A1 Flashcards

(67 cards)

1
Q

What causes a nova in a white dwarf system?

A

Surface-burning of material accreted from a companion star, which is unstable compared to core-burning.

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2
Q

How does material transfer lead to nova in a white dwarf?

A

Material from a companion star falls onto the white dwarf. Once enough accumulates, fusion reignites suddenly, burning off the new material.

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3
Q

What is a nova and how does it behave in terms of brightness?

A

A nova flares up suddenly and then returns to former luminosity. Its brightness can increase by 10,000 times for a few months.

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4
Q

What do the images of Nova Persei and Nova Cygni show?

A

They show expanding ejected material from the star after a nova explosion.

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5
Q

What is a carbon-detonation supernova?

A

Occurs when a white dwarf exceeds the Chandrasekhar limit of 1.4 solar masses, triggering carbon fusion and an explosion.

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6
Q

What differentiates Type I and Type II supernovae?

A

Type I is from a binary system with a white dwarf; Type II results from iron core collapse of a massive star.

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7
Q

What happens in a binary system that leads to Type-I SN?

A

One star dies leaving a white dwarf which may later accrete enough mass from its companion to trigger a supernova.

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8
Q

Why is Sirius B potentially dangerous?

A

If it becomes a supernova, being only 9 light years from Earth, it could cause mass extinction.

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9
Q

What conditions must be met for Pegasi-A to transfer mass to Pegasi-B?

A

Pegasi-A must expand to a radius of 24.4 R☉; then nova or Type-I SN can occur depending on mass accumulation.

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10
Q

Describe the mechanisms behind Type-I and Type-II supernovae.

A

Type-I: WD accretes >1.4 M☉, fusion ignites throughout, leading to explosion. Type-II: High-mass star core collapses after iron fusion ends.

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11
Q

What is the fate of low-mass vs high-mass isolated stars?

A

Low-mass stars eject outer envelopes and become white dwarfs. High-mass stars end in Type-II SN after iron core collapse.

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12
Q

What happens to a white dwarf in a binary when mass >1.4 M☉?

A

It undergoes carbon fusion throughout and explodes as a Type-I SN.

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13
Q

What occurs in a semidetached binary system during mass transfer?

A

Gentle mass transfer alters star evolution but doesn’t cause supernova immediately.

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14
Q

How does mass transfer affect binary star evolution?

A

As a red giant transfers mass, the smaller star may become more massive and evolve into a blue giant.

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15
Q

What is a contact binary?

A

A binary system where mass is shared extensively, often beginning as a detached binary and evolving over time.

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16
Q

What causes X-ray bursts in neutron-star binaries?

A

Explosive nuclear burning on the surface of an accreting neutron star.

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17
Q

What are the possible outcomes of mass transfer in binary systems?

A

Nova, Type-I SN, X-ray burst, gamma-ray burst depending on the components (e.g., star+WD, star+NS, star+BH).

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18
Q

How bright is a supernova compared to a nova?

A

Supernova is over a million times brighter than a nova, reaching luminosities of a billion suns.

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19
Q

Why are Type-I supernovae considered cosmic yardsticks?

A

Because all Type-I SN reach the same peak luminosity, 9×10^34 W, due to uniform explosion conditions.

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20
Q

What is a standard candle and how is Type-I SN used as one?

A

An object with known absolute brightness used to measure distance by comparing to apparent brightness.

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21
Q

What is the energy source for the Sun?

A

Nuclear fusion.

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22
Q

What is the relation between mass and energy?

A

E = mc², where energy equals mass times the speed of light squared.

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23
Q

What is an electron volt (eV)?

A

It is the energy gained by an electron when pushed by a potential difference of 1 volt. 1 eV = 1.602 x 10^-19 J.

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24
Q

What is the Q value in nuclear reactions?

A

It is the change in total mass energy of a system, positive when energy is released.

