1.2 Mass Spectroscopy - OCHS Chemistry
Transcript of 1.2 Mass Spectroscopy - OCHS Chemistry
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1.2 Mass Spectroscopy
• LT: Explain the quantitative relationship between the mass spectrum of an element and the masses of the element's isotopes.
IsotopesIsotopes are atoms of the same element having different
masses due to varying numbers of neutrons.
Isotope Protons Electrons Neutrons Nucleus
Hydrogen–1
(protium)
1 1 0
Hydrogen-2
(deuterium)
1 1 1
Hydrogen-3
(tritium)
1 1 2
Atomic Masses
Isotope Symbol Composition of the nucleus
% in nature
Carbon-12 12C 6 protons
6 neutrons
98.89%
Carbon-13 13C 6 protons
7 neutrons
1.11%
Carbon-14 14C 6 protons
8 neutrons
<0.01%
Atomic mass is the average of all the naturally
isotopes of that element.
Carbon = 12.011
Atomic Number
Atomic number (Z) of an element is the
number of protons in the nucleus of
each atom of that element.
Element # of protons Atomic # (Z)
Carbon 6 6
Phosphorus 15 15
Gold 79 79
Mass NumberMass number is the number of
protons and neutrons in the nucleus
of an isotope.
Mass # = p+ + n0
Nuclide p+ n0 e- Mass #
Oxygen - 10
- 33 42
- 31 15
8 8 1818
Arsenic 75 33 75
Phosphorus 15 3116
Mass Spectrometry
• Mass spectrometry provides mass to charge ratio and provides us with information to determine the molecular mass of atoms/molecules in a sample.
• High-energy electrons bombard the sample, causing it to ionize
• An electric field separates the ions based on their mass to charge ratio this data is compiled into a mass spectrum
• (it separates isotopes by mass)
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Mass Spectrometry
• The relative size of the peaks indicates the relative number of particles
1.2 Closure
• Mass Spec…
1.3 Empirical and Molecular Formulas
• LT: Explain the quantitative relationship between the elemental composition by mass and the empirical formula of a pure substance.
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Formulas (continued)
Formulas for molecular compounds MIGHTbe empirical (lowest whole number ratio).
Molecular:
H2O
C6H12O6 C12H22O11
Empirical:
H2O
CH2O C12H22O11
Empirical Formula Determination
1. Base calculation on 100 grams of compound.
2. Determine moles of each element in 100 grams of compound.
3. Divide each value of moles by the smallest of the values.
4. Multiply each number by an integer to obtain all whole numbers.
Empirical Formula Determination
Adipic acid contains 49.32% C, 43.84% O, and 6.85% H by mass. What is the empirical formula of adipic acid?
49.32g C 1 mol C=4.107 mol C
12.01 g C
6.85 16.78
1.01
g H mol Hmol H
g H
43.84 12.74
16.00
g O mol Omol O
g O
Empirical Formula Determination(part 2)
Divide each value of moles by the smallest of the values.
Carbon:
Hydrogen:
Oxygen:
4.1071.50
2.74
mol C
mol O
6.782.47
2.74
mol H
mol O
2.741.00
2.74
mol O
mol O
Empirical Formula Determination(part 3)
Multiply each number by an integer to obtain all whole numbers.
Carbon: 1.50 Hydrogen: 2.50 Oxygen: 1.00x 2 x 2 x 2
3 5 2
Empirical formula: C3H5O2
Finding the Molecular FormulaThe empirical formula for adipic acid is C3H5O2. The molecular mass of adipic acid is 146 g/mol. What is the molecular formula of adipic acid?
1. Find the formula mass of C3H5O2
3(12.01 g) + 5(1.01) + 2(16.00) = 73.08 g
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Finding the Molecular FormulaThe empirical formula for adipic acid is C3H5O2. The molecular mass of adipic acid is 146 g/mol. What is the molecular formula of adipic acid?
3(12.01 g) + 5(1.01) + 2(16.00) = 73.08 g
2. Divide the molecular mass by the mass given by the emipirical formula.
1462
73
Finding the Molecular FormulaThe empirical formula for adipic acid is C3H5O2. The molecular mass of adipic acid is 146 g/mol. What is the molecular formula of adipic acid?
3(12.01 g) + 5(1.01) + 2(16.00) = 73.08 g
3. Multiply the empirical formula by this number to get the molecular formula.
(C3H5O2) x 2 = C6H10O4
1462
73
Percent Composition
PERCENT COMPOSITION BY MASS: Because compounds must have a constant composition, it is possible to find the percent by mass of each element in the compound:
% composition =mass of element
mass of compound´100%
% Composition example 1
Ammonium is used extensively in the production of fertilizer, where the ammonia is converted in ammonium nitrate. Find the percent nitrogen in ammonium nitrate.
% composition =mass of element
mass of compound´100%
% Composition example 1
Calculate the percent water in strontium hydroxide octahydrate
% composition =mass of element
mass of compound´100%
1.4 Composition of a Mixture
• LT: Explain the quantitative relationship between the elemental composition by mass and the composition of substances in a mixture.
