a tour of the solar system

A Tour of the Solar System

• An image of each planet will be visible on individual slides.

• Each slide will also describe the general composition, size, motion and relative position of each planet in the solar system.

• Additional slides of planetary satellites, comets, and asteroids will be included.

• Hyperlinks to additional slides and web sites will provide supplemental information.

Presented by Keith DeLongPresented by Keith DeLong

In this PowerPoint presentation, students explore the solar system. The relative position of each planet in the solar system is illustrated and students examine the appearance of each planet as well as investigate its composition, size and motion. Also, planetary satellites, comets and asteroids are discussed. Additional information on the solar system and its component elements are available to students via hyperlinks to slides and additional web sites.

Abstract

The Standard Addressed in this Presentation

Earth’s Place in the Universe

1. Astronomy and planetary exploration reveal the solar system’s structure, scale, and change over time. As a basis for understanding this concept:

a. Students know how the differences and similarities among the sun, the terrestrial planets, and the gas giants may have been established during the formation of the solar system.

The Solar System

MERCURY

VENUS

EARTH

MARS

JUPITER

SATURN

URANUS

NEPTUNE

PLUTO(Dwarf Planet)

SUN

COMETS OR METEOROIDS

Mercury, Venus, Earth, and Mars are the inner planets.

They are also known as terrestrial planets.

Jupiter, Saturn, Uranus, Neptune, and Pluto are the outer planets.

Jupiter, Saturn, Uranus, and Neptune are also known as gas giants or Jovian planets.

Pluto is a big ball of ice.

Not to scale

Between Mars and Jupiter there is a large number of rocks orbiting the sun.

Each rock is known as an ASTEROID.

This ring of rocks is called the Asteroid Belt.

| The Solar System | Sun | Mercury | Venus | Earth | Mars | Jupiter | Saturn | Uranus | Neptune | Pluto (Dwarf Planet) | Asteroids | Comets | Meteors, Meteoroids, and Meteorites | End Show |

Sun• The Sun is a star at the center of our solar system.• It is estimated to be 4.5 billion years old.• It supports all life on Earth through photo-

synthesis and is the ultimate source of all food and fossil fuel.

• It is 333,400 times more massive than the Earth (this means that 333,400 Earths can make up the Sun).

• 99.86% of all the mass of the solar system is found in the Sun.

• The core of the Sun is 16 million °C.• The surface of the Sun is 7000° C• It takes several hundred thousand years for

photons to escape from the dense core and reach the surface.

• The Sun generates energy the equivalent of 100 billion tons of TNT exploding every second.

ADDITIONAL INFORMATION ABOUT NUCLEAR FUSION

Links to Sun sites:•Live from the Sun•StarDate: The Sun•Solar Data Analysis Center


http://passporttoknowledge.com/sun/

http://stardate.org/resources/ssguide/sun.html

http://umbra.nascom.nasa.gov/sdac.html

Nuclear Fusion in the Sun

The Sun is basically a huge ball of hydrogen gas held together by the gravity created by its own mass. Under the intense pressure created at the centre of the Sun by gravity, hydrogen nuclei are fused together to produce helium nuclei. Very simply stated, four hydrogen nuclei are fused into one helium nucleus, however one helium atom has less mass than four hydrogen atoms. The fusion process releases enough energy to account for the lost mass.

The energy released by nuclear fusion in the Sun's core heats the Sun. The hot Sun radiates light into space, warming the Earth and the other planets.

About 1300 watts per square meter reaches the Earth's orbit, of which about 1000 watts per square meter reaches the Earth's surface (on a clear day).


VIDEONUCLEAR FUSION IN THE SUN

Nuclear Fusion in the SunVideo


QuickTime™ and aSorenson Video 3 decompressorare needed to see this picture.

Relative position: 1st planet out from the sun. Appearance: Resembles Earth's Moon, scarred

by thousands of impact craters. There are areas of smooth terrain as well as cliffs, some soaring a mile high, formed by ancient impacts.

General composition: Rocky material. It is a terrestrial planet.

Density: 5.43 g/cm3

Atmosphere: Almost no atmosphere. The very little atmosphere that exists is composed chiefly of oxygen, sodium, and helium.

Size: .054 the volume of the EarthPlanetary satellites (Moons): NoneRotation: 58.65 days (very slow rotation)Revolution: 88 days to go around the Sun once.Temperatures: High: 467 °C on the sunny side

of the planet. Low: -183 °C on the dark side of the planet.

