Solar System #1
Chemistry
Beginnings
Endings
Misc
100

A measure of how circular an orbit is.

Eccentricity

100

a pure substance

element

100

step in the formation of a solar system where matter has formed large clumps not big enough to clear their orbital path

protoplanet

100

what a white dwarf is called after it stops radiating light

black dwarf

100

what is thought to form at the bottom of a black hole

singularity

200

A line that connects a planet to the sun sweeps out equal areas in equal times.

Kepler's 2nd Law

200

found in the nucleus

protons and neutrons

200

contracting, spinning ball of gas that is not experiencing nuclear fusion

protostar

200

object that has a gravitational pull so strong not even light can escape

black hole

200

model of universe formation governe by the gas laws

open

300

Point on Earth's orbit that is closest to the sun.

Perihelion

300

occurs in the core of a star

nuclear fusion
300

a large field of gas and dust in space

nebula

300

process that results in the formation of elements larger than Iron

Super Nova

300

area of dust and gas around a new star from which planets form

accretion disk

400

Planets travel on elliptical paths around the sun.

Kepler's 1st Law

400

states that matter cannot be created or destroyed

conservation of mass

400

another word for the outer planets

gas giants

400

object that forms at the end of a stars life that is 8-20x the size of the sun ends

neutron star

400

evidence that most galaxies are traveling away from us

red shift

500

Point on the Earth's orbit that is furthest from the sun.

Aphelion

500

The formation of new elements larger than hydrogen.

Nucleosynthesis

500

responsible for stripping the rocky planets of gas

solar wind

500

process that happens at the end of an average stars life

nova

500

set of stars that travel through space together

galaxy