gravitational collapse
Học thuậtThân thiện
Definition
Noun: - The implosion of a star resulting from its own gravity; the result is a smaller and denser celestial object: This is the process where a massive star's internal pressure can no longer counteract its own immense gravitational pull, causing it to violently collapse inward upon itself. This event is a critical phase in stellar evolution and leads to the formation of extremely dense remnants.
Usage
- This term is used almost exclusively in astrophysics and cosmology to describe a specific, catastrophic phase in the life cycle of massive stars.
- It is a singular, uncountable noun phrase describing the process or event itself.
Examples
Advanced Usage
- In cosmological contexts: The term can be applied theoretically to the collapse of very large-scale structures or hypothetical early universe conditions, though its primary use remains stellar.
- As a modifier: The phrase can function adjectivally in compound terms (e.g., , ), but the core definition remains the noun phrase described above.
Variants and Related Words
- Collapse (n.): A more general term for a sudden failure or falling in. In astrophysics, it is often understood to mean gravitational collapse.
- Implosion (n.): A bursting inward, which is the mechanical action at the heart of gravitational collapse.
- Core collapse: A closely related term often used synonymously with gravitational collapse, specifically referring to the collapse of the star's central region.
Synonyms
- Stellar collapse: A near-synonym that emphasizes the astronomical object involved.
- Implosion due to gravity: A descriptive phrase conveying the same meaning.
Related Phrases
- To undergo gravitational collapse: The verbal phrase describing the action of the star.
- When the fuel is exhausted, the star will undergo gravitational collapse.
- Trigger a gravitational collapse: Describes the initiation of the process.
- The fusion of iron in the core can trigger gravitational collapse.
Noun
- the implosion of a star resulting from its own gravity; the result is a smaller and denser celestial object