Quick relativity lowdown
Well, the theory of relativity was a new physics idea
developed in the early 1900's by Albert Einstein, radically
generalizing ideas from electromagnetism at the
time (e.g. invariance of Maxwell's equations in
different reference frames). It says that the old
laws of kinematics and dynamics - motion and
forces - by Newton and Kepler and all those guys who we
learn about in school are in fact only
approximations to what really happens. The
equations we learned early on, like "distance
equals speed multiplied by time", work just fine
for daily life things like cars and airplanes and
bowling balls, and are still important for those
describing things. But when we deal with objects
that move at close to the speed of light, or that
are near large gravity fields, our traditional
equations and experiences are way off, time and
space don't act like you would expect, and we need
to use more complicated equations to describe the
motion.
In this diagram we can see how the curved blue line
is approximated pretty well by the straight red line
for about half the graph. In the same way, the
traditional physics of Newton only approximate what's
predicted by the theory of relativity at slower
speeds.
An example of this strange relativity behavior is on
the GPS satellites which orbit the Earth and allow
our handheld GPS receivers to find our location. You
may have seen these gadgets in cars and boats. The
GPS satellites carry very fast-ticking, very accurate
clocks on board, and radio their times down to us on
the ground as part of the location-finding process.
Now it may sound weird since we don't see it in daily
life, but relativity effects actually cause time to
flow differently when you move at a high speed or are
in the presence of a large gravitational field. Those
effects in fact happen to us all the time on the
Earth here but they're so small that we don't notice
them since we walk and drive around pretty slowly,
and Earth's gravitational field is strong but not
ultra-strong. And yet, it turns out these GPS
satellites move fast enough in their orbits, and
their clocks are so accurate and work on such a fine
scale, that we actually do notice these small
relativity effects in their clocks. One finds that
time itself goes a tiny bit slower on board the
moving satellite than it goes for us on the ground,
and this causes the onboard clock to disagree with
the clocks on the ground. So we actually have to
change our calculations to compensate for that or
else the calculated location on the surface of the
Earth is off. There's nothing wrong with the clocks,
it's just they are so accurate that they can measure
effects we don't generally notice in our daily lives.
Now if we start using our imaginations a bit, and
think of spaceships people might use in the future to
travel to distant stars, the effects predicted by
this theory of relativity get even stranger. To get
to a star 5 lightyears away in your lifetime, you
would have to move much faster than the GPS
satellite, say at 99% the speed of light. At this
faster speed, the time effect is much more noticable.
If an astronaut were to hop in one of these
spaceships and fly at 99% the speed of light for 5
years, when she returned home at the end of that time
she'd find that over 35 years have passed for the
people she left back on Earth! For her it seemed like
time flowed normally, and for the people on Earth it
seemed like time flowed normally, but different
amounts of time passed for each. This happens to you
on a tiny scale in daily life too, but the speeds we
go in cars and planes are much too slow to notice the
time difference. We can, however, measure the effect
in cases like the GPS satellite mentioned above.
The theory of relativity also tells us that time
flows differently in strong gravitational fields too,
like those very close to a star. We've measured this
by watching the light from distant stars bend a
little around our Sun. When we filter out the Sun's
glare, we find the stars in the background are in
slightly different places than when the Sun is not
front of them. We've also noticed this gravity effect
by looking at the orbit of the planet Mercury, the
closest planet to our Sun. When measured very
carefully, Mercury's orbit doesn't go exactly where
Kepler's equations say it should go; instead it goes
where the theory of relativity's equations say it
should go.
In both the speed and the gravity examples described
above, I haven't explained why we see those
effects. That's where relativity gets a little more
complicated, but it's really pretty easy to follow
(until you hit the math of general relativity!). Let
us for now say that distance, time, speed, and
gravity are all far more intimately connected
together scientists before Einstein thought, and this
intimate connection causes strange effects like those
I described above to become noticeable when the speed
or gravity become large. Here are a few resources
explaining where these effects come from: One
starting place is Einstein's own 1905 special
relativity paper, "On the Electrodynamics of Moving
Bodies" (in html or pdf), which is amazingly
understandable and describes everything in terms
of moving clocks and rods. (This is a scientific
paper and so does have some math in it, but
overall is much more readable by the layperson
than many scientific papers.) There are also nice
technical writeups at Wikipedia on special relativity and general relativity, and a very well
done website on the subject for the layperson
here. Finally, there's a fabulous
podcast by PBS Nova with various
famous physicists describing the significance of
E=mc2, really enjoyable by scientists
and laypeople alike. (I didn't mention it above,
but E=mc2 is a direct consequence of
special relativity - maybe I should come back and
fill in some of that...).