... _____ 2. Which of the following is the largest planet in our solar system? a. Jupiter b. Earth c. Saturn d. Neptune _____ 3. What makes up the outer part of Jupiter’s atmosphere? a. oxygen, nitrogen, helium b. water, methane, ammonia c. carbon dioxide, oxygen, nitrogen d. hydrogen, oxygen, water ___ ...
Neptune
... They are probably planetesimals that formed within the Kuiper belt. The Kuiper belt Objects are scattered too thinly for them to have accreted into a larger body. ...
... They are probably planetesimals that formed within the Kuiper belt. The Kuiper belt Objects are scattered too thinly for them to have accreted into a larger body. ...
Kuiper belt objects - Rosemary`s ePortfolio
... Discovered in January 2005 by Mike Brown, Chad Trujillo and David Rabinowitz Named after the Greek goddess of discord and strife Eris was what provoked the debate on whether or not Pluto should be classified as a planet. Since Eris is slightly bigger than Pluto, they were both classified as dwarf pl ...
... Discovered in January 2005 by Mike Brown, Chad Trujillo and David Rabinowitz Named after the Greek goddess of discord and strife Eris was what provoked the debate on whether or not Pluto should be classified as a planet. Since Eris is slightly bigger than Pluto, they were both classified as dwarf pl ...
The Solar System At least 7 billion miles across, home to 8 planets
... It was in that distant region of the solar system that in the year 2006 astronomy was shaken to its very core. After almost 80 years Pluto lost its status as the ninth planet. The International Astronomical Union couldn’t ignore findings that similar, even larger bodies than Pluto, traverse the oute ...
... It was in that distant region of the solar system that in the year 2006 astronomy was shaken to its very core. After almost 80 years Pluto lost its status as the ninth planet. The International Astronomical Union couldn’t ignore findings that similar, even larger bodies than Pluto, traverse the oute ...
Slide 1
... Discuss and demonstrate lunar motion, relate to day & night Count and graph moons for each planet Introduce new vocabulary concepts: lunar, satellite, solar, orbit, galaxy, system, cycle • Sing “The Planet Song” to reinforce planetary names and order from the Sun while playing guitar ...
... Discuss and demonstrate lunar motion, relate to day & night Count and graph moons for each planet Introduce new vocabulary concepts: lunar, satellite, solar, orbit, galaxy, system, cycle • Sing “The Planet Song” to reinforce planetary names and order from the Sun while playing guitar ...
The Formation of Uranus and Neptune in the Jupiter
... the cores must have accreted a signi cant amount of gas. Jupiter was most likely the largest core and thus the rst to reach this point since it is closest to the Sun, where the disk density was highest and the timescales shortest. Perhaps Saturn's core was larger than the others (due to stochastic ...
... the cores must have accreted a signi cant amount of gas. Jupiter was most likely the largest core and thus the rst to reach this point since it is closest to the Sun, where the disk density was highest and the timescales shortest. Perhaps Saturn's core was larger than the others (due to stochastic ...
Explained in 60 Seconds: Why Visit a Comet?
... outbursts reveal material from within the comet’s interior, opening a window onto the processes that drove the evolution of the early Solar System. ...
... outbursts reveal material from within the comet’s interior, opening a window onto the processes that drove the evolution of the early Solar System. ...
21trans-neptunian7s
... In the late 1800’s it was believed that Neptune’s orbit was being perturbed by a ...
... In the late 1800’s it was believed that Neptune’s orbit was being perturbed by a ...
meteoroid
... characteristics of shape and orbit in a region in the solar system known as the asteroids? asteroid belt b/t Mars & Jupiter • movement: based on revolution around the Sun • some outside of the asteroid belt have orbits that cross Earth’s orbit & scientists monitor their position ...
... characteristics of shape and orbit in a region in the solar system known as the asteroids? asteroid belt b/t Mars & Jupiter • movement: based on revolution around the Sun • some outside of the asteroid belt have orbits that cross Earth’s orbit & scientists monitor their position ...
The Outer Solar System - Super Teacher Worksheets
... are violent wind storms that circle around Jupiter. The most famous storm is called the Great Red Spot. It has been churning for more than four hundred years and scientists don’t think it will be slowing down any time soon. Jupiter has its own system of moons. At last count Jupiter has sixty-three k ...
