By Andrew Newbound © Andrew Newbound 2013 Unit 1 © Andrew Newbound 2013 Galaxies ◦ Group of stars and planets Tectonics ◦ Plate movements Radioactive ◦ An element which gives off radiation Subduction ◦ A location where a layer sinks into hot magma Geological ◦ The study of rocks © Andrew Newbound 2013 Era ◦ A group of periods Strata ◦ Layers of rock Seismic ◦ The force given off by earthquakes Precambrian ◦ A period in geological time Period ◦ A length of time © Andrew Newbound 2013 Half-life ◦ The time taken for an element to have half of its radioactivity Volcano ◦ A location where magma comes out of a mountain like structure Stratigraphy ◦ The study of determining the age of rocks Trilobite ◦ An exoskeleton-ed creature from the Cambrian period © Andrew Newbound 2013 Fossil ◦ The remains of an ancient creature Convection ◦ Heat cycle in a liquid or gas © Andrew Newbound 2013 Determine age of earth Material accumulates in layers Cross section – stratigraphical column Law of Superposition ◦ Oldest = bottom ◦ Youngest = top ◦ Except when disturbed © Andrew Newbound 2013 Each layer identified by looks, texture etc. Rocks of certain type = same (no matter what) Sedimentary rocks – form by deposition Different strategraphic columns correlated ◦ Information on how environment changed ◦ Relate types of rock to type of environment present © Andrew Newbound 2013 Coal Mudstones Mudstones with sandstones Sandstones Swamp Lagoon Tidal Shallow marine © Andrew Newbound 2013 Artefacts may be found in rock strata Fossils in 1 layer = 1 age Many fossils distinct to time period © Andrew Newbound 2013 1. 2. 3. 4. Animal dies Body eaten by decomposers Hard parts left behind Become fossil if not decomposed © Andrew Newbound 2013 Found in sedimentary rock Layers of sediments Found when rocks break away Changed into rock (sediments) Heat & pressure over period of time ◦ Lithification Minerals seep in – change composition Fossils dissolved – minerals fill gaps Fossils – similar to sediments ◦ ◦ Petrified = turned to stone Silica, apatite, calcite common © Andrew Newbound 2013 Animal droppings, wood ◦ Don’t smell Soft parts fossilised ◦ Sometimes only outlines Valuable ◦ Zircon – don’t decompose ◦ Copies – plaster © Andrew Newbound 2013 1. 2. 3. 4. 5. 6. 7. Animal dies in swamp Remains buried Layers build up Chemicals seep in Surrounding sediments = sedimentary rocks Layers pushed upwards Weathering exposes fossils © Andrew Newbound 2013 Meteors/Asteroids ◦ Rare metal found in asteroids ◦ Melted rock from asteroid ◦ Fractured crystals = high energy Volcanoes ◦ Rare metal = large scale volcanic activity ◦ Fractured crystals = high energy ◦ Fossil record = gradual decline © Andrew Newbound 2013 Competing with mammals ◦ Fossil record – lots of mammal fossils after dinosaur extinction Cooling climate ◦ Fossil record – gradual decline ◦ Sea level – dryer continents © Andrew Newbound 2013 Volcano ◦ ◦ ◦ ◦ ◦ Lava dating to period 500,000 + years leading up to extinction Stopped sunlight Temp fell Plants stopped producing ◦ ◦ ◦ ◦ Impact crater near Yucatan peninsula 10km wide asteroid 30km per second Melted granite (common at time of dinosaur extinction) Asteroid © Andrew Newbound 2013 Both ◦ ◦ ◦ ◦ ◦ ◦ Left rare metals Powerful force Sudden catastrophe End of Cretaceous/Tertiary period Fossil records Fractured crystals © Andrew Newbound 2013 Time divided into periods ◦ Special fossils associated with ◦ Dated exactly (in millions of years) Radioactive dating ◦ Used to explain age of fossil End of period ◦ Large number of extinctions Geological time scale ◦ Shows names, order of periods, absolute age © Andrew Newbound 2013 Alfred Wegener (1915) ◦ Theory on continental drift ◦ Coined term Continental Drift (now Plate Tectonics) Continents once joined ◦ ◦ ◦ ◦ ◦ ◦ Shape of continents Eroded mountain ranges Deposits of minerals Patterns by glaciers Similar fossils & closely related living species Ancient coral reefs in cold climates © Andrew Newbound 2013 © Andrew Newbound 2013 Continents once joined together Pangaea ◦ Original land mass ◦ Everything joined together 200 million years ago ◦ 2 super continents ◦ Laurasia & Gondwana © Andrew Newbound 2013 Laurasia ◦ Northern Hemisphere North America Greenland Europe Asia Gondwanaland ◦ Southern Hemisphere South America Africa India Antarctica Australia © Andrew Newbound 2013 Lithosphere – upper layer Asthenosphere – lower layer Earth’s crust not a single piece About 30 plates ◦ Move a few centimetres per year More evidence of continental drift © Andrew Newbound 2013 Earth’s crust & upper mantle broken into moving plates of mantle Lithosphere plates = solid rock Several very large plates (both continental, oceanic portions) 12 + smaller plates Average = 80km in thickness All plates = moving Slide on asthenosphere ◦ A little magma © Andrew Newbound 2013 Plates move – convection, gravity Subduction zones – 1 plate sinks into mantle ◦ Rest of plate is dragged in ◦ Like pushing paper off table Convection currents – in Lithosphere ◦ Heat deeper – mantle made to circulate Contains a little magma Behaves like hot mush © Andrew Newbound 2013 Marked by earthquakes, volcanoes, mountain