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Astronomy 101 The Solar System Tuesday, Thursday 2:30-3:45 pm Hasbrouck 20 Tom Burbine [email protected] Course • Course Website: – http://blogs.umass.edu/astron101-tburbine/ • Textbook: – Pathways to Astronomy (2nd Edition) by Stephen Schneider and Thomas Arny. • You also will need a calculator. Office Hours • Mine • Tuesday, Thursday - 1:15-2:15pm • Lederle Graduate Research Tower C 632 • Neil • Tuesday, Thursday - 11 am-noon • Lederle Graduate Research Tower B 619-O Homework • We will use Spark • https://spark.oit.umass.edu/webct/logonDisplay.d owebct • Homework will be due approximately twice a week Astronomy Information • Astronomy Help Desk • Mon-Thurs 7-9pm • Hasbrouck 205 • The Observatory should be open on clear Thursdays • Students should check the observatory website at: http://www.astro.umass.edu/~orchardhill for updated information • There's a map to the observatory on the website. Final • Monday - 12/14 • 4:00 pm • Hasbrouck 20 HW #15 • Due next Tuesday Exam #3 • This Thursday • Covers material from October 15th – November 5th • Bring pencil and a calculator • Review Session – Wed. at 6 pm in Hasbrouck 134 • Formulas (I also would not forget the formulas that I learned earlier) Density = mass/volume Volume = 4/3r3 HW Review Mercury/Venus • Mercury is the closest planet to the Sun • Venus is next closest Mercury • • • • orbit: 0.38 AU from Sun diameter: 4,880 km (38.3% of Earth) mass: 3.30 x 1023 kg (5.5% of Earth) temperature: 90 K (minimum) 440 K (average) 700 K (maximum) • Satellites: Zero Difficult to study Mercury • Because of Mercury's proximity to the Sun – makes reaching it with spacecraft technically challenging – Earth-based observations difficult. Mercury • Videos • http://www.gecdsb.on.ca/d&g/astro/html/Mercury .html Mariner 10 • The only spacecraft to approach Mercury was NASA's Mariner 10 (1974-1975). Caloris Basin Caloris Basin (Some of the hill are 1,800 meters tall) Messenger data Mariner 10 data Caloris Basin • A basin was defined by Hartmann and Kuiper (1962) as a "large circular depression with distinctive concentric rings and radial lineaments." • Others consider any crater larger than 200 kilometers a basin. • The Caloris basin is 1,550 kilometers in diameter, and was probably caused by a projectile larger than 100 kilometers in size. • The impact produced concentric mountain rings three kilometers high and sent ejecta 600 to 800 kilometers across the planet. Weird Terrain The weird terrain is almost opposite Caloris Basin. It consists of hills, ridges and grooves that cut across craters. The weird terrain my have been formed by shock waves that raced through the center of the planet and outward early in Mercury's history. Mercury has high density • Its density is 5.44 g/cm3 which is comparable to Earth's 5.52g/cm3 density. • In an uncompressed state, Mercury's density is 5.5 g/cm3 where Earth's is only 4.0 g/cm3. http://www.psrd.hawaii.edu/WebImg/MercuryCore.gif Messenger • Mission to Mercury • Launched August 3, 2004 • Flew by Mercury in 2008 and 2009 • Will orbit Mercury in 2011 Messenger video • A set of five 11-band images was captured by MESSENGER just after the spacecraft crossed the night/day line (the “terminator”), which are the highest-resolution color images ever obtained of Mercury’s surface. • At the beginning of this movie, it is dawn in that region of Mercury, and the Sun is just off the horizon. The long shadows that are cast by crater walls exaggerate the ruggedness of the terrain and highlight variations in topography. • Though Mercury’s true colors are subtle, the 11 color bands of MDIS were combined in a statistical method used to highlight differences in color units. Older, low-reflectance, and relatively blue material is encroached by younger, relatively red smooth plains. Several lobate scarps or cliffs are observed, which are places where compressional stresses caused Mercury’s crust to fracture and shorten. http://messenger.jhuapl.edu/news_room/presscon5_images/Robinson%20Image%205.7.mov Mercury Much of the image to the right of the Kuiper crater (in the centre here) had never been imaged by a spacecraft before. Researchers were surprised to see long crater rays that extend thousands of kilometers from a crater at the planet's north pole http://space.newscientist.com/data/images/ns/cms/dn14893/dn14893-1_450.jpg Mercury Dark material, shown in deep blue in the enhanced colour image at right (a composite of visible and near-infrared images), was kicked up by impacts. The material seems to be widespread but patchy, suggesting the planet's interior is not homogenous. http://space.newscientist.com/data/images/ns/cms/dn15077/dn15077-1_600.jpg Mercury • Double ringed basin • 290 