a huge lake of hot liquid rock beneath the surface. This boiling hot
... Where is the lake of hot liquid rock? a. sixty miles beneath the surface b. in Canada c, beneath the rock crust in Yellowstone d, above the rock crust inYellowstone Where is the largest volcano in history located? ...
... Where is the lake of hot liquid rock? a. sixty miles beneath the surface b. in Canada c, beneath the rock crust in Yellowstone d, above the rock crust inYellowstone Where is the largest volcano in history located? ...
Universal gravitation
... 5. Fill in the last column of the data table. 6. What do you notice about the values in the last column? What law is this? 7. Use the graphing capabilities of your TI calculator to plot T 2 vs. R3 (T2 should be plotted along the vertical axis) and to determine the equation of the line. Write the equ ...
... 5. Fill in the last column of the data table. 6. What do you notice about the values in the last column? What law is this? 7. Use the graphing capabilities of your TI calculator to plot T 2 vs. R3 (T2 should be plotted along the vertical axis) and to determine the equation of the line. Write the equ ...
astron_ch_13b
... are slightly higher in the atmosphere than the belts. Differences in temperature causes the differences in ...
... are slightly higher in the atmosphere than the belts. Differences in temperature causes the differences in ...
$doc.title
... For the geocentric case, sketch the expected phase of Venus at each of the six epochs shown in the diagram. Don’t worry about showing which “side” of the planet is bright -‐-‐ it will always ...
... For the geocentric case, sketch the expected phase of Venus at each of the six epochs shown in the diagram. Don’t worry about showing which “side” of the planet is bright -‐-‐ it will always ...
Solar System
... the fourth largest. It is slightly smaller than the Earth’s moon. The surface strongly resembles images of sea ice on Earth. There may be a liquid water sea under the crust. Europa is one of the five known moons in the solar system to have an atmosphere. ...
... the fourth largest. It is slightly smaller than the Earth’s moon. The surface strongly resembles images of sea ice on Earth. There may be a liquid water sea under the crust. Europa is one of the five known moons in the solar system to have an atmosphere. ...
Earth Science
... the fourth largest. It is slightly smaller than the Earth’s moon. The surface strongly resembles images of sea ice on Earth. There may be a liquid water sea under the crust. Europa is one of the five known moons in the solar system to have an atmosphere. ...
... the fourth largest. It is slightly smaller than the Earth’s moon. The surface strongly resembles images of sea ice on Earth. There may be a liquid water sea under the crust. Europa is one of the five known moons in the solar system to have an atmosphere. ...
Earth Science - MrsHeatonsWiki
... resembles images of sea ice on Earth. There may be a liquid water sea under the crust. Europa is one of the five known moons in the solar system to have an atmosphere. ...
... resembles images of sea ice on Earth. There may be a liquid water sea under the crust. Europa is one of the five known moons in the solar system to have an atmosphere. ...
Europa`s structure
... Io has a thin, SO2 atmosphere. Some freezes out on the night side and ices evaporate on the day side. Jupiter's magnetic field sweeps material off of Io and into a doughnut-shaped cloud of intense radiation. ...
... Io has a thin, SO2 atmosphere. Some freezes out on the night side and ices evaporate on the day side. Jupiter's magnetic field sweeps material off of Io and into a doughnut-shaped cloud of intense radiation. ...
A Brief History of Planetary Science
... The six large moons of the gas giants resemble the terrestrial planets of the inner solar system They can have volcanoes, atmospheres, and evidence of resurfacing ...
... The six large moons of the gas giants resemble the terrestrial planets of the inner solar system They can have volcanoes, atmospheres, and evidence of resurfacing ...
Document
... What was significant about Galileo's discovery of Jupiter's four brightest satellites? A. It showed that theories that a planet can only have one satellite are wrong. B. It showed that there are some objects which do not orbit the Earth. C. It showed that some satellites have ...
... What was significant about Galileo's discovery of Jupiter's four brightest satellites? A. It showed that theories that a planet can only have one satellite are wrong. B. It showed that there are some objects which do not orbit the Earth. C. It showed that some satellites have ...
A Brief History of Planetary Science
... c) Near the orbit of Mercury d) A large, differentiated asteroid that got broken up e) The collision that made the Moon ...
... c) Near the orbit of Mercury d) A large, differentiated asteroid that got broken up e) The collision that made the Moon ...
The Jovian Planets
... • Gaseous surface, liquid interior, solid core (like Jupiter) • Rings! • Many moons • Visited by Pioneer 11 (1979), Voyager 1 & 2 (1980-81); Cassini currently in orbit, 4-year mission ...
