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SC Science TEST

Terms

undefined, object
copy deck
floated
as the material melted the more dense material sunk and the less dense materials _ to the surface
rocks
convection currents in are interior may have brought these to the curface
mantle
the middle layer
orbit
the path that a body traveles around another body in space
gravity
the matter is affected by the force of gravity& the particles are attracted to each other
period of revolution
amount of time it takes a body to complete a trip along an orbit
gravity becomes gr8r than the strength of the rock
what happenes when the earths diameter reached 350 kmr
solar nebula
cloud of gas & dust that formed our solare system
oxygen
that process released this into the air
astononmical unit
avg distance between the Earth and the sun
pressure
AS the particles of matter get closer, pressure increases& works oppsite of gravity
major axis
maximum lenghth of an ellipse
greater
newtons law of universal gravitation states that the larger & closer obj. are the _ the force of gravity
crust
the thin and solid outer most layer of the earth
Nuclear Fusion
the combination of the nuclei of small atoms to form a larger necleus
photosynthesis
about 3.4 bill yrs ago organisms that produced food by this
sunspot
a dark area of the photosphere of the sun that is cooler than the surrounding areas and that has a strong magnetic feild
keplers 1st law
this laws of motion says that planets orbit the sun in an elliptical path
3rd
2 helium-3 nuclei conbine to for a helium-4 nuclei si the _ step
revolution& semimajor axis
the 3rd law explains the relationship betweeen the period of a planets _ & its _
revolution
the motion of a body thqat traveles around another body in space
planetesimals
tiny building blocks of the planet, some becom the core of planets
planet & the sun
it is the distand between a _&_
collide and stick
in the outer regions of the solar nebula particles start to _&_ together
gravity
this pulls an obj toward another obj.
gases
the 1st atmosphere was a mixture of _ that were released as earth cooles
planetesimals and radioactive material
the collision of these 2 things caused the earth to heat up
interia
an obj tends to travel in a straight path inlesss acted on by an outside force
Nebula
Lg cloud of gas and dust in intersteller space
carbon dioxide& water vapor
molted rocks released lg amounts of thins & this in the atomsphere
Energy
during each step this is released
semimajor axis
1/2 of the distance to the major axis
photosphere
the visible layer of the sun adn is considered the surface since we can see it
coronaq
thin outer layer of the atmosphere can be seen during a solar eclipses
radiative zone
dense region where light can take millions of years to pass through
core
the central part of earth
Cinvective zone
where hot and cooler gases circulate in convection currents
closer, slower
the 2nd law states planets travel faster when they are_ to the sun and _ when they are farther away
2 hydrigen neucli collide to form a heavy hydrogen neuclei called devterium
1st step of fusion in the sun
core
where the energy is produced
solarflare
regions of extremly high temp and brightness that develope on the suns surface
2nd step
deuteriunm combines with another hydrogen neucli to form helium is the _ step
gravity& pressure
what are the two forces that are acting on the matter in a nebula
rotation
the spin of a body on its axis
chromosphere
a thin red region and can be seen during a tota solar eclipse

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