Please explain special relativity in simple terms, including the meaning of E=mc^2.
Special relativity is a theory of physics that explains how space and time are related when objects are moving very fast, close to the speed of light. It was developed by Albert Einstein in 1905. 

One of the main ideas of special relativity is that the speed of light is the same for everyone, no matter how fast they are moving or where they are. This means that time and distance are not fixed, but depend on the observer's point of view. For example, if you are on a spaceship traveling at half the speed of light, your clock will tick slower than someone on Earth, and your spaceship will appear shorter along the direction of motion. This is called **time dilation** and **length contraction**.

Another important idea of special relativity is that mass and energy are equivalent, and can be converted into each other. This is expressed by the famous equation E=mc^2, where E is energy, m is mass, and c is the speed of light. This equation tells us that a small amount of mass can produce a huge amount of energy, as in nuclear reactions.

Special relativity has many consequences that have been tested and confirmed by experiments, such as the relativistic Doppler effect, the relativistic mass increase, the Lorentz transformation, and the twin paradox. Special relativity also forms the basis of other theories of physics, such as quantum field theory and general relativity.
Great, thank you! Could you also explain how special relativity relates to general relativity?
Certainly! General relativity is an extension of special relativity that includes gravity. While special relativity deals with objects moving at high speeds in flat spacetime (i.e., without gravity), general relativity describes how objects move in the presence of gravity, which is caused by the curvature of spacetime.

Albert Einstein developed general relativity in 1915, about ten years after he introduced special relativity. The main idea of general relativity is that gravity is not a force between objects, as described by Newton's law of universal gravitation, but rather a curvature of spacetime caused by the presence of mass and energy. Objects move along the shortest paths (called geodesics) in this curved spacetime, which we perceive as the force of gravity.

General relativity reduces to special relativity in the absence of gravity or when dealing with objects moving at high speeds in a small region of spacetime where the curvature is negligible. In other words, special relativity can be seen as a special case of general relativity, where the effects of gravity are not considered.

General relativity has been confirmed by many experiments and observations, such as the bending of light by massive objects (gravitational lensing), the shift in the orbit of Mercury (perihelion precession), and the detection of gravitational waves. It is also the basis for our current understanding of black holes and the expansion of the universe.