: 1\) and their mean densities in the ratio\({\text{1: 2}}\). The acceleration due to gravity on \(t\) he planets will be in ratio

359601 A body of supercondense material with mass twice the mass of earth but size very small compared to the size of earth starts from rest from \(h < < R\) above the earth's surface. It reaches earth in time

359598 A star suddenly shrinks and its density becomes \(10^{9}\) times the original value. The value of acceleration due to gravity on its surface will increase by a factor of

359599 In order to simulate different values of \(g\), aspiring astronauts are put on a plane which dives in a parabola given by the equation:
\(x^{2}=500 y\)
Where \(x\) is horizontal, \(y\) is vertically upwards; both being measured of the velocity of the plane is constant throughout, and has the value of 360 \(km/h\). The effective \(g\) experienced by an astronaut on the plane equals

359600 The diameters of two planets are in the ratio \(4: 1\) and their mean densities in the ratio\({\text{1: 2}}\). The acceleration due to gravity on \(t\) he planets will be in ratio

359601 A body of supercondense material with mass twice the mass of earth but size very small compared to the size of earth starts from rest from \(h < < R\) above the earth's surface. It reaches earth in time

359598 A star suddenly shrinks and its density becomes \(10^{9}\) times the original value. The value of acceleration due to gravity on its surface will increase by a factor of

359599 In order to simulate different values of \(g\), aspiring astronauts are put on a plane which dives in a parabola given by the equation:
\(x^{2}=500 y\)
Where \(x\) is horizontal, \(y\) is vertically upwards; both being measured of the velocity of the plane is constant throughout, and has the value of 360 \(km/h\). The effective \(g\) experienced by an astronaut on the plane equals

359600 The diameters of two planets are in the ratio \(4: 1\) and their mean densities in the ratio\({\text{1: 2}}\). The acceleration due to gravity on \(t\) he planets will be in ratio

359601 A body of supercondense material with mass twice the mass of earth but size very small compared to the size of earth starts from rest from \(h < < R\) above the earth's surface. It reaches earth in time

359598 A star suddenly shrinks and its density becomes \(10^{9}\) times the original value. The value of acceleration due to gravity on its surface will increase by a factor of

359599 In order to simulate different values of \(g\), aspiring astronauts are put on a plane which dives in a parabola given by the equation:
\(x^{2}=500 y\)
Where \(x\) is horizontal, \(y\) is vertically upwards; both being measured of the velocity of the plane is constant throughout, and has the value of 360 \(km/h\). The effective \(g\) experienced by an astronaut on the plane equals

359600 The diameters of two planets are in the ratio \(4: 1\) and their mean densities in the ratio\({\text{1: 2}}\). The acceleration due to gravity on \(t\) he planets will be in ratio

359601 A body of supercondense material with mass twice the mass of earth but size very small compared to the size of earth starts from rest from \(h < < R\) above the earth's surface. It reaches earth in time