AI C19 Flashcards

1
Q

What is a star?

A

A star is a luminous sphere of plasma held together by its own gravity.

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2
Q

What is the primary source of a star’s energy?

A

The primary source of a star’s energy is nuclear fusion in its core.

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3
Q

What is the process of nuclear fusion in a star?

A

Nuclear fusion in a star is the process where hydrogen atoms combine to form helium, releasing a large amount of energy.

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4
Q

What are the two forces that are in balance within a star?

A

The two forces that are in balance within a star are gravity pulling inward and radiation pressure pushing outward.

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5
Q

What determines the size and mass of a star?

A

The size and mass of a star are determined by the balance between gravity and radiation pressure.

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6
Q

What is the life cycle of a star like the Sun?

A

The life cycle of a star like the Sun involves stages such as main sequence, red giant, planetary nebula, and white dwarf.

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7
Q

What is the Chandrasekhar limit?

A

The Chandrasekhar limit is the maximum mass of a stable white dwarf star, approximately 1.4 times the mass of the Sun.

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8
Q

What is a neutron star?

A

A neutron star is a highly dense remnant of a massive star that has undergone a supernova explosion.

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9
Q

What is a black hole?

A

A black hole is a region in space where gravity is so strong that nothing, not even light, can escape.

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10
Q

What is Hawking radiation?

A

Hawking radiation is thermal radiation predicted to be emitted by black holes due to quantum effects near the event horizon.

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11
Q

What is the Hertzsprung-Russell diagram used for?

A

The Hertzsprung-Russell diagram is used to classify stars based on their luminosity, temperature, and evolutionary stage.

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12
Q

What is a main sequence star?

A

A main sequence star is a star fusing hydrogen into helium in its core, like our Sun.

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13
Q

What is a red giant star?

A

A red giant star is a star that has exhausted its core hydrogen and expanded to a larger size.

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14
Q

What is a white dwarf star?

A

A white dwarf star is the remnant core of a low to medium mass star after it has shed its outer layers as a planetary nebula.

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15
Q

What is a supernova?

A

A supernova is a stellar explosion that briefly outshines an entire galaxy, releasing an immense amount of energy.

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16
Q

What is the ultimate fate of a massive star?

A

The ultimate fate of a massive star is to undergo a supernova explosion, potentially leaving behind a neutron star or black hole.

17
Q

What is stellar nucleosynthesis?

A

Stellar nucleosynthesis is the process by which elements are formed within stars through nuclear reactions.

18
Q

What is the significance of the iron peak in stellar nucleosynthesis?

A

The iron peak in stellar nucleosynthesis is the point where nuclear fusion of elements becomes endothermic, leading to the end of a star’s life.

19
Q

What is a planetary nebula?

A

A planetary nebula is a glowing shell of gas ejected by a low to medium mass star in the late stages of its life.

20
Q

What is the role of magnetic fields in star formation?

A

Magnetic fields play a crucial role in regulating the collapse of interstellar gas clouds to form stars.

21
Q

What is the concept of hydrostatic equilibrium in stars?

A

Hydrostatic equilibrium in stars is the balance between the inward gravitational force and the outward pressure force.

22
Q

What are the two types of nuclear reactions that power stars?

A

The two types of nuclear reactions that power stars are the proton-proton chain and the CNO cycle.

23
Q

What is the main sequence phase of a star’s life cycle?

A

The main sequence phase of a star’s life cycle is when it fuses hydrogen into helium in its core and is in a stable state.

24
Q

What is the solar neutrino problem?

A

The solar neutrino problem refers to the discrepancy between the predicted and observed number of neutrinos emitted by the Sun.

25
Q

What is a Type II supernova?

A

A Type II supernova is a supernova that occurs in massive stars when they reach the end of their life cycle.

26
Q

What is the concept of degeneracy pressure in white dwarfs?

A

Degeneracy pressure in white dwarfs is a quantum mechanical effect that prevents further collapse of the star’s core.

27
Q

What is the Eddington luminosity limit?

A

The Eddington luminosity limit is the maximum luminosity that a star can achieve before the outward radiation pressure exceeds the inward gravitational force.

28
Q

What is a pulsar?

A

A pulsar is a highly magnetized rotating neutron star that emits beams of electromagnetic radiation.

29
Q

What is the Schwarzschild radius of a black hole?

A

The Schwarzschild radius of a black hole is the radius at which the escape velocity equals the speed of light.

30
Q

What is the event horizon of a black hole?

A

The event horizon of a black hole is the boundary beyond which nothing can escape its gravitational pull.

31
Q

What is the concept of gravitational lensing in black holes?

A

Gravitational lensing in black holes is the bending of light around the black hole due to its strong gravitational field.

32
Q

What is the role of dark matter in the formation of galaxies and stars?

A

Dark matter plays a crucial role in the formation of galaxies and stars by providing the additional mass needed for gravitational collapse.