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Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere...

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Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957
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Page 1: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Equilibrium and Radioactivity

From there to here, from here to there, funny things are everywhere

--TSG 1957

Page 2: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

The rate of a reaction

• Expressed in mol/sec or M/s

Page 3: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

N2 + 3H22NH3

• If 2.40 moles of NH3 are produced each second, what is the rate of use of N2 and H2?

Page 4: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

N2 + 3H22NH3

• If 2.40 moles of NH3 are produced each second, what is the rate of use of N2 and H2?

• 2.40 mol NH3/s x 1 N2/2 NH3

=1.20 mol N2/s

• 2.40 mol NH3/s x 3 H2/2 NH3

=3.60 mol H2/s

Page 5: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

How can you speed up a reaction?

Page 6: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

How can you speed up a reaction?

• --Heat it up.

• --Crush, grind or powder a solid reactant.

• --Increase pressure of a gaseous reactant

• --Increase concentrations of aqueous reactants

• --Add a catalyst (if known)

• (Stir or shake to bring reactants together.)

Page 7: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

How would you speed up…

• Hydrochloric acid acts on tin metal to form hydrogen gas and aqueous tin (II) chloride

Page 8: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

How would you speed up…

• Hydrochloric acid acts on tin metal to form hydrogen gas and aqueous tin (II) chloride

• Increase concentration of HCl

• Powder the tin

• Heat the reactants

• Stir or shake

• (I don’t know of a catalyst—it’s pretty fast already)

Page 9: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Reversible reactions.

• AKA “all reactions”

• All reactions work in reverse, at least a little bit.

should be written as

Page 10: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Write the reverse reaction

• 2NaHCO3 (s) Na2CO3 (s) + H2O (g)

• CaCO3 (s) CaO (s) +CO2 (g)

• H2 (g) +Cl2 (g) 2HCl (g)

• N2 (g) + 3H2 (g) 2NH3 (g)

Page 11: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

H2 +I2 2HI

1 mole H2

and 1 mole I2

(1L)

If you start with 1 mole H2 and 1 mole I2 in a 1L flask…

Page 12: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

H2 +I2 2HI

1 mole H2

and 1 mole I2

(1L)

.8 mole H2 .8 mole I2

and .4 mole HI

(1L)

…it will proceed forwards. Some of the reactants will form products.

Page 13: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

H2 +I2 2HI

2 mole HI

(1L)

If you start with 2 moles HI in a 1L flask…

Page 14: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

H2 +I2 2HI

2 mole HI

(1L)

.8 mole H2 .8 mole I2

and .4 mole HI

(1L)

…it will proceed in reverse. Some of the “products” will form reactants

Page 15: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

H2 +I2 2HI

1 mole H2

and 1 mole I2

(1L)

2 mole HI

(1L)

Did you notice?

.8 mole H2 .8 mole I2

and .4 mole HI

(1L)

Page 16: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

H2 +I2 2HI

1 mole H2

and 1 mole I2

(1L)

2 mole HI

(1L)

You get the same final concentrations

.8 mole H2 .8 mole I2

and .4 mole HI

(1L)

Page 17: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Starting with reactants…

0

0.005

0.01

0.015

0.02

0.025

0.03

0.035

0 20 40 60

The forward reaction starts out fast, then slows as reactants are used up

Rat

e of

rea

ctio

n (m

ol/s

)

Time (s)

Page 18: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Starting with reactants…

The reverse reaction starts out at 0 mol/s, then speeds up as products are produced

0

0.005

0.01

0.015

0.02

0.025

0 20 40 60

Rat

e of

rea

ctio

n (m

ol/s

)

Time (s)

Page 19: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Starting with reactants…

Did you notice?

0

0.005

0.01

0.015

0.02

0.025

0.03

0.035

0 10 20 30

Rat

e of

rea

ctio

n (m

ol/s

)

Time (s)

Page 20: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Starting with reactants…

The forward and reverse reactions reach the same rate. Concentrations will stabilize

0

0.005

0.01

0.015

0.02

0.025

0.03

0.035

0 10 20 30

Rat

e of

rea

ctio

n (m

ol/s

)

Time (s)

Page 21: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Eventually…

…reactants make products just as fast as products make reactants.

Page 22: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Eventually…

…reactants make products just as fast as products make reactants.

• It’s inevitable.

Page 23: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Eventually…

…reactants make products just as fast as products make reactants.

• It’s inevitable.

• It’s dynamic equilibrium

Page 24: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.
Page 25: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Try it.

• N2 + 3H2 2NH3

• Describe the rate of the forward reaction if you start with nitrogen and hydrogen.

• What is the rate of the reverse reaction?

• What happens to each rate?

• Why?

• Eventually…

Page 26: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

The equilibrium constant expression

• For aA +bB cC + dD

(if all substances are gasses or aqueous)

• The expression

[C]c [D]d

[A]a [B]b is a constant (K) at a given temperature

Page 27: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Please note:

• Products on top

• Coefficients become exponents

• Brackets mean “molarity”

• Concentrations are multiplied

• Solid and liquid substances are not included

…then this ratio is a constant!

Page 28: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

For example

• For: H2(g) +I2 (g)2HI (g)

• The equilibrium constant expression is:

• K= [HI]2 = (.4M)2 = .25

[H2][I2] (.8M)(.8M)

Page 29: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Write the equilibrium constant expression for …

1) 4NH3(g)+5O2(g)4NO(g)+6H2O(g)

2) CO (g) + 2H2 (g) CH3OH (g)

3) NH3(g)+H2O (l) NH4+ (aq) + OH-(aq)

Page 30: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Rookie mistakes:

• --putting reactants on top• --using coefficients inside the brackets• --adding instead of multiplying

concentrations• --multiplying by coefficients, instead of

raising to the power• --including liquids and solids.

Avoid these errors!

Page 31: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

What is the value of K?

1) 4NH3(g)+5O2(g)4NO(g)+6H2O(g)

.050 M .30 M .20 M .40 M

2) CO (g) + 2H2 (g) CH3OH (g)

.20 M .20 M .030 M

3) NH3(g)+H2O (l) NH4+ (aq) + OH-(aq)

.10 M 55.5 M .0013 M .0013 M

Page 32: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

What is the unknown concentration?

1) 4NH3(g)+5O2(g)4NO(g)+6H2O(g)

.060 M .40 M .15 M ? M

2) CO (g) + 2H2 (g) CH3OH (g)

? M .25 M .070 M

3) NH3(g)+H2O (l) NH4+ (aq) + OH-(aq)

? M 55.5 M .0019 M .00030M

Page 33: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Le Chatelier’s Principle

If a system in equilibrium is subjected to a stress, the system will shift in the direction that will relieve that stress

Page 34: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Application of LeChatelier’s principle

• “Shift right”--forward reaction is faster, --more of all products are formed--all reactants are used

• “Shift left”--reverse reaction is faster, --more of all reactants are formed--all products are used

Page 35: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Application of LeChatelier’s principle

• An aqueous or gas substance in the reaction added—shift away to use it up

• Increasing pressure—shift toward side with fewer moles of gas to relieve pressure

• Increasing temperature—shift in the endothermic direction to absorb heat

Page 36: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

N2(g) + 3H2(g) 2NH3(g) + Which way would the equilibrium

shift if you:1. Add N2(g)

2. Add H2(g)

3. Add NH3(g)

4. Increase P (compress)

5. Increase T

6. Add a catalyst

7. Remove N2(g)

7. Remove H2(g)

8. Remove NH3(g)

9. Decrease P (allow to expand)

10. Decrease T

11. Increase pressure by adding He (g)

Page 37: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

N2(g) + 3H2(g) 2NH3(g) + Which way would the equilibrium

shift if you:1. Add N2(g)

2. Add H2(g)

3. Add NH3(g)

4. Increase P (compress)

5. Increase T

6. Add a catalyst

7. Remove N2(g)

7. Remove H2(g)

8. Remove NH3(g)

9. Decrease P (allow to expand)

10. Decrease T

11. Increase pressure by adding He (g)

Page 38: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

N2(g) + 3H2(g) 2NH3(g) + Why?

