Nebulae and Star Formation
Stellar Life Cycle
Star Colors and Types
Black Holes
Stars Spectrum
100

What is a nebula? 

A vast cloud of gas and dust in space, often a stellar nursery where stars form. 

100

What is the main sequence?

A stable phase when a star fuses hydrogen into helium in its core. 

100

What color indicates the hottest stars?

Blue or blue-white

100

What is a black hole?

A region of space where gravity is so strong that nothing, not even light, can escape. 

100

How do we determine a star's composition?

By analyzing its spectrum for absorption/emission lines.

200

Name three types of nebulae

Emission nebulae (glowing), reflection nebulae (reflecting starlight), and dark nebulae (blocking light). 

200

What happens during a supernova? 

A massive star explodes, ejecting its outer layers and leaving behind a neutron star or black hole. 

200

What type of star is our Sun?

A yellow dwarf (spectral type G)

200

How is a black hole formed?

From the collapse of a massive star's core after a supernova. 

200

What information do dark lines in a spectrum provide?

The elements present, based on which wavelengths are absorbed. 

300

What triggers nuclear fusion in a star?

Gravitational collapse increases core temperatures and pressure until fusion begins. 

300

What is a red giant? 

A late-stage star that explodes and cools after exhausting hydrogen in its core. 

300

What spectral type is the coolest?

M-type (red stars)

300
What happens to an object that crosses the event horizon?

It cannot escape and falls toward the singularity. 

300

How do we classify stars on the Herzsprung-Russel diagram?

By surface temperature (spectral type) and luminosity (brightness)

400

What role does gravity play in star formation? 

Gravity pulls gas and dust together, increasing density and heat until a star forms. 

400

What are the final stages of a high-mass star?

It undergoes a supernova, then becomes a neutron star or block hole.

400

What is mnemonic device for spectral types?

O, B, A, F, G, K, M --> "Oh Be A Fine Girl/Guy, Kiss Me"

400
Describe the difference between stellar-mass and supermassive black holes.

Stellar-mass are a few to tens of solar masses; supermassive are millions to billions of solar mases, found at galaxy centers. 

400

What can we learn from a star's spectrum?

Temperature, composition, motion (Doppler shift), and sometimes age. 

500

Explain the process of gravitational collapse. 

A cloud of gas and dust contracts under gravity, raising temperature and pressure until nuclear fusion stars. 

500

What occurs during the protostar phase?

A collapsing gas cloud heats up into a dense core but hasn't yet started nuclear fusion. 

500

How does temperature relate to a star's color?

Hotter stars look blue/white, cooler stars look yellow/red

500

Why is the term "suck" misleading when talking about black holes?

They don't pull objects in like vacuums; objects fall in only if they cross their gravitational influence. 

500

What is cosmic equilibrium in relation to stars?

The balance between gravity pulling inward and fusion pressure pushing outward, keeping a star stable.