Atomic Theory
Structure of the Atom
Isotopes
Light
Electrons & Spectroscopy
100

Q: This scientist created the first modern atomic theory in the early 1800s.

A: John Dalton

100

Q: This subatomic particle carries a positive charge.

A: Proton

100

Q: Isotopes of the same element differ in the number of these particles.

A: Neutrons

100

Q: This color of visible light has the highest energy.

A: Violet

100

Q: When an electron falls from a higher to a lower energy level, it does this.

A: Releases a photon of light (emits energy)

200

Q: He discovered the electron using cathode ray tubes.

A: J.J. Thomson

200

Q: The number of protons in an atom is called this.

A: Atomic number

200

Q. What does it mean when we ask for % abundance?

A. % abundance tells you what percentage of all atoms of an element are a particular isotope

200

Q: What happens to the wavelength when the frequency of light increases?

A: It decreases (inverse relationship).

200

Q: Spectral lines differ between elements because of what?

A: Unique electron energy levels

300

Q: This model of the atom incorrectly described electrons as scattered in a positively charged sphere.

A: The Plum Pudding Model

300

Q: This value equals the total number of protons and neutrons in an atom.

A: Mass number

300

Q: Why is the atomic mass on the periodic table rarely a whole number?

A: It is a weighted average of all naturally occurring isotopes.

300

Q: If red light has a longer wavelength than blue light, which one has greater frequency and energy?

A: Blue light (shorter wavelength → higher frequency and energy)

300

Q: When white light is viewed through a spectroscope, it produces a continuous spectrum. Explain what a continuous spectrum looks like and why it forms.

A: A continuous spectrum shows an unbroken “rainbow” of all visible wavelengths. It forms because white light contains all wavelengths, and no electrons are absorbing or emitting specific energies to create lines.

400

Q: He concluded that atoms are mostly empty space with a dense, positively charged nucleus.

A: Ernest Rutherford

400

Q: How do you calculate the number of neutrons in an atom?

A: Subtract the atomic number from the mass number (Neutrons = Mass number – Atomic number)

400

Q: Chlorine has two main isotopes: Cl-35 and Cl-37. Explain why the atomic mass on the periodic table is closer to 35 than to 37.

A: Because Cl-35 is more abundant, so it contributes more to the weighted average atomic mass.

400

Q. In the equation c = λv what do each of the variables represent and what are their units?

c — Speed of Light

  • What it represents: The speed of light in a vacuum

  • Units: meters per second (m/s)

  • Value: 3.00×108 m/s3.00×108m/s

λ — Wavelength

  • What it represents: The distance between two consecutive crests (or troughs) of a wave

  • Units: meters (m)

    • Can also be written in nanometers (nm), micrometers (μm), etc.

v — Frequency

  • What it represents: The number of wave cycles that pass a point per second

  • Units: Hertz (Hz)

    • Equivalent to 1/s or s⁻¹

400

Q: What is the difference between an absorption spectrum and an emission spectrum?

A:

  • Absorption spectrum: dark lines appear where light is absorbed.

  • Emission spectrum: bright lines appear where light is emitted.

500

Q: This scientist discovered the neutron, explaining why isotopes differ in mass.

A: James Chadwick

500

Q: Copper has atomic number 29 and mass number of 63.546. How many protons, neutrons, and electrons does Cu²⁺ have?

  • Protons: 29

  • Neutrons: ≈ 35 (63.546 ≈ 64 → 64 – 29 = 35)

  • Electrons: 27 (Cu²⁺ has lost 2 electrons)

500

Q: An element has two isotopes:
• 70% with mass 35
• 30% with mass 37
Calculate the weighted average atomic mass.

A: (0.70)(35) + (0.30)(37) = 24.5 + 11.1 = 35.6 amu

500

Q: A green photon has a wavelength of 5.20×10⁻⁷ m. Calculate its frequency.

A.
c = λv
ν=(3.00×10^8 / 5.20×10^−7) ≈ 5.77×10^14 Hz

500

Q: Describe the full process that creates an emission spectrum (5 steps)

A:
Electrons absorb energy → jump to excited state → fall back to lower energy levels → release photons of specific wavelengths → spectral lines appear.

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