chapter 14

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81 Terms

1
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what is a white dwarf

a small, dense remnant of a low-mass star

2
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what can happen to a white dwarf in a close binary system

it can explode as a supernova

3
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what prevents a white dwarf from collapsing under its own gravity

degeneracy pressure

4
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what is a neutron star

a remnant core left after a supernova explosion, composed of mostly neutrons

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how were neutron stars discovered

by detecting pulsars, which are rapidly rotating neutron stars emitting beams of radiation

6
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what can happen to a neutron star in a close binary system

it can accrete matter and emit x-rays

7
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what is a black hole

a region of space where gravity is so strong that not even light can escape

8
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what would it be like to visit a black hole

you would experience time dilation and extreme tidal forces

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do black holes really exist

yes, they have been confirmed through various observations such as gravitational waves and x-ray emissions from accretion disks

10
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what causes gamma-ray bursts

the collision and merger of neutron stars or the collapse of massive stars

11
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what happens when neutron stars merge

they form either a more massive neutron star or collapse into a black hole while emitting gravitational waves and gamma-ray bursts

12
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what happens when black holes merge

they form a single, more massive black hole while emitting gravitational waves

13
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what is a white dwarf

the exposed core of a star that has died and shed its outer layers

14
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which type of pressure supports a white dwarf against the crush of gravity

electron degeneracy pressure

15
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what happens to the temperature of a white dwarf over time

it slowly cools

16
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what is the primary composition of a white dwarf left behind by a sun-like star

carbon

17
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how does the size of more massive white dwarfs compare to less massive ones

more massive white dwarfs are smaller in size

18
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what would be the approximate weight of a teaspoon of a white dwarf matter on earth

several tons

19
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what is the maximum mass that a white dwarf can have, known as the chandrasekhar limit

1.4 times the mass of the sun

20
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why can’t a white dwarf have a mass greater than 1.4 times the mass of the sun

electron speeds would reach the speed of light, which is not possible

21
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what observational evidence supports the theoretical limit on the mass of white dwarfs

all observed white dwarfs have masses below 1.4 times the mass of the sun

22
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what can happen to a white dwarf in a close binary system with a main-sequence or giant star companion

it can gradually gain mass through an accretion disk

23
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how does gas behave in an accretion disk around a white dwarf

gas in the inner region orbits faster than gas in the outer region

24
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what new energy source can accretion provide to an otherwise “dead” white dwarf

gravitational potential energy converted into thermal and radiative energy

25
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what causes hydrogen fusion to ignite on the surface of a white dwarf, leading to a nova

the temperature at the bottom of an accreted hydrogen layer reaches about 10 million k

26
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how does accretion affect successive novae on a particular system

accretion resumes after each nova explosion, allowing for repeated novae

27
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what happens when carbon fusion ignites almost instantly throughout an entire white dwarf

the white dwarf explodes completely in what is called a white dwarf

28
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how can two closely orbiting white dwarfs lead to one reaching the chandrasekhar limit

they emit gravitational waves, causing them to spiral inward and merge

29
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how do astronomers distinguish between different types of supernovae

by studying thier light spectra and luminosity patterns

30
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what primarily supports a neutron star against the crush of gravity

neutron degeneracy pressure

31
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how does the density of neutron star material compare to that of ordinary matter

it is so dense that a paper clip made of it would outweigh mount everest

32
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what would happen if a small piece of neutron star material appeared on earth

it would pass through the earth due to its immense weight and density

33
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how does the mass and size of a typical neutron star compare to that of the sun

more massive and much smaller than the sun

34
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what is the escape velocity at the surface of a neutron

about half the speed of light

35
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who discovered the first observational evidence for neutron stars and when

jocelyn bell burnell in 1967

36
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what phenomenon did jocelyn bell burnell discover that led to identifying neutron stars

rapidly pulsing radio waves at precise intervals

37
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why are pulsars considered cosmic lighthouses

they emit beams of radiation that sweep past earth as they rotate, creating pulses we can detect

38
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why do pulsars gradually slow down over time

their magnetic fields generate electromagnetic radiation that carries away energy and angular momentum

39
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what rule can be derived about pulsars and neutron stars based on their characteristics

all pulsars are neutron stars, but not all neutron stars are pulsars

40
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what type of radiation do accretion disks around neutron stars primarily emit

x-ray radiation

41
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why do x-ray binaries with accreting neutron stars often have rapidly pulsating emissions

the accreting matter adds angular momentum, causing the neutron star’s rotation rate to increase, leading to rapid pulsations in x-rays emitted by the accretion disk

