In 1948, Ralph
Alpher and Robert Herman (both in George Gamow’s team) came to the conclusion
that if the universe had come out of a Big Bang and had expanded since that
point in time, there should exist a cosmic background radiation in
the frequency of microwaves (or what means the same, at a temperature of about
5K, 5 degrees above absolute zero). Alpher and Gamow had published that same
year another prediction about the average composition of the cosmos, starting
from the Big Bang theory.
In 1964, Arno
Penzias and Robert Wilson were working with a newly built very powerful radio
telescope and detected a background noise that could not be eliminated. First
they thought that it would be of terrestrial origin, but once all the possible
sources of noise had been taken into account, the effect persisted. Then they
came to the conclusion that such noise could not come from the solar system or
from our galaxy (for in that case it would be more intense in one direction
than in another), and that its origin had to be cosmic. The
temperature of that radiation (that is, its frequency, considering the Wien
equation) turned out to be about 3K. Robert Burke of MIT
suggested to Penzias that such noise could be the cosmic background radiation
predicted by Alpher and Herman. This was in fact confirmed. For their
discovery, Penzias and Wilson received the Nobel Prize in 1978.
Along with the
argument based on the average composition of the universe, the cosmic background
radiation gave the accolade to the Big Bang theory, which became the
standard cosmological theory (although see an
earlier article on this blog).