CHE 1: Math Prep - Scientific Notation and Significant Figures

Course Overview and Logistics

  • Course: CHE 1 (Prep for Gen Chem), Section B, UC Davis, Fall Quarter 2026.

  • Instructor: Yu Wang.

  • Lecture Schedule: Lecture 1 presented on Wednesday, 9/23.

  • Required Readings: Math Toolbox Sections 1.1 and 1.2 in the course textbook.

  • Syllabus Requirement: Review the official course syllabus thoroughly.

  • ALEKS Online Homework: Complete "Math Prep" and the assigned portion of "Chapter 1" (the remainder of Chapter 1 is covered the following Monday). Both assignments are due next Wednesday before lecture at 1:00 PM1:00\,\text{PM}.

Working with Extreme Quantities in Chemistry

  • Chemistry frequently deals with quantities that are exceptionally large or infinitesimally small, making standard decimal notation unwieldy and prone to counting errors.

  • Macroscopic Quantities of Atoms:

    • A single mole (1 mol1\,\text{mol}) of carbon contains approximately 602,200,000,000,000,000,000,000602,200,000,000,000,000,000,000 atoms (6.022×10236.022 \times 10^{23} atoms).

  • Microscopic Mass of Individual Atoms:

    • A single carbon atom has an approximate mass of 0.0000000000000000000000199 g0.0000000000000000000000199\,\text{g}.

  • Calculation of Molar Mass:

    • Finding the mass of 1 mol1\,\text{mol} of carbon requires multiplying these two extreme numbers:     (602,200,000,000,000,000,000,000 atoms)×(0.0000000000000000000000199 g/atom)≈12.0 g(602,200,000,000,000,000,000,000\,\text{atoms}) \times (0.0000000000000000000000199\,\text{g/atom}) \approx 12.0\,\text{g}

    • Writing and calculating with strings of dozens of zeros in conventional notation is inefficient and introduces counting mistakes.


Graphite and raw diamond allotropes of carbon


Bohr model diagram of a carbon atom showing 6 protons, 6 neutrons, and 6 electrons

Fundamentals of Scientific Notation

  • Purpose of Scientific Notation:

    • Replaces long strings of leading or trailing zeros with a numeric exponential power of 1010 to prevent counting errors and simplify calculations.

  • Standard Mathematical Form:

    • Any number is written as:     C×10nC \times 10^n

    • Coefficient (CC): A decimal number restricted to the interval 1≤C<101 \le C < 10. It is obtained by moving the decimal point until exactly one non-zero digit remains to the left of the decimal point.

    • Exponent (nn): A whole integer representing the exact number of places the decimal point was shifted.

  • Directional Rules for Exponent Sign:

    • When the decimal point is moved to the left, the exponent is positive (n>0n > 0).

    • When the decimal point is moved to the right, the exponent is negative (n<0n < 0).


Step-by-step decimal point shift converting 523 to scientific notation

Converting Normal Notation to Scientific Notation

  • Step 1: Categorize the Original Magnitude:

    • (a) If the number is 1010 or larger: The decimal point must move to the left, resulting in a positive exponent (n>0n > 0).

    • (b) If the number is between 11 and 1010 (1≤number<101 \le \text{number} < 10): No conversion is strictly necessary because the exponent is zero (n=0n = 0).

    • (c) If the number is smaller than 11: The decimal point must move to the right, resulting in a negative exponent (n<0n < 0).

  • Step 2: Determine the Value of nn:

    • Count the exact number of digit positions the decimal point must cross to produce a coefficient CC satisfying 1≤C<101 \le C < 10.

    • Assign the magnitude of shifts to nn, combining it with the sign identified in Step 1.

  • Practice Conversions:

    • Converting 90065.0090065.00:

    • Magnitude category: Greater than 1010, so n>0n > 0.

    • Movement: Decimal point shifts left across 44 places (0,6,5,00, 6, 5, 0) to sit after 99.

    • Result: 9.006500×1049.006500 \times 10^4.

    • Converting 0.00008340.0000834:

    • Magnitude category: Smaller than 11, so n<0n < 0.

    • Movement: Decimal point shifts right across 55 places (0,0,0,0,80, 0, 0, 0, 8) to sit after 88.

    • Result: 8.34×10−58.34 \times 10^{-5}.

    • Converting 6.36.3:

    • Magnitude category: Between 11 and 1010, so no shift is required (n=0n = 0).

    • Result: 6.36.3 (or 6.3×1006.3 \times 10^0).

Addition and Subtraction in Scientific Notation

  • Step 0: Ensure Both Numbers Are in Scientific Notation:

    • Convert all components if presented in normal decimal notation.

  • Step 1: Equalize Exponents to the Larger Exponential Power:

    • Compare exponents and convert the term with the smaller exponent to match the larger exponent.

    • Adjust the smaller number's coefficient by moving its decimal point to the left by Δn\Delta n places, where Δn=nlarger−nsmaller\Delta n = n_{\text{larger}} - n_{\text{smaller}}.

  • Step 2: Perform the Operation on Coefficients:

    • Add or subtract the coefficients (CC) directly while keeping the shared exponent (10n10^n) unchanged.

  • Step 3: Re-normalize the Exponential Power (if necessary):

    • If the resulting coefficient C≥10C \ge 10 or C<1C < 1, adjust the decimal point and exponent to return to proper scientific notation.

  • Worked Example (0.0000325+0.01230.0000325 + 0.0123):

    • Convert to scientific notation:     0.0000325=3.25×10−50.0000325 = 3.25 \times 10^{-5}     0.0123=1.23×10−20.0123 = 1.23 \times 10^{-2}

    • Align exponents to the larger value (10−210^{-2} vs. 10−510^{-5}, where −2>−5-2 > -5):

    • Difference: −2−(−5)=3-2 - (-5) = 3 places.

    • Shift the decimal point of 3.253.25 to the left by 33 digits:       3.25×10−5=0.00325×10−23.25 \times 10^{-5} = 0.00325 \times 10^{-2}

    • Add coefficients together:     (0.00325×10−2)+(1.23×10−2)=(0.00325+1.23)×10−2=1.23325×10−2(0.00325 \times 10^{-2}) + (1.23 \times 10^{-2}) = (0.00325 + 1.23) \times 10^{-2} = 1.23325 \times 10^{-2}

    • Check normalization: Since 1≤1.23325<101 \le 1.23325 < 10, the final result is 1.23325×10−21.23325 \times 10^{-2}.

Multiplication and Division in Scientific Notation

  • Step 0: Convert Terms to Scientific Notation:

    • Put all terms into standard C×10nC \times 10^n format.

  • Step 1: Compute Coefficients:

    • Multiply or divide the coefficients (CC) directly.

  • Step 2: Combine Exponents Using Index Laws:

    • For multiplication, add the exponents:     10n1×10n2=10n1+n210^{n_1} \times 10^{n_2} = 10^{n_1 + n_2}

    • For division, subtract the denominator exponent from the numerator exponent:     10n110n2=10n1−n2\frac{10^{n_1}}{10^{n_2}} = 10^{n_1 - n_2}

  • Step 3: Combine and Re-normalize:

    • Combine the new coefficient and power of 1010.

    • If C≥10C \ge 10 or C<1C < 1, re-normalize following the exponential adjustment rules.

  • Worked Example (0.0000325×0.01230.0000325 \times 0.0123):

    • Scientific notation conversion:     0.0000325=3.25×10−50.0000325 = 3.25 \times 10^{-5}     0.0123=1.23×10−20.0123 = 1.23 \times 10^{-2}

    • Multiply coefficients:     3.25×1.23=3.99753.25 \times 1.23 = 3.9975

    • Add exponents:     10−5×10−2=10(−5)+(−2)=10−710^{-5} \times 10^{-2} = 10^{(-5) + (-2)} = 10^{-7}

    • Combine terms:     3.9975×10−73.9975 \times 10^{-7}

    • Normalization check: Since 1≤3.9975<101 \le 3.9975 < 10, no adjustment is required.

Exponential Adjustment Rules for Non-Normalized Coefficients

  • Case 1: When Coefficient C≥10C \ge 10:

    • The decimal point must move to the left by the number of places needed to satisfy 1≤C<101 \le C < 10.

    • Each shift to the left increases the exponent (+1+1 per shift).

    • Example:     983.5×104=9.835×104+2=9.835×106983.5 \times 10^4 = 9.835 \times 10^{4 + 2} = 9.835 \times 10^6

  • Case 2: When Coefficient C<1C < 1:

    • The decimal point must move to the right by the number of places needed to satisfy 1≤C<101 \le C < 10.

