Star Formation
Star Life Cycle & Remnants
Big Bang Evidence
H–R Diagram
Spectra & Motion
100

What two forces fight each other during star formation?

Gravity vs. pressure

100

What will the Sun eventually become?

A white dwarf

100

What does redshift tell us about distant galaxies?

They are moving away

100

What two variables are plotted on the H-R diagram?

Temperature and luminosity  

100

What causes dark absorption lines?

Elements absorbing specific wavelengths of light

200

What event marks the transition from protostar to main sequence?

The start of hydrogen fusion

200

What causes a star to expand into a red giant?

The core runs out of hydrogen and contracts

200

Why is the CMB so cold today?

The universe expanded and cooled over billions of years

200

Where are the hottest stars located?

Upper left

200

A star with strong iron lines has high or low metallicity?

High

300

What causes a nebula to begin collapsing?

Uneven density leading to gravitational collapse

300

Which stars explode as supernovae?

High-mass stars

300

What do small temperature variations in the CMB represent?

Early clumps where galaxies later formed

300

What determines where a star falls on the main sequence?

Its mass

300

If a star’s spectrum is shifted to shorter wavelengths, what is happening?

It’s moving toward us (blueshift)

400

What process grows a forming protostar as dust and gas stick together?

Accretion

400

What determines whether a supernova leaves a neutron star or black hole?

Mass of the collapsing core

400

Why do hydrogen and helium abundances support the Big Bang?

They match predicted early universe ratios

400

Stars in the lower right of the diagram are what type?

Cool and dim

400

Why do different elements produce different line patterns?

Each element absorbs light at unique energy levels

500

Why do stars form only in certain parts of molecular clouds?

Those regions are denser and colder, allowing collapse to begin

500

Why does fusion stop after iron forms in a massive star?

Fusing iron requires more energy than it releases

500

What type of radiation is the CMB?

Microwave radiation

500

Why are giant stars so luminous even if they’re cooler than the Sun?

Their large radius increases energy output

500

What can spectra reveal about a star besides composition?

Motion (redshift/blueshift) and relative temperature