V. OUR COSMIC LOCATION
Much of the agonizing that mankind has gone through has been directed
at better understanding his place in time and space. Starting from an ethnocentric
point of view that considered every tribe or civilization or religion at
the center of things, we have slowly, and often painfully, come to understand
that the universe in which we live is vastly different from anything that
we conceived in the past and that our earth, in all its beauty and majesty
is but a small part of a grand cosmos.
A. How we measure distances
One of the most awesome and incomprehensible facets of astronomy is
the distances involved. Here on the earth, we measure larger distances
in miles. But miles become small units when we begin to explore
even the solar system. The Earth has a diameter of some 8000 miles and
a circumference of some 25,000 miles. The moon is ten times as far away
as the earth's circumference. But even a quarter of a million miles pales
when compared to our distance from the sun, about 93 million miles, or
the distance between Pluto and the sun, over 3.6 billion miles from the
sun on average. So, to reduce these numbers to sizes that made sense when
navigating the solar system, astronomers evolved another more convenient
unit. The astronomical unit (AU) is defined as the mean earth sun
distance (93 million miles). Using AUs, the earth would lie 1 AU from the
sun, Pluto nearly 40 AUs.
As we look beyond the Solar system, the vast scale of the universe renders
the use of AUs cumbersome. To measure the universe, we use how far light
travels in a given amount of time. Because light travels at 186,000 miles
per second, at the end of a second it will have gone 186,000 miles. We
call this a light second. A light year (LY) would we how far light
has gone in a year, (some 6 trillion miles). We commonly use light years
for interstellar (between stars) and intergalactic (between galaxies) distances.
Astronomers also use the parsec, which is approximately three and
a quarter light years (3.26 LY). |