    • Each shift to the right decreases the exponent (−1-1 per shift).

    • Example:     0.09835×104=9.835×104−2=9.835×1020.09835 \times 10^4 = 9.835 \times 10^{4 - 2} = 9.835 \times 10^2

Measurement Uncertainty and Significant Figures

  • Scientific Meaning vs. Mathematical Exactness:

    • In mathematics, numbers are abstract and exact. In physical science, numbers represent measurements tied to measuring instruments with finite precision.

    • Any measured number contains a limited quantity of reliably known digits plus one final estimated/uncertain digit.

  • Semi-Truck Scale Case Study:

    • A semi-truck weighs 6.8 tons6.8\,\text{tons} on a highway truck scale. Two drivers weighing a combined 130.8 kg130.8\,\text{kg} board the truck.

    • Conversion factor: 1 ton=1000 kg1\,\text{ton} = 1000\,\text{kg}, so the drivers weigh 0.1308 tons0.1308\,\text{tons}.

    • Mathematical addition: 6.8 tons+0.1308 tons=6.9308 tons6.8\,\text{tons} + 0.1308\,\text{tons} = 6.9308\,\text{tons}.

    • Scientific reality: The scale only reads to the tenths place (±0.1 ton\pm 0.1\,\text{ton}). The truck's true weight could be 6.84 tons6.84\,\text{tons} or 6.76 tons6.76\,\text{tons} (6.8??? tons6.8???\,\text{tons}).

    • Adding 0.1308 tons0.1308\,\text{tons} to an unknown hundredths and thousandths place yields an unknown value: 6.8??? tons+0.1308 tons=6.9??? tons6.8???\,\text{tons} + 0.1308\,\text{tons} = 6.9???\,\text{tons}.

    • Claiming 6.9308 tons6.9308\,\text{tons} falsely implies measurement precision that does not exist. Scientifically, 6.8 tons≠6.8000 tons6.8\,\text{tons} \ne 6.8000\,\text{tons}.


Icon showing semi-truck and two human drivers representing relative measurement precision
  • Laboratory Balance Sensitivity and Percent Yield:

    • In a chemical synthesis with a theoretical yield of 38.5412 g38.5412\,\text{g}, an experimenter collects 17 g17\,\text{g} of product on a coarse balance.

    • Calculator output:     17 g38.5412 g×100%=44.108642…%\frac{17\,\text{g}}{38.5412\,\text{g}} \times 100\% = 44.108642\ldots\%

    • If a more precise balance measures the same product as 17.1 g17.1\,\text{g}, the yield becomes 44.368105…%44.368105\ldots\%.

    • If the product weighs 16.9 g16.9\,\text{g}, the yield becomes 43.849180…%43.849180\ldots\%.

    • Retaining digits past the first two has zero scientific validity because experimental inaccuracy causes those digits to fluctuate wildly.


Laboratory glassware including graduated cylinder and volumetric flasks containing colored solutions

Rules for Identifying Significant Figures

  • Rule 1: Non-Zero Digits:

    • All non-zero digits are always significant.

  • Rule 2: Leading Zeros Before Decimal Point:

    • A zero alone in front of a decimal point is not significant (e.g., in 0.2050.205, the leading zero is merely a placeholder).

  • Rule 3: Leading Zeros After Decimal Point:

    • Zeros to the right of a decimal point but preceding the first non-zero digit are not significant placeholders (e.g., in 0.002050.00205, the first three zeros are not significant; the value has 33 significant figures: 2,0,52, 0, 5).

  • Rule 4: Trailing Zeros After Decimal Point:

    • All zeros to the right of the decimal point that appear after non-zero digits are significant (e.g., 0.20500000.2050000 has 77 significant figures).

  • Rule 5: Trailing Zeros in Whole Numbers:

    • Zeros at the end of a number to the left of an implied decimal point are not significant unless an explicit decimal point is written:

    • 2560025600 contains 33 significant figures.

    • 25600.25600. contains 55 significant figures.

  • Significant Figures in Scientific Notation:

    • Exponential multiplier terms (10n10^n) do not contribute to significant figure counts; only digits in the coefficient CC are counted.

  • Significant Figure Counting Practice:

    • 2626: Contains 22 significant figures (both non-zero digits).

