Matter, Light, and Energy Flashcards

1
Q

Explain Rutherford experiment

A

Shot positive alpha particles at gold foil and noted how occasionally they bounced backwards. Discovered most of atom was empty and dense positive core(nucleus)

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2
Q

What does number of protons in atom determine?

A

Which element it is

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3
Q

What did Planck and Einstein show about electrons in atoms?

A

Can only occupy at specific energies i.e energies are quantized

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4
Q

What happens if you add enough energy to electron?

A

It leaves atom altogether and atom is ionised. Ion left with net positive charge

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5
Q

What happens if electron with low enough energy wanders by ion?

A

Can be captured and become neutral again. Called recombining

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6
Q

What happens when an electron moves from higher level to lower level?

A

Loses energy and releases photon

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7
Q

Range of visible wavelengths

A

4x10^-7 m (violet) to 8x10^-7m (red)

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8
Q

What is the photoelectric effect?

A

Light can knock out electrons evidence for being a particle

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9
Q

What is luminosity?

A

•energy per second emitted in photons
•intrinsic property of the object

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10
Q

What is Flux?

A

•energy in photons passing through a given area per second
•measurable (apparent) property

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11
Q

What is a spectrum?

A

The flux of photons at each wavelength

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12
Q

What most matter be to thermalise photons and atoms?

A

Opaque

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13
Q

What is a black body spectrum?

A

The spectrum arising from thermal emission.
Peak wavelength scales inversely with temperature

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14
Q

Explain emission spectra

A

Photon energies correspond to difference in energy levels for that particular atom. Hence photons emitted at specific wavelengths for each atom

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15
Q

Explain absorption spectrum

A

Photon of precisely right energy hits electron, electron jumps to higher level swallowing photon and photon then missing from light

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16
Q

When do things emit vs absorb?

A

Dependent on object temperature.
•when hot electrons excited and smash into each other emit light
•when cold fall into lower energy states ready to absorb light

17
Q

What are Fraunhofer lines?

A

Resulting absorption lines of sun due to atoms in cooler photosphere absorbing black body light generated in hot interior