1. Add N2(g)

2. Add H2(g)

3. Add NH3(g)

4. Increase P (compress)

5. Increase T

6. Add a catalyst

7. Remove N2(g)

7. Remove H2(g)

8. Remove NH3(g)

9. Decrease P (allow to expand)

10. Decrease T

11. Increase pressure by adding He (g)

Forward reaction

speeds up

Reverse reaction

slows down

Page 39: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

How would you shift this reaction to the left?

HCOOH (aq)+ HCOO- (aq) + H+ (aq)

(formic (heat) (formate (hydrogen

acid) ion) ion)

Page 40: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Why do reactions proceed at all?

Page 41: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Why do reactions proceed at all?

• To go to a more stable, lower energy state.

1) If H is (-), reaction gives off heat. (H<0)

OR

2) an advantage in gaining entropy, S. (S>0)

OR BOTH!

Page 42: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Enthalpy and Entropy

H

• Endo- or exothermic

• Energy is stored in/released from chemical bonds

• Measured in kJ/mol

S

• Gains or loses entropy

• A system becomes more or less disordered (s<l<aq<<g)

• Measured in J/ mol k

Page 43: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

2H2 +O22H2O…

Page 44: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

2H2 +O22H2O…

• H is very negative—it gives up a lot of heat.

2H2 +O22H2O +

Releasing heat is an advantage for a reaction

Page 45: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

2H2 +O22H2O…

• S is also negative—it loses entropy as 3 moles of gasses form only 2 moles.

This is a disadvantage, it’s worse at higher temperatures. Over 5000oC, hydrogen gas won’t even burn.

The advantage for entropy depends on temperature

Page 46: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

What is H, S and G?

• + CaCO3 (s) CaO (s) +CO2 (g)

• H2 (g) +Cl2 (g) 2HCl (g) +

• N2 (g) + 3H2 (g) 2NH3 (g) +

Page 47: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

• What happens at a higher temperature?

Page 48: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

…at a higher temperature…

1) Particles move faster.

2) There are more collisions.

3) Those collisions have more energy.

Page 49: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

To react, reactants must collide with enough energy, the activation energy.

Page 50: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Cool, medium, warm

Page 51: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Notice:

1) The bell-shaped distributions

2) The average speed is higher at higher To

3) The speeds spread out more at higher To

Page 52: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

What is “fast enough” to react?

More collisions will have enough energy to react at higher temperatures

Page 53: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

What if this is “fast enough”?

Page 54: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

What if this is “fast enough”?

Page 55: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

To react, reactants must collide with enough energy, the activation energy.

Page 56: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Catalysis

• A catalyst speeds up a reaction

• This is done by lowering the energy barrier, Ea

• When the barrier is lower, more collisions are “fast enough”

Page 57: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.
Page 58: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Nuclear Chemistry--

--as opposed the the unclear chemistry you have studied

Page 59: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Nuclear Chemistry

• --breaks the rules that one atom cannot be converted to another.

Chemistry: the dance of the electrons —nuclear reactions change the nuclei of atoms

• --charge and mass are still conserved.

Page 60: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Nuclide Notation

• A nuclide is a nucleus or atom of a specific isotope of an element

K39

19

• Potassium-39.

-- has 19 protons (atomic number = 19), making it potassium, and 20 neutrons (making a mass number of 39)

Page 61: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

How many p, n, e- in each?What is the mass number and

atomic number?

Cl-36

17

Sr+290

38

I-131

53

Th228

90

H3

1

Fe+359

26

Page 62: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

How many p, n, e- in each?What is the mass number and

atomic number?

