Chemistry for Students: The Only Chemistry Study Guide You'll Ever Need to Ace Your Course
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About this ebook
The aim of this guide is not to be your teacher. Think of it as a road map. A way to navigate the world of chemistry and enjoy the scenery as you do so. And believe me, there is a lot to see. Atoms, the periodic table, chemical equations, acids, the Arrhenius theory; all these and many other concepts, as well as the minds behind them, are vital to understanding the world we inhabit. Our destination? Your success in the tests and exams that come your way. We want you to understand these concepts in a concise manner so that they are easy to remember.
However, speeding by won't accomplish much with anything in life. This guide is structured for your knowledge of the topic to aggregate incrementally. The more you learn, the easier things become. Do not let the strange words and confusing equations cloud your mind. Take these chapters one by one, and enjoy the trip.
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Chemistry for Students - Oakridge Press
Chemistry For Students
The Only Chemistry Guide You’ll Need to Ace Your Course
Leonel Travers
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Table of Contents
Book Description
Table of Contents
Chapter 1: High School Chemistry Review
The Basic Concepts of Chemistry
Measurements and Units
Derived Units
Chapter 2: The Structure of Matter
Atomic Theory
The Periodic Table
Periodic Trends
Electronegativity Trends
Ionization Energy Trends
Electron Affinity Trends
Atomic Radius Trends
Melting Point Trends
Practice Questions
Chapter 3: Chemical Bonds
Electron Configuration
Shorthand Electron Configuration
The Aufbau Principle
The Two Main Bonds
Ionic Bonds
Covalent Bonding
Additional Information & Other Bonds
The Difference Between Ionic And Covalent Bonds
Polar And Nonpolar Covalent Bonds
Sigma And Pi Bonds
Metallic Bonds
Practice Questions
Chapter 4: Chemical Reactions
Decomposition Reactions
Displacement Reactions
Single-Displacement Reactions
Double-Displacement Reactions
Combustion Reactions
Redox Reactions
Collision Theory
Practice Questions
Chapter 5: Thermodynamics and Electrochemistry
Electrolysis
Thermodynamics
The Zeroeth Law of Thermodynamics
The First Law of Thermodynamics
The Second Law of Thermodynamics
The Third Law of Thermodynamics
Equilibrium
Practice Questions
Chapter 6: Acid Base Chemistry
Arrhenius Theory
Brønsted-Lowry Theory
pH Levels
Acid-Base Indicators
Practice Questions
Chapter 7: Organic Chemistry
Hydrocarbons
Alkanes
Alkenes
Alkynes
Cyclic Hydrocarbons
Alcohols
Practice Questions
Chapter 8: Biochemistry
Biomolecules
Carbon Based Life
Carbohydrates
Lipids
Proteins
Practice Questions
Conclusion
Glossary
References
Chapter 1: High School Chemistry Review
No one misses high school. Piles of homework, alarm bells, teachers who were as bored as you were. I’m sure you’re glad to be out. But believe it or not, many things during those tedious years were invaluable. It’s a shame that we have so few passionate teachers to bring such knowledge to life.
Thanks to the schooling system and a lack of enthusiasm on the part of teachers, people make the mistake of viewing chemistry as something boring, unnecessary, and even laborious. Fear not, for chemistry is only such things in the mind of the unknowing.
Once you get the axioms down and have an appreciation for all that chemistry has enabled us to do, you will enjoy it far more than before. It will provide answers to questions you didn’t even know you had and open doors to worlds you completely ignored.
So, without homework to worry about, and without a teacher breathing down your neck, let’s delve back into the H2O and recap the basics of this fascinating science.
The Basic Concepts of Chemistry
When we think about chemistry, the average person will probably think of white lab coats and beakers on a table. Some will probably think of the popular TV show, Breaking Bad.
What many do not realize is how important chemistry is as a science and how much it has helped us collectively as the human race to accomplish. Chemistry, alongside physics and mathematics, is one of the most important sciences in terms of understanding the universe and ourselves.
We often take the periodic table for granted. But it is the result of thousands of years of human discoveries placed into one colorful little chart. It’s a great deal more than a chart, though. The periodic table is, in a technical sense, an array of legos from which the universe is built. The laws of physics and mathematics simply put those legos in place. Those who conceptualized and created the periodic table were true geniuses who dedicated themselves to finding out more about our reality. Of the 118 elements in the periodic table, 92 are natural. The rest are man-made, meaning that they are unstable (OpenStax, 2015).
The periodic table helps us understand and categorize what the things around us are made from. And knowing what things are made of and how they interact is vital to comprehending reality, a skill that seems to be sadly lacking in society these days.
For example, did you know that atoms are 99% space? So why don’t you simply fall through your seat right now?
Atoms are comprised of subatomic particles known as neutrons, protons, and electrons. Neutrons and protons are roughly the same size at nearly one Dalton (or atomic mass unit), whereas electrons are approximately 1/1800th of their size. Because of this, only neutrons and protons really add to the mass of an atom.
Positively (+) charged protons and uncharged neutrons bond to form the nucleus of an atom, and negatively (-) charged electrons reside on the outside. The only exception to this rule is hydrogen, which contains only one proton and one electron (OpenStax, 2015). Most of the time, atoms have a balanced number of protons and electrons, meaning that their net charge is neutral. Having an equal number of positively charged particles (protons) and negatively charged particles (electrons) means that, essentially, the two cancel each other out, leaving no excess positive or negative charge. Later on, we’ll look at what happens when this balance is disrupted.
