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)
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Question
Chapter 29, Problem 70TE
To determine
Whether old or new stars are expected to be abundant with metals.
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Most stars (Main sequence) generate light
through the same mechanism. Because of this,
there is an empirical relation between their
mass, M, and their Luminosity, L. This relation
could be written in the form
L/Lsun = (M/Msun,
This relation is shown in the log-log diagram
below. Find the value of a and round it to the
nearest integer.
10
104
102
10-2
10-4
0.1
1.0
2.0
0.2
0.5
5.0
10.0
20.0
Mam (solar masses)
Luminosty (solar units)
If the hottest star in the Carina Nebula has a surface temperature of 51,000 K, at what wavelength (in nm) does it radiate the most energy?
Hint: Use Wien's law:
?max =
2.90 ✕ 106 nm · K
T
How does that compare with 91.2 nm, the wavelength of photons with just enough energy to ionize hydrogen?
-The wavelength calculated above is shorter than 91.2 nm. Photons at this calculated wavelength will have more than enough energy to ionize hydrogen.
-The wavelength calculated above is longer than 91.2 nm. Photons at this calculated wavelength will have more than enough energy to ionize hydrogen.
-The wavelength calculated above is shorter than 91.2 nm. Photons at this calculated wavelength will not have enough energy to ionize hydrogen.
-The wavelength calculated above is longer than 91.2 nm. Photons at this calculated wavelength will not have enough energy to ionize hydrogen.
Let’s say you’re looking for extrasolar planets. You observe a star that has a spectral shift in the line that is supposed to be at at 656.28011 nm – this star shows this line at 656.28005 nm. What is the radial velocity of star (in m/s) and in what direction in relation to you? a) 27.4 m/s, towards b) 27.4 km/s, away c) -27.4 m/s, toward d) -27.4 km/s, away
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
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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
- H II regions can exist only if there is a nearby star hot enough to ionize hydrogen. Hydrogen is ionized only by radiation with wavelengths shorter than 91.2 nm. What is the temperature of a star that emits its maximum energy at 91.2 nm? (Use Wien’s law from Radiation and Spectra.) Based on this result, what are the spectral types of those stars likely to provide enough energy to produce H II regions?arrow_forwardIn which of these star groups would you mostly likely find the least heavy-element abundance for the stars within them: open clusters, globular clusters, or associations?arrow_forwardAre supergiant stars also extremely massive? Explain the reasoning behind your answer.arrow_forward
- What elements are stars mostly made of? How do we know this?arrow_forwardAccording 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_forwardIron is unique among the elements in terms of its nuclear properties, and this gives it a decisive role in stellar evolution. Explain.arrow_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_forward: What does the H-R diagram show? Explain the main sequence of stars.arrow_forwardConsider the following question: How many times bigger than the sun would a cool star (4000K) have to be to give off the same amount of light as a sun-like star (T=6000K, R=1Rsun)?arrow_forward
- 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)arrow_forwardImagine that you are observing the light from a distant star that is located in a galaxy 100 million lightyears away from you. By analysis of the starlight received, you are able to tell that the image we see is of a 10- million-year-old star. You are also able to predict that the star will have a total lifetime of 50 million years, at which point it will end in a catastrophic supernova. a) How old does the star appear to be to us here on Earth now? b) How long will it be before we receive the light from the supernova event? c) Has the supernova already occurred? If so, when did it occur?arrow_forwardWhy do old stars have less metal compared to new ones?arrow_forward
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