|
Astronomers believe that for approximately 300,000 to just
over a billion years after the Big Bang, there was nothing in the universe but
clouds of gas that would someday coalesce to form galaxies, stars and planets.
When the first celestial objects formed, radiation appeared in the universe for
the first time. Astronomers are trying
to learn more about this time, and about the first sources of radiation in the
universe.
Sometimes, a hydrogen atom in a gas cloud will emit a low
energy radio signal. While the radio wave starts out being tiny, only 21
centimetres long, the expansion of the universe causes it to stretch to several
metres by the time it reaches earth. This means that ordinary radio receivers can
perceive it, and thus detect these primordial clouds.
The Low Frequency Array (LOFAR), which was developed by the
Netherlands Institute for Radio Astronomy (ASTRON), has been testing the
ability to detect these radio waves since 2006. ASTRON is now in the process of
constructing satellite stations across Europe.
The first was completed in November 2008 at the Max Planck Institute for
Radio Astronomy in Effelsberg, Germany.
Astronomers hope that they will find not only the gas that
filled the universe in primordial times, but also see the “bubbles” that were
blown in the universe by the radiation that was released from the first
celestial objects. These objects would have filled their corner of space with
highly energetic radiation that would have ripped apart hydrogen atoms in a
process called re-ionisation, and thus prevented them from giving off radio
waves. LOFAR should be able to detect
how the radio emissions have dwindled as radiation began to be given off.
Meanwhile, Planck, a new European Space Agency (ESA)
telescope launching this year, will detect the microwave radiation that was
released by the Big Bang. About one in every 10 million microwaves has bounced
off a free electron on its way to the Earth. These electrons were freed when
the universe’s hydrogen atoms were ripped apart by the radiation from the first
celestial objects. Planck will be sensitive enough to supply details about how
quickly the atoms were ripped apart, which will help provide a better
understanding about the first celestial objects, for example, whether they were
stars or black holes.
Herschel, another ESA telescope set to launch at the same
time as Planck, will have a primary mirror of 3.5 metres, over one and a half
times larger than Hubble’s. Astronomers hope that Herschel will detect the
first star clusters to form in the universe.
www.planetsurveyor.com
|