can you planet? - Moore Public Schools
... result of information gathered by Voyagers 1 and 2. Students should be encouraged to look for articles that continue to report on new information about our solar system. An excellent web site for current information is http://nineplanets.org All information included was correct at the time of printi ...
... result of information gathered by Voyagers 1 and 2. Students should be encouraged to look for articles that continue to report on new information about our solar system. An excellent web site for current information is http://nineplanets.org All information included was correct at the time of printi ...
Neptune - SUSD Student Community
... system was found to contain several faint rings, the outermost of which, Adams, contains three prominent arcs now named Liberty, Equality and Fraternity. The existence of arcs is very difficult to understand because the laws of motion would predict that arcs spread out into a uniform ring over very ...
... system was found to contain several faint rings, the outermost of which, Adams, contains three prominent arcs now named Liberty, Equality and Fraternity. The existence of arcs is very difficult to understand because the laws of motion would predict that arcs spread out into a uniform ring over very ...
Dwarf Planets
... A. The Discovery of Uranus B. The Motion of Uranus C. The Atmosphere of Uranus D. The Interior of Uranus E. The Rings of Uranus F. The Moons of Uranus G. A History of Uranus II. Neptune A. The Discovery of Neptune B. The Atmosphere and Interior of Neptune C. The Rings of Neptune D. The Moons of Nept ...
... A. The Discovery of Uranus B. The Motion of Uranus C. The Atmosphere of Uranus D. The Interior of Uranus E. The Rings of Uranus F. The Moons of Uranus G. A History of Uranus II. Neptune A. The Discovery of Neptune B. The Atmosphere and Interior of Neptune C. The Rings of Neptune D. The Moons of Nept ...
Chapter 24: Uranus, Neptune, and the Dwarf - Otto
... A. The Discovery of Uranus B. The Motion of Uranus C. The Atmosphere of Uranus D. The Interior of Uranus E. The Rings of Uranus F. The Moons of Uranus G. A History of Uranus II. Neptune A. The Discovery of Neptune B. The Atmosphere and Interior of Neptune C. The Rings of Neptune D. The Moons of Nept ...
... A. The Discovery of Uranus B. The Motion of Uranus C. The Atmosphere of Uranus D. The Interior of Uranus E. The Rings of Uranus F. The Moons of Uranus G. A History of Uranus II. Neptune A. The Discovery of Neptune B. The Atmosphere and Interior of Neptune C. The Rings of Neptune D. The Moons of Nept ...
asteroid
... The size of asteroids is estimated by the amount of light reflected and the amount of heat radiated. Rare stellar occultations aid in determining size. ...
... The size of asteroids is estimated by the amount of light reflected and the amount of heat radiated. Rare stellar occultations aid in determining size. ...
Planetary Rings
... probes. These structures appear to arise from gravitational interactions between ring particles and Saturn’s many small moons and, electromagnetic forces experienced by small ice and dust particles. However, planetary scientists are still struggling to explain many of these phenomena. ...
... probes. These structures appear to arise from gravitational interactions between ring particles and Saturn’s many small moons and, electromagnetic forces experienced by small ice and dust particles. However, planetary scientists are still struggling to explain many of these phenomena. ...
Jupiter: Cosmic Jekyll and Hyde - Mary Ann Liebert, Inc. publishers
... objects already on Earth-crossing trajectories. The study by Wetherill (1994) contains only one reference that might be interpreted to mean that Jupiter has a role in shielding the inner Solar System in this manner. In regard to simulations where the jovian planets had acquired masses significantly ...
... objects already on Earth-crossing trajectories. The study by Wetherill (1994) contains only one reference that might be interpreted to mean that Jupiter has a role in shielding the inner Solar System in this manner. In regard to simulations where the jovian planets had acquired masses significantly ...
Power Point Presentation
... (Galileo): Io, Europa Ganymede and Callisto Spacecraft exploration since 1973, Galileo is still in orbit around Jupiter Liquid metallic hydrogen mantle Possible hot, rocky core High velocity winds driven by internal heat ...
... (Galileo): Io, Europa Ganymede and Callisto Spacecraft exploration since 1973, Galileo is still in orbit around Jupiter Liquid metallic hydrogen mantle Possible hot, rocky core High velocity winds driven by internal heat ...
Planetary Rings - Physics and Astronomy
... Ganymede is the largest moon in the solar system – larger than Pluto and Mercury. It has a history similar to Earth’s Moon, but with water ice instead of lunar rock. ...
... Ganymede is the largest moon in the solar system – larger than Pluto and Mercury. It has a history similar to Earth’s Moon, but with water ice instead of lunar rock. ...
