Chapter 6 Flashcards

1
Q

Electromagnetic radiation is

A

Everywhere and is eneergy that travels in a continuous wavelike manner

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2
Q

Visible spectrum goes in order from left to right of

A

Rainbow backwards

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3
Q

All emr travels at

A

The speed of light (3.0 * 10^8 m/s)

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4
Q

Wavelength and frequency (v) are

A

Inversely related

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5
Q

Order of spectrum

A

Gammaray➡️xray➡️uv➡️visual➡️infared➡️microwave➡️fm➡️am➡️long radio waves

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6
Q

Frequency times wavelength equals

A

Speed of light

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7
Q

1m=

A

1*10^9 nm

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8
Q

Max plank proposed that

A

Atoms could only absorb(or release) energy in discrete chucks Called quantum

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9
Q

A quantum of light energy is

A

A photon

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10
Q

He also proposed that energy could be calculated by:

A

E=h*v

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11
Q

Planks constant

A

6.63*10^-34

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12
Q

When atoms absorb energy

A

They produce unique spectral lines

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13
Q

High density and hot matter produce

A

Continuous spectrum (white light)

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14
Q

Hot gas produces

A

Emission spectrum

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15
Q

Cold gas produces

A

Absorption spectrum

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16
Q

Neil’s Bohr showed that spectral lines are caused by

A

quantized jumps of electrons between energy levels

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17
Q

Bohr calculated the energy for each level

A

E= -2.18 * 10^-18J / n^2

18
Q

Black ________ all

White ________ all

A

Absorbs

Reflects

19
Q

Wavelength visible spectrum

A

400-700 nm

20
Q

Infared radiation we feel as

21
Q

Speed of light =

A

Frequency times wavelength

22
Q

Energy equals

A

Planks comstant times frequency

23
Q

The colored spectral lines on the emission spectrum are the result of

A

Electrons jumping from one energy level to another

24
Q

The difference between energy levels of electrons jumping from one energy level to another is

A

(-2.18 * 10^-18)(1/final squared - 1/initial squared)

25
All electromagnetic radiation tracked at
The speed of light
26
Lyman's series ends at energy level
1
27
Balmer series ends at energy level
2
28
Vance electrons
Participate in bonding and determine how an atom will behave
29
Core electrons are
Everything except for the balance electrons
30
Aufbau principle
Electrons enter orbitals of lowest energy first
31
Pauli exclusion principle
An orbital can hold a maximum of 2 electrons. Electrons in the same orbital have opposite spins
32
Hunts rule
Electrons will half fill degenerate orbitals until they have to double up
33
Our current understanding of the atom is the
Quantum mechanical model
34
Heisenberg uncertainty principle
We can't know the exact location of an electron we can only speak of probability
35
Schrodinger
Used his wave equation to map out probable electron locations
36
S
O
37
P
Dumbbell
38
D
🍀
39
F
🌼
40
Visible light is a type of
Electromagnetic radiation