Unraveling the Mystery of the Sun's Composition and the Fate of Matter Within

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In summary, matter that falls into a sun is heated up to high temperatures and can turn into a plasma state. It then joins the rest of the material in the outer areas of the sun and swirls around in convection currents. It may also continue to make its way further into the sun. As for the energy contained in detached solar prominences and what happens to them, they can potentially fall back into the sun or disperse without a trace. Some stars have odd spectra that suggest they have swallowed hot jupiters, possibly affecting their spin and rotation.
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moejoe15
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What happens to regular matter that falls into a sun?

Why is the sun made up primarily of light elements and the rest of the solar system isn't when a solar system evolves? (maybe with the gas giants it is but why isn't there a lot of heavy elements in the sun)
 
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moejoe15 said:
Why is the sun made up primarily of light elements and the rest of the solar system isn't when a solar system evolves? (maybe with the gas giants it is but why isn't there a lot of heavy elements in the sun)

The answer is that there's simply more light elements available in the universe. Since the universe is ~24% He and 75% H, you only get 1% left over for all the other elements! Now, it might seem like the sun has far fewer heavy elements than say Earth, but that's not true. Earth merely has a higher proportion of heavy element,s since it doesn't have any of the light gasses (H,He). Of course the reason the Earth doesn't have H,He is because its gravity is too weak to hold onto these light gasses, and if they ever were present on the planet they've since leaked out into space. The sun and gas giants don't have this problem, which is why we see them as primarily gaseous!
 
  • #3
What happens to regular matter that falls into a sun?

It is heated up to high temperatures as it gets closer. If it enters the sun and can fall far enough into it, it will be turned into a plasma state. From there it probably joines the rest of the material in the outer areas of the sun and swirls around in the convection currents. It's possible it could continue to make its way further and further into the sun, but I really don't know.
 
  • #5
IIRC, stuff falls into our sun on a regular basis. SOHO spots many sun-grazer and sun-impactor comets. Given the relative sizes, the impactor is vaporised, ionised and dispersed without a trace. So far, AFAIR, no impactor has triggered any anomalous solar activity, and certainly no 'Jupiter Bruises' per the Shoemaker-Levy-9 event...

Uh, I've read that some stars have odd spectra that have been attributed to them swallowing one or more 'hot jupiters'. They also seem to have higher spin / shorter 'days' than our sun...
 

FAQ: Unraveling the Mystery of the Sun's Composition and the Fate of Matter Within

What is the Sun made of?

The Sun is primarily composed of hydrogen (about 73%) and helium (about 25%), with small amounts of other elements such as oxygen, carbon, and iron. These elements make up the Sun's outer layers, while the inner core is primarily made of hydrogen under extreme pressure and temperature.

How do scientists study the composition of the Sun?

Scientists use various methods to study the Sun's composition, including spectroscopy, which involves analyzing the light emitted from the Sun to identify the elements present. They also use models and simulations to understand how different elements behave under the extreme conditions within the Sun.

What happens to matter within the Sun?

Matter within the Sun undergoes nuclear fusion, where hydrogen atoms combine to form helium, releasing large amounts of energy in the process. This is what powers the Sun and keeps it shining. As the Sun ages, it will eventually run out of hydrogen fuel and begin to fuse helium, leading to changes in its composition and structure.

Why is it important to study the Sun's composition and the fate of matter within?

The Sun is not only our closest star, but it also plays a crucial role in sustaining life on Earth. By understanding its composition and how matter behaves within it, scientists can gain insights into the processes that govern stars and their evolution. This knowledge can also help us better understand the origins of our solar system and the universe.

What are some potential implications of unraveling the mystery of the Sun's composition?

Studying the Sun's composition and the fate of matter within could have practical applications, such as improving our ability to predict and prepare for solar flares and other space weather events that can impact Earth. It could also lead to advancements in energy production through nuclear fusion, as we strive to replicate the Sun's energy-producing processes on Earth.

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