The Jovian Planets
... systems wrap completely around the planet. • Because of the pressure difference, belts and zones lie at slightly different heights in the atmosphere, and thus have slightly different temperatures. This temperature difference is responsible for the difference in colors between the two regions. • Zona ...
... systems wrap completely around the planet. • Because of the pressure difference, belts and zones lie at slightly different heights in the atmosphere, and thus have slightly different temperatures. This temperature difference is responsible for the difference in colors between the two regions. • Zona ...
Jupiter Reading Comprehension Worksheet
... Jupiter is surrounded by a system of thin rings. The majority of the rings are made up of very small particles thought to be debris from meteoroid collisions. Jupiter rotates on its axis every 9.925 hours, faster than any other planet in our solar system. It takes Jupiter almost 12 Earth years (11.8 ...
... Jupiter is surrounded by a system of thin rings. The majority of the rings are made up of very small particles thought to be debris from meteoroid collisions. Jupiter rotates on its axis every 9.925 hours, faster than any other planet in our solar system. It takes Jupiter almost 12 Earth years (11.8 ...
File - Homeschooling Mommie
... Jupiter is surrounded by a system of thin rings. The majority of the rings are made up of very small particles thought to be debris from meteoroid collisions. Jupiter rotates on its axis every 9.925 hours, faster than any other planet in our solar system. It takes Jupiter almost 12 Earth years (11.8 ...
... Jupiter is surrounded by a system of thin rings. The majority of the rings are made up of very small particles thought to be debris from meteoroid collisions. Jupiter rotates on its axis every 9.925 hours, faster than any other planet in our solar system. It takes Jupiter almost 12 Earth years (11.8 ...
Lecture 1
... No Reading days are scheduled this semester Exam Period begins at 7:30 a.m. on Monday, December 14 and ends on December 21 ...
... No Reading days are scheduled this semester Exam Period begins at 7:30 a.m. on Monday, December 14 and ends on December 21 ...
The Structure of Earth`s Atmosphere
... magnetic poles. ~ 1000 times more powerful than aurorae on Earth. Particles producing the aurorae originate mostly from moon Io ...
... magnetic poles. ~ 1000 times more powerful than aurorae on Earth. Particles producing the aurorae originate mostly from moon Io ...
Week 5 Lecture
... distinctive colors of these different layers are not yet known. The cloud layers in Saturn’s atmosphere are spread out over a greater range of altitude than those of Jupiter, giving Saturn a more washed-out appearance. • Saturn’s atmosphere contains less helium than Jupiter’s atmosphere. This lower ...
... distinctive colors of these different layers are not yet known. The cloud layers in Saturn’s atmosphere are spread out over a greater range of altitude than those of Jupiter, giving Saturn a more washed-out appearance. • Saturn’s atmosphere contains less helium than Jupiter’s atmosphere. This lower ...
Jovian Planets
... • After its discovery, astronomer noticed that Uranus did not appear to follow Newton’s laws of motion – At certain points in its orbit Uranus appeared to speed up for no apparent reason – At other points it appeared to slow down, also without any apparent reason ...
... • After its discovery, astronomer noticed that Uranus did not appear to follow Newton’s laws of motion – At certain points in its orbit Uranus appeared to speed up for no apparent reason – At other points it appeared to slow down, also without any apparent reason ...
Tidal Heating of Moons
... Gravity depends on the mass of object and the distance they’re separated. The greater the separation, the weaker the force of gravity. Since moons and planets are not points (they’re big balls), this results in tides being raised. For example, the Moon raises tides on the Earth. One side of the Eart ...
... Gravity depends on the mass of object and the distance they’re separated. The greater the separation, the weaker the force of gravity. Since moons and planets are not points (they’re big balls), this results in tides being raised. For example, the Moon raises tides on the Earth. One side of the Eart ...
largest and most massive planets [Figure 12
... High pressures (Jupiter ~ 50 Mb, Saturn ~10Mb) and Temperatures (~20,000 K) → “exotic” states of matter → metallic Hydrogen (fluid conductor) Density indicates some heavier materials rock, metals and ice at core Interiors hot, planets radiate more than they absorb self luminous (in infrared) Interna ...
... High pressures (Jupiter ~ 50 Mb, Saturn ~10Mb) and Temperatures (~20,000 K) → “exotic” states of matter → metallic Hydrogen (fluid conductor) Density indicates some heavier materials rock, metals and ice at core Interiors hot, planets radiate more than they absorb self luminous (in infrared) Interna ...
Chapter 30 - Cloudfront.net
... Neptune’s relatively small number of rings are clumpy rather than thin and uniform. ...
... Neptune’s relatively small number of rings are clumpy rather than thin and uniform. ...
What is the biggest planet in the solar system?
... its northern and southern poles. But on Jupiter, the auroral activity is much more intense and rarely ever stops. The intense radiation, Jupiter's magnetic field, and the abundance of material from The temperature and pressure inside Jupiter increase steadily toward the core. At the "surface", Io's ...