Cl-36

17

Sr+290

38

I-131

53

Th228

90

H3

1

Fe+359

26

undergoes a decay

undergoes an decay

Page 63: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Natural decays

• —the loss of particle from a nuclide--The particle is composed of 2p and 2n,

the 4He nucleus--decreases the mass by 4 and the atomic

number by 2• —emission of an electron ( particle) from the

nucleus by the conversion of a n p + e---the electron is the particle--increases the atomic number by 1, does

not affect mass

Page 64: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Write the reaction

• Argon-39 undergoes a decay

• Thorium-228 undergoes an decay

• An decay forms lead-204

• A decay forms nitrogen-14

• A natural decay forms Sc-45 from Ca-45

• A natural decay forms Ac-227 from Pa-231

Page 65: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Stable?

Page 66: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Nuclear reactions

• Many nuclear reactions involve colliding nuclei or smaller particles at some significant fraction of the speed of light,

• --find the missing particle by balancing mass and charge.

Page 67: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Fission vs Fusion• Fission=breaking up large nuclei—

--natural radioactive decay of large atoms --used for nuclear power

• Fusion=combining small nuclei --occurs naturally in stars --prospects for nuclear energy—no radioactive byproducts

Both are transmutations—one nuclide is converted into another

Page 68: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Consider the relationships

• Half life

• Original amount

• Final amount

• Time elapsed

Page 69: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Consider the relationships

A=A0(1/2)

• A is the amount of the sample remaining

• A0 is the original amount in the sample

• t is the time that has passed, and

• t 1/2 is the half-life of the nuclide

t/t1/2

Page 70: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Please notice

A=A0(1/2)

A / A0 = the fraction remaining and

t / t 1/2=the number of half-lifes that have passed

t/t1/2

Page 71: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Try it.

• Hydrogen-3 has a half life of 12.3 years. If you start with a 20 g sample of H-3

--how much is left after 12.3 years?

--how much is left after 24.6 years?

--how much is left after 30.2 years?

Page 72: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Try it.

• Br-82 has a half life of 35.3 hours. If you start with a 6.5 mg sample of Br-82

--how much is left after 4 days?

--how long will it take to reach .75 mg?

Page 73: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Try it.

• Br-82 has a half life of 35.3 hours. If you start with a 6.5 mg sample of Br-82

--how much is left after 4 days?

--how long will it take to reach .75 mg?

How do you solve for an exponent?

Page 74: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Use a log function

log (A/A0)= log(1/2)

log (A/A0)= log(1/2)

= log (A/A0) log(1/2)

t/t1/2

t/t1/2

t/t1/2

Page 75: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Try it.

• Br-82 has a half life of 35.3 hours. If you start with a 6.5 mg sample of Br-82

--how much is left after 4 days?

--how long will it take to reach .75 mg?

Page 76: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Try it.

• If you start with 1.38 mg of U-234 and t1/2=2.44 x 105 yrs for its decay:

--how much is left after 20,000 years?

--how long will it take to reach 0.40 mg?

Page 77: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Try it.

• A .350 mg sample of K-42 decays to only .066 mg in 29.7 hours.

--what is the half life?

--how much was left after 20.0 hours?

--how long will it take to reach .010 mg?

Page 78: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

The uses of radioactivity

Page 79: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

The uses of radioactivity

• Medicine—tracers, radiation therapy

• History/geology—radioisotope dating

• Nuclear energy

• Nuclear weapons

Page 80: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

The uses of radioactivity

• Medicine—

Tracers:

I-131, S-35, F-18, P-32

Radiation therapy

I-131, Lu-177, Y-90, Sr-89

Page 81: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

The uses of radioactivity

• History/geology—radioisotope dating

• C-14, U-238, Sm-147, K-40

Page 82: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

The uses of radioactivity

• Nuclear Energy

• Nuclear reactions give off a large amount of energy

• This energy is often converted to electricity

• A nuclear reactor contains the reactants so the by-products (usually neutrons) carry out the chain reaction

Page 83: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Pressurized water reactor

Page 84: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Boiling water reactor

Page 85: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Heavy water reactor

Page 86: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Gas-cooled reactor

Page 87: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Hydride salt reactor

Page 88: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

Pebble bed modular reactor

Page 89: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.
Page 90: Equilibrium and Radioactivity From there to here, from here to there, funny things are everywhere --TSG 1957.

NERVA


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