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8th- Galaxy,Sun,Star

TermDefinition
Absolute Magnitude the measure of how bright a star would be if it were located 10 parsecs from Earth
Apparent Magnitude the measure of how bright a star appears to be to an observer on Earth
Astronomical Unit the average distance between the Earth and the Sun; about 150 million km
Auroras when the gases in Earth’s atmosphere glow with different colors when excited by solar winds
Black Dwarf the core of the star after it runs out of all energy and becomes cold
Black Hole a large amount of mass left over from a supernova that has such a strong gravitational pull, everything near it gets pulled in; even light cannot escape its gravity
Brown Dwarf failed star that is too small in mass to have fusion but too large to be considered a planet
Chromosphere inner atmosphere of the sun that consists of a thick region of red glowing gas
Core the center most area of a star that can reach temperatures up to 15 million ºC where thermonuclear fusion occurs
Corona outer atmosphere of the sun that consists of a thin layer of gas; appears as a faint halo of light around the sun
Coronal Mass Ejections eruptions of high energy particles that travel less than speed of light; takes hours to reach us
Galaxy collection of stars, gas and dust; estimated to be 100 billion; grouped together in clusters, bound together by gravity
Elliptical Galaxy spherical or egg-shaped galaxy usually red in color because they are generally older and colder; less gas and dust
Irregular Galaxy galaxies without a well-defined shape; amount of gas and dust varies
Spiral Galaxy pinwheel shaped galaxy with spiral bands protruding from the center; usually blue in color due to being younger and hotter; contains a lot of gas and dust
Geomagnetic Storms electromagnetic storms influenced by solar wind that can affect our electrical systems
Gravity an attractive force that holds the universe together
Interstellar Matter clouds of gas and dust that is in between the stars; these clouds provide materials for new stars to form
Light Year the distance that light travels in 1 year (5.9 trillion miles)
Magnetosphere the protective magnetic field that surrounds Earth
Milky Way Galaxy the spiral galaxy that we live in that contains more than 400 billion stars
Nebula large amount of gas and dust spread out in space that is the precursor to stars
Neutron Star the material left over in the core after a supernova occurs; extremely dense and small
Parallax the apparent shift in one object’s position relative to another object caused by a change in the location of the observer
Parsec a unit of measurement used to describe distances between celestial objects; equal to 3.258 light years
Photosphere inner layer of the sun’s atmosphere made of Hydrogen gas that is visible to us
Protostar early stage of a star’s life that is a spinning collection of gas and dusts that is contracting
Pulsars a neutron star that gives off short bursts of radio waves
Quasar galaxies with black holes in their center; recently discovered that the Milky Way Galaxy is a quasar
Red Giant occurs when a star gets older and cooler; the Hydrogen atoms in the star begin to expand greatly
Solar Flares hot gases that erupt from the surface of the sun sending ions and radiation into space towards Earth
Solar Maximum the peak of an 11 year cycle in which the sun reverses its magnetic poles and an enormous amount of energy is released
Solar Minimum the part of the solar cycle during which the sun releases the least amount of energy
Solar Prominence streamers of hot gases arching above the photosphere that last for several hours but do not disrupt our communication
Solar Radiation Storms storms rated from S1 to S5 that affect electrical systems, radio communications and can cause biological damage
Solar Wind a continuous flow of electrons and protons from the sun into space that can affect Earth
Star ball of gas and dust that is extremely hot and gives off massive amounts of energy due to nuclear fusion
Sun a main sequence star that is the center of our solar system
Sunspots dark, cooler areas on the surface of the sun that have strong magnetic activity and produce solar flares; usually last 2 weeks at a time and occur in 11 year cycles
Supernova occurs when a red giant is too big and unstable which results in a huge explosion; only happens to large stars
Thermonuclear Fusion the changing of one type of element into a new element due to extreme temperatures and pressure
Universe everything physical that exists in space and time; consists of all matter and energy
White Dwarf the white hot core of the star left behind after the outer parts expand so much they drift off into space
Created by: holtzmanscience
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