133 days on sun

The concept of a "day" on the Sun is quite different from what we experience on Earth because the Sun is a massive, hot, and gaseous celestial body with no solid surface. However, if we were to refer to a "day" on the Sun in terms of its rotation period, here is some information:

Rotation Period: The Sun does indeed rotate, but its rotation is not uniform across its surface. It exhibits differential rotation, meaning that different parts of the Sun rotate at different rates. The equator rotates faster than the poles. On average, the Sun's equatorial regions rotate approximately once every 24 to 25 Earth days, while the polar regions can take up to 35 Earth days to complete one rotation.

Solar Features: The Sun is covered in various features, such as sunspots, solar flares, and prominences. These features are the result of complex magnetic interactions within the Sun's interior. Over the course of 133 days, you would likely see various sunspots appearing and disappearing on the Sun's surface, as well as occasional solar flares and prominences.

Solar Activity: The Sun goes through an approximately 11-year solar cycle, during which its activity waxes and wanes. This cycle is characterized by periods of increased solar activity, which can lead to more sunspots, solar flares, and coronal mass ejections. The level of solar activity on any given 133-day period would depend on where the Sun is in its solar cycle. It could range from relatively quiet to highly active.

Solar Energy Output: Throughout this 133-day period, the Sun would continue to emit a tremendous amount of energy in the form of light and heat. The Sun's energy is what powers our solar system, including Earth, and enables life to exist on our planet.

It's important to note that observing the Sun directly without proper solar filters can be extremely dangerous and can cause severe eye damage or blindness. Any observations of the Sun should be conducted with the appropriate safety measures and equipment.