Which is FALSE about Cosmic Microwave Background Radiation (CMBR)? O a. The radiation indicates that as the universe expands, it heats up. O b. It reveals that the universe is isotropic and homogeneous. O . t is the radiation footprint created by the Big Bang. O d. The radiation is most visible in the microwave part of the EM spectrum. O e. It supports the notion of the universe having no edge nor center.

Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
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Which is FALSE about Cosmic Microwave Background Radiation (CMBR)?
O a. The radiation indicates that as the universe expands, it heats up.
O b. It reveals that the universe is isotropic and homogeneous.
O c.t is the radiation footprint created by the Big Bang.
O d. The radiation is most visible in the microwave part of the EM spectrum.
O e. It supports the notion of the universe having no edge nor center.
Transcribed Image Text:Which is FALSE about Cosmic Microwave Background Radiation (CMBR)? O a. The radiation indicates that as the universe expands, it heats up. O b. It reveals that the universe is isotropic and homogeneous. O c.t is the radiation footprint created by the Big Bang. O d. The radiation is most visible in the microwave part of the EM spectrum. O e. It supports the notion of the universe having no edge nor center.
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If Mercury has an orbital period of 0.241 and has an average distance of 0.387 from the Sun, how will you
llustrate the Kepler's third law of Planetary Motion in an equation?
(0.241)² = (0.387)?
Eb. (0.241)² = (0.387)³
(0.241)³ = (0.387)³
od (0.241)? = (0.387)
O• (0.241) = (0.387)²
More
Transcribed Image Text:3:39 ull Done Edit If Mercury has an orbital period of 0.241 and has an average distance of 0.387 from the Sun, how will you llustrate the Kepler's third law of Planetary Motion in an equation? (0.241)² = (0.387)? Eb. (0.241)² = (0.387)³ (0.241)³ = (0.387)³ od (0.241)? = (0.387) O• (0.241) = (0.387)² More
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