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docbgeochangesans updated Jan 19th 2008 |
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GCSE-KS4 Science answer notes on ATMOSPHERIC and GEOLOGICAL CHANGES on EARTH based on a GCSE TASK SHEET * Earth Science Homepage 5 multi-word fill GCSE worksheets + answers * EMAIL query?comment GCSE Earth Science: Foundation-easier m/c Quiz and Higher-harder level m/c Quiz ANSWERS 1. The Evolution of the Earth's atmosphere and Carbon Cycle ... 2. The Rock Cycle and types of rock (details 'evolve' through sections 3. to 9.) ... 3. Weathering of Rocks ... 4. Igneous Rocks ... 5. Sedimentary Rocks ... 6. Metamorphic Rocks ... 7. The Structure of the Earth ... 8. Plates and their movement ... 9. Plate Tectonics ... 10. The Moon and Planets 1. The Evolution of the Earth's atmosphere breathe easy! 1(a)(i) Today's atmosphere consists of the elements: 78% nitrogen (about 4/5ths), 21% oxygen (about 1/5th), 1% argon (1/100th), traces of other Group 0 Noble Gases (He, Ne, Kr, Xe), plus the compounds 0.036% carbon dioxide (360 ppm or parts per million) and variable amounts of water vapour (depends on humidity) and traces of many other gases from natural or man-made pollution sources (e.g. sulphur dioxide, nitrogen dioxide and carbon monoxide from fossil fuel combustion (see Oil Products notes) and methane (greenhouse gas) from cows and decomposing plant material). The composition of our atmosphere is thought to be relatively unchanged for about 200 million years due to the Carbon-Cycle balance. 1(a)(ii) One method to determine the % of oxygen in air is to use two 100cm3 glass gas syringes are connected either side of a piece of silica tubing containing copper powder or fine granules. One syringe is empty and the other filled with 100cm3 of air. The silica tube/copper is strongly heated and the gas syringes moved to and fro to pass the air over the hot copper. The oxygen in the air reacts with the copper to form copper(II) oxide. 2Cu(s) + O2(g) ==> 2CuO(s) This is a black solid of little volume. Eventually the total volume reading reaches a minimum value when all the oxygen in the air has reacted. 100 - final reading gives the % oxygen in air. 1(a) water + carbon dioxide + sunlight energy ==> glucose sugar + oxygen 6H2O(l) + 6CO2(g) ==> C6H12O6(aq) + 6O2(g) 1(a)(iv) Production of carbon dioxide: Natural burning of biomass like forests, plant and animal respiration**, biological decay of plant and animal material, 'mans' burning/combustion of fossil fuel, volcanic activity e.g. the thermal decomposition of minerals like carbonates in magma/lava. See Oil notes for more on fossil fuels. ** Respiration: glucose sugar + oxygen ==> water + carbon dioxide + energy (exothermic, energy given out) C6H12O6(aq) + 6O2(g) ==> 6H2O(l) + 6CO2(g) 1(a)(v) Oxygen balance: The main process of CO2 removal by photosynthesis also produces oxygen. Respiration and combustion (natural/man) mainly remove the oxygen from our atmosphere. So this means the Carbon-Cycle effectively maintains a constant % of oxygen in the atmosphere as well as controlling the carbon dioxide levels. (Note: as far as we know the Greenhouse Effect will not significantly change the oxygen level in the Earth's atmosphere). There is no evidence to suggest that the increase in the world's population (respiration!) or the burning of forests (deforestation by combustion) is having any effect on the oxygen level BUT increase in 'man's' industrial and domestic activity by burning fossil fuels is causing the carbon dioxide concentration to rise.
1(c)(i) Seas and oceans would form from condensed water vapour as the early Earth surface cooled down. Carbon dioxide and ammonia would dissolve in this water. 1(c)(ii) The carbon dioxide could form soluble sodium carbonate, sodium hydrogencarbonate or calcium hydrogencarbonate and insoluble calcium carbonate.
