Outer Planets - MrTravisSciencePage
... Neptune • Neptune’s atmosphere is similar to Uranus’s – Hydrogen, helium,methane & nitrogen – The core/center of Neptune is probably ice and rock – Called an “ice giant like Uranus ...
... Neptune • Neptune’s atmosphere is similar to Uranus’s – Hydrogen, helium,methane & nitrogen – The core/center of Neptune is probably ice and rock – Called an “ice giant like Uranus ...
Our Solar System
... terrestrial worlds — Mercury, Venus, Earth and Mars. After that are four gas giants — Jupiter, Saturn, Uranus and Neptune. Between the orbits of Mars and Jupiter lies the asteroid belt, which includes the dwarf planet Ceres. Beyond the orbit of Neptune one finds the disk-shaped Kuiper belt, in which ...
... terrestrial worlds — Mercury, Venus, Earth and Mars. After that are four gas giants — Jupiter, Saturn, Uranus and Neptune. Between the orbits of Mars and Jupiter lies the asteroid belt, which includes the dwarf planet Ceres. Beyond the orbit of Neptune one finds the disk-shaped Kuiper belt, in which ...
Planets Around Sun
... than 0.1 AU all reside in circular orbits, plausibly induced by tidal interactions with the host star. In contrast, all 9 planet candidates that orbit farther than 0.2 AU (out to 2.5 AU) reside in eccentric orbits with ellipticities, e>0.1, more elliptical than the orbits of Jupiter (e=0.048) and Ea ...
... than 0.1 AU all reside in circular orbits, plausibly induced by tidal interactions with the host star. In contrast, all 9 planet candidates that orbit farther than 0.2 AU (out to 2.5 AU) reside in eccentric orbits with ellipticities, e>0.1, more elliptical than the orbits of Jupiter (e=0.048) and Ea ...
Video review
... 1. _______________ is greater in volume than all of the other planets combined. 2. In the most distant part of Pluto’s eccentric orbit, its atmosphere turns from gas to ___________. 3. The largest planetary storm system is Jupiter’s ________________________. 4. Cassini used a ______________ from Ven ...
... 1. _______________ is greater in volume than all of the other planets combined. 2. In the most distant part of Pluto’s eccentric orbit, its atmosphere turns from gas to ___________. 3. The largest planetary storm system is Jupiter’s ________________________. 4. Cassini used a ______________ from Ven ...
Chapter Overview
... thin atmosphere of mostly carbon dioxide. The surface of Mars shares many features in common with Earth. There are shield volcanoes (extinct) and a deep canyon that indicate that tectonic activity once occurred on Mars, and there are erosional features—dried river and lake beds, gullies, and runoff ...
... thin atmosphere of mostly carbon dioxide. The surface of Mars shares many features in common with Earth. There are shield volcanoes (extinct) and a deep canyon that indicate that tectonic activity once occurred on Mars, and there are erosional features—dried river and lake beds, gullies, and runoff ...
Other tenants
... We have already mentioned that the planets with their satellites and rings are not the only bodies that occupy the Solar System. To start with, between the orbits of Mars and Jupiter, there is the Main Asteroid Belt that is not just a flat disc with rocks of different sizes and shapes as we usually ...
... We have already mentioned that the planets with their satellites and rings are not the only bodies that occupy the Solar System. To start with, between the orbits of Mars and Jupiter, there is the Main Asteroid Belt that is not just a flat disc with rocks of different sizes and shapes as we usually ...
A Tour of Our Solar System
... • Kuiper Belt: rocky/icy objects beyond Pluto. – Short orbit comets (orbit less than 100 years). ...
... • Kuiper Belt: rocky/icy objects beyond Pluto. – Short orbit comets (orbit less than 100 years). ...
The Solar System
... and comets Halley and Hale-Bopp are shown. The brighter color is used for the portion of the orbit above the ecliptic plane. Trans-Neptunian objects larger than about 700 km in diameter are shown as white diamonds, ...
... and comets Halley and Hale-Bopp are shown. The brighter color is used for the portion of the orbit above the ecliptic plane. Trans-Neptunian objects larger than about 700 km in diameter are shown as white diamonds, ...
Long-period
... New Horizons Mission • Launch January, 2006 •Swing by Jupiter in 2007 •Pass by Pluto/Charon 2015, ASAP, before atmosphere freezes out. • Kuiper belt by 2026 ...
... New Horizons Mission • Launch January, 2006 •Swing by Jupiter in 2007 •Pass by Pluto/Charon 2015, ASAP, before atmosphere freezes out. • Kuiper belt by 2026 ...
How the Universe Works – Planets
... 22. Auroras on Jupiter and Saturn are proof that Gas Giants have ____________ ____________, too. 23. Why will we probably never really figure out what’s at Jupiter’s core? ...
