Concept explainers
(a)
The Schwarzschild radius and the density of a black hole which is having a mass equal to the planet Earth.
Answer to Problem 60Q
The Schwarzschild radius of the black hole which is having the mass of the planet Earth is
The density of the black hole is
Explanation of Solution
Given:
Mass of the Earth is
Radius of the Earth is
Formula Used:
Schwarzschild radius of an object can be found by using the formula
Where,
Density of an object can be found by using the formula
Calculation:
Therefore, the radius of the black hole to the event horizon
Density of the black hole,
Conclusion:
Therefore, the Schwarzschild radius of the black hole which is having the mass of the planet Earth is
(b)
The Schwarzschild radius and the density of a black hole which is having a mass equal to the Sun.
Answer to Problem 60Q
The Schwarzschild radius of the black hole which is having the mass equal to the Sun is
The density of the black hole is
Explanation of Solution
Given data:
Mass of the Sun is
Radius of the Sun is
Formula used:
Schwarzschild radius of an object can be found by using the formula
Where,
Density of an object can be found by using the formula
Calculation:
Therefore, the radius of the black hole to the event horizon
Density of the black hole
Conclusion:
Therefore, the Schwarzschild radius of the black hole which is having the mass equal to the Sun is
(c)
The Schwarzschild radius and the density of a black hole which is having a mass equal to the supermassive black hole in NGC 4261.
Answer to Problem 60Q
The Schwarzschild radius of the black hole which is having the mass of the supermassive black hole in NGC 4261 is
The density of the black hole is
Explanation of Solution
Given:
Mass of the supermassive black hole in NGC 4261 is
Radius of the supermassive black hole is
Formula used:
Schwarzschild radius of an object can be found by using the formula,
Where
Density of an object can be found by using the formula,
Calculation:
Therefore, the radius of the black hole to the event horizon
Density of the black hole,
Conclusion:
Therefore, the Schwarzschild radius of the black hole which is having the mass of the supermassive black hole in NGC 4261 is
Want to see more full solutions like this?
Chapter 21 Solutions
Universe: Stars And Galaxies
- Assume the event horizon is the size of the black hole (it is not: in reality, the black hole is a point source). What is the density of a black hole that has the mass of the Sun in units of kg/cm3? Please express your answer in scientific notation with the "e" format inside the text box, and keep three significant figures (for example, 5.01e3 for 5.01 × 103).arrow_forwardDark matter Consider the rotation curves of a galaxy with density profile p(r). Assuming that sufficiently far from the centre of the galaxy the radial speed v depends on the dis- tance from the centre of the galaxy according to the relation v(r) oc where a is a constant, determine a relation between the density and radius, up to a constant of proportionality which you do not need to determine. If there is a supermassive black hole in the centre of the galaxy with mass MSMBII, how would the velocity depend on r close to the centre of the galaxy? Ignore any relativistic effects. Which condition could you use to estimate the radius at which the velocity profile would start to deviate away from the result you derived for v(r) close to the black hole? Consider the hypothesis that dark matter could be made out of black holes which are stellar remnants. Briefly list six pieces of observational evidence for the existence of dark matter and state clearly which items on your list are compatible…arrow_forwardBlack holes radiate emission through Hawking radiation: (a) Calculate the luminosity (in W) of a 100 solar mass black hole? (b) Calculate the fractional differences in temperature and luminosity between a 100 and 10 solar mass black hole? (c) Calculate the mass of a black hole which has peak radiation at optical wavelength (500 nm)?arrow_forward
- 1.2 1.0 0.8 0.6 Cosmic background data from COBE 0.4 0.2 0.0 0.5 10 Wavelength A in mm c) Background (CMB) undertaken by the COBE satellite. Use this diagram to estimate the current temperature of the CMB. Based on your estimate, what would the temperature of the CMB have been at a redshift of z = 5000? The left hand diagram above shows the results from observations of the Cosmic Microwave Radiated Intensity per Unit Wavelength (16° Watts/m per mm)arrow_forwardAs a mass m of gas falls into a black hole, at most 0.1mc2 is likely to emerge as radiation; the rest is swallowed by the black hole. Show the Eddington luminosity for a black hole of mass M is equivalent to 2*10-9 Mc2yr-1. Explain why we expect the black hole's mass to grow by at least a factor of e every 5*107 years. Where Edding Luminicity is defined as LE=(4piGMmpc)/(sigmaT), where G is the gravitational constant, M is the mass of the black hole, mp is the mass of a proton, c is the speed of light, and sigmaT is Thomson scattering where sigmaT=6.653*10-25 cm2.arrow_forwardDistribution of Dark matter The most mass of our Milky Way is contained in an inner region close to the core with radius R0.Because the mass outside this inner region is almost constant, the density distribution can bewritten as following (assume a flat Milky Way with height z0):ρ(r) = (ρ0, r ≤ R00, r > R0(a) Derive an expression for the mass M(r) enclosed within the radius r.(b) Derive the expected rotational velocity of the Milky Way v(r) at a radius r.arrow_forward
- what is the answer for sub-item (b) if the radius of the neutron star is 6.676 km? (express your answer in the proper SI unit and without scientific notation) (b)What is the average density of a neuron star that has the same mass as the sun but a radius of only 20.0 km?arrow_forwardWhat is the orbital period (in s) of a bit of matter in an accretion disk that is located 6 ✕ 105 km from a 99 M black hole? Hint: Use the circular orbit velocity formula, Vc = GM r . sarrow_forwardDo it plzarrow_forward
- a) If you were to measure the distances and recessional velocities to nearby galaxies, you would find that they don’t fall exactly on the Hubble law, with their scatter around this law being larger for the nearest galaxies. What is the reason for this scatter? Assume that you made the measurements perfectly (i.e. that you really did measure the exact distances and velocities). b) At what distances do you expect the scatter from this effect to be about 10% of the velocity inferred from Hubble's law? What about 1%?arrow_forwardWhat is the orbital period of a bit of matter in an accretion disk that is located 4 ✕ 105 km from a 87 M black hole? Use the circular orbit velocity formula.arrow_forward10arrow_forward
- AstronomyPhysicsISBN:9781938168284Author:Andrew Fraknoi; David Morrison; Sidney C. WolffPublisher:OpenStaxPrinciples of Physics: A Calculus-Based TextPhysicsISBN:9781133104261Author:Raymond A. Serway, John W. JewettPublisher:Cengage Learning
- Foundations of Astronomy (MindTap Course List)PhysicsISBN:9781337399920Author:Michael A. Seeds, Dana BackmanPublisher:Cengage LearningStars and Galaxies (MindTap Course List)PhysicsISBN:9781337399944Author:Michael A. SeedsPublisher:Cengage LearningPhysics for Scientists and Engineers: Foundations...PhysicsISBN:9781133939146Author:Katz, Debora M.Publisher:Cengage Learning