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Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And Ions

Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

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Page 1: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

Lecture 3Ch.2

Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58

Lecture 3Ch.2

Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58

Atomic Structure, Isotopes, And IonsAtomic Structure, Isotopes, And Ions

Page 2: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

Understanding the Nature of Atoms

• If you cut a piece of graphite from the tip of a pencil into smaller and smaller pieces, how far could you go?

• Could you divide it forever, or would the small pieces eventually become indivisible?

• You would eventually end up with atoms (translates to “indivisible” in greek) of pure carbon.

• You can not divide a carbon atom into smaller pieces and still have carbon

Page 3: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• An atom is the smallest identifiable unit of an element

• The theory that all matter is composed of atoms grew out of two primary laws

1. Law of conservation of mass 2. Law of constant composition

Matter

Page 4: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

In a chemical reaction, atoms are not created or destroyed, but merely

rearranged. In other words, the total mass of substances present before a

reaction is equal to the total mass after.

Law of Conservation of Mass

Page 5: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

The relative amounts of each element in a given substance are always the

same, regardless of how the substance was made.

Law of Constant Composition

Page 6: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• For a molecule, AB:

• mass A + mass B = total mass AB• %A + %B = 100• %A =

• Example: We analyze 1.630 g of CaS and find that it’s 0.906 g Ca. Find the mass of S? Find the mass% of Ca and S?

* 55.6% Ca, 44.4% S* This means that all pure CaS in the universe has the same composition as calculated above, regardless of how it was made or where it was found.

Law of Constant Composition

Page 7: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• We have established that matter is comprised of atoms. But what are atoms made of?

• In the 1800’s, physicists conducted numerous experiments which revealed that the atom itself is made up of even smaller, more fundamental particles.

• The three types of sub-atomic particles that make up the atom are known as:• electrons• protons• neutrons

Atomic Structure

Page 8: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

J.J. Thomson’s Cathode Ray Experiment (late 1800’s)

• No Electric Field• With Electric Field

Discovery of the Electron

Page 9: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Atoms are charge neutral. If electrons reside within an atom, then an equivalent number of positive charges must also exist, appropriately named protons.

• How do all these charges coexist?

• Thomson proposed the very first theoretical model of the atom, the so-called plum pudding model (PM) shown to the right.• Electrons reside in a sea of

uniform positive charge

Plum Pudding Model

Page 10: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Ernest Rutherford sought to test the PM model using the gold foil experiment (below)

• A beam of positively charged α-particles were focused on a very thin sheet of gold

• Based on the PM model, this beam would pass right through the gold foil. In actuality, the beam was deflected at odd angles, with some α-particles bouncing directly back!!

Protons and The Nucleus

Page 11: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

True model of the atom is a dense, positively charged,

proton-loaded nucleus surrounded by a sparse

electron cloud ! The vast majority of an atom’s mass is contained within the nucleus.

Nucleus

Electron cloud

α particles

scattered, repulsed particles

transmitted through cloud

THE ATOM

Page 12: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Rutherford’s model was incomplete. For example, a hydrogen atom has one proton and one electron, but is only ¼th the mass of a helium atom which has two electrons and two protons.

• If all of the mass of an atom comes from its sub-atomic particles, how do we explain the unaccounted for mass?

• The answer is neutrons, particles that are equal in mass to protons, but with no electrical charge.

Neutrons

Page 13: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

Particle Relative Charge Mass (amu)

Proton +1 1.007

Neutron 0 1.008

Electron -1 .000548

Charges shown in table are relative to the charge of a proton. A proton has an actual charge of 1.602 x 10-19 Coulombs (C), an electron has a charge of -1.602 x 10-19 C. Opposite charges attract! Like charges repel!!

Subatomic Particles and Their Relative Masses & Charges

Page 14: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• The number of protons in an atom is called the atomic number. An element is defined by its atomic number. (ex. only carbon has 6 protons)

• For a given element, the number of protons DOES NOT CHANGE

• In a neutral atom, the number of protons is equal to the number of electrons.

6

CCarbon

12.0107

Atomic #

Elemental Symbols

Page 15: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

6

CCarbon

12.0107 Mass #

Elemental Symbols

• The mass number of an element is the sum of its protons and neutrons.

• The mass #’s listed on the periodic table are average masses (the unit of atomic mass is the amu, or atomic mass unit).

• These averages are used because numerous variations of elements called isotopes exist in nature.

Page 16: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Isotopes are variations of elements with the same number of protons but different numbers of neutrons.

(98.93%)

(1.07%)

(~ 0%)

mass number

atomic number

Three isotopes of carbon. The % abundances of each are shown.

