EP COSMIC PERSPECTIVE-MOD.MASTERING
EP COSMIC PERSPECTIVE-MOD.MASTERING
9th Edition
ISBN: 9780137453481
Author: Bennett
Publisher: SAVVAS L
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Chapter 17, Problem 9EAP

What will happen to Earth as the Sun changes in the future?

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Multiple choice.   The total Sun's energy output for every second can power Earth in modern time hundreds of years several hundreds of thousands years about 50-100 years millions of years billions of years
The sun’s energy comes from nuclear reactions that fuse lighter nuclei into heavier ones, releasing energy in the process. The solar fusion process begins when two protons (the nuclei of hydrogen atoms) merge to produce a deuterium nucleus. Deuterium is the “heavy” isotope of hydrogen, with a nucleus consisting of a proton and a neutron. To become deuterium, one of the protons that fused has to turn into a neutron.  Our interest for now lies not with the nuclear physics but with the conditions that allow fusion to occur.                                                                            Before two protons can fuse, they must come into contact. However, the energy required to bring two protons into contact is considerable because the electric potential energy of the two protons increases rapidly as they approach each other. Fusion occurs in the core of the sun because the ultra-high temperature there gives the protons the kinetic energy they need to come together. a. A proton…
Even if the Earth's orbit were circular, we would still have seasons.  The reason is that     the seasons are actually caused by the tidal influence of the Moon     the Sun would still be off-center and our distance from it would still vary     the Sun would still have an annual cycle of storms and sunspots     the seasons are actually determined by the tilt of the Earth's axis
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