Conceptual Integrated Science
3rd Edition
ISBN: 9780135197394
Author: Hewitt, Paul G., LYONS, Suzanne, (science Teacher), Suchocki, John, Yeh, Jennifer (jennifer Jean)
Publisher: PEARSON EDUCATION (COLLEGE)
expand_more
expand_more
format_list_bulleted
Concept explainers
Question
Chapter 29, Problem 40TS
To determine
Whether it is possible for two galaxies with stars evenly distributed to pass right through each other on the basis of preceding problem.
Expert Solution & Answer
Want to see the full answer?
Check out a sample textbook solution
Students have asked these similar questions
Are the galaxies red-shifting or blue-shifting? Explain. (You may find the big-bang theory helpful). Andromeda galaxy is currently approaching our galaxy with a radial velocity of 266 km/sec. How far is our galaxy from Andromeda? (Hubble’s constant, H, is 73 km/sec/MParsec). When can the two galaxies be anticipated to collide?
Assume that we have measured the distance to a close by galaxy, with apparent magnitude
m1 = 6, to be d1 = 1Mpc. We now assume that all galaxies are similar and have therefore
the same intrinsic or absolute, luminosity. Then measuring the apparent magnitude of a second
galaxy to be m2 = 11, estimate the distance to that galaxy.
Please answer within 90 minutes.
Suppose you want to observe every galaxy within
some distance. Your enterprising assistant says that
instead you can observe every galaxy within double
the original distance. What is the ratio of the number
of galaxies you can now observe as opposed to
before? (For example, if you can observe twice as
many: 2. If you can observe half as many: 0.5)
Your answer
Chapter 29 Solutions
Conceptual Integrated Science
Ch. 29 - Why does an observer at a given location see one...Ch. 29 - Prob. 2RCCCh. 29 - Is the light-year a measurement of time or...Ch. 29 - Prob. 4RCCCh. 29 - Prob. 5RCCCh. 29 - What is an H-R diagram?Ch. 29 - Prob. 7RCCCh. 29 - Prob. 8RCCCh. 29 - Prob. 9RCCCh. 29 - Prob. 10RCC
Ch. 29 - Prob. 11RCCCh. 29 - Prob. 12RCCCh. 29 - Why don't we think the Sun will eventually become...Ch. 29 - If black holes are invisible, what is the evidence...Ch. 29 - What type of galaxy is the Milky Way?Ch. 29 - What is a starburst galaxy?Ch. 29 - How many spiral galaxies are in our Local Group?Ch. 29 - Is the universe in space, or is space in the...Ch. 29 - Prob. 19RCCCh. 29 - What is the approximate age of the universe?Ch. 29 - If we cant see dark matter, how do we know it is...Ch. 29 - What does WMAP stand for?Ch. 29 - Which is more abundantdark matter or ordinary...Ch. 29 - Why is the Drake equation limited to our galaxy?Ch. 29 - Which variable within the Drake equation make the...Ch. 29 - Prob. 28TCCh. 29 - Prob. 29TCCh. 29 - Prob. 30TCCh. 29 - Prob. 31TCCh. 29 - Rank the nuclear fuels in order of being consumed,...Ch. 29 - Rank in order of increasing size: a solar system,...Ch. 29 - Rank these elements in order of increasing...Ch. 29 - Rank the following in order of increasing...Ch. 29 - Prob. 36TSCh. 29 - If you were to travel straight up from the core of...Ch. 29 - Prob. 38TSCh. 29 - Prob. 39TSCh. 29 - Prob. 40TSCh. 29 - When can winter constellations be seen in the...Ch. 29 - Prob. 42TECh. 29 - On the Moon, stars other than the Sun can be seen...Ch. 29 - We see the constellations as distinct groups of...Ch. 29 - Distinguish between the daily and intrinsic motion...Ch. 29 - Which moves faster from horizon to horizon: the...Ch. 29 - Prob. 47TECh. 29 - Why does the Big Dipper change its position in the...Ch. 29 - Prob. 49TECh. 29 - Prob. 50TECh. 29 - Prob. 51TECh. 29 - Prob. 52TECh. 29 - Why dont we see the ultraviolet color of stars?Ch. 29 - Does a blue star contain yellow light?Ch. 29 - Does a yellow star contain blue light?Ch. 29 - Prob. 56TECh. 29 - Prob. 57TECh. 29 - Prob. 58TECh. 29 - Prob. 59TECh. 29 - Prob. 60TECh. 29 - Prob. 61TECh. 29 - Prob. 62TECh. 29 - Prob. 63TECh. 29 - Prob. 64TECh. 29 - Prob. 65TECh. 29 - Prob. 66TECh. 29 - Prob. 67TECh. 29 - Prob. 68TECh. 29 - Prob. 69TECh. 29 - Prob. 