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Stars

Characteristics, Structure, Life Cycle

TermDefinition
spectroscope a tool used by astronomers that spreads light into different wavelengths
parallax an apparent change in an object’s position when viewed from two different points
apparent magnitude how bright a star appears to be from Earth
actual (absolute) magnitude how bright a star actually is based on temperature and size
luminosity brightness of a star
stars giant balls of burning gas (mostly hydrogen and helium) held together by gravity with a very hot core where nuclear fusion occurs
nuclear fusion combining of hydrogen into helium in the core of a star
radiative zone zone of a star where heat radiates out from the core
convection zone hot gasses move as the warm and cool, light energy emitted
photosphere layer of the Sun's atmosphere visible to Earth
chromosphere middle layer of the Sun's atmosphere where energy transfer occurs, appears red when visible
corona outer layer of the Sun's atmosphere, visible during solar eclipses
Hertzsprung-Russell diagrams graphs used to categorize stars that plot the luminosity and temperature of stars
sunspot temporary spots on the Sun's surface that are darker and cooler than surrounding regions
solar flare intense, sudden eruptions of electromagnetic radiation and energy from the Sun, lasting minutes to hours, often occurring near sunspots
prominence large, bright eruption of plasma from the Sun's surface extending in a loop shape
coronal mass ejection massive, fast-moving clouds of plasma and magnetic fields released from the Sun, often following solar flares
solar wind a continuous stream of plasma from the Sun's corona causing geomagnetic storms and auroras
main sequence stars most common type of star in the longest phase of their life, nuclear fusion occurs during this phase
nebular a hazy, large, dense cloud of gas and dust
protostar a very young, developing star formed when gravity collapses forming a flattened spinning disk of material around a dense core
red giant a medium sized, dying star that expands outwards
red supergiant massive, dying stars that have expanded outwards
white dwarf very dense, faint, hot leftover of a low to medium mass star at the final stage of their lifecycle
supernova a massive, bright and colorful explosion of a high mass star
neutron star the gravitationally collapsed core of a massive supergiant star after a supernova explosion
black hole an incredibly compact, dense body that not even light can escape from, formed from the collapse of the most massive stars
Created by: user-1960358
 

 



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