Sun
Kepler & Newton
Stars
HR Diagram
Misc.
Solstices, Eclipses and Tides
100

The process by which the Sun produces energy 

Nuclear fusion (hydrogen atoms fusing into helium atoms)

100

Kepler's First Law states that planetary orbits are this shape

elliptical

100

Force that holds stars and galaxies together

Gravity

100

The HR Diagram plots stars on the basis of these two characteristics

Temperature and luminosity

100
You can calculate this if you know the mass and gravity of a planet

It's acceleration due to gravity

100

Location of the moon during a solar eclipse

Between the Sun and Earth

200

the layer of the sun we see

photosphere

200

In the equation p2=a3, p represents what?

orbital period in Earth years

200

The hottest stars are this color

blue

200

Most stars are in this area of the HR diagram

Main sequence

200

The four types of galaxies

elliptical, spiral, peculiar, and irregular

200

During the summer solstice in the Northern Hemisphere, the Earth is...

at aphelion and thus moving the slowest

300
The reason why sunspots are dark

They are cooler than the surrounding areas

300

Newton's First Law (inertia) states that an object in motion will...

Stay in motion unless acted upon by an outside force

300

When a massive star collapses and then explodes

supernova

300

Where the hottest brightest stars are on the HR diagram

top left

300

Light years and parsecs are units of this

distance

300

Cause of tides on Earth

gravitational pull of the sun and moon as well as the Earth's rotation

400

The group of stars the sun is in/ type of star

main sequence

400

According to Kepler's Laws, a planet will move the slowest in its orbit at this time

When it's at aphelion, or the furthest from the sun

400

The swirling cloud of gas and dust that is a birthplace of stars

nebula

400

Where supergiants are on the HR diagram

Top right

400

The Big Bang theory explains this

Origin and expansion of the universe

400

Type of tides Earth will have when the moon is either in the first or last/ third quarter position

Neap tides

500

Layers of the sun in order from inside to outside

Core, radiative zone, convective zone, photosphere, chromosphere, corona

500
The Earth is at perihelion during this season in the Northern Hemisphere

Winter

500

Reason our sun will never go supernova

It's too small- it is a small/ medium sized star. Only large mass stars go supernova.

500

The sun is this color star

yellow

500

Redshift of light from distant galaxies suggests this

The universe is expanding

500
When there are equal amounts of daylight and sunlight, usually around March 20 and September 22

Equinoxes