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Transcript
Astronomy - Chapter 3 Section 1: A Solar System is Born p. 64-67
Vocabulary/Main Ideas
The Solar Nebula
Nebula
Details and Supporting Facts
o A large cloud of gas and dust in
interstellar space; a region in space
where stars are born or where stars
explode at the end of their lives
o Gravity and pressure interact in a
nebula to form stars
Gravity Pulls Matter Together o The gravitational attraction in a
nebula is very weak, but it holds the
gas and dust together
Pressure Pushes Matter
Apart
o In a nebula, outward pressure
balances the inward gravitational
pull and keeps the cloud from
collapsing
Upsetting the Balance
o The balance between gravity and
pressure can be upset if two
nebulas collide or a nearby star
explodes
o Globules form and contract,
collapse inward, and the
temperature rises and stars begin to
form
Solar Nebula
o The cloud of gas and dust that
formed our solar system
How the Solar System
Formed
(See Figure 3 on p. 65)
1) The young solar nebula begins
to collapse
2) The solar nebula rotates,
flattens, and becomes warmer
near its center
3) Planetesimals begin to form
within the swirling disk
4) As the largest planetesimals
grow in size, their gravity
attracts more gas and dust
5) Smaller planetesimals collide
with larger ones and planets
begin to grow
6) A star is born and the remaining
gas and dust are blown out of
the new solar system
Pictures and Diagrams
Astronomy - Chapter 3 Section 1: A Solar System is Born p. 64-67
From Planetesimals to
Planets
o Bits of dust continued to collide
within the solar nebula, and
grew into large bodies called
planetesimals.
Gas Giant or Rocky Planet?
o The largest planetesimals
formed near the outside of the
rotating solar disk, where
hydrogen and helium were
located. These grew and
became the gas giants – Jupiter,
Saturn, Uranus and Neptune.
o It was too hot in the center of
the nebula for gases to remain,
so the rocky planets Mercury,
Venus, Earth, and Mars formed
here.
The Birth of a Star
o As the planets were forming
within the nebula, the center
became so dense and hot that
hydrogen atoms fused to form
helium
o Fusion released huge amounts
of energy and created enough
outward pressure to balance the
inward pull of gravity. When
the gas stopped collapsing, the
sun was born and our solar
system was complete!