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 8RCC
To determine
To find:
The position of the Sun on an H-R diagram.
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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
- 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.arrow_forwardAssuming that at the end of the He burning phase of the stellar core (r < R_core) has no H or He or other metals and is composed completely of Carbon, X=Y=0, X_c = 1 ; The envelope above the core has a normal stellar composition ( r > R_core). Calculate the length of time in years that a 1M_sol and 10M_sol star will live on the horizontal branch or the time between the start and end of the He burning phase. Assume that the normal relationship between mass and luminosity holds for horizontal branch stars. Please be as detailed as possiblearrow_forwardMost 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)arrow_forward
- What is nebulae?arrow_forwardA planetary nebula expanded in radius 0.3 arc seconds in 30 years. Doppler measurements show the nebula is expanding at a rate of 35 km/s. How far away is the nebula in parsecs? First, determine what distance the nebular expanded in parsecs during the time mentioned. Δd = vpc/sTs So we first need to convert the rate into pc/s and the time into seconds: vpc/s = vkm/s (1 pc / 3.09 x 1013km) vpc/s = ? Ts = (Tyr)(365 days/yr)(24 hrs/day)(3600 s/hr) Ts = ? s Δd= vpc/sTs Therefore, Δd = ? pcarrow_forward: What does the H-R diagram show? Explain the main sequence of stars.arrow_forward
- The best parallaxes obtained with Hipparcos have an accuracy of 0.001 arcsec. If you want to measure the distance to a star with an accuracy of 10%, its parallax must be 10 times larger than the typical error. How far away can you obtain a distance that is accurate to 10% with Hipparcos data? The disk of our Galaxy is 100,000 light-years in diameter. What fraction of the diameter of the Galaxy’s disk is the distance for which we can measure accurate parallaxes?arrow_forwardH 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_forwardAppendix J lists the stars that appear brightest in our sky. Are most of these hotter or cooler than the Sun? Can you suggest a reason for the difference between this answer and the answer to the previous question? (Hint: Look at the luminosities.) Is there any tendency for a correlation between temperature and luminosity? Are there exceptions to the correlation?arrow_forward
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