59. Gravitational Time Dilation on Earti. For a relatively weakgravitational field, such as that of a ptanet or an ordinarystar, the following formula tells us the iractional amount ofgravitational time dilation at a distanes r from the center ofan object of mass Mobject-GMobject(G = 6.67 × 10-ll m³/(kg × s²); c = 3 × 10° m/s.]example, while 1 hour passes in deep space far from theobject, the amount of time that passes at a distance r is1 hour multiplied by the factor above. (This formula doesnot apply to strong gravitational fields, like those near blackholes.) Calculate the amount of time that passes on Earth'ssurface while 1 hour passes in deep space.60/Gravitational Time Dilation on the Sun. Use the formulagiven in Problem 59 to calculate the percentage by whichtime runs slower on the surface of the Sun than in deepspace. Based on your answer, approximately how much ofa gravitational redshift should you expect for a spectral linewith a rest wavelength of 121.6 nm?For

Let the mass of the sun M =2×1030kg G =6.67×10-11m3kg-1s2-1 radius of the sun R=6.95×108m and the…

Answered: 60/ Gravitational Time Dilation on the…

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