The cosmic triangle is introduced as a way of representing the past, presen
t, and future status of the universe. Our current location within the cosmi
c triangle is determined by the answers to three questions: How much matter
is in the universe? Is the expansion rate stowing down or speeding up? And
, is the universe flat? A review of recent observations suggests a universe
that is lightweight (matter density about one-third the critical value), i
s accelerating, and is flat. The acceleration implies the existence of cosm
ic dark energy that overcomes the gravitational self-attraction of matter a
nd causes the expansion to speed up.