Understanding Our Universe
3rd Edition
ISBN: 9780393614428
Author: PALEN, Stacy, Kay, Laura, Blumenthal, George (george Ray)
Publisher: W.w. Norton & Company,
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Chapter 16, Problem 19QAP
To determine
The reason why CMB looks like the spectrum of blackbody at low temperature of
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What has occurred after the Big Bang?
Objects in the universe have reached a critical density.
Objects that were once close together have moved apart as space expanded.
Space expanded without affecting the distances between objects.
Objects that were once close together have expanded apart into already existing space.
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Which of the following did NOT happen during the first few minutes after the Big Bang?
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O matter and antimatter collided and turned into energy
O two or three of the simplest elements fused together
O temperatures throughout the universe were hotter than the cores of stars are today
some very massive early stars formed
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O energy was converted to matter
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The cosmic microwave background consists of:
huge clouds of dark matter interspersed with equally huge clouds of H and He
enormous cold voids separating warmer filaments of young protostas and
protogalaxies
denser areas of slightly warmer Hydrogen mixed with slightly less dense areas
of slightly cooler Helium
an enormous number of photons, particles of light that emerged after the Big
Bang
atoms of H and He, dark matter, and an immense amount of energy
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Chapter 16 Solutions
Understanding Our Universe
Ch. 16.1 - Prob. 16.1CYUCh. 16.2 - Prob. 16.2CYUCh. 16.3 - Prob. 16.3CYUCh. 16.4 - Prob. 16.4CYUCh. 16.5 - Prob. 16.5CYUCh. 16.6 - Prob. 16.6CYUCh. 16 - Prob. 1QAPCh. 16 - Prob. 2QAPCh. 16 - Prob. 3QAPCh. 16 - Prob. 4QAP
Ch. 16 - Prob. 5QAPCh. 16 - Prob. 6QAPCh. 16 - Prob. 7QAPCh. 16 - Prob. 8QAPCh. 16 - Prob. 9QAPCh. 16 - Prob. 10QAPCh. 16 - Prob. 11QAPCh. 16 - Prob. 12QAPCh. 16 - Prob. 13QAPCh. 16 - Prob. 14QAPCh. 16 - Prob. 15QAPCh. 16 - Prob. 16QAPCh. 16 - Prob. 17QAPCh. 16 - Prob. 18QAPCh. 16 - Prob. 19QAPCh. 16 - Prob. 20QAPCh. 16 - Prob. 21QAPCh. 16 - Prob. 22QAPCh. 16 - Prob. 24QAPCh. 16 - Prob. 25QAPCh. 16 - Prob. 26QAPCh. 16 - Prob. 27QAPCh. 16 - Prob. 28QAPCh. 16 - Prob. 29QAPCh. 16 - Prob. 30QAPCh. 16 - Prob. 31QAPCh. 16 - Prob. 32QAPCh. 16 - Prob. 33QAPCh. 16 - Prob. 34QAPCh. 16 - Prob. 35QAPCh. 16 - Prob. 36QAPCh. 16 - Prob. 37QAPCh. 16 - Prob. 38QAPCh. 16 - Prob. 39QAPCh. 16 - Prob. 40QAPCh. 16 - Prob. 41QAPCh. 16 - Prob. 42QAPCh. 16 - Prob. 43QAPCh. 16 - Prob. 44QAPCh. 16 - Prob. 45QAP
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- Theory predicts that the irregularities in the hot gas of the big bang should be how many degrees in diameter if the universe is flat? a. 0.01 degree b. 1 degree c. 5 degrees d. 10 degrees e. 20 degreesarrow_forwardThe Analysis of the Big Bang Theory.arrow_forwardAfter the Big Bang the Universe expanded and cooled. What was the temperature of the Universe when it became transparent 380,000 years after the Big Bang? Group of answer choices 100 billion K 1 billion K 10 million K 3,000 Karrow_forward
- The light coming from stars is closer to red (long wavelength, low frequency) than we would expect. What does this imply? Your answer: the universe is expanding the universe is rotating the universe is shrinking the universe is staticarrow_forwardWhat are the three important pieces of evidence that led scientists to accept the Big Bang as the most likely model for the origin of the universe?arrow_forwardIn the context of the Big Bang theory, cosmic inflation refers to: A. A rapid expansion of the universe in its early stages. B. The steady increase in the temperature of the universe. C. The formation of galaxies from primordial gas clouds. D. The eventual collapse of the universe.arrow_forward
- Does Hubble's Law work well for galaxies in the Local Group (such as Andromeda)? No, because dark energy is accelerating the universe's expansion over those distances. No, because we do not know the precise value of Ho. No, because Hubble did not know the Local Group existed when he discovered his law. Yes, it works well for all galaxies. No, because galaxies in the Local Group are bound gravitationally together.arrow_forwardPlace all of the following in order from earliest to the most recent: Dark energy begins acceleration of the expansion of the universe You study for your final in astronomy Last scattering of the Cosmic Microwave Background Radiation First stars and galaxies form Big Bang Universe becomes transparent (no longer opaque) aka photon decoupling time Inflationary Epoch Formation of first complex elements (hydrogen isotopes, helium & lithium)arrow_forwardThe objects that are detected at the points where the gas of a radio jet hits the extragalactic medium are called a. quasars. b. Herbig–Haro objects. c. Dyson spheres. d. hot spots.arrow_forward
- The cosmic "dark ages" represent that time in the history of the universe when: the inflation of a singularity in the first trillionth of a trillionth of a second of time when matter and energy were interchangeable and darkness prevailed atoms of H and He had not formed yet, so the dark ages represent the time just before the release of the cosmic microwave background dark energy came into being around 5 to 6 billion years ago, accelerating the expansion of the universe the light of the cosmic microwave background began to dim and stars and galaxies had yet to form photons of light energy were trapped within a plasma of H and He nuclei and loose electrons, creating a foggy, opaque universe MacBook Airarrow_forwardIf the Hubble constant equals 70 km/s/Mpc, the age of the universe roughly equals a. 6 billion years. b. 10 billion years. c. 12 billion years. d. 14 billion years. e. 20 billion years.arrow_forwardGalaxy seeds around which galaxies, clusters, and walls grew may have been a. caused by hot dark matter. b. caused by baryons. c. the result of the separation of the electromagnetic and weak forces. d. the result of freezing water molecules shortly after the universe became transparent to photons. e. caused by microscopic random fluctuations in the infant universe.arrow_forward
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