42
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what is the defining characteristic of a black hole

its escape velocity exceeds the speed of light

43
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according to einstein’s general theory of relativity, what causes gravity

the curvature of spacetime

44
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why is it impossible for light to escape from a black hole

the gravitational pull inside a black hole is too strong for light to escape

45
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what is the event horizon of a black hole

the boundary at which the escape velocity equals the speed of light

46
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what determines the schwarzchild radius of a black hole

its mass

47
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how does the size of the schwarzchild radius change with increasing mass

its mass increases

48
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what happens to matter inside a black hole according to current theories

it gets crushed into an infinitely tiny and dense point called a singularity

49
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which two theories make different predictions about the nature of singularities in black holes

general relativity and quantum physics

50
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why can’t we observe what happens inside a black hole’s event horizon

because it emits no radiation or light detectable by telescopes

51
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what is a gravitational redshift

a shift in light frequency due to strong gravitational fields affecting time and space

52
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what would happen to an object as it approaches the event horizon from an outside observer’s perspective

it would appear to slow down and eventually freeze in time as it reaches the event horizon due to gravitational redshift effects

53
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why would tidal forces near a small black hole be lethal for humans

because they would stretch and compress objects with extreme force differences over short distances

54
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how does supernova contribute towards formation process leading up to creation involving possible stellar remnants like neutron stars and black holes

by causing collapse under own gravity leading up to formation involving neutron star or possibly even further collapsing into forming black hole if conditions exceed certain limits

55
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what evidence supports existence regarding supermassive black holes residing within centers involving many galaxies including milky way

observations regarding extreme events occurring within universe along with indirect influences exerted upon surrounding celestial bodies suggesting presence regarding such massive objects influencing their behavior significantly over time periods involved during study conducted so far till date

56
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why do astronomers believe some x-ray binaries contain black holes instead of neutron stars

because they emit stronger x-rays compared against those emitted by neutron stars indicating presence involving more massive object involved within system studied so far till date

57
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what was the initial purpose of the satellites that first detected gamma-ray bursts

to detect nuclear bomb tests

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why do scientists believe that gamma-ray bursts channel their energy into narrow beams

because their luminosity is too high to be explained otherwise

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what is the primary evidence linking gamma-ray bursts to exploding stars

observations of gamma-ray bursts coinciding with supernova explosions in other wavelengths of light

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what type of supernova is likely responsible for the most extreme gamma-ray bursts

a supernova forming a black hole

61
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what percentage of gamma-ray bursts are different in character and last only a few seconds

about 30%

62
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what happens when 2 neutron stars merge

they emit gravitational waves and produce a blend of rare elements, including gold and platinum

63
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how was it confirmed that neutron star mergers can produce short gamma-ray bursts

by detecting gravitational waves followed by a burst of gamma rays from the fermi satellite in 2017

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where did the first confirmed neutron star merger occur, as detected by ligo in 2017

in a galaxy called ngc 4993, located about 130 million light-years from earth

65
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what happens when two black holes merge

they form a single more massive black hole and emit strong gravitational waves

66
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why are gravitational waves from black hole mergers particularly intense during the final death spiral

because their greater masses lead to much stronger emission of gravitational waves at this stage

67
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what was significant about ligo’s detection on september 14, 2015

it provided strong evidence for the existence of black holes through signals matching supercomputer models of black hole mergers

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which even releases more energy than a massive star supernova

the merger of two neutron stars emitting gravitational waves and producing rare elements like gold and platinum

69
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how do astronomers identify extreme outbursts of energy in space

by watching for extreme outbursts across various wavelengths, including gamma rays, x-rays, and visible light using different types of telescopes simultaneously or sequentially after initial detection events like gamma-ray bursts or gravitational waves are observed by specialized instruments like ligo or fermi satellite systems respectively

70
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what supports a white dwarf against the crush of gravity

electron degeneracy pressure

71
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what can cause a white dwarf to explode as a supernova in a close binary system

the white dwarf’s mass reaching the white dwarf limit of 1.4 solar masses

72
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how does hydrogen build-up on a white dwarf’s surface in a close binary system

through an accretion disk that swirls toward the white dwarf’s surface

73
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what is a neutron star primarily composed of

neutrons

74
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how were neutron stars first discovered

by detecting pulsars, which are rapidly spinning neutron stars emitting beans of radiation

75
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what phenomenon can occur when a neutron star in a close binary system accretes hydrogen from its composition

x-ray bursts due to periodic helium fusion on the neutron star’s surface

76
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what marks the boundary between our observable universe and the inside of a black hole

the event horizon

77
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what happens to light emitted by an object as it falls closer to a black hole

it becomes increasingly redshifted until it disappears from view

78
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what evidence supports the existence of black holes in x-ray binaries

the presence of compact objects too massive to be neutron stars

79
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what are gamma-ray bursts most likely associated with

unusually powerful supernova explosions that may create black holes

80
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what is believed to be one primary source of gold, platinum, and uranium in the universe

mergers of neutron stars in close binary systems emitting gravitational waves before merging

81
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how have gravitational waves provided evidence for black hole mergers

by being directly detected from systems consisting of two merging black holes, representing strong evidence for their existence