The Sun

In the atmosphere, vertical mixing processes like convection and turbulence help distribute heat by transferring warm air from the surface to higher altitudes and bringing cooler air downwards. This mixing contributes to the overall temperature balance in the atmosphere by equalizing temperature differences between different layers of the atmosphere.

The sun has gone through many changes in its existence. It began as a gas nebula before it went through its initial collapse. Then it went through nuclear ignition. After that, once it was ignited, it went through helium flashed and became a red giant. Today, it is a white dwarf.

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The distance is 36,000,000 miles from the Sun.

The Sun is 4.6 billion years old and about halfway through the phase where is shines as it does now due to fusion reactions that convert hydrogen into helium. The Sun will continue this phase, with some variability, until it is about 10 billion years years old.

About 5 billion years from now, the Sun will enter a red giant phase and expand greatly. This lasts for hundreds of millions of years before it blows off its outer layers creating a planetary nebula. In the next several billion years, what is left of the core of the sun will fade to a white dwarf and then continue to cool further forever.

The Sun does not have enough mass to explode as a supernova.

Early humans likely saw the sun as a powerful and essential force in their daily lives. They may have viewed it with a mix of reverence and fear, influencing aspects of their culture, such as sun worship and agriculture practices tied to the sun's cycle.

The closest planet to the Sun is Mercury. This is followed by Venus, then Earth.

In the solar sytem there are 9 planets.There is also a milky way. I think that some people found 2 more new planets.

No, the sun is not a protostar. It is a mature star that is in the main sequence phase of its life cycle, where it fuses hydrogen into helium in its core. A protostar is a young star that is still in the process of accumulating mass and contracting before it begins hydrogen fusion in its core.

Rock: asteroid. Liquid: none. Gas: comet.

Energy from the sun reaches the Earth through electromagnetic radiation, primarily in the form of visible light. This light travels through the vacuum of space and reaches the Earth's atmosphere, where it is absorbed and converted into heat energy.

Yes, it is possible to get a second-degree burn from the sun, known as a severe sunburn. Prolonged exposure to the sun's UV rays can damage the outer and inner layers of the skin, resulting in blistering, pain, and peeling. It is important to protect your skin with sunscreen and clothing to prevent sunburns.

Most of the energy generated by the Sun travels to Earth as Electromagnetic Radiation. A very tiny amount of energy of the Sun is given off as particles, mostly electrons and protons, flying off into space.

Electromagnetic energy is, of course, light. The light energy from the Sun includes the visible spectrum we can see and much more in the infrared part of the spectrum that we can not see and a little in the ultraviolet as well. It all travels at the speed of light from the Sun outwards and a tiny fraction of the Sun's energy strikes the Earth and is absorbed. As a result, the electromagnetic energy is converted to thermal (heat) energy and keeps Earth warm.

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The sun will eventually expand into a red giant before shedding its outer layers and forming a planetary nebula, leaving behind a cooling remnant known as a white dwarf. It will not implode or explode in the traditional sense.

For the same reason the sunset is a different colour. You are looking at it through a higher density of particles in the atmosphere. So there is more atmosphere to protect your eyes from the bright light of the sun

Mimas, one of Saturn's moons, is on average about 1.2 million kilometers, or 0.0032 astronomical units (AU), away from the Sun.

The sun's diameter can be measured using angular diameter, which is typically around 31-32 arcminutes. The sun's distance can be measured using methods like parallax or the astronomical unit (AU), which is the average distance from Earth to the sun, approximately 93 million miles. Its temperature can be estimated through spectral analysis, which reveals it to be around 5,500 degrees Celsius at its surface.

We cannot directly observe the Sun's core from Earth since it is deep within the Sun's layers. However, we can study it indirectly through models and simulations based on scientific principles and observations of the Sun's surface and behavior. The core is a region where nuclear fusion reactions occur, generating tremendous heat and energy that powers the Sun.

white dwarf star

The diameter of the Sun is about 1.4 million kilometers.

A solar eclipse occurs when the moon passes between the Earth and the sun, blocking all or part of the sun's light. This can result in a partial or total eclipse, where the sun appears completely covered by the moon.

"The sun doesn't really change color, it's just that from your perspective it changes color. The reason is that as the sun lowers in the horizon the sunlight has to travel through much more fine particulate matter and the related angle disfuses such that the brighter/whiter wavelengths get to bounce more. Try this: when there is a forest fire look to the west and you'll see lots of different shades of yellow and orange..."
-Backyard Mech537

It depends on what planet your talking about, but if your talking about Earth then it's 365 days (+1 quarter of a day, that's why you get leap years every 4 years). Or if you want to be really specific it's 8,766 hours. Or to be exact it's 31,536,000 seconds

A shadow forms when an object blocks the path of light. In the case of the sun shining, the object blocking the light is you, which casts a shadow behind you. The sun's rays are not able to pass through your body, creating the shadow on the ground.