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Chapter 5 Light and Matter

Chapter 5 Light and Matter. Astronomy 2014. Light: Radiative Energy. Light is a form of energy Energy and Power Energy is measured in the unit joules (J) Energy of light: “rate at which light carries energy in a direction”

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Chapter 5 Light and Matter

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  1. Chapter 5Light and Matter Astronomy 2014

  2. Light: Radiative Energy • Light is a form of energy • Energy and Power • Energy is measured in the unit joules (J) • Energy of light: • “rate at which light carries energy in a direction” • Rate of energy flow is a measurement of power, measured in the unit watt • 1 watt = energy flow of 1 joule / second

  3. Example Question: How many joules of energy are used by a 70 watt light bulb in a lamp over a minute time period? 1 watt = 1 joule/second >>> 70 watts = 70 joules/second 60 seconds per minute >>> 70 joules/second x 60 seconds = 4200 J used in 1 minute

  4. Light and Color • The various forms of light occur across a spectrum • Colors are the small area of the spectrum that can be seen by the human eye: Visible Spectrum

  5. Light, Color, and Our Sight: Why do we see a basketball as orange? A) The basketball absorbs orange light. B) The basketball emits orange light. C) The basketball transmits orange light. D) The basketball reflects orange light.

  6. Properties of Light • Light is both particles and waves • Photons are mass-less particles of light • Light is an electromagnetic wave • Light travels via vibrations of particles in the electric and magnetic fields • Waves of light carry energy, not matter • All light travels through empty space at the same speed • Speed of light (c) = ~300,000 km/second • Speed of a certain bullet = 0.9 km/second

  7. Properties of Light, cont. • The speed of any wave is determined by the wavelength times the frequency • hWavelength = iFrequency • iWavelength = hFrequency

  8. Page 143 in textbook

  9. Properties of Matter • Light carries information about matter • We must understand the properties of matter in order to interpret the messages sent in light from these objects

  10. Structure of Matter, cont. • Matter is made up of atoms • Atoms are made of protons, neutrons, and electrons • An element is the most basic unit of pure matter • Same atoms of a specific atomic number

  11. Structure of an Atom Page 145 in Textbook

  12. Properties of Matter, cont. Atomic Terminology • Atomic Number Number of Protons (# of positively charged particles) • Atomic Mass Number of Protons + Neutrons (# of total particles) • Isotope Variant of an element with the same number of protons but a different number of neutrons

  13. Phases of Matter • Matter exists in solids, liquids, and gases. • Phase of a substance determined by • Substance’s physical properties (melting point, freezing point) • Conditions of the environment (temperature) • Example: • The planet Jupiter is made of various elements including hydrogen and helium. • The nature of Jupiter’s environment is determined by • physical properties of these elements • temperature of the planet’s atmosphere.

  14. How do Atoms Store Energy? • Atoms possess energy in three components: • Mass-Energy in amount of mc2 • Kinetic Energy determined by their motion • Electrical Potential Energy: dependent on the arrangement of electrons around the atomic nuclei • Electrical Potential Energy is stored within the energy levels occupied by an atom’s electrons • This energy is released as electrons move within these energy levels.

  15. How do Atoms Store Energy, cont. Energy levels for an electron of a H atom, Page 149 in Textbook

  16. Learning from Light: Spectroscopy • Spectroscopy is the process of obtaining a spectrum and interpreting the information it contains. • A spectrum for studying an astrological object is usually a graph that plots each wavelength

  17. Continuous Spectrum Continuous Spectrum: A spectrum of light that spans a broad range of wavelengths without interruption by emission or absorption lines.

  18. Emission Line Spectrum Emission Line Spectrum: A spectrum that contains emission lines (includes specific bands from a source emitting light at different, varied wavelengths)

  19. Emission Line Spectrum, cont. Emission Line Spectra can be thought of as “fingerprints” • Each element has a unique band presence • Analysis can reveal what elements an astrological body is composed of

  20. Emission Line Spectrum, cont. Emission Line Spectrum showing the chemical composition of our Sun

  21. Absorption Line Spectrum Absorption Line Spectrum: A spectrum that contains absorption lines (includes bands showing where specific wavelengths of light are being excluded from an otherwise continuous spectrum)

  22. Thermal Radiation • Thermal Radiation is the spectrum of energy radiation produced by an object based on temperature • Wavelengths can span the ultraviolet to infrared spectra • Two Laws of Thermal Radiation • Law 1: Stefan-Boltzmann Law Each square meter of a hotter object’s surface emits more light at all wavelengths • Law 2: Wien’s Law Hotter objects emit photons with a higher average energy, and therefore a shorter average wavelength

  23. Thermal Radiation, cont.

  24. Thermal Radiation of Living Things: From the previous graph, we see that a human emits wavelengths in the infrared. Why is it then that a human does not glow in the dark? A) Humans do not emit any kind of light. B) Humans only emit light that is outsight of the visible spectrum and therefore is invisible to us. C) Humans emit quantities of light too small for us to see. D) Humans do not contain enough radioactive material to produce thermal radiation.

  25. The Doppler Effect • Doppler Effect: Effect that shifts the wavelengths of objects that are moving toward or away from the observer • Movement distorts waves • For example, the shifting sound heard as a horn sounds on a car moving past a stationary person • This change is also observed in waves of light

  26. The Doppler Effect: Shift Blueshift • BLUESHIFT - Object moving toward an observer • Light waves bunch up between the object and observer • Gives the appearance of shorter wavelengths • Shorter wavelengths are bluer • REDSHIFT - Object moving away from an observer • Light waves stretch out between the object and the observer • Gives the appearance of longer wavelengths • Longer wavelengths are redder Redshift

  27. The Doppler Effect, cont.

  28. Measuring the Effects of the Doppler Shift

  29. Chapter 5 Key Vocabulary 16. Electron 17. Atomic Number 18. Atomic Mass 19. Isotope 20. Electrical Potential Energy 21. Spectroscopy 22. Thermal Radiation 23. Doppler Effect 24. Blueshift 25. Redshift 1. Power 2. Watts 3. Continuous Spectrum 4. Emission Line Spectrum 5. Absorption Line Spectrum 6. Wavelength 7. Frequency 8. Electromagnetic Wave 9. Electromagnetic Spectrum 10. Speed of Light 11. Photons 11. Visible Light 12. Infrared 13. Atom 14. Proton 15. Neutron

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