the outer planets - J. Seguin Science
... __Hydrogen___. For this reason, they are called the gas ___Giants__. The gas giants appear to lack _solid_ surfaces, however, as the gases become more dense, eventually becoming _liquid__ and __solid_. The outermost planet __pluto__ is unique among the outer planets. JUPITER Jupiter is the __largest ...
... __Hydrogen___. For this reason, they are called the gas ___Giants__. The gas giants appear to lack _solid_ surfaces, however, as the gases become more dense, eventually becoming _liquid__ and __solid_. The outermost planet __pluto__ is unique among the outer planets. JUPITER Jupiter is the __largest ...
Jupiter - QZAB Teachers
... • Asteroids- many small celestial bodies that revolve around the Sun with orbits in between Mars and Jupiter and characteristic diameters between a few and several hundred kilometers. They are also called minor planet ...
... • Asteroids- many small celestial bodies that revolve around the Sun with orbits in between Mars and Jupiter and characteristic diameters between a few and several hundred kilometers. They are also called minor planet ...
Jupiter is 90000 miles in diameter. It is 10 times the size of the earth
... The atmosphere appears as alternating bands of light regions, called zones, and dark regions called belts, that run parallel to the equator. The zones are higher in altitude than the belts, and are lower in temperature. It is believed that the belts represent descending areas of low pressure. Jupi ...
... The atmosphere appears as alternating bands of light regions, called zones, and dark regions called belts, that run parallel to the equator. The zones are higher in altitude than the belts, and are lower in temperature. It is believed that the belts represent descending areas of low pressure. Jupi ...
Planet Walk Activity
... 1) Measure the distance from the “Sun” to the #4 position of Mars, Jupiter, and Saturn. Plot and label their positions on the grid. (Each floor tile is 1 foot by 1 foot) 2) Plot and label the #2 and #6 positions of Earth on the grid, as well. 3) Draw lines from the #2 position of Earth through each ...
... 1) Measure the distance from the “Sun” to the #4 position of Mars, Jupiter, and Saturn. Plot and label their positions on the grid. (Each floor tile is 1 foot by 1 foot) 2) Plot and label the #2 and #6 positions of Earth on the grid, as well. 3) Draw lines from the #2 position of Earth through each ...
Stratigraphy and composition of lava flows in Mare Nubium
... The discovery that an object other than Earth had satellites, or moons, was an amazing revelation. It proved that our world was not the centre of all motion in the Universe, and provided support for the view that Earth and the other planets orbited the Sun. ...
... The discovery that an object other than Earth had satellites, or moons, was an amazing revelation. It proved that our world was not the centre of all motion in the Universe, and provided support for the view that Earth and the other planets orbited the Sun. ...
Exploring the Universe, Test #3, Summer 97
... d) the maximum distance a spacecraft can be sent from Earth 27. Cassini’s division is a) a new form of math b) imaginary line which divides a planet into Eastern and Western hemispheres c) a gap in Saturn’s rings d) the space between Mars and Jupiter where there is no planet 28. The many ringlets w ...
... d) the maximum distance a spacecraft can be sent from Earth 27. Cassini’s division is a) a new form of math b) imaginary line which divides a planet into Eastern and Western hemispheres c) a gap in Saturn’s rings d) the space between Mars and Jupiter where there is no planet 28. The many ringlets w ...
Mid-term Exam 3 - Practice Version
... They formed from the atmosphere of the Sun. They migrated inward after forming far from the Sun in the outer Solar System. They formed inside the radius at which ice mantles could not exist on dust grains. Ice grains are limited to highly eccentric and highly inclined orbits. Dust grains only exist ...
... They formed from the atmosphere of the Sun. They migrated inward after forming far from the Sun in the outer Solar System. They formed inside the radius at which ice mantles could not exist on dust grains. Ice grains are limited to highly eccentric and highly inclined orbits. Dust grains only exist ...
Jupiter Reading Comprehension Worksheet
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
File - Homeschooling Mommie
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
ADDITIONAL NOTES THE JOVIAN PLANETS AND SOME OF
... to its orbital plan. The ring system and many of its satellites orbit around its equator. ...
