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Living Under the Sun: Challenges

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Page 1: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Living Under the Sun: Challenges

Page 2: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Interactions of light and matter

Emission TransmissionAbsorption Reflection or Scattering

Page 3: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Light is an electromagnetic wave*.

Page 4: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Wave Characteristics

Frequency (ν): number of waves that pass a point in a given period of timeTotal energy is proportional to amplitude and frequency of waves. Because speed of light (c) is a constant (3 x 108 m/s),wavelength and frequency of electromagnetic waves are inversely proportional: E = hν; c = νλ

Page 5: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

White light is composed of all colors which can be separated into a rainbow, or a

spectrum, by passing the light through a prism.

Each color light has a different wavelength, and, therefore, frequency.

Color

Page 6: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

6

Amplitude & Wavelength

Page 7: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Are there other “Colors”?

Page 8: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

The Electromagnetic Spectrum• Visible light comprises only a small fraction of all the

wavelengths of light – called the electromagnetic spectrum.

• Short wavelength (high frequency) light has high energy.

- Gamma ray light has the highest energy.

• Long wavelength (low frequency) light has low energy. - Radiowave light has the lowest energy.

Page 9: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Electromagnetic Spectrum

Page 10: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Each chemical element produces its own unique set of spectral lines.

Oxygen spectrum

Neon spectrum

Page 11: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Emission and absorption spectraare inversely related.

Spectra of Mercury

Page 12: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

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Light can induce electron transitions.

• To transition to a higher energy state, the electron must absorb energy equal to the energy difference between the final and initial states.

• Electrons in high energy states are unstable. They will transition to lower energy states and emit light.

Page 13: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Light induces electron transitions in molecules.

O O······ ··

absorbs UV light “colorless”

Visible light does not have enough energy to move electrons to next energy

level.

absorbs visible light“colored”

Energy levels are closer in “conjugated” system. Visible light is energetic enough to

induce transition!

Page 14: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Light induces other transitions in molecules.

Energy can also be absorbed and emitted in other “modes” including vibration and

rotation.

OH

Page 15: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Light can induce photochemical reactions.

• Photolysis O2(g) 2 O(g)

O3(g) O2(g) + O(g)

• Conformational change

Page 16: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Visible

Greenhouse gases!

Ozone!

Page 17: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Sunburn, vitamin D

Page 18: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

UV Absorbing Molecules

Skin Pigments – absorb and dissipate energy

http://www.clinuvel.com/

Page 19: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

How about those beads?Photochromic Pigments!

Higher energy formLower energy form

Page 20: Living Under the Sun: Challenges. Interactions of light and matter EmissionTransmission AbsorptionReflection or Scattering

Sunscreen Ingredients

Homosalate Octyl methoxycinnamate

Inorganic compounds, e.g. ZnO and TiO2, reflect or scatter light.

Organic compounds absorb light and dissipate energy as heat.