1(d) Primitive bacterial life evolved about 3500 million years ago (3.5 billion y) and the first green algae like plants from about 2000 million years ago (2.0 billion y). The increasingly successful evolution of green photosynthesizing plants colonising both land and water, produced an increasingly oxygen richer atmosphere and in so doing removing most of the carbon dioxide from the original early atmosphere. This 'oxygenated' atmosphere would be 'polluting' and 'toxic' to many microorganisms which could not tolerate oxygen, having evolved in a non-oxygen environment. However, by 1000 million (1 billion years) years ago, there was sufficient oxygen to allow the evolution of respiring animal life. 1(e)(i) Ammonia would be converted to soluble nitrates mainly by nitrifying bacteria or, to a small extent, ammonia would be directly oxidised to nitrogen gas by the newly formed oxygen. The nitrates are absorbed by plants to form proteins or converted to atmospheric nitrogen by denitrifying bacteria. 1(e)(ii) Methane would be oxidised to carbon dioxide and water by the new 'oxygenated' atmosphere. 1(e)(iii) Ozone (O3) would now be formed and this would absorb and filter out much of the ultraviolet light that is harmful to many organisms. This uv filtering would then allow the much wider evolutionary development of plant and animal organisms. 2. The Rock Cycle the "1st Big Picture View" Many of the features of the rock cycle are illustrated below in Fig 2.1 The Rock cycle. (see also Fig 8.1 and Fig 9.2) Sections 3. to 9. take you through all the details. Rocks are classified into groups of IGNEOUS, METAMORPHIC and SEDIMENTARY ROCKS depending on their origin.
3. Weathering of Rocks they all wear away eventually! (3a) Weathering of Rocks means the process of breaking them up into smaller fragments and it can occur in many different ways.
3(b) (3b) Erosion is the wearing away of the rock as a result of the weathering processes described above. Examples of erosion are the wearing away of mountains and the creation of river valleys and gorges.
4. Igneous Rocks form the fastest and last the longest!
Note (i): There is quite a variety of mode of formation though e.g. some volcanic rocks are very hard and 'glassy', others form from ash deposits from volcanic eruptions. They sometimes occur as intrusions into other pre-existing rocks (see below) and the crystal size and type of igneous rock also depends on the rate of cooling. Note (ii): You often see the lava bubbling as dissolved gasses under pressure in the mantle are released into the atmosphere - sometimes with explosive force!
4(c)(i) An igneous intrusion is where a mass of very hot 'plastic' magma from the mantle rises and 'bulges' up into the crust and cools to form igneous rock. This is often granite because it will cool very slowly as the surrounding rocks act as an insulator. The intrusion may 'push' up through many layers of previously formed sedimentary rock (see section 5. and section 6.). 4(c)(ii) If these sedimentary rocks are then weathered away, the harder wearing granite remains as a hill or mountain. 4(c)(iii) The igneous intrusion rock must be younger than the surrounding sedimentary rock because it is formed by the magma cooling in the previously existing rock layers.
Basalt is described as an extrusive rock because it 'extrudes' out into air or water to cool and form the solidified rock. It is formed by the fast cooling of magma and the crystals are relatively small because of the fast cooling. It consists of interlocked microscopic crystals which are darker in appearance compared to granite. This situation is found when lava/magma cools rapidly when flowing out into air or water. Basalt rocks are sometimes called fine-grained rocks because of the mixture of interlocking tiny crystals. 5. Sedimentary Rocks slow to form and weather the fastest!
5(b) Types of sedimentary rock
5(c) Since limestone is mainly calcium carbonate CaCO3, and a simple test is to add acid - should giving fizzing of a colourless gas that turns limewater 'milky' i.e. carbon dioxide CO2 is formed. Heating limestone to a high temperature in a limekiln produces calcium oxide (quicklime, a strong alkali). Lime is used in agriculture to treat fields which are too acidic for healthy crop growth. Limestone is used as building stone and in the manufacture of glass and concrete. 5(d) Any rocks which are not eroded away, are eventually returned to the mantle when plates descend in tectonic activity - see later.
5(f)
5(g) At the surface of the Earth younger sedimentary rocks usually lie on the top of older rocks. All sorts of features found in sedimentary rock formations allow scientists to work out their origin and what has happened to them over long time periods of time e.g.
6. Metamorphic Rocks formed through the action of heat and pressure!
Large scale movements of the Earth's crust can cause mountain ranges to form very slowly over millions of years. These replace older mountain ranges worn down by weathering and erosion. Metamorphic rocks are associated with the Earth movements (tectonic activity) which created present-day and ancient mountain belts. They are evidence of the high temperatures and pressure created by these mountain-building processes. 6(a) A metamorphic rock is one that is formed directly from a pre-existing rock. Heat and pressure are the 'driving forces' for metamorphic rock formation in which the grains of pre-existing rocks are re-crystallised. The pre-existing rocks involved are usually deep in the crust where they are subjected to great pressure. The high temperatures often needed, are due to rocks being near the hot mantle, or when an igneous intrusion rises, or volcanic rock heats other surrounding rock and when continental plate meets oceanic plate (see (3) in Fig 8.1).
