The universe was expected to be decelerating because of the gravitational force applied by its own mass. But in 1998, from the observation of a distant type Ia supernova we came to know that the universe is speeding up its expansion. Type Ia supernovae are identified as the end result of a carbon-oxygen white dwarf star which, as the victim of generosity by its binary companion, grows in mass until it reaches the Chandrasekhar limit (If a white dwarf exceeds 1.4 solar masses, it can't support itself by electron degeneracy pressure. A white dwarf that exceeds this mass must continue its collapse until a new source of pressure, neutron degeneracy pressure, is able to stop the collapse.) At this critical mass, the white dwarf is engulfed by a runaway thermonuclear explosion, which reaches a peak luminosity of about 4 billion times the Sun’s. These supernovae are so bright they can be seen with the Hubble Space Telescope 75% of the way across the Universe and used by astronomers as "standard candles."
Astronomers can measure the distance of supernova and they also know that when it occurred. Though our universe is expanding,so light from the supernova is redshifted. The degree of this `redshift’ provides a direct measure of the change in the size scale of the Universe during the journey of the light.