Gravity Articles
... As the scientists tell it, it starts a few million years after the Solar System's birth. At first, the four giant planets had tight orbits. Neptune, for example, was only half as far away from the Sun as it now. A slowly circulating band of ice, dust, and gas lay beyond these planets. Ice, dust, and ...
... As the scientists tell it, it starts a few million years after the Solar System's birth. At first, the four giant planets had tight orbits. Neptune, for example, was only half as far away from the Sun as it now. A slowly circulating band of ice, dust, and gas lay beyond these planets. Ice, dust, and ...
Jupiter and Saturn: Lords of the Planets Chapter Fourteen
... Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 6. How do astronomers know about the deep interiors of Jupiter a ...
... Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 6. How do astronomers know about the deep interiors of Jupiter a ...
7.5 X 12 long title.p65 - Beck-Shop
... close to their planet were discovered from spacecraft flybys. All major satellites, except Triton, orbit the respective planet in a prograde manner (i.e., in the direction that the planet rotates), close to the planet’s equatorial plane. Small, close-in moons are also exclusively in lowinclination, l ...
... close to their planet were discovered from spacecraft flybys. All major satellites, except Triton, orbit the respective planet in a prograde manner (i.e., in the direction that the planet rotates), close to the planet’s equatorial plane. Small, close-in moons are also exclusively in lowinclination, l ...
Lecture 12 - Seattle Central College
... - Volatiles more prevalent further away from Sun - Jupiter and Saturn’s larger masses allowed them to trap H and He ...
... - Volatiles more prevalent further away from Sun - Jupiter and Saturn’s larger masses allowed them to trap H and He ...
What happened to Pluto?
... • This new find, named Ceres, must be really small. • But an even bigger problem soon became apparent: Three more similar objects were found over the next six years: Pallas, Juno and Vesta. • One small planet, maybe, but four? • Luckily, no more “asteroids” followed, at least for a while... ...
... • This new find, named Ceres, must be really small. • But an even bigger problem soon became apparent: Three more similar objects were found over the next six years: Pallas, Juno and Vesta. • One small planet, maybe, but four? • Luckily, no more “asteroids” followed, at least for a while... ...
Comparative Planetology of the Outer Planets A Travel Guide to the
... • Orbit highly inclined (17o) against other planets’ orbits → Neptune and Pluto will never collide. • Surface covered with nitrogen ice; traces of frozen methane and carbon monoxide. • Daytime temperature (50 K) enough to vaporize some N and CO to form a very tenuous atmosphere. ...
... • Orbit highly inclined (17o) against other planets’ orbits → Neptune and Pluto will never collide. • Surface covered with nitrogen ice; traces of frozen methane and carbon monoxide. • Daytime temperature (50 K) enough to vaporize some N and CO to form a very tenuous atmosphere. ...
The Jovian Planets
... Saturn and Uranus both have rings Scientists decided to look for rings around Jupiter. As it turns out, Jupiter also has a ring. It is VERY small, and difficult to see because of solar radiation. The Probe Voyager I was able to take pictures of the ring ...
... Saturn and Uranus both have rings Scientists decided to look for rings around Jupiter. As it turns out, Jupiter also has a ring. It is VERY small, and difficult to see because of solar radiation. The Probe Voyager I was able to take pictures of the ring ...
The Jovian Planets
... Saturn and Uranus both have rings Scientists decided to look for rings around Jupiter. As it turns out, Jupiter also has a ring. It is VERY small, and difficult to see because of solar radiation. The Probe Voyager I was able to take pictures of the ring ...
... Saturn and Uranus both have rings Scientists decided to look for rings around Jupiter. As it turns out, Jupiter also has a ring. It is VERY small, and difficult to see because of solar radiation. The Probe Voyager I was able to take pictures of the ring ...
Astronomy
... Moons of Neptune Neptune has 13 known moons. Most are small icy bodies similar to the small moons of Uranus. Triton is the one large moon. Triton is in a retrograde orbit around Neptune. The orbit is inclined by 23o. It probably formed else where in the solar system. It surface is mainly water ice ...
... Moons of Neptune Neptune has 13 known moons. Most are small icy bodies similar to the small moons of Uranus. Triton is the one large moon. Triton is in a retrograde orbit around Neptune. The orbit is inclined by 23o. It probably formed else where in the solar system. It surface is mainly water ice ...
Chapter 8 Jovian Planet Systems
... Why do the jovian planets have rings? • Ring particles are too small to survive for very long periods of time • So there must be a continuous replacement of them • The most likely source is continuing impacts between small jovian moons ...
... Why do the jovian planets have rings? • Ring particles are too small to survive for very long periods of time • So there must be a continuous replacement of them • The most likely source is continuing impacts between small jovian moons ...
Chapter 8 (in pdf)
... Which of these facts is NOT explained by the nebular theory? a) There are two main types of planets: terrestrial and jovian. b) Planets orbit in same direction and plane. c) Existence of asteroids and comets. d) Number of planets of each type (4 terrestrial and 4 jovian). ...
... Which of these facts is NOT explained by the nebular theory? a) There are two main types of planets: terrestrial and jovian. b) Planets orbit in same direction and plane. c) Existence of asteroids and comets. d) Number of planets of each type (4 terrestrial and 4 jovian). ...
File
... Our Solar System has eight known planets divided into two categories – the inner and the outer planets. The first group consists of the four ones that are closest to the Sun: Mercury, Venus, Earth, and Mars. They are also called terrestrial or rocky planets and are separated from the second group by ...
... Our Solar System has eight known planets divided into two categories – the inner and the outer planets. The first group consists of the four ones that are closest to the Sun: Mercury, Venus, Earth, and Mars. They are also called terrestrial or rocky planets and are separated from the second group by ...
Astronomy Assignment #1
... ALL planets begin with the accumulation of solid material. In the Solar Nebula, close to the Sun temperatures were too high to allow ices to condense and only rock was solid. Far from the Sun temperatures were low enough that ices could condense as well as rock. The boundary between these regions is ...
... ALL planets begin with the accumulation of solid material. In the Solar Nebula, close to the Sun temperatures were too high to allow ices to condense and only rock was solid. Far from the Sun temperatures were low enough that ices could condense as well as rock. The boundary between these regions is ...
A Comet Nucleus
... The Outer Solar System Summary of Important Features Beyond Neptune, there are at least 70,000 ice/rock bodies with diameters larger than 100 km and orbits of radius 30 to more than 50 AU. This ring of bodies (cf. the Asteroid belt) is called the Kuiper belt. Astronomers believe that it is the sour ...
... The Outer Solar System Summary of Important Features Beyond Neptune, there are at least 70,000 ice/rock bodies with diameters larger than 100 km and orbits of radius 30 to more than 50 AU. This ring of bodies (cf. the Asteroid belt) is called the Kuiper belt. Astronomers believe that it is the sour ...
The Solar System - MrDanielASBSukMSSci
... Venus This figure combines images of Venus taken from space with a camera (left) and radar (right). The camera image shows Venus’s thick atmosphere. Radar is able to penetrate Venus’s clouds to reveal the surface. Both images are false color. ...
... Venus This figure combines images of Venus taken from space with a camera (left) and radar (right). The camera image shows Venus’s thick atmosphere. Radar is able to penetrate Venus’s clouds to reveal the surface. Both images are false color. ...
Question 2 (9-3 thru 9-4 PPT Questions)
... thought to be the result of a close-orbiting, icy moon that was shattered by a collision with a passing asteroid. Another possibility is that an object from the outer solar system came too close to Saturn and was torn apart by the planet’s gravity. ...
... thought to be the result of a close-orbiting, icy moon that was shattered by a collision with a passing asteroid. Another possibility is that an object from the outer solar system came too close to Saturn and was torn apart by the planet’s gravity. ...
the Solar System PowerPoint
... exchanging orbits with one another in a "waltz" -- they are called the coorbital satellites. ...
... exchanging orbits with one another in a "waltz" -- they are called the coorbital satellites. ...
Elliptic Orbits
... However, that is not the whole story: what if a rogue planet comes flying towards the Solar System from outer space? What kind of orbit will it follow as it encounters the Sun’s gravity? In fact, our analysis of the equations of motion is equally valid in this case, and the ( r , θ ) equation is the ...
... However, that is not the whole story: what if a rogue planet comes flying towards the Solar System from outer space? What kind of orbit will it follow as it encounters the Sun’s gravity? In fact, our analysis of the equations of motion is equally valid in this case, and the ( r , θ ) equation is the ...
ppt version
... • Accrete H & He gas from the Solar Nebula. • Planets with the biggest cores grow rapidly. ...
... • Accrete H & He gas from the Solar Nebula. • Planets with the biggest cores grow rapidly. ...
Neptune - Midland ISD
... storm system was discovered by NASA's Voyager 2 spacecraft. The storm resembled the Great Red Spot of Jupiter. Some five years later, on 2 November 1994, the Hubble Space Telescope did not see the Great Dark Spot on the planet. Instead, a new storm similar to the Great Dark Spot was found in the pla ...
... storm system was discovered by NASA's Voyager 2 spacecraft. The storm resembled the Great Red Spot of Jupiter. Some five years later, on 2 November 1994, the Hubble Space Telescope did not see the Great Dark Spot on the planet. Instead, a new storm similar to the Great Dark Spot was found in the pla ...
The formation of the Solar system
... During the collapse of the gaseous nebula, most of the material tended to collect far from the Sun because of the large centrifugal forces, which provided the necessary material to build the large Jovian planets The large gravitational forces of Jupiter tended to prevent planet formation in the inne ...
... During the collapse of the gaseous nebula, most of the material tended to collect far from the Sun because of the large centrifugal forces, which provided the necessary material to build the large Jovian planets The large gravitational forces of Jupiter tended to prevent planet formation in the inne ...
Intro to Solar System
... Saturn - Atmosphere •belts - driven by rapid rotation •period - 10 hrs 14 min •storms at intervals of 30 years •mostly H, He, some methane, water vapor, ammonia •clouds - less colorful than Jupiter, yellow and orange •winds 500 m/s near equator Intro to Solar System ...
... Saturn - Atmosphere •belts - driven by rapid rotation •period - 10 hrs 14 min •storms at intervals of 30 years •mostly H, He, some methane, water vapor, ammonia •clouds - less colorful than Jupiter, yellow and orange •winds 500 m/s near equator Intro to Solar System ...