What Determines the Evolutionary Path of Stars?

In summary, the conversation discusses finding quality websites and asking for help with questions about stars. The questions include defining a star, how astronomers differentiate between stellar objects, what powers a star, the evolutionary process and stages of a star, and the reasons for stars going through this cycle and how it is affected by their mass. The person also thanks Nath for their assistance and suggests searching for "Stellar Evolution" on Google for more information.
  • #1
nath_quam
13
0
Hey, would anyone be able to tell me quality websites/ or help to answer the following questions:
1. What is a star?
2. How Astronomers can tell the difference between different stellar objects?
3. What powers a star?
4. The evelotionary path of a star and it's different stages.
5. Why Stars move though this evolutionary cycle and why the cycle is altered for stars of different mass?

Thanks for your help Nath
 
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  • #2
There's lots of good websites, nath. Do a google search on "Stellar Evolution" and you see things like this from Nasa.

http://observe.arc.nasa.gov/nasa/space/stellardeath/stellardeath_intro.html
 
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  • #3
alie

I would be happy to provide some information on stars and stellar evolution.

1. A star is a massive, luminous sphere of plasma held together by its own gravity. It is primarily composed of hydrogen and helium, and generates energy through nuclear fusion in its core.

2. Astronomers can tell the difference between different stellar objects through various observations and measurements. These include the star's spectral characteristics, such as its temperature and chemical composition, as well as its luminosity, size, and motion.

3. The power source of a star is nuclear fusion, where hydrogen atoms fuse together to form helium. This process releases a tremendous amount of energy, which is what makes stars shine.

4. The evolutionary path of a star depends on its mass. Generally, stars go through several stages: protostar, main sequence, red giant, planetary nebula, and white dwarf. High-mass stars also go through additional stages, such as supernova and neutron star or black hole formation.

5. The evolutionary cycle of a star is determined by its mass because the amount of mass a star has affects its internal pressure, temperature, and fusion rate. The more massive a star is, the faster it consumes its fuel and the shorter its lifespan. This is why high-mass stars have shorter lifetimes and go through more stages than low-mass stars. Additionally, the mass of a star also determines the type of elements it can fuse, which can also affect its evolution.
 

What is a star?

A star is a massive, luminous sphere of plasma held together by its own gravity. It emits light and other forms of electromagnetic radiation, and is the most basic building block of the universe.

How are stars formed?

Stars are formed from large clouds of gas and dust, known as nebulae, which collapse under their own gravity. As the gas and dust come together, it heats up and forms a protostar. This protostar continues to grow and eventually becomes a fully formed star.

What is stellar evolution?

Stellar evolution is the process by which a star changes over its lifetime. It involves the fusion of hydrogen into helium, which releases energy and causes the star to shine. As a star ages, it may go through different stages, such as becoming a red giant, before eventually running out of fuel and dying.

How do stars die?

Stars die when they run out of fuel to sustain nuclear fusion in their core. The type of death a star experiences depends on its mass. Smaller stars, like our Sun, will become a red giant and eventually shed their outer layers to form a planetary nebula. Larger stars, on the other hand, will undergo a supernova explosion before collapsing into a neutron star or black hole.

Can stars be born again?

Technically, no. Once a star dies, it cannot be reborn. However, the materials from a dead star can be recycled and used to form new stars. This is because when a star dies, it releases elements like carbon, oxygen, and iron into space, which can then be incorporated into new stars and planets.

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