Cosmic Perspective Fundamentals
3rd Edition
ISBN: 9780134988504
Author: Bennett, Jeffrey O., Donahue, M. (megan), SCHNEIDER, Nicholas, Voit, Mark
Publisher: Pearson,
expand_more
expand_more
format_list_bulleted
Concept explainers
Textbook Question
Chapter 12, Problem 4QQ
Choose the best answer to each of the following. Explain your reasoning.
According to Lcavitt’s law, we can determine the luminosity of a Cepheid in a distant galaxy by (a) measuring its parallax. (b) measuring its period of brightening and dimming. (c) measuring its recession speed.
Expert Solution & Answer
Want to see the full answer?
Check out a sample textbook solutionStudents have asked these similar questions
Part 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
kpe
Astronomy question:
Answer correctly and read the questions corretly, this is all one quesiton if done correclty and organized I will write a very nice review about you!
1. How did Edwin Hubble measure the distance to the Andromeda Galaxy?
He deduced it from its redshift.
He measured its parallax.
He used Cepheid variables in the Andromeda Galaxy.
He used white dwarf supernovae in the Andromeda Galaxy.
Please answer this within 30 mins to get a thumbs up! Please show neat and clean work . Thank you !
Chapter 12 Solutions
Cosmic Perspective Fundamentals
Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Prob. 2QQCh. 12 - Prob. 3QQCh. 12 - Choose the best answer to each of the following....Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Choose the best answer to each of the following....
Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Choose the best answer to each of the following....Ch. 12 - Prob. 13SEQCh. 12 - Explain all answers clearly, with complete...Ch. 12 - Explain all answers clearly, with complete...Ch. 12 - Explain all answers clearly, with complete...Ch. 12 - Explain all answers clearly, with complete...Ch. 12 - Explain all answers clearly, with complete...Ch. 12 - Explain all answers clearly, with complete...Ch. 12 - Explain all answers clearly, with complete...
Additional Science Textbook Solutions
Find more solutions based on key concepts
8. What is an advantage of using chlorine gas to disinfect drinking water supplies?
It provides residual protec...
Conceptual Physical Science (6th Edition)
The height to which object can be lifted.
Physics (5th Edition)
9. Blocks with masses of 1 kg, 2 kg, and 3 kg are lined up in a row on a frictionless table. All three are push...
Physics for Scientists and Engineers: A Strategic Approach with Modern Physics (4th Edition)
The setup depicted in Figure 4.6 is used in a diffraction experiment using X-rays of 0.26 nm wavelength. Constr...
Modern Physics
An ideal diatomic gas, in a cylinder with a movable piston, undergoes the rectangular cyclic process shown in F...
An Introduction to Thermal Physics
What class of motion, natural or violent, did Aristotle attribute to motion of the Moon?
Conceptual Physics (12th 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
- I need help with one circledarrow_forwardexplain each physics formula by saying what each variable means/stands for and explain the formula as a whole, please.arrow_forwardState the definition for a parsec, and derive its value in terms of As- tronomical Units. Convert your answer for the value of the distance of a parsec in Astronomical Units into light years. Be sure to include a large and clearly labeled diagram showing how you arrived at your conclusions. Be sure to show all work!arrow_forward
- Question B1 [This question will required roughly two single-sided A4 pages to answer.] Consider a hypothetical, spherically symmetric star of mass M and radius R, for which the den- sity profile is represented by p(r) = Pc [1 − (r/R)²], where pc is the central density and r is the radial distance from the center of the star. a) If the star is in hydrostatic equilibrium, by considering the forces acting on a volume ele- ment, show that the following expression must apply: dP dr Gm(r) p 12 where P is the pressure as a function of radial position and m(r) is the mass interior to the radius r. b) For the hypothetical star, with the given density as a function of radius p(r) = pc [1-(r/R)²], show that m(r) can be written as m(r) = 1½πr³ p 31.2 5R² c) Show that the average density p of the star (i.e., total mass divided by total volume) is given by p = 0.4pc. d) e) Given that the pressure is zero when r = R, show that the central pressure is given by Pe= 15 G M² 16π R4 ΜΗ The star is…arrow_forwardUsing MBH = 6.6 × 10 Mo, calculate the below. a. Find radius of the Schwarzschild sphere (Schwarzschild radius Rs). You can calculated from the appropriate formula or just use the fact that for an object of 1 solar mass Rs = 3 km. b. Express Rs in km, in AU, in parsecs. c. Using the distance to M87 and your result above, find angular radius of the SMBH (Schwarzschild radius). Express it in arcseconds (") and micro- arcseconds (pas) d. Take the radius of Pluto's orbit equal to 40 AU and find its angular size (in micro-arcseconds, pas) at the distance of M87.arrow_forwardPlease 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_forward
- 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 yearsarrow_forwardfor 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_forwardPlease help me answer part A and Barrow_forward
- detail answer please i will give you 2 likes on answerarrow_forwardPlease answer each and every question. Please double check your work and DO NOT SKIP ANY STEPS! Include appropriate notes next to each formula and make sure to include allllll work. Thank you!arrow_forwardPlease only do part III . The second variation! it's in the blue box! please show all the work! Thanks so much!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