... to its orbital plan. The ring system and many of its satellites orbit around its equator. ...
Section 22.3: Space Probes
... Sampled solar wind: the flow of particles coming from the sun Pioneer 10 (1983) because the first to travel past Pluto ...
... Sampled solar wind: the flow of particles coming from the sun Pioneer 10 (1983) because the first to travel past Pluto ...
Saturn - Otterbein University
... diameters >2500 km, largest: 5260 km • Medium moons: diameter 400-1600 km e.g. all of Uranus’ major moons ...
... diameters >2500 km, largest: 5260 km • Medium moons: diameter 400-1600 km e.g. all of Uranus’ major moons ...
Outer Planet review Much of what we know about the outer planets
... 4) How does the composition of outer planets differ from that of the inner planets? 5) What are the names of Jupiter’s (large) moons? 6) What are incomplete planetary rings, similar to those around Neptune, called? 7) Where does Jupiter’s name come from? 8) Who first proposed the presence of Neptune ...
... 4) How does the composition of outer planets differ from that of the inner planets? 5) What are the names of Jupiter’s (large) moons? 6) What are incomplete planetary rings, similar to those around Neptune, called? 7) Where does Jupiter’s name come from? 8) Who first proposed the presence of Neptune ...
Saturn - Otterbein University
... diameters >2500 km, largest: 5260 km • Medium moons: diameter 400-1600 km e.g. all of Uranus’ major moons ...
... diameters >2500 km, largest: 5260 km • Medium moons: diameter 400-1600 km e.g. all of Uranus’ major moons ...
VOCABULARY: Roche Limit, Shephard Moon, Ring, Galilean Moon
... Satellites: Identify key properties and features of the following moons: Jupiter’s Galilean satellites: Io, Europa, Ganymede, Callisto Saturn: Titan Neptune: Triton Define Tidal Heating. Discuss which moons undergo tidal heating and why. Explain why tidal heating causes Io and Europa to be very diff ...
... Satellites: Identify key properties and features of the following moons: Jupiter’s Galilean satellites: Io, Europa, Ganymede, Callisto Saturn: Titan Neptune: Triton Define Tidal Heating. Discuss which moons undergo tidal heating and why. Explain why tidal heating causes Io and Europa to be very diff ...
Worlds of the Outer Solar System
... 1. The largest satellites of Jupiter are known as the ____ satellites. 2.Volcanism is apparent on many objects in the solar system. However, volcanic activity is known to be currently occurring only on Earth and 3.The one object in the solar system besides Earth suspected of currently having a liqui ...
... 1. The largest satellites of Jupiter are known as the ____ satellites. 2.Volcanism is apparent on many objects in the solar system. However, volcanic activity is known to be currently occurring only on Earth and 3.The one object in the solar system besides Earth suspected of currently having a liqui ...
The Planets - Giants video questions
... communicate with probes across billions of miles. 7) The asteroid belt is a belt of rocks between Mars and Jupiter. Voyager would have only one chance, so to less elaborate probes were sent ahead to test the way. Pioneer _____ and _____ were launched to Jupiter and Saturn. 8) Since the 1950’s radio ...
... communicate with probes across billions of miles. 7) The asteroid belt is a belt of rocks between Mars and Jupiter. Voyager would have only one chance, so to less elaborate probes were sent ahead to test the way. Pioneer _____ and _____ were launched to Jupiter and Saturn. 8) Since the 1950’s radio ...
The most important questions to study for the exam
... frozen surface, as deduced from ice-flow patterns on spacecraft images and their inferred movement. If so, what would be the source of heating that keeps this water from freezing? • Solar radiation, which at Jupiter's orbital distance is easily capable of melting ice. • Tidal distortion and stress c ...
... frozen surface, as deduced from ice-flow patterns on spacecraft images and their inferred movement. If so, what would be the source of heating that keeps this water from freezing? • Solar radiation, which at Jupiter's orbital distance is easily capable of melting ice. • Tidal distortion and stress c ...
Jupiter
... beneath an icy crust several kilometers thick. More surprising was the discovery in October, 1998, that another Jovian moon, Callisto, may also have a hidden salty sea. Callisto was previously thought to be a solid sphere of rock and ice. A liquid ocean on Callisto, however, seems to be the only exp ...
