Atmos. Chem. Lecture 4, 9/16/13 Light and Spectroscopy Electromagnetc spectrum 9/16/13

Atmos. Chem. Lecture 4, 9/16/13

Light and Spectroscopy

Why/how do molecules absorb light?

PSet 1 - due in class 9/25

Electromagnetc spectrum

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9/16/13

1

Blackbody radiaton

Sun: 5777 K

F

B

(

λ

)

=

2

π

c e ch / k

2 h

B

λ T

λ

− 5

1

F

B

=

σ

T

4

σ   = 2/15 π 5 k 4 c

= 5.671 x 10 -8

-2 h -3

W m -2 K -4

S&P

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tive

Light and energy

E

= hv

= hc

λ

9/16/13

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Commons license. For more information, see http://ocw.mit.edu/help/faq-fair-use/ .

Zumdahl, Chemistry , 8 th ed.

2

Photochemistry: Absorpton of light

A + h v → A*

Excited state: vibratonal, rotatonal, electronic

Molecule can absorb radiaton efciently if:

1)   The photon energy matches the energy spacing

between molecule's quantum levels

2)   Optcal transiton between these quantum levels is allowed by "selecton rules" ("forbidden" transitons are weaker)

3)   Electronic: overlap between wavefunctons is high

Vibratonal excitaton

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htp://wiki.verkata.com/en/wiki/Morse potental

[ Note: A dditional material is discussed here during lecture.

]

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Polyatomic molecules

  bands more common

Finlayson-Piis and Piis

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.

v

1

+v

3

band of H

2

O

(from S. Nizkorodov, VC/)

Courtesy of Sergey Nizkorodov. Used with permission.

Electronic transitons

4

J' 3

2

Quantum numbers: Λ, S , Ω

4

J" 3

2 v '=1 v "=0

Excited (upper) electronic state

For more detail see F-P&P, pp. 46-47; or

Herzberg, Molecular spectra and molecular structure , Van Nostrand 1950

4

J' 3

2

4

J" 3

2 v '=1 v "=0

[ Note: A dditional material is discussed here during lecture.

]

Ground (lower) electronic state

9/16/13

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In reality.

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