Jupiter - Moodle
... – (after the Sun, the Moon and Venus; at some times Mars is also brighter). ...
... – (after the Sun, the Moon and Venus; at some times Mars is also brighter). ...
Our Solar System
... Ancient observers believed that the Sun and all the other celestial bodies revolved around Earth. But astronomers gradually realized that the Earth-centered model did not account for the motions of the planets. In the early 17th century, Galileo Galilei’s discoveries using the recently invented tele ...
... Ancient observers believed that the Sun and all the other celestial bodies revolved around Earth. But astronomers gradually realized that the Earth-centered model did not account for the motions of the planets. In the early 17th century, Galileo Galilei’s discoveries using the recently invented tele ...
Midterm 2 – Wed. March 2 SIT IN YOUR ASSIGNED ROW! YOUR
... with 10-15 x mass of Earth. • Lots of weather on Jupiter • Ammonia (NH3) clouds. • Strong winds at different latitudes. (differential rotation) • Cyclonic storms • Great Red Spot – 2 x size of Earth – 400 yrs so far ...
... with 10-15 x mass of Earth. • Lots of weather on Jupiter • Ammonia (NH3) clouds. • Strong winds at different latitudes. (differential rotation) • Cyclonic storms • Great Red Spot – 2 x size of Earth – 400 yrs so far ...
File - Miss Burnett`s 6th grade Classroom
... gas surface unlike the rocky surface of the inner planets, like Earth. ...
... gas surface unlike the rocky surface of the inner planets, like Earth. ...
November 2013 - Pomona Valley Amateur Astronomers
... like the tiny moon Io, orbiting Jupiter. With just 1.5% the mass of Earth despite being more than one quarter of the Earth's diameter, Io seems like an unlikely candidate for volcanoes, as 4.5 billion years is more than enough time for it to have cooled and become stable. Yet Io is anything but stab ...
... like the tiny moon Io, orbiting Jupiter. With just 1.5% the mass of Earth despite being more than one quarter of the Earth's diameter, Io seems like an unlikely candidate for volcanoes, as 4.5 billion years is more than enough time for it to have cooled and become stable. Yet Io is anything but stab ...
Observing the Solar System
... • According to the new definition, a full-fledged planet is an object that orbits the sun and is large enough to have become round due to the force of its own gravity. In addition, a planet has to dominate the neighborhood around its orbit. • Pluto does not dominate its neighborhood Charon is half i ...
... • According to the new definition, a full-fledged planet is an object that orbits the sun and is large enough to have become round due to the force of its own gravity. In addition, a planet has to dominate the neighborhood around its orbit. • Pluto does not dominate its neighborhood Charon is half i ...
The Planets: An Overview
... • Saturn’s atmosphere is very active, with winds roaring at up to 1500 kilometers per hour. • Large cyclonic “storms” similar to Jupiter’s Great Red Spot, although smaller, occur in Saturn’s atmosphere. Saturn’s Rings • Until the discovery that Jupiter, Uranus, and Neptune have ring systems, this ...
... • Saturn’s atmosphere is very active, with winds roaring at up to 1500 kilometers per hour. • Large cyclonic “storms” similar to Jupiter’s Great Red Spot, although smaller, occur in Saturn’s atmosphere. Saturn’s Rings • Until the discovery that Jupiter, Uranus, and Neptune have ring systems, this ...
The Jovian Planets + Pluto and the TNOs Jupiter 12 of Jupiter`s
... ☼ Meteoric matter is slowly taken below surface by water breaking through ice ☼ Ingredients for life: water, heat, organic compounds all present NASA mission ☼ Periods Io, Europa, Ganymede in ratio 1:2:4 ...
... ☼ Meteoric matter is slowly taken below surface by water breaking through ice ☼ Ingredients for life: water, heat, organic compounds all present NASA mission ☼ Periods Io, Europa, Ganymede in ratio 1:2:4 ...
Jupiter` moons
... · Impact craters tell us a lot about the orbit, surface age, surface material, etc. · In terms of their orbit, planets have a trailing and leading hemisphere, as is confirmed by the ratio of impacts on each hemisphere (trailing = less, leading = more). Indicates that these moons are tidally locked t ...
... · Impact craters tell us a lot about the orbit, surface age, surface material, etc. · In terms of their orbit, planets have a trailing and leading hemisphere, as is confirmed by the ratio of impacts on each hemisphere (trailing = less, leading = more). Indicates that these moons are tidally locked t ...
3.what color is the surface of saturn?
... A: Kepler B: Newton C: Galileo What makes Europa so unique compared to other moons of Jupiter? A: It’s super big B: It’s really pretty C: Aliens live there D: It has water What makes the surface of Europa look so unique? A: It’s red cracks B: It’s pink color ...
... A: Kepler B: Newton C: Galileo What makes Europa so unique compared to other moons of Jupiter? A: It’s super big B: It’s really pretty C: Aliens live there D: It has water What makes the surface of Europa look so unique? A: It’s red cracks B: It’s pink color ...