6(b) The link between metamorphic rocks and igneous intrusions is shown on the left and in diagram Fig 4.1. The rising magma heats up the surrounding sedimentary (or igneous) rocks producing metamorphic rocks such as marble, slate, gneiss or schist. Note: There are high-low grades of metamorphism depending on the high-low temperatures and pressures particular pre-existing rocks are subjected to. For example, the rocks become 'less metamorphic' the further you go from the igneous intrusion as you go to a lower temperature. 6(c) Slate is formed from sedimentary rocks such as shale, mudstone or clay deposits and the re-crystallised layers are easily split - hence its use in roofing. Sometimes, but rarely, fossil traces are preserved in the layers through the crystallisation process. 6(d) Marble is a hard rock formed from the action of heat and pressure on the sedimentary rock limestone. It will still give carbon dioxide with acid but is much harder physically than limestone or chalk. 6(e) Gneiss, quartzite and schist are metamorphic rocks formed by the action of heat and pressure on pre-existing igneous or sedimentary rocks. They can form from igneous rocks* like granite or basalt, from metamorphic rocks* like slate or from sedimentary rocks like shale, mudstone or sandstone, and chemically they are mainly 'silica' SiO2. * Note, the original pre-existing rock does not have to be sedimentary!
6(f) Metamorphic rock has the same chemical composition as the original rock it was formed from (in terms of % elements). This is because no minerals are added or lost in the recrystallisation process. For example, the Ca:C:O ratio is the same in the sedimentary limestone rock as it is in the resulting metamorphic rock marble, because chemically they are both mainly calcium carbonate CaCO3. 7. The Structure of the Earth a sort of egg?
7(a-b) The three layered structure of the Earth. X is the crust: is the relatively thin and cool outer layer of the Earth. The thickness ranges from 6 to 40km. It is much cooler, harder, brittle and less dense than the other layers. The crust is divided into sections or 'plates' which 'float' and move on the mantle. 2/3rds of the surface is water. Y is the mantle: is very hot rock material, it is almost solid but the 'plastic' rock can move very slowly as huge convection currents driven by the heat from radioactive decay in the core. It is these convection currents which move the 'plates'. The mantle's 'thickness' is 3000 km and its temperature is usually over 1000oC. It consists mainly of non-metallic silicates with some metal ions. Magma is heated molten rock, from the more 'runny' mantle material and comes up to the surface in volcanic activity or igneous intrusions. The mantle has a higher density and a different chemical composition compared to the crust. It is relatively cold and rigid just below the crust, but lower down it is much hotter and non-rigid and so is able to flow. Z is the core: is composed mainly of iron, nickel and other metals. Its diameter is about half that of the Earth (3500 km radius) and its is very hot and dense. The core consists of an outer liquid layer and a solid inner layer. The heat is generated by radioactive decay of longer lived isotopes and is transferred into the mantle. It is this heat that drives the convection currents in the mantle, which ultimately moves the tectonic plates of the crust. The mainly iron core generates a magnetic field through and around the Earth. Some general points: The overall density of the Earth is much greater than the average density of the rock of the crust. This is evidence that the inner layers of the Earth are made of different more denser materials from that of the crust e.g. the metallic core. The lithosphere is the rigid, relatively cool crust, and the outer or upper part of the mantle. It is split into sections called plates. 7(c) The age when rocks where formed in or on the crust can be estimated in various ways ..
8. Plates and their movement unstoppable tectonics! (introducing the basic ideas and evidence - see also section 9.)
The 'compact' diagram Fig 8.1 Plate Tectonics above gives the "2nd Big Picture View" view of plate tectonics and the situations at (1) to (4) will be referred to throughout the answer notes to 8. and 9. "The Earth's lithosphere (the crust and the upper part of the mantle) is cracked into a number of large pieces (tectonic plates) which are constantly moving at relative speeds of a few centimetres per year as a result of convection currents within the Earth's mantle driven by heat released by natural radioactive processes. Earthquakes and/or volcanic eruptions occur at the boundaries between tectonic plates." 8(a) The Earth's lithosphere is the crust and the upper part of the mantle. The Earth’s lithosphere is divided into plates meaning they are divided into sections that meet at plate boundaries (situations (1) to (4) all represent plate boundary regions). The plates effectively float on the more dense mantle material and move at speeds of 1-4 cm/year. The crust is the lightest rock of the three layers of the Earth. The crust plate material under continents tends to be thicker and made of lighter 'granites' but oceanic crust is a thinner but more denser 'basalt' type rock. 8(b) Plate movement, refer on the Fig 8.1 to (2)
8(c) Where the plates of the Earth meet is called a plate boundary. Some of the evidence which is used to ‘map out’ the plate boundaries ...