70TECh. 29 - Prob. 71TECh. 29 - Prob. 72TECh. 29 - Prob. 73TECh. 29 - Prob. 74TECh. 29 - Prob. 75TECh. 29 - Prob. 76TECh. 29 - Prob. 77TECh. 29 - Prob. 78TECh. 29 - What happens to a light beam bouncing between two...Ch. 29 - Prob. 80TECh. 29 - Prob. 81TECh. 29 - Prob. 82TECh. 29 - Prob. 83TECh. 29 - Prob. 84TECh. 29 - Are there other galaxies other than the Milky Way...Ch. 29 - Prob. 86TECh. 29 - Draw an analogy between a galaxy and a forest.Ch. 29 - Draw an analogy between a galaxy and a swarm of...Ch. 29 - How would finding microbial nonterrestrial life on...Ch. 29 - Prob. 90TECh. 29 - What is SETI? Was it a mistake for Congress to cut...Ch. 29 - Prob. 92TECh. 29 - Where did the Big Bang occur?Ch. 29 - When was most of the helium in the universe...Ch. 29 - What does the expansion of space do to light...Ch. 29 - A police officer pulls you over for speeding. He...Ch. 29 - If the universe remained hotter for a longer...Ch. 29 - No galaxy found so far is made of less than 25...Ch. 29 - Are astronomers able to point their telescopes in...Ch. 29 - A helium balloon here on Earth pops, releasing...Ch. 29 - Prob. 101TECh. 29 - Prob. 102TECh. 29 - Early astronomers such as Kepler and Newton...Ch. 29 - What force allows dark matter to clump?Ch. 29 - Why doesn't dark matter clump together as...Ch. 29 - If dark matter is affected by gravity, might there...Ch. 29 - What is one important difference between dark...Ch. 29 - The y-axis in the largest graph for Figure 29.47...Ch. 29 - Prob. 109TECh. 29 - Prob. 110TECh. 29 - Compare and contrast astronomy and astrology.Ch. 29 - Project what human civilization would be like if...Ch. 29 - Why is it important to have a science-based...Ch. 29 - Compare and contrast the Big Bang with a black...Ch. 29 - Prob. 115TDICh. 29 - Summer and winter constellations are different...Ch. 29 - Prob. 2RATCh. 29 - Prob. 3RATCh. 29 - Prob. 4RATCh. 29 - Prob. 5RATCh. 29 - Prob. 6RATCh. 29 - Prob. 7RATCh. 29 - Scientists estimate the age of our universe to be...Ch. 29 - Which of the following is not accepted evidence...Ch. 29 - Prob. 10RAT
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
- When comparing two isolated spiral galaxies that have the same apparent brightness, but rotate at different rates, what can you say about their relative luminosity?arrow_forwardGiven the ideas presented here about how galaxies form, would you expect to find a giant elliptical galaxy in the Local Group? Why or why not? Is there in fact a giant elliptical in the Local Group?arrow_forwardSuppose you want to observe the molecular gas in a galaxy with redshift z using the rotational transition of CO J=4-3. What frequency would you observe this transition at? (Hint: the CO J=1-0 emits a photon at 115.27 GHz, and higher order transitions emit photons with frequencies in multiples of J, e.g., use the knowledge you gained from the problem above). Express your answer as an integer. Values: z = 1.3arrow_forward
- Please answer within 90 minutes.arrow_forwardExplain why galaxies can have different shapes. please explain briefly and clearlyarrow_forwardAn observational survey of distant galaxies is undertaken that involves measuring their distances using cepheid variables and red-shifts using spectroscopy. Explain how cepheid variables can be used to measure the distances to galaxies. A spectral line is observed whose wavelength in the laboratory is de length of this spectral line observed in each galaxy, Xo, is listed in the table, along with the distance, d, to the galaxy. Determine the red-shift and the recession velocity of each galaxy and tabulate your results by making a copy of the table and filling in the blank spaces. Sketch a Hubble diagram using your results and determine the value of the Hubble constant Ho in units of km s-1 Mpc. 650 nm. The wave- Galaxy 1 652.69 Galaxy 2 Galaxy 3 Galaxy 4 Galaxy 5 653.01 do (nm) d (Mpc) 658.54 662.18 681.63 17 19 54 77 200 v (km s-1)arrow_forward