• Gravimetric Analysis Lab
– First, isolate either a mixture or a compound
– Then, we mixed with water to dissolve all ions.
– Finally, we mixed with another chemical that would create one precipitate that we could filter out and measure.
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1.5 Electron Configuration
• LT: Represent the electron configuration of an element or ions of an element using the Aufbau principle.
Quantum MechanicalModel of the Atom
Mathematical laws can identify the regions outside of the nucleus where electrons are most likely to be found.
These laws are beyond the scope of this class…
Heisenberg Uncertainty Principle
The more certain you are about where the electron is, the less certain you can be about where it is going.
The more certain you are about where the electron is going, the less certain you can be about where it is.
“One cannot simultaneously determine both the position and momentum of an electron.”
WernerHeisenberg
Quantum Numbers
Each electron in an atom has a unique set of 4 quantum numbers which describe it. (**Not Tested!)
Principal quantum number
Angular momentum quantum number
Magnetic quantum number
Spin quantum number
Electron Energy Level (Shell)
Generally symbolized by n, it denotes the probable distance of the electron from the nucleus. “n” is also known as the Principle Quantum number
Number of electrons that can fit in a shell: 2n2
Orbital shapes are defined as the surface that contains 90% of the total electron probability.
An orbital is a region within an energy level where there is a probability of finding an electron.
Electron Orbitals
The angular momentum quantum number, generally symbolized by l, denotes the orbital (subshell) in which the electron is located.
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The s orbital (l = 0) has a spherical shape centered aroundthe origin of the three axes in space.
s Orbital shape
There are three dumbbell-shaped porbitals (l = 1) in each energy level above n = 1, each assigned to its own axis (x, y and z) in space.
p orbital shape
Things get a bit more complicated with the five d orbitals (l = 2) that are found in the dsublevels beginning with n = 3. To remember the shapes, think of “double dumbells”
…and a “dumbell with a donut”!
d orbital shapes Shape of f (l = 3) orbitals
EnergyLevel (n)
Sublevels inmain energy
level (n sublevels)
Number oforbitals per
sublevel
Number ofElectrons
per sublevel
Number ofelectrons permain energylevel (2n2)
1 s 1 2 2
2 sp
13
26
8
3 spd
135
2610
18
4 spdf
1357
261014
32
Energy Levels, Sublevels, Electrons Magnetic Quantum NumberThe magnetic quantum number, generally symbolized by m, denotes the orientation of the electron’s orbital with respect to the three axes in space.
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Electron SpinThe Spin Quantum Number describes the behavior (direction of spin) of an electron within a magnetic field.
Possibilities for electron spin:
1
2
1
2
Pauli Exclusion Principle
Two electrons occupying the same orbital must have opposite spins
Wolfgang Pauli
© 1998 by Harcourt Brace & Company
sp
d
f
1
2
3
4
5
6
7
6
7
C. Periodic Patterns ATOMIC ORBITALS• Atomic Orbital: region of
space in which there is a high probability of finding an electron.
• Denoted by letters: s, p, d, and f
• Each atomic orbital corresponds to a specific shape at a specific energy level.
s - spherical
p – dumbbell-shaped
d – clover leaf-shaped
f – more complex
ATOMIC ORBITALS
Type of Sublevel Number of Orbitals Number of Electrons
s 1 2
p 3 6
d 5 10
f 7 14
MAXIMUM NUMBER OF ELECTRONS FOR EACH ENERGY LEVEL
Energy level (n) Max number of Electrons
1 2
2 8
3 18
4 32
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Nucleus
n = 1
n = 2
n = 3
n = 4
s
s p
Energy Levels
s p
s p
d
d
f
Sublevels
Electron ConfigurationThe most stable arrangement of electrons in sublevels and orbitals.
A. General Rules
• Aufbau Principle
– Electrons fill the lowest energy orbitals first.
– “Lazy Tenant Rule”
A. General Rules
• Pauli Exclusion Principle
– Each orbital can hold TWO electrons with
opposite spins.
RIGHTWRONG
A. General Rules
• Hund’s Rule
– Within a sublevel, place one e- per orbital before pairing them.
– “Empty Bus Seat Rule”
O
8e-
B. Notation
• Orbital Diagram
Electron Configuration
1s2 2s2 2p4
1s 2s 2p
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Shorthand Configuration
S 16e-
Valence ElectronsCore Electrons
S 16e- [Ne] 3s2 3p4
1s2 2s2 2p6 3s2 3p4
B. Notation
• Longhand Configuration
C. Periodic Patterns
• Period #– energy level (subtract for d & f)
• A/B Group # – total # of valence e-
• Valence electrons are electrons in the outermost energy level. Determines the chemical and physical properties of an element.