... are violent wind storms that circle around Jupiter. The most famous storm is called the Great Red Spot. It has been churning for more than four hundred years and scientists don’t think it will be slowing down any time soon. Jupiter has its own system of moons. At last count Jupiter has sixty-three k ...
Some additional information on Dwarf Planets
... sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a nearly round shape (due to a hydrostatic equilibrium); and (c) has cleared the neighborhood around its orbit. As now defined, the Solar System has eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uran ...
... sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a nearly round shape (due to a hydrostatic equilibrium); and (c) has cleared the neighborhood around its orbit. As now defined, the Solar System has eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uran ...
The Solar System: An Insider`s Guide
... Why is its axis so unusually tilted? Was it due to a massive collision? Why do Uranus and Neptune have so much less hydrogen and helium than Jupiter and Saturn? Is it simply because they are smaller? or because they're farther from the Sun? What will happen to Uranus's weather as it progresses thru ...
... Why is its axis so unusually tilted? Was it due to a massive collision? Why do Uranus and Neptune have so much less hydrogen and helium than Jupiter and Saturn? Is it simply because they are smaller? or because they're farther from the Sun? What will happen to Uranus's weather as it progresses thru ...
How Was the Solar System Formed?
... As the disk continued to spin over millions of years, the mass in the center continued to grow. The temperature increased. Eventually it caught fire, and nuclear fusion began. This event was the birth of our Sun. The disk continued to spin. It contained all the gas and dust that did not go into the ...
... As the disk continued to spin over millions of years, the mass in the center continued to grow. The temperature increased. Eventually it caught fire, and nuclear fusion began. This event was the birth of our Sun. The disk continued to spin. It contained all the gas and dust that did not go into the ...
Module G: Unit 2, Lesson 5 – The Gas Giant Planets
... • Jupiter, Saturn, Uranus, and Neptune are the gas giant planets. • Gas giants have deep, massive gas atmospheres, which are made up mostly of hydrogen and helium. They have no surface to stand on. • The gas giant planets are large and cold. What is known about Jupiter? • Jupiter is the largest plan ...
... • Jupiter, Saturn, Uranus, and Neptune are the gas giant planets. • Gas giants have deep, massive gas atmospheres, which are made up mostly of hydrogen and helium. They have no surface to stand on. • The gas giant planets are large and cold. What is known about Jupiter? • Jupiter is the largest plan ...
GEOL3025, Section 030 Lecture #11 31 August 2007
... AKA Terrestrial Planets (like Earth) AKA Rocky Planets ...
... AKA Terrestrial Planets (like Earth) AKA Rocky Planets ...
How Was the Solar System Formed? Questions
... planets. The Oort Cloud and the Kuiper Belt are in this region of the solar system. Here is where the dwarf planets, comets, and other icy objects exist. We now know our solar system contains eight planets. There are also dwarf planets. We know of at least 178 moons, as well as numerous comets and a ...
... planets. The Oort Cloud and the Kuiper Belt are in this region of the solar system. Here is where the dwarf planets, comets, and other icy objects exist. We now know our solar system contains eight planets. There are also dwarf planets. We know of at least 178 moons, as well as numerous comets and a ...
sorption feature centered near 0.7 µm and attributed → Fe 3+
... System, including physical distribution of objects out through the Kuiper Belt, are not yet fully understood. Unifying these diverse characteristics has been the subject of multiple dynamical studies of the Solar System. The recent “Nice model” [1,2,3] describes a scenario in which the Jovian planet ...
... System, including physical distribution of objects out through the Kuiper Belt, are not yet fully understood. Unifying these diverse characteristics has been the subject of multiple dynamical studies of the Solar System. The recent “Nice model” [1,2,3] describes a scenario in which the Jovian planet ...
Neptune - Milan Area Schools
... supposed to be much smaller than their parent planet. This is yet another reason that Pluto gives astronomers problems in classification. Not only are they about they same size but, they have the same rotational period (6.4 days) Although it is common for a satellite to travel in a synchronous orbit ...
... supposed to be much smaller than their parent planet. This is yet another reason that Pluto gives astronomers problems in classification. Not only are they about they same size but, they have the same rotational period (6.4 days) Although it is common for a satellite to travel in a synchronous orbit ...
