Time Traveling With Spitzer
Written by Nancy Atkinson
While time
travel is
seemingly
impossible, we
can actually look back
in time with our
telescopes to
learn about the
conditions of
our universe in
times past. The
Spitzer Space
Telescope has
found some very
dim and distant
galaxies located
at the edge of
our universe
that have never
been seen
before.
Approximately
12.5 billion
light-years away
from Earth,
we’re seeing
these galaxies
as when our
universe was
just one billion
years old. With
Spitzer's
infrared
capability,
astronomers have
been able to
take infrared
portraits and
even "weigh"
many of these
early galaxies.
"Understanding
the mass and
chemical makeup
of the
universe's first
galaxies and
then taking
snapshots of
galaxies at
different ages,
gives us a
better idea of
how gas, dust
and metals– the
material that
went into making
our Sun, solar
system, and
Earth –has
changed
throughout the
Universe's
history," said
Spitzer
scientist Dr.
Ranga Ram Chary.
Unlike the
galaxies of
today, Chary
says that
galaxies living
in the one
billion year old
universe were
much more
pristine. They
were comprised
primarily of
hydrogen and
helium gas and
contained less
than 10% of the
heavier elements
we see in the
local Universe
today, and even
on Earth.
Astronomers have
found these
distant galaxies
were cosmic
"lightweights",
or not very
massive compared
to mature
galaxies we see
nearby.
"A few billion years after the big bang, 90 percent of the stars being born were occurring in these types of faint galaxies. By identifying this population, we hope to gain insights into the environments where the universe's first stars formed," said Chary.
To find these faint galaxies, astronomers followed the lingering afterglow of gamma ray bursts back to their sources. Astronomers believe gamma ray bursts appear when a very massive star dies and becomes a black hole.
The afterglow occurs when energetic electrons spiral around magnetic fields, and release light. In its explosive death, material shooting out of the massive star smashes into surrounding gas. This violent collision heats nearby gas and energizes its electrons.
Once coordinates of the faint galaxies were determined, Chary's team then used Spitzer's supersensitive infrared array camera to snap a picture of the faint galaxy. The amount of light from the galaxies allowed Chary to find the mass of the galaxies.