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Digital Universe Guide - Hayden Planetarium

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3.2. MILKY WAY ATLAS TUTORIAL 53<br />

stars and turn the boxes on, a box will appear around the bright blue stars. Press the Box Toggle<br />

Button to turn the boxes off.<br />

Red Stars Are Cooler Stars Now let’s see the redder stars by typing<br />

see red<br />

The red stars are more numerous (more than 80% of the stars) and are distributed in a spherical shape.<br />

Of course, because these are observed from Earth, the distribution is centered on the Sun, but one can<br />

imagine the entire Galaxy filled with these dim stars.<br />

Red stars are cooler stars that form throughout the Galaxy. They burn their fuel slowly and have long<br />

lifespans; some stars are as old as the Galaxy. The Sun is among these red stars, a relatively cool star<br />

with a (B − V ) = 0.65. It has been burning its fuel for about 5 billion years and has about another<br />

5 billion to go before entering the end stages toward a red giant and a white dwarf star.<br />

Stellar Color Traces Galactic Structure These two contrasting views tell us about the structure of<br />

the stars in our Galaxy. The red stars are typically known as Population II stars and revolve around the<br />

center of the Galaxy in elliptical, sometimes highly inclined orbits. Bluer stars are referred to as<br />

Population I stars and lie in the Galactic disk, orbiting in orderly paths around the Galactic center. While<br />

we plot only the stars we have accurate distances for, you can imagine the disk (turn on the Milky Way<br />

image using the galaxy button) filled with blue stars with many red stars as well. Also imagine a<br />

spherical distribution around the entire Galaxy filled with cool, red stars. This is called the Galactic Halo<br />

(halo button), and we’ll talk about it soon.

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