AST101: The Sun and its Neighbours Class 2: A Pictorial View of our Solar System Professor Jeremy Webb A Pictorial Tour of our Solar System AST 101 | UofT | Prof. Webb | 15 Learning Goals • How can we describe the shape and motion of objects in the solar system? • How are the patterns of motion in the solar system related to how it is formed? • What is the difference between a terrestrial and a Jovian planet? • What are some facts about our solar system planets? AST 101 | UofT | Prof. Webb | 16 A solar system consists of a star orbited by planets, moons, and lots of debris (comets, asteroids, dust)* * “Solar System” or “The Solar System” means our solar system; “solar system” or “star system” can be any such system. AST 101 | UofT | Prof. Webb | 17 Our Solar System is HUGE and the vast majority of it is empty.* *It’s not quite empty—tiny, tiny quantities of gas and dust fill the space AST 101 | UofT | Prof. Webb | 18 AST 101 | UofT | Prof. Webb | 19 Our Solar System (image credit: NASA) AST 101 | UofT | Prof. Webb | 20 AST 101 | UofT | Prof. Webb | 21 The Inner Solar System: Mercury, Venus, Earth, and Mars AST 101 | UofT | Prof. Webb | 22 The Outer Solar System: Jupiter, Saturn, Uranus, Neptune, many dwarf planets & comets AST 101 | UofT | Prof. Webb | 23 What do you think? • In addition to their orbit, inner and outer planets also differ by their: – A) Composition – B) Size – C) Atmospheres – D) All of the above – E) What is an atmosphere? AST 101 | UofT | Prof. Webb | 24 Terrestrial = Earth-like AST 101 | UofT | Prof. Webb | 27 Terrestrial planets – small, rocky, thin or no atmosphere, few moons, made of heavy elements AST 101 | UofT | Prof. Webb | 28 Mercury Earth NASA / © Calvin J. Hamilton Venus Mars AST 101 | UofT | Prof. Webb | 29 Jovian = Jupiter-like AST 101 | UofT | Prof. Webb | 30 Jovian planets – large, liquid + gas, small rocky core, many moons, made of light elements AST 101 | UofT | Prof. Webb | 31 “gas giants” AST 101 | UofT | Prof. Webb | 32 Saturn Uranus NASA / © Damien Peach Jupiter Neptune AST 101 | UofT | Prof. Webb | 33 AST 101 | UofT | Prof. Webb | 34 What do you think? • How many planet Earth’s could fit inside Jupiter? – A) 10 – B) 100 – C) 1000 – D) 10,000 AST 101 | UofT | Prof. Webb | 35 AST 101 | UofT | Prof. Webb | 36 Inner Planets AST 101 | UofT | Prof. Webb | 39 Mercury • No atmosphere, highly cratered surface • Rocky exterior with a huge iron core • Temperature fluctuates between -170 C and 425 C (lead melts at 327 C) • No moons • Only two probes have ever been sent to Mercury: – Mariner 10 (1974-1975) – MESSENGER (2011-2015) AST 101 | UofT | Prof. Webb | 40 NASA Images of Mercury from MESSENGER (both images are in false colour). AST 101 | UofT | Prof. Webb | 41 Credit: MESSENGER AST 101 | UofT | Prof. Webb | 42 Credit: MESSENGER AST 101 | UofT | Prof. Webb | 43 Venus • Thick CO2 atmosphere, lots of possibly active volcanoes • About the same size as Earth • Runaway greenhouse effect makes it even hotter than Mercury: 460 C everywhere all the time (lead melts at 327 C) • Rains acid • No moons • Rotates very slowly and backwards! AST 101 | UofT | Prof. Webb | 46 AST 101 | UofT | Prof. Webb | 47 Magellan (1991) radar map sees through the clouds NASA AST 101 | UofT | Prof. Webb | 48 Earth • Wet planet covered in creepy-crawlies • Unusually big moon • Only planet we have to live on. Probably shouldn’t wreck the place, huh? + way too much CO2 à AST 101 | UofT | Prof. Webb | 49 Mars • Very thin CO2 atmosphere • Many huge, extinct volcanoes • Was probably Earth-like in the distant past (i.e. wet & warmish) • Many surface features appear to have been carved by water • Lots of sub-surface water • No life known to date AST 101 | UofT | Prof. Webb | 50 Credit: NASA/JPL AST 101 | UofT | Prof. Webb | 51 Olympus Mons Credits: NASA; © 2004 Wolfgang Weiser ; Wikipedia user Resident Mario ; ESA / DLR / FU Berlin (G. Neukum) AST 101 | UofT | Prof. Webb | 52 Valles Marineris Credit: NASA / R. Kline; ESA / DLR / FU Berlin (G. Neukum) AST 101 | UofT | Prof. Webb | 53 NASA: Spirit and Opportunity (2004- ) • Spirit stopped working in 2011 • Opportunity was still going (43 km and counting …) until we lost contact with it in 2018 L Credit: NASA/JPL-Caltech/Cornell/MAAS Digital LLC AST 101 | UofT | Prof. Webb | 54 Lots of Evidence That Mars Was Once Wet Credit: © 2014 Pearson