Presentation is loading. Please wait.

Presentation is loading. Please wait.

Our Solar System ©Mark Place, 2007-2008 www.LearnEarthScience.com.

Similar presentations


Presentation on theme: "Our Solar System ©Mark Place, 2007-2008 www.LearnEarthScience.com."— Presentation transcript:

1 Our Solar System ©Mark Place,

2 The total mass of all the asteroids is less than that of the Moon.
rocky objects with round or irregular shapes lie in a belt between Mars and Jupiter The total mass of all the asteroids is less than that of the Moon.

3

4 only visible when they are close to the sun

5 Comet orbit (notice tail)
Famous comets

6 shooting stars Meteor showers (link)

7 Meteorites Meteoroids (in space) that STRIKE the ground = MeteoriTes!!
3 main types: 1 – Stony - Si, Al = “crust” 2 – Metallic - Fe, Ni = “core” 3 – Carbonaceous chondrites – C = “life”

8 Apophis Nasa

9 The Planets

10 Terrestrial vs. Jovian Terrestrial planets are the inner, earth-like planets Jovian planets are the outer, Jupiter-like planets

11 Draw a line across the table between
the terrestrial and Jovian planets and label.

12

13 Which are more dense? Jovian or terrestrial

14 Which have more moons ? Jovian or terrestrial

15 Which have longer periods of revolution?
Jovian or terrestrial

16 Which are larger in size on average ?
Jovian or terrestrial

17 Which planet has the longest day?
Venus

18 Which planet has the longest year?
Neptune

19 Pg. 7

20 How are the orbits of the planets described?
slightly, eccentric ellipse - Kepler's 1st Law eccentricity website

21 More eccentric Which planet has the least Mercury
perfectly circular orbit? More eccentric Mercury

22 Least eccentric Venus Which planet has the most
perfectly circular orbit? Least eccentric Venus

23 Calculate the eccentricity
of the ellipse below: length of major axis Formula: eccentricity = distance between foci (d) length of major axis (L)

24 d = 1.7 cm _________ L = 6.5 cm e = 0.262 Eccentricity e = d L
-Round to nearest thousandth -NO labels

25 When does a planet move fastest in its orbit? When closest to Sun When does a planet move slowest in its orbit? When furthest from Sun

26

27 Area A = Area B Equal areas
Kepler's Second Law Area A = Area B Equal areas eccentricity website Website 2

28 Explain the difference between the geo- and helio-centric
models of the solar system. Helio-centric Geo-centric Earth- centered Sun- centered


Download ppt "Our Solar System ©Mark Place, 2007-2008 www.LearnEarthScience.com."

Similar presentations


Ads by Google