Mercury (Planet)

Links to Mercury sites:•Exploring the Planets - Mercury•Missions to Mercury•NASA Planetary Photojournal: Mercury


http://www.nasm.edu/ceps/etp/mercury/

http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Mercury

http://photojournal.jpl.nasa.gov/targetFamily/Mercury

Relative position: 2nd planet out from the sun. Appearance: It is covered by thick, rapidly spinning

clouds. Due to its thick cloud layer reflecting sunlight, it is the brightest planet in the sky

General composition: Rocky material. It contains an iron core and a molten rocky mantle. The crust is a solid, rocky material. It is a terrestrial planet.

Density: 5.24 gm/cm3

Atmosphere: Consists mainly of carbon dioxide, nitrogen, and droplets of sulfuric acid; it contains almost no water vapor. This thick atmosphere traps immense amounts of heat in a large-scale greenhouse effect.

Size: .88 the volume of the EarthPlanetary satellites (Moons): NoneRotation: -243 days (retrograde) Revolution: 225 Earth days. Its day is longer than its

year.Temperature: 450 °C. It’s hotter than Mercury due to

the greenhouse effect. It is actually hot enough to melt lead.

Venus (Planet)

Links to Venus sites:•Exploring the Planets - Venus•Missions to Venus•StarDate: Venus


http://www.nasm.si.edu/ceps/etp/venus/

http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Venus

http://stardate.org/resources/ssguide/venus.html

Relative position: 3rd planet out from the sun. Appearance: The Earth looks blue and green

from space with clouds moving through the atmosphere. The surface of the Earth is 70% water and 30% land.

General composition: Rocky material. It is a terrestrial planet. It has a nickel-iron core with a molten mantle and solid rocky crust.


Atmosphere: Mostly oxygen (21%) and nitrogen (78%). Some argon, carbon dioxide, and water vapor.

Size: 40,000km (24,8000miles) around at the equator.

Planetary satellites (Moons): 1 - The MoonRotation: 23 hours, 56miutes (1 day)Revolution: 365.25 daysTemperature: Mean surface 15 °C to 20 °C

Earth (Planet)

Links to Earth sites:•Exploring the Planets - Earth•Missions to Explore Earth•StarDate: Earth

Special feature: Earth sustains life as we know it. Water exists in all three states (solid, liquid , and gas) on the Earth. There is a delicate balance between its oceans, air, land, and life.


http://www.nasm.edu/ceps/etp/earth/

http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Earth&Era=Past

http://stardate.org/resources/ssguide/earth.html

The Moon• The Moon is the Earth’s only natural satellite.

• The Moon contains no water and has no atmosphere

• Its has about 1/6 the mass of the Earth, therefore it has 1/6 the gravitational pull of the Earth.

• • It is 384 401 km from the Earth.

• It takes 27.32 days to orbit the Earth once.

• The gravitational pull of the Moon is responsible for the Earth’s tides.

• The surface of the Moon is covered with craters and flatlands. The craters are due to repeated meteorite bombardments while the dark, flatlands are the result of ancient lava flows.

Links to Moon sites:Missions to the MoonStarDate: MoonCollecting Moon Rocks BACK


http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Moon

http://stardate.org/resources/ssguide/moon.html

http://stardate.org/resources/ssguide/moon.html

http://www.lpi.usra.edu/expmoon/Apollo11/A11_Samples_tools.html

Mars (Planet)

Relative position: 4th planet out from the sun. Appearance: Mars appears red due to the iron

oxide in its soil. It has polar ice caps that grow and recede with the seasons, and it has dust storms, which cause giant dunes, wind streaks, and wind-carved features.

General composition: Rocky material. It is a terrestrial planet.


Atmosphere: Mostly carbon dioxide, nitrogen, and argon.

Size: .149 times the volume of the Earth.Planetary satellites (Moons): 2 MoonsRotation: 24 hours, 33 minutes.Revolution: 686.67 days.Temperature: -87 °C to -5 °C

Links to Mars sites:•Missions to Mars•Mars Explorations•StarDate: Mars

Special Features: Mars has the largest volcanic mountain in the solar system, Olympus Mons (27 km high and 600 km across); volcanoes in the northern Tharsis region that are so huge they deform the planet's roundness; and a gigantic equatorial rift valley, the Valles Marineris. This canyon system would stretch from New York to Los Angeles; the Grand Canyon could fit into one of the side canyons of this great chasm.


http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Mars

http://mars.jpl.nasa.gov/

http://stardate.org/resources/ssguide/mars.html

Moons of MarsPhobos

Gouged by a giant impact crater and beaten by thousands of meteorite impacts, Phobos is on a

collision course with Mars. It may collide with Mars in 50 million years or break up into

a ring.

