The Earth as a PlanetHow to find the basic parameters?Why is the Earth still hot?Structure of the Earth’s InteriorMotions of the Earth’s crustThe Earth’s AtmosphereThe Greenhouse EffectCarbon Dioxide is a critical factorCarbon Dioxide is Increasing due to HumansThe Ozone Hole is Different (and less critical)The Origin and History of the MoonCraters on the MoonGetting Ages from Half-livesThe Origin of the Moon – A Stupendous ImpactTidesWhy Tides HappenPhases of the MoonWhere to find the Moon in the SkyPhase MovieLunar EclipsesSolar EclipsesShadowDanceAstro QuizThe Earth as a PlanetBasic Properties(size, density, composition)Interior structureInterior dynamicsAtmosphereFormation and EvolutionHow to find the basic parameters?We find that the bulk density of the Earth is much higher than that of surface rocks. It must have something denser inside.Why is the Earth still hot?The heat was generated by the violent accumulation of planetesimals which created the Earth. Further heat is added by decay of radioactive elements. The main source is the crystallization of our iron core from liquid to solid. The heat has trouble getting out because of the large volume to surface area ratio. Smaller planets cool faster. Heat is carried out from the interior by “convection”. Hot rock rises up to the surface where it radiates its energy and cools, sinking back down. This causes the dynamics on our crust.Structure of the Earth’s InteriorWe can use seismic waves generated by earthquakes to “see” inside the Earth. We find that it has a “liquid” iron/nickel core, surrounded by a “plastic” mantle. The crust of solid rock is thinner than an eggshell in relative terms. Thus, the Earth is still basically a molten ball.The denser stuff is in the middle because it sunk there – “differentiation”.Motions of the Earth’s crustThe Earth’s AtmosphereOur atmosphere is about 80% molecular nitrogen and 20% molecular oxygen, with water and carbon dioxide in small amounts. The temperature changes direction several times as you go up.The Greenhouse Effect1) In equilibrium, a planet must re-radiate all the energy it absorbs.2) Solar energy tends to be converted from visible to infrared radiation.3) Some gases are transparent to visible radiation, but opaque to infrared radiation.4) When radiation is blocked, you need a bigger temperature gradient to push the energy through.Carbon Dioxide is a critical factorWithout subduction and water, the atmosphere and climate on the Earth would have been very different. A little more conversion of CO2 to rock, or lack of subduction and vulcanism, and we would have “snowball Earth”. Less conversion could make us more like Venus (human greenhouse gases not really enough for that). Lifehas played an important role by using CO2 in plant respiration and production of shells which sink to the ocean bottom.Carbon Dioxide is Increasing due to HumansThe Ozone Hole is Different (and less critical)Slide 21 Fig. 6-11b, p.105Ozone blocks solar UV, which causes tans and skin cancer. The hole is due to CFCs (a chemical) which is now being controlled. The atmosphere should recover in about 50 years (we hope).The Origin and History of the MoonThe surface of the Moon has craters, highlands, and “maria” (dark lava basins). Its composition is similar to that of the Earth’s mantle, with little or no iron core.Craters on the MoonThe craters on the Moon are almost all impact craters. They tell of an early violent history, one which is also recorded around the rest of the Solar System. The first half-billion years were filled with flying debris (some of it planet-sized).Getting Ages from Half-livesStart1 half-life2 half-lives3 half-livesIf you know the starting composition of a material, and you know the time it takes for half of it to change into a decay product, you can figure out how old it is by measuring the ratio of original material to decay product.The Origin of the Moon – A Stupendous ImpactTidesThere are 2 high and 2 low tides every day.Why Tides HappenTides are caused by the difference in the pull of gravity from one body on the near and far side of another (1/r3). They are important in all kinds of astronomical contexts. They cause the Earth to slow down and the Moon to recede.Phases of the MoonWhere to find the Moon in the SkyThe angle between the Sun and the Moon determines its phase.A crescent Moon must be near the SunA half Moon (first or last quarter) must be overhead when the Sun is rising or settingThe full Moon must rise when the Sun sets, and be on the meridian near midnightThe waning Moon will tend to be seen in the daytimePhase MovieLunar EclipsesA lunar eclipse occurs when the Moon goes into the Earth’s shadow. Everyone who can see the Moon then sees the eclipse. It looks red because sunlight is refracted through our air.The Moon must be full.Solar EclipsesSolar eclipses happen when the Moon passes between us and the Sun. The eclipse can only be seen where the alignment is perfect. The sky goes dark, the stars come out, and the solar corona becomes visible. It only lasts a few minutes in any given spot. Although there are 1 or 2 per year, any given place has a long wait to see one.The Moon must be new.ShadowDanceEclipses usually don’t happen, because the Moon’s orbit is tilted.The Moon just happens to have about the same angular size as the Sun.This is a coincidence of the present, the distant past and future will not get perfect solar eclipses because the Moon’s distance is growing.Astro QuizUnder which condition below would there be a total solar eclipse every month?1) The moon’s orbit crosses the ecliptic at 12 points.2) The moon’s orbit appears to move along the ecliptic.3) The moon’s orbit is perpendicular to the celestial
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