Physics, asked by boshungmeber, 9 months ago

PLEASE I DON'T WANT ANY NONSENSE ANSWER BRAINLIEST PERSONS PLEASE ANSWER THIS NOW! Our Sun shines bright with a luminosity of 3.828 x 1026 Watt. Her energy is responsible for many processes and the habitable temperatures on the Earth that make our life possible. (a) Calculate the amount of energy arriving on the Earth in a single day. (b) To how many litres of heating oil (energy density: 37.3 x 106 J/litre) is this equivalent? (c) The Earth reflects 30% of this energy: Determine the temperature on Earth’s surface. (d) What other factors should be considered to get an even more precise temperature estimate? Note: The Earth’s radius is 6370 km; the Sun’s radius is 696 x 103 km; 1 AU is 1.495 x 108 km.

Answers

Answered by komalkukreja2609
0

Answer:

100π/3 radians/second

Explanation:

100 revolutions / min = ( 100×2π ) radians/( 60 s) = 10π/3 radians / second

In 10 seconds=100π/3 radians/secon

Answered by HariesRam
3

a)

The potential is enormous, says MIT physics professor Washington Taylor, who co-teaches a course on the physics of energy. A total of 173,000 terawatts (trillions of watts) of solar energy strikes the Earth continuously. That's more than 10,000 times the world's total energy use.

b)

c)

Earth's average albedo is about 0.3. In other words, about 30 percent of incoming solar radiation is reflected back into space and 70 percent is absorbed. A sensor aboard NASA's Terra satellite is now collecting detailed measurements of how much sunlight the earth's surface reflects back up into the atmosphere.

d)

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