![PDF format](http://s1.studyres.com/store/data/000178236_1-edf4a9214a8445554901fffe6a089c95-300x300.png)
PDF format
... b) Uranus and Neptune are mostly rocky while Jupiter and Saturn are mostly hydrogen and helium. c) Uranus and Neptune are mostly hydrogen and helium while Jupiter and Saturn are mostly hydrogen compounds. d) Uranus and Neptune are mostly hydrogen compounds while Jupiter and Saturn are mostly hydr ...
... b) Uranus and Neptune are mostly rocky while Jupiter and Saturn are mostly hydrogen and helium. c) Uranus and Neptune are mostly hydrogen and helium while Jupiter and Saturn are mostly hydrogen compounds. d) Uranus and Neptune are mostly hydrogen compounds while Jupiter and Saturn are mostly hydr ...
Structure of Mercury`s Interior
... surface temperatures high enough to melt lead. The atmosphere of Venus is made up mainly of carbon dioxide, and thick clouds of sulfuric acid completely cover the planet. The atmosphere traps the small amount of energy from the sun that does reach the surface along with the heat the planet itself re ...
... surface temperatures high enough to melt lead. The atmosphere of Venus is made up mainly of carbon dioxide, and thick clouds of sulfuric acid completely cover the planet. The atmosphere traps the small amount of energy from the sun that does reach the surface along with the heat the planet itself re ...
Ex3-Planets,F10
... significantly modified by the influence of wind, running water, ice, waves or gravity. One very important consideration in studying the history of a planetary surface is to determine the age of the surface under study. Impacts occurred at the greatest rate early in the history of the solar system, a ...
... significantly modified by the influence of wind, running water, ice, waves or gravity. One very important consideration in studying the history of a planetary surface is to determine the age of the surface under study. Impacts occurred at the greatest rate early in the history of the solar system, a ...
Moons, Pluto, and Rings - Wayne State University
... They were first seen by Galileo (the astronomer) Studied by the Galileo space probe and by Hubble Space Telescope The combined data about the moons has shown important similarities to the terrestrial planets The differences between the moons seem to be mostly due to distance from Jupiter ...
... They were first seen by Galileo (the astronomer) Studied by the Galileo space probe and by Hubble Space Telescope The combined data about the moons has shown important similarities to the terrestrial planets The differences between the moons seem to be mostly due to distance from Jupiter ...
ASTR 380 Possibilities for Life on the Moons of Giant Planets
... and atmosphere!!! energy: Very cold surface, sunlight there but weak liquid: evidence of liquid methane, water frozen solid stability: likely very stable for long period Chance for life? Can you do it with liquid methane? Argument can be made that it is not a good liquid for ...
... and atmosphere!!! energy: Very cold surface, sunlight there but weak liquid: evidence of liquid methane, water frozen solid stability: likely very stable for long period Chance for life? Can you do it with liquid methane? Argument can be made that it is not a good liquid for ...
Determination of meteor showers on other planets using comet
... about the possibility of meteor showers on other planets. It may be impractical for a skyobserver of the future to view meteor showers from some worlds: Mercury has no atmosphere, the clouds of Venus are so thick most meteors will likely burn up before a planetbound observer could see them, Jupiter ...
... about the possibility of meteor showers on other planets. It may be impractical for a skyobserver of the future to view meteor showers from some worlds: Mercury has no atmosphere, the clouds of Venus are so thick most meteors will likely burn up before a planetbound observer could see them, Jupiter ...
Dense (> 3000 kg/m 3 )
... categories of planets: terrestrial and Jovian 7-2 The similarities and differences among the large planetary satellites, including Earth’s Moon 7-3 How the spectrum of sunlight reflected from a planet reveals the composition of its atmosphere and surface 7-4 Why some planets have atmospheres and oth ...
... categories of planets: terrestrial and Jovian 7-2 The similarities and differences among the large planetary satellites, including Earth’s Moon 7-3 How the spectrum of sunlight reflected from a planet reveals the composition of its atmosphere and surface 7-4 Why some planets have atmospheres and oth ...
Chapter 12 (in pdf)
... through the atmosphere ( shooting star ) • Fireball: a very bright meteor • Meteorite: A rock from space that survives the Earth s atmosphere and is found on the ground. ...
... through the atmosphere ( shooting star ) • Fireball: a very bright meteor • Meteorite: A rock from space that survives the Earth s atmosphere and is found on the ground. ...
THE MAGNETIC ENVIRONMENT OF THE KNOWN RADIO PLANETS
... maximum value of cyclotron radio emission (43 MHz) observed from the polar regions, providing further confirmation of the validity of the planetary magnetic field model. More recently, radio emission studies using the Very Large Array (VLA) by a number of workers including DePater (1983) and Roberts ...
... maximum value of cyclotron radio emission (43 MHz) observed from the polar regions, providing further confirmation of the validity of the planetary magnetic field model. More recently, radio emission studies using the Very Large Array (VLA) by a number of workers including DePater (1983) and Roberts ...
07_Jovian planets
... Do your research • In assigned pairs, make a model for all the jovian planets. Use available materials. Your model must show or allow demonstration of: • Interior structure • Atmosphere and clouds • Rings • Magnetosphere • Weather • Differential rotation ...
... Do your research • In assigned pairs, make a model for all the jovian planets. Use available materials. Your model must show or allow demonstration of: • Interior structure • Atmosphere and clouds • Rings • Magnetosphere • Weather • Differential rotation ...
Uranus and Neptune
... • Thick, slushy mantle of water, ammonia, and methane ices • Rocky cores about the size of Earth • Both planets lack the deep metallic hydrogen mantles found on Jupiter and Saturn because of their smaller size (pressure doesn’t get large enough) ...
... • Thick, slushy mantle of water, ammonia, and methane ices • Rocky cores about the size of Earth • Both planets lack the deep metallic hydrogen mantles found on Jupiter and Saturn because of their smaller size (pressure doesn’t get large enough) ...
SOLAR SYSTEM - Heart of the Valley Astronomers
... The period of rotation at the poles is about 10 minutes less than that of the equator, while the interior rotates at an intermediate speed. ...
... The period of rotation at the poles is about 10 minutes less than that of the equator, while the interior rotates at an intermediate speed. ...
Document
... 8.2 The Large Moons of Saturn and Neptune Titan has been known for many years to have an atmosphere thicker and denser than Earth’s; mostly nitrogen and argon. Makes surface impossible to see; the picture at right was taken from only 4000 km away. ...
... 8.2 The Large Moons of Saturn and Neptune Titan has been known for many years to have an atmosphere thicker and denser than Earth’s; mostly nitrogen and argon. Makes surface impossible to see; the picture at right was taken from only 4000 km away. ...
Is the Solar System stable?
... expense - computer time is not cheap. The breakthrough came in 1981 when Jack Wisdom, then a PhD student at the California Institute of Technology, developed a new numerical method for studying the motion of asteroids at resonance. Wisdom [Another pertinent name! -LB] knew about chaotic dynamics, an ...
... expense - computer time is not cheap. The breakthrough came in 1981 when Jack Wisdom, then a PhD student at the California Institute of Technology, developed a new numerical method for studying the motion of asteroids at resonance. Wisdom [Another pertinent name! -LB] knew about chaotic dynamics, an ...
Life in the Universe
... • Ganymede does not have an atmosphere at Jupiter’s distance, only water ice could condense…, but at Saturn’s distance, ices such as methane and ammonia could condense! • Due to the stronger gravity of Jupiter, impacts were generally stronger at Jupiter’s moons than Saturn’s moon. Stronger impacts ...
... • Ganymede does not have an atmosphere at Jupiter’s distance, only water ice could condense…, but at Saturn’s distance, ices such as methane and ammonia could condense! • Due to the stronger gravity of Jupiter, impacts were generally stronger at Jupiter’s moons than Saturn’s moon. Stronger impacts ...
ANALYSIS OF SELF – GRAVITATING PLANETARY SATELLITES IN
... planetary satellites discovered in the Solar system, and the number of outer moons found continues to grow. Most of those natural satellites have insufficient mass and are able to retain their shape only due to the strength of the electromagnetic force. The purpose of this paper is to analyze the mo ...
... planetary satellites discovered in the Solar system, and the number of outer moons found continues to grow. Most of those natural satellites have insufficient mass and are able to retain their shape only due to the strength of the electromagnetic force. The purpose of this paper is to analyze the mo ...
Question 2 (9-3 thru 9-4 PPT Questions)
... these probes was used to guide scientists in decisions concerning probes that followed. 2. Saturn’s magnetic field is only 5% as strong as Jupiter’s because Saturn’s liquid metallic hydrogen only extends about half way to its cloud tops. 3. As for the case of Jupiter, Saturn’s interior structure is ...
... these probes was used to guide scientists in decisions concerning probes that followed. 2. Saturn’s magnetic field is only 5% as strong as Jupiter’s because Saturn’s liquid metallic hydrogen only extends about half way to its cloud tops. 3. As for the case of Jupiter, Saturn’s interior structure is ...
Planetary Satellites,Asteroids,Comets
... small (below 20 km) moons identified by astronomers using large ground-based telescopes. It is anticipated, however, that the number could well treble over the next decade, as more distant moons ranging down to about 1 km in size are found. These small satellites are actually asteroids and comets th ...
... small (below 20 km) moons identified by astronomers using large ground-based telescopes. It is anticipated, however, that the number could well treble over the next decade, as more distant moons ranging down to about 1 km in size are found. These small satellites are actually asteroids and comets th ...
ASTR 330: The Solar System
... • In the simplest form of the model, material ‘falling’ inwards in a gravitational field releases energy, which becomes heat (imagine a large asteroid impacting the Earth). • However, this simple theory, where the whole planet gradually contracts, does not account for the present-day energy source: ...
... • In the simplest form of the model, material ‘falling’ inwards in a gravitational field releases energy, which becomes heat (imagine a large asteroid impacting the Earth). • However, this simple theory, where the whole planet gradually contracts, does not account for the present-day energy source: ...
Jupiter–friend or foe? I: the asteroids
... to study the exact relationship between the giant planet and the impact rate on the Earth, we decided to run a series of n-body simulations to see how varying the mass of a giant planet in Jupiter’s orbit would change the impact rate on Earth. Since there are three distinct populations which provide ...
... to study the exact relationship between the giant planet and the impact rate on the Earth, we decided to run a series of n-body simulations to see how varying the mass of a giant planet in Jupiter’s orbit would change the impact rate on Earth. Since there are three distinct populations which provide ...
Solar Sytem Lithograph Set pdf
... pieces of debris. Many of these were discovered by planetary spacecraft. Some of these have atmospheres (Saturn’s Titan); some even have magnetic fields (Jupiter’s Ganymede). Jupiter’s moon Io is the most volcanically active body in the solar system. An ocean may lie beneath the frozen crust of Jupi ...
... pieces of debris. Many of these were discovered by planetary spacecraft. Some of these have atmospheres (Saturn’s Titan); some even have magnetic fields (Jupiter’s Ganymede). Jupiter’s moon Io is the most volcanically active body in the solar system. An ocean may lie beneath the frozen crust of Jupi ...
Uran_Nep
... Diameter: 51,118 km (4.01 Dearth) Mass: 8.69x1025 kg (14.54 Mearth) Density: 1.24 g/cm3 Rotation Period: 17.24 hours o Tilt of Axis: 98 (retrograde rotation!) o Surface Temperature: 52 K (-366 F) ...
... Diameter: 51,118 km (4.01 Dearth) Mass: 8.69x1025 kg (14.54 Mearth) Density: 1.24 g/cm3 Rotation Period: 17.24 hours o Tilt of Axis: 98 (retrograde rotation!) o Surface Temperature: 52 K (-366 F) ...
Jupiter – friend or foe? II: the Centaurs Accepted for publication in
... resulting from objects on Centaur-like orbits is affected by the presence of a giant planet, in an attempt to fully understand the impact regime under which life on Earth has developed. The Centaurs are a population of ice-rich bodies which move on dynamically unstable orbits in the outer Solar syst ...
... resulting from objects on Centaur-like orbits is affected by the presence of a giant planet, in an attempt to fully understand the impact regime under which life on Earth has developed. The Centaurs are a population of ice-rich bodies which move on dynamically unstable orbits in the outer Solar syst ...
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.