ranges ◦ Caused by qualities of plate boundaries Volcanoes ◦ Magma coming between plates Mountain ranges ◦ Created by plates converging © Andrew Newbound 2013 © Andrew Newbound 2013 Oceanic plate = thin Continental plate = thick Plates moving 2-10cm per year Diverging ◦ Lava fills gap ◦ Mid-Ocean Ridge Only ridge above sea level = Iceland 1975-1981 = widened by 5m © Andrew Newbound 2013 © Andrew Newbound 2013 Transform ◦ Get stuck = earthquake ◦ E.g. San Andreas fault in California Converging ◦ Oceanic meets continental = oceanic subducted Molten rock rises as volcano Subduction zone ◦ OR Continent meets continent = fold mountains produced E.g. Indian/Asian Marine sediments squashed, crinkled, sediments pushed upwards Still moving = earthquakes © Andrew Newbound 2013 © Andrew Newbound 2013 Form at subduction zones ◦ E.g. ring of fire Found in middle of plate – hot spot ◦ Heated spot in mantle © Andrew Newbound 2013 Unit 2 © Andrew Newbound 2013 Element ◦ Chlorine Mixture ◦ Citric acid Compound ◦ ◦ ◦ ◦ Sodium chloride Ammonia Natural gas Mentholated spirits © Andrew Newbound 2013 Reactants recombine to form product Reactants Products Law of conservation ◦ means reacts ◦ Mass of reactants = mass of products ◦ No matter created/destroyed Atoms rearranged ◦ Our matter around at time of dinosaurs Chemical reaction ◦ ◦ ◦ ◦ ◦ Change of colour Change of temperature Gas given off Odour Solid produced © Andrew Newbound 2013 Salt – combination of a metal & non-metal E.g. NaCl (table salt) = metal (sodium) + non-metal (chlorine) Acid + metal Salt + Hydrogen Acid + carbonate salt + Carbon Dioxide + water Acid + base salt + water © Andrew Newbound 2013 Ion ◦ Charged molecule Tell if acid/base = use indicator Acid ◦ Compound contains hydrogen compounds which detach when dissolved to form H+ ions ◦ Taste sour, are corrosive Name Formula Ion when dissolved Hydrochloric HCl H+ + Cl- Sulphuric H2SO4 2H+ + SO42- Nitric HNO3 H+ + NO3- © Andrew Newbound 2013 Base ◦ Compound contains OH- ion which detaches when dissolved ◦ Alkali ◦ Strip fats out of skin – caustic ◦ Used for soup ◦ Bitter Name Formula Ion when dissolved Sodium hydroxide NaOH Na+ + OH- Potassium hydroxide KOH K+ + OH- Calcium hydroxide Ca(OH)2 Ca2+ + 2OH- © Andrew Newbound 2013 Acid + base neutralise to form water + salt © Andrew Newbound 2013 Power/concentration of hydrogen O-14 Neutral = 7 Measuring with pH meter Use universal indicator ◦ Mixture of indicators Small change in pH = large change in concentration ◦ Body sensitive to changes pH of medical = body pH © Andrew Newbound 2013 Compound of metal & non-metal In neutralisation reaction ◦ metal from base ◦ non-metal from acid © Andrew Newbound 2013 Bases Acids Base name Formula Type of salt Formula Sodium hydroxide NaOH Sodium Na Potassium hydroxide KOH Potassium K Magnesium hydroxide Mg(OH)2 Magnesium Mg Calcium hydroxide Ca(OH)2 Calcium Ca Ammonium hydroxide H4OH Ammonium NH4 Acid name Formula Type of salt Formula Hydrochloric acid HCl Chloride Cl Sulfuric acid H2SO4 Sulfate SO4 Nitric acid HNO3 Nitrate NO3 Phosphoric acid H3PO4 Phosphate PO4 © Andrew Newbound 2013 Acids and bases used in topic dissolved in water Water + substance dissolved in it = solution Water = solvent Dissolved substance = solute Solution – no more solute can be dissolved ◦ Saturated ◦ Heat & super saturate © Andrew Newbound 2013 Common solvent ◦ ◦ ◦ ◦ Water Acetone Methylated spirits Turpentine Nail polish ◦ Non soluble in water ◦ Soluble in acetone Solvents evaporate at different rates © Andrew Newbound 2013 In past ◦ Combustion = mystery ◦ Substance burnt = smaller in size ◦ All substances that combusted contained phlogiston Released during burning process ◦ Disproved – burning makes heavier Now – use oxygen theory Combustion needs: Products of combustion ◦ Combustible material ◦ Oxygen ◦ Ignition temp to be reached ◦ Water ◦ Carbon dioxide © Andrew Newbound 2013 Oxygen + Combustible material Water + Carbon dioxide Not enough oxygen = incomplete combustion ◦ Products = carbon and/or carbon monoxide ◦ E.g. Cars – black smoke Safety Bunsen flame © Andrew Newbound 2013 Reaction of metals, in which they dissolve away Only metals not corrode = gold, platinum Iron corrodes – rusting, turning reddish orange Copper turns aqua-green (turquoise) Stop corrosion ◦ Prevent water/oxygen reaching metal Oil, paint, plastic, air conditioning (e.g. museum) © Andrew Newbound 2013 Metal Water Oxygen Corrosion © Andrew Newbound 2013 Chemical process - compound is broken down E.g. CuCO3 CuO + Co2 2H2O 2H2 + O2 Requires energy ◦ Usually heat ◦ Sometimes electricity © Andrew Newbound 2013 Metal = 1st (from base) Non-metal = 2nd (from acid) Hydrochloric acid + sodium hydroxide Sodium chloride + water Hydrochloric acid + potassium hydroxide potassium chloride Sulfuric acid (H2SO4) Sulfate Nitric acid (HNO3) nitrate Hydrochloric acid (HCl) chloride © Andrew Newbound 2013 Carbonate ◦ Compound containing carbon & oxygen Neutralisation ◦ Acids and bases crossing each other out to produce a salt and water Reactant ◦ Starting compounds of a chemical reaction Equations ◦ A method of writing a chemical formula in a