... 22. Auroras on Jupiter and Saturn are proof that Gas Giants have ____________ ____________, too. 23. Why will we probably never really figure out what’s at Jupiter’s core? ...
How the Universe Works – Planets Astronomy Name: Date: 1. How
... 22. Auroras on Jupiter and Saturn are proof that Gas Giants have ____________ ____________, too. 23. Why will we probably never really figure out what’s at Jupiter’s core? ...
... 22. Auroras on Jupiter and Saturn are proof that Gas Giants have ____________ ____________, too. 23. Why will we probably never really figure out what’s at Jupiter’s core? ...
Outer Planets and Moons Notes
... What are Uranus’s mass, density, radius (diameter divided by 2), rotation period, and period of revolution? How do they compare with Earth? ...
... What are Uranus’s mass, density, radius (diameter divided by 2), rotation period, and period of revolution? How do they compare with Earth? ...
28.1-notes - Stout Middle School
... the planets and satellites is called debris. Most of this debris diminished as it crashed into planets or was diverted out of the solar system. Some of the debris that remained became icy objects called comets. Other debris formed rocky planetesimals called asteroids. Most asteroids are found in the ...
... the planets and satellites is called debris. Most of this debris diminished as it crashed into planets or was diverted out of the solar system. Some of the debris that remained became icy objects called comets. Other debris formed rocky planetesimals called asteroids. Most asteroids are found in the ...
class16.ppt [Read-Only] - University of Texas Astronomy Home Page
... cores form first, then their gravity draws in gases 2. Gravitational Instability: clumps of gas form within a protoplanetary disk, they have strong enough gravity to collapse rapidly ...
... cores form first, then their gravity draws in gases 2. Gravitational Instability: clumps of gas form within a protoplanetary disk, they have strong enough gravity to collapse rapidly ...
Title: "Pluto - New Horizons Mission to the Edge of the Solar System"
... worlds combined - yet, no spacecraft has been sent to a planet in this class. NASA's New Horizons mission to Pluto, its moon Charon and the Kuiper Belt is provisionally planned for launch in January 2006. After using a flyby of Jupiter in 2007 to get a gravitational kick, the spacecraft will reach P ...
... worlds combined - yet, no spacecraft has been sent to a planet in this class. NASA's New Horizons mission to Pluto, its moon Charon and the Kuiper Belt is provisionally planned for launch in January 2006. After using a flyby of Jupiter in 2007 to get a gravitational kick, the spacecraft will reach P ...
NS2-M3C15_-_The_Planets_Exam
... surface temperature as high as 800 F smallest of the inner planets none of the above are true ...
... surface temperature as high as 800 F smallest of the inner planets none of the above are true ...
Chapter 7 – Our Planetary System 7.1 Studying the Solar System
... Rings are ________________________; they are made of countless small chunks of ice and rock, each orbiting like a tiny moon. ...
... Rings are ________________________; they are made of countless small chunks of ice and rock, each orbiting like a tiny moon. ...
A Brief History of Planetary Science
... Find time to get half way there and double it In general, distance equals ½at2 ...
... Find time to get half way there and double it In general, distance equals ½at2 ...
Page one 2011 November Rock Magnet
... “Hello, I am called Jupiter, after the Roman God Jupiter! I am the fifth planet from the SUN and largest planet in our Solar System. I am a Gas Giant, the third brightest object in the night sky after the Moon and Venus. My gasses are hydrogen and helium and I am thought to have a rocky core of heav ...
... “Hello, I am called Jupiter, after the Roman God Jupiter! I am the fifth planet from the SUN and largest planet in our Solar System. I am a Gas Giant, the third brightest object in the night sky after the Moon and Venus. My gasses are hydrogen and helium and I am thought to have a rocky core of heav ...
HW Solar System Mnemonic
... The asteroid belt is the region of the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets. The asteroid belt region is also termed the main belt to distinguish it from other concentra ...
... The asteroid belt is the region of the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets. The asteroid belt region is also termed the main belt to distinguish it from other concentra ...
File - CVHS Chicklas
... • Shines because it is hot: – Surface Temp ~6000 C – Mostly Visible, UV & IR light ...
... • Shines because it is hot: – Surface Temp ~6000 C – Mostly Visible, UV & IR light ...
579 The Family of the Sun The Inner Planets The Outer Planets The
... Millions of Tiny Planets between Mars and Jupiter • State the nature and location in space of asteroids and describe the likelihood and danger of collisions with them. ...
... Millions of Tiny Planets between Mars and Jupiter • State the nature and location in space of asteroids and describe the likelihood and danger of collisions with them. ...