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.
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.
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.
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.
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).
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.
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.
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.
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.
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.
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.
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.
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.