Transcript Chapter 19
Astronomy
Our Solar System
Chapter 29.4
Formation of our Solar System
Stars and planets
form from clouds of
gas and dust, called
interstellar clouds,
which exist in space
between the stars.
A Collapsing Interstellar Cloud
Our solar system
may have begun
when interstellar gas
started to condense
as a result of
gravity.
Sun and Planet Formation
The disk of dust and gas that formed the
Sun and planets is known as the solar
nebula.
GROWTH OF OBJECTS
–
Condensed
material started
to accumulate
and merge
together to form
larger bodies.
PLANETESIMALS
–
Planetesimals are
solid bodies,
reaching hundreds
of kilometers in
diameter, that
formed as smaller
particles collided
and stuck together.
ASTEROID BELT
–
Between Jupiter and
Mars
–
Jupiter’s
gravitational force
prevented them
from merging to
form a planet.
ASTEROIDS
Orbit the Sun
within the
planetary orbits
that are leftovers
from the
formation of the
solar system.
PIECES OF ASTEROIDS
A meteoroid is an
asteroid that falls
toward Earth and enters
Earth’s atmosphere.
A meteor is the streak
of light produced when
a meteoroid burns up in
Earth’s atmosphere.
A meteorite is part of
a meteoroid, that does
not completely burn up,
that collides with the
ground.
COMETS
small, icy bodies
that orbits around
the Sun and are
remnants from solar
system formation.
made of ice and
rock