The Scales of the Cosmos

The vastness of the cosmos and the things that make up the cosmos are a real challenge to our minds as we begin the study of Astronomy. Below are some of the dimensions most important to us at the beginning of our course. We, out of necessity, employ Scientific Notation, when using these numbers. We do not normally use English units (inches, feet, miles, etc.; but for conversion purposes recall that 1 mile ~ 1.6 km and 1 km ~ 0.6 mile).

Starting from the "small" to the truly enormous, the dimensions of the following are interesting to contemplate. Items in red are important terms in the first unit. The important definitions you must memorize. In the following table, the first column lists the dimension, the second column its distance/size in the appropriate unit, and the third column is that dimension in terms of our Thousand Yard Walk.
 

Dimension Measure Thousand Yard Walk
The diameter of the earth ~12,700 km = 1.27 x 10 4 km 0.08 inch
The average distance to the moon ~ 384,000 km = 3.84 x 10 5 km 2.5 inches
The diameter of the sun ~ 1,400,000 km =1.4 x 10 6 km 8.6 inches
The average distance of  the sun ~ 1.49 x 10 8 km = 1 astronomical unit (au)(important definition!) 77.5 feet
The average distance to Pluto  ~ 5.8 x 10 9 km = 39 au 3022.5 feet ~ 3/5 mile
A light year (the distance light travels in one year at a speed of 300,000 km/sec) (important definition!) ~ 9.46 x 10 12 km (about 5.9 trillion miles)  931 miles
The distance to the nearest star (Proxima Centauri) ~ 4.2 ly 3,900 miles
Center of our galaxy ~ 25,000 ly 23,000,000 miles
Our galaxy (the Milky Way) ~ 80,000 ly 75,000,000 miles (comparable to the actual orbit of Venus)
Nearest big galaxy (M31 in Andromeda) ~ 2.6 million ly 2.4 billion miles (from here to Neptune)
Nearest big galaxy cluster (Virgo)  ~ 50 million ly ~ 50 billion miles (16 times farther than Pluto)
Nearest quasars  ~ 1 billion ly ~ 2 ly
Edge of the observable universe ~ 14 billion ly ~ 28 ly (about as far as Vega)

The Units we will use in Astronomy:
 
Name (with abreviation) Equivalent Typical Phenomenon
1 angstrom  (Å) 1 x 10-10 m Size of an atom
1 nanometer (nm) 10 Å = 1 x 10-9 m One wave of X-radiation
1 meter (m) 1000 mm or 0.001 km
Moderate sized meteoroid
1 kilometer (km) 1000 or 1 x 10³ m Small asteroid
1 astronomical unit (au) 1.49 x 10 8 km Earth-sun distance; diameter of a red giant star
1 light-year (ly) 9.46 x 10 12  km Extent of the solar system (including the Oort Cloud)
1 parsec (pc) 3.26 ly Distance between "neighboring" stars
1 kiloparsec (kpc) 1000 pc = 32,600 ly Giant molecular cloud (star forming region of a galaxy)
1 megaparsec (Mpc)  1 million parsecs Distance between "neighboring" galaxies

Our study of astronomy takes us from the very smallest particles in the universe (electrons that are involved in the creation of the light we see) the the very largest known structures in the universe (filaments that are vast chains of galaxy clusters).

Of interest might be the description of our Cosmic Address (apologies to Thornton Wilder who wrote "Our Town").
 

Our Cosmic Address
This figure illustrates our cosmic address. The Earth is one of the nine planets in our solar systems, our solar system is one among more than 100 billion star systems in the Milky Way Galaxy; the Milky Way is one of the largest of about 30 galaxies in the Local Group; the Local Group lies near the outskirts of the Local Supercluster; and the local Supercluster fades into the background of structure throughout the universe. Wilder adds, "...the Universe, the Mind of God." 

Concept and image credit: Aeree & Ben's Astronomy Lab of Columbia University
http://www.astro.columbia.edu/~archung/labs/fall2001/lec01_fall01.html. Used with permission of the author.