In 1929, Edwin Hubble discovered that galaxies are receding more quickly they are distant. Our universe is expanding, what is the Hubble constant (H = 70 km / s / Mpc), which gives this speed depending on the distance at which it is observed (speed = H x distance). This is not an extraordinary expansion because it gives only an increase of the distance of 7% per billion years. Since several methods of observation have corroborated the hypothesis of the accelerating expansion of the universe (standard candles, standard rules,...).
A supernova is a gravitational collapse of stars with a mass greater than 8 solar masses. These events are rare in a galaxy (1 per century), but when the star explodes it is as bright as the galaxy itself. In addition they are true standard candles because they shine up to 400 days after explosion with a perceived brightness which allows us to determine the distance and speed of the galaxies. Thus identifying extremely distant galaxies and in particular those that host cosmic standard candles we can study the evolution of the universe in the past.
The method of standard candles confirms the accelerating expansion of the universe and thus the existence of a new component called dark energy. The Universe is incredibly "empty" of matter, there is one atom per cubic meter. It is composed of 4% baryonic matter, 23% cold dark matter and non-baryonic and 73% black or dark energy.
NB: to search supernovae, we photograph a region of galaxies and a month later we take again a picture, then by treating the two images, the bright objects are subtracted to identify the supernova present in the second picture. This search is performed with larger telescopes Planets (Gemini, CFHT, VLT).