A \(1.0-\mathrm{m}^{2}\) solar panel on a satellite that keeps the panel oriented perpendicular to radiation arriving from the Sun absorbs $1.4 \mathrm{kJ}\( of energy every second. The satellite is located at \)1.00 \mathrm{AU}\( from the Sun. (The Earth Sun distance is defined to be \)1.00 \mathrm{AU} .$. How long would it take an identical panel that is also oriented perpendicular to the incoming radiation to absorb the same amount of energy, if it were on an interplanetary exploration vehicle 1.55 AU from the Sun? ( W) tutorial: sunlight on Io).

Short Answer

Expert verified
Answer: It takes approximately 2.405 seconds for the solar panel at a distance of 1.55 AU to absorb the same amount of energy as the one at a distance of 1.00 AU.

Step by step solution

01

Calculate the initial intensity

First, we will find the intensity of the sunlight per square meter when the solar panel is at a distance of 1.00 AU from the sun. Intensity (I) is given by the power (P) divided by the area (A). The absorbed energy is given as 1.4 kJ per second. Therefore, the power absorbed is P_absorbed = 1.4 kW. The area of the solar panel is given as A = 1.0 m². Now, we can calculate the intensity I_initial, I_initial = P_absorbed / A = (1.4 kW) / (1.0 m²) = 1.4 kW/m².
02

Calculate the ratio of intensities

Next, we need to find the ratio of the intensities when the panel is at 1.00 AU and 1.55 AU. The inverse square law dictates that the intensity is inversely proportional to the square of the distance. Thus, Intensity ratio = (I_initial / I_final) = (distance_final² / distance_initial²) = (1.55 AU / 1.00 AU)² = (1.55)² = 2.4025
03

Calculate the final intensity

Now, we can find the intensity of the sunlight when the solar panel is at a distance of 1.55 AU from the sun. I_final = I_initial / Intensity ratio = 1.4 kW/m² / 2.4025 = 0.5824 kW/m²
04

Calculate the power absorbed by the solar panel at the new distance

Next, we will calculate the power (P_final) absorbed by the solar panel when it is at a distance of 1.55 AU from the sun. P_final = I_final * A = (0.5824 kW/m²) * (1.0 m²) = 0.5824 kW
05

Calculate the time taken to absorb the same amount of energy at the new distance

Finally, we will determine the time (t) it would take for the solar panel to absorb the same amount of energy when it is at a distance of 1.55 AU from the sun. Energy_absorbed = P_initial * t_initial = P_final * t_final Using the given values of P_initial = 1.4 kW and P_final = 0.5824 kW, t_final = (P_initial * t_initial) / P_final = (1.4 kW * 1 s) / 0.5824 kW ≈ 2.405 s It would take about 2.405 seconds for the solar panel at a distance of 1.55 AU from the sun to absorb the same amount of energy as the one at a distance of 1.00 AU.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

How long does it take light to travel from this text to your eyes? Assume a distance of \(50.0 \mathrm{cm}\).
A star is moving away from Earth at a speed of $2.4 \times 10^{8} \mathrm{m} / \mathrm{s} .\( Light of wavelength \)480 \mathrm{nm}$ is emitted by the star. What is the wavelength as measured by an Earth observer?
A polarized beam of light has intensity \(I_{0} .\) We want to rotate the direction of polarization by \(90.0^{\circ}\) using polarizing sheets. (a) Explain why we must use at least two sheets. (b) What is the transmitted intensity if we use two sheets, each of which rotates the direction of polarization by \(45.0^{\circ} ?\) (c) What is the transmitted intensity if we use four sheets, each of which rotates the direction of polarization by \(22.5^{\circ} ?\)
Vertically polarized light with intensity \(I_{0}\) is normally incident on an ideal polarizer. As the polarizer is rotated about a horizontal axis, the intensity \(I\) of light transmitted through the polarizer varies with the orientation of the polarizer \((\theta),\) where \(\theta=0\) corresponds to a vertical transmission axis. Sketch a graph of \(I\) as a function of \(\theta\) for one complete rotation of the polarizer $\left(0 \leq \theta \leq 360^{\circ}\right)$.(W) tutorial: polarized light).
The magnetic field of an EM wave is given by \(B_{y}=\) $B_{\mathrm{m}} \sin (k z+\omega t), B_{x}=0,\( and \)B_{z}=0 .$ (a) In what direction is this wave traveling? (b) Write expressions for the components of the electric field of this wave.
See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free