Newton first defined these laws in Philosophiae Naturalis Principia Mathematica (1687) and, using his newly developed calculus, proved many results concerning "idealised" particles. In the third volume (of the text), he showed how, combined with his Law of Universal Gravitation, the laws of motion would explain Kepler's laws of planetary motion. Newton's laws were modified, in 1916, by Einstein's theory of relativity.
This means that a stationary object will remain stationary, and a moving object will continue to move (forever and in the same manner), unless a force acts upon it. In everyday life, the force of friction usually acts upon moving objects. Newton's law indicates that some force (gravity) must be acting upon the planets, as they do not travel in a straight line.
This is expressed by the equation:
This expresses that the more force an object receives, the greater its acceleration will be; and that, the less mass an object has, the less force will be needed, to accelerate it; the more mass an object has, the more force will be required, to accelerate it. For example, the force of a nuclear explosion will acclerate a kitten more than a water buffalo; because, the kitten has less mass. This law is associated with the conservation of angular momentum.
If you strike an object with a force of 200 N, then the object also strikes you (with a force of 200 N). Not only does a bullet exert force upon a target; but, the target exerts equal force upon the bullet. Not only do planets accelerate toward stars; but, stars acclerate toward planets. The reaction force has the same line of action, and is of the same type and magnitude as the original force.