- Indicate whether the following statements are true or false. (Select T-True, F-False. If the first is T and the rest F, enter TFFFFF). A) The nearest large spiral Galaxy, similar in size to the Milky Way, is the Andromeda Galaxy (M31). It is located about 2 million light years from Earth. B) On very large scales, matter in the Universe is distributed in clumps and voids. C) RR Lyrae and Cepheid variable stars are used to measure the distance to nearby galaxies. D) Distances to most stars in the Milky Way are measured by parallax. E) If we find an O type star in our galaxy, it must be in the disk. F) The disk of the Milky Way galaxy is about 1,000,000 light years in diameter.arrow_forwardUse the photo to answer the question. If an observer looked out from a planet near the center of this galaxy, what would it look like to that observer? O A broad band of stars forming a ring around the planet O A sphere of stars evenly spread in every direction O A spiral shape with arms reaching out from a center O A band of stars in one direction, with fewer stars in other directionsarrow_forwardSuppose you want to observe every galaxy within some distance. Your enterprising assistant says that instead you can observe every galaxy within double the original distance. What is the ratio of the number of galaxies you can now observe as opposed to before?arrow_forward
- Using our example from the previous unit, let's try to determine the Hubble time for this example universe. You were given that a good representative galaxy receded at a speed of 4000 km/s and was found to be 20 Mpc away. With that in mind, what would the age of that universe be in years (aka what is that universe's Hubble time)? Go ahead and take the number of kilometers per Mpc to be approximately 3.1*10^19 km/Mpc. While this problem may look scary at first, this is really just bringing you full circle to one of the unit conversion problems you encountered at the beginning of this course.arrow_forwardIn the reading, you were told that there were roughly 10,000 galaxies in the image of the Hubble Ultra Deep Field alone. The image is roughly 10 square arcminutes and there are roughly 1.5*10^8 square arcminutes composing the entire sky. With that in mind and assuming that the Hubble Ultra Deep Field represents an average part of the sky, roughly how many galaxies may exist in the observable universe? (Please include commas for every factor of 1,000; for example 2,343,567,890)arrow_forwardThe figure below is based on an assumed Hubble constant of 70 km/s/Mpc. How would you change the diagram to fit a Hubble constant of 50 km/s/Mpc? If the evolution of the universe were determined only by gravity, then its fate would be linked to its geometry. Open Negligible normal matter Flat Closed 14 9.5 Past Future Time Billion years ago Now The slope of the "negligible normal matter" line would be ---Select--- C and cross the time axis ---Select--- O than 14 billion years ago. The curved line separating the open and closed universe regions would cross the time axis O than 9.5 billion years ago. ---Select--- Scale of the universe, R © Cengage Learning 2013arrow_forward
arrow_back_ios
SEE MORE QUESTIONS
arrow_forward_ios
Recommended textbooks for you
AstronomyPhysicsISBN:9781938168284Author:Andrew Fraknoi; David Morrison; Sidney C. WolffPublisher:OpenStax
Stars and Galaxies (MindTap Course List)PhysicsISBN:9781337399944Author:Michael A. SeedsPublisher:Cengage Learning
Foundations of Astronomy (MindTap Course List)PhysicsISBN:9781337399920Author:Michael A. Seeds, Dana BackmanPublisher:Cengage Learning
Stars and GalaxiesPhysicsISBN:9781305120785Author:Michael A. Seeds, Dana BackmanPublisher:Cengage Learning
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax
Stars and Galaxies (MindTap Course List)
Physics
ISBN:9781337399944
Author:Michael A. Seeds
Publisher:Cengage Learning
Foundations of Astronomy (MindTap Course List)
Physics
ISBN:9781337399920
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Stars and Galaxies
Physics
ISBN:9781305120785
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning