source - UC Berkeley Astronomy w
... - Gaps in rings due to (1) resonance interactions with large moons outside the rings, (2) direct gravitational interaction with small moons orbiting inside the gaps. - Very narrow rings (F ring) due to shepherd moons on either side of the ring that keep material confined to a narrow band between the ...
... - Gaps in rings due to (1) resonance interactions with large moons outside the rings, (2) direct gravitational interaction with small moons orbiting inside the gaps. - Very narrow rings (F ring) due to shepherd moons on either side of the ring that keep material confined to a narrow band between the ...
Astronomy 12 Final Review Sheet Sun
... - Gaps in rings due to (1) resonance interactions with large moons outside the rings, (2) direct gravitational interaction with small moons orbiting inside the gaps. - Very narrow rings (F ring) due to shepherd moons on either side of the ring that keep material confined to a narrow band between the ...
... - Gaps in rings due to (1) resonance interactions with large moons outside the rings, (2) direct gravitational interaction with small moons orbiting inside the gaps. - Very narrow rings (F ring) due to shepherd moons on either side of the ring that keep material confined to a narrow band between the ...
Comets People were very superstitious in ancient times. They
... Comets come from places in the outer solar system called the Kuiper Belt and the Oort Cloud. The Kuiper Belt and the Oort Cloud are made up of chunks of ice and rock. Comets that orbit the Sun in less than 200 years come from the Kuiper Belt. The Kuiper Belt is just beyond the planet Neptune. Comets ...
... Comets come from places in the outer solar system called the Kuiper Belt and the Oort Cloud. The Kuiper Belt and the Oort Cloud are made up of chunks of ice and rock. Comets that orbit the Sun in less than 200 years come from the Kuiper Belt. The Kuiper Belt is just beyond the planet Neptune. Comets ...
Big Moons in the Outer Solar System
... Smallest of the “big” moons, 10% smaller than Europa. Orbits in a retrograde direction (i.e., “backwards”) unlike every other large moon, and its orbit is highly inclined to Neptune’s equator. No reasonable explanation for Triton’s orbital behavior exists; this moon was almost certainly captur ...
... Smallest of the “big” moons, 10% smaller than Europa. Orbits in a retrograde direction (i.e., “backwards”) unlike every other large moon, and its orbit is highly inclined to Neptune’s equator. No reasonable explanation for Triton’s orbital behavior exists; this moon was almost certainly captur ...
Lecture 11
... (c) has NOT cleared the neighborhood around its orbit; and (d) is not a satellite Dwarf Planets (so far): Eris, Pluto, Haumea, Makemake, Ceres ASTR111 Lecture11 ...
... (c) has NOT cleared the neighborhood around its orbit; and (d) is not a satellite Dwarf Planets (so far): Eris, Pluto, Haumea, Makemake, Ceres ASTR111 Lecture11 ...
Worksheet
... A 12. Sent an impactor to collide with Comet Tempel 1. C 13. Took pictures of the Comet Tempel 1, photo graphing the crater. B 14. Studied Comet Hartley 2. 15. What will we find at the outermost edge of the Solar System? c. The Oort Cloud. 16. How small are some meteors? d. No bigger than a grain of ...
... A 12. Sent an impactor to collide with Comet Tempel 1. C 13. Took pictures of the Comet Tempel 1, photo graphing the crater. B 14. Studied Comet Hartley 2. 15. What will we find at the outermost edge of the Solar System? c. The Oort Cloud. 16. How small are some meteors? d. No bigger than a grain of ...
Chapter 23 Section 4 Minor Members of the Solar System
... and the moon as shown by the diagram in Figure 21. Many of the most recent impact craters on the moon and Earth were probably caused by collisions with asteroids. Inevitably, future Earth- asteroid collisions will occur, as discussed in this chapter’s feature on page 665. Figure 21 The orbits of mos ...
... and the moon as shown by the diagram in Figure 21. Many of the most recent impact craters on the moon and Earth were probably caused by collisions with asteroids. Inevitably, future Earth- asteroid collisions will occur, as discussed in this chapter’s feature on page 665. Figure 21 The orbits of mos ...
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 ...
Objects in Space
... Satellites and Orbits • Imagine a firing a gun horizontally. • The bullet will eventually fall to Earth. But what if the bullet were travelling fast enough that it passed the horizon before starting to drop? • As the bullet fell to Earth, the curvature of the Earth would mean the ground was ...
... Satellites and Orbits • Imagine a firing a gun horizontally. • The bullet will eventually fall to Earth. But what if the bullet were travelling fast enough that it passed the horizon before starting to drop? • As the bullet fell to Earth, the curvature of the Earth would mean the ground was ...
