26.1 The Sun
26.2 Stars
26.3 Life Cycle of Stars
26.4 Groups of Stars
26.5 Expanding Universe
100

The process that the sun uses to produce energy in the form of electromagnetic radiation.

Nuclear fusion.

100

The distance between stars is typically measured in this unit of distance equaling 9.5 trillion kilometers.

Light year.

100

This is the cloud of dust and gas spread out over a large region of space.

Nebula.

100

A group of Stars that form a pattern to observers on earth is called what?

A constellation.

100

This theory states that the universe came into existence during an enormous instantaneous explosion.

The Big Bang Theory

200

The primary fuel source for the majority of main sequence stars.

Hydrogen

200

Astronomers utilize this property of stellar objects to measure the distance of an object from earth.

Parallax 

200

90% of a star's lifetime is spent on this diagonal band of planets that run from the top left to the bottom right of a Hertzsprung-Russell (H-R diagram) that relates size, temperature and brightness.

Main Sequence 

200

Constellations are important as they were and can still be used for this purpose.

Navigation or Mapping

200

This stuff does not give off any heat or light, but scientists are still able to detect its existence, even if they don't know much more about it.

Dark Matter

300

The Sun and other stars are kept stable by the equilibrium of these two forces.

Thermal Pressure and gravity.

300

While many elements are believed to have originated from stars, the most common chemical composition for stars are of these elements.

Hydrogen and Helium

300
At what point does a protostar become a true main sequence star?

When nuclear fusion begins in the core of the protostar.

300

Large groupings of older stars are known as what type of star system?

Gloubular clusters.

300

What do we call the residual heat left over in the universe, often called the echo of the big bang. This residual heat is consistent throughout the universe and often used as evidence to support the big bang theory.

Cosmic Microwave Background Radiation

400

List each layer of the Sun's atmosphere.

Photosphere, Chromosphere, Corona 

400

The chemical composition of a star can be identified by using this characteristic feature of the star's light.

The star's spectrum or absorption lines.
400

What a star becomes when fusion ends in its core (the star dies), is dependent on its mass. What are the three possible end stages of Stars?

White Dwarf, Neutron Star, Black Hole

400

Associations and open clusters are similar in that they typically contain bright young stars; however, they differ because of what reason?

Associations are larger than open cluster (And are also temporary, not yet sorted out by gravity.)

400

The change in wavelength and frequency of light and sound of a moving object relative to a stationary observer is known as what?

The Doppler Effect 

500

Three common features are present on or about the sun's surface, list each one and describe how they are distinct.

Sunspots - cool areas of gas formed from convective currents
Prominence - Huge loops of heated gas erupting from the edges of sunspots and shaped by the sun's magnetic forces.
Solar Flares - Eruption near sunspots of Charged Particles and X-rays into the universe.

500

The Hertzsprung-Russell or H-R diagram is a chart displaying the relationship between these three star characteristics.

Star Color/Temperature
Star Size
Star Absolute Brightness/Luminosity

500

From the very beginning, describe a low-medium mass star at each major phase of its lifespan - identify each form the star takes from birth to death.

(Nebula), Protostar, Main Sequence, Planetary Nebula, White Dwarf, (Black Dwarf)

500

Identify each of the 4 types of galaxies we discussed in class and explain what makes them distinct from one another.

Spiral - Many stars at the center with gas and dust in pinwheel arms extending outward.
Barred Spiral - Like Spiral but with a bar through the center with arms extending out on either side.
Elliptical - Large spherical galaxy with no arms and mostly old stars.
Irregular - Many young stars with disorganized appearance.

500

This law states that the speed at which a galaxy moves away from us is proportional to its distance from us.

Hubble's Law