8(d) At one time it was believed that the major features of the earth's surface were the result of the shrinking of the crust as the Earth cooled down following its formation. Wegener's theory of crustal movement ('continental drift') was not generally accepted until more than 50 years after it was proposed, so why not?
9. Plate Tectonics (using the basic ideas to explain all the effects) 9(a) When plates move apart: New crust is formed mainly at mid-ocean ridges where magma breaks through a huge fractures in the crust. ((2) in Fig 8.1) This is known as sea floor spreading and is happening along oceanic ridges, including the mid-Atlantic ridge. This causes cracks through which more molten magma material from deep below the lithosphere can push through producing new rock. The magma from theses chains of linked undersea volcanoes (or just long gashes of hundreds of kilometres!) rapidly cools to form basalt type rocks of the new crust spreading out on either side. (see also evidence for this mechanism) Sometimes a long central rift valley forms (4). All in all, what is described below, is the detail of the ultimate rock recycling machine! 9(b) When plates collide [more in 9(c)]: Crust material is removed from the tectonic plates whenever two plates collide head on because one plate descends into the subduction zone to be melted and combined with the mantle material ((1) oceanic-oceanic plates meeting (e.g. Pacific Ring of Fire) and (3) oceanic-continental plates meeting (e.g. Andes Mountains) in Fig 8.1). One plate descends into a deep ocean trench, and mud and sand pour into these trenches and at (3) can end up as bands of metamorphic rock in the 'fold' mountains - see 9(c). 9(c) When continental plate meets oceanic plate the thinner more dense oceanic plate subducts below the continental plate, and partly melts under the thicker but less dense granitic plate. Deep ocean off-shore trenches are formed and parallel mountain chains with volcanoes and earthquake activity too. The geology can be complex and the sediments of the continental crust get crunched up into fold mountains. Metamorphic rocks can be formed due to the heat and pressure in the processes (casing recrystallisation without melting), accompanied by considerable faulting, folding, igneous intrusions and volcanoes. Some of the molten rock cools deep below the surface to form course-grained grained rocks like granite. The magma which rises to the surface cools rapidly to form fined grained rocks like basalt lava or volcanic ash. If continental plates meet (i.e. after all the ocean has been squeezed out!), the massive collision and compression can build up huge mountain ranges like the Himalayas. Even the pre-existing sedimentary rocks, like limestone and sandstone from the seas originally between the plates, can be squashed up and become part of the fold mountain ranges (the top of Mount Everest is limestone!). They can also be heated to give regions of metamorphic rock, more folding and compressional faulting. The whole process goes on for millions of years! and these 'new' mountain ranges replace 'older' ones worn down by weathering and erosion processes. See below for side-ways passing movement.
9(e) Volcanoes tend to form where plates meet ((1) (e.g. Pacific Ring of Fire) and (3) (e.g. the east Pacific ocean trench and the Andes Mountains on the South American plate) in Fig 8.1). The crust and mantle are disturbed in the subduction zone and extra heat is generated from compression and friction. Some of the upper mantle becomes much more fluid, 'gassy' and less dense. This results in hot magma working its way upwards to break through as a volcano. The explosive force of volcanoes is usually due to the rapid release of high pressure gas trapped in the magma. This can throw out huge quantities of magma, rocks and volcanic ash to form surrounding deposits which can be studied by volcanologists to research the history of a volcanoes eruptions.
