Thinking About a Conceptual Physics Pacing Guide?
Most teachers who pick up Hewitt's textbook realize within the first month that the book is much longer than the school year allows. You cannot teach every chapter in depth. A Conceptual Physics Pacing Guide is really just a document that tells you which chapters to cover, in what order, and roughly how many days each unit deserves. It exists because otherwise you will spend three weeks on units 1 and 2 and realize in March that you have never touched torque or thermodynamics. I built mine from scratch during my third year teaching. The first version I used was a Google Doc with color-coded rows for each chapter, estimated instructional days, suggested lab periods, and a column for quarterly assessments. That format still works fine if you keep it simple. The real utility comes from calibrating it against your actual calendar, not from finding a perfect template online.
What a Conceptual Physics Pacing Guide Actually Needs to Show
Your document should map the academic year onto the major units in the text. For a typical semester-based course covering the full book, here is the rough distribution I settled on after three years of trial and error: Measurement and Vectors — 4 days. This is non-negotiable foundation work. Do not compress this to two days because students who are weak here will struggle with everything that follows. Kinematics — 8 to 10 days including the lab. Graphing motion, relative velocity, and free fall each deserve separate attention. Many guides lump these together and then wonder why students cannot distinguish slope from area on a position-time graph.
Newton's Laws of Motion — 10 to 12 days. This is the single largest unit in most pacing guides, and for good reason. Free-body diagrams alone can consume three or four class periods before students stop drawing arrows pointing in random directions. Linear Momentum — 5 to 6 days. Conservation problems are where students either click or they do not. One poorly designed homework set can eat a full period without anyone learning anything useful. Energy — 8 to 10 days. Work, kinetic energy, potential energy, and conservation of energy. I usually spend one day specifically on energy bar charts because the physics education research community treats that as a legitimate learning target.
Get the Full Details

Rotational Motion — 6 to 8 days. Centripetal force, torque, and angular momentum. Students tend to understand this better than Newton's laws because the scenarios are more concrete, so I sometimes front-load it slightly when I need a morale boost mid-semester. Gravity and Projectiles — 4 to 5 days. Orbital motion often gets squeezed out entirely if you fall behind, so I reserve a hard cutoff date for it. Fluids — 3 to 4 days. Pascal's principle and Bernoulli's principle are short chapters. Use that time to do a proper lab rather than racing through theory.
Thermal Physics — 4 to 5 days. Temperature, heat transfer, and phase changes. This unit is easier for students but still requires conceptual clarity around what heat actually is. Wave Motion and Sound — 6 to 7 days. Standing waves, resonance, and the Doppler effect. Labs here are satisfying and worth protecting. Light and Color — 5 to 6 days. Reflection, refraction, and the electromagnetic spectrum. Ray diagrams take longer than you expect when you require students to draw them properly.
Electricity and Magnetism — 8 to 10 days. Circuit basics, Ohm's law, and magnetic fields. This is the unit most likely to run into schedule conflicts because it sits at the end of the year when energy is low and testing looms.

How to Build Your Own Without Wasting a Week
Start with your official school calendar. Mark every holiday, early dismissal, test window, and scheduled lab day. Subtract those from your total instructional days. If you teach a standard 180-day year and lose about 25 days to non-instructional time, you are working with roughly 155 days. That is your hard constraint. Next, list every lab the book suggests. Do not assume you will do them all. Pick the ones that actually reinforce the concept being taught and drop the rest. I typically run about eighteen labs across the year. Any more than that and you are spending more time cleaning up equipment than teaching physics. Assign day counts to each unit based on the estimates above, then subtract the lab days. What remains is your lecture and practice time. If the math does not fit your calendar, you need to cut units, not compress them. Compressed instruction produces students who can solve problems on Friday but cannot explain the underlying concept on Monday's quiz.
Build in two buffer weeks somewhere in the second semester. Something always goes wrong. A unit takes longer. A fire drill eats a block period. Standardized testing arrives early. Without buffers, your pacing guide becomes fiction by October.
The Problem I Faced and How I Fixed It
During my second year, I discovered that my pacing guide was technically sound but completely unusable in practice. The issue was that the first quarter always bled into two additional weeks because students could not handle the mathematical rigor of kinematics. By the time I caught up, I had no room left for rotational motion and had to skip it entirely. That was unacceptable. My workaround was to split kinematics into two phases. I taught the basic concepts and introduced the graphs in the first phase, then returned to them in the second phase specifically for problem-solving practice after students had seen force diagrams. This reversed sequence meant the algebra got easier the second time around, and the extra practice windows absorbed naturally. It added maybe two days total but prevented the domino effect that was destroying my schedule. I also started using a soft deadline system. Each unit had a firm end date, but if I hit that date with students who still had gaps, I would carry the gap forward rather than abandon the next unit. Teaching through incomplete understanding is worse than teaching the next topic with some review sprinkled in.

Things No One Tells You About Using a Pacing Guide
First, do not treat it as a contract. It is a planning document. You will revise it at least twice per year. The version you hand out in August is wrong, and knowing that in advance saves you from panic later. Second, counter-intuitively, Newton's laws are harder for students than circular motion. Students see a ball on a string and understand it needs to go somewhere. They do not see an invisible force balancing another invisible force on an inclined plane. Plan more time for forces than you think you need. Third, pacing guides fail completely in schools that operate on block scheduling without modification. If you teach 90-minute blocks instead of traditional periods, your day counts need to shift. A unit that takes ten traditional days might take six blocks because the extended time allows for deeper exploration. Do not copy a traditional pacing guide into a block schedule and expect it to work.
Fourth, if your district requires a final exam, budget two full weeks before the exam date for cumulative review. This is not optional. Students will not retain enough from September by May without structured review time, and a pacing guide that ignores this will leave you teaching new content while the exam approaches faster than expected. The most practical approach is to build your guide in a shared spreadsheet. Include columns for unit, chapter range, instructional days, lab days, assessment days, and notes. Keep the notes column honest. Write things like "students consistently need two extra days here" or "this lab can be skipped if behind." Over three years, that notes column becomes more valuable than the rest of the document. If you want a starting template, search for "Conceptual Physics Pacing Guide Google Sheets" and modify one to fit your schedule. Do not adopt someone else's day counts blindly. Adjust them to your student population, your administrative requirements, and the realities of your calendar. A pacing guide that matches your actual conditions is infinitely better than one that looks perfect on paper but breaks in week three.