Chapter 29
... • Has 63 moons, at last count. Jupiter’s four largest moons, Io, Europa, Ganymede, and Callisto, are called Galilean satellites. Three of these are larger than our moon and all are larger than Pluto! • There is volcanic activity on Jupiter’s closest major moon, Io. – Europa is believed to possibly h ...
... • Has 63 moons, at last count. Jupiter’s four largest moons, Io, Europa, Ganymede, and Callisto, are called Galilean satellites. Three of these are larger than our moon and all are larger than Pluto! • There is volcanic activity on Jupiter’s closest major moon, Io. – Europa is believed to possibly h ...
workbook - teacher version
... NOTE: It takes Earth one year to revolve completely around the Sun, and it takes Jupiter 12 years because it is much farther from the Sun (see previous question). Since Earth and Jupiter are on opposite sides of the Sun in the diagram, it will take less than a year for Earth to catch up and pass Jup ...
... NOTE: It takes Earth one year to revolve completely around the Sun, and it takes Jupiter 12 years because it is much farther from the Sun (see previous question). Since Earth and Jupiter are on opposite sides of the Sun in the diagram, it will take less than a year for Earth to catch up and pass Jup ...
Models
... Use a ruler to measure the diameter of each object then draw a circle around the diameter to show the scale size of the planet. Color the planet to look like the planet Add at least one fact about the planet. ...
... Use a ruler to measure the diameter of each object then draw a circle around the diameter to show the scale size of the planet. Color the planet to look like the planet Add at least one fact about the planet. ...
Pluto
... Objects might also harbor multiple satellites and raises the possibility that Pluto is encircled by rings fashioned from debris ejected from the surface of the tiny moons. ...
... Objects might also harbor multiple satellites and raises the possibility that Pluto is encircled by rings fashioned from debris ejected from the surface of the tiny moons. ...
Outer Planets Lab
... dictated by the atmospheric levels at which various gases can condense into liquid droplets or solid flakes. ...
... dictated by the atmospheric levels at which various gases can condense into liquid droplets or solid flakes. ...
The Asteroid Belt
... Belt between about 2.1 and 4.1 AU. The majority of main belt asteroids follow slightly elliptical stable orbits, orbiting the Sun in the same direction as the Earth. Typically the orbital periods of these asteroids range from 3 to 8 years. There are also a few special resonances where asteroids like ...
... Belt between about 2.1 and 4.1 AU. The majority of main belt asteroids follow slightly elliptical stable orbits, orbiting the Sun in the same direction as the Earth. Typically the orbital periods of these asteroids range from 3 to 8 years. There are also a few special resonances where asteroids like ...
The Planets
... Features of Saturn • Saturn’s atmosphere is very active, with winds roaring at up to 1500 kilometers per hour. • Large cyclonic “storms” similar to Jupiter’s Great Red Spot, although smaller, occur in Saturn’s atmosphere. ...
... Features of Saturn • Saturn’s atmosphere is very active, with winds roaring at up to 1500 kilometers per hour. • Large cyclonic “storms” similar to Jupiter’s Great Red Spot, although smaller, occur in Saturn’s atmosphere. ...
The Cosmic Perspective Our Planetary System
... Why do orbiters typically cost more than flyby missions? a) They typically carry more scientific instruments. b) They need expensive protection from the charged particles in a planet's magnetosphere. c) They must carry extra fuel so that they can go into orbit. d) They require more powerful radi ...
... Why do orbiters typically cost more than flyby missions? a) They typically carry more scientific instruments. b) They need expensive protection from the charged particles in a planet's magnetosphere. c) They must carry extra fuel so that they can go into orbit. d) They require more powerful radi ...
*Do you know why the Outer Planets are called the “Gassy Giants
... Now that you have looked at each of the planets, did you notice any common characteristics among the outer planets? Here are some things that you should know: —The outer planets are all large, and they are made of gas which is why they are called the “Gassy Giants.” —The outer planets all have rings ...
... Now that you have looked at each of the planets, did you notice any common characteristics among the outer planets? Here are some things that you should know: —The outer planets are all large, and they are made of gas which is why they are called the “Gassy Giants.” —The outer planets all have rings ...
File - IGS Intro Materials
... The Voyager Probes and Galileo • In 1979, Voyager1 and Voyager 2 flew past Jupiter, and the Galileo space probe reached Jupiter in 1995. • The major discoveries of these probes include information about the composition and motion of Jupiter’s atmosphere, characteristics of some of its moons and the ...
... The Voyager Probes and Galileo • In 1979, Voyager1 and Voyager 2 flew past Jupiter, and the Galileo space probe reached Jupiter in 1995. • The major discoveries of these probes include information about the composition and motion of Jupiter’s atmosphere, characteristics of some of its moons and the ...
Lining Up the Planets - Math-4326
... 2. Divide the class into teams of four. 3. Explain that each team member will have a card that he or she reads to the group. Other team members are not to read each other’s cards, but they are to practice listening and then apply what they hear. 4. Have the students use the scaled planet drawings to ...