Education, Inc. AST 101 | UofT | Prof. Webb | 55 NASA: Perseverance Rover • Looking for signs of ancient life • Collecting rock and soil samples – Potentially for return flight home! • Brought a helicopter with it! AST 101 | UofT | Prof. Webb | 56 NASA: Ingenuity Helicopter AST 101 | UofT | Prof. Webb | 57 Asteroid Belt • In between orbits of Mars and Jupiter • Many thousands or millions of “rubble piles” • Material left over from the formation of the solar system, prevented from turning into a planet by tides from Jupiter AST 101 | UofT | Prof. Webb | 62 False colour image of asteroid Gaspra captured by the Galileo spacecraft (NASA). AST 101 | UofT | Prof. Webb | 63 Asteroid 433 Eros, as seen by the NEAR spacecraft in 2000 AST 101 | UofT | Prof. Webb | 64 NEAR actually landed on Eros AST 101 | UofT | Prof. Webb | 65 Outer Planets AST 101 | UofT | Prof. Webb | 66 Jupiter • Largest planet in the solar system • Thick gaseous atmosphere surrounds a giant ball of liquid hydrogen • > Earth-sized rock somewhere deep inside? • Has very faint rings • Many moons: more than 60 known to date AST 101 | UofT | Prof. Webb | 67 True colour image of Jupiter from the Cassini spacecraft (NASA) AST 101 | UofT | Prof. Webb | 68 Juno was launched by NASA in 2011, and arrived at Jupiter on July 5, 2016 Image credit: NASA/JPL AST 101 | UofT | Prof. Webb | 69 AST 101 | UofT | Prof. Webb | 70 Io is the most volcanically active body in the solar system, thanks to tides from Jupiter. AST 101 | UofT | Prof. Webb | 71 Eruption of the Tvashtar volcano on Io as seen by the New Horizons spacecraft on its way to Pluto. AST 101 | UofT | Prof. Webb | 72 Saturn • A real gas giant – it’s mostly gas • Spectacular rings • Also more than 60 known moons • Cassini spacecraft is there now, taking gorgeous pictures AST 101 | UofT | Prof. Webb | 73 Image Credit: NASA/JPL-Caltech/Space Science Institute AST 101 | UofT | Prof. Webb | 74 Image Credit: NASA/JPL-Caltech/Space Science Institute AST 101 | UofT | Prof. Webb | 75 The rings of Saturn are made of tiny particles of mainly ice (artist’s conception) AST 101 | UofT | Prof. Webb | 76 Uranus and Neptune • Like gas giants, but these two are principally a slushy ice mixture à “ice giants” ? • Both about the same size • Both bluey/green • Both have many moons • Both have faint rings AST 101 | UofT | Prof. Webb | 79 Uranus, as seen by Voyager 2 AST 101 | UofT | Prof. Webb | 80 direction to Sun Uranus is tipped over! AST 101 | UofT | Prof. Webb | 81 Neptune, as seen by Voyager 2 AST 101 | UofT | Prof. Webb | 82 Beyond Neptune AST 101 | UofT | Prof. Webb | 83 Trans-Neptunian Objects • Beyond Neptune, there are many dwarf planets • These are small, icy bodies • Pluto is the largest one known • They take a long time to orbit the Sun • New Horizons has recently given us our first-ever close up view of a trans-Neptunian object AST 101 | UofT | Prof. Webb | 84 The best picture we had of Pluto until 2017, using lots of computer enhancement. AST 101 | UofT | Prof. Webb | 85 New Horizons was launched on 19 January 2006, swung by Jupiter and took 6 months of ‘flyby’ footage of Pluto and its moons in 2015. Credit: NASA AST 101 | UofT | Prof. Webb | 86 Credit: NASA AST 101 | UofT | Prof. Webb | 87 AST 101 | UofT | Prof. Webb | 88 The Kuiper Belt is a ring of comets orbiting just beyond Neptune. This is debris left over from the formation of the solar system. AST 101 | UofT | Prof. Webb | 89 The Oort cloud is a spherical cloud of perhaps a trillion comets surrounding the solar system. AST 101 | UofT | Prof. Webb | 90 Rosetta, the mission to comet https://petapixel.com/2019/09/09/this-video-was-made-from400000-actual-photos-of-a-comet-in-space/ AST 101 | UofT | Prof. Webb | 91 ‘Oumuamua is an interstellar asteroid that flew through the solar system at an accelerated rate AST 101 | UofT | Prof. Webb | 94 AST 101 | UofT | Prof. Webb | 95 Learning Goals • How can we describe the shape and motion of objects in the solar system? – Except comets, most things have near circular orbits and are often rotating • How are the patterns of motion in the solar system related to how it is formed? – Most things orbit and rotate in the same direction • What is the difference between a terrestrial and a Jovian planet? – Distance from Sun, chemical composition, size, mass,….. AST 101 | UofT | Prof. Webb | 96