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Earth Science Chapter 28

Key Words

Terms

undefined, object
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auroras
sheets of coloured light produced by a magnetic storm in the earths upper atmosphere
solar flare
sudden violent eruption of electrically charged atomic particles from the suns surface
convective zone
region around the suns radiative zone in which moving gases transfer energy
sunspot cycles
periodic variation in the number of sunspots that occurs aproximately every 11 years
prominences
cloud of glowing gases that arches high above the suns surface
chromosphere
thin layer of the sun's atmosphere that lies above the photosphere and glows with a redish light; colour sphere
solar wind
electrically charged atomic particles that stream out into space through holes in the suns corona
nebular theory
theory that the sun and the planets condensed out of a spinning cloud of gas and dust
corona
outmost layer of the suns atmospere; crown
plantesimals
small body of matter that formed in outer regions of the solar nebula while the sun was forming in its center
solar system
the sun and the bodies that revolve around it
planets
nine major bodies that orbit the sun
protoplanets
large body of matter that formed from the coalescene of plantesimals in the solar nebula
solar nebula
cloud of gas and dust that developed into the solar system
radiative zone
region surrounding the core of the sun in which energy is transferred in the form of electro magnetic waves
sunspots
cool, dark area of gas within the protosphere caused by powerful magnetic fields
photosphere
innermost layer of the solar atmosphere light sphere

Deck Info

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