The Mass of an object, in astronomy and Newtonian physics, concerns how much matter an astronomical body is made up of. The mass of an object can be characterised by its ability to resist a given force (we sometimes call this a body’s inertial mass and thus mass is intimately associated with the concept of inertia). This is a simple consequence of Newton’s second law where the force F, on a body is equal to the mass m, times the acceleration a, it experiences, ie:

F=ma or m=F/a

In deep space, away from the gravitational field of Earth (or another large body), an object will be “weightless” – however, it will still have mass, and thus a resistance to a given force.

Masses are often expressed in the units kilograms (kg), grams (g) or solar masses (M⊙). A body is more massive than another when it has a greater mass. One of the least massive objects in the Universe is the electron, which has a mass of just 9.11 × 10-31 kg whilst the Sun has a mass of 1.989 × 1030 kg, and galaxies like the Milky Way have masses in excess of 1042 kg.

Newton’s universal law of gravitation states that all masses in the Universe are attracted to each other.

In special relativity there is an equivalence between mass m, and energy E, given by the famous equation E= mc2 where c is the speed of light. Thus all particles and even light have a mass associated with them.

In Einstein’s special theory of relativity the mass of a body changes when it has a velocity v, with respect to an observer. If the rest mass is m0, then the mass m, of a body becomes: