Solar System Fact Sheet - University of South Alabama
... 1. Mercury 2. Venus 3. Earth 4. Mars 5. Jupiter 6. Saturn 7. Uranus 8. Neptune 9. Pluto (no longer a planet, just a dwarf planet) B. Terrestrial Planets 1. Have high average density 2. Rocky structure 3. relatively small planets 4. near the Sun 5. includes Mercury, Venus, Earth, Mars C. Jovian Plane ...
... 1. Mercury 2. Venus 3. Earth 4. Mars 5. Jupiter 6. Saturn 7. Uranus 8. Neptune 9. Pluto (no longer a planet, just a dwarf planet) B. Terrestrial Planets 1. Have high average density 2. Rocky structure 3. relatively small planets 4. near the Sun 5. includes Mercury, Venus, Earth, Mars C. Jovian Plane ...
To Jupiter … and Beyond! - Five Star Publications, Inc.
... could hold 1,300 Earths. But the giant Jupiter is only 318 times heavier than Earth. Why? Because Earth is four times denser than this massive ball of gas. Scientists say that Jupiter contains about the same concentration of hydrogen as the sun itself. It also contains a concentration of materials s ...
... could hold 1,300 Earths. But the giant Jupiter is only 318 times heavier than Earth. Why? Because Earth is four times denser than this massive ball of gas. Scientists say that Jupiter contains about the same concentration of hydrogen as the sun itself. It also contains a concentration of materials s ...
Jupiter
... observed. They are made of mostly dust. The rings are a reddish color accept the Halo Ring which is blue. ...
... observed. They are made of mostly dust. The rings are a reddish color accept the Halo Ring which is blue. ...
File
... massive high pressure system which rotates in 6 days. Without surface friction to slow their speed, storms last for hundreds of years or longer. ...
... massive high pressure system which rotates in 6 days. Without surface friction to slow their speed, storms last for hundreds of years or longer. ...
The Solar System - Academic Resources at Missouri Western
... Very Earth like Distinct “reddish” color Interesting features: The plains The “channels” Dried river beds Martians and other good stories Seasonal changes Polar ice caps Frozen CO2 Olympus Mons volcano 15 mi. high 370 mi. wide The size of Texas ...
... Very Earth like Distinct “reddish” color Interesting features: The plains The “channels” Dried river beds Martians and other good stories Seasonal changes Polar ice caps Frozen CO2 Olympus Mons volcano 15 mi. high 370 mi. wide The size of Texas ...
early views of the universe
... allowed him to observe the heavens. The telescope allowed him to make the observations that supported a heliocentric model of the universe • Galileo's telescope video ...
... allowed him to observe the heavens. The telescope allowed him to make the observations that supported a heliocentric model of the universe • Galileo's telescope video ...
Jupiter
... It takes Jupiter about 11 years to orbit its axis. Though, it takes 1186 years to orbit the sun. ...
... It takes Jupiter about 11 years to orbit its axis. Though, it takes 1186 years to orbit the sun. ...
30-4 Satellites of other Planets
... • Neptune and Uranus contain ices of water, ammonia, and methane. • The methane in Neptune and Uranus is what gives the planets their blue color. ...
... • Neptune and Uranus contain ices of water, ammonia, and methane. • The methane in Neptune and Uranus is what gives the planets their blue color. ...
Lecture 08a: Galilean moons - Sierra College Astronomy Home Page
... Size: 1.38× Earth’s moon, mass: 1.46× Earth’s moon; Ice and rock, with outer several hundred km of H2O ice? It never probably warmed enough to differentiate; Yet Galileo spacecraft detected an induced magnetic field; Not locked in orbital resonance (no tidal heating); Smallest craters are missing (e ...
... Size: 1.38× Earth’s moon, mass: 1.46× Earth’s moon; Ice and rock, with outer several hundred km of H2O ice? It never probably warmed enough to differentiate; Yet Galileo spacecraft detected an induced magnetic field; Not locked in orbital resonance (no tidal heating); Smallest craters are missing (e ...
2.4 - Horace Mann Webmail
... • They all have such a strong gravitational pull that they have thick atmospheres. ...
... • They all have such a strong gravitational pull that they have thick atmospheres. ...
Big Moons in the Outer Solar System
... The Big Moons of the Outer Planets Six large moons exist in the outer solar system, which are as large or larger than Earth's Moon. Each displays unusual properties; no two are alike. Jupiter Io, Europa, Ganymede & Callisto Saturn ...
... The Big Moons of the Outer Planets Six large moons exist in the outer solar system, which are as large or larger than Earth's Moon. Each displays unusual properties; no two are alike. Jupiter Io, Europa, Ganymede & Callisto Saturn ...
Chapter 6 Lecture 1
... • Gigantic for a planet: 300 Earth mass; >1,000 Earth volume. • Many moons, rings ...
... • Gigantic for a planet: 300 Earth mass; >1,000 Earth volume. • Many moons, rings ...
ppt
... for the inner solar system This helps reduce the probability of an impact event that could wipe out life on Earth However, Jupiter cannot be too massive as some comets must reach the primordial Earth to supply it with water ...
... for the inner solar system This helps reduce the probability of an impact event that could wipe out life on Earth However, Jupiter cannot be too massive as some comets must reach the primordial Earth to supply it with water ...
Day-34
... Called giant planets because of their mass— from 14.5 Earth masses (Uranus) to 318 (Jupiter)—and also, their physical size. No solid surfaces: We just see the cloud layers in the atmospheres. ...
