Pearson eText The Cosmic Perspective Fundamentals -- Instant Access (Pearson+)
3rd Edition
ISBN: 9780135775394
Author: Jeffrey Bennett, Megan Donahue
Publisher: PEARSON+
expand_more
expand_more
format_list_bulleted
Concept explainers
Textbook Question
Chapter 10, Problem 9QQ
Choose the best answer to each of the following. Explain your reasoning.
How would a flashing red light apppear as it fell into a black hole? (a) Its flashes would look the same. (b) Its flashes would appear bluer. (c) Its flashes would shift to the infrared part of the spectrum.
Expert Solution & Answer
Want to see the full answer?
Check out a sample textbook solutionStudents have asked these similar questions
Please answer the LAST THREE QUESTIONS USING THE VALUES PROVIDED. PLEASE DO NOT SKIP ANY STEPS AND COMPLETELY EXPLAIN YOUR ANSWER. I have submitted this question now FOUR times and have gotten different answers each time.
Please make sure to answer ALL question in terms of AU where appropriate!!
Please double check your work, and please make sure you fully undrestand the question before you undertake the problem.
For the given black hole, its Schwarzschild radius is
Rs=2.94814×109 m
perihelion =0.3941 AU
aphelion = 0.4927 AU
The semi-major is calculated using the formula
a = (0.492+0.3942)/2
a = 0.443 AU
The time it takes for a cloud 106,000 AU in radius
to collapse in "free-tall to form a new star is half
the time it would take for an object to orbit the star
on an extremely elliptical orbit with a semimajor
axis of 53,000 AU (half the 106.000 AU radius).
Part A
Use Kepler's third law to find the collapse time, assuming the star has the same mass as the Sun.
Express your answer in years to two significant figures.
VE ΑΣΦΑ
t=
Submit
Provide Feedback
Request Answer
years
Match each characteristic below to the appropriate stellar end state.
(Select W-White dwarf, N-Neutron star, B-Black hole. If the first is W and the rest N, enter
WNNNNNNN).
A) Has a mass no greater than 1.4 solar-masses.
B) Sometimes appears as a pulsar.
C) Size defined by its Schwarzschild radius.
D) In a binary system it can explode as a supernova.
E) Supported by electron degeneracy pressure.
F) Typically about the size of Earth.
G) Usually has a very strong magnetic field.
H) Viewed from afar, time stops at its event horizon.
Answer:
Submit All Answers
Chapter 10 Solutions
Pearson eText The Cosmic Perspective Fundamentals -- Instant Access (Pearson+)
Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Prob. 6QQCh. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....
Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Explain all answers clearly, with complete...Ch. 10 - Explain all answers clearly, with complete...Ch. 10 - Prob. 15SEQCh. 10 - Prob. 16SEQCh. 10 - Prob. 17SEQCh. 10 - Prob. 18SEQCh. 10 - Prob. 19SEQCh. 10 - Explain all answers clearly, with complete...Ch. 10 - Explain all answers clearly, with complete...Ch. 10 - Prob. 22SEQ
Additional Science Textbook Solutions
Find more solutions based on key concepts
Discuss how potential difference and electric field strength are related. Give an example.
University Physics Volume 2
(I) A solar cooker, really a concave mirror pointed at the Sun, focuses the Sun’s rays 18.8 cm in front of the ...
Physics for Scientists and Engineers with Modern Physics
42. A solid copper disk has a radius of 0.2 m, a thickness of 0.015 m, and a mass of 17 kg. (a) What is the mom...
College Physics (10th Edition)
A rocket takes off from Earth and reaches a speed of 100 m/s in 10.0 s. If the exhaust speed is 1500 m/s and th...
University Physics Volume 1
8. A stationary boat in the ocean is experiencing waves from a storm. The waves move at 56 km/h and have a wave...
College Physics: A Strategic Approach (3rd Edition)
Repeal Problem 59 for the case where the charge density in the slab is given by = 0|x/d|, where 0 is a constan...
