To Jupiter … and Beyond! - Five Star Publications, Inc.
... 14-year mission by plunging into the dense atmosphere of Jupiter. Moving at more than 100,000 miles per hour, it was crushed, disintegrated and lost forever. But that little spacecraft taught us much about Jupiter. Never fear, your spaceship will not have the same fate. When you get to Jupiter, you ...
... 14-year mission by plunging into the dense atmosphere of Jupiter. Moving at more than 100,000 miles per hour, it was crushed, disintegrated and lost forever. But that little spacecraft taught us much about Jupiter. Never fear, your spaceship will not have the same fate. When you get to Jupiter, you ...
Now - National Geographic Magazine, UK
... The computer simulations by Bottke’s team trace the source of those impacts to a now vanished inner rim of the asteroid belt, which shed asteroids for two billion years after Jupiter disturbed it. According to Bottke, as many as 70 may have struck Earth, each comparable to the one that extinguished ...
... The computer simulations by Bottke’s team trace the source of those impacts to a now vanished inner rim of the asteroid belt, which shed asteroids for two billion years after Jupiter disturbed it. According to Bottke, as many as 70 may have struck Earth, each comparable to the one that extinguished ...
The Outer Planets - Jupiter
... • Jupiter, the largest of the planets, is 2.5 times more massive than all the other planets combined • It is covered by clouds made up of ammonia ice crystals. • Beneath the clouds the atmosphere continues for many thousands of kilometers • Jupiter’s Day is only 9.9 hrs. • A year on Jupiter is 11.9 ...
... • Jupiter, the largest of the planets, is 2.5 times more massive than all the other planets combined • It is covered by clouds made up of ammonia ice crystals. • Beneath the clouds the atmosphere continues for many thousands of kilometers • Jupiter’s Day is only 9.9 hrs. • A year on Jupiter is 11.9 ...
pptx format - Hildas and Trojans
... Jovian Trojans The L4 and L5 “points” are stable. (Actually, there is a region around the L4 and L5 points in which objects can move around and stay – on average- at the same period as the massive object orbiting the Sun) Objects near the L4 and L5 points of the Jupiter-Sun system are in 1:1 reson ...
... Jovian Trojans The L4 and L5 “points” are stable. (Actually, there is a region around the L4 and L5 points in which objects can move around and stay – on average- at the same period as the massive object orbiting the Sun) Objects near the L4 and L5 points of the Jupiter-Sun system are in 1:1 reson ...
JUPITER: King of the Planets
... Density is only 0.687 g/cm3 or 0.125 of Earth's. • The most distant naked eye planet. • Period of 29.42 years. Semi-major axis, a = 9.54 AU, e = 0.054. Inclination to ecliptic = 2.49 deg • 9 moons discovered from the ground. • No solid surface: differential rotation Magnetic (interior) spin period: ...
... Density is only 0.687 g/cm3 or 0.125 of Earth's. • The most distant naked eye planet. • Period of 29.42 years. Semi-major axis, a = 9.54 AU, e = 0.054. Inclination to ecliptic = 2.49 deg • 9 moons discovered from the ground. • No solid surface: differential rotation Magnetic (interior) spin period: ...
Slide 1 - WordPress.com
... Astronomers have found at least 146 moons orbiting planets in our solar system. Another 27 moons are awaiting official confirmation of their discovery. This number does not include the six moons of the dwarf planets, nor does this tally include the tiny satellites that orbit some asteroids and other ...
... Astronomers have found at least 146 moons orbiting planets in our solar system. Another 27 moons are awaiting official confirmation of their discovery. This number does not include the six moons of the dwarf planets, nor does this tally include the tiny satellites that orbit some asteroids and other ...
Extrasolar Planets: The (more or less) Standard Theory for Planet
... Minimum mass of the disk: probably ~ 0.01MO , similar to masses of observed disks (although these are very uncertain). Note that the sum of our solar system’s planets’ masses is about 0.001Mo (mostly Jupiter), but this is partly because most of the hydrogen and helium have been lost (escaped from pl ...
... Minimum mass of the disk: probably ~ 0.01MO , similar to masses of observed disks (although these are very uncertain). Note that the sum of our solar system’s planets’ masses is about 0.001Mo (mostly Jupiter), but this is partly because most of the hydrogen and helium have been lost (escaped from pl ...
16gasgiants2s
... The gas giants are not perfectly round, they are oblate due to rotation Degree of oblateness depends on mass distribution ...
... The gas giants are not perfectly round, they are oblate due to rotation Degree of oblateness depends on mass distribution ...
Survey of the Solar System
... history Mars’s two moons resemble asteroids; may be captured from the nearby Main Belt. ...