mathematical format © Andrew Newbound 2013 Combustion ◦ Where a combustible material reacts with oxygen to form carbon dioxide and water Decomposition ◦ The chemical process where a substance is broken down Corrosion ◦ Reaction of metals in which it reacts with water and oxygen to produce an oxide Metal ◦ A group of elements which share similar properties ◦ E.g. Shiny, conductive © Andrew Newbound 2013 Product ◦ The end compounds of a chemical reaction Acid ◦ pH <7, H+ ion disassociates with in water Bases ◦ pH >7, OH- ion disassociates with in water Indicator ◦ A substances that changes colour in acids and bases © Andrew Newbound 2013 Unit 3 © Andrew Newbound 2013 Biosphere ◦ All the plants and animals on earth Magnification ◦ Poisons accumulating up the food chain Carbon ◦ An element of the periodic table ◦ Essential for life Abiotic ◦ Non living parts of the environment © Andrew Newbound 2013 Insecticides ◦ Poison that kills insects Ecosystem ◦ Interactions of living things Nitrogen ◦ An element of the periodic table ◦ Essential for life Conservation ◦ Preserving the environment © Andrew Newbound 2013 Atmosphere ◦ All the gases in the environment Oxygen ◦ An element of the periodic table ◦ Essential for life ◦ A waste of photosynthesis Environment ◦ Everything surrounding a living thing © Andrew Newbound 2013 Pollution ◦ Waste products of another living organism in the environment Hydrosphere ◦ All of the water in the world Biotic ◦ All of the living things Renewable ◦ Able to be reused Greenhouse ◦ Layer of gases surrounding the earth to keep in gases, thus heating the earth © Andrew Newbound 2013 Environment ◦ All the things surrounding an organism which affect it in its life Habitat ◦ Where an organism lives © Andrew Newbound 2013 Study of Earth as life support system Study of living things in the environment © Andrew Newbound 2013 Animal behaviour Taxonomy Physiology Maths-population studies Abiotic (non-living) Climatology Hydrology Oceanography Physics Chemistry Geology Soil analysis Biotic (Living) © Andrew Newbound 2013 Competitors Disease Predators Food Mates Population sizes Shelter Nesting sites Biotic pH Oxygen levels Carbon dioxide levels Altitude Light availability Type of soil Water availability Shelter Topography Minerals Available space Abiotic © Andrew Newbound 2013 Teachers Students Trees Fish Illness Soil Grass Biotic (living) Desks Chairs Shelter Glass Paper Weather Bins Chemicals Carpet Abiotic (non-living) © Andrew Newbound 2013 Biosphere Atmosphere Hydrosphere Lithosphere © Andrew Newbound 2013 Gaseous envelope surrounding Earth to 500km Minor constituents are very important ◦ Greenhouse gases ◦ Ozone shield Composition changing overtime ◦ Still changing © Andrew Newbound 2013 Other Oxygen 1% Gases 21% Nitrogen 78% © Andrew Newbound 2013 Includes all liquid and solid water above & below ground Physical & chemical properties ◦ Important for life © Andrew Newbound 2013 Glacial Ice 2% Water Locations Other 1% Oceans 97% © Andrew Newbound 2013 Dynamic outer portion of the solid Earth Extends to about 100km Includes crust and uppermost part of mantle Source of earthquakes & volcanoes Comprised of tectonic plates © Andrew Newbound 2013 Organisms & their environments Includes living and dead organic matter © Andrew Newbound 2013 Constant movement of water from atmosphere ◦ From atmosphere to surface of the earth and back again Some water temporarily stored in ground ◦ Until drains Returns to atmosphere through ◦ Evaporation ◦ Plant transpiration ◦ Animal respiration © Andrew Newbound 2013 Ice Snow Oceans Seas Lakes Rivers Streams © Andrew Newbound 2013 Rain Hail Frost Snow Dew © Andrew Newbound 2013 © Andrew Newbound 2013 Oxygen (Photosynthesis) Animal Plant Carbon dioxide (Respiration) © Andrew Newbound 2013 sun Water + carbon dioxide glucose + oxygen 6H2O + 6CO2 C6H12O6 + 6O2 Takes place in leaves Needs water + carbon dioxide ◦ As well as sunlight and a plant Carbon dioxide ◦ Comes from animals Makes glucose + oxygen Glucose = plant’s food © Andrew Newbound 2013 Oxygen = waste gas ◦ Used by animals © Andrew Newbound 2013 © Andrew Newbound 2013 Way animals obtain energy ◦ Eat plants, other animals ◦ Get energy out of food through respiration Oxygen gas (O2)is needed Waste products ◦ Carbon dioxide (CO2) ◦ Water (H2O) Glucose + oxygen carbon dioxide + water C6H12O6 + 6O2 6CO2 + 6H2O © Andrew Newbound 2013 Plants to •Animals •Respiration (digestion) •Soil •Death, decay •Air/water Animals to •Air/water •Respiration •Fossil fuels •Burning •Soil •Death, decay •Burning © Andrew Newbound 2013 Fossil Fuels to •Air/water •Burning Air/water to •Plants Soil to •Fossil fuels •Photosynthesis •Heat/pressure •Air/water •Bacteria © Andrew Newbound 2013 Carbon in Plants Carbon in animals Carbon in the soil Carbon in fossil fuels Carbon dioxide in air/water © Andrew Newbound 2013 Key component in many molecules ◦ Form basic building blocks of life In ◦ Mainly in atmosphere (N2) 79% of air we breath Cannot directly use ◦ Living organisms ◦ Soil ◦ Oceans Responsible for DNA, RNA ◦ Molecules responsible for genetic code of life © Andrew Newbound 2013 Plants & animals need