Deimos

It is also heavily cratered with a small lumpy appearance.

BACK


Relative position: 5th planet out from the sun. Appearance: It is sometimes called a “mini-solar

system” because of its numerous moons and several rings. Jupiter appears striped because light and dark belts are created by strong east-west winds.

General composition: It is a gas giant, meaning it is mostly made of gases. Jupiter's core is probably not solid but a dense, hot liquid with a consistency like thick soup.


Atmosphere: Mostly hydrogen, helium and methane.

Size: 1316 times the volume of the Earth. It is the planet with the highest gravity in the solar system.

Planetary satellites (Moons): 63 Moons; some of them have been named and some have alphanumeric designations.

Rotation: 9 hours, 54 minutesRevolution: 11.86 Earth yearsTemperature: -108 °C

Jupiter (Planet)

Links to Jupiter sites:•Exploring the Planets - Jupiter•Missions to Jupiter•StarDate: Jupiter

Special Feature: The Great Red Spot has existed for at least 100 years, and perhaps longer. It is a hurricane-like storm on Jupiter. (Galileo reported seeing a similar feature nearly 400 years ago). Three Earths could fit across the Great Red Spot.


http://www.nasm.edu/ceps/etp/jupiter/

http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Jupiter

http://stardate.org/resources/ssguide/jupiter.html

http://stardate.org/resources/ssguide/jupiter.html

Moons of Jupiter1. Io2. Europa3. Ganymede4. Callisto5. Amalthea6. Himalia7. Elara8. Pasiphae9. Sinope10. Lysithea11. Carme12. Ananke13. Leda14. Thebe15. Adrastea16. Metis

17. Callirrhoe18. Themisto19. Megaclite20. Taygete21. Chaldene22. Harpalyke23. Kalyke24. Iocaste25. Erinome26. Isonoe27. Praxidike28. Autonoe29. Thyone30. Hermippe31. Aitne32. Eurydome

33. Euanthe34. Euporie35. Orthosie36. Sponde37. Kale38. Pasithee39. Hegemone40. Mneme41. Aoede42. Thelxinoe43. Arche44. Kallichore45. Helike46. Carpo47. Eukelade48. Cyllene

49. Kore50. S/2003 J251. S/2003 J352. S/2003 J453. S/2000 J1154. S/2000 J555. S/2003 J956. S/2003 J1057. S/2003 J1258. S/2003 J1559. S/2003 J1660. S/2003 J1761. S/2003 J1862. S/2003 J1963. S/2003 J23

BACK


Saturn (Planet)Relative position: 6th planet out from the

sun. Appearance: Saturn has a large system of

rings, and the yellow and gold bands in its atmosphere are caused by super-fast winds combined with heat rising from its interior.

General composition: It is a Gas giant, meaning it is mostly made of the gases hydrogen and helium.

Density: .70 gm/cm3 (This low density means that Saturn could float on water if their was a body of water big enough).

Atmosphere: Mostly hydrogen and helium.Size: 755 times the volume of the Earth. Planetary satellites (Moons): 60 Moons;

some have been named and others have alphanumeric designations

Rotation: 10 hours, 38 minutesRevolution: 29.45 Earth yearsTemperature: -139 °C

Links to Saturn sites:•Exploring the Planets - Saturn•Missions to Saturn•StarDate: Saturn

Special feature: Saturn's ring system is the most extensive and complex in our solar system; it extends hundreds of thousands of kilometers from the planet. The rings are mostly water ice with particles ranging in size from a few micrometers to several tens of meters.


http://www.nasm.edu/ceps/etp/saturn/

http://solarsystem.nasa.gov/missions/profile.cfm?Object=Saturn

http://stardate.org/resources/ssguide/saturn.html

http://stardate.org/resources/ssguide/saturn.html

Moons of Saturn1. Mimas2. Enceladus3. Tethys4. Dione5. Rhea6. Titan7. Hyperion8. Iapetus9. Erriapus10. Phoebe11. Janus12. Epimetheus13. Helene14. Telesto15. Calypso

