Physics Flashcards: Waves and Wavelengths
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Questions and Answers

What is wavelength?

The separation of peaks in a wave, typically represented by the symbol λ (lambda).

What is the speed of a wave?

The speed at which its wave peaks move.

What is frequency?

The rate at which wave peaks pass a point in space, measured in Hertz (Hz).

What formula describes the relation between wavelength, speed, and frequency?

<p>Wavelength x frequency = speed, or λ ν = c.</p> Signup and view all the answers

What are the properties of electrons, protons, and neutrons?

<p>Electrons have a mass of $9 x 10^{-28}$ gm and a negative charge; protons have a mass of $2 x 10^{-24}$ gm and a positive charge; neutrons have a mass of $2 x 10^{-24}$ gm and no charge.</p> Signup and view all the answers

Explain electric fields.

<p>Electric charges are surrounded by electric fields that extend to infinite distances and can exert forces on other charged particles.</p> Signup and view all the answers

What is the link between light and vibrating electric fields?

<p>Light is a vibrating electric field that causes electrons in the retina to vibrate, which is perceived as light.</p> Signup and view all the answers

What is the electromagnetic spectrum?

<p>The range of all types of light, from radio waves to gamma rays, most of which are invisible to the human eye.</p> Signup and view all the answers

Explain the transmission of light through the Earth's atmosphere.

<p>Electromagnetic radiation is reflected or absorbed by atmospheric gases, but visible light largely passes through.</p> Signup and view all the answers

Describe the structure of atoms.

<p>Atoms consist of a nucleus made of protons and neutrons, with electrons whirling around the nucleus.</p> Signup and view all the answers

How many protons and neutrons are in hydrogen, helium, and carbon?

<p>Hydrogen has 1 proton and no neutrons; helium has 2 protons and 2 neutrons; carbon has 6 protons and 6 neutrons.</p> Signup and view all the answers

How many protons and neutrons are in nitrogen, oxygen, iron, and uranium?

<p>Nitrogen has 7 protons and 7 neutrons; oxygen has 8 protons and 8 neutrons; iron has 26 protons and 30 neutrons; uranium has 92 protons and 146 neutrons.</p> Signup and view all the answers

What is Kirchhoff's First Law?

<p>A hot solid, liquid, or opaque gas emits light at all wavelengths, forming a continuous spectrum.</p> Signup and view all the answers

What is a spectrum?

<p>A plot of the amount of light emitted at each wavelength, with intensity or flux typically on the vertical axis.</p> Signup and view all the answers

What does the equation E = hν represent?

<p>It shows that the energy of a photon is proportional to its frequency, where h is Planck's constant.</p> Signup and view all the answers

What occurs during the emission and absorption of photons by electrons?

<p>When an electron jumps from a higher to a lower energy level, it emits a photon that carries the energy difference.</p> Signup and view all the answers

What does temperature measure?

<p>Temperature measures how fast the atoms and molecules are moving.</p> Signup and view all the answers

What are Kirchhoff's three laws?

<ol> <li>A hot solid, liquid, or gas gives off a continuous spectrum. 2. A hot, rarefied gas emits light at discrete wavelengths. 3. Light with a continuous spectrum passing through a cool gas produces an absorption line spectrum.</li> </ol> Signup and view all the answers

What are the properties of black body radiation?

<p>Hot objects emit more energy than cool objects and have a continuous spectrum with a single broad maximum.</p> Signup and view all the answers

What is the equation for the luminosity of an object emitting black body radiation?

<p>L = area × T⁴, where L is luminosity and T is temperature.</p> Signup and view all the answers

Describe the Hertzsprung-Russell (H-R) Diagram.

<p>The H-R diagram plots star temperature against luminosity, with higher temperatures on the left and lower temperatures on the right.</p> Signup and view all the answers

How can you interpret the H-R diagram?

<p>Stars are clustered in groups; main groups include Main Sequence, White Dwarfs, Red Giants, and Supergiants.</p> Signup and view all the answers

How is density defined?

<p>Density is defined as mass divided by volume.</p> Signup and view all the answers

How can you find the volume of a sphere?

