Chapter 7 PowerPoint
... – Mercury & Venus have no moons – Earth has one moon – Mars has two moons – Pluto has five moons – All Jovian planets have many moons – All Solar System moons are terrestrial objects • Solid surfaces ...
... – Mercury & Venus have no moons – Earth has one moon – Mars has two moons – Pluto has five moons – All Jovian planets have many moons – All Solar System moons are terrestrial objects • Solid surfaces ...
Astr 557 - The origin and early evolution of the solar system
... Heated by internal dissipation Viscosity driven turbulence causes mass & angular momentum distribution Viscosity due to magneto-rotational instability (MRI) or other casues ...
... Heated by internal dissipation Viscosity driven turbulence causes mass & angular momentum distribution Viscosity due to magneto-rotational instability (MRI) or other casues ...
Document
... Mars has gigantic volcanos on its surface that grow to a hundred times larger than it does on Earth. ...
... Mars has gigantic volcanos on its surface that grow to a hundred times larger than it does on Earth. ...
Dwarf Planets - cloudfront.net
... • Has enough mass so that gravity makes them roughly spherical • But have not cleared their orbit of other objects ...
... • Has enough mass so that gravity makes them roughly spherical • But have not cleared their orbit of other objects ...
other objects in solar system
... because the dust tail is often slightly curved, it follows the orbit of the comet, while the gas or ion tail is more strongly affected by the solar winds and is pushed away from the sun. ...
... because the dust tail is often slightly curved, it follows the orbit of the comet, while the gas or ion tail is more strongly affected by the solar winds and is pushed away from the sun. ...
Solar System-3
... Here's a real challenge. If you watch the graph in the model, you will notice that the Earth-Sun distance changes with two different rhythms – a short cycle and a longer more gradual cycle. See if you can figure out what each of these rhythms corresponds to and what causes it. Here are some hints: C ...
... Here's a real challenge. If you watch the graph in the model, you will notice that the Earth-Sun distance changes with two different rhythms – a short cycle and a longer more gradual cycle. See if you can figure out what each of these rhythms corresponds to and what causes it. Here are some hints: C ...
1. Name the planet*..
... 27. How did the planets and other objects in the solar system form out of material in a disk? • The solid material stuck together in clumps, and the clumps stuck together and became larger. 28. Why do the planets all orbit in one direction? • The planets formed out of material that was moving aroun ...
... 27. How did the planets and other objects in the solar system form out of material in a disk? • The solid material stuck together in clumps, and the clumps stuck together and became larger. 28. Why do the planets all orbit in one direction? • The planets formed out of material that was moving aroun ...
hw3
... Describe Pluto. Describe a typical Kupier Belt Object. How would you classify Pluto – as a planet or Kupier Belt Object? Support your answer. Kupier Belt Objects are small icy planetesimals that lie beyond the orbit of Neptune (30AU) out to 50AU from the Sun. Pluto is the outermost planet with semi ...
... Describe Pluto. Describe a typical Kupier Belt Object. How would you classify Pluto – as a planet or Kupier Belt Object? Support your answer. Kupier Belt Objects are small icy planetesimals that lie beyond the orbit of Neptune (30AU) out to 50AU from the Sun. Pluto is the outermost planet with semi ...
Acquaintance with solar system. By Edgaras Montvila 6D
... Uranus is named after the ancient Greek deity of the sky Uranus, the father of Cronus (Saturn ) and grandfather of Zeus( Jupiter). Surface temperature varies from –197.2 °C to ? °C. Uranus has a ring system. The planet system has a unique configuration among those of the planets because its axis of ...
... Uranus is named after the ancient Greek deity of the sky Uranus, the father of Cronus (Saturn ) and grandfather of Zeus( Jupiter). Surface temperature varies from –197.2 °C to ? °C. Uranus has a ring system. The planet system has a unique configuration among those of the planets because its axis of ...
Planetary Chart
... - atmospheres formed from gases that poured out of volcanoes (atmosphere can make a surface warmer and more uniform in temperature) - four types of processes that shape planets’ surfaces (tectonics, volcanism, weathering and erosion, impact cratering) - asteroids are also located in the inner solar ...
... - atmospheres formed from gases that poured out of volcanoes (atmosphere can make a surface warmer and more uniform in temperature) - four types of processes that shape planets’ surfaces (tectonics, volcanism, weathering and erosion, impact cratering) - asteroids are also located in the inner solar ...
chapter7OurPlanetary..
