Answer:
ar = 5.86*10^-3 m/s^2
Step-by-step explanation:
In order to calculate the radial acceleration of the Earth, you first take into account the linear speed of the Earth in its orbit.
You use the following formula:
(1)
G: Cavendish's constant = 6.67*10^-11 m^3 kg^-1 s^-2
Ms: Sun's mass = 1.98*10^30 kg
r: distance between Sun ad Earth = 1.50*10^8 km = 1.50*10^11 m
Furthermore, you take into account that the radial acceleration is given by:
(2)
You replace the equation (1) into the equation (2) and replace the values of all parameters:
![a_r=(1)/(r)(GM_s)/(r)=(GM_s)/(r^2)\\\\a_r=((6.67*10^(-11)m^3kg^(-1)s^(-2))(1.98*10^(30)kg))/((1.50*10^(11)m)^2)\\\\a_r=5.86*10^(-3)(m)/(s^2)](https://img.qammunity.org/2021/formulas/physics/college/km9domoeec19ykx18ff71lotsv7lc2t75r.png)
The radial acceleration of the Earth, towards the sun is 5.86*10^-3 m/s^2