... history Mars’s two moons resemble asteroids; may be captured from the nearby Main Belt. ...
Astronomy Chapter 10 – The Outer Planets A. Main Ideas Beyond
... ⇒ Neptune’s blue color is caused by the abundance of methane in its atmosphere, just like Uranus. Unlike Uranus, however, Neptune has cloud belts and high winds caused by the convection currents that rise to its outer atmosphere • Rings and Moons ⇒ Neptune has very narrow rings like Uranus, but are ...
... ⇒ Neptune’s blue color is caused by the abundance of methane in its atmosphere, just like Uranus. Unlike Uranus, however, Neptune has cloud belts and high winds caused by the convection currents that rise to its outer atmosphere • Rings and Moons ⇒ Neptune has very narrow rings like Uranus, but are ...
The Discovery of Planet X
... are called plutinos, after their most prominent member, Pluto. Classical Kuiper belt objects (also called cubewanos) have no such resonance, moving on almost circular orbits, unperturbed by Neptune. Examples are Quaoar and Makemake. The scattered disk contains objects further from the Sun, usually w ...
... are called plutinos, after their most prominent member, Pluto. Classical Kuiper belt objects (also called cubewanos) have no such resonance, moving on almost circular orbits, unperturbed by Neptune. Examples are Quaoar and Makemake. The scattered disk contains objects further from the Sun, usually w ...
The Outer Planets
... • All are tens of thousands of miles across – Much larger than the inner planets ...
... • All are tens of thousands of miles across – Much larger than the inner planets ...
1 The Outer Planets: Jupiter, Saturn, Uranus, Neptune
... - The outer planets are furthest from the sun. - They are: Jupiter, Saturn, Uranus, and Neptune - These are giant planets called Jovian Planets, Planets, named for Jupiter. - Made mostly of gas so they have low density. density. ...
... - The outer planets are furthest from the sun. - They are: Jupiter, Saturn, Uranus, and Neptune - These are giant planets called Jovian Planets, Planets, named for Jupiter. - Made mostly of gas so they have low density. density. ...
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 ...
Lecture 5. Origin of the Solar System, Formation of the Earth
... Realized if solid, gravity would disrupt it. Calculated Saturn must be a rotating sphere of gas. If mass in the center, periphery rotates rapidly, outer part distends outward to form disk If spinning faster, would form a ring. If gravitational interactions in the ring, get several rings. Then reason ...
... Realized if solid, gravity would disrupt it. Calculated Saturn must be a rotating sphere of gas. If mass in the center, periphery rotates rapidly, outer part distends outward to form disk If spinning faster, would form a ring. If gravitational interactions in the ring, get several rings. Then reason ...
Planets, Galaxies and Constellations
... significantly smaller objects, such as dwarf planets and small Solar System bodies. Of the objects that orbit the Sun indirectly, the moons, two are larger than the smallest planet, Mercury. ...
... significantly smaller objects, such as dwarf planets and small Solar System bodies. Of the objects that orbit the Sun indirectly, the moons, two are larger than the smallest planet, Mercury. ...
Distance from Sun - Barnhill-Memorial
... Earth hours long. Year length: One year on Jupiter is 11.86 Earth years long. Moons: Jupiter has 39 moons. The four largest are Io, Europa, Ganymede, and ...
... Earth hours long. Year length: One year on Jupiter is 11.86 Earth years long. Moons: Jupiter has 39 moons. The four largest are Io, Europa, Ganymede, and ...
The Gas Giant Planets
... huge size because it is composed of lightweight elements. – Hydrogen and helium make up the majority of Jupiter’s atmospheric gas. – Below the liquid hydrogen, there is a layer of liquid metallic hydrogen. – Liquid metallic hydrogen is a form of hydrogen that has properties of both a liquid and a me ...
... huge size because it is composed of lightweight elements. – Hydrogen and helium make up the majority of Jupiter’s atmospheric gas. – Below the liquid hydrogen, there is a layer of liquid metallic hydrogen. – Liquid metallic hydrogen is a form of hydrogen that has properties of both a liquid and a me ...
Moons, Rings, Pluto and other Solar System Debris
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
Review for Test #2 March 9
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
Powerpoint for today
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
Life in the Universe lab1
... Main belt: It is thought that this material “should’ve” formed a planet between Mars and Jupiter, based on models, but that Jupiter’s gravity prevented it from forming. Which resulted in this asteroid belt. The amount of material that makes up the main asteroid belt is quite small, all the asteroids ...
... Main belt: It is thought that this material “should’ve” formed a planet between Mars and Jupiter, based on models, but that Jupiter’s gravity prevented it from forming. Which resulted in this asteroid belt. The amount of material that makes up the main asteroid belt is quite small, all the asteroids ...