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25
What is the PP-chain reaction?
A 3-step fusion process in stars, converting hydrogen to helium and releasing energy in the form of gamma rays and neutrinos.
26
Why is iron the limit for fusion in stars?
Fusion of iron does not release energy; instead, it consumes it, triggering core collapse.
27
What are the remnants of a high-mass star explosion?
They can be neutron stars (if core <3 solar masses) or black holes (if >3 solar masses).
28
What is the HR diagram used for?
It plots luminosity against temperature and helps classify stars and understand stellar evolution.
29
What causes Doppler shifts in exoplanet studies?
The motion of stars due to gravitational tug from orbiting planets.
30
What determines a star's color?
Its surface temperature: cooler stars are redder, hotter stars are bluer.
31
What is a pulsar?
A rotating neutron star emitting beams of radiation observed as pulses.
32
What is a protostar?
A collapsing cloud of gas and dust that heats up but hasn’t started fusion yet.
33
What happens when a low-mass star dies?
It ejects outer layers as a planetary nebula, leaving a white dwarf.
34
What is the magnitude scale in astronomy?
A logarithmic scale measuring apparent brightness, where a lower magnitude means a brighter object.
35
How does spectroscopic parallax measure distance?
By comparing a star’s spectral class and apparent magnitude to determine luminosity and distance.
36
What is electromagnetic radiation?
Transmission of energy through space via varying electric and magnetic fields.
37
What does the equation E = hf represent?
The energy of a photon, where h is Planck’s constant and f is frequency.
38
What generates Earth's magnetic field?
The rotating molten core of Earth.
39
How did the Moon form?
Likely from a giant impact between Earth and a Mars-sized object.
40
What is the nebular theory?
A model explaining the formation of the solar system from a collapsing cloud of gas and dust.
41
What is the frost line in planet formation?
The distance from the Sun where it was cold enough for ices to form.
42
What is the Doppler Effect?
The change in frequency or wavelength of a wave in relation to an observer moving relative to the source.
43
What does a red shift indicate?
An object is moving away from the observer.
44
What do spectral lines tell us?
They identify the elements in a star or gas.
45
What is an absorption line?
A dark line where light at a specific wavelength has been absorbed by a substance.
46
What are meteoroids, meteors, and meteorites?
Meteoroids are space rocks; meteors are streaks seen in the sky; meteorites reach Earth's surface.
47
Where do most comets originate?
Kuiper Belt or Oort Cloud.
48
What is the habitable zone?
The distance from a star where conditions may allow liquid water.
49
What percentage of solar system mass is in the Sun?
0.9990000000000001
50
What causes tidal forces?
Differences in gravitational pull on different parts of a body.
51
What is tidal locking?
When an object's orbital and rotational periods match, showing the same face.
52
What is linear momentum?
The product of an object's mass and velocity.
53
What is angular momentum?
The rotational equivalent of linear momentum, defined as L = Iω.
54
What is mechanical work in physics?
Work done when a force causes displacement. W = F·d·cos(θ)
55
What is the Work-Kinetic Energy Theorem?
The net work done on an object equals its change in kinetic energy: Wnet = ΔK.
56
What is gravitational potential energy near Earth's surface?
Ug = mgh, an approximation valid only near Earth's surface.
57
What is the escape speed from Earth?
About 11.2 km/s.
58
What is total mechanical energy in orbit?
E = K + U = -GMm/2a for elliptical orbit, constant for bound motion.
59
What is non-conservative work?
Work done by forces like friction, altering mechanical energy: ΔE = Wnc.
60
What is the expression for gravitational potential energy at large distances?
Ug = -GMm/r.
61
Why do astronauts appear weightless on the ISS?
Because both they and the station are in free fall; gravity is present but there's no normal force.
62
What is the equivalence principle?
It's impossible to distinguish between gravitational acceleration and acceleration from motion.
63
What defines the Schwarzschild radius?
The radius where escape speed equals the speed of light: Rs = 2GM/c².
64
What is the event horizon?
The boundary of a black hole beyond which nothing, not even light, can escape.
65
What is gravitational lensing?
The bending of light around massive objects due to curved spacetime.
66
What causes gravitational time dilation?
Clocks run slower in stronger gravitational fields.
67
What is a wormhole?
A theoretical bridge through spacetime connecting distant points.