Neptune Facts Mr J Neptune is the eighth planet from the sun. It was
... planet, but he mistook it for a star due to its slow motion. In accordance with all the other planets seen in the sky, this new world was given a name from Greek and Roman mythology — Neptune, the Roman god of the sea. ...
... planet, but he mistook it for a star due to its slow motion. In accordance with all the other planets seen in the sky, this new world was given a name from Greek and Roman mythology — Neptune, the Roman god of the sea. ...
Document
... Long, eccentric orbit which goes outside the 9 (or 8) planets Orbital periods can be long or short Comet Shoemaker-Levy 9 slammed into Jupiter’s atmosphere in 1994 ...
... Long, eccentric orbit which goes outside the 9 (or 8) planets Orbital periods can be long or short Comet Shoemaker-Levy 9 slammed into Jupiter’s atmosphere in 1994 ...
Introduction
... • Clyde Tombaugh searches for planet at Lowell Observatory • uses blink comparator • Feb. 1930: discovers object within 6° of Lowell's prediction – Pluto Pluto and Charon ...
... • Clyde Tombaugh searches for planet at Lowell Observatory • uses blink comparator • Feb. 1930: discovers object within 6° of Lowell's prediction – Pluto Pluto and Charon ...
Kuiper Mission Team Presentation
... What is the KBO Discovery Mission? • What has preceded it? New Horizons! • Planetary Telescope • Connections between weather and climate in giant planet atmospheres, satellites, and their external environments • Flexible launch dates; primary mission completed by mid-2024 ...
... What is the KBO Discovery Mission? • What has preceded it? New Horizons! • Planetary Telescope • Connections between weather and climate in giant planet atmospheres, satellites, and their external environments • Flexible launch dates; primary mission completed by mid-2024 ...
Document
... • For a given pressure, “condensation temperature” determines gas or solid phase. • Water, methane, ammonia ~ 100 K • Rocky substances ~ 1500 K • Hydrogen, helium ~ 0K • So hydrogen and helium always are in gas phase. ...
... • For a given pressure, “condensation temperature” determines gas or solid phase. • Water, methane, ammonia ~ 100 K • Rocky substances ~ 1500 K • Hydrogen, helium ~ 0K • So hydrogen and helium always are in gas phase. ...
Gravity - MsAskins
... What keeps objects in orbit in the solar system? • Inertia is the tendency of an object to resist a change in motion. • The greater an object’s mass, the greater its inertia. • Newton’s first law of motion says that an object at rest will stay at rest and an object in motion will stay in motion with ...
... What keeps objects in orbit in the solar system? • Inertia is the tendency of an object to resist a change in motion. • The greater an object’s mass, the greater its inertia. • Newton’s first law of motion says that an object at rest will stay at rest and an object in motion will stay in motion with ...
At this point of its orbit, any solar satellite such as a comet or a
... The planets were formed from these small chunks of dust, rocks and frozen gasses as they collided and stuck together. ...
... The planets were formed from these small chunks of dust, rocks and frozen gasses as they collided and stuck together. ...
Scattered disc
The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets, a subset of the broader family of trans-Neptunian objects. The scattered-disc objects (SDOs) have orbital eccentricities ranging as high as 0.8, inclinations as high as 40°, and perihelia greater than 30 astronomical units (4.5×109 km; 2.8×109 mi). These extreme orbits are thought to be the result of gravitational ""scattering"" by the gas giants, and the objects continue to be subject to perturbation by the planet Neptune.Although the closest scattered-disc objects approach the Sun at about 30–35 AU, their orbits can extend well beyond 100 AU. This makes scattered objects among the most distant and coldest objects in the Solar System. The innermost portion of the scattered disc overlaps with a torus-shaped region of orbiting objects traditionally called the Kuiper belt, but its outer limits reach much farther away from the Sun and farther above and below the ecliptic than the Kuiper belt proper.Because of its unstable nature, astronomers now consider the scattered disc to be the place of origin for most periodic comets in the Solar System, with the centaurs, a population of icy bodies between Jupiter and Neptune, being the intermediate stage in an object's migration from the disc to the inner Solar System. Eventually, perturbations from the giant planets send such objects towards the Sun, transforming them into periodic comets. Many Oort cloud objects are also thought to have originated in the scattered disc. Detached objects are not sharply distinct from scattered disc objects, and some such as Sedna have sometimes been considered to be included in this group.