it to be converted to use ◦ Ammonia (NH4-) ◦ Nitrate (NO3-) ◦ Urea ((NH3)2CO) In urine Animals consume through ◦ Living/dead matter © Andrew Newbound 2013 Conversion of Nitrogen Gas into Ammonia/Nitrate Nitrogen made available to plants Nitrogen fixing bacteria ◦ Pluck non-reactive nitrogen gas from atmosphere ◦ Combine it with hydrogen to form ammonia ◦ Only use nitrogen they require to live Rest is for plants when bacteria die © Andrew Newbound 2013 Also fixed by ◦ ◦ ◦ ◦ ◦ Combustion Volcanic activity Lightning discharges Commercial fertilizer production Intense heat breaks 2 nitrogen atoms apart Nitrogens combines with oxygen to form nitrate © Andrew Newbound 2013 Conversion of ammonia into nitrate Soil bacteria ◦ Combine oxygen with ammonia ◦ Form nitrate (NO3-) Negatively charged nitrates can’t bind to clay particles Easily leached from the soil into the groundwater © Andrew Newbound 2013 Plant uptake and use Plants ◦ Draw ammonia + nitrate from soil ◦ Must convert nitrate into ammonia to use Done through assmilation © Andrew Newbound 2013 Conversion of Organic Nitrogen into Ammonia © Andrew Newbound 2013 Nitrogen contained in urine & faeces ◦ Much in form of urea Quickly reacts with other compounds in atmosphere Form ammonia Bacteria & fungi continue to break it down into ammonia 1. Organisms die 2. Decomposers break down Process significant amount of nitrogen from dead organism Converted to ammonia Plants use for growth, repair In high demand Quickly depleted in soil © Andrew Newbound 2013 Reduction of Nitrate into Nitrate Gas Environment doesn’t have enough oxygen OR too many nitrates ◦ Denitrifying bacteria reduce nitrates back into nitrate gas © Andrew Newbound 2013 Too much manure ◦ Stuffs up nitrogen throughout the ecosystem ◦ Can leach into groundwater ◦ Can runoff into lakes & steams Cause eutrophication Eutrophication ◦ Additional nutrients in lakes ◦ Huge amounts of algae grow ◦ Algae blooms on surface of affected lakes & streams Mats of thick green slime Block sunlight for plants in lakes © Andrew Newbound 2013 Algae consumed excess nitrogen compounds in water ◦ Die Bacteria break down dead algae ◦ Large quantities of dissolved oxygen Lake becomes hypoxic/oxygen-poor Oxygen-requiring organisms suffocate Aquatic insects & fish © Andrew Newbound 2013 Nitrogen in air Nitrate in plant decay Animal wastes Water nitrates Bacteria in soil produces nitrates © Andrew Newbound 2013 Interact with Earth’s spheres Litho Hydro Event Atmo © Andrew Newbound 2013 Bio Lava Ash into atmosphere Death to plants and animals Fertile soils Explosions Tsunami Landslide Forest fires New land Movement of earth heat © Andrew Newbound 2013 Hydrosphere •More debris into waterways •Pollutants Atmosphere •Gases/ash into atmosphere Biosphere •Death •Inhalation of gas/ash •More nutrients •Pollutant •Destroys crops © Andrew Newbound 2013 Lithosphere •Rearrangement of mantle •New material Hydrosphere Atmosphere • Displacement of water • Gas chamber opens Biosphere • Loss of life • Environmental disruption © Andrew Newbound 2013 Lithosphere • Movement of earth’s plates • New land formed Hydrosphere Atmosphere Biosphere • Pollutants in waterway • Pollutants in atmosphere • Disrupting respiration © Andrew Newbound 2013 Lithosphere • Displacement of soil Movement of plates Destroying cities ◦ Killing many © Andrew Newbound 2013 Movement of dust Not seeing © Andrew Newbound 2013 Animals/plants that have gone wild Feral cats ◦ Offspring of house cats ◦ Living wild in bush Unwanted plants = weeds ◦ Huge problems on Farms Forests Public land Foxes & dingoes poisoned ◦ No predators for kangaroos Population increases to plague proportions © Andrew Newbound 2013 Animals that have gone wild ◦ Often started as domestic animals Released/escaped Cause damage to environment Controls ◦ Biological ◦ Chemical – introducing other animals - poisons © Andrew Newbound 2013 Animal Impact on Environment Control methods Goat -Introduce weeds -Compete for resources -Footrot & other diseases -Soil damage -Culling -Young females sold as breeding stock -Shooting from helicopters Camels -Drink all water -Eat native plants -Shoot them -Harvesting/culling -Fencing -Live in them Fox -Kills animals -Economic loss -Rabies -Fences -Poison baits -Prevention of introduced weeds -Kill -Don’t introduce them to new places © Andrew Newbound 2013 Animal Impact on Environment Control Methods Cat -Kills native birds -Traps -Poison baits -Fencing Water Buffalo -Wreck soil -Shoot them -Eat all food -Shoot them again -Dung causes soil erosion Rabbits -Compete with native animals -Destroy vegetables -Destroying the places they live -tapping -Fencing -Shooting -Poisoning © Andrew Newbound 2013 Animal Impact on Environment Control Methods Pigs -Destroy vegetation -Compete with wildlife -Destroy breeding sites -Carries diseases -Shooting -Poison -Bait -Food Horses -Loss of native plants -Soil loss -Spread weeds -Compete for food -Economic loss -Shoot them (culling) -Baits -Traps © Andrew Newbound 2013 Pesticides are placed on produces ◦ Can lead to problems 1. Primary consumers eat problems 2. Secondary consumers eat them Concentration increases