<p>V = (4/3) π R³.</p> Signup and view all the answers

Name three ways in which star temperatures can be measured.

<p>From their spectral type, color, and the wavelength of the peak in their continuous spectra.</p> Signup and view all the answers

How can you identify chemical elements in stars?

<p>By analyzing the unique pattern of emission and absorption lines of each element.</p> Signup and view all the answers

Study Notes

Wavelength

  • Defined as the distance between wave peaks, symbolized by λ (lambda).
  • Commonly measured in Ångstroms for light, with wavelengths corresponding to color.

Speed (of Waves)

  • The velocity at which wave peaks travel.

Frequency

  • Describes how often wave peaks pass a designated point, measured in Hertz (Hz) or cycles per second.
  • Represented by symbols f or ν (nu).

Relationship Between Wavelength, Speed, and Frequency

  • Expressed by the equation: Wavelength × Frequency = Speed (λν = c).

Properties of Fundamental Particles

  • Electrons: Mass = 9 x 10⁻²⁸ grams, negative charge.
  • Protons: Mass = 2 x 10⁻²⁴ grams, positive charge.
  • Neutrons: Mass similar to protons (2 x 10⁻²⁴ grams), no charge.
  • Protons and neutrons are approximately 2000 times heavier than electrons.

Electric Fields

  • Surround electric charges, exerting forces on other charges; oppositely charged particles attract, like charges repel.

Light & Vibrating Electric Fields

  • Light is a form of electromagnetic radiation created by vibrating electric fields, which induce vibrations in electrons in the retina, perceived as light.

Electromagnetic Spectrum

  • Encompasses all types of light from radio waves to gamma rays; visible light ranges from 4000 Å to 7000 Å.

Transmission of Light Through Earth's Atmosphere

  • Visible light generally passes through the atmosphere, while other wavelengths can be absorbed or reflected by gases like water vapor and carbon dioxide.

Structure of Atoms

  • Atoms consist of a nucleus with protons and neutrons, surrounded by fast-moving electrons in defined energy levels.

Atomic Composition of Common Elements

  • Hydrogen: 1 proton, 0 neutrons.
  • Helium: 2 protons, 2 neutrons.
  • Carbon: 6 protons, 6 neutrons.
  • Nitrogen: 7 protons, 7 neutrons.
  • Oxygen: 8 protons, 8 neutrons.
  • Iron: 26 protons, 30 neutrons.
  • Uranium: 92 protons, 146 neutrons.

Kirchhoff's Laws

  • First Law: Continuous spectrum emitted by hot solids, liquids, or gases.
  • Second Law: Rarefied hot gas emits light at specific wavelengths (emission line spectrum).
  • Third Law: Light passing through cool gas produces absorption line spectrum.

Spectrum

  • Graph plotting light intensity versus wavelength, typically measured in Ångstroms.

Einstein's Equation (E = hν)

  • Established light's quantized nature, leading to quantum mechanics; h is Planck's constant (6.6 x 10⁻²⁷).

Photon Emission & Absorption

  • Transition of an electron between energy levels involves emission or absorption of a photon, with frequency and wavelength determined by energy differences.

Temperature & Kelvin Scale

  • Temperature reflects atomic and molecular movement rates; Kelvin = Celsius + 273.

Black Body Radiation

  • Hot objects emit more energy; emission spectrum has a broad maximum influenced by temperature. Key equations include:
    • Luminosity (L) = Area × T⁴
    • Peak wavelength (λmax) = 2.9 × 10⁷/T.

Hertzsprung-Russell (H-R) Diagram

  • Plots stars based on temperature (backwards axis) and luminosity (vertical axis in Solar Luminosities); clusters indicate different star types.

Star Temperature Measurement

  • Determined via spectral type, color, or wavelength of peak emission.

Chemical Element Identification in Stars

  • Unique patterns of emission/absorption lines allow element identification; each element has characteristic wavelengths due to differing atomic energy levels.

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Study essential concepts of waves with these flashcards covering definitions and key terms like wavelength and wave speed. Perfect for reinforcing your understanding of physical phenomena related to light and sound. Ideal for students preparing for exams in physics.

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