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Created by
Millie W
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Cards (19)
Protostar
Cloud of
dust
and
gas
where stars initially form
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Star formation
1. Cloud of
dust
and gas pulls together to form a
protostar
2.
Temperature
and
density
increase as more particles collide
3.
Nuclear
fusion begins,
heating
the core
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Main sequence star
Outward force from
nuclear fusion balances gravity
, stable period lasting
billions
of years
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Life cycle of a small-to-medium star
1.
Hydrogen
runs out, star
expands
into red giant
2.
Outer
layers ejected, leaving behind a
white dwarf
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Life cycle of a large star
1. Undergoes more
fusion
,
expands
and contracts several times
2. Eventually explodes in a
supernova
, forming elements heavier than
iron
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Neutron star
Very dense core left behind after a
supernova explosion
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Black hole
Super
dense
point in space that even
light
cannot escape
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The Solar System has one star - the
Sun
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Objects in the Solar System
8
planets
Dwarf
planets
Moons
Asteroids
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The
Solar System
is a tiny part of the
Milky Way
galaxy
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Gravity
The
force
that creates
orbits
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Orbits
1. Object constantly changes direction,
accelerating
towards the
centre
2.
Velocity
changes but
speed
remains constant
3.
Gravitational
force keeps object in a
circular
orbit
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Orbital speed
Faster
moving objects have
smaller
orbits
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The
universe
appears to be
expanding
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Red-shift
Increase in the wavelength of light from distant
galaxies
, indicating they are moving
away
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More distant galaxies have greater red-shifts, indicating they are moving away
faster
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Big Bang theory
The
universe
started from a very small, dense and
hot
space that then expanded
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New
evidence
may change our theories about the
universe
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Dark
matter
and dark
energy
are not well understood
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