E.g. DDT Sprayed on plants ◦ Builds up down food chain ◦ Birds have very high concentration Causes shells to break No more baby birds Is a bad thing © Andrew Newbound 2013 Hawk Weasels Mouse Cricket Wheat © Andrew Newbound 2013 E.g. Mercury in Fish ◦ Little fish absorb mercury ◦ Bigger fish eat little fish ◦ We eat big fish Concentration of mercury is high E.g. In tuna © Andrew Newbound 2013 Australia has bad salinity problem Salt deep down brought closer to surface ◦ Farming and erosion Bad for plant growth Salt at surface cannot be returned Plants move water by capillary action © Andrew Newbound 2013 Farming Erosion © Andrew Newbound 2013 Unit 4 © Andrew Newbound 2013 Turn on electricity ◦ Some electrons shuffle from 1 electron to the next Quick in metals Conductors ◦ E.g. Metal Insulators ◦ E.g. rubber & plastic Circuit ◦ Like a pipe/tube of wires © Andrew Newbound 2013 © Andrew Newbound 2013 Insulators and Conductors Battery of galvanic cell © Andrew Newbound 2013 Thicker wires = higher electricity ◦ Dangerous with thinner insulation Semiconductor ◦ Properties between insulators and conductors ◦ Can be changed by heat/light © Andrew Newbound 2013 Leclanché cells ◦ Zinc case which slowly dissolves Releases electrons Move through wire, produce current Button cells ◦ Use zinc + mercury/silver Fuel cells ◦ Make electric current Controlled reaction between a fuel & oxygen © Andrew Newbound 2013 Lead-acid batteries in cars & trucks ◦ Don’t make electricity ◦ Store chemicals which release electrons in chemical reactions ◦ Accumulator Proper name Storage battery Solar panels ◦ ◦ ◦ ◦ Consist of solar cells Made of thin slices of silicon Also called photovoltaic cells Convert sunlight energy to electrical energy © Andrew Newbound 2013 © Andrew Newbound 2013 Electrochemical cells ◦ Produce electricity by chemical reactions Wet cell ◦ Zinc + copper dipped in SALT WATER Dry cell ◦ Contains NO FREE LIQUID © Andrew Newbound 2013 Atoms ◦ Everything has ◦ Have nucleus Orbited by electrons Flow of electrons from one atom to another ◦ Always in wire Turn switch on Turns on immediately ◦ Electrical energy in electrons is converted to Heat energy Light energy Kinetic energy © Andrew Newbound 2013 Electricity travels through wires ◦ Makes an electric current Series Circuit Parallel Circuit © Andrew Newbound 2013 Used by scientists to draw circuits Straight lines ◦ Wires = easier to follow Universal symbols ◦ Easier to read © Andrew Newbound 2013 Single battery (power pack) Wire Light bulb Ammeter Voltmeter © Andrew Newbound 2013 Double cell (2 batteries) Triple cell (3 batteries) Open switch Joined wires Resistor © Andrew Newbound 2013 Controlled break in circuit Break in circuit ◦ Electricity stops flowing Series circuit ◦ 1 bulb broken = no lights on Parallel circuit ◦ 1 bulb broken = most on © Andrew Newbound 2013 Used to turn lights on and off at different spots On Off On Off © Andrew Newbound 2013 Measure in amperes (amps) ◦ Symbol = A ◦ E.g. 5 A = 5 amps Measure of number of electrons that flow in given time Measured using ammeter © Andrew Newbound 2013 Electrons only have 1 path to follow ∴ Current is the same at all ammeters © Andrew Newbound 2013 Electrons only have 2 paths to follow ∴ Current less than total through each light © Andrew Newbound 2013 Energy before use minus energy after use Symbol = V Tells how much energy has been used © Andrew Newbound 2013 How easy it is for electricity to flow through a conductor Thin wires greater resistance than thick wires ◦ Less atoms for electrons to flow through Measured in Ohms Symbol = Ω © Andrew Newbound 2013 𝑉 𝑅= 𝐼 © Andrew Newbound 2013 Voltage increases = current increases = resistance increases Resistance increases = current decreases = voltage increases Current increases = voltage increases = resistance decreases © Andrew Newbound 2013 Voltage (potential difference) ◦ Pushes electrons Current ◦ How fast electrons are moving Ammeter Voltmeter Multimeter – measures amps – measures volts – measures amps and volts © Andrew Newbound 2013 Switch = dam in river Current = how fast water flows Potential difference = difference between speed of water © Andrew Newbound 2013 Used to produce heat & light Called a filament Used in ◦ ◦ ◦ ◦ Light bulb Oven Heater Toaster etc. Thermal effect ◦ Electrons produce heat They are moving but have nowhere to go © Andrew Newbound 2013 Electrons returning to start having done no work © Andrew Newbound 2013 Watt ◦ Rate energy is used by an electric device Converted from electrical energy to another form 1 watt = 1 joule per second Kilowatt (kWh) = 1000 watts Kilowatt-hour Determine amount of power used ◦ Multiply kilowatts by amount of hours © Andrew Newbound 2013 𝑃 = 𝐼𝑉 © Andrew Newbound 2013 𝑤𝑎𝑡𝑡𝑠 × ℎ𝑜𝑢𝑟𝑠 1000 © Andrew Newbound 2013 Work out current a machine normally needs Choose smallest fuse value that will comfortably do the job © Andrew Newbound 2013 𝑃 𝐼= 𝑉 © Andrew Newbound 2013 Located in ◦ ◦ ◦ ◦ Iron Cobalt Nickel But facing different dirrection © Andrew Newbound 2013 Stroke with magnet Electricity Heating and tapping © Andrew Newbound 2013 Electricity aligns domains Can be turned on and off