Chapter 13: Problem 34
Choose the best answer to each of the following. Explain your reasoning with one or more complete sentences. Where do gamma-ray bursts tend to come from? (a) neutron stars in our galaxy (b) black holes in our galaxy (c) extremely distant galaxies
Short Answer
Expert verified
Gamma-ray bursts come from extremely distant galaxies (option c).
Step by step solution
01
Understanding the Question
We want to determine the source of gamma-ray bursts, which are highly energetic explosions observed in the universe.
02
Analyze the Options
Let's analyze each option: (a) suggests that gamma-ray bursts come from neutron stars within our galaxy; (b) suggests that black holes in our galaxy are the source, and (c) suggests that they originate from extremely distant galaxies.
03
Review Scientific Facts
Gamma-ray bursts are known to originate from extremely energetic events that occur far away from our galaxy. Observations of gamma-ray bursts indicate they are often linked to distant, massive stars collapsing or neutron star mergers in very remote galaxies.
04
Evaluate Each Option
- Option (a) neutron stars in our galaxy: This is unlikely as our galaxy does not have the energy events required for typical gamma-ray bursts.
- Option (b) black holes in our galaxy: Black holes could be involved post-burst, but they are not the initial source within our galaxy.
- Option (c) extremely distant galaxies: This matches observations that gamma-ray bursts come from far-off galaxies, indicating they are extragalactic events.
05
Conclusion
Based on the analysis, the most accurate answer is option (c) as gamma-ray bursts are known to come from extremely distant galaxies.
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Neutron Stars
Neutron stars are fascinating remnants of massive stars that have exhausted their nuclear fuel. When a star, with a mass greater than the Sun, undergoes supernova explosion, its core collapses into an incredibly dense object known as a neutron star.
This core is composed almost entirely of neutrons, subatomic particles with no charge and slightly larger than protons. The density of these stars is astonishing, with a single teaspoon of neutron-star material weighing billions of tons on Earth. These stellar remnants are small, typically only about 20 kilometers in diameter, yet they can have masses about 1.4 times that of the Sun. Neutron stars possess powerful magnetic fields and can rotate very rapidly, often detected as pulsars through their emitted electromagnetic radiation. Despite their intense conditions, neutron stars within our galaxy are not usually the source of gamma-ray bursts. While they can contribute to these phenomena through collisions or mergers, the most significant gamma-ray bursts typically occur in distant galaxies.
This core is composed almost entirely of neutrons, subatomic particles with no charge and slightly larger than protons. The density of these stars is astonishing, with a single teaspoon of neutron-star material weighing billions of tons on Earth. These stellar remnants are small, typically only about 20 kilometers in diameter, yet they can have masses about 1.4 times that of the Sun. Neutron stars possess powerful magnetic fields and can rotate very rapidly, often detected as pulsars through their emitted electromagnetic radiation. Despite their intense conditions, neutron stars within our galaxy are not usually the source of gamma-ray bursts. While they can contribute to these phenomena through collisions or mergers, the most significant gamma-ray bursts typically occur in distant galaxies.
Black Holes
Black holes are another intriguing feature of our universe, known for their mysterious nature and extreme gravitational pull. They form from the gravitational collapse of massive stars after they exhaust their nuclear fuel.
When the core of a dying star collapses, the gravity becomes so intense that not even light can escape, creating the "black" in black hole. At their core, known as singularity, the laws of physics as we know them break down. Black holes can vary greatly in size:
When the core of a dying star collapses, the gravity becomes so intense that not even light can escape, creating the "black" in black hole. At their core, known as singularity, the laws of physics as we know them break down. Black holes can vary greatly in size:
- Stellar-mass black holes, a few times larger than our Sun, formed from collapsing stars.
- Supermassive black holes, with millions to billions of solar masses, often found at the centers of galaxies.
Distant Galaxies
Distant galaxies are vast engines of cosmic activity and diversity, often home to explosive phenomena that intrigue scientists. Galaxies, which are massive collections of stars, gas, dust, and dark matter, can be billions of light-years away from us. Observing them allows us to peer into the universe's past, as their light takes eons to reach Earth.
Most gamma-ray bursts, these intense flashes of gamma rays, originate from such far-off galaxies. Their sources include:
Most gamma-ray bursts, these intense flashes of gamma rays, originate from such far-off galaxies. Their sources include:
- The collapse of massive stars into black holes, producing long-duration gamma-ray bursts.
- Collisions between neutron stars or between a neutron star and a black hole, often resulting in short gamma-ray bursts.