WebEach second, the burning Sun's mass Astronomy Question 1 1.5 out of 1.5 points Arrange the following features of our Solar System from closest to the Sun (#1) to farthest from … WebThe sun provides four benefits These benefits are: 1. heat energy. 2. light energy. 3. photosynthesis in plants. 4. a distance just right for us to live comfortably. Heat energy. …
Solved 1. Energy generation in the Sun, The principal - Chegg
Web1,391,000 km. 109 times Earth's diameter. Sun. By human standards, the Sun is eternal. It rises in the east every morning, sets in the west every evening, and shines brightly as it … WebEach second, the burning Sun's mass A)decreases. B)increases. C)remains unchanged. Q11: With daytime temperatures that can reach 430°C, why is nighttime on Mercury so cold? A)Because the year is so short, there isn't enough time for the heat to build up in the equatorial regions. B)With very little atmosphere, heat is quickly lost back into space. how far will you go for fantastic delites
THE SUN
WebExpert Answer. 1. Energy generation in the Sun, The principal energy-producing reaction in the Sun fuses four protons into a helium nucleus. Four protons, each with mass 1.0079 amu, form a helium nucleus with mass 4.0026 amu (1 arnu = 1 atomic mass unit = 1.66 x 10-22 kg). (1) How much mass in kg is lost in the creation of a single helium nucleus? WebThe End Of The Sun. The Helium Flash. The beginning of the end for a red giant the mass of our Sun occurs very suddenly. As the helium "ashes" continue to pile up at its center, a higher fraction of them turn electron-degenerate. It is an odd paradox: even as the outer layers of a red giant star are expanding into a huge but tenuous cloud, its ... WebThe inner core. Nebular theory pertains to the formation of the. solar system. The predominant gas in the atmosphere of Venus is. carbon dioxide. Most meteors seen as … high country no deposit code