E.g. ◦ Compass changes direction around electricity ◦ Wire around nail Is magnet © Andrew Newbound 2013 Speakers Microphones Security system 1. Button turns on electromagnet 2. Pulls steel latch from door Electric bell ◦ Makes and breaks ringing © Andrew Newbound 2013 Circuit breaker ◦ Will turn off when a certain amount of magnetism is reached ◦ Does not turn itself back on Must be reset manually Solenoids ◦ Coils of wires that produce electromagnetism ◦ Used to detect electric current Used in ammeters Coil of wire attracts and repels needle © Andrew Newbound 2013 Unit 5 © Andrew Newbound 2013 Aristotle ◦ Though earth was centre of universe ◦ Geocentric Copernicus ◦ Though solar system revolved around sun ◦ Heliocentric Tycho Brahe ◦ Couldn’t prove earth moved © Andrew Newbound 2013 Kepler ◦ Proved that planets moved in elliptical orbit Law of areas ◦ Built on Brahe’s work Kepler’s Laws 1. Sun at centre – planets move in elliptical orbit 2. Planets move faster the closer to the sun 3. Planets that are further out move slower © Andrew Newbound 2013 Geocentric (Aristotle) Heliocentric (Copernicus) © Andrew Newbound 2013 Brahe’s Model Kepler’s Model © Andrew Newbound 2013 Galileo ◦ Used a telescope ◦ Discovered there were stars in the milky way Not just glowing dust ◦ Discovered moon was not perfect sphere Had craters ◦ Discovered other centres of the universe Jupiter had moons ◦ Law of inertia If you set something in motion it will continue in that motion if nothing influences it © Andrew Newbound 2013 Newton ◦ Discovered gravity Combined with inertia to describe how planets moved ◦ Believed gravity was between every particle and every other particle © Andrew Newbound 2013 Object Wave Type Radio Radio waves Mobile Microwave TV TV waves Remote Infra-red Microwaves Microwaves X-Rays X-Rays UV Lamp U V rays Sun/sunscreen UV rays Radiotherapy for cancer Gamma rays © Andrew Newbound 2013 All have electromagnet energy Travels in waves Does not need a medium to pass through © Andrew Newbound 2013 λ © Andrew Newbound 2013 Wavelength ◦ Distance of 1 wave ◦ Measured from one point on wave to corresponding point (E.g. from crest to crest) ◦ How long it is Amplitude ◦ Distance up or down from middle Frequency ◦ How frequent the waves are ◦ How many waves travel in a second ◦ Measured in hertz (Hz) © Andrew Newbound 2013 Inverse relationship between wavelength and energy Smaller the wavelength, the more energy The larger the wavelength, the less energy © Andrew Newbound 2013 Or natural or visible light Made up of different colours Violet Blue Green Yellow Orange Red Small wavelength Long wavelength Large energy Small energy Each colour has own wavelength Part of electromagnetic spectrum ◦ Part we can see © Andrew Newbound 2013 Ultraviolet ◦ Beyond violet Infrared ◦ Below red © Andrew Newbound 2013 © Andrew Newbound 2013 Most comes from radiation ◦ From objects that are extremely hot Iron at 100°C radiates heat at 0.03 watts per cm2 ◦ Small but measurable ◦ Cannot see as is infrared In a fire ◦ A lot more energy is radiated Some as visible light © Andrew Newbound 2013 Ways can be produced ◦ ◦ ◦ ◦ Heat Electricity Sun Solar wind Light meets another object ◦ Reflection – bounces back ◦ Refraction – goes through at angle ◦ Transparent – straight through © Andrew Newbound 2013 Through transparent material ◦ Vibrates particles in material ◦ Creates new photons ◦ Slows down Sunlight consists of ◦ Colours of rainbow © Andrew Newbound 2013 Radio waves ◦ Longest wavelength on spectrum ◦ Carry news, ball games and music on the radio ◦ Carry TV and phone signals Microwaves ◦ Shorter than radio waves ◦ Heat food we eat ◦ Used for radar images Like Doppler radar used in weather forcases © Andrew Newbound 2013 Infrared ◦ Longer wavelengths Detected as heat Given off by radiator/heater Thermal infrared ◦ Shorter wavelengths Given off by sun Plants reflect Near infrared waves © Andrew Newbound 2013 Visible light ◦ ◦ ◦ ◦ ◦ ◦ Can see Colours of rainbow Each colour has different wavelength Red = longest wavelength Violet = shortest wavelength Combine to make white light ◦ ◦ ◦ ◦ Shorter than visible light waves Invisible to human eyes Some insects see them Responsible for sunburns Ultraviolet © Andrew Newbound 2013 X-Rays ◦ More energy than ultraviolet waves ◦ Can pass through skin Let doctors see bones Gamma Rays ◦ Most amount of energy ◦ Generated by radioactive atoms + nuclear explosions ◦ Can kill living cells Used in cancer treatment © Andrew Newbound 2013 Most of time spent on studying electromagnetic energy ◦ Made in universe Only visible light, radio waves come through atmosphere ◦ Telescopes on ground can only detect these Light telescope (optical) ◦ Lenses to reflect, refract light to magnify object Radio telescope ◦ Detect radio waves Change into picture © Andrew Newbound 2013 Different types of stars ◦ Different types, amounts of electromagnetic energy © Andrew Newbound 2013 Brightness ◦ How far away the star is ◦ How big star is Colour ◦ Blue = hottest ◦ Red = coolest Distance ◦ Using red-shift © Andrew Newbound 2013 Light from star = Brocken into spectrum Black lines on spectrum ◦ Colours