    • 19628.0019628.00: Contains 77 significant figures (55 non-zero digits plus 22 trailing zeros after the decimal point).

    • 0.0034160.003416: Contains 44 significant figures (leading zeros are placeholders; 3,4,1,63, 4, 1, 6 are significant).

    • 9×10199 \times 10^{19}: Contains 11 significant figure (only the digit 99 counts; 101910^{19} is ignored).

    • 1.2407661×10−21.2407661 \times 10^{-2}: Contains 88 significant figures (all 88 digits in the coefficient are significant; 10−210^{-2} is ignored).

Calculation Rules for Significant Figures

  • Addition and Subtraction Rule:

    • Round off the final result to the same decimal place as the least precise measurement in the problem (the first uncertain digit position, or fewest decimal places).

    • Worked Practice Problem:     14.668+12.2+0.1355=27.003514.668 + 12.2 + 0.1355 = 27.0035

    • Precision breakdown:

      • 14.66814.668 has 33 decimal places (thousandths place).

      • 12.212.2 has 11 decimal place (tenths place) — this is the least precise value.

      • 0.13550.1355 has 44 decimal places (ten-thousandths place).

    • Rounding: Round 27.003527.0035 to the tenths place (11 decimal place).

    • Final Answer: 27.027.0.

  • Multiplication and Division Rule:

    • The final result must have the same number of significant figures as the measurement with the fewest significant figures in the calculation.

    • Worked Practice Problem:     (5.5×10−8)(4×1010)6.65×1045=3.30827…×10−43\frac{(5.5 \times 10^{-8})(4 \times 10^{10})}{6.65 \times 10^{45}} = 3.30827\ldots \times 10^{-43}

    • Significant figure count breakdown:

      • 5.5×10−85.5 \times 10^{-8} has 22 significant figures.

      • 4×10104 \times 10^{10} has 11 significant figure — this is the limiting precision.

      • 6.65×10456.65 \times 10^{45} has 33 significant figures.

    • Rounding: Round the unrounded output to 11 significant figure.

    • Final Answer: 3×10−433 \times 10^{-43}.

Comprehensive Practice: Circumference Flight Duration

  • Problem Statement:

    • Earth's equatorial circumference is 40,075 km40,075\,\text{km}. An aircraft travels at an average ground speed of 925 km/h925\,\text{km/h}. Calculate how many hours it takes for the aircraft to complete one full flight around the equator.

  • Step 0: Conversion to Scientific Notation:

    • Distance (dd): 40,075 km=4.0075×104 km40,075\,\text{km} = 4.0075 \times 10^4\,\text{km} (55 significant figures).

    • Speed (vv): 925 km/h=9.25×102 km/h925\,\text{km/h} = 9.25 \times 10^2\,\text{km/h} (33 significant figures).

  • Step 1: Division Formulation (t=dvt = \frac{d}{v}):

    • Divide coefficients:     4.00759.25≈0.43324324…\frac{4.0075}{9.25} \approx 0.43324324\ldots

    • Divide exponential powers of 1010:     104102=104−2=102\frac{10^4}{10^2} = 10^{4 - 2} = 10^2

    • Unadjusted intermediate expression:     0.43324324…×102 h0.43324324\ldots \times 10^2\,\text{h}

  • Step 2: Exponential Normalization:

    • Since C=0.43324324…<1C = 0.43324324\ldots < 1, shift the decimal point 11 digit to the right to obtain 4.3324324…4.3324324\ldots.

    • Decrease the exponent by 11:     102−1=10110^{2 - 1} = 10^1

    • Normalized intermediate form:     4.3324324…×101 h4.3324324\ldots \times 10^1\,\text{h}

  • Step 3: Application of Significant Figure Rules:

    • The division involves a 55-sig-fig numerator (40,07540,075) and a 33-sig-fig denominator (925925).

    • The final answer must be restricted to 33 significant figures (limited by 925 km/h925\,\text{km/h}).

    • Round 4.3324324…×101 h4.3324324\ldots \times 10^1\,\text{h} to 33 significant figures:

    • In scientific notation: 4.33×101 h4.33 \times 10^1\,\text{h}.

    • In standard decimal notation: 43.3 h43.3\,\text{h}.


Illustration of an airplane in flight circling around planet Earth along the equator