16. Kiviuq17. Atlas18. Prometheus19. Pandora20. Pan21. Ymir22. Paaliaq23. Tarvos24. Ijiraq25. Suttungr26. Mundilfari27. Albiorix28. Skathi29. Siarnaq30. Thrymr

31. Narvi32. Methone33. Pallene34. Polydeuces35. Daphnis36. Aegir37. Bebhionn38. Bergelmir39. Bestla40. Farbauti41. Fenrir42. Fornjot43. Hati44. Hyrokkin45. Kari

46. Loge47. Skoll48. Surtur49. S/2004 S750. S/2004 S1251. S/2004 S1352. S/2004 S1753. S/2006 S154. S/2006 S355. Greip56. Jarnsaxa57. Tarqeq58. S/2007 S259. S/2007 S360. Anthe

BACK


Relative position: 7th planet out from the sun. Appearance: It has a blue-green color from the

methane gas above the deeper clouds. Methane absorbs red light and reflects blue light. It does have a small system of rings.

General composition: It is a Gas giant, meaning it is mostly made of the gases hydrogen and helium, with a small amount of methane and traces of water and ammonia. It has no solid surface, but it does contain a liquid core made mostly of “icy” materials (water, methane, and ammonia)


Atmosphere: Mostly hydrogen, helium, and methane.

Size: 52 times the volume of the Earth.Planetary satellites (Moons): 27 MoonsRotation: 17 hours, 11 minutesRevolution: 84.02 Earth yearsTemperature: -197 °C

Uranus (Planet)

Links to Uranus sites:•Exploring the Planets - Uranus•Missions to Uranus•StarDate: Uranus

Special feature: Uranus’ axis is tilted so that it seems to rotate on its side. This tilt gives it seasons that last over twenty years.


http://www.nasm.edu/ceps/etp/uranus/

http://solarsystem.nasa.gov/missions/profile.cfm?Object=Uranus

http://stardate.org/resources/ssguide/uranus.html

Moons of Uranus

BACK

1. Cordelia2. Ophelia3. Bianca4. Cressida5. Desdemona6. Juliet7. Portia8. Rosalind9. Mab10. Belinda11. Perdita12. Puck13. Cupid14. Miranda

15. Francisco16. Ariel17. Umbriel18. Titania19. Oberon20. Caliban21. Stephano22. Trinculo23. Sycorax24. Margaret25. Prospero26. Setebos27. Ferdinand


Neptune (Planet)Relative position: 8th planet out from the sun. Appearance: Neptune has a blue color because of the

methane in its atmosphere. The methane reflects blue light while it absorbs red light. It has a small system of rings and periodically Great Dark Spots (hurricane-like storms) appear.

General composition: It is a Gas giant, meaning it is mostly made of the gases hydrogen, helium, and methane. It has no solid surface, but its liquid core is composed of water and other “melted ices.”


Atmosphere: Mostly hydrogen, helium,and methane.Size: 44 times the volume of the Earth.Planetary satellites (Moons): 13 MoonsRotation: 16 hours, 4 minutesRevolution: 164.79 Earth yearsTemperature: -200 °C

Links to Neptune sites:•Exploring the Planets - Neptune•Missions to Neptune•StarDate: Neptune

Special features: Neptune is actually the farthest planet from the Sun for a 20-year period out of every 248 Earth years due to Pluto’s unusual elliptical orbit.


http://www.nasm.edu/ceps/etp/neptune/

http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Neptune

http://stardate.org/resources/ssguide/neptune.html

Moons of Neptune

BACK

1. Triton2. Nereid3. Naiad4. Thalassa5. Despina6. Galatea7. Larissa8. Proteus9. Halimede10. Psamathe11. Sao12. Laomedeia13. Neso


Pluto (Dwarf Planet)Charon

Relative position: 9th planet out from the sun. Appearance: A large frozen ball of ice.General composition: Rocky core surrounded by

water ice.Density: 2.0 gm/cm3

Atmosphere: Frozen most of the time. When it is closest to the Sun the bright layer of frozen methane, nitrogen, and carbon monoxide thaws out and gives it a thin atmosphere.

Size: .005 the volume of the Earth. It is the planet with the lowest gravity in the solar system.

