Star: A huge ball of hot gas that makes its own light by fusion Nebula: A cloud of gas and dust in space Protostar: A young star still forming inside a nebula Main sequence: The long stage when a star fuses hydrogen into helium Red giant: A swollen, cool star near the end of its life White dwarf: The small hot core left after a medium star ends Planetary nebula: A glowing shell of gas thrown off by a dying star Supernova: The explosion of a massive star at the end of its life Neutron star: The super-dense core left by some supernovae Pulsar: A spinning neutron star that sends out beams of radiation Black hole: A region where gravity is so strong that not even light can escape Event horizon: The boundary around a black hole beyond which nothing returns Red dwarf: A small, cool, long-lived star Supergiant: A very large, luminous star Binary star: Two stars orbiting each other Variable star: A star whose brightness changes Nova: A white dwarf suddenly brightening by pulling in gas Star color and temperature: Blue stars are hottest; red stars are coolest Spectral classes from hot to cool: O, B, A, F, G, K, M Spectral class of the Sun: G Luminosity: The total amount of light a star gives off Apparent magnitude: How bright a star looks from Earth Absolute magnitude: How bright a star would look from a standard distance Hertzsprung-Russell diagram: A graph plotting star brightness against temperature Light-year: The distance light travels in one year, about 9.5 trillion kilometers Parallax: The apparent shift of a nearby star against the background as Earth moves Galaxy: A huge collection of stars, gas and dust held together by gravity Milky Way: Our home galaxy, a spiral with a central bar Spiral galaxy: A galaxy with arms curling out from the center Elliptical galaxy: A smooth oval-shaped galaxy Irregular galaxy: A galaxy with no regular shape Galaxy cluster: A group of many galaxies bound by gravity Local Group: The cluster of galaxies that includes the Milky Way Large Magellanic Cloud: A small galaxy that orbits the Milky Way Quasar: An extremely bright center of a distant galaxy powered by a black hole Dark matter: Unseen matter that adds gravity to galaxies Dark energy: A mysterious force that speeds up the expansion of the universe Big Bang theory: The universe began extremely hot and dense about 13.8 billion years ago Expanding universe: Space is stretching, carrying galaxies apart Redshift: Light from receding objects stretches toward red Who found that galaxies move away from us in 1929?: Edwin Hubble Cosmic microwave background: The faint glow left from the early universe Observable universe: The part of the universe we can see from Earth Exoplanet: A planet orbiting a star other than the Sun Habitable zone: The region around a star where liquid water could exist on a planet Telescope: An instrument that gathers light to see faraway objects Refracting telescope: A telescope that uses lenses Reflecting telescope: A telescope that uses mirrors Radio telescope: A dish that collects radio waves from space Spectrum of starlight: Shows what elements a star contains Astronomy: The study of space and everything in it Astrophysics: The branch of astronomy using physics to explain objects in space Cosmology: The study of the origin and structure of the universe Who proposed the Sun-centered solar system in 1543?: Nicolaus Copernicus Who first used a telescope to study the sky in 1609?: Galileo Galilei Who described the laws of planetary motion?: Johannes Kepler Which star is closest to Earth?: The Sun Which star is the closest after the Sun?: Proxima Centauri Star formation location: Inside dense nebulae Chandrasekhar limit: The maximum mass of a white dwarf, about 1.4 solar masses Solar mass: A unit equal to the mass of the Sun Gravitational waves: Ripples in space-time first detected in 2015 First image of a black hole shadow, released: 2019, in the galaxy M87 Free flashcards from Peabody at peabody.kids/flashcards/space-stars-universe