5.4 Learning from Light Our goals for learning

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Presentation transcript:

5.4 Learning from Light Our goals for learning What are the three basic types of spectra? How is energy stored in an atom? How does light tell us what things are made of?

How do astronomers study light? Astronomers use a spectrograph – an instrument that separates light by wavelength and records the spectrum Uses a prism or diffraction grating

What are the three basic types of spectra? Continuous Spectrum Emission Line Spectrum Absorption Line Spectrum Spectra of astrophysical objects are usually combinations of these three basic types

Continuous Spectrum An unbroken band of colors produced by glowing solids, liquids & high pressure gases. Ex: The spectrum of a common (incandescent) light bulb spans all visible wavelengths, without interruption

Emission Line Spectrum Produced by hot gases under low pressure. EX: A thin or low-density cloud of gas emits light only at specific wavelengths that depend on its composition and temperature, producing a spectrum with bright emission lines

Absorption Line Spectrum Produced when a continuous spectrum of light is passed through a cooler, low pressure gas. EX: A cloud of gas between us and a light bulb can absorb light of specific wavelengths, leaving dark absorption lines in the spectrum

Stellar Spectra

How does light tell us what things are made of? Spectrum of the Sun

Sun’s Spectrum hydrogen sodium magnesium what is in the Sun? iron

Remember, energy stored in atoms Electrons are restricted to particular energy levels The lowest level is called the ground state Higher levels are called excited states

The energy is measured in electron-Volts. 1 eV = 1.6 x 10 – 19 J Excited States Ground State The energy is measured in electron-Volts. 1 eV = 1.6 x 10 – 19 J

The only allowed changes in energy are those corresponding to a transition between energy levels Not Allowed Allowed

Excited States Ground State Electrons gain energy (by absorbing light) and jump to a higher level Electrons lose energy ( by emitting light) and drop to a lower level

Chemical Fingerprints Each type of atom has a unique set of energy levels Each transition corresponds to a unique photon energy, frequency, and wavelength Energy levels of Hydrogen

Chemical Fingerprints Downward transitions produce a unique pattern of emission lines

Chemical Fingerprints Because those atoms can absorb photons with those same energies, upward transitions produce a pattern of absorption lines at the same wavelengths

Chemical Fingerprints Each type of atom has a unique spectral fingerprint Observing the fingerprints in a spectrum tells us which kinds of atoms are present

Energy Levels of Molecules Molecules have additional energy levels because they can vibrate and rotate

Energy Levels of Molecules Spectrum of Molecular Hydrogen The large numbers of vibrational and rotational energy levels can make the spectra of molecules very complicated Many of these molecular transitions are in the infrared part of the spectrum

Video – How do we know what the air on other planets is made of?

What have we learned? What are the three basic type of spectra? Continuous spectrum, emission line spectrum, absorption line spectrum How does light tell us what things are made of? Each atom has a unique fingerprint. We can determine which atoms something is made of by looking for their fingerprints in the spectrum.