survey of the universe tom burbine tburbine@mtholyoke
DESCRIPTION
Survey of the Universe Tom Burbine [email protected]. Prospective Astronomy Majors Lunch. Monday, March 4 th 12:15-1:10pm Kendade 303. Meet the faculty, learn about the Mars Rover, and enjoy a delicious lunch. HW# 3. Due March 6. Characteristics of waves. - PowerPoint PPT PresentationTRANSCRIPT
Survey of the Universe
Prospective Astronomy Majors Lunch
Meet the faculty, learn about the Mars Rover, and enjoy a delicious lunch.
Monday, March 4th
12:15-1:10pmKendade 303
HW# 3
• Due March 6
Characteristics of waves• velocity = wavelength x frequency• Wavelength = distance• Frequency = cycles per second = hertz
For light
• c = wavelength x frequency• In a vacuum, speed of light stays the same• So if wavelength goes up• Frequency does down• f = frequency• λ = wavelength• c = λ x f
Calculations
• c = λ x f• So if the wavelength is 1 x 10-12 m• 3 x 108 m/s = 1 x 10-12 m * f• f = 3 x 108 m/s/1 x 10-12 m • f = 3 x 1020 s-1 = 3 x 1020 Hz
Calculations
• c = λ x f• So if the frequency is 1 x 1015 Hz• 3 x 108 m/s = λ * 1 x 1015 Hz • λ = 3 x 108 m/s/1 x 1015 Hz • λ = 3 x 10-7 m
Energy of light
• Energy is directly proportional to the frequency• E = h * f• h = Planck’s constant = 6.626 x 10-34 J*s• since f = c/λ• Energy is inversely proportional to the wavelength• E = hc/λ
Calculations
• What is the energy of a radio wave with a frequency of 1 x 107 Hz?
• E = h * f• h = Planck’s constant = 6.626 x 10-34 J*s• E = 6.626 x 10-34 J*s * 1 x 107
• E = 6.626 x 10-27 J
Calculations
• What is the energy of a gamma ray photon with wavelength of 1 x 10-15 m
• E = hc/λ• h = Planck’s constant = 6.626 x 10-34 J*s• E = 6.626 x 10-34 J*s * 3 x 108 m/s / 1 x 10-15 m• E = 1.99 x 10-10 J
Higher the frequency, Higher the energy of the photonHigher the wavelength, Lower the energy of the photon
redviolet
VIBGYOR
ROYGBIV
• ROYGBIV • Red – long wavelength• Violet – short wavelength
http://www.arpansa.gov.au/images/basics/emr.jpg
Any Questions?