Elliptic Orbits
... Sun’s gravity causes it to deviate, it swings around the Sun, then recedes tending to another straight line path as it leaves the System. There is also the theoretical possibility of a parabolic orbit, going out to infinity but never approaching a straight line asymptote. However, this requires exac ...
... Sun’s gravity causes it to deviate, it swings around the Sun, then recedes tending to another straight line path as it leaves the System. There is also the theoretical possibility of a parabolic orbit, going out to infinity but never approaching a straight line asymptote. However, this requires exac ...
The Outer Planets - Duplin County Schools
... 1 and 2 spacecraft came within 100,000 kilometers of Saturn More information was gained in a few days that had been acquired since Galileo first viewed this elegant planet 1. Saturn’s atmosphere is very active, with winds roaring at up to 1500 kilometers per hour 2. Large cyclonic “storms” similar t ...
... 1 and 2 spacecraft came within 100,000 kilometers of Saturn More information was gained in a few days that had been acquired since Galileo first viewed this elegant planet 1. Saturn’s atmosphere is very active, with winds roaring at up to 1500 kilometers per hour 2. Large cyclonic “storms” similar t ...
File - peter ditchon velarde
... Jupiter is primarily composed of hydrogen with a quarter of its mass being helium, although helium only comprises about a tenth of the number of molecules. It may also have a rocky core of heavier elements, but like the other giant planets, Jupiter lacks a well-defined solid surface. Because of its ...
... Jupiter is primarily composed of hydrogen with a quarter of its mass being helium, although helium only comprises about a tenth of the number of molecules. It may also have a rocky core of heavier elements, but like the other giant planets, Jupiter lacks a well-defined solid surface. Because of its ...
Primordial Matter in the Solar System
... • Keplerian orbits, e.g. P2 = a3 • Gaps, such as the Kirkwood Gap, due to orbital resonance with Jupiter and other asteroids (like the Cassini Division in Saturn’s rings) • Jupiter maintains the asteroid belt, although may have prevented planet formation • Families of asteroids: Floras, Trojans, and ...
... • Keplerian orbits, e.g. P2 = a3 • Gaps, such as the Kirkwood Gap, due to orbital resonance with Jupiter and other asteroids (like the Cassini Division in Saturn’s rings) • Jupiter maintains the asteroid belt, although may have prevented planet formation • Families of asteroids: Floras, Trojans, and ...
Comets, Meteors, and Asteroids Oh My!! Terms
... • These parts stream away from the head of the comet to form a shimmering tail • A comets tail ALWAYS points away from the sun ...
... • These parts stream away from the head of the comet to form a shimmering tail • A comets tail ALWAYS points away from the sun ...
The Jovian Planets
... means we must look deeper into the atmosphere to see structures (bands and spots) which characterize the flow patterns like on the other jovian planets. • Stratospheric haze also washes out any of the structure that would be visible below it. • Uranus’s atmospheric clouds and flow patterns move arou ...
... means we must look deeper into the atmosphere to see structures (bands and spots) which characterize the flow patterns like on the other jovian planets. • Stratospheric haze also washes out any of the structure that would be visible below it. • Uranus’s atmospheric clouds and flow patterns move arou ...
Study Guide
... What is the asteroid belt and where is it located? The asteroid belt is a band of rock and ice particles that separates the terrestrial planets from the gas giants (located between Mars and Jupiter) ...
... What is the asteroid belt and where is it located? The asteroid belt is a band of rock and ice particles that separates the terrestrial planets from the gas giants (located between Mars and Jupiter) ...
The Structure of Earth`s Atmosphere
... Io’s volcanoes blow out sulfur-rich gases → tenuous atmosphere, but gases can not be retained by Io’s gravity → gases escape from Io and form an ion torus in Jupiter’s magnetosphere. ...
... Io’s volcanoes blow out sulfur-rich gases → tenuous atmosphere, but gases can not be retained by Io’s gravity → gases escape from Io and form an ion torus in Jupiter’s magnetosphere. ...
01 - MrPetersenScience
... _______________________________________________________________ 12. How often does Jupiter rotate on its axis? _______________________________________________________________ 13. Jupiter has at least 63 ______________________ , 4 of which are the size of small planets. 14. How much of Jupiter’s atmo ...
... _______________________________________________________________ 12. How often does Jupiter rotate on its axis? _______________________________________________________________ 13. Jupiter has at least 63 ______________________ , 4 of which are the size of small planets. 14. How much of Jupiter’s atmo ...