absorbed ◦ Each element absorbs 1 or more colours ◦ Where black lines are = which elements in star © Andrew Newbound 2013 Spherical ◦ Sphere like shape Celestial sphere ◦ Belief that night sky is a sphere Independently ◦ By oneself Heliocentric ◦ The sun is the centre of the solar system Classifying ◦ Put into groups © Andrew Newbound 2013 Reflected ◦ To put out light from another source Heretical ◦ Crime against the state Geo… (prefix) ◦ Earth Helio… (prefix) ◦ Sun © Andrew Newbound 2013 Wanderers ◦ Term from early astronomy ◦ Objects that moved independently of the celestial sphere ◦ Moon ◦ Sun Inquisition ◦ Killing anyone who spoke out against church ◦ Took anyone who said sun was centre of universe © Andrew Newbound 2013 No one spoke out against church ◦ Power in communities ◦ Killed if did Church stopped stopping advance of scientific understanding in 1600s ◦ Believed that if meddled would look even worse ◦ Weren’t only learned in community ◦ More evidence against church’s view on science © Andrew Newbound 2013 Early astronomers noticed earth was round ◦ Curved shadow on moon during eclipse Venus proved heliocentric model ◦ Went through phases like moon ◦ Earth blocking sun ◦ Light reflecting off it © Andrew Newbound 2013 Later scientists contributed more to astronomy ◦ ◦ ◦ ◦ ◦ ◦ More mapping Didn’t disagree with beliefs Built on others teachings Invented technologies More intelligent No death threats © Andrew Newbound 2013 384-322BC ◦ First evidence of curved earth 310-230BC ◦ Heliocentric model 276-194BC ◦ Circumference of earth determined (46000km) Slightly higher than actual circumference (41000km) 127-151AD ◦ Stars catelogued © Andrew Newbound 2013 1473-1543AD ◦ Heliocentric model proof 1571-1630AD ◦ 3 laws of planetary motion 1564-1642AD ◦ 1st telescope 1643-1727AD ◦ 1st astronomer to use maths © Andrew Newbound 2013 In sound ◦ Pitch increases as source approaches Waves shoved together Apparent increase in pitch ◦ Pitch decreases as source moves away Waves spread apart Apparent decrease in pitch Sound ◦ Consists of travelling compressions/refractions of air pressure Longitudinal/compressional waves Closer crests = higher frequency © Andrew Newbound 2013 Same with electromagnetic radiation ◦ Just another wave phenomenon Frequency increases = blue shift Frequency decreases = red shift ◦ Not actual colours ◦ Just redder/bluer Most parts of electromagnetic spectrum used Determine how fast objects move toward and away from earth © Andrew Newbound 2013 Use hydrogen ◦ Wavelengths 21cm = no shift 21.1cm = 0.1cm red shift 19.9cm = 0.1cm blue shift © Andrew Newbound 2013 Galaxy moving towards earth ◦ Waves bunch up as approaches telescope Shifts colour towards blue ◦ Visa versa © Andrew Newbound 2013 About 14 billion years ago ◦ Universe compressed into very tiny space Size of pinhead ◦ Exploded ◦ Created universe that expanded in all directions Evidence ◦ Red shift Spectrum is shifted towards red (moving away) ◦ Static radiation can be detected Back radiation from Big Bang © Andrew Newbound 2013 Object with gravity so strong that nothing can escape it ◦ Not even light If earth compressed to black hole ◦ 12cm diameter Detect ◦ Observing bodies orbiting them ◦ Observing them ripping the gas off a star As gas accelerates – gives off x-rays Typical black hole ◦ 40 million times heavier than sun © Andrew Newbound 2013 Clusters of star systems which themselves join together into larger systems Types: ◦ Spiral galaxy elliptical galaxy irregular galaxy © Andrew Newbound 2013 Small rocky world Most revolve around sun between Mars and Jupiter (asteroid belt) Struck earth many times Made of ◦ ◦ ◦ ◦ Carbon (C-type) Silicate (S-type) Metallic (m-type) (metal) Dark Water ice/frozen carbon monoxide mixed with rock © Andrew Newbound 2013 © Andrew Newbound 2013 Dirty snowball Size of mountain Long/narrow Tails of gas and dust when approaching sun Haley’s Comet ◦ Orbits every 76 years © Andrew Newbound 2013 Chunk of rock/metal/dust in space Shooting star ◦ Not actually stars Small bits of rock burning up in the atmosphere © Andrew Newbound 2013 Meteoroids that pass through Earth's atmosphere that survive and hit Earth’s surface Types ◦ Stone ◦ Iron ◦ Stony iron © Andrew Newbound 2013 Sky as seen from Earth Large hollow ball with Earth in centre Stars = inside of hollow sphere © Andrew Newbound 2013 Angle from north to point on the horizon Measured in a clockwise direction by a compass E N S S © Andrew Newbound 2013 Point above horizon Azimuth and elevation used together to locate a star Zenith (90°) Horizon (0°) © Andrew Newbound 2013 © Andrew Newbound 2013 All elements made in star by fusion 2 hydrogen's fuse together to make helium and energy © Andrew Newbound 2013 © Andrew Newbound 2013 Oldest = Sirius B (white dwarf) Burning hydrogen as fuel ◦ Main sequence ◦ Vega, Alpha, Centuri B Burning helium as fuel ◦ Red giants, blue giants Betelgeuse (beetle juice) Closest to death ◦ Sirius B (white dwarf) © Andrew Newbound 2013 Highest luminosity ◦ Blue giants/super giants Cause of luminosity ◦ Size Lowest luminosity ◦ White dwarf, red dwarf ◦ E.g. Sirius B Highest surface temperature ◦ Blue giants © Andrew Newbound 2013 Main sequence stars ◦ Become Red Giants when runs out of hydrogen Vega, Alpha, Century B ◦ Will become white dwarfs Sirius B ◦ Will not become a main sequence star Was Vega = next Red Giant Betelgeuse = next black hole/neutron star © Andrew Newbound 2013 Unit 6 © Andrew Newbound 2013 Neurons ◦ Shape and size to allow them to carry messages Verves ◦ Bundles of neurons Sensory neurons ◦ Neurons in sense organs ◦ Carry a message in 1 direction only From sense organ to brain/spinal column ◦ Work constantly if internal ◦ Essential in maintaining homeostasis © Andrew Newbound 2013 Neuron ◦ Carry messages Axon ◦ Carries the nerve impulse Dendrites ◦ Joints in cells Toxins ◦ Poisons Synapse ◦ Gap between neurons CNS ◦ Central Nervous System © Andrew Newbound 2013 MS (Multiple Sclerosis) ◦ Caused by myelin sheath breaking down Paraplegia ◦ Caused by broken nerves © Andrew Newbound 2013 Sensory neurons ◦ Detect stimulus of light/heat ◦ All about senses ◦ Carry messages in 1 direction From sense to brain Motor neurons ◦ Movement ◦ Joins CNS to a muscle/gland Interneuron ◦ Connects sensory and motor neurons © Andrew Newbound 2013 Skeleton ◦ ◦ ◦ ◦ ◦ >200 bones Supports Protects Helps body move Place where bones meet joint Muscles ◦ No muscles = movement ◦ Only pull ◦ In pairs © Andrew Newbound 2013 Nerves ◦ Switch muscles on and off ◦ Messages = nervous impulses ◦ Joined at spinal chord Cerebral cortex ◦ Movement Blood ◦ Over half=plasma ◦ Go around world twice if put end to end © Andrew Newbound 2013 Heart ◦ Can fill a petrol tanker in 1 day ◦ Beats faster after exercise Digestive system ◦ Energy ◦ 7.5m – length of small intestine © Andrew Newbound 2013 Nervous system ◦ Group of tissues and organs Just like digestive/circulatory system Nerve cells ◦ Longest cell in our body ◦ Called a neuron © Andrew Newbound 2013 Organised into Central Nervous System (CNS) and Peripheral Nervous System (PNS) CNS ◦ Brain and spinal chord ◦ Body’s control centre ◦ Organises information from sensory organs and receptors ◦ Issues outgoing commands to parts of the body ◦ Brain protected by skull ◦ Spinal chord protected by spine © Andrew Newbound 2013 PNS ◦ ◦ ◦ ◦ Sensory neurons and motor neurons Sense organs Muscles Glands © Andrew Newbound 2013 © Andrew Newbound 2013 Receptors Stimulus Sensory organs CNS Response Motor neurons Effectors © Andrew Newbound 2013 Receptors – sensory neurons ◦ Hands, eyes, nose, tongue, ears, detect blood pressure, organs ◦ Receive information which gets transmitted to the brain © Andrew Newbound 2013 Rapid involuntary movement or response Important in times of danger E.g. Blinking, being startled by a bad noise Fast ◦ Few neurons involved ◦ Many never reach brain, only go as far as spinal cord © Andrew Newbound 2013 Brain Spinal cord Nerves Controls everything we do ◦ Sends information through neurons Allows us to read stimuli and respond accordingly © Andrew Newbound 2013 Longest cells in the body Neural messages ◦ Received in the dendrites ◦ Transmitted along the axon to axon terminals ◦ Transmitted between neurons by chemicals Neurotransmitters © Andrew Newbound 2013 © Andrew Newbound 2013 Controls organs of our bodies Hormones ◦ Releases hormones ◦ Control various functions Growth Development Reproduction ◦ Produced in glands E.g. Thyroid Pituitary Adrenal Pancreas Testes Ovaries © Andrew Newbound 2013 Glands ◦ Small organs that release hormones Hormones ◦ Go through bloodstream ◦ Tell cells what to do © Andrew Newbound 2013 Pituitary gland ◦ Incharge ◦ Releases hormones to control many other glands ◦ Controls body functions Thyroid ◦ Growth hormones ◦ Stay alert ◦ Full of energy Adrenal glands ◦ Gives boost Pancreas ◦ Helps glucose enter cells © Andrew Newbound 2013 Puberty ◦ Type of rapid growth and development Sexual maturity ◦ Lead to when sex hormones cause changes Hypothalamus releases hormone ◦ Tells pituitary gland to release a hormone Acts on the gonads to release sex hormones Testosterone and oestrogen Male sex cells Female sex cell = testes = ova (egg) © Andrew Newbound 2013 Cerebrum c © Andrew Newbound 2013 Weighs 1.4kg Cerebrum ◦ ◦ ◦ ◦ Thinking part of brain Controls muscles Where memory lives Lets you reason Hypothalamus ◦ Controls temperature Cerebellum ◦ Balance, movement and coordination © Andrew Newbound 2013 Brain stem ◦ ◦ ◦ ◦ Connects rest of brain with spinal cord Breathing air Digesting food Circulating blood Pituitary gland ◦ Produce + release hormones into body ◦ Puberty ◦ Metabolism Amygdala ◦ emotions © Andrew Newbound 2013 Cortex ◦ Controls activity of body’s moving parts Cortex ◦ Thinking, remembering & problem solving Receptors ◦ Sense Effectors ◦ React to sense © Andrew Newbound 2013 Hormone Source of Hormone Comment Adrenalin Adrenal Glands Increases breathing rate May be caused by fright, rage or and heart beat excitement Insulin Pancreas Too much glucose in blood Helps cells extract glucose from blood. Thyroxin Thyroid glands Controls rate of cell respiration Pituitary Pituitary gland (under brain) Hormones Controls other glands Sex Testes Hormones Ovaries Produce sperm Produce ova (eggs) © Andrew Newbound 2013