km in diameter • Appears young (few craters on it) • ~ 1 billion years old • Lava may have covered up the central part of the basin http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/presscon6_img4_5_lg.jpg • 160 km in diameter http://en.wikipedia.org/wiki/File:Mercury_Double-Ring_Impact_Basin.png Spectra of Mercury Weak to absent absorption features – no iron in the silicates Mercury’s Surface • Made of Enstatite (MgSiO3) – Mg-rich pyroxene • Made of material like the Lunar Highlands – Plagioclase feldspar - CaAl2Si2O8 Venus • orbit: 0.72 AU from Sun • diameter: 12,103.6 km (94.9% of Earth) (called Earth‘s twin) • mass: 4.869 x 1024 kg (81.5% of Earth) • Temperature on surface: 726 K(average) • Satellites: Zero Venus’ atmosphere • Atmospheric pressure at surface is 92 times the pressure on the Earth’s surface • • • • • • Atmospheric content: Carbon dioxide 96.5 % Nitrogen 3.5 % Sulfur dioxide 150 ppm Argon 70 ppm Water vapor 20 ppm Venus’ clouds • Venusian clouds are thick and are composed of sulfur dioxide and droplets of sulfuric acid. • These clouds reflect about 75% of the sunlight that falls on them, Greenhouse Effect • The greenhouse effect is the rise in temperature that a planet experiences because certain gases in the atmosphere (H2O, CO2, CH4) trap energy emitted from the surface. • Visble light hits the surface • Surface warms and emits infrared radiation • Atmospheric gases absorb some of the infrared light • Surface and Atmosphere heat up Stefan-Boltzman Law Emitted power (per square meter of surface) = σT4 λ·Tmax = 2,900,00 nm Runaway Greenhouse Effect • Runaway greenhouse effect to describe the effect as it occurs on Venus • Venus is sufficiently strongly heated by the Sun that water is vaporized and so carbon dioxide is not reabsorbed by the planetary crust Why does Venus has such a thick atmosphere? • The luminosity of the Sun has increased by 25% from 3.8 billion years ago • The atmosphere of Venus up to around 4 billion years ago maybe was more like that of Earth with liquid water on the surface. • The runaway greenhouse effect may have been caused by the evaporation of the surface water and the rise of the levels of greenhouse gases that followed. Surface • Mapped by Magellan spacecraft (1990-1994) • How was it mapped if it has a dense atmosphere? How did it do it? • Used Radar (radio waves) • Most of Venus' surface consists of gently rolling plains with little relief. • Data from Magellan's imaging radar shows that much of the surface of Venus is covered by lava flows. • Lava flows stopped ~300-500 million years ago • Very few craters Craters • Venusian craters range from 3 km to 280 km in diameter. • There are no craters smaller than 3 km because the dense atmosphere stops small incoming objects. • 200 km long channel • 2 km wide http://hyperphysics.phy-astr.gsu.edu/hbase/Solar/venusurf.html Pancakes Domes • Flattened lava domes are attributed to upwellings of molten rock which then subsided. • The solid crust left behind then flattened and cracked. Coronae • Corona is an oval-shaped feature. • hot rising bodies of magma reach the crust and cause it to partially melt and collapse • Generates volcanic flows and fault patterns that radiate from the central structure. 100 km in diameter http://pds.jpl.nasa.gov/planets/captions/venus/vencor.htm Arachnoids • concentric ovals surrounded by a complex network of fractures, and can span 200 kilometers • Almost all Venusian surface features are named after historical and mythological women. • The only exceptions are Maxwell Montes, named after James Clerk Maxwell, and two highland regions, Alpha Regio and Beta Regio Venera • Venera probes were launched by the Soviet Union and enter Venus’ atmosphere • 1961-1984 • Venera 3-16 • 10 probes landed on surface Venera 9 Venera 9 pictures Venus Express • Launched November 9, 2005 (Soyuz-Fregat from Baikonur, Kazakhstan) • First global monitoring of composition of lower atmosphere in near-infrared transparency ‘windows’ • First coherent study of atmospheric temperature and dynamics at different levels of atmosphere, from surface up to ~200 km • First measurements from orbit of global surface temperature distribution Mostly spare parts from Mars Express or Rosetta • ASPERA-4 - Neutral and ionised plasma analysis - Mars Express • MAG - Magnetic field measurements - Rosetta Lander • PFS - Atmospheric vertical sounding by infrared Fourier spectroscopy - Mars Express • SPICAV - Atmospheric spectrometry by star or Sun occultation - Mars Express • VeRa - Radio sounding of atmosphereFrance)VeRaRadio sounding of atmosphere - Rosetta • VIRTIS - Spectrographic mapping of atmosphere and surface - Rosetta • VMC - Ultraviolet and visible imaging Mars Express and Rosetta Any Questions?