Isotopes

Page 17: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

Transitional PageAvg. atomic mass is obtained using the % abundance and the isotope mass.

𝐴𝑣𝑒𝑟𝑎𝑔𝑒𝑎𝑡𝑜𝑚𝑖𝑐𝑚𝑎𝑠𝑠=∑ (𝑖𝑠𝑜𝑡𝑜𝑝𝑒𝑚𝑎𝑠𝑠 ) 𝑥(% 𝑎𝑏𝑢𝑛𝑑𝑎𝑛𝑐𝑒)

Page 18: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• For the table below, fill in the numbers of protons, neutrons, and electrons for each isotope of carbon.

• Then, using the given abundances and isotope masses, calculate the average atomic mass of C. Does it match the reported value?

ISOTOPE P N E % A Mass (amu)

98.93 12

1.07 13.003 354 8378

~0 14.003 2420

Group Work

Page 19: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Boron has two isotopes, 10B and 11B. Using the given isotope masses, determine the % abundances of each isotope.

ISOTOPE % A Mass (amu)

10.013

11.009

Group Work

Page 20: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• The nuclei of most naturally occurring isotopes are very stable, despite the massive repulsive forces that exist between the protons in the nucleus.

• A strong force of attraction between neutrons and protons known as the nuclear force counteracts this repulsion.

• As the number of protons increases, more neutrons are required to stabilize the atom. Stable nuclei up to atomic number 20 have equal numbers of protons and neutrons.

• For nuclei with atomic number above 20, the number of neutrons exceeds the protons to create a stable nucleus.

Proton-Neutron Ratio and Radioactivity

Page 21: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Radioactive isotopes are unstable (high in energy). This instability is attributed to a neutron/proton ratio that is either too high or too low.

• To become stable, they spontaneously release particles or radiation to lower their energy.

• This release of energy is called radioactive decay.

Proton-Neutron Ratio and Radioactivity

Page 22: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

Property α β γ

Charge 2+ 1- 0

Mass 6.64 x 10-24 g 9.11 x 10-28 g 0

Emitted Radiation Type

2 protons and 2 neutrons ()

High energy electron.

Pure energy (Radiation)

Penetrating Power Low. Stopped by paper. Blocked by skin.

Moderate. Stopped by aluminum foil. (10α)

High. Can penetrate several inches of lead. (10000α)

• The three most common types of radioactive decay are alpha, beta, and gamma

Radioactivity

Page 23: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• For example, the isotope undergoes alpha decay to decrease its n/p ratio:

• The Thorium-234 isotope then undergoes beta decay which lowers the ratio even more:

– In beta decay, a neutron is converted to a proton and an electron. This causes the proton count to increase:

• Gamma (γ) decay usually accompanies α or β decay to release residual excess energy. γ is not shown in equations.

𝑈→ h𝑇 + 𝐻𝑒24

90234

92238

h𝑇 → 𝑃𝑎+ 𝑒−10

91234

90234

𝑛→ 𝑝+ 𝑒− 10

11

01

Radioactivity

Page 24: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

Stable isotopes within the belt

*too few protons (β-decay)

*too many protons (α-decay)

All elements beyond atomic number 83 are

radioactive.

Belt of Stability

Page 25: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Thus far, we’ve learned that each element has an exact number of protons. – For example, Hydrogen has only one proton. If you force a

second proton onto the atom, you no longer have hydrogen… you now have Helium.

• We have also learned that atoms can have variable numbers of neutrons (isotopes).

• Next, we will discuss ions.

Ions

Page 26: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Ions are electrically charged atoms, resulting from the gain or loss of electrons.

• Positively charged ions are called cations. You form cations when electrons are lost

• Negatively charged ions are called anions. You form anions when electrons are gained

Ions

Page 27: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• A cation is named by adding the word “ion” to the end of the element name

• Anions are named by adding the suffix –ide to the end of an element

𝑳𝒊+¿ ¿

𝑵𝒂+¿ ¿

𝑴𝒈𝟐+¿ ¿

𝑨𝒍𝟑+¿¿

Lithium ion

Sodium ion

Magnesium ion

Aluminum ion

𝑪𝒍−

𝑺𝟐−

𝑶𝟐−

𝑷 𝟑−

Chloride

Sulfide

Oxide

Phosphide

Ion Nomenclature

Page 28: Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Lecture 3 Ch.2 Suggested HW: 15, 19, 23, 28, 38, 49, 52, 58 Atomic Structure, Isotopes, And

• Fill in the missing information below

ISOTOPE P N E

2-

?? 13 14 10

4+

Group Work