Essential University Physics: Volume 2 (3rd Edition)
Knowledge Booster
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
- Please Explain The hotness of stars goes up to millions of degrees Celsius. The coldness of gases can go as low as -273.15 o C. How do you explain the absence of symmetry between hot and cold? Is it possible that there is also a limit to the hotness of any object in the universe? Show your step-by-step solutions.arrow_forwardMatch each characteristic below to the appropriate stellar end state. (Select W-White dwarf, N-Neutron star, B-Black hole. If the first is W and the rest N, enter WNNNNNNN). A) Size defined by its Schwarzschild radius. B) Typically about the size of Earth. C) Usually has a very strong magnetic field. D) In a binary system it can explode as a supernova. E) Supported by electron degeneracy pressure. F) Sometimes appears as a pulsar. G) Viewed from afar, time stops at its event horizon. H) Has a mass no greater than 1.4 solar-masses.arrow_forwardHigh Mass Stars Problem 4. Black Holes The Schwarzschild radius determines the event horizon of a black hole. Construct the equation defining this radius using the fact that the escape velocity at this radius is c (the speed of light). Use M for the black hole mass and RS for the Schwarzchild radius. (Do not simply write down the equation, show and explain the logical steps of your construction and algebra)arrow_forward
- Please explain the theory also. I need to understand the concept. Thank you in advance. A light of wavelength 620 nm is emitted from 5 Schwarzschild radii from a 20 solar mass black hole. What wavelength is observed for this light by an observer a long distance away? (The objects are not moving with respect to the observer)arrow_forwardPart A What was the distance between the points that would someday become, respectively, the center of the Milky Way Galaxy and the center of the Virgo Cluster at the time of decoupling? (The present separation is 18 Mpc.) Express your answer using two significant figures. 1ΨΕΙ ΑΣΦ ? Request Aswer Submit kpearrow_forwardKindly provide the solution to the following question using the GRASS method. Gravitational Fields - Orbital Speed question, (Unit: Gravitational, Electric, and Magnetic Fields). The images attached are the formulas for this unit and the question. Please make sure to show all your work using the GRASS (given, required, analysis, solution, and statement) method and using formulas from this unit (Gravitational, Electric, and Magnetic Fields).arrow_forward
- for question three can you solve the question directly using the formula N=N0e-t/? given that t1/2=?ln2=0.693? because I cant find it in the textbook of how you plugged in lambdaarrow_forwardFour research teams measured the rotation period of a newly detected neutron star, and what each team wrote in its team notebook is shown in the table below. Suppose a later and more reliable measurement gives 0.460 s for the period of the same star. Decide which of the earlier measurements was the most accurate, and which was the most precise. team A B C D what was written in the notebook "0.51s 0.05s" "between 0.480s and 0.490s" "0.360s + 7.0%" "0.560s" most accurate measurement O O O O most precise measurement O O O O X Śarrow_forwardPlease do not give solution in image formate thanku Q: You’ve just discovered another new X-ray binary, which we will call Hyp-X2 (“Hyp” for hypothetical). The system Hyp-X2 contains a bright, G2 main-sequence star orbiting an unseen companion. The separation of the stars is estimated to be 12 million kilometers, and the orbital period of the visible star is 5 days. Use Newton’s version of Kepler’s third law to calculate the sum of the masses of the two stars in the system. a)Express your answer in kilograms to two significant figures. b) Give your answer from the previous part in solar masses. ( Msun= 2.0 x 10 /30 kg). Express your answer as a multiple of sun’s mass to two significant figures. C) Determine the mass of the unseen companion. ( Hint: A G2 main-sequence star has a mass of 1 Msun.) Express your answer as a multiple of sun’s mass to two significant figures. The previous answer was not correct, please help mearrow_forward
- Please anwer the quesiton correctly and take your time Convert light-minutes to km by following the steps described below.1. A) What is the speed of light (300,000,000 m/s) in km/s? Note that 1 km = 1000 m.1. B)Use your answer to the previous question to find the distance traveled by light in one minute. Give your answer in millions of km. (Note that 1 million = 106).arrow_forwardPlease answer the questions in bold, thank you. What is a solar sail? and how does solar sailing work? How does a solar sail control it'd direction? How fast can it go? What is a solar sail made of, how big it has to be? What are the advantages? How expensive is it? Why do we want solar sails and where would they take us? What is the future of solar sailing and are there any existing missions? How can you relate solar sails with solar panels? How are they both like and unlike?arrow_forwardWrite a CR for the solved problem. A example of one is attached as well. The problem about the ROCK is the example CR. The problem you ARE writing a CR for is 5x^2-8x=3. Instructions below. For the CR's, claim you should answer the question of , do you get 2 real solutions, 1 real solution, or 2 complex solutions? For your reasoning you should explain how you know. Use the example attached to help you answer. hints: that plus minus sign means there are two answers. If the number under the square root is positive, you have two real solutions. If the number is negative you have two complex solutions. If the number is 0 under the square root you have 1 real number solution.arrow_forward
arrow_back_ios
SEE MORE QUESTIONS
arrow_forward_ios
Recommended textbooks for you
- College PhysicsPhysicsISBN:9781305952300Author:Raymond A. Serway, Chris VuillePublisher:Cengage LearningUniversity Physics (14th Edition)PhysicsISBN:9780133969290Author:Hugh D. Young, Roger A. FreedmanPublisher:PEARSONIntroduction To Quantum MechanicsPhysicsISBN:9781107189638Author:Griffiths, David J., Schroeter, Darrell F.Publisher:Cambridge University Press
- Physics for Scientists and EngineersPhysicsISBN:9781337553278Author:Raymond A. Serway, John W. JewettPublisher:Cengage LearningLecture- Tutorials for Introductory AstronomyPhysicsISBN:9780321820464Author:Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina BrissendenPublisher:Addison-WesleyCollege Physics: A Strategic Approach (4th Editio...PhysicsISBN:9780134609034Author:Randall D. Knight (Professor Emeritus), Brian Jones, Stuart FieldPublisher:PEARSON
College Physics
Physics
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Cengage Learning
University Physics (14th Edition)
Physics
ISBN:9780133969290
Author:Hugh D. Young, Roger A. Freedman
Publisher:PEARSON
Introduction To Quantum Mechanics
Physics
ISBN:9781107189638
Author:Griffiths, David J., Schroeter, Darrell F.
Publisher:Cambridge University Press
Physics for Scientists and Engineers
Physics
ISBN:9781337553278
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Lecture- Tutorials for Introductory Astronomy
Physics
ISBN:9780321820464
Author:Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher:Addison-Wesley
College Physics: A Strategic Approach (4th Editio...
Physics
ISBN:9780134609034
Author:Randall D. Knight (Professor Emeritus), Brian Jones, Stuart Field
Publisher:PEARSON
General Relativity: The Curvature of Spacetime; Author: Professor Dave Explains;https://www.youtube.com/watch?v=R7V3koyL7Mc;License: Standard YouTube License, CC-BY