EBK CONCEPTUAL PHYSICAL SCIENCE
6th Edition
ISBN: 8220101459787
Author: Hewitt
Publisher: PEARSON
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Chapter 27, Problem 10RCQ
To determine
Which star is larger among the main sequence. Red star or Yellow star.
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If the main-sequence mass lower limit is 0.08 solar mass and the brightest main-sequence stars are 1 million times more luminous than the Sun, what is the mass range along the main sequence in the figure below? (answer in solar masses)
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The mass-luminosity relation describes the mathematical relationship between luminosity and mass for main sequence stars. It describes how a star with a mass of 4 M⊙ would have a luminosity of ______ L⊙.
If a star has a radius 1/2 that of the Sun and a temperature 4 that of the Sun, how many times higher is the star's luminosity than that of the Sun? (If it is smaller by a factor of 8, you would write 0.125 because 1/8=0.125)
If a star has a radius 2 times larger than the Sun's and a luminosity 1/4th that of the Sun, how many times higher is the star's temperature than that of the Sun? (If it is smaller by a factor of 8, you would write 0.125 because 1/8=0.125)
If a star has a surface temperature 2 times lower than the Sun's and a luminosity the same as the Sun, how many times larger is the star than the Sun? (If it is smaller by a factor of 8, you would write 0.125 because 1/8=0.125)
Chapter 27 Solutions
EBK CONCEPTUAL PHYSICAL SCIENCE
Ch. 27 - What are constellations?Ch. 27 - Why does an observer at a given location see one...Ch. 27 - Prob. 3RCQCh. 27 - Is the light-year a measurement of time or...Ch. 27 - Prob. 5RCQCh. 27 - Prob. 6RCQCh. 27 - What is an H-R diagram?Ch. 27 - Prob. 8RCQCh. 27 - Prob. 9RCQCh. 27 - Prob. 10RCQ
Ch. 27 - Prob. 11RCQCh. 27 - Prob. 12RCQCh. 27 - Prob. 13RCQCh. 27 - Prob. 14RCQCh. 27 - Prob. 15RCQCh. 27 - Prob. 16RCQCh. 27 - Prob. 17RCQCh. 27 - Prob. 18RCQCh. 27 - Prob. 19RCQCh. 27 - Why dont we think the Sun will eventually become a...Ch. 27 - How does the mass of a star before its collapse...Ch. 27 - If black holes are invisible, what is the evidence...Ch. 27 - Prob. 23RCQCh. 27 - What type of galaxy is the Milky Way?Ch. 27 - What are the consequences of galaxies colliding?Ch. 27 - What is a starburst galaxy?Ch. 27 - Prob. 27RCQCh. 27 - How many spiral galaxies are in the Local Group?Ch. 27 - Is the Local Group a relatively small or large...Ch. 27 - Prob. 30RCQCh. 27 - Prob. 34TASCh. 27 - The brightest star in the sky, Sirius, is about 8...Ch. 27 - If you were to travel straight up from the core of...Ch. 27 - Prob. 37TASCh. 27 - Prob. 38TASCh. 27 - Prob. 39TASCh. 27 - Prob. 40TARCh. 27 - Prob. 41TARCh. 27 - Prob. 42TARCh. 27 - Prob. 43TARCh. 27 - Rank the nuclear fuels in order of being consumed,...Ch. 27 - Prob. 45TARCh. 27 - Rank in order of increasing size: (a) solar...Ch. 27 - The 19th-century author and social commentator...Ch. 27 - Prob. 48ECh. 27 - On the Moon, stars other than the Sun can be seen...Ch. 27 - Which figure in this chapter best shows that a...Ch. 27 - We see the constellations as distinct groups of...Ch. 27 - Prob. 52ECh. 27 - Which moves faster from horizon to horizon: the...Ch. 27 - Prob. 54ECh. 27 - Why does the Big Dipper change its position in the...Ch. 27 - Prob. 56ECh. 27 - Prob. 57ECh. 27 - Prob. 58ECh. 27 - Why dont we see the ultraviolet color of stars?Ch. 27 - Does a blue star contain yellow light?Ch. 27 - Does a yellow star contain blue light?Ch. 27 - Prob. 62ECh. 27 - Prob. 63ECh. 27 - Prob. 64ECh. 27 - Prob. 65ECh. 27 - Prob. 66ECh. 27 - Prob. 67ECh. 27 - Prob. 68ECh. 27 - Prob. 69ECh. 27 - Prob. 70ECh. 27 - Prob. 71ECh. 27 - Prob. 72ECh. 27 - Prob. 73ECh. 27 - Prob. 74ECh. 27 - Prob. 75ECh. 27 - What evidence suggests that our Sun is a...Ch. 27 - Prob. 77ECh. 27 - Prob. 78ECh. 27 - Prob. 79ECh. 27 - Prob. 80ECh. 27 - Prob. 81ECh. 27 - Prob. 82ECh. 27 - Prob. 83ECh. 27 - Prob. 84ECh. 27 - Prob. 85ECh. 27 - Prob. 86ECh. 27 - Prob. 87ECh. 27 - What is the difference between a black hole's...Ch. 27 - Prob. 89ECh. 27 - Prob. 90ECh. 27 - Prob. 91ECh. 27 - Are there galaxies other than the Milky Way that...Ch. 27 - Prob. 93ECh. 27 - Prob. 94ECh. 27 - Draw an analogy between a galaxy and a forest.Ch. 27 - Draw an analogy between a galaxy and a swarm of...Ch. 27 - Compare and contrast astronomy and astrology.Ch. 27 - Project what human civilization would be like if...Ch. 27 - Prob. 99DQCh. 27 - Why is it important to have a science-based...Ch. 27 - Choose the BEST answer to each of the following....Ch. 27 - Prob. 2RATCh. 27 - The star nearest Earth is (a) Proxima Centauri....Ch. 27 - Prob. 4RATCh. 27 - Prob. 5RATCh. 27 - Prob. 6RATCh. 27 - Prob. 7RATCh. 27 - A black hole is (a) an empty region of space with...Ch. 27 - Prob. 9RATCh. 27 - Prob. 10RAT
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- According to the text, a star must be hotter than about 25,000 K to produce an H II region. Both the hottest white dwarfs and main-sequence O stars have temperatures hotter than 25,000 K. Which type of star can ionize more hydrogen? Why?arrow_forwardWhat elements are stars mostly made of? How do we know this?arrow_forwardA red giant star might have radius = 104 times the solar radius, and luminosity = 1730 times solar luminosity. Use the data given below to calculate the temperature at the surface of the red giant star. Data: solar radius R = 7 x 108 meters solar luminosity L = 4 x 1026 watts Stefan-Boltzmann constant a = 5.67 x 10-8 W m² K-4 (in K) A: 1226 OB: 1434 OC: 1678 OD: 1963 OE: 2297 OF: 2688 OG: 3145 OH: 3679arrow_forward
- QUESTION 16 Use the figure shown below to complete the following statement: A low-mass protostar (0.5 to 8M the mass compared to our sun) remains roughly constant in decreases in until it makes a turn towards the main sequence, as it follows its evolutionary track. Protostars of different masses follow diferent paths on their way to the main sequence. 107 Luminosity (L) 10 105 10 107 10² 101 1 10-1 10-2 10-3 Spectral type 0.01 R 0.001 Re 60 M MAIN SEQUENCE 40,000 30,000 20 Mau 10 Mgun 5 Mun 0.1 Run Ren radius; temperature luminosity; radius 3 Min. 05 BO temperature; luminosity Oluminosity: temperature radius: luminosity 1 M 10,000 6000 Surlace temperature (K) 1,000 Rs 2 M STAR L 0.8 M B5 AO FOGO КБ МБ -10 +10 3000 Absolute visual magnitude andarrow_forwardUsing solar units, we find that a star has 4 times the luminosity of the Sun, a mass 1.25 times the mass of the Sun, and a surface temperature of 4090 K (take the Sun's surface temperature to be 5784 K for the sake of this problem). This means the star has a radius of.................... solar radii and is a .................... star (use the classification).arrow_forwardIn the H-R diagram we see that stellar masses__________ downward along the main sequence. At the upper end of the main sequence, the hot, luminous O stars can have masses as high as _________ or more times that of the Sun. On the lower end, cool, dim M stars may have as little as __________ times the mass of the Sun. Many more stars fall on the lower end of the main sequence than on the upper end, which tells us that _________stars are much more common than __________ stars.arrow_forward
- Question 41 .Suppose you are looking at H-R diagrams of two similar star clusters. The most luminous main sequence stars in the Porcini cluster are much more luminous than the most luminous main sequence stars in the Morel cluster. What can you conclude? O the Porcini cluster is younger than the Morel cluster O the Porcini cluster is farther away than the Morel cluster O the Porcini cluster is lower in metallicity than the Morel cluster O the Porcini cluster is larger in diameter than the Morel clusterarrow_forwardUsing the Hertzsprung-Russell diagram match theletter with the type of star that is located at that position. 1) A class M main sequence star2) A supergiant star3) A red giant star4) Our Sun5) A class O main sequence star6) A white dwarf stararrow_forwardAn O8 V star has an apparent visual magnitude of +5. Use the method of spectroscopic parallax to estimate the distance to the star (in pc). (Hints: Refer to one of the H–R diagrams in the chapter, and use the magnitude–distance formula, d = 10(mV − MV + 5)/5 where d is the distance in parsecs, mV and MV are the apparent and absolute visual magnitude respectively.)arrow_forward
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