3.5 Energy Levels and Spectra Flashcards

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1
Q

What is a rainbow

A

A natural display of the colours of the spectrum of sunlight

Raindrops split sunlight into a continuous spectrum of colours

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2
Q

What is the difference between using a tube of glowing gas as the light source instead of a filament lamp when looking at colour spectrums

A

We see a spectrum of discrete lines of different colours rather than a continuous spectrum

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3
Q

The wavelengths of the lines of a line spectrum of an element are characteristic of…

A

…the atoms of that element

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4
Q

How can we identify the element that produced the light from a line spectrum

A

By measuring the wavelengths

No other element produces the same pattern of light wavelengths

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5
Q

Why does every element produce a different pattern of light wavelengths

A

Because the energy levels of each type of atom are unique to that atom so photons emitted are characteristic of the atom.

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6
Q

What is each line in a line spectrum due to

A

Light of a certain colour and therefore a certain wavelength

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7
Q

The photons that produce each line all have the ______ energy, which is ______ from the energy of the photons that produce any other line.

A

Same

Different

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8
Q

Each photon is emitted when an atom de-excites due to…

A

… one of its electrons moving to an inner shell

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9
Q

If the electron moves from energy level E1 to a lower energy level E2, the energy of the emitted photon hf =

A

E1 - E2

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10
Q

What is the simplest type of atom

A

The hydrogen atom

One proton as its nucleus and one electron

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11
Q

General formula for the energy levels of the hydrogen atom relative to the ionisation level

A

E = - 13.6eV / n^2

Where n=1 for the ground state, n=2 for the next excited state etc.

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12
Q

When a hydrogen atom de-excites from energy level n1 to a lower energy level n2, the energy of the emitted photon is given by…

A

E = (1/n2^2 - 1/n1^2) * 13.6 eV

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13
Q

What does each energy level correspond to

A

The electron in a particular shell.

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14
Q

How was the energy level formula for hydrogen first deduced?

A

From the measurements of the wavelengths of the lines

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15
Q

Why are measurements of the wavelength of light important in branches of science such as astronomy and forensic science

A

They enable us to identify the chemical elements in the light source.

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16
Q

What was helium discovered from

A

The spectrum of sunlight
Pattern of lines in spectrum was observed at wavelengths that had never been observed from any known gas and were therefore due to presence of previously unknown element in the Sun.

17
Q

How is helium produced

A

As a result of the nuclear fusion of hydrogen nuclei in the Sun
Named after Greek word ‘Helios’ for Sun

18
Q

How is helium produced in the earth

A

As alpha particles from the radioactive decay of elements such as uranium.
Can be collected at oil wells and stored for use in fusion reactors, helium-neon lasers and for very low temperature devices.

19
Q

What happens to helium in liquid state below a temperature of 2.17K

A

Becomes a superfluid

20
Q

What is a superfluid

A

A fluid with no resistance to flow, which escapes from an open container by creeping - as a thin film - up and over the sides of the container