Do extrasolar planets go bang
... case of H3+ since the perturbations soon became the determining feature, not the basic model. Better understanding of what was happening came from an accurate calculation of the electronic structure of the molecule, by Wilfred Meyer, Peter Botschwina and Peter Burton, and a calculation from first pr ...
... case of H3+ since the perturbations soon became the determining feature, not the basic model. Better understanding of what was happening came from an accurate calculation of the electronic structure of the molecule, by Wilfred Meyer, Peter Botschwina and Peter Burton, and a calculation from first pr ...
jupiter 1
... the solar system. No impact craters have been observed on the moon, indicating that the surface is very young (probably less than one million years old). Io is capable of erasing its craters as fast as they are formed. Unlike the Earth, Io’s main source of internal heat comes from tidal flexing rath ...
... the solar system. No impact craters have been observed on the moon, indicating that the surface is very young (probably less than one million years old). Io is capable of erasing its craters as fast as they are formed. Unlike the Earth, Io’s main source of internal heat comes from tidal flexing rath ...
Institute of Shock Physics: Computational Modelling
... Transfer of material between planets via impact ejecta Impact induced hydrothermal systems may have provided a cradle for early life Environmental catastrophes following impacts leading to mass extinctions ...
... Transfer of material between planets via impact ejecta Impact induced hydrothermal systems may have provided a cradle for early life Environmental catastrophes following impacts leading to mass extinctions ...
Chapter 11 The Jovian Planets
... • Roche Limit - the closest distance an object can come to another object without being pulled apart by tidal forces ...
... • Roche Limit - the closest distance an object can come to another object without being pulled apart by tidal forces ...
Review 3
... The more distant planets formed in a cooler region of the solar nebula and contain as much hydrogen but greater proportion of ices B) They differ due to giant impacts at the late stages of planet formation C) The closer planets formed their cores first and captured more of the gasses D) The more dis ...
... The more distant planets formed in a cooler region of the solar nebula and contain as much hydrogen but greater proportion of ices B) They differ due to giant impacts at the late stages of planet formation C) The closer planets formed their cores first and captured more of the gasses D) The more dis ...
Jupiter - UC Berkeley Astronomy w
... •This is the original Voyager 'Blue Movie' (so named because it was built from blue filter images). It records Voyager 1's approach during a period of 60 Jupiter days. Notice the difference in speed and direction of the various zones of the atmosphere. ...
... •This is the original Voyager 'Blue Movie' (so named because it was built from blue filter images). It records Voyager 1's approach during a period of 60 Jupiter days. Notice the difference in speed and direction of the various zones of the atmosphere. ...
Comet ISON - Lone Star Science with Mr. Zuber
... Comet C/2012 S1 (ISON) • ISON started its journey towards the Sun (out of the Oort Cloud) a few million years ago • Discovered by Russian astronomers, part of the ISON Project (International Scientific Optical Network) in September 2012. • Comet ISON is a sungrazer, a comet that travels close to th ...
... Comet C/2012 S1 (ISON) • ISON started its journey towards the Sun (out of the Oort Cloud) a few million years ago • Discovered by Russian astronomers, part of the ISON Project (International Scientific Optical Network) in September 2012. • Comet ISON is a sungrazer, a comet that travels close to th ...
Comet Shoemaker–Levy 9
Comet Shoemaker–Levy 9 (formally designated D/1993 F2) was a comet that broke apart and collided with Jupiter in July 1994, providing the first direct observation of an extraterrestrial collision of Solar System objects. This generated a large amount of coverage in the popular media, and the comet was closely observed by astronomers worldwide. The collision provided new information about Jupiter and highlighted its role in reducing space debris in the inner Solar System.The comet was discovered by astronomers Carolyn and Eugene M. Shoemaker and David Levy. Shoemaker–Levy 9, at the time captured by and orbiting Jupiter, was located on the night of March 24, 1993, in a photograph taken with the 40 cm (16 in) Schmidt telescope at the Palomar Observatory in California. It was the first comet observed to be orbiting a planet, and had probably been captured by the planet around 20 – 30 years earlier.Calculations showed that its unusual fragmented form was due to a previous closer approach to Jupiter in July 1992. At that time, the orbit of Shoemaker–Levy 9 passed within Jupiter's Roche limit, and Jupiter's tidal forces had acted to pull apart the comet. The comet was later observed as a series of fragments ranging up to 2 km (1.2 mi) in diameter. These fragments collided with Jupiter's southern hemisphere between July 16 and July 22, 1994, at a speed of approximately 60 km/s (37 mi/s) or 216,000 km/h (134,000 mph). The prominent scars from the impacts were more easily visible than the Great Red Spot and persisted for many months.