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 115TDI
To determine
To find:
The reason why then should we continue to keep looking for answers.
Expert Solution & Answer
Want to see the full answer?
Check out a sample textbook solutionStudents have asked these similar questions
You record the spectrum of a distant star using a telescope on the ground on Earth. Upon
analysing the spectrum, you discover absorption lines spaced at intervals typical of oxygen
atoms. Which of the following are possible interpretations of this evidence? Select all that
apply.
The width of the spectral lines gives the diameter of the star
The star is likely orbited by habitable planets with breathable atmospheres.
The height of the spectral lines above the star's general blackbody spectral curve tells us how much
oxygen is in the star
The atmosphere of Earth contains oxygen
The red or blueshift of the set of lines can tell us the speed of the star's motion toward or away from us
Please Box the final answers. Thank you!
Please help me with this. No long answers, plz just get straight to the point and briefly explain why. Also make sure to use the information from the table and not the internet as they are different. Thanks
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
- Suppose astronomers discover a radio message from a civilization whose planet orbits a star 35 lightyears away. Their message encourages us to send a radio answer, which we decide to do. Suppose our governing bodies take 2 years to decide whether and how to answer. When our answer arrives there, their governing bodies also take two of our years to frame an answer to us. How long after we get their first message can we hope to get their reply to ours? (A question for further thinking: Once communication gets going, should we continue to wait for a reply before we send the next message?)arrow_forwardI need the answer for question 4arrow_forwardExplain the Higher-Order Systems?arrow_forward
- The Apollo program (not the lunar missions with astronauts) being conducted at the Apache Point Observatory uses a 3.5 - m telescope to direct lasers at retro-reflectors left on the Moon by the Apollo astronauts. the Moon is 384, 472 km away approximately how long do the operators need to wait to see the laser light return to Earth? (Hint: The speed of light is 300,000 km/s.]arrow_forwardYour friends are talking about Olber's Paradox: Friend 1: When the universe was quite young, it was also quite small, and therefore light was trapped inside the universe. This is why we don't see light from the edge of the universe in every direction. Friend 2: No, Olber's Paradox describes only light from stars, not from galaxies, and why you can't use light from distant stars to see at night. Friend 3: You're both right and you're both wrong. The paradox concerns itself with the expansion of the universe, and explains why light from the early universe was able to be released. Are any of them right, in part or in whole?arrow_forwardWhich of the following is least reasonable regarding the "water hole"? Group of answer choices It consists of frequencies which are greater than the frequencies of atmospheric emissions. It relates to the natural frequencies of vibration of hydroxyl (OH) and hydrogen (H), respectively. It occurs in that part of the electromagnetic spectrum where the galactic "noise" from stars and interstellar clouds is minimized. It is considered the "electromagnetic oasis" for interstellar communication. It corresponds to wavelengths in the 18-21 cm range.arrow_forward
- In a globular cluster, astronomers (someday) discover a star with the same mass as our Sun, but consisting entirely of hydrogen and helium. Is this star a good place to point our SETI antennas and search for radio signals from an advanced civilization? Group of answer choices No, because such a star (and any planets around it) would not have the heavier elements (carbon, nitrogen, oxygen, etc.) that we believe are necessary to start life as we know it. Yes, because globular clusters are among the closest star clusters to us, so that they would be easy to search for radio signals. Yes, because we have already found radio signals from another civilization living near a star in a globular cluster. No, because such a star would most likely not have a stable (main-sequence) stage that is long enough for a technological civilization to develop. Yes, because such a star is probably old and a technological civilization will have had a long time to evolve and develop there.arrow_forwardMost of the stars we can see with the unaided eye in our night sky are hundreds or even thousands of lightyears away from Earth. (The very closest ones are only a few dozen lightyears away, but most are much further.) The vast majority of stars in our galaxy are many tens of thousands of lightyears away. IF intelligent life existed on planets orbiting some of these stars – and that’s a huge IF! – comment on the likelihood and practicality of (a) visiting, (b) communicating with, or (c) verifying the existence of those life forms. Describe how you might go about approaching EACH of these three tasks, or if you think they are even possible. (One or two sentences for each part would be appropriate.)arrow_forwardRadio astronomy involves wavelengths much longer than those of visible light, and many orbiting observatories have probed the universe for radiation of very short wavelengths. What sorts of objects and physical conditions would you expect to be associated with emission of radiation at very long and very short wavelengths? (Select all that apply.) very long wavelengths cold cold gas cosmic background radiation nuclear reactions ++ Opulsars solar corona very high-energy processes very short wavelengths cold gas cosmic background radiation nuclear reactions pulsars solar corona very high-energy processesarrow_forward
- In Table 2, there is a list of 15 planets, some of which are real objects discovered by the Kepler space telescope, and some are hypothetical planets. For each one, you are provided the temperature of the star that each planet orbits in degrees Kelvin (K), the distance that each planet orbits from their star in astronomical units (AUs) and the size or radius of each planet in Earth radii (RE). Since we are concerned with finding Earth-like planets, we will assume that the composition of these planets are similar to Earth's, so we will not directly look at their masses, rather their sizes (radii) along with the other characteristics. Determine which of these 15 planets meets our criteria of a planet that could possibly support Earth-like life. Use the Habitable Planet Classification Flow Chart (below) to complete Table 2. Whenever the individual value you are looking at falls within the range of values specified on the flow chart, mark the cell to the right of the value with a Y for…arrow_forwardComplete answers please!arrow_forwardThe Sloan Digital Sky Survey O searches to see whether extra-terrestrial civilizations are sending any digitally recorded music our way O searches for Trans-Neptunian objects, small icy bodies in the outer solar system, whose orbits sometimes resemble Pluto's O takes images and spectra of millions of objects, to find the positions and redshifts of as many galaxies and quasars as possible J' O searches for planets around neighbor stars by looking for changing Doppler shifts in their spectra O searches for supernova remnants that could have pulsars inside and then try to find the pulsars F3 $ R F F4 V Q Search DII % 5 T F5 G ^ 6 B F6 Y H C F7 7 U 900 PrtScn N F8 J 8 Home F9 M P 9 K yapa End F10 O ) Pg 0 <arrow_forward
arrow_back_ios
SEE MORE QUESTIONS
arrow_forward_ios
Recommended textbooks for you
- Stars and Galaxies (MindTap Course List)PhysicsISBN:9781337399944Author:Michael A. SeedsPublisher:Cengage LearningFoundations of Astronomy (MindTap Course List)PhysicsISBN:9781337399920Author:Michael A. Seeds, Dana BackmanPublisher:Cengage Learning
- Stars and GalaxiesPhysicsISBN:9781305120785Author:Michael A. Seeds, Dana BackmanPublisher:Cengage LearningAstronomyPhysicsISBN:9781938168284Author:Andrew Fraknoi; David Morrison; Sidney C. WolffPublisher:OpenStaxHorizons: Exploring the Universe (MindTap Course ...PhysicsISBN:9781305960961Author:Michael A. Seeds, Dana BackmanPublisher:Cengage Learning
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
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax
Horizons: Exploring the Universe (MindTap Course ...
Physics
ISBN:9781305960961
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning