Origin Of the Universe
Scale, Distance, and Structure
Electromagnetic Radiation
Spectroscopy
Stellar Evolution
100

The scientific explanation that the universe began as an extremely hot, dense state and has been expanding over time.

Big Bang Theory

100

The distance light travels in one year; used to measure large distances in space.

Light-year

100

The distance between successive wave peaks.

Wavelength

100

The study of light to determine the composition, temperature, motion, and density of objects in space.

Spectroscopy

100

The longest stage of a star’s life, where it fuses hydrogen into helium.

Main Sequence

200

All of space, time, matter, and energy that exists.

Universe

200

A massive system of stars, gas, dust, and dark matter held together by gravity.

Galaxy

200

The number of waves that pass a point in a given amount of time.

Frequency

200

A spectrum with dark lines where specific wavelengths have been absorbed by cooler gas.

Absorption Spectrum

200

A powerful explosion marking the death of a high-mass star.

Supernova

300

Faint radiation left over from the early universe that provides strong evidence for the Big Bang.

Cosmic Microwave Background (CMB)

300

The average distance between Earth and the Sun, used to measure distances within the solar system.

Astronomical Unit (AU)

300

The full range of electromagnetic radiation, from radio waves to gamma rays.

Electromagnetic Spectrum

300

A spectrum with bright lines produced when excited atoms emit light at specific wavelengths.

Emission Spectrum

300

An object with gravity so strong that not even light can escape.

Black Hole

400

The stretching of light to longer wavelengths when an object in space is moving away from Earth.

Redshift

400

A group of galaxies held together by gravity.

Galaxy Cluster

400

The highest-energy form of electromagnetic radiation, produced by extreme cosmic events.

Gamma Ray

400

Unique lines in a spectrum that identify specific elements.

Spectral Lines

400

The small, dense remains of a low-mass star after it sheds its outer layers.

White Dwarf

500

The observation that more distant galaxies move away faster, showing that the universe is expanding.

Hubble’s Law

500

The curved path an object follows as it moves around another object due to gravity.

Orbit

500

The small portion of the electromagnetic spectrum that humans can see.

Visible Light

500

The unique pattern of spectral lines that identifies an element.

Elemental Fingerprint

500

An extremely dense stellar remnant made mostly of neutrons.

Neutron Star