... its northern and southern poles. But on Jupiter, the auroral activity is much more intense and rarely ever stops. The intense radiation, Jupiter's magnetic field, and the abundance of material from The temperature and pressure inside Jupiter increase steadily toward the core. At the "surface", Io's ...
How Big Is Jupiter? - Nevada Outdoor School
... be about equal size. If they are between planets, color, shapes, about nine third graders. So, not, have them remark the cuts. surface, etc. this would be When the pieces are relatively ...
... be about equal size. If they are between planets, color, shapes, about nine third graders. So, not, have them remark the cuts. surface, etc. this would be When the pieces are relatively ...
Saturn
... of 50 or more years -- Hyperion (1848) and Phoebe (1898). As telescopic resolving power increased through the 19th century, Saturn's family of known moons grew. In 1966 Epimetheus and Janus were discovered. By the time Cassini-Huygens was launched in 1997, Saturn's moon count had reached 18. The num ...
... of 50 or more years -- Hyperion (1848) and Phoebe (1898). As telescopic resolving power increased through the 19th century, Saturn's family of known moons grew. In 1966 Epimetheus and Janus were discovered. By the time Cassini-Huygens was launched in 1997, Saturn's moon count had reached 18. The num ...
on Earth
... • Miller’s assumption was that no O2 existed in Earth’s early atmosphere – Incorrect: at least some was there (but not much) ...
... • Miller’s assumption was that no O2 existed in Earth’s early atmosphere – Incorrect: at least some was there (but not much) ...
Jupiter - waka6b
... How Big is Jupiter ? • Jupiter has an equatorial diameter of 141,700 km compared to Earth's 12,800 km. This means that Jupiter is 11 times the diameter of the Earth, and 1,300 times its volume. This is about like comparing a basketball to a ping pong ball. • Compared to the Sun, Jupiter is about 0. ...
... How Big is Jupiter ? • Jupiter has an equatorial diameter of 141,700 km compared to Earth's 12,800 km. This means that Jupiter is 11 times the diameter of the Earth, and 1,300 times its volume. This is about like comparing a basketball to a ping pong ball. • Compared to the Sun, Jupiter is about 0. ...
Lecture 1
... Jupiter’s deep atmosphere • There are presumed to be three cloud layers in the atmospheres of Jupiter and Saturn • The reasons for the distinctive colors of these different layers are not yet known • The cloud layers in Saturn’s atmosphere are spread out over a greater range of altitude than those o ...
... Jupiter’s deep atmosphere • There are presumed to be three cloud layers in the atmospheres of Jupiter and Saturn • The reasons for the distinctive colors of these different layers are not yet known • The cloud layers in Saturn’s atmosphere are spread out over a greater range of altitude than those o ...
Ch10_Lecture
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
Chapter 10 The Outer Worlds… Jupiter Jupiter Jupiter`s Interior
... composed of meter-sized objects • These objects are very dark, implying they are rich in carbon particles or organic-like materials • The extremely narrow rings may be held in place by shepherding satellites ...
... composed of meter-sized objects • These objects are very dark, implying they are rich in carbon particles or organic-like materials • The extremely narrow rings may be held in place by shepherding satellites ...
Chapter 9
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
11/11/08 Chapter 9 The Outer Worlds… Jupiter Jupiter Jupiter`s
... – the Great “Dark” Spot being, at one time, the most prominent feature • Neptune was discovered from predictions made by John C. Adams and Urbain Leverrie, who calculated its orbit based on disturbances in Uranus’s orbit ...
... – the Great “Dark” Spot being, at one time, the most prominent feature • Neptune was discovered from predictions made by John C. Adams and Urbain Leverrie, who calculated its orbit based on disturbances in Uranus’s orbit ...
Today`s Powerpoint
... The closer to Jupiter, the higher the moon density: from 3.5 g/cm3 (Io) to 1.8 g/cm3 (Callisto). Higher density indicates higher rock/ice fraction. ...
... The closer to Jupiter, the higher the moon density: from 3.5 g/cm3 (Io) to 1.8 g/cm3 (Callisto). Higher density indicates higher rock/ice fraction. ...
SATURN
... was named after a roman god Saturn. Saturn is a gas giant. Saturn. Saturn was discovered by Chirstitaan Huygen in 1659. Saturn has 60 moons. ...
... was named after a roman god Saturn. Saturn is a gas giant. Saturn. Saturn was discovered by Chirstitaan Huygen in 1659. Saturn has 60 moons. ...
Is the Earth Really Round
... Rotation – the spinning of the Earth on its axis Axis – imaginary line drawn from Earth’s North Pole through to the South Pole. Revolution – the motion of the Earth around the Sun. Equator – imaginary line drawn around the Earth at its largest circumference. Orbit – curved path of one planetary body ...
... Rotation – the spinning of the Earth on its axis Axis – imaginary line drawn from Earth’s North Pole through to the South Pole. Revolution – the motion of the Earth around the Sun. Equator – imaginary line drawn around the Earth at its largest circumference. Orbit – curved path of one planetary body ...