How Old Is the Universe?
You can tell how old a fallen tree was when it died by counting the rings in its trunk. No one was around when the Universe was born, but there are tricks to determining how old it is too.
We get an idea about how old objects are in the Universe when we see their light. The speed of light is constant, and distance is a measure of time. When we see a distant star explosion that occurs billions of light years
away, we know that that star exploded billions of years ago. Likewise, seeing
the light from the very first stars or seeing the afterglow of the Big Bang will tell us when these events occurred.
Determining distances and thus age can be tricky business. We have one
constant, the speed of light, which is about 300,000 kilometers a second.
We have another ruler called redshift.
Objects moving away from us emit light that is "redshifted," meaning its wavelengths
are shifted from higher energy to lower energy. A star that is really blue
might look red if it is moving away from us fast enough, for the higher-energy
blue wavelengths have shifted to lower-energy red wavelengths.
In the Universe, everything outside of our local group of galaxies
is moving away. Imagine the Universe as a rising loaf of raisin bread, in
which the raisins represent the galaxies. As the loaf rises, other galaxies
move away from our galaxy. The more distant the galaxy, the faster it is
moving away. And the faster something recedes, the greater the redshift
in the light it emits.
Yet the fact that distant objects have greater redshift is merely relative,
though. There is no firm number or constant that allows us to say that a
redshift of "x" quantity equals a distance of "y" kilometers. Scientists
make educated guesses on the relationship between redshift and distant.
MAP plans to eliminate the guesswork by determining this connection. Then,
when we see an object of known redshift, we can determine exactly how far
it is and (because we know the speed of light) figure out a minimum age for
The redshift-distance connection depends on the mass content of the Universe and the cosmological constant,
or dark energy. MAP will determine both of these parameters. The speed
of light is constant in a vacuum, but it varies as it penetrates the dust
and gas of space. Knowing how much mass is out there, then, will lead to
a value for the speed of light in this medium. Dark energy acts to accelerate
the expansion of the Universe. The greater the force of dark energy, the
faster the acceleration and thus the greater the distance traveled by receding
galaxies. So knowing the contribution of dark energy, termed the cosmological
constant, places another limit on the redshift-distance connection.
Once we have a firm redshift ruler, we can measure the distance and age
of all types of objects with greater accuracy. First on the agenda: the
background. This microwave light as a redshift. The redshift yields the
distance. The distance (knowing the speed of light) yields the age. So
we can determine the age of the Universe by dating its first light, which
broke free 400,000 years after that initial spark called the Big Bang.
Scientists think the Universe is about 10 to 15 billions years old. Expect MAP to determine a much more precise age.