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OCR GCSE Physics

GCSE · OCRPhysics33 notes dans 9 dossiers, 187 KB

33 notes de révisions, créée par cookie, répartie en 9 sections qui suivent les thèmes du cours.

Notes for OCR GCSE Physics A (Gateway Science, J249), in folders for the specification's eight physics topics in its order (Matter to Global challenges), with the required practicals in the topics they belong to and a final folder on scientific thinking, error analysis, units and maths skills. Higher-tier content is marked where it sits. Delete any note your tier does not need once the notes are yours.

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Contenu

  • Matter
    • The atom and density6 KB
    • Changes of state and thermal energy6 KB
    • Gases, pressure and fluids7 KB
  • Forces
    • Motion6 KB
    • Forces and Newton's laws10 KB
    • Momentum, work done and power5 KB
    • Springs and elasticity5 KB
    • Gravity, weight and moments6 KB
  • Electricity
    • Static electricity and charge5 KB
    • Current, potential difference and resistance7 KB
    • Series and parallel circuits5 KB
    • Electrical power and energy transfer4 KB
  • Magnetism and magnetic fields
    • Magnets and magnetic fields6 KB
    • The motor effect and electric motors4 KB
    • Induction, generators and transformers6 KB
  • Waves in matter
    • Wave behaviour5 KB
    • Sound, ultrasound and waves inside materials5 KB
    • The electromagnetic spectrum5 KB
    • Reflection, refraction, lenses and colour7 KB
  • Radioactivity
    • Nuclei, isotopes and radiation6 KB
    • Decay equations and half-life5 KB
    • Uses and hazards of radiation5 KB
    • Nuclear fission and fusion4 KB
  • Energy
    • Energy stores, transfers and calculations6 KB
    • Power, efficiency and reducing energy waste6 KB
  • Global challenges
    • Physics on the move: stopping distances and road safety5 KB
    • Energy resources and their use5 KB
    • The National Grid and mains electricity5 KB
    • The Solar System and orbits4 KB
    • Red-shift, stars and the Big Bang6 KB
  • Working scientifically
    • Scientific thinking, models and risk5 KB
    • Planning investigations, error and analysing data8 KB
    • Quantities, units and maths skills8 KB

La première note

Matter / The atom and density

How the model of the atom changed

Scientists build models of the atom to explain the evidence they have, and change the model when new evidence does not fit. The order matters because each model was a response to an experiment the one before could not explain.

After the electron was discovered, J. J. Thomson proposed that an atom is a ball of positive charge with negatively charged electrons embedded in it, which is often called the plum pudding model. It explained why atoms are neutral overall, since the positive charge and the electrons balance.

Hans Geiger and Ernest Marsden, working with Ernest Rutherford, fired alpha particles (which are positively charged) at a very thin sheet of gold foil and detected where they went. Most passed straight through, a small number were deflected through large angles and a very few bounced almost straight back. The plum pudding model predicted only small deflections, so it could not explain this. Rutherford concluded that the positive charge and nearly all the mass are concentrated in a tiny nucleus at the centre, and that the rest of the atom is mostly empty space with electrons around it. A particle only bounces back if it meets something small, dense and positive, which repels it.

Niels Bohr then changed the model again to say that electrons orbit the nucleus at set distances, in fixed energy levels, rather than anywhere. This explained why atoms emit and absorb radiation only at particular frequencies, and it is the model most often drawn today. Later work showed that the nucleus itself contains positively charged protons and uncharged neutrons, the neutron being identified by James Chadwick.

Each new model came from different scientists testing and building on each other's results, and a model is accepted only when the results of experiments agree with it.

The structure of the atom

An atom has a positively charged nucleus surrounded by negatively charged electrons. The radius of the nucleus is many thousands of times smaller than the radius of the atom, but almost all of the mass of the atom is in the nucleus because electrons have very little mass.