... beneath an icy crust several kilometers thick. More surprising was the discovery in October, 1998, that another Jovian moon, Callisto, may also have a hidden salty sea. Callisto was previously thought to be a solid sphere of rock and ice. A liquid ocean on Callisto, however, seems to be the only exp ...
1. Which of the following statements does not describe Jupiter? A. It
... A. It is the largest planet in the solar system. B. It has a stormy atmosphere. C. It emits radio waves. D. Jupiter and its Galilean satellites resemble a miniature solar system. E. All of them correctly describe Jupiter. 2. The most massive jovian planet is A. Jupiter. B. Saturn. C. Uranus. D. Plut ...
... A. It is the largest planet in the solar system. B. It has a stormy atmosphere. C. It emits radio waves. D. Jupiter and its Galilean satellites resemble a miniature solar system. E. All of them correctly describe Jupiter. 2. The most massive jovian planet is A. Jupiter. B. Saturn. C. Uranus. D. Plut ...
Exploration of Io
The exploration of Io, Jupiter's third-largest moon, began with its discovery in 1610 and continues today with Earth-based observations and visits by spacecraft to the Jupiter system. Italian astronomer Galileo Galilei was the first to record an observation of Io on January 8, 1610, though Simon Marius may have also observed Io at around the same time. During the 17th century, observations of Io and the other Galilean satellites helped with the measurement of longitude by map makers and surveyors, with validation of Kepler's Third Law of planetary motion, and with measurement of the speed of light. Based on ephemerides produced by astronomer Giovanni Cassini and others, Pierre-Simon Laplace created a mathematical theory to explain the resonant orbits of three of Jupiter's moons, Io, Europa, and Ganymede. This resonance was later found to have a profound effect on the geologies of these moons. Improved telescope technology in the late 19th and 20th centuries allowed astronomers to resolve large-scale surface features on Io as well as to estimate its diameter and mass.The advent of unmanned spaceflight in the 1950s and 1960s provided an opportunity to observe Io up-close. In the 1960s the moon's effect on Jupiter's magnetic field was discovered. The flybys of the two Pioneer probes, Pioneer 10 and 11 in 1973 and 1974, provided the first accurate measurement of Io's mass and size. Data from the Pioneers also revealed an intense belt of radiation near Io and suggested the presence of an atmosphere. In 1979, the two Voyager spacecraft flew through the Jupiter system. Voyager 1, during its encounter in March 1979, observed active volcanism on Io for the first time and mapped its surface in great detail, particularly the side that faces Jupiter. The Voyagers observed the Io plasma torus and Io's sulfur dioxide (SO2) atmosphere for the first time. NASA launched the Galileo spacecraft in 1989, which entered Jupiter's orbit in December 1995. Galileo allowed detailed study of both the planet and its satellites, including six flybys of Io between late 1999 and early 2002 that provided high-resolution images and spectra of Io's surface, confirming the presence of high-temperature silicate volcanism on Io. Distant observations by Galileo allowed planetary scientists to study changes on the surface that resulted from the moon's active volcanism.Following Galileo and a distant encounter by the Pluto-bound New Horizons spacecraft in 2007, NASA and the European Space Agency (ESA) made plans to return to the Jupiter system and Io. In 2009, NASA approved a plan to send an orbiter to Europa called the Jupiter Europa Orbiter as part of a joint program with ESA called the Europa/Jupiter System Mission. The ESA component of the project was the Jupiter Ganymede Orbiter. However, the EJSM mission collaboration was cancelled. ESA is continuing with its initiative under the name Jupiter Icy Moon Explorer (JUICE) to explore Ganymede, Europa, and Callisto, without plans to investigate Io at all. The proposed NASA Discovery mission Io Volcano Observer, currently going through a competitive process to be selected, would explore Io as its primary mission. In the meantime, Io continues to be observed by the Hubble Space Telescope as well as by Earth-based astronomers using improved telescopes such as Keck and the European Southern Observatory, that use new technologies such as adaptive optics.