Planetary satellites (Moons): 31. Charon2. Hydra3. Nix

Rotation: -6.39 days (retrograde)Revolution: 247.9 Earth yearsTemperature: -233 °C

Links to Pluto sites:•Missions to Pluto•Pluto Portal•StarDate: Pluto


http://solarsystem.nasa.gov/missions/profile.cfm?Mission=PKB

http://www.plutoportal.net/

http://stardate.org/resources/ssguide/pluto.html

• Asteroids are either rocky or metallic objects that orbit the Sun. They are too small to considered planets but are sometimes called planetoids.

• They can be anywhere from the size of a pebble up to a 1000km (620 miles) in diameter; the asteroid Ceres is an example of an asteroid that is this large.

• They have been found inside Earth’s orbit and all the way out past Saturn’s orbit. Most asteroids, however, are located in the asteroid belt which exists between the orbit’s of Mars and Jupiter.

Asteroids

Links to Asteroids sites:•Missions to Asteroids•The Nine Planets: Asteroids•StarDate: Asteroids


http://solarsystem.nasa.gov/missions/profile.cfm?Object=Asteroids

http://www.seds.org/nineplanets/nineplanets/asteroids.html

http://stardate.org/resources/ssguide/asteroids.html

Asteroid Belt

BACK


• Comets - small, fragile, irregular-shaped body composed of a mixture of non-volatile grains and frozen gases. Components of Comets can be seen by clicking on the link.

• Their orbits are elliptical (oval) or parabolic (U-shaped). The orbit brings them in very close to the Sun and swings them far out into space, sometimes out past Pluto. Example of a comet’s orbit.

• As comets approach the Sun, radiation from the Sun evaporates the ice and gases, creating the lone tail. The closer to the Sun, the longer the tail of the comet. The tail of the comet always faces away from the Sun because of the solar wind coming from the Sun.

Comets

Links to Comet sites:•Asteroid and Comet Impact Hazards•The Planetary Society’s Near Earth Objects Page•Missions to Comets


http://impact.arc.nasa.gov/index.html

http://neo.planetary.org/

http://solarsystem.nasa.gov/missions/profile.cfm?Sort=Planet&Object=Comets

Components of Comets

BACK


Example of a Comet’s OrbitComet 2P/Encke

BACK


Meteors, Meteoroids, and Meteorites

• Meteoroids - asteroids that are on a collision course with Earth.

• Meteor - streak of light created when a meteoroid strikes our atmosphere at high velocity and friction causes the chunk of space matter to burn up.

• Meteorite - what is left that strikes the Earth’s surface if the meteoroid does not burn up completely.

• 92.8% of all meteorites are composed of silicate (stone), and 5.7% are composed of iron and nickel; the rest are a mixture of the three materials.

• Stony meteorites are the hardest to identify since they look very much like terrestrial rocks.

Meteorite sample that is from the crust of the asteroid Vesta

Links to meteorite sites:•ANSMET: Antarctic Search for Meteorites•Asteroids, Comets, and NASA Research•Meteorites from Antarctica•Meteorites from Mars


http://www.cwru.edu/affil/ansmet/index.html

http://www.hq.nasa.gov/office/pao/facts/HTML/FS-023-HQ.html

http://www-curator.jsc.nasa.gov/curator/antmet/antmet.htm

http://www-curator.jsc.nasa.gov/curator/antmet/marsmets/contents.htm

1. Greenhouse Effect - warming of a planet’s surface as a result of atmospheric gases trapping heat. Carbon dioxide is one of these greenhouse gases.

2. Photon - a quantum of visible light or other form of electromagnetic radiation coming from the Sun. A particle of light.

3. Retrograde - this means that the planet is spinning backwards compared to the other planets.

4. Revolution - one complete circle made around something. The orbit made by a planet or satellite around another body.

5. Rotation - the turning motion of a planet spinning on its axis.

6. Star - a glowing, hot, gaseous mass in space such as the Sun ranging in size from that of a planet to larger than the Earth’s orbit. It generates energy by thermonuclear reactions.

7. Terrestrial - similar in composition and density to Earth. Relating to Earth. Earth-like.

8. Volume - amount of space an object takes up.

Vocabulary

BACK


9. Dwarf Planet - a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, (c) has not cleared the neighborhood around its orbit, and (d) is not a satellite.

10. Planet - a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape and (c) has cleared the neighborhood around its orbit.

11. Plutoids - celestial bodies in orbit around the Sun at a semi-major axis greater than that of Neptune that have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (near-spherical) shape, and that have not cleared the neighborhood around their orbit.

Vocabulary (p.2)

BACK


a tour of the solar system

Documents