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How do we really know what's out there?

Discover how scientists use the electromagnetic spectrum and spectral analysis to determine the composition of stars, and learn about the Doppler Effect and redshift, which reveal that the universe is expanding.

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How do we really know what's out there?

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  1. How do we really know what's out there? Space is a pretty big place and, after all, we've never been farther from earth than our moon. How do we know what the stars are made of?

  2. This is the electromagnetic spectrum. It consists of waves which vary in length from very long (radio waves) to incredibly short (gamma rays). A special part of the spectrum consists of waves that we can see. This is called the visible spectrum. We see different wavelengths as different colors ranging from red (long wavelengths) to blue/violet (short wave- lengths).

  3. Doppler Effect The only way to measure motions of objects in the Universe

  4. Resting sound source Frequency fs V=340m/s Frequency fo source at rest observer at rest

  5. Sound source moving toward observer Observer hears increased pitch (shorter wave length) Frequency fo Frequency fs source observer at rest

  6. Sound source moving away from observer Observer hears decreased pitch (longer wave length) Frequency fo Frequency fs observer at rest source

  7. The size of the spectral shift is proportional only to the velocity directly away from the observer • This is redshift velocity is called radial motion

  8. White light consists of all visible wavelengths together. When white light passes through a prism, a triangular piece of glass or plastic, the different wavelengths are separated and can be seen individually. This is known as a SPECTRUM Discovered by Newton

  9. When any element is heated hot enough it begins to emit light. The pattern of wavelengths emitted by an element are like a fingerprint. Each element emits its own unique pattern. Above you can see the pattern of wavelengths emitted by the element hydrogen. Whenever this pattern is seen in the light coming from a star it means that hydrogen is present on that star. This is called the emission spectrum of hydrogen.

  10. So by using a spectroscope scientists can analyze all the wavelengths that are emitted by a star and can tell exactly what the star is made of even though it may be thousands of light years away. calcium uranium oxygen

  11. Remember, the greater the amount of shift, the faster the star is moving! Helium Helium slightly red shifted. Moving away. Helium more red shifted. Moving away even faster!

  12. Spectra of galaxies, starting in 1910, shows that the light is always red shifted. What does that mean? It means that everything is moving away from us! How can everything be moving away from us? The only explanation for that is ............................................. THE UNIVERSE IS EXPANDING!

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