Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
bartleby

Concept explainers

Question
Book Icon
Chapter 22, Problem 39Q

(a)

To determine

The Schwarzschild radius for a black hole, which has a mass of 4.1×106 M, in km and astronomical units.

(a)

Expert Solution
Check Mark

Answer to Problem 39Q

Solution:

The radius is 1.2×107 km or 0.08 au.

Explanation of Solution

Given data:

Mass of the black hole is 4.1×106 M

Formula used:

The expression for the Schwarzschild radius is:

RSch=2GMc2

Here, RSch is the Schwarzschild radius, G is the gravitational constant, M is the mass of the black hole and c is the speed of light.

The conversion formula for km into au is:

1.5×108 km=1 au

The conversion formula from m to km is:

1 m=103 km

Explanation:

Consider the value of G as 6.67×1011 N.m2/kg2, c as 3×108 m/s and M as,

1.989×1030 kg.

Recall the expression for Schwarzschild radius.

RSch=2GMc2

Substitute 6.67×1011 N.m2/kg2 for G, 4.1×106M for M, 3×108 m/s for c and 1.989×1030 kg for M. Also, use the conversion formula to convert m to km.

RSch=2(6.67×1011 Nm2/kg2)(4.1×106)(1.989×1030 kg)(3×108 m/s)2=12.08×109 m×103 km1 m1.2×107 km

To convert the value of radius from km to au, use the conversion formula.

1.2×107 km=1.2×107 km×(1 au1.5×108 km)=0.08 au

Conclusion:

Therefore, the Schwarzschild radius of the black hole is 1.2×107 km or 0.08 au.

(b)

To determine

The angular diameter of a black hole, which is at a distance of 8 kpc between Earth and the center of the galaxy. If the radius of the black hole is the radius calculated in sub-part (a).

(b)

Expert Solution
Check Mark

Answer to Problem 39Q

Solution:

2×105 arcsec.

Explanation of Solution

Given data:

The distance between Earth and the center of the galaxy is 8 kpc.

Formula used:

The angular diameter can be calculated by the following expression:

α=206265Dd

Here, D is the width or linear size of the object, d is the distance to the object and α is the angular size of the object.

The conversion formula from parsec to au is:

1 pc=206265 au

Explanation:

Refer the sub-part (a) for the value of radius of black hole that is 0.8 au.

The linear size, D is twice the radius. So, the value of D is:

D=2×0.8 au=1.6 au

Recall the expression for angular diameter.

α=206265Dd

Substitute 8 kpc for d, 0.16 au for D. Also, use the conversion formula.

α=206265×(0.16 au)8000 pc×(206265 au1 pc)=2×105 arcsec

Conclusion:

The angular diameter is 2×105 arcsec.

(c)

To determine

The angular diameter of a black hole which is at a distance of 45 au between Earth and the center of the galaxy. If the radius of the black hole is the radius calculated in sub-part (a).

(c)

Expert Solution
Check Mark

Answer to Problem 39Q

Solution:

730 au.

Explanation of Solution

Given data:

The distance between Earth and the center of the galaxy is 45 au.

Formula used:

The angular diameter can be calculated as,

α=206265Dd

Here, D is the width or linear size of the object, d is the distance to the object and α is the angular size of the object.

Explanation:

Refer the sub-part (a) for the value of radius of black hole that is 0.8 au.

The linear size, D is twice the radius. So, the value of D is:

D=2×0.8 au=1.6 au

Recalling the expression for angular diameter as,

α=206265Dd

Substitute 45 au for d and 0.16 au for D.

α=206265×(0.16au)45au=730arcsec

Conclusion:

The angular diameter is 730 arcsec, and it would be visible to the naked eyes if it was not a black hole.

Want to see more full solutions like this?

Subscribe now to access step-by-step solutions to millions of textbook problems written by subject matter experts!
Students have asked these similar questions
The Tully-Fischer method relies on being able to relate the mass of a galaxy to its rotation velocity. Stars in the outer-most regions of the Milky Way galaxy, located at a distance of 50 kpc from the galactic centre, are observed to orbit at a speed vrot = 250 km s−1. Using Kepler’s 3rd Law, determine the mass in the Milky Way that lies interior to 50 kpc. Express your answer in units of the Solar mass.
A Cepheid variable in the Andromeda galaxy has a period of 22 days and a mean apparent magnitude of19.5.(a) Calculate the distance modulus of the Andromeda galaxy.(b) Given that the Andromeda galaxy is approaching the Milky Way with a velocity of 119 km/s, roughlyestimate how long before these two galaxies collide? Provide your answer in years.
An astronomical image shows two objects that have the same apparent magnitude, i.e., the same brightness. However, spectroscopic follow up observations indicate that while one is a star that is within our galaxy, at a distance dgal away, and has the same luminosity as the Sun, the other is a quasar and has 100x the luminosity of the entire Milky Way galaxy. What is the distance to the quasar? (You may assume, for this rough calculation, that the Milky Way has 1011 stars and that they all have the luminosity as the Sun.) Give your response in Mpc. Value: dgal = 49 pc
Knowledge Booster
Background pattern image
Physics
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.
Similar questions
SEE MORE QUESTIONS
Recommended textbooks for you
Text book image
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax
Text book image
Foundations of Astronomy (MindTap Course List)
Physics
ISBN:9781337399920
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Text book image
Stars and Galaxies (MindTap Course List)
Physics
ISBN:9781337399944
Author:Michael A. Seeds
Publisher:Cengage Learning