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The True Speed of Light
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Learn About the True Speed of Light and How It's Used
By John
P. Millis, Ph.D
Light moves through the universe at the fastest
speed astronomers can measure.
In fact, the speed of light is a cosmic speed
limit, and nothing is known to move faster.
How fast does light move? This limit can be
measured and it also helps define our understanding of the universe's size and
age.
What Is Light: Wave or Particle?
Light travels fast, at a velocity of 299, 792,
458 meters per second. How can it do this?
To understand that, it's helpful to know what
light actually is and that's largely a 20th-century discovery.
The nature of light was a great mystery for
centuries. Scientists had trouble grasping the concept of its wave and particle
nature.
If it was a wave what did it propagate through?
Why did it appear to travel at the same speed in all directions?
And, what can the speed of light tell us about
the cosmos?
It wasn't until Albert Einstein described his
theory of special relativity in 1905 it all came into focus.
Einstein argued that space and time were
relative and that the speed of light was the constant that connected the two.
What Is the Speed of Light?
It is often stated that the speed of light is
constant and that nothing can travel faster than the speed of light.
This isn't entirely accurate. The value of
299,792,458 meters per second (186,282 miles per second) is the speed of light
in a vacuum.
However, light actually slows down as it passes
through different media. For instance, when it moves through glass, it slows
down to about two-thirds of its speed in a vacuum.
Even in air, which is nearly a vacuum, light
slows down slightly.
As it moves through space, it encounters clouds
of gas and dust, as well as gravitational fields, and those can change the
speed a tiny bit. The clouds of gas and dust also absorb some of the light as
it passes through.
This phenomenon has to do with the nature of
light, which is an electromagnetic wave.
As it propagates through a material its electric
and magnetic fields "disturb" the charged particles that it comes in
contact with.
These disturbances then cause the particles to
radiate light at the same frequency, but with a phase shift.
The sum of all these waves produced by the
"disturbances" will lead to an electromagnetic wave with the same
frequency as the original light, but with a shorter wavelength and, hence a
slower speed.
Interesting, as fast as light moves, its path
can be bent as it passes by regions in space with intense gravitational fields.
This is fairly easily seen in galaxy clusters,
which contain a lot of matter (including dark matter), which warps the path of
light from more distant objects, such as quasars.
Lightspeed and Gravitational Waves
Current theories of physics predict that
gravitational waves also travel at the speed of light, but this is still being
confirmed as scientists study the phenomenon of gravitational waves from colliding
black holes and neutron stars.
Otherwise, there are no other objects that
travel that fast. Theoretically, they can get close to the speed of light, but
not faster.
One exception to this may be space-time itself.
It appears that distant galaxies are moving away from us faster than the speed
of light.
This is a "problem" that scientists
are still trying to understand.
However, one interesting consequence of this is
that a travel system based on the idea of a warp drive.
In such a technology, a spacecraft is at rest
relative to space and it's actually space that moves, like a surfer riding a
wave on the ocean.
Theoretically, this might allow for superluminal
travel. Of course, there are other practical and technological limitations that
stand in the way, but it's an interesting science-fiction idea that is getting
some scientific interest.
Travel Times for Light
One of the questions that
astronomers get from members of the public is: "how long would it
take light to go from object X to Object Y?"
Light gives them a very accurate way to measure
the size of the universe by defining distances. Here are a few of the common
ones distance measurements:
The Earth to the Moon: 1.255 seconds
The Sun to Earth: 8.3 minutes
Our Sun to the next closest star: 4.24 years
Across our Milky Way galaxy: 100,000 years
To the closest spiral galaxy (Andromeda): 2.5
million years
Limit of the observable universe to Earth: 13.8
billion years
Interestingly, there are objects that are beyond
our ability to see simply because the universe IS expanding, and some are
"over the horizon" beyond which we cannot see.
They will never come into our view, no matter
how fast their light travels. This is one of the fascinating effects of living
in an expanding universe.
Edited
by Carolyn Collins Petersen
John
P. Millis, Ph.D
Introduction
Chairman, Department
of Physical Sciences and Engineering at Anderson University
Associate
Professor of Physics
Ph.D.
in Physics and Astronomy at Purdue University
Conducts
astronomical research at the VERITAS observatory
Experience
John
Millis, Ph.D., is a former writer for ThoughtCo, where he contributed articles
on space and astronomy for three years. He has taught physics and astronomy at
the collegiate level since 2001 and is currently the chair of the Department of
Physical Sciences and Engineering at Anderson University in Indiana. He teaches
a wide variety of courses while maintaining an active research program in high
energy astrophysics.
John's
research focus is on pulsars, pulsar wind nebulae, and supernova remnants.
Using the VERITAS gamma-ray observatory in southern Arizona, he studies the
very high energy radiation from these dynamic sources to extract information
about their formation and emission mechanisms. In 2010, he co-founded a small
consulting business, Aurum Consulting, LLC, assisting with biological testing,
chemical formulations, and product development.
Education
Dr.
John Millis received a Bachelor of Science in physics, with a mathematics minor
from Purdue University. He remained at Purdue for the completion of his Doctor
of Philosophy degree, where he focused on High Energy Astrophysics.
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