Astronomers have two approaches to trying to determine the age of the
Universe. They can estimate the ages of individual objects in the Univ
erse and specifically in our Galaxy. These estimates use either the ob
served properties of stars and theoretical ideas concerning stellar ev
olution or the abundances of long-lived radioactive isotopes and their
decay products. Alternatively they can use cosmological theories and
observations to try to determine the age of the entire Universe. Obvio
usly the Universe must be older than its component parts but neither o
f the above methods is sufficiently reliable that this is true of the
deduced ages. As a result, it is from time to time reported that some
object in the Universe is older than the Universe itself. In this arti
cle lye discuss the methods that are currently being used to determine
the age and we emphasize the problems in obtaining reliable results.
It is not at present possible to provide a definite value for the age
of the Universe.