# What is the gravitational force felt on Earth from the other planets in our solar system?

How much gravitational force is felt on earth from the other planets in the solar system? The sun exerts the strongest g-force, holding us in it's orbit, followed by the moon which affects the tides on earth, but how much force do we feel from Jupiter, Saturn, Venus, etc?

• Well, one could use $GM/r^2$, where $GM$ is the standard gravitational parameter and $r$ is some typical distance. So the question is basically equivalent to asking for a typical distance between Earth and the body in question. For Earth-Sun or Earth-Moon, it's sensible to use the semi-major axis of the relevant orbit, but... how do you want to measure the rest? It's essentially easy to get a rough figure, but potentially hard if you want some spatial or temporal average, etc. – Stan Liou Dec 30 '15 at 3:58
• I know I can calculate with the mass of the planet and the distance from it, i was just hoping these are well known figures i could find on the internet, without having to calculate all of them myself. It is a simple calculation though, I will if I have to, just trying to save myself some time. though i probably could have done it by now myself :) – Marcus Quinn Rodriguez Tenes Dec 30 '15 at 5:00
• @MarcusQuinnRodriguezTenes : Please post your results if you decide to do the calculations yourself. I think I might be a little lazy... :p – Nico Dec 30 '15 at 8:07
• @MarcusQuinnRodriguezTenes Remember that all planets form a corotational system together with the sun, so the distances between two planets - or a planet and a point of observation on Earth - is not constant. Henceforth, the values you calculate with and get for the gravity change with time, but you can fairly easily create a program to compute the exact values at a given time, as the "exact" positions of the planets with respect to time can be found on various freely available databases :) – V-J Jan 2 '16 at 14:24

Because of the inverse square law for Newtonian gravity we have the acceleration due the gravity $g_b$ at the surface of the Earth due to a body of mass $m_b$ at a distance $d_b \gg r_e$ (where $r_e\approx 6371 \mbox{km}$ denotes the radius of the Earth, note all distances will need be in $\mbox{km}$ in what follows) is: $$g_b=g\times \frac{m_b}{m_e}\times \left(\frac{r_e}{d_b}\right)^2$$ where $g$ is the usual accelleration due to gravity (from the Earth at the Earth's surface $\approx 10 \mbox{m/s}^2$, and $m_e\approx 6.0 \times 10^{24} \mbox{kg}$. We get the maximum acceleration due to a body when that body is at its closest to the Earth, which is what we do from now on (except for the Sun and Moon where the mean distance is used).
Now for the Moon $r_b\approx 0.384 \times 10^6 \mbox{km}$, and $m_b\approx 7.3 \times 10^{22} \mbox{kg}$, so the accelleration at the Earth's surface due to the Moon $g_b\approx 3.3 \times 10^{-5} \mbox{m/s}^2$
Then putting this relation and Solar-System data into a spread sheet we get: • No, look at the exponents the Moon has a "g" of $\approx 6\times 10^{-3} \mbox{ m/s}^2$ and Mars has a "g" of $\approx 7\times 10^{-9} \mbox{ m/s}^2$, that is about six orders of magnitude lower. – Conrad Turner Dec 31 '15 at 8:26