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Transcript
The Gas Giants Astronomy Lesson 13 The four outer planets: Jupiter, Saturn, Uranus, and Neptune, are much larger and more massive than Earth, and they do not have solid surfaces. Because these planets are so large and composed of gases, they are commonly referred to as the gas giants. Like the sun, the gas giants are comprised of mainly hydrogen and helium. Because they are so massive, the gas giants have a much larger gravitational force than the terrestrial planets. This increased gravity prevents the gases of the planet from escaping, so they have thick atmospheres. Because of the gravitational pull and thick atmospheres, the pressure inside the planet is enormous. Thus, the hydrogen and helium comprising the planet is in liquid form. Because the gas giants are so far from the sun, their outer layers are extremely cold. But, due to the increased pressure inside the planet, temperature increased greatly within the planet. Each gas giant has many moons and is surrounded by a set of rings. A ring is a thin disk of small particles of ice and rock. Jupiter Jupiter is the largest and most massive of the planets. In fact, it is 2 ½ times larger than all of the other planets combined! Scientists think that Jupiter, like the other gas giants, probably has a dense core of rock and iron. This inner core is overlaid by a deep layer of metallic hydrogen. Jupiter also has four moons: Io, Europa, Genymede, and Callisto. The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. A prominent result is the Great Red Spot, a giant storm that is known to have existed since at least the seventeenth century. Saturn The second-largest planet in the solar system is Saturn. Saturn also has a thick atmosphere made up of helium and hydrogen. Saturn's interior is similar to that of Jupiter, having a small rocky core surrounded mostly by hydrogen and helium. The rocky core is similar in composition to the Earth, but denser. Above this, there is a thicker liquid metallic hydrogen layer, followed by a layer of liquid hydrogen and helium, and in the outermost 1,000 kilometers (600 mi) a gaseous atmosphere. Saturn has the most spectacular rings of any planet. These rings are made up of chunks of ice and rock, each orbiting the planet. Saturn’s rings are very thin and broad, like a CD with a planet in the hole. Saturn’s largest moon, Titan, is larger than the planet Mercury. Saturn has at least 60 moons, but NASA and astronomers are discovering new moons all the time! Uranus Although the gas giant Uranus is about four times the diameter (what’s that?) of Earth, it is still much smaller that Jupiter or Saturn. Uranus is twice as far from the sun as Saturn, so it is much colder. Uranus looks blue-green because of methane in its atmosphere. Uranus’ axis of rotation is tilted about 90˚ in the vertical, so from Earth it looks like it’s rotating on its side. Compared to Earth, it takes Uranus 30,799 days or 84 years to orbit the sun! Finally, Uranus has at least 27 moons that we’ve been able to detect to date – and, like Saturn, we’re always looking for more! Neptune Neptune is even farther from the sun than Uranus. Neptune is a cold, blue planet. Scientists think that Neptune is slowly shrinking, causing the interior to heat up. Astronomers have discovered at least thirteen moons orbiting Neptune, the largest of which is Triton. Neptune’s orbit around the sun takes approximately 60,327 days. How many years is that? (~165 years) Images used in this lesson: Jupiter Source: http://en.wikipedia.org/wiki/File:Jupiter.jpg License: Public Domain Jupiter to Earth Comparison Source: http://en.wikipedia.org/wiki/File:Jupiter-EarthSpot_comparison.jpg License: Public Domain Jupiter’s Interior Source: http://en.wikipedia.org/wiki/File:Jupiter_interior.png License: Public Domain Giant Red Spot Source: http://en.wikipedia.org/wiki/File:Great_Red_Spot_From_Voyager_ 1.jpg License: Public Domain Jupiter Seen Cassini Source: http://en.wikipedia.org/wiki/File:PIA04866_modest.jpg License: Public Domain Saturn as Seen by Cassini Source: http://en.wikipedia.org/wiki/File:Saturn_from_Cassi ni_Orbiter_(2004-10-06).jpg License: Public Domain Saturn to Earth Comparison Source: http://en.wikipedia.org/wiki/File:Saturn,_Earth_size_compariso n.jpg License: Public Domain Titan Source: http://en.wikipedia.org/wiki/File:Titan_in_natural_color_Cassin i.jpg License: Public Domain Saturn with Moons Titan and Tethys Source: http://www.titanexploration.com/Titan%20Images/titanimages 2008.htm License: Public Domain Uranus Source: http://en.wikipedia.org/wiki/File:Uranus2.jpg License: Public Domain Uranus Rings Source: http://en.wikipedia.org/wiki/File:Uranusandrings.jpg License: Public Domain Uranus with Clouds and Rings Source: http://en.wikipedia.org/wiki/File:Uranus_clouds.jpg License: Public Domain Uranus to Earth Comparison Source: http://en.wikipedia.org/wiki/File:Uranus,_Earth_size_comparis on.jpg License: Public Domain Uranus Moons (A montage of Uranus' large moons and one smaller moon: from left to right Puck, Miranda, Ariel, Umbriel, Titania and Oberon. Other moons are not yet photographed in detail. Size proportions are correct.) Source: http://commons.wikimedia.org/wiki/File:Uranus_moons.jpg License: Public Domain Neptune Source: http://en.wikipedia.org/wiki/File:Neptune.jpg License: Public Domain Neptune to Earth size comparison Source: http://en.wikipedia.org/wiki/File:Neptune,_Earth_size_comparis on.jpg License: Public Domain The Rings of Neptune Source: http://en.wikipedia.org/wiki/File:Neptune_ring_arcs.jpg License: Public Domain Neptune and Triton Source: http://en.wikipedia.org/wiki/File:Voyager_2_Neptune_and_Trito n.jpg License: Public Domain