1. Energy Energy is a property that enables something to do work
Energy has various forms (kinetic, potential, rest energy)
Kinetic energy is the energy of a moving object
mv2
KE = 2
It takes ~1000 N (or ~ 225 lbs) to hit a nail and drive it 5 mm into a surface.
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2. Potential Energy Potential energy is a capacity of doing some work
Potential energy is the energy of position
Gravitational Potential Energy
W = Fd = mgh = PE (potential energy)
PE of a 1000-kg car at the top of a 50-m multilevel parking lot is:
mgh= (1000 kg)(9.8 m/s2)(50 m)=490 kJ
PE is relative!

3. Rest Energy
Mass and Energy are related to each other and can be converted into each other.
The rest energy of a body is the energy equivalent of its mass.
E0 = m0c2
E0 (m=1 kg) = 1 kg x (3 108)2 (cm/s)2 ~ 1017 J
PE (m=1 kg, h=9 km) = mgh = 1 kg x 9.8 m/s2 x 9000 m ~ 105 J

4. Energy Transformations
Many mechanical processes involve interchanges between KE, PE, and work.
Energy exists in some other forms: chemical energy, heat energy, radiant energy, etc.

5. Conservation of Energy
Energy cannot be created or destroyed.
It can only be changed from one form to another.
The above statement is called the law of conservation of energy

6. Light and Atomic Structure
Chapter 5
Light and Atomic Structure
Light and its properties
Atomic structure
Interaction between Light and Matter
Spectrum

7. Light in Everyday Life Light is a form of energy, radiative energy
1 Watt = 1 Joule/sec
Light has color
A prism split light into a spectrum (rainbow of colors)
Light travels with a speed of c = 300,000 km/s

8. Rainbow

9. Interaction of Light and Matter
Emission
Absorption
Transmission (passing through)
Reflection (scattering)

10. Properties of Light light demo
Light behaves as both a particle and a wave
Light particles are called photons, which can be counted individually.
Light is also an electromagnetic wave
The wavelength is the distance between adjacent peaks of the electric or magnetic field
1 nm (nanometer) = 10–9 m μm (micron) = 10–6 m
The frequency is the number of peaks that pass by any point each second, measured in cycles per second or Hertz (Hz).
light demo

11. Light is an electromagnetic wave
Light consists of many individual photons.
Each travels at the speed c and can be characterized by a wavelength and a frequency.

12. Many Forms of Light
The spectrum of light is called the electromagnetic spectrum
Different portions of the spectrum are called:
The visible light - what we see with our eyes
The infrared light - beyond of the red end of rainbow
The ultraviolet light - beyond the blue end
Radio waves - light with the longest wavelengths
X rays - wavelengths shorter than ultraviolet
Gamma rays - the shortest wavelength light

13. Electromagnetic spectrum

14. Electromagnetic spectrum
Frequency units – Hertz
1 Hz = 1 c1

15. Light and Matter The amount of light is called intensity
Studying spectra of celestial bodies one can learn a wealth of information about them

16. Atomic Structure
92 chemical elements have been identified in the Universe.
Nearly 20 more have been created artificially.
Each chemical element is made from a different type of atom.
Atoms are made from particles called protons, neutrons, and electrons.
Protons and neutrons form the nucleus in the center of the atom.
Electrons surround the nucleus.

17. Atomic Structure
Positively charged protons are hold together by the strong force, which overcomes electrical repulsion.
Negatively charged electrons are attracted to the nucleus.
The number of protons in an atom is called the atomic number, which is unique for different chemical elements.
The combined number of protons and neutrons in an atom is called the atomic mass number.
Atoms of the same element with different number of neutrons are called isotopes.

18. Absorption and Emission in Gases
Since electrons in atoms can have only specific
energies, the atoms can absorb or release energy
only in these amounts (quanta)
Electron gets energy, jumps to an excited state,
release the energy, and falls back down
The energy is emitted as a photon of light
The photon has exactly the same energy that
the electron has lost

19. Types of Spectra
Emission line spectrum consists of photons emitted as each electron falls back to lower levels
Absorption line spectrum appears when photons
are absorbed, causing electrons to jump up in energy
Each element or molecule produces its own distinct
set of spectral lines

20. Emission by Hydrogen

21. Hydrogen lines in the visible

22. Examples of Spectra

23. Thermal Radiation ``Complex’’ objects - planets, stars, people -
produce thermal radiation
Its spectrum depends only on the object’s
temperature
Hotter objects emit more total radiation per unit surface area
The radiated energy is proportional to the fourth power of the temperature
Hotter objects emit photons with a higher average energy

24. Temperature and Color

25. Temperature and Intensity

26. Reflected light When the light (for example, sunlight) strikes an
object (ground, clouds, people), we see only the
wavelengths of light that are reflected
Different objects (fruits, rocks, atmospheric gases)
reflect and absorb light at different wavelengths

27. The Doppler Shift
Radial motion of a distant object can be determined due to the Doppler effect
The Doppler effect causes shifts in the wavelengths
of light
If an object is moving toward us, its entire spectrum is shifted to shorter wavelengths
Because shorter wavelengths of the visible light are bluer, the Doppler shift of this object is called a blueshift
The Doppler shift of a moving away object - redshift

28. Doppler Effect
Demo Doppler effect

29. Summary
Spectral information gives us more knowledge about the objects (composition, surface temperature, moving properties)
Visible light is only a small portion of the electromagnetic spectrum
The Doppler effect tells us how quickly light is moving toward or away from us