there is something which handles everything....there's invisible supreme power in the world.....
In terms of science, it is the nature of the nuclear reactions that power the Sun.
No, the size of the sun remains relatively stable over short periods of time. The sun does go through changes over long periods, but these changes occur gradually over millions of years.
Oh sweetheart, don't you worry about that. The distance between Earth and the sun actually stays fairly consistent every year, thanks to our beautiful elliptical orbit. We're just twirling gracefully through space, hanging out at a comfortable distance from our favourite star. His warm rays light up our world just right.
The sun's mass is gradually decreasing over time due to the process of nuclear fusion, which converts hydrogen into helium and releases energy. Additionally, the sun loses mass through the solar wind, a stream of charged particles released from its outer layers. However, this loss is minuscule compared to its total mass, so the sun remains stable in its life cycle for billions of years to come. Overall, while the sun's mass is decreasing, the rate is very slow and not significant in the short term.
No, the sun's brightness remains relatively constant over time. Any fluctuations would likely be due to atmospheric conditions or personal perception, rather than the sun itself becoming brighter than usual.
The Sun's mass remains relatively constant as it burns because the process of nuclear fusion, which powers the Sun, converts mass into energy. This mass-energy conversion maintains a balance that keeps the Sun stable.
No, the size of the sun remains relatively stable over short periods of time. The sun does go through changes over long periods, but these changes occur gradually over millions of years.
The distance between the planets and the sun typically remains fairly constant over time. The orbits of the planets are generally stable due to the gravitational forces between the sun and the planets. Any changes in distance are usually minimal and occur over long time scales.
Oh sweetheart, don't you worry about that. The distance between Earth and the sun actually stays fairly consistent every year, thanks to our beautiful elliptical orbit. We're just twirling gracefully through space, hanging out at a comfortable distance from our favourite star. His warm rays light up our world just right.
The mass of the sun is decreasing over time.
No, the Earth's rate of speed in its orbit around the sun remains relatively constant. However, the Earth's distance from the sun varies slightly throughout the year, affecting its orbital speed slightly.
"Inertia" plus gravity (of the sun). Note that the orbits do change over time, but that in the last few billion years they have been quite stable.
The sun's mass is gradually decreasing over time due to the process of nuclear fusion, which converts hydrogen into helium and releases energy. Additionally, the sun loses mass through the solar wind, a stream of charged particles released from its outer layers. However, this loss is minuscule compared to its total mass, so the sun remains stable in its life cycle for billions of years to come. Overall, while the sun's mass is decreasing, the rate is very slow and not significant in the short term.
No, the sun's brightness remains relatively constant over time. Any fluctuations would likely be due to atmospheric conditions or personal perception, rather than the sun itself becoming brighter than usual.
Hydrostatic equilibrium in the Sun refers to the balance between the inward gravitational force and the outward pressure force generated by nuclear fusion. This balance maintains the Sun's stable structure and allows it to maintain its size and shape over time.
The Sun's mass remains relatively constant as it burns because the process of nuclear fusion, which powers the Sun, converts mass into energy. This mass-energy conversion maintains a balance that keeps the Sun stable.
It means that an object remains in a stable orbit around a central object. For example the Earth stays in a stable near-circular orbit around the Sun although it is continuously moving at around 18 miles per second in a direction that is along the ecliptic and at right angles (approximately) to the direction of the Sun.
The sun is expect to remain stable for another three billion years.