... – Venus: Same size as Earth but much hotter – Earth: Only planet with liquid water on surface – Mars: Could have had liquid water in past – Jupiter: A gaseous giant – Saturn: Gaseous with spectacular rings – Uranus: A gas giant with a highly tilted axis – Neptune: Similar to Uranus but with normal a ...
... – Venus: Same size as Earth but much hotter – Earth: Only planet with liquid water on surface – Mars: Could have had liquid water in past – Jupiter: A gaseous giant – Saturn: Gaseous with spectacular rings – Uranus: A gas giant with a highly tilted axis – Neptune: Similar to Uranus but with normal a ...
Our Solar System
... All other objects in the solar system _________________________ around the sun in elliptical orbits at different speeds. 2. How did our solar system form? A ____________________________ of gas, ice, and dust slowly formed in space, and rotated in space. The cloud began to ________________________ ...
... All other objects in the solar system _________________________ around the sun in elliptical orbits at different speeds. 2. How did our solar system form? A ____________________________ of gas, ice, and dust slowly formed in space, and rotated in space. The cloud began to ________________________ ...
What else is in our solar system, besides the sun, the planets, and
... colored orange. The four outer planets are blue. Neptune's few known Trojan asteroids are yellow, while Jupiter's are pink. The scattered objects between the Sun and the Kuiper belt are known as centaurs. The scale is in astronomical units. The pronounced gap at the bottom is due to obscuration by t ...
... colored orange. The four outer planets are blue. Neptune's few known Trojan asteroids are yellow, while Jupiter's are pink. The scattered objects between the Sun and the Kuiper belt are known as centaurs. The scale is in astronomical units. The pronounced gap at the bottom is due to obscuration by t ...
Our Sidewalk Flier — in PDF format
... SATURN, the sixth planet from the Sun, is the most distant of the five planets known to ancient stargazers. In 1611, Italian Galileo Galilei was the first astronomer to gaze at Saturn through a telescope. Like Jupiter, Uranus, and Neptune, Saturn is a gas giant. It is made mostly of helium and hydroge ...
... SATURN, the sixth planet from the Sun, is the most distant of the five planets known to ancient stargazers. In 1611, Italian Galileo Galilei was the first astronomer to gaze at Saturn through a telescope. Like Jupiter, Uranus, and Neptune, Saturn is a gas giant. It is made mostly of helium and hydroge ...
STATE UNIVERSITY OF NEW YORK COLLEGE OF TECHNOLOGY CANTON, NEW YORK
... F. Resolution, the atmosphere, and astronomy in practice The formation of stars and planets A. Molecular clouds start the process B. Protostars becoming stars C. The birth of planets D. Compare and contrast the composition and characteristics of the eight planets The inner terrestrial planets A. The ...
... F. Resolution, the atmosphere, and astronomy in practice The formation of stars and planets A. Molecular clouds start the process B. Protostars becoming stars C. The birth of planets D. Compare and contrast the composition and characteristics of the eight planets The inner terrestrial planets A. The ...
Moonstruck Scientists Count 63 and Rising
... It is a rare person who knows the answer—63 moons and climbing. Just last year, two more satellites were discovered circling counterclockwise around Uranus, the seventh planet from the sun. It’s almost inconceivable there aren’t more moons out there.” Said Brett Gladman, an astronomer at Cornell Uni ...
... It is a rare person who knows the answer—63 moons and climbing. Just last year, two more satellites were discovered circling counterclockwise around Uranus, the seventh planet from the sun. It’s almost inconceivable there aren’t more moons out there.” Said Brett Gladman, an astronomer at Cornell Uni ...
Nice model
The Nice model (/ˈniːs/) is a scenario for the dynamical evolution of the Solar System. It is named for the location of the Observatoire de la Côte d'Azur, where it was initially developed, in Nice, France. It proposes the migration of the giant planets from an initial compact configuration into their present positions, long after the dissipation of the initial protoplanetary gas disk. In this way, it differs from earlier models of the Solar System's formation. This planetary migration is used in dynamical simulations of the Solar System to explain historical events including the Late Heavy Bombardment of the inner Solar System, the formation of the Oort cloud, and the existence of populations of small Solar System bodies including the Kuiper belt, the Neptune and Jupiter Trojans, and the numerous resonant trans-Neptunian objects dominated by Neptune. Its success at reproducing many of the observed features of the Solar System means that it is widely accepted as the current most realistic model of the Solar System's early evolution, though it is not universally favoured among planetary scientists. One of its limitations is reproducing the outer-system satellites and the Kuiper belt (see below).