SNAP (SuperNova/ Acceleration Probe) is a
satellite experiment designed to verify the remarkable cosmological
discovery that the Universal expansion is accelerating, and to
determine the nature and evolution of the “dark energy”
driving this acceleration. Recent measurements carried out by
the Supernova Cosmology Project (SCP) and the High-Z Supernova team
have made the startling discovery that the expansion of the universe
is accelerating. The SNAP mission is expected to provide
an understanding of the mechanism driving the acceleration of the
universe. The satellite observatory will be capable of measuring up
to 2,000 distant supernovae each year of the three year mission
lifetime. These measurements will map out in detail the expansion rate
of the universe at epochs varying from the present to 10 billion years
in the past. SNAP will determine the spatial curvature of the
universe, thus providing a fundamental test of the theory of inflation
- the theoretical mechanism that drove the initial formation of the
universe. Like its ground-based predecessors, SNAP uses type Ia
supernovae as astronomical standard candles to provide a distance
scale, which, combined with the redshift obtained from the spectral
lines from the supernova and its host galaxy determine the
cosmological parameters and ultimately the nature of the "missing
energy" in the universe.