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The Life Cycle of a Star. A Really “Hot” Topic. By Samantha Edgington . Objectives. Describe how stars are formed. Explain the concept of equilibrium. Define the “death” of a star. Identify the different types of stars.

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the life cycle of a star

The Life Cycle of a Star

A Really “Hot” Topic

By Samantha Edgington

objectives
Objectives
  • Describe how stars are formed.
  • Explain the concept of equilibrium.
  • Define the “death” of a star.
  • Identify the different types of stars.
  • Describe how the process of nuclear fusion works within a star.
what is a nebula
What is a Nebula?
  • A nebula can be defined as a thinly spread cloud of interstellar gas and dust.
  • Some nebulae are the remains of a supernova explosion.
    • the death and collapse of a massive star can cause this explosion, this means nebulae can be the remains of old, dead stars.
  • Most nebulae are gravity-induced condensations of gases where protostars are born.
how is a protostar formed
How is a Protostar Formed?
  • Inside a nebula, there are areas where gravity causes dust and gas to “clump” together.
  • As these “clumps” gather more and more mass their gravitational pull increases, forcing more atoms together.
  • This process is known as accretion, and the result is a protostar.
how does a protostar become a star
How does a Protostar Become a Star?
  • In order to comprehend this process, the concept of equilibrium must be understood.
  • Equilibrium is in essence a balance.
  • In the case of star formation this balance exists between gravity and gas pressure.
achieving equilibrium
Achieving Equilibrium
  • First gravity pulls gas and dust inward towards the core of the prospective star.
  • Inside the core, density and temperature increases as atomic collisions increase, causing a rise in gas pressure.
  • Finally when gas pressure is equal to gravity, the protostar has reached equilibrium and is therefore reached a reasonably stable size.
the birth
The Birth
  • Once the protostar has achieved equilibrium one of two things occur:
      • If there is not a sufficient mass, it becomes a brown dwarf which is a “star” that doesn’t radiate much heat and light.
      • In the event it does contain an appropriate amount of matter, nuclear fusion begins and light is emitted.
the main sequence
The Main Sequence
  • A star is basically a huge ball of gas undergoing nuclear fusion.
  • The main sequence phase is where stars spend the majority of their “life” by fusing hydrogen into helium.
  • There are two types of main sequence stars:
    • a red giant which is alarge bright star with a cool surface.
    • a red dwarf which are very cool, faint and small stars
the ending of main sequence
The Ending of Main Sequence
  • The star slowly shrinks over billions of years as the hydrogen is used by fusion.
  • The star’s temperature, density, and pressure at the core continues to increase.
  • Once the hydrogen is depleted, the helium is fused into carbon, when this occurs the star has reached “old age”.
the death
The Death
  • There are one of two ways a star can die depending on its size.
  • If the star is of low mass, it expands its outer layers, creating nebulae and a white dwarf forms from the core.
  • If it is of high mass, death occurs in a massive explosion known as a supernova, the remaining core then transforms into a neutron star or a black hole.
what is a white dwarf
What is a White Dwarf?
  • They form from the core of a dead red giants that were too small to fuse carbon.
  • Since they do not undergo fusion, they have no energy source and gradually fade.
  • When they radiate away all of their energy they will theoretically become a black dwarf.
  • Since white dwarfs cannot be older than the universe (13.7 billion years) no black dwarfs are currently in existence.
what is a supernova
What is a Supernova?
  • They can form when the gravitational potential energy—created by a sudden gravitational collapse of a large red giant—heats and expels the star\'s outer layers, resulting in an explosion.
  • Also, they can form when a white dwarf ignites carbon fusion, which results in a runaway nuclear fusion reaction and causes a supernova.
  • Supernovae can be so immense that the energy produced can equal the energy the Sun creates over a time period of 10 billion years!
what is a neutron star
What is a Neutron Star?
  • A neutron star is formed as a result of a massive star being compressed.
  • The core material, known as neutron degenerate matter, mostly consists of neutrons with a few protons and electrons.
  • The gravity is so intense that if an object were to reach the surface it would disperse all of its subatomic particles and merge with the star!
  • The matter is so dense that a teaspoon would weigh billions of tonnes!
  • Some people view neutron stars as giant atoms.
what is a stellar black hole
What is a Stellar Black Hole?
  • If a collapsing star exceeds the maximum mass a neutron star can be it will develop into a stellar black hole.
  • Black holes are extremely dense areas with a gravitational pull so powerful not even light can escape!
  • What could be a reason why black holes are black?
the sun s life
The Sun’s Life
  • Now that a basic overview of a star’s life cycle has been covered, the details of the most important star’s life can be revealed.
  • Can you guess what type of star the Sun is?
the sun in main sequence
The Sun in Main Sequence
  • The Sun was born like any other star, out of a nebulae and into a protostar.
  • It is now in its main sequence and can be classified as a yellow dwarf.
  • The Star is about 4.57 billion years old, about halfway through its complete lifecycle.
the sun s death
The Sun’s Death
  • Since the Sun is considerably smaller it will not explode in a supernova.
  • Instead it is predicted that it will become a red giant in about ~6 billion years.
  • When this occurs, all the water on earth will be vaporized and life will cease to exist.
  • In the final phase the Sun will form a white dwarf and slowly fade out of existence.
works cited
Works Cited
  • www.dictionary.com
  • aspire.cosmicray.org/labs/star_life/starlife_proto.html
  • www.astro.keele.ac.uk/workx/starlife/StarpageS_26M.html
  • http://www.telescope.org/pparc/res8.html
  • www.antonine-education.co.uk
  • www.darkstar1.co.uk
  • www.pbs.org
  • outreach.jach.hawaii.edu
  • www.spaceflightnow.com
  • wikipedia.org
  • www.cosmographica.com
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