The phenomenon known as a "supernova" is best described as:a...
A supernova occurs when a massive star exhausts its nuclear fuel and undergoes a catastrophic explosion at the end of its life cycle, releasing vast amounts of energy and forming heavy elements. This distinguishes it from star formation, neutron star mergers, or black hole formation from white dwarfs.
The phenomenon known as a "supernova" is best described as:a...
Understanding Supernovae
Supernovae are one of the most spectacular cosmic events in the universe, marking the end of a massive star's life cycle.
Definition of a Supernova
- A supernova is an astronomical explosion that occurs at the end of a massive star's life.
- This event is not just a simple explosion; it signifies the release of an immense amount of energy, often outshining entire galaxies for a short period.
Life Cycle of a Massive Star
- Massive stars, those with at least eight times the mass of our Sun, undergo nuclear fusion, converting hydrogen into heavier elements.
- As these stars exhaust their nuclear fuel, they can no longer support themselves against gravitational collapse.
Explosion Process
- When the core of a massive star collapses, temperatures and pressures rise dramatically, leading to the fusion of heavier elements.
- Eventually, the core becomes iron, as iron cannot produce energy through fusion.
- Once fusion ceases, the core collapses under gravity, triggering a violent explosion that expels the outer layers of the star into space.
Significance of Supernovae
- Supernovae play a crucial role in the universe by dispersing elements formed in the star into the interstellar medium, contributing to the formation of new stars and planets.
- They also serve as important distance markers in cosmology, helping astronomers measure the expansion of the universe.
In summary, a supernova is best described as the explosion of a massive star at the end of its life cycle, making option 'B' the correct answer.