The outward pressure of hot gas in the sun

WebbThe pressure is also greater when the molecules or atoms are moving faster. Since the molecules move faster when the temperature is hotter, higher temperatures produce … WebbThe outward pressure of hot gas in the Sun A) is increasing the Sun's diameter. B) is balanced by the inward gravitational pressure. C) is cooling the photosphere. D) is …

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Webb20 aug. 2024 · In the Sun’s core, nuclear fusion takes place. It produces the energy that reaches Earth. The fusion reactions convert hydrogen nuclei into helium nuclei. The … Webb8) The outward pressure of hot gas in the Sun A) is balanced by the inward gravitational pressure. B) is increasing the Sun's diameter. C) is cooling the photosphere. D) is … daily limit of caffeine https://mindceptmanagement.com

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WebbSOLVED:The outward pressure of hot gas in the sun is VIDEO ANSWER:in this problem. First time writing the given data. So BB. is given as 10 to the power food bi Chen and E. … Webb9 apr. 2024 · The Sun is a yellow dwarf star, a hot ball of glowing gases at the heart of our solar system. Its gravity holds the solar system together, keeping everything – from the … WebbSunspots are cooler than the surrounding region of the Suns surface True The Suns size remains stable because the outward pressure of hot gas in the Sun balances the inward … daily limit of carbohydrates

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The outward pressure of hot gas in the sun

Solved Question 16 1 points Save Answer What keeps the sun

Webb12 juli 2024 · Well, that depends…. The temperature of the sun varies from around 27 million degrees Fahrenheit (15 million degrees Celsius) at the core to only about 10,000 … WebbThe Sun's temperature and pressure and the gas desnity is largest in the centre and decreases outwards. Central Temperature T c = 15 million K Central Density &rho c = 150 tons/m 3 Central Pressure P c = 10 11 atm …

The outward pressure of hot gas in the sun

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WebbThe pattern of rising hot gas cells all over the photosphere is called: Granulation The outward pressure of hot gas in the Sun: Is balanced by the inward gravitational … WebbThe New Book of Popular Science. New York: Grolier, 1996: 81. "There's pressure at the center of the sun of more than 1 million metric tons/cm sq." 9.9 × 10 8 atm. The sun is …

Webb17 feb. 2024 · The hot corrosion experiment was performed considering the influence of NaCl. To be introduced corrosive environments containing NaCl, the sample was first heated on an electric hot plate at 120 ~ 150 °C. Ultrafine droplets of mixed saturated NaCl solution and alcohol were sprayed to preheated specimens (~200 °C) by an ultrasonic … WebbThe hydrogen gas in the Sun is balanced so that it never rises upward or falls downward The Sun maintains a steady temperature This is another way of stating that the Sun …

Webb8. The outward pressure of hot gas in the Sun A) is increasing the Sun's diameter. B) is responsible for variations in the sunspot cycle. C) is balanced by the inward gravitational … WebbIn other words, the Sun doesn't explode because its forces are balanced. It also won't explode in the future because the mass of the Sun is not enough to trigger a supernova. …

WebbStellar convection occurs as currents of hot gas flow up and down through the star (Figure 3). Such currents travel at moderate speeds and do not upset the overall stability of the …

Webb8 mars 2024 · The Sun is currently a yellow dwarf. Like all stars, it began as a contracting nebula - effectively a cloud of dust and gas. As each particle has its own tiny … daily limit of bing chatWebbWhen stars the size of the Sun and larger run out of hydrogen, the outward pressure of fusion is no longer produced, and gravity causes the stellar cores to contract. Gas in the … daily limit of calciumhttp://earthguide.ucsd.edu/virtualmuseum/ita/07_2.shtml daily limit for upiWebb24 apr. 2024 · Calculations show that, in order to exert enough pressure to prevent the Sun from collapsing due to the force of gravity, the gases at its center must be maintained at … daily limit of chatgptWebb13 apr. 2024 · Self-excited horizontal oscillations are found in the center of the monolayer prior to the appearance of the coexistence state. It is observed that a molten center coexists with a solid periphery. Various structural, thermodynamic, and dynamical quantities are used to characterize the phase state. daily limit of google payWebb3 juli 2024 · How Stars Work. Like all other stars in the universe, the Sun is a huge, bright sphere of hot, glowing gas held together by its own gravity. It lives in the Milky Way … daily limit of caffeine intakeWebbSolar corona. Flare. Prominence. Solar wind. The core of the Sun is considered to extend from the center to about 0.2 to 0.25 of solar radius (140,000–170,000 kilometres … biolage root lifter