ParticleRelative chargeRelative massPosition
Proton+11Nucleus
Neutron01Nucleus
Electron−1about 1/2000Around the nucleus

An atom has the same number of electrons as protons, so it has no overall charge. Atoms are typically about 1×10−10 m1 \times 10^{-10}\ \mathrm{m} across, and small molecules are of the same order of magnitude.

It is easy to mix up the words for particles. An atom is a single particle of an element. A molecule is two or more atoms joined together, as in water or oxygen. Protons, neutrons and electrons are subatomic particles, which are smaller than an atom and are what atoms are made of.

Density

The density of a material is its mass per unit volume. It says how tightly the mass is packed.

ρ=mV\rho = \frac{m}{V}

ρ\rho (the Greek letter rho) is the density in kilograms per cubic metre (kg/m³), mm is the mass in kilograms and VV is the volume in cubic metres. Densities are often given in g/cm³, and 1 g/cm3=1000 kg/m31\ \mathrm{g/cm^3} = 1000\ \mathrm{kg/m^3}. Volumes need converting with care, since 1 m3=1 000 000 cm31\ \mathrm{m^3} = 1\,000\,000\ \mathrm{cm^3}.

Worked example

A steel block measures 5.0 cm by 4.0 cm by 3.0 cm and has a mass of 0.472 kg. Find its density in kg/m³.

V=5.0×4.0×3.0=60 cm3=60÷1 000 000=6.0×10−5 m3ρ=0.4726.0×10−5=7900 kg/m3 (to 2 significant figures) \begin{aligned} V &= 5.0 \times 4.0 \times 3.0 = 60\ \mathrm{cm^3} \\ &= 60 \div 1\,000\,000 = 6.0 \times 10^{-5}\ \mathrm{m^3} \\ \rho &= \frac{0.472}{6.0 \times 10^{-5}} \\ &= 7900\ \mathrm{kg/m^3}\ \text{(to 2 significant figures)} \end{aligned}

The same equation rearranged gives m=ρVm = \rho V. A tank holding 0.25 m³ of water, which has a density of 1000 kg/m³, holds 1000×0.25=2501000 \times 0.25 = 250 kg of water.

Density and the states of matter

In a solid the particles are packed closely in a regular pattern and vibrate about fixed positions. In a liquid they are also close together but arranged irregularly and free to move past each other. In a gas they are far apart and move freely at random. Since the same mass of particles takes up much more space as a gas, gases have far lower densities than solids and liquids. Solids are usually a little denser than the same substance as a liquid, because the regular arrangement is usually slightly more compact. Water is a well-known exception, since ice is less dense than liquid water and floats.

Mass does not change when a substance changes state, because the same particles are still there. Only the volume changes, and so the density does. If 1.0 kg of water with a volume of 1.0×10−3 m31.0 \times 10^{-3}\ \mathrm{m^3} freezes and the volume increases by about 9%, the density falls from 1000 kg/m³ to about 917 kg/m³.

Practical: measuring density

The apparatus used depends on the object.

For a regular solid, measure the lengths with a ruler or, for a more precise value, a micrometer or vernier callipers, calculate the volume from them, and measure the mass on a balance. Divide the mass by the volume.

For an irregular solid that sinks, measure its mass on a balance. Find its volume by lowering it into a eureka can (a can with a spout, filled to the spout) and collecting the water that overflows in a measuring cylinder. The volume of the water displaced equals the volume of the object, which is the principle Archimedes used. Alternatively, lower it into a measuring cylinder part-filled with water and read the volume before and after. An object that floats can be pushed under with a thin, dense sinker of known volume.

For a liquid, place a measuring cylinder on a balance and set the balance to zero, then pour in a volume of the liquid and read both the volume and the mass. The reading of volume is taken with the eye level with the bottom of the curved surface (the meniscus).

Repeating the measurement and finding a mean reduces the effect of random errors. Air bubbles stuck to an object, water left on it, and reading the scale from an angle all cause errors in the volume.

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