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A population of 10,000 in 1960 grew to 12,000 in 1970. Estimate the population in 1980 and find the doubling time.

Mathematics

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Answers

3 parts
a

14400\text{14400}

b

38.01 years\text{38.01 years}

c
2

π3 radians or 60∘\frac{\pi}{3} \text{ radians or } 60^\circ

Step-by-step solution

6 steps

Part a· 2 steps

Step 1: Set up the exponential growth model.

The exponential growth model is given by P(t)=P0ektP(t) = P_0 e^{kt}, where P(t)P(t) is the population at time tt, P0P_0 is the initial population, and kk is the growth rate.
Given:
P0=10000P_0 = 10000 (population in 1960, which we take as t=0t=0)
P(10)=12000P(10) = 12000 (population in 1970, so t=1970−1960=10t=1970-1960=10 years)

  1. Calculate the growth rate kk.

    Substitute the values into the model:

    12000=10000ek⋅1012000 = 10000 e^{k \cdot 10}

    Divide by 10000:

    1200010000=e10k\frac{12000}{10000} = e^{10k} 1.2=e10k1.2 = e^{10k}

    Take the natural logarithm of both sides:

    ln⁡(1.2)=ln⁡(e10k)\ln(1.2) = \ln(e^{10k}) ln⁡(1.2)=10k\ln(1.2) = 10k k=ln⁡(1.2)10k = \frac{\ln(1.2)}{10}
  2. Estimate the population in 1980.

    The time from 1960 to 1980 is t=1980−1960=20t = 1980 - 1960 = 20 years.
    Substitute kk and t=20t=20 into the model:

    P(20)=10000e(ln⁡(1.2)10)⋅20P(20) = 10000 e^{\left(\frac{\ln(1.2)}{10}\right) \cdot 20} P(20)=10000e2ln⁡(1.2)P(20) = 10000 e^{2 \ln(1.2)}

    Using the logarithm property aln⁡b=ln⁡baa \ln b = \ln b^a:

    P(20)=10000eln⁡((1.2)2)P(20) = 10000 e^{\ln((1.2)^2)}

    Using the property eln⁡x=xe^{\ln x} = x:

    P(20)=10000×(1.2)2P(20) = 10000 \times (1.2)^2 P(20)=10000×1.44P(20) = 10000 \times 1.44 P(20)=14400P(20) = 14400

    The estimated population in 1980 is 14400\boxed{\text{14400}}.

Part b

38.01 years\text{38.01 years}

Step 1: Define doubling time.

The doubling time TdT_d is the time it takes for the population to double. If the initial population is P0P_0, the population after TdT_d years will be 2P02P_0.
Using the exponential growth model P(t)=P0ektP(t) = P_0 e^{kt}:

2P0=P0ekTd2P_0 = P_0 e^{kT_d} 2=ekTd2 = e^{kT_d}
  1. Solve for TdT_d.

    Take the natural logarithm of both sides:

    ln⁡2=ln⁡(ekTd)\ln 2 = \ln(e^{kT_d}) ln⁡2=kTd\ln 2 = kT_d Td=ln⁡2kT_d = \frac{\ln 2}{k}

    From part (a), we found k=ln⁡(1.2)10k = \frac{\ln(1.2)}{10}. Substitute this value:

    Td=ln⁡2ln⁡(1.2)10T_d = \frac{\ln 2}{\frac{\ln(1.2)}{10}} Td=10ln⁡2ln⁡(1.2)T_d = \frac{10 \ln 2}{\ln(1.2)}
  2. Calculate the numerical value for TdT_d.

    Using a calculator:

    ln⁡2≈0.6931\ln 2 \approx 0.6931 ln⁡1.2≈0.1823\ln 1.2 \approx 0.1823 Td≈10×0.69310.1823T_d \approx \frac{10 \times 0.6931}{0.1823} Td≈6.9310.1823T_d \approx \frac{6.931}{0.1823} Td≈38.01 yearsT_d \approx 38.01 \text{ years}

    The doubling time for the town's population is approximately 38.01 years\boxed{\text{38.01 years}}.

Part c2

Step 1: Set up the identity.

We want to express sin⁡x+3cos⁡x\sin x + \sqrt{3}\cos x in the form Rsin⁡(x+θ)R \sin(x+\theta).
Using the angle addition formula for sine, Rsin⁡(x+θ)=R(sin⁡xcos⁡θ+cos⁡xsin⁡θ)R \sin(x+\theta) = R(\sin x \cos \theta + \cos x \sin \theta).

Rsin⁡(x+θ)=(Rcos⁡θ)sin⁡x+(Rsin⁡θ)cos⁡xR \sin(x+\theta) = (R \cos \theta)\sin x + (R \sin \theta)\cos x

Comparing this to sin⁡x+3cos⁡x\sin x + \sqrt{3}\cos x:

Rcos⁡θ=1(Equation 1)R \cos \theta = 1 \quad \text{(Equation 1)} Rsin⁡θ=3(Equation 2)R \sin \theta = \sqrt{3} \quad \text{(Equation 2)}
  1. Find RR.

    Square both equations and add them:

    (Rcos⁡θ)2+(Rsin⁡θ)2=12+(3)2(R \cos \theta)^2 + (R \sin \theta)^2 = 1^2 + (\sqrt{3})^2 R2cos⁡2θ+R2sin⁡2θ=1+3R^2 \cos^2 \theta + R^2 \sin^2 \theta = 1 + 3 R2(cos⁡2θ+sin⁡2θ)=4R^2 (\cos^2 \theta + \sin^2 \theta) = 4

    Since cos⁡2θ+sin⁡2θ=1\cos^2 \theta + \sin^2 \theta = 1:

    R2(1)=4R^2 (1) = 4 R=4R = \sqrt{4}

    Since RR represents an amplitude, it must be positive:

    R=2R = 2
  2. Find θ\theta.

    Divide Equation 2 by Equation 1:

    Rsin⁡θRcos⁡θ=31\frac{R \sin \theta}{R \cos \theta} = \frac{\sqrt{3}}{1} tan⁡θ=3\tan \theta = \sqrt{3}

    Since Rcos⁡θ=1>0R \cos \theta = 1 > 0 and Rsin⁡θ=3>0R \sin \theta = \sqrt{3} > 0, θ\theta is in the first quadrant.

    θ=arctan⁡(3)\theta = \arctan(\sqrt{3}) θ=π3 radians or 60∘\theta = \frac{\pi}{3} \text{ radians or } 60^\circ

    So, sin⁡x+3cos⁡x=2sin⁡(x+π3)\sin x + \sqrt{3}\cos x = 2 \sin\left(x + \frac{\pi}{3}\right).

    The values are R=2R=\boxed{2} and θ=π3 radians or 60∘\theta=\boxed{\frac{\pi}{3} \text{ radians or } 60^\circ}.

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