... Called giant planets because of their mass— from 14.5 Earth masses (Uranus) to 318 (Jupiter)—and also, their physical size. No solid surfaces: We just see the cloud layers in the atmospheres. ...
Lecture 28: The Galilean Moons of Jupiter
... The Galilean moons of Jupiter are heated by tides from Jupiter – closer moons are hotter. Ganymede and Callisto are old, geologically dead worlds: mostly ice mantles over rocky cores. Innermost Io is tidally melted inside, making it the most volcanically active world in the Solar System. Europa may ...
... The Galilean moons of Jupiter are heated by tides from Jupiter – closer moons are hotter. Ganymede and Callisto are old, geologically dead worlds: mostly ice mantles over rocky cores. Innermost Io is tidally melted inside, making it the most volcanically active world in the Solar System. Europa may ...
PHYS 178 – Assignment 5 Sketchy Answers
... The craters are less well-defined on Jupiter’s moons (e.g. Callisto) because the ice is warmer, and it slumps/flows over long periods of time. The ice on the surfaces of (non-tidally heated) moons around Saturn is cold and more rock-like. The craters on Rhea, for example, resemble those on the Moon ...
... The craters are less well-defined on Jupiter’s moons (e.g. Callisto) because the ice is warmer, and it slumps/flows over long periods of time. The ice on the surfaces of (non-tidally heated) moons around Saturn is cold and more rock-like. The craters on Rhea, for example, resemble those on the Moon ...
Make up notes
... • Mercury, Venus, Earth, and Mars • Earth - only one with water on the surface and can support life ...
... • Mercury, Venus, Earth, and Mars • Earth - only one with water on the surface and can support life ...
space - Kidblog
... a gas giant, rather than a terrestrial planet, and is made largely of hydrogen and helium. Jupiter was first visited by Pioneer 10 in 1973 and later by Pioneer 11, Voyager 1, Voyager 2 and Ulysses. The unmanned ...
... a gas giant, rather than a terrestrial planet, and is made largely of hydrogen and helium. Jupiter was first visited by Pioneer 10 in 1973 and later by Pioneer 11, Voyager 1, Voyager 2 and Ulysses. The unmanned ...
Europa
... • They are composed principally of rocky material • The two outermost Galilean satellites, Ganymede and Callisto, are roughly the size of Mercury • Lower in density than either the Moon or Mercury, they are made of roughly equal parts of ice and rock ...
... • They are composed principally of rocky material • The two outermost Galilean satellites, Ganymede and Callisto, are roughly the size of Mercury • Lower in density than either the Moon or Mercury, they are made of roughly equal parts of ice and rock ...
Outer or Jovian Planets - Academic Computer Center
... How did they determine that the radio waves were coming from Jupiter? • They noticed that the timing of the bursts changed at a sidereal rate, that is at the same rate that the stars appeared to move across the sky so it had to be coming from something in space and not something on the ground. • Fu ...
... How did they determine that the radio waves were coming from Jupiter? • They noticed that the timing of the bursts changed at a sidereal rate, that is at the same rate that the stars appeared to move across the sky so it had to be coming from something in space and not something on the ground. • Fu ...
Our own Earth`s interior structure, and surface features will be
... comprised of liquid metallic hydrogen. Inside each of these planets is a rocky core. Three outer solar system moons were discussed: Io (Jupiter), Europa (Jupiter) and Titan (Saturn). Latest information from spacecraft provides new insights to these interesting worlds. Future missions to Europa and T ...
... comprised of liquid metallic hydrogen. Inside each of these planets is a rocky core. Three outer solar system moons were discussed: Io (Jupiter), Europa (Jupiter) and Titan (Saturn). Latest information from spacecraft provides new insights to these interesting worlds. Future missions to Europa and T ...
JUpiter ICy moons Explorer (JUICE): AN ESA L-CLASS
... on Earth are not yet clearly understood, one can assume that the necessary conditions involve the simultaneous presence of organic compounds, trace elements, water, energy sources and a relative stability of the environment over time. JUICE will address the question: Are there current habitats elsew ...
... on Earth are not yet clearly understood, one can assume that the necessary conditions involve the simultaneous presence of organic compounds, trace elements, water, energy sources and a relative stability of the environment over time. JUICE will address the question: Are there current habitats elsew ...
Space - Jupiter
... d. The liquid is a transitional phase between Jupiter's solid core and gaseous atmosphere ...
... d. The liquid is a transitional phase between Jupiter's solid core and gaseous atmosphere ...
PPT - University of Delaware
... – Students calculate distances and planet/moon sizes if the Earth were 1 cm, 1 inch or 1 foot in diameter. – Plot orbits on 40”x36” map of Wilmington. – Determine location of planets today and plot. – Compute and plot location of planets in one ...
... – Students calculate distances and planet/moon sizes if the Earth were 1 cm, 1 inch or 1 foot in diameter. – Plot orbits on 40”x36” map of Wilmington. – Determine location of planets today and plot. – Compute and plot location of planets in one ...
Jupiter=Zeus=Indra
... Jupiter’s moon Io is very hot because: a) It has so many volcanoes b) It has not had time to cool since its formation c) Of impacts from the dust in the plasma torus d) Electric currents generated by its motion through Jupiter’s magnetic field e) Orbital resonances with Europa and Ganymede ...
... Jupiter’s moon Io is very hot because: a) It has so many volcanoes b) It has not had time to cool since its formation c) Of impacts from the dust in the plasma torus d) Electric currents generated by its motion through Jupiter’s magnetic field e) Orbital resonances with Europa and Ganymede ...
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.