The Sun pt 1
The Sun pt 2
Lives of Stars pt 1
Lives of Stars pt 2
Misc.
100

This is the visible surface of the sun, where sunspots and solar weather occur

Photosphere

100

___________________ refers to how reflective a surface is, and is measured as a percentage of how much light is reflected by the surface

BONUS: What types of surfaces on Earth are highly reflective?

Albedo

BONUS: Snow/ice -- albedo of 0.8

100

Stars are born from _____________ _____________, dense nebulas of gas and dust

molecular clouds

100

True or False: M class stars are likely to have shorter lifespans that O class stars

False

100

True or False: Solar flares, large outbursts of energy from the sun, can cause mass power outages on Earth

True

200

Nuclear fusion occurs in the __________ of stars, generating the energy that makes stars luminous


BONUS: What temperature must be reached for nuclear fusion to begin?

Core

BONUS: 15 million K

200

__________________ is the phenomenon by which shorter wavelengths of light bounce off the molecules in our atmosphere, leaving longer wavelengths to pass through and reach our eyes


Scattering

200

____________ _____________ is how bright a star appears from Earth, and is therefore distance dependent. 

_____________ ____________ or luminosity is a measure of how bright the star actually is, independent of distance from Earth

Apparent magnitude

Absolute magnitude

200

The stellar remnants shown here are the results of the death of a _____-mass star

This remnant could still undergo a type-1 _____________ if it exists in a binary pair

Only massive stars undergo _______ supernovas



Low

Supernova

Type-2

200

True or False: Elements heavier than iron can only be created upon the death of a massive star

BONUS: The explosive shockwave created upon the death of a massive star is known as a _____________________

True

Supernova

300

In this layer of the sun's interior, gamma rays bounce around and lengthen out, becoming less energetic as they transition to the outer layers of the star.

Radiation/radiative zone

300

_______________ are areas on the surface of the sun that appear dark because of their relatively lower temperatures.

The ___________ ___________ is the constant stream of charged particles that is emitted by the sun. 

Sunspots

Solar wind

300

____-class stars are small, dim, and red

____-class stars are medium sized and yellow

____-class stars are large, blue, and bright

M

G

O

300

________ _________ stars are those that are still fusing H into He, and are therefore still alive

_________ ________ are stars that are no longer fusing hydrogen into helium; radiation pressure has broken down in the core and the outer layers of the star are now expanding and cooling

__________ __________ are the extremely dense corpses of low mass stars, that can no longer undergo nuclear fusion 

Main sequence

Red giants

White dwarfs

300

A list of apparent magnitudes is given below. Which of the following stars would be brightest?

Star A: -3.5

Star B: 1.0

Star C: 15.0

Star A

400

In this layer of the sun's interior, heat is transferred from inner layers of the star to outer layers by the following process:

Warm material near the core of the star heats, becoming less dense and rising. This material cools as it transfers energy to outer layers of the star, and sinks back down


Convective/convection zone

400

The ______________ of the sun radiates most strongly in the UV portion of the EM spectrum. The ______________ radiates most strongly in the X-ray portion of the EM spectrum

BONUS: What may be causing these outer layers to be higher in temperature than more interior layers?

Chromosphere

Corona

BONUS: Electromagnetic field interactions

400

The color of a star is mainly determined by a star's temperature

_________ stars have the highest temperatures and shortest lifespans

________ stars have the lowest temperatures and longest lifespans

BONUS: Our sun has a lifespan of about 10 _____________ years

Blue

Red

BONUS: 10 billion

400
Briefly list the steps of star formation (two or three steps)

1. Dense areas of molecular cloud collapse due to gravitational disturbance (supernova shockwave)

2. As dense areas collapse and heat up, they eventually reach nuclear fusion temps in core (15 million K)

400

Sunspots typically occur in an _______-year cycle


BONUS: True or false -- the maximum of the sunspot cycle (more sunspots) typically corresponds with calm solar weather

11-year cycle

BONUS: False

500

Draw a diagram of the sun with all layers labeled. You should have six layers.


500
BRIEFLY explain how the northern and southern lights are caused


BONUS: What causes the different colors of the northern lights?

Charged particles from the solar wind excite electrons in atmospheric gases, causing them to emit light

BONUS: Different gases (with different electron configurations) will emit different wavelengths of light

500

Utilizing the HR diagram shown below, describe the type of star that would be found at the following points:

A: 3000 K, 0.0001 luminosity

B: 10,000 K, 0.01 luminosity

C: 3500 K, 10,000 luminosity


A: Main sequence, red dwarf

B: White dwarf

C: Red giant

500

List what products will be formed upon the death of each type of star:

A -- low mass star

B -- high mass star

C -- very high mass star

A: white dwarf and planetary nebula

B: Neutron star

C: Neutron star which collapses into a black hole

500

Explain why, during high noon, the sun appears yellow, whereas during sunsets or smoky days it appears red.

The sun has more atmosphere to travel through during sunset, meaning even yellow light is scattered (leaving only red). Smoky days also enhance the scattering effect.