/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q16P Question: Frank D. Drake, an inv... [FREE SOLUTION] | 91影视

91影视

Question: Frank D. Drake, an investigator in the SETI (Search for Extra-Terrestrial Intelligence) program, once said that the large radio telescope in Arecibo, Puerto Rico (Fig.33-36), 鈥渃an detect a signal which lays down on the entire surface of the earth a power of only one picowatt.鈥 (a) What is the power that would be received by the Arecibo antenna for such a signal? The antenna diameter is 300m.(b) What would be the power of an isotropic source at the center of our galaxy that could provide such a signal? The galactic center is 2.2104lyaway. A light-year is the distance light travels in one year.

Short Answer

Expert verified
  1. The power received by the Arecibo antenna is 1.4x10-22w.
  2. The power of the source at the center of our galaxy is 1.11015W.

Step by step solution

01

Listing the given quantities

Antenna diameter, DA=300m.

Distance of galactic center from source, RS= 2.2x104ly.

02

Understanding the concepts of intensity and power

We equatetheintensity of the receiver and the intensity of the earth to findthepower ofthereceiver. Inthesecond case, we equate the intensity of the source to the intensity of the earth to find the power ofthesource.

03

(a) Calculations of the power received by the Arecibo antenna

The intensity of the signal on the surface of the earth and the intensity of the signal received by the antenna have to be the same.

IE=IA (1)

The intensity is nothing but power per unit area.

I=PA

Now, we can write equation 1 as,

PEAE=PAAA

Here,

AEsurfaceareaofearth=4蟺搁E2AAareaofantenna=蟺搁A2

PA=AAAEPE

Here PAis the power radiated by the antenna.

Substitute the values in the above expression, and we get,

PA=RA24RE2PE

Substitute the values in the above expression, and we get,

PA=110-12w300m2446.37106m2=1.410-22w

Thus, the power received by the Arecibo antenna is 1.410-22w.

04

(b) Calculations of the power of the source at the center of our galaxy

The intensity of the source is equal to the intensity on earth:

IE=IS (2)

The intensity is nothing but power per unit area.

I=PA

Now, we can write equation 2 as,

PEAE=PsAs

Here

AE (Surface area of earth)= 4RE2

AS (area of source) =4RS2

Ps=AsAEPE

Here Psis the power of the source.

Substitute the values in the above expression, and we get,

Ps=Rs2RE2PE (3)

Here RS is the radial distance of the galactic center.

1 year = 3.154x107s.

So the distance traveled by the light in 1 year is given by,

1ly=31083.154107=9.4621015m

role="math" localid="1662984011590" RS=2.2104ly=2.21049.4621015m=20.821019m

Substitute the values in the above expression (3), and we get,

PS=110-12w20.821019m26.37106m2=1.11015w

Thus, the power of the source at the center of our galaxy is 1.11015w.

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 91影视!

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

Two polarizing sheets, one directly above the other, transmit p% of the initially unpolarized light that is perpendicularly incident on the top sheet. What is the angle between the polarizing directions of the two sheets?

Assume (unrealistically) that a TV station acts as a point source broadcasting isotopically at 1.0MW. What is the intensity of the transmitted signal reaching Proxima Centauri, the star nearest our solar system,4.3lyaway? (An alien civilization at that distance might be able to watchXFiles.) A light-year (ly) is the distance light travels in one year.

A certain helium鈥搉eon laser emits red light in a narrow band of wavelengths centered at632.8nm and with a 鈥渨avelength width鈥 (such as on the scale of Fig. 33-1) of0.0100nm. What is the corresponding 鈥渇requency width鈥 for the emission?

The leftmost block in Fig. 33-33 depicts total internal reflection for light inside a material with an index of refractionn1when air is outside the material. A light ray reaching point A from anywhere within the shaded region at the left (such as the ray shown) fully reflects at that point and ends up in the shaded region at the right. The other blocks show similar situations for two other materials. Rank the indexes of refraction of the three materials, greatest first.

In a region of space where gravitational forces can be neglected, a sphere is accelerated by a uniform light beam ofintensity6.0鈥尘奥/m2.The sphere is totally absorbing and has a radius of2.0mand a uniform density of5.0103鈥塳驳/尘3. What is the magnitude of the sphere鈥檚 acceleration due to the light?

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.