Name: Notes – #30 Jupiter and Its Amazing Moons 1. Jupiter is
... 3. Jupiter is ______ times more massive than all of the other planets put together. 4. Jupiter rotates about its axis in ________ hours. 5. Jupiter consists mostly of ________________ and _________________. 6. True or False: Jupiter has a strong magnetic field. 7. The outer planets retained so much ...
... 3. Jupiter is ______ times more massive than all of the other planets put together. 4. Jupiter rotates about its axis in ________ hours. 5. Jupiter consists mostly of ________________ and _________________. 6. True or False: Jupiter has a strong magnetic field. 7. The outer planets retained so much ...
jupiter interpretive sign - Town of Cumberland, Indiana
... • Rotation period: 0.4 earth days (9.8 hours) • Revolution period: 11.86 earth years ...
... • Rotation period: 0.4 earth days (9.8 hours) • Revolution period: 11.86 earth years ...
Astronomy: Week #5 Assignment
... 1. Why does Jupiter appear brighter than Mars despite Jupiter’s greater distance from the Earth? 2. Even though Jupiter’s atmosphere is very active, the Great Red Spot has persisted for a long time. How is this possible? 3. What advantages over the 5 meter Palomar telescope on Earth did Voyagers 1 a ...
... 1. Why does Jupiter appear brighter than Mars despite Jupiter’s greater distance from the Earth? 2. Even though Jupiter’s atmosphere is very active, the Great Red Spot has persisted for a long time. How is this possible? 3. What advantages over the 5 meter Palomar telescope on Earth did Voyagers 1 a ...
Chpt 27 Notes
... 2. Explain what a dwarf planet is. A dwarf planet is a protoplanet that is still in the developmental process and has not met the two requirements of a plant. The first requirement is that the object has coalesced into a globe shaped object (their shape is not oblong or random like an asteroid). The ...
... 2. Explain what a dwarf planet is. A dwarf planet is a protoplanet that is still in the developmental process and has not met the two requirements of a plant. The first requirement is that the object has coalesced into a globe shaped object (their shape is not oblong or random like an asteroid). The ...
Facts about Planets Answer Key File
... 1. _____Mercury___________ atmosphere is so thin that it is barely detectable. 2. Mercury is only _____0.38 x________ the diameter of the Earth. 3. Venus rotates in a ______Retrograde (backward)_________ direction. 4. Mars is sometimes referred to as the _______Red_________ planet. 5. Venus has a th ...
... 1. _____Mercury___________ atmosphere is so thin that it is barely detectable. 2. Mercury is only _____0.38 x________ the diameter of the Earth. 3. Venus rotates in a ______Retrograde (backward)_________ direction. 4. Mars is sometimes referred to as the _______Red_________ planet. 5. Venus has a th ...
generalsciencenotes - Geoscience Research Institute
... a near-infrared mapping spectrometer which will also measure heat from Io’s volcanoes. an ultraviolet spectrometer to study the composition and structure of the atmospheres and the cloud of charged atoms injected into the magnetosphere by Io. a photopolarimeter-radiometer. a magnetometer to measure ...
... a near-infrared mapping spectrometer which will also measure heat from Io’s volcanoes. an ultraviolet spectrometer to study the composition and structure of the atmospheres and the cloud of charged atoms injected into the magnetosphere by Io. a photopolarimeter-radiometer. a magnetometer to measure ...
Moons Jupiter was known to have at least 16 moons at the time this
... crisscrossing lines over bright clear fields of water ice. The lines may be cracks in the ice. Europa has few craters. ...
... crisscrossing lines over bright clear fields of water ice. The lines may be cracks in the ice. Europa has few craters. ...
The Solar System: JUPITER by - Etiwanda E
... Earth and more than twice as big as all the rest of the planets added together) • is 778,330,000 km from the sun • has 39 known satellites ...
... Earth and more than twice as big as all the rest of the planets added together) • is 778,330,000 km from the sun • has 39 known satellites ...
Jupiter_Io_13_3
... lightning in Jupiter's upper atmosphere. As Jupiter rotates, it takes its magnetic field around with it, sweeping past Io and stripping off about 1,000 kg (1 ton) of Io's material every second! This material becomes ionized in the magnetic field and forms a doughnut-shaped cloud of intense radiation ...
... lightning in Jupiter's upper atmosphere. As Jupiter rotates, it takes its magnetic field around with it, sweeping past Io and stripping off about 1,000 kg (1 ton) of Io's material every second! This material becomes ionized in the magnetic field and forms a doughnut-shaped cloud of intense radiation ...
JUPITER Jacob davis
... • What is it made of:(rocky, gas)-Jupiter is made up of gases. • Moons:Io,Europa,Ganymede,Callisto. • Day(rotation):A day on Jupiter is 10 earth hours. • Year(orbit period)A year on Jupiter is 11.86 earth years. ...
... • What is it made of:(rocky, gas)-Jupiter is made up of gases. • Moons:Io,Europa,Ganymede,Callisto. • Day(rotation):A day on Jupiter is 10 earth hours. • Year(orbit period)A year on Jupiter is 11.86 earth years. ...
Video review
... 2. In the most distant part of Pluto’s eccentric orbit, its atmosphere turns from gas to ___________. 3. The largest planetary storm system is Jupiter’s ________________________. 4. Cassini used a ______________ from Venus and Earth to reach Saturn. 5. ___________ is the only moon in the solar syste ...
... 2. In the most distant part of Pluto’s eccentric orbit, its atmosphere turns from gas to ___________. 3. The largest planetary storm system is Jupiter’s ________________________. 4. Cassini used a ______________ from Venus and Earth to reach Saturn. 5. ___________ is the only moon in the solar syste ...
www.roe.ac.uk
... The Jovian, or gaseous, planets have rocky cores surrounded by thick atmospheres. The radius is measured to the point at which the pressure drops to 1 atmosphere. ...
... The Jovian, or gaseous, planets have rocky cores surrounded by thick atmospheres. The radius is measured to the point at which the pressure drops to 1 atmosphere. ...
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.