... 2. Divide the class into teams of four. 3. Explain that each team member will have a card that he or she reads to the group. Other team members are not to read each other’s cards, but they are to practice listening and then apply what they hear. 4. Have the students use the scaled planet drawings to ...
Making the Cards - Teaching Made Practical
... gas giant and does not have a solid surface. One of Jupiter’s most well known features is the Great Red Spot, a huge storm that has been raging for at least 300 years. ...
... gas giant and does not have a solid surface. One of Jupiter’s most well known features is the Great Red Spot, a huge storm that has been raging for at least 300 years. ...
Student`s guide - Cosmos
... that the students will have to realize about that phenomenon and understand the reason why it is produced. As an inner planet, Venus passes in front of the Sun but and behind it viewed from Earth. As consequence when Venus is closest to the Earth, the Sun, Venus and the Earth are all aligned on the ...
... that the students will have to realize about that phenomenon and understand the reason why it is produced. As an inner planet, Venus passes in front of the Sun but and behind it viewed from Earth. As consequence when Venus is closest to the Earth, the Sun, Venus and the Earth are all aligned on the ...
Student`s guide - Cosmos
... that the students will have to realize about that phenomenon and understand the reason why it is produced. As an inner planet, Venus passes in front of the Sun but and behind it viewed from Earth. As consequence when Venus is closest to the Earth, the Sun, Venus and the Earth are all aligned on the ...
... that the students will have to realize about that phenomenon and understand the reason why it is produced. As an inner planet, Venus passes in front of the Sun but and behind it viewed from Earth. As consequence when Venus is closest to the Earth, the Sun, Venus and the Earth are all aligned on the ...
Webquest – Answer Key
... 15. List the 2 planet that have the greatest density? Earth and Mercury. Are they inner or outer planets? inner. 16. Why are the outer planets less dense than the inner planets? The outer planets are less dense because they don't have water on them and the rocky planets tend to have more water. Also ...
... 15. List the 2 planet that have the greatest density? Earth and Mercury. Are they inner or outer planets? inner. 16. Why are the outer planets less dense than the inner planets? The outer planets are less dense because they don't have water on them and the rocky planets tend to have more water. Also ...
Exploration of Jupiter
The exploration of Jupiter has been conducted via close observations by automated spacecraft. It began with the arrival of Pioneer 10 into the Jovian system in 1973, and, as of 2014, has continued with seven further spacecraft missions. All of these missions were undertaken by the National Aeronautics and Space Administration (NASA), and all but one have been flybys that take detailed observations without the probe landing or entering orbit. These probes make Jupiter the most visited of the Solar System's outer planets as all missions to the outer Solar System have used Jupiter flybys to reduce fuel requirements and travel time. Plans for more missions to the Jovian system are under development, none of which are scheduled to arrive at the planet before 2016. Sending a craft to Jupiter entails many technical difficulties, especially due to the probes' large fuel requirements and the effects of the planet's harsh radiation environment.The first spacecraft to visit Jupiter was Pioneer 10 in 1973, followed a year later by Pioneer 11. Aside from taking the first close-up pictures of the planet, the probes discovered its magnetosphere and its largely fluid interior. The Voyager 1 and Voyager 2 probes visited the planet in 1979, and studied its moons and the ring system, discovering the volcanic activity of Io and the presence of water ice on the surface of Europa. Ulysses further studied Jupiter's magnetosphere in 1992 and then again in 2000. The Cassini probe approached the planet in 2000 and took very detailed images of its atmosphere. The New Horizons spacecraft passed by Jupiter in 2007 and made improved measurements of its and its satellites' parameters.The Galileo spacecraft is the only one to have entered orbit around Jupiter, arriving in 1995 and studying the planet until 2003. During this period Galileo gathered a large amount of information about the Jovian system, making close approaches to all of the four large Galilean moons and finding evidence for thin atmospheres on three of them, as well as the possibility of liquid water beneath their surfaces. It also discovered a magnetic field around Ganymede. As it approached Jupiter, it also witnessed the impact of Comet Shoemaker–Levy 9. In December 1995, it sent an atmospheric probe into the Jovian atmosphere, so far the only craft to do so.Future probes planned by NASA include the Juno spacecraft, launched in 2011, which will enter a polar orbit around Jupiter to determine whether it has a rocky core. The European Space Agency selected the L1-class JUICE mission in 2012 as part of its Cosmic Vision programme to explore three of Jupiter's Galilean moons, with a possible Ganymede lander provided by Roscosmos. JUICE is proposed to be launched in 2022. Some NASA administrators have even speculated as to the possibility of human exploration of Jupiter, but such missions are not considered feasible with current technology; such as radiation protection.