Stellar evolution Flashcards

1
Q

What is a star?

A
  • A massive, glowing sphere of plasma held together by gravity.
  • Produces energy through nuclear fusion.
  • Made mostly of hydrogen and helium.
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2
Q

What is nuclear fusion?

A
  • A process where hydrogen nuclei fuse to form helium.
  • Releases enormous amounts of energy in the form of light and heat.
  • Occurs in the core of stars under extreme temperature and pressure.
  • Responsible for the star’s energy output and stability.
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3
Q

What is absolute magnitude and how does it relate to the brightness of a star?

A
  • Absolute magnitude measures a star’s brightness at a standard distance of 10 parsecs.
  • Unlike apparent magnitude, it removes the effect of distance.
  • Brighter stars have lower absolute magnitude values.
  • Example: Rigel (-7.0) is brighter than the Sun (+4.8).
  • Used to classify stars on the Hertzsprung-Russell diagram.
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4
Q

What is the Hertzsprung-Russell (HR) diagram?

A
  • A graph showing the relationship between a star’s absolute magnitude and surface temperature.
  • X-axis: Surface temperature (decreases from left to right, measured in Kelvin).
  • Y-axis: Absolute magnitude (higher up = more luminous).
  • Helps classify stars and predict stellar evolution.
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5
Q

What are the main components of the Hertzsprung-Russell diagram?

A
  • Main Sequence: Diagonal band from hot, bright stars to cool, dim stars.
  • Red Giants & Supergiants: Large, bright but cool stars in the upper right.
  • White Dwarfs: Small, hot but dim stars in the lower left.
  • X-axis: Surface temperature (hot blue stars on the left, cool red stars on the right).
  • Y-axis: Absolute magnitude (brighter stars at the top).
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6
Q

What happens to a star after the main sequence phase?

A
  • Stars run out of hydrogen fuel in their cores.
  • Low-mass stars (like the Sun) become red giants, then white dwarfs.
  • Massive stars become red supergiants, then explode as supernovae.
  • Supernova remnants form either a neutron star or black hole.
  • Supernovae spread heavier elements into space, aiding future star formation.
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7
Q

What are the stages in the life cycle of a star similar to the Sun?

A
  • Nebula: Cloud of gas and dust pulled together by gravity.
  • Protostar: Gravity causes compression; temperature rises; nuclear fusion starts.
  • Main Sequence Star: Longest stage; fusion of hydrogen into helium.
  • Red Giant: Hydrogen runs out; outer layers expand.
  • Planetary Nebula: Outer layers ejected into space, leaving the core.
  • White Dwarf: Small, dense, hot core remains; cools over time.
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8
Q

What are the stages in the life cycle of a massive star?

A
  • Nebula → Protostar → Main Sequence Star
  • Red Supergiant: Hydrogen runs out; fusion of heavier elements.
  • Supernova: Outer layers collapse and explode.
  • Neutron Star: If core is 1.4–3 solar masses.
  • Black Hole: If core is more than 3 solar masses, collapses into a black hole.
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9
Q

What determines whether a star becomes a black hole or a neutron star?

A
  • The mass of the core after a supernova.
  • Neutron star: Core between 1.4–3 solar masses.
  • Black hole: Core greater than 3 solar masses.
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10
Q

What happens in a supernova?

A
  • A massive star explodes at the end of its life cycle.
  • The core collapses, and outer layers eject into space.
  • Produces heavy elements like iron and gold.
  • Releases immense energy, briefly outshining an entire galaxy.
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11
Q

What is a black hole?

A
  • A region of space with gravity so strong that not even light can escape.
  • Formed when a massive star collapses beyond the neutron star stage.
  • Detectable by observing gravitational effects on nearby objects.
  • Can distort spacetime and pull in nearby stars.
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12
Q

What is a neutron star?

A
  • A dense core left after a supernova.
  • Composed almost entirely of neutrons, with incredible density.
  • Has a strong magnetic field and can emit pulses of radiation (pulsars).
  • One of the densest objects in the universe.
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13
Q

What is the significance of supernovae?

A
  • Creates and disperses heavy elements like carbon, oxygen, and iron.
  • Provides materials needed for planets and life.
  • Can trigger new star formation by compressing nearby gas clouds.
  • Plays a crucial role in the chemical evolution of galaxies.
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