Title: OUR SOLAR SYSTEM
1OUR SOLAR SYSTEM ITS PLANETS!
2Solar System to Scale
3Planets to Scale
4The Inner Planets
- Inner Planets- Mercury, Venus, Earth, and Mars
- Called Terrestrial planets (Earthlike)
- These planets have a rocky crust, denser mantle,
and very dense core
5(No Transcript)
6MERCURY
7VENUS
8EARTH
9MARS
10The Grand Canyon of Mars Valles Marineras
Its length is the distance from NY to
California! Its widest point is the distance
from NY to Georgia!
11(No Transcript)
12Mars sure looks a lot like Arizona, eh?
13(No Transcript)
14The Outer Planets
- Outer Planets- Jupiter, Saturn, Uranus, Neptune
and Pluto - Called Jovian planets (Jupiter-like)
- These planets are much larger, more gaseous, and
less dense than the inner planets
15JUPITER
16The Moons of Jupiter
Calisto
Io
Europa
Ganymede
17SATURN
18"Saturn's diminutive moon, Mimas, poses as the
Death Star - the planet-destroying space station
from the movie Star Wars - in an image recently
captured by NASA's Cassini spacecraft
19URANUS
20NEPTUNE
21PLUTO The Planet of NO More!
- Pluto is not dense enough to be terrestrial, or
large enough to be Jovian - However, because of its location, it is
considered an Outer Planet, but IS NOT a Jovian
Planet
22(No Transcript)
23The 10th Planet!
- The new planet is the most distant object ever
seen in orbit around the sun, even more distant
than Sedna, the planetoid discovered almost 2
years ago. - It is almost 10 billion miles from the sun and
more than 3 times more distant than the next
closest planet, Pluto and takes more than twice
as long to orbit the sun as Pluto.
24(No Transcript)
25(No Transcript)
26(No Transcript)
27- CHRONOLOGY OF SOLAR SYSTEM DISCOVERY
- Sun
- Mercury
- Venus
- Earth
- Mars
- Jupiter
- Saturn
- Uranus 19th century, by telescope
- Neptune 19th century, predicted by
calculations based on Newtons Law, and by
telescope - Pluto 20th century, predicted by accident, then
by telescope observation
17th century, visual observation
28Data on the planets is located in your Earth
Science Reference Tables, page 15
29(No Transcript)
30Comets, Asteroids, and Meteoroids
31COMETS
- masses of rock, dust, ice and gases that revolve
around the sun in their own orbits - orbits are usually very eccentric (stretched
out), which means that one complete orbit of the
sun may take many years - Ex. Halleys Comet is only viewable on Earth
every 76 years! It will next appear in the year
2062!
32(No Transcript)
33Comet Hyakutake
Comet Hale-Bopp
34Tails get longer the closer the comet gets to the
Sun.
Comet Tails always point away from the Sun. Gas
(Ion) tails point straight away from the Sun.
Dust tails curves toward the orbital path.
Orbit of Comet
35ION TAIL
ION TAIL
DUST TAIL
DUST TAIL
36The orbit of Haleys Comet is highly eccentric,
and therefore the comet can only be seen on Earth
every 72 years!
37(No Transcript)
38ASTEROIDS
- solid chunks of rock floating in space
- Most asteroids are found in a nearly circular
orbit between Mars and Jupiter, revolving in the
same direction as the planets - Asteroid belt
- Most asteroids a less than 1 meter long!
39(No Transcript)
40(No Transcript)
41METEROIDS
- fragments of rocks or ice traveling through space
- Occasionally, these fragments may get pulled into
Earths atmosphere by its gravity - As the meteoroid shoots through the atmosphere,
friction causes heat to build up and the
meteoroid begins to glow - This is now called a METEOR (shooting star)
42METEROIDS
- Sometimes many meteoroids enter our atmosphere at
one time, this is called a meteor shower - If the meteor survives its trip through the
atmosphere and hits Earths surface, it is then
called a meteorite - Impact craters are potholes in the Earths
crust caused by meteorites hitting the ground
with great speed and force - Ex. the Barringer Crater in Arizona (1,300m wide,
200m deep).
43(No Transcript)
44(No Transcript)
45(No Transcript)
46(No Transcript)