• Column within sublevel block– # of e- in sublevel
s-block1st Period
1s1 1st column of s-block
C. Periodic Patterns
• Example - Hydrogen
Element Configuration
notation
Orbital notation Noble gas
notation
Lithium 1s22s1
____ ____ ____ ____ ____
1s 2s 2p
[He]2s1
Beryllium 1s22s2
____ ____ ____ ____ ____
1s 2s 2p
[He]2s2
Boron 1s22s2p1
____ ____ ____ ____ ____
1s 2s 2p
[He]2s2p1
Carbon 1s22s2p2
____ ____ ____ ____ ____
1s 2s 2p
[He]2s2p2
Nitrogen 1s22s2p3
____ ____ ____ ____ ____
1s 2s 2p
[He]2s2p3
Oxygen 1s22s2p4
____ ____ ____ ____ ____
1s 2s 2p
[He]2s2p4
Fluorine 1s22s2p5
____ ____ ____ ____ ____
1s 2s 2p
[He]2s2p5
Neon 1s22s2p6
____ ____ ____ ____ ____
1s 2s 2p
[He]2s2p6
1.6 Photoelectron Spectroscopy Coulomb's Law
• a law stating that like charges repel and opposite charges attract, with a force proportional to the product of the charges and inversely proportional to the square of the distance between them.
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PHOTOELECTRON SPECTROSCOPY
Using PES data and other data to understand:
• Atomic structure
• Electron configurations
• Ionization energy
• Periodic trends
What is PES?
• Photoelectron spectrophotometers use high-energy radiation (UV or X-rays) to eject electrons from an atom
• The photoelectron spectrophotometer inputs only one type of radiation (with a specific energy)
• Because electrons within an atom are in different energy levels, different electrons can require different amounts of energy to eject– Electrons that are closer to the nucleus are HARDER to remove
(More attraction between protons and electrons)– Valence electrons (outer level) are the EASIEST to remove
• The photoelectron spectrophotometer removes electrons from multiple atoms, so electrons from all levels will be observed (& graphed)
What is measured?
• The “input” energy removes the electron from the atom• Any “leftover” energy determines how fast the electrons is
moving when it leaves the atom
• If only a small amount of energy is needed to remove an electron, a lot of energy is “leftover”
• These electrons will be moving fast
• If a lot of amount of energy is needed to remove an electron, not much energy is “leftover”
• These electrons will be moving slow
Reading PES Graphs
Reading PES Graphs Sample Graphs
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1 2
3 4
5 6
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7 8
9 10
11 12
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13 14
15 16
17 18
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19 20
21 Which element?
Which element? Real Spectra
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1.7 Periodic Trends
• Justify all of the trends on the periodic table can be simplified using these two generalizations:
1. Use Zeff to justify trends across a period
2. Use increased distance (greater value of n) to justify trends down a group
Zeff
• Effective Nuclear Charge
Value of n
• Energy levels
Atomic Radius
• Refers to the distance between the nucleus and the outer edge of the electron cloud. It is influenced by the nuclear pull an the number of energy levels.
Atomic Radius
• Atomic radii decrease as atomic numbers increase in any given period.
– Greater effective nuclear charge, Zeff, increases the attractive force of the nucleus and therefore pulls the electron cloud closer to the nucleus resulting in smaller atomic radius.
Atomic Radius
• Atomic radii increases as atomic number increases down a column or group
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Ionization Energy
• Refers to the energy needed to remove an electron from a gaseous atom or ion, i.e. an isolated one, not part of a solid, liquid, or a molecule. It is always endothermic.
Ionization Energy• Ionization energy increases as atomic number
increases in any given period.
Ionization Energy
• Ionization energy decreases as atomic number increases down a column or group.
Electron Affinity
• Is NOT the opposite of ionization energy, but involves the addition of an electron to the gaseous atom, which can be exothermic or endothermic.
• Positive electron affinities indicate that the nucleus is not as effective at attracting the electron, and it must be forced into the atom.
Electronegativity
• An assigned property which indicates the attraction of an atom for the pair of outer shell electrons in a covalent bod with another atom. Electronegativity patterns are the same as electron affinity patterns for the same reasons.
• Focus on the attraction that the nucleus has for electrons.
Electronegativity
• Increases as atomic number increase in any given period.
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Electronegativity
• Decreases as atomic number increases down a column or group.
Ionic Radius
• The distance from the nucleus to the outer edge of the electron cloud in a charged ion.
• The same radii trends apply once you divide the table into the metal and non-metal sections.
• Positive (metals) ionic radii decrease from left to right with only minor changes in the transition metals
• Negative (nonmetal) ionic radii are larger and they will decrease in radii from left to right.
Ionic Radius
• Positive ions are smaller than their respective neutral atoms.
Ionic Radius
• Negative ions are larger than their respective neutral atoms
Reactivity
• Depends on whether the element reacts by losing electrons (metals) or gaining electrons (non-metals).
Reactivity
• Metals are more reactive as you move down a column.
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Reactivity
• Non-metals are more reactive as you move up a column
1.8 Valence Electrons and Ionic Compounds