Observing Matter & Space
Stars
The Universe
Evidence for the Big Bang
More on Stars!
100

What problem is solved by sending telescopes into space?

interference of Earth’s atmosphere in detecting electromagnetic radiation

100

Scientists determine the composition and temperature of stars _____.

by analyzing the spectra of the light that stars emit

100

What type of galaxy is the Milky Way?

Spiral

100

During the first few minutes after the Big Bang, the universe was opaque. Light could not go through it. Why?

The mix of particles was so dense that photons could not get through.

100

The apparent magnitude of a star changes with the _________ .

Distance

200

If a dense, non-light producing, interstellar gas were to move between a star and Earth, what would happen to the spectra of the light from the star as measured on Earth?

The number of absorption lines would likely decrease.

200

What is the small, hot, extremely dense core left after a star collapses called?

white dwarf

200

What is an irregular galaxy?

a galaxy with no particular shape

200

What characteristic of the Cosmic Microwave Background Radiation (CMBR) provides evidence that the universe is expanding?

The CMBR can be detected coming from all directions.

200

The _________ magnitude is the measure of how bright each star would be if it were at the same distance (10 parsecs) from an observer.

Absolute

300

How will the spectra lines recorded on Earth be shifted for a light-emitting object that is moving neither toward nor away from Earth?

They will not be shifted at all.

300

What would an older star be most likely composed of?

is composed mostly of hydrogen

300

What measurement would be best used to measure the distance to the edge of the observable universe?

gigalight-year (or one billion light-years)

300

If the spectral lines from a star are shifted toward the red end of the spectrum, what must be true about how the star is moving?

the star is moving away from Earth

300

During the main-sequence stage, how is energy generated in a star’s core?

Hydrogen fuses into helium.

400

Where is our sun's energy produced?

in the core

400

Relates a star with a large mass to its expected life cycle.

Stars with a greater mass conduct fusion at a faster rate, which leads to a shorter lifespan as a main-sequence star.

400

An observer indicated a well-shaped structure with many closely spaced stars. Spectra indicate dominantly older stars. What is he likely looking at?

A star cluster

400

What is the apparent magnitude of a star a measure of?

The brightness of the star as seen from Earth

400

How long would a star with the sun’s mass stay on the main sequence?

as long as it fuses hydrogen

500

How does solar wind effect Earth's magnetic field?

It shifts the field in a direction away from the sun.

500

What is a large, bright star whose hot core has used most of its hydrogen?

Giant

500

How could an observer tell which way a spiral galaxy is turning even though they can't see it move?

By looking at the direction the spiral arms are going.

500

During a star's main-sequence stage, how is energy generated in the star's core?

Hydrogen fuses into helium

500

What can parallax be used to determine about stars?

The distance to a star