an anticline near Mizen Head, West Cork, Ireland
9(g) A rift valley is formed on continental crust when two plates move away from each other and the land in between falls as shown in (4). This is exemplified by the Great Rift Valley of Africa but it can also be filled with sea water e.g. the Red Sea between the African Continent and the Arabic states. 9(h) In Fig 8.1 the loss of plate at (1) and (3) is matched by the creation of new crust at (2)! 9(i) In situation (2) new crust is formed but at (1) and (3) crust is being moved. So all new rocks have their start at (1) and eventually end up, in whatever rock form, by returning to the mantle at (1) or (3). Hence all mineral material is eventually recycled in the 'big picture' shown in Fig 2.1 and Fig 8.1. Most of these 'answer notes' are looking at the details of all the primary and secondary processes involved. Note in Fig 8.1 the arrow ==> on the right could match up with the ==> on the left i.e. its a 'balanced' global cycle both internally and externally! Any mountain ranges not subducted still get worn away by weathering and erosion, so everything gets recycled in the end! Fig 9.2 A simpler approach to the "THE ROCK CYCLE" to show the relationship between the three types of rocks - the "3rd Big Picture View"
10. The Moon and Planets What atmosphere and rocks are out there beyond Earth? (just a little extension!) 10(a) There would be little or no oxygen like all of the other planets, no photosynthesising life on them, but they have gases such as hydrogen, ammonia, methane and carbon dioxide on planets which you find in the atmosphere of Jupiter, Saturn, Neptune and Uranus. 10(b) On Mars there appears to be eroded, but now dry, river beds and cliffs showing 'weathered' or 'erosion' features. 10(c)
10(d)(i) The surface on Venus is much hotter than the Earth, not only because it is closer to the Sun, but because it has a dense atmosphere of mainly carbon dioxide. This produces a Super-Greenhouse-Effect! (d)(ii) The surface on Mars is much colder than Earth, not only because it is further away from the Sun, but because it has very little atmosphere even though its mainly carbon dioxide. This means there is little of the so-called 'Greenhouse-Effect', i.e. little trapping of re-radiated infrared heat radiation from the surface of Mars. ks4 science modular courses examinations gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision * ks4 science examinations-gcse-igcse chemistry revision * SITE PURPOSE EDUCATION - online learning or 'self-private-tuition' using revision notes, quizzes, practice tests involving GCSE Science CHEMISTRY in the areas of REVISING only the CHEMISTRY-Earth Science-Radioactivity at Doc Brown's Chemistry Clinic via HOMEPAGE in secondary school/schools, 6th form college/colleges, academy/academies or home self-study. Hopefully it will encourage interest and understanding of Chemistry, Earth Science and Radioactivity in any country of the world, though the site is written entirely in English. The website is designed to help and unofficially support students/teachers revise-learn/teach the chemistry for modular or co-ordinated examination science courses from UK QCA based AQA, OCR (Oxford and Cambridge) Twenty First (21st) Century and Gateway Science, Edexcel 360Science , Nuffield, Salters, Cambridge International (CIE), London International, WJEC, CCEA exams etc. Also, national award assessments-examinations for GCSE-IGCSE-KS4-O level-BTEC-NVQ applied, additional and chemistry national science courses. Also covers, mainly via quizzes the UK National KS3 SATs Science-biology/chemistry/physics (SAT revision levels 3-5 or 5-7) and covers much of the revising, learning and teaching chemistry examinations for the national curriculum for secondary schools and colleges. The site does not support the content of England, Wales or Northern Ireland primary science KS1 or KS2. The notes should also provide some background theory for a coursework assignment or project. BUT please note that my on-line revision notes and quizzes are no substitute for good classroom teaching-lecturing and thorough studying of your own notes and textbooks, practicing past papers and a copy of the syllabus which are readily downloaded from the examination board sites, but I hope here and there they will lend a tutoring hand on some topic, unit, module etc. For final revision you have to be intellectually honest about what you don't know or follow, YOU have to take the stuff to pieces, analyse what you do/do not understand and reconstruct it so it all makes sense in the end. There is no other way, there are no magic secrets on how to revise and learn, its mainly down to hard work and just good old fashioned study and employing teach-yourself strategies without the need for extra tutors and tutoring lessons. I also think there is too much hit and miss revision using past papers (which I do NOT supply) and not enough systematic revision. I also hope it will help teachers in planning lessons and developing schemes of work for science-chemistry. There are no lesson plans on the site but there are plenty of quizzes to incorporate into classroom activities whether photocopied or on electronic whiteboard projector for use as self-tuition-assessment purposes and a variety of teaching and learning styles and the images may be used in Microsoft Word documents and powerpoint projections. The site seems to be used by a large number of home study tutors, particularly the revision notes. An individual tutor may print out the notes for science-chemistry learning teaching-tuition purposes and for background material for assignments and projects. I have no interest or time in producing WORD.doc or xxxx.pdf files of the notes at the moment. Neither have I time to write up many practical laboratory experiments ('lab'-'labs') at the moment, but the notes contain lots of background information of chemical reactions in terms of observations-balanced equations-reactants-products-theory etc. I also find it difficult to recommend specific exam websites or syllabus textbooks, it depends exactly on what you need, what you have time for, and there are so many of them to choose from and I do not supply past examination papers for classes. The sites resources include revision notes, quizzes and worksheets which provide support for home study or tuition for homework and coursework help e.g. science investigations for any of the key stage courses indicated, but I do not supply lesson plans. Dr W P Brown gcse 19-11-2007 * ks4 science examinations gcse-igcse chemistry revision * ks4 science examinations-gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision * ks4 science modular courses examinations-gcse-igcse chemistry revision
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docbgeochangesans updated Jan 19th 2008 |