The kinetic energy of the earth is often estimated using the formula: K = E0 + E1, where E0 is the energy of the sun, and E1 is the kinetic energy of the earth. But there are other ways to estimate the kinetic energy. This one is especially common for a scientist or mathematician to do, since they often have a better grasp on the concepts involved than many laymen do.

In this book we’ve just started to take a look at what’s going on in Earth’s atmosphere. The main thrust of this book is to show you how Earth’s atmosphere can be used to estimate the kinetic energy of the earth.

So let’s do this. First let’s look at the kinetic energy of the earth.

We know that energy is conserved. If we have a small mass of something, like a rock, and we let this mass move at a certain speed, then the kinetic energy is conserved. However, this is not true in general for a large mass like the earth. The bigger the mass, the greater the centrifugal force that must be overcome to move the mass at a certain speed. To overcome this, the kinetic energy must be added to the mass, thus increasing its kinetic energy.

A lot of this is not true for the earth, but for the sun. The sun is the sum of two main forces, the gravitational force on the earth and the centrifugal force that must be overcome to move the sun at a certain speed. For example, the gravitational force may be too great to overcome, but it is not impossible for the gravitational force to be overcome to move the sun.

For the earth, we are working with the sun’s exact mass. If we assume that it is at rest, then the kinetic energy of the earth with respect to the sun will be the same as the kinetic energy of the sun with respect to the earth.

I’m going to assume that this is true for our calculation. The gravitational force on the earth may be so great that the centrifugal force cannot be overcome to cause the sun to move.

The Earth has two distinct parts: The core of the Earth and the mantle and crust. The core is the solid core of the Earth. It is a sphere about 1.5 billion tons, and contains about 99% of the Earth’s mass. This is the part of the Earth that we are interested in. The mantle is a thin layer of the Earth that lies beneath the core. It has a mass of about 9.8 billion tons, and is about 1.

The core is really the only part of the Earth that we can directly measure. There is no way to accurately measure the Earth’s crust, where the layers of rock are separated by water and other minerals. We can estimate the total mass of the Earth’s crust, but the amount of material that we can measure is very small. The amount of mass that the crust contains is probably less than a percent of the mass of the Earth.