Chapter 7
... • Used Jupiter’s strong gravity to send them on to Saturn - gravity assist • Voyager 2 used Saturn’s gravity to propel it to Uranus and then on to Neptune • Studied planetary magnetic fields and analyzed multi-wavelength radiation • Both are now headed out into interstellar space! ...
... • Used Jupiter’s strong gravity to send them on to Saturn - gravity assist • Voyager 2 used Saturn’s gravity to propel it to Uranus and then on to Neptune • Studied planetary magnetic fields and analyzed multi-wavelength radiation • Both are now headed out into interstellar space! ...
23.3 Note Guide The Outer Planets In 2004, the space probe
... In this section, we’ll take a clue from Cassini and explore the outer planets—Jupiter, Saturn, Neptune, Uranus, and Pluto ...
... In this section, we’ll take a clue from Cassini and explore the outer planets—Jupiter, Saturn, Neptune, Uranus, and Pluto ...
Astronomy 1400 – 001: Solar System Astronomy
... b) Because they are hot, they appear brighter in the infrared than the rest of Io ...
... b) Because they are hot, they appear brighter in the infrared than the rest of Io ...
solution
... often in our orbit around the Sun, so we would observe more retrograde motion for Saturn in a given period of time. 12.8 What would happen if you tried to land a spacecraft on the surface of Jupiter? While there is a rocky core at the center of Jupiter, it is surrounded by a very massive atmosphere ...
... often in our orbit around the Sun, so we would observe more retrograde motion for Saturn in a given period of time. 12.8 What would happen if you tried to land a spacecraft on the surface of Jupiter? While there is a rocky core at the center of Jupiter, it is surrounded by a very massive atmosphere ...
December - Naples Free-Net
... Yet volcanoes occur on worlds that you might never expect, like the tiny moon Io, orbiting Jupiter. With just 1.5% the mass of Earth despite being more than one quarter of the Earth's diameter, Io seems like an unlikely candidate for volcanoes, as 4.5 billion years is more than enough time for it to ...
... Yet volcanoes occur on worlds that you might never expect, like the tiny moon Io, orbiting Jupiter. With just 1.5% the mass of Earth despite being more than one quarter of the Earth's diameter, Io seems like an unlikely candidate for volcanoes, as 4.5 billion years is more than enough time for it to ...
Chapter 8
... and the low frequency radio emission The gasses ejected from the volcanic activity are ionized by the UV radiation from the Sun and form a torus of ionized material around the orbits of Io. This ionized material are accelerated by Io and interact with the magnetic field of the planet and triggers th ...
... and the low frequency radio emission The gasses ejected from the volcanic activity are ionized by the UV radiation from the Sun and form a torus of ionized material around the orbits of Io. This ionized material are accelerated by Io and interact with the magnetic field of the planet and triggers th ...
Jupiter
... Jupiter is the most stormiest planet in our solar system with wind that mostly reach 300 miles per hour and one of the strongest, biggest and the longest storm to last is the great red spot in southern hemisphere and it has lasted for more than 300 years and the wind speed over 500 miles per hour . ...
... Jupiter is the most stormiest planet in our solar system with wind that mostly reach 300 miles per hour and one of the strongest, biggest and the longest storm to last is the great red spot in southern hemisphere and it has lasted for more than 300 years and the wind speed over 500 miles per hour . ...
The solar system
... Discovered in 1930 Highly elongated orbit causes it to occasionally travel inside the orbit of Neptune, where it resided from ...
... Discovered in 1930 Highly elongated orbit causes it to occasionally travel inside the orbit of Neptune, where it resided from ...
Thinking Critically
... Use the image of Jupiter’s moon Ganymede to answer the next five questions. ...
... Use the image of Jupiter’s moon Ganymede to answer the next five questions. ...
Chapter 11 The Jovian Planets
... • The cutoff of Jupiter low frequency radio emission is around 40 MHz, the highest frequency of all the planets. •It is the only planet from which we can receive the low frequency emission in ground-based radio telescopes •The rest of the Jovian planets emit low radio emission but it cannot be recei ...
... • The cutoff of Jupiter low frequency radio emission is around 40 MHz, the highest frequency of all the planets. •It is the only planet from which we can receive the low frequency emission in ground-based radio telescopes •The rest of the Jovian planets emit low radio emission but it cannot be recei ...
Section 14.4 Outer Planets
... regions like the largest "gap" called the Cassini division, also contain fainter rings. They may possibly be either a moon torn apart by tidal forces, or material that was never allowed to turn into moons because of the tidal forces. ...
... regions like the largest "gap" called the Cassini division, also contain fainter rings. They may possibly be either a moon torn apart by tidal forces, or material that was never allowed to turn into moons because of the tidal forces. ...
jupiter 1
... observed. These characteristics suggest a continuing process that resurfaces the moon with fresh material below. Like Io, Europa is subjected to tidal heating, but because Europa is further from Jupiter than Io the tidal effect is less dramatic. Specifically, the effect of the tides induced by Jupit ...
... observed. These characteristics suggest a continuing process that resurfaces the moon with fresh material below. Like Io, Europa is subjected to tidal heating, but because Europa is further from Jupiter than Io the tidal effect is less dramatic. Specifically, the effect of the tides induced by Jupit ...
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.