Uplearn electromagnetic radiation from stars

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17 Terms

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Quantised

energy levels exist in discrete values

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Why are energy levels in an atom negative?

The electrons bound to the atom must gain energy in order to move up to a higher energy level or escape the atom, therefore we write that they have negative energy

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The electron has been excited

It has gained sufficient energy to move from one energy level to another that is at a higher energy

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electronvolt

The electronvolt is the amount of energy transferred to an electron when it is passed through a potential difference of one volt

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An electron undergoes de-excitation within an atom. What happens to the energy it loses?

It is released as a single photon

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Luminosity

total radiant power output of a star, measured in W

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Hertzsprung-Russell diagram

a graph of log ( L / Lsolar) on the y-axis and log(T) on the x-axis. The log(T) axis runs from high values on the left to low values on the right

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Electron energy level

a discrete energy that an electron in an atom is allowed to possess. Energy levels in atoms are negative

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Ground state

the lowest electron energy level of an atom

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The wavelengths of light emitted by an atom form a unique pattern called an:

  • Emission spectrum or emission spectra

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Which of the following is an emission spectrum?

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1)Which of the following might be produced by heated metal such as a filament lamp?

optionoptionoption

2)What is this type of spectrum called?

1) B

2)continuous spectrum

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1)Which of the following might be produced by continuous spectrum passing through a cool gas?

optionoptionoption

2)What is this type of spectrum called?

1)A

2)absorption spectrum or absorption spectra

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Absorption spectra are used to study stars. They can be used to:

Identify the elements within a star

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Emission spectrum

A set of electromagnetic frequencies produced by excited atoms and visible as bright lines in spectroscopy. Each atom has a characteristic emission spectrum that represents its unique set of energy levels

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Continuous spectrum

A spectrum containing all visible electromagnetic frequencies are present, for example produced by a lamp filament or other heated solid metals

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Absorption spectrum

A set of electromagnetic frequencies that are missing from an otherwise continuous spectrum and therefore show as dark lines on the spectrum. The missing frequencies have been absorbed and re-emitted in all directions by atoms or molecules present in between the source and detector. The absorbed frequencies correspond to the energy levels present in the absorbing atoms or molecules