Electrons, more often than not, are depicted as ring-like, orbiting the nuclei (protons and neutrons) of the atom. But newer findings have shown them to form a structure resembling that of a ‘cloud’ (Siegel, 2020) around the nucleus. These clouds of electrons then repel each other in a manner not unlike that of magnets to form what we perceive as solidity. However, we will be referring to the more traditional ‘shell’ or ‘orbital’ (OpenStax, 2015) depiction and understanding of electrons for the rest of this book to avoid confusion.
How do we differentiate atoms? We look at the number of protons within them. This is similar to the way in which we differentiate animals or plants from one another. Animals and plants have characteristics that differ between species and help us identify them at multiple levels of analysis.
The way we do this with elements isn’t by looking at their DNA, plumage, or leaf structure. Rather, in the realm of chemistry, elements are differentiated by the number of protons in their nuclei.
Measurements and Units
Measuring quantities in any and all sciences is vital. When you take a measurement of something, a quantitive comparison is being made between the thing that you are measuring and the instrument of measurement used for that substance.
The International System of Units
(Abozenadah et al., 2017), or SI, is the list of 7 internationally recognized units of measurement used in science. All other forms of measurement are derived from these 7.
These seven units make up what is commonly known as the metric system. In chemistry, we will typically be sticking to 5 of the 7; mole, kilogram, meter, second, and kelvin. Kelvin—the measure of absolute temperature—is often substituted with celsius (°C). These are not identical values. The difference between them can be defined as follows:
K = °C + 273.15
OR
°C = K − 273.15
When dealing with temperature, be mindful to never confuse it with heat. Temperature is the average kinetic energy of the particles that make up a material, a measure of how hot or cold an object is relative to another object (its thermal energy content), whereas heat is the flow of thermal energy between objects with different temperatures
(LibreTexts, 2014a).
Mass in SI is measured in kilograms. Within each kilogram are 1,000 grams, and within each gram are 1,000 milligrams. In 1889, the first prototypical model of the kilogram, or IPK (International Prototype of the Kilogram), was made from platinum-iridium alloy and is currently held in Paris, France. All other kilograms are equal to this prototype (Abozenadah et al., 2017). It is important to know that mass and weight are not the same. The weight of an object is influenced by the force of gravity.
Weight= Mass x The Acceleration of Gravity
OR
W=mg (Kramer, 2017)
People often use weight and mass interchangeably in day-to-day language, but in the realm of science, it is important to understand the distinction. The mass of an object is the total amount of matter within it. It does not change regardless of where you place it. Weight, on the other hand, is the exertion of gravitational force upon that object. It can change depending on where you place it in the universe.
The mass of a coconut stays the same in your bedroom, at the bottom of the ocean, and on the moon. The weight of the coconut changes across those locations based on the presence of gravity. The force of gravity is not constant, not even on the earth’s surface. Thus, the weight of objects is not constant and is not a reliable form of measurement.
Length is measured in meters. For those of you who are cheering for metric supremacy, it is wise to note that the metric system is just as arbitrary as the imperial system.
The meter, similar to the kilogram, has a prototypical ‘model’ (for lack of a better word) that is representative of all meters. Unlike the kilogram, though, it has gone through a number of changes. In 1889, it was represented by a bar of platinum-iridium alloy, then it changed to a wavelength of krypton-86 radiation in 1960, and in 1983, it changed for the final time to the length of the path traveled by light in a vacuum during a time interval of 1/299,792,458 second
(Abozenadah et al., 2017). This information is really just background knowledge. For now, focus on the meter as the SI unit of length.
The SI unit of time is... interesting. The second (1/60 of a minute) is not the simple little tick of the clock that we normally associate with it. It has been redefined several times over the years, but we currently define it as the duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the cesium-133 atom
(Abozenadah et al., 2017). However, for simplicity’s sake, think of it as the usual fraction of a minute.
How about measuring the amount of a substance? The mole—or mol in SI units—is used to measure very small particles in relatively large amounts. It is also known as Avogadro’s number,
named after the Italian physicist Amadeo Avogadro. Why ‘number’ and not ‘measurement’ or ‘unit’? Just as the word ‘dozen’ means twelve of a given item (for example, a dozen apples) a mole or mol refers to a set number of atoms or molecules. Unlike a dozen though, we must use scientific notation to define the number that constitutes one mol. Any other form would simply be too long and take up far too much space on a page. Additionally, ignoring the use of scientific notation will make such equations tedious, hard to read, and even harder to remember.
Using Avogadro’s number, 1 mol of hydrogen atoms is equal to 6.02214076 × 10²³. Two mols of hydrogen, then, are equal to 2(6.02214076 × 10²³).
The number of particles in a mole is the same across elements and substances, but remember not to confuse the number with the mass. The use of mols also extends into chemical equations, but we will discuss that later on (Encyclopaedia Britannica, 2019b).
Derived Units
Now that we have a grasp on the five primary SI units in chemistry, let us take a brief look at 3 units that have been derived from them: volume,