Module 5: Newtonian World and Astrophysics Flashcards

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1
Q

What are energy levels?

A

The name of the discrete set of energies that electrons of atoms in a gas can exist in

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2
Q

Why are the energy level of gaseous atoms negative?

A

Energy is required to remove an electron.

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3
Q

What does if mean is an electron has an energy of zero?

A

It’s free from the atom.

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4
Q

What is the ground state (Energy levels)?

A

Most negative energy level.

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5
Q

What does it mean when an electron has been “excited”?

A

It has moved from a lower energy level to a higher energy level.

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6
Q

What happens if a photon doesn’t have enough energy to free an electron?

A

If it has just enough energy to move it up an energy level, it excites the electron. This energy is the difference in energy between the two energy levels.

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7
Q

What happens once electrons have been excited?

A

They go back down to the lowest energy level they can and emit a photon, and when this light is diffracted, you get an emission line spectrum.

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8
Q

What is a spectrum?

A

A graph of intensity vs frequency.

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9
Q

What is a line spectrum?

A

A series of lines against a background formed by the diffraction of light emitted from excited electrons.

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10
Q

What are the three types of spectra?

A

Continuous spectra: The diffraction of white light produces this spectrum.

Emission line spectra: The result of the diffraction of photons emitted when electrons move to lower energy levels, the colourful lines indicate different energies and are against a dark background.

Absorption line spectra: Similar to emission line spectra but there are dark lines against a continuous spectra.

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11
Q

What are the similarities and differences between emission and absorption line spectra?

A

Similarity: Lines appear at the same frequencies / positions

Difference: Emission is coloured lines against a dark background, while absorption is dark lines against a coloured background

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