... • Gaseous surface, liquid interior, solid core (like Jupiter) • Rings! • Many moons • Visited by Pioneer 11 (1979), Voyager 1 & 2 (1980-81); Cassini currently in orbit, 4-year mission ...
Moons of Giant Planets
... the tidal bulge always has about the same size, because orbits of Earth and Moon are nearly circular. To get heating, the distance between Earth and Moon would have to be changing with time need more eccentric orbits However the pull of Earth’s bulge on the Moon slows the Earth and makes Moon mo ...
... the tidal bulge always has about the same size, because orbits of Earth and Moon are nearly circular. To get heating, the distance between Earth and Moon would have to be changing with time need more eccentric orbits However the pull of Earth’s bulge on the Moon slows the Earth and makes Moon mo ...
20gasgiantmoons2s
... The six large moons of the gas giants resemble the terrestrial planets of the inner solar system They can have volcanoes, atmospheres, and evidence of resurfacing ...
... The six large moons of the gas giants resemble the terrestrial planets of the inner solar system They can have volcanoes, atmospheres, and evidence of resurfacing ...
jupiter_ppt
... planet from the Sun Named after the father of Saturn Discovered in 1781. It was the first planet discovered in 2000 years. ...
... planet from the Sun Named after the father of Saturn Discovered in 1781. It was the first planet discovered in 2000 years. ...
The Voyagers opened a new frontier — the worlds of the outer solar
... flock of smaller icy moons. That was followed by bland-looking Uranus, a planet that rolls around the Sun on its side. It boasts a set of dark rings and its own collection of icy worlds. Voyager’s close flyby of Neptune showed storms in its upper atmosphere, and revealed the mottled surface of the u ...
... flock of smaller icy moons. That was followed by bland-looking Uranus, a planet that rolls around the Sun on its side. It boasts a set of dark rings and its own collection of icy worlds. Voyager’s close flyby of Neptune showed storms in its upper atmosphere, and revealed the mottled surface of the u ...
Kepler`s Laws Questions
... 5. The moon has a period of 27.3 days and has a mean distance of 3.9 x 105 km from the center of the Earth. Find the period of an artificial satellite that is 6.7 x 103 km from the center of the Earth. ...
... 5. The moon has a period of 27.3 days and has a mean distance of 3.9 x 105 km from the center of the Earth. Find the period of an artificial satellite that is 6.7 x 103 km from the center of the Earth. ...
Jupiter - Courseweb
... (4) A system is a collection of cycles, structures, and processes that interact. Students should understand a whole in terms of its components and how these components relate to each other and to the whole. All systems have basic properties that can be described in terms of space, time, energy, and ...
... (4) A system is a collection of cycles, structures, and processes that interact. Students should understand a whole in terms of its components and how these components relate to each other and to the whole. All systems have basic properties that can be described in terms of space, time, energy, and ...
Moon and Rings - Mid
... Would you expect Jupiter to be hotter or cooler very early in its history? What might this imply for the Jupiter-Galilean moon system? ...
... Would you expect Jupiter to be hotter or cooler very early in its history? What might this imply for the Jupiter-Galilean moon system? ...
Lobby Display Banners
... most spectacular results made by NASA and a number of other organizations dedicated to unlocking the secrets of Earth’s ...
... most spectacular results made by NASA and a number of other organizations dedicated to unlocking the secrets of Earth’s ...
Jupiter
... many orders of magnitude greater than is found on any other planet in the Solar System) • Infrared absorption bands caused by methane (CH4) (about 1 part per million in Earth's atmosphere), a gas which must be replenished by either volcanic or ...
... many orders of magnitude greater than is found on any other planet in the Solar System) • Infrared absorption bands caused by methane (CH4) (about 1 part per million in Earth's atmosphere), a gas which must be replenished by either volcanic or ...
Jupiter is the fifth planet from the sun. It is by far the
... scientist only knew of Saturn’s rings. Rings were seen on Uranus and Neptune as well. Both Voyager spacecraft have now left our solar system. They continue to fly outward through space. Who knows if they may make another unexpected discovery? ...
... scientist only knew of Saturn’s rings. Rings were seen on Uranus and Neptune as well. Both Voyager spacecraft have now left our solar system. They continue to fly outward through space. Who knows if they may make another unexpected discovery? ...
ppt
... similar to a class of asteroid Matches mixture of organic compounds from carbonaceous meteorites, ice and hydrated silicates ...
... similar to a class of asteroid Matches mixture of organic compounds from carbonaceous meteorites, ice and hydrated silicates ...
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.