ASTRO 4 Final

48 flashcardsby Jamie
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1
What is an Active Galactic Nucleus (AGN)
The central region of a galaxy emitting extraordinarily high energy, powered by accretion (accumulated matter) onto a supermassive black hole.
2
What evidence supports that AGN are powered by black holes
Compactness of energy source, Broad spectral lines from gas moving at high velocities., Relativistic jets aligned with theoretical models of black hole magnetospheres.
3
How does the viewing angle affect observed properties of an AGN
The Broad Line Region (BLR) and dusty torus can block or reveal certain emissions depending on orientation.
4
Why do AGN exhibit rapid variability, and what does it indicate about their size
Rapid fluctuations indicate a compact emission region. Timescales of variability are proportional to the size of the region, constrained by the light travel time formula t=R/c
5
How do radio jets form in AGN
Formed by twisted magnetic fields near the black hole, which accelerate charged particles outward.
6
What properties of AGN strongly suggest they are powered by accreting black holes
Extreme luminosity, small size, rapid variability, emission across a wide range of wavelengths, and the presence of radio jets all point to a black hole as the energy source.
7
Extreme Luminosity
Emits up to a trillion times the Sun's energy.
8
Small Size:
Emission originates from a region smaller than a light-month.
9
Rapid Variability
Changes in brightness over short timescales (days or weeks).
10
Wide Wavelength Range
Emits radiation from radio waves to gamma rays.
11
Radio Jets
High-energy jets of matter ejected perpendicular to the accretion disk.
12
What components make up the structure of an AGN
A supermassive black hole, accretion disk, broad line region (BLR), dusty torus, and relativistic jets.
13
Relativistic Jets
Narrow streams of particles moving near the speed of light.
14
What is the relationship between an AGN’s size and its rapid variability
Short variability timescales suggest a compact region, with size limited by the formula t=R/ct = R/ct=R/c (time equals size divided by the speed of light).
15
How do magnetic fields contribute to the formation of AGN radio jets
Twisted magnetic fields near the black hole accelerate particles to near-light speeds, forming narrow jets that emit synchrotron radiation.
16
What is superluminal motion, and how does it occur
Apparent faster-than-light motion observed in relativistic jets. It occurs by a relativistic effect where a jet moving close to the speed of light and pointed toward Earth appears to move faster due to projection effects.
17
What mechanisms feed an AGN
Galaxy mergers, bars in spiral galaxies, and cooling flows funnel gas to the central black hole.
18
What is superluminal motion, and why does it occur
Superluminal motion is an illusion caused by jets moving close to the speed of light toward us, compressing emission times.
19
How do AGN feeding mechanisms differ between galaxy types
Spiral galaxies use bars to drive gas inward, while elliptical galaxies rely on gas from galaxy mergers.
20
What is Hubble’s Law, and how is it calculated
velocity = Hubble constant × distance. Hubble’s Law states that a galaxy’s recession velocity is proportional to its distance.
21
What is the relationship between the Hubble constant and the Universe’s age
A larger hubble constant​ means a younger Universe.
22
How does cosmological redshift differ from the Doppler effect
Cosmological redshift is Caused by the stretching of space, light wavelengths. the Doppler Effect is from wavelength changes due to relative motion through space.
23
Homogeneous and Isotropic Universe
Uniform distribution of matter.
24
Cosmic Microwave Background (CMB)
Radiation from the early Universe.
25
Primitive Galaxies and Type Ia Supernovae
Indicators of cosmic evolution and expansion.
26
Why are Type Ia supernovae considered standard candles
Type Ia supernovae have predictable brightness/luminosity, allowing accurate cosmic distance measurements.
27
What evidence supports the Big Bang theory
A homogeneous and isotropic Universe, cosmic microwave background (CMB), and observations of distant galaxies and Type Ia supernovae.
28
What is the origin of the cosmic microwave background (CMB)
The CMB comes from photons as faint radiation released 380,000 years after the Big Bang, when electrons and protons combine to form neutral hydrogen.
29
What are quasars, and why are they significant
Extremely luminous AGN from the early Universe, representing the growth phase of supermassive black holes. They help us study early galaxy formation and cosmic conditions.
30
Why were quasars more common in the past
Abundant gas and frequent galaxy mergers in the dense early Universe fueled quasar activity.
31
What are gravitational waves, and how are they created
they’re ripples in spacetime caused by accelerating massive objects, like merging black holes or neutron stars.
32
What happens to objects as gravitational waves pass through them
they stretch and compress due to spacetime distortion.
33
How has LIGO contributed to astrophysics
it confirmed black hole mergers and provided direct evidence of gravitational waves, validating Einstein's theory of general relativity.
34
What is Hawking radiation, and how does it occur
it’s radiation emitted by black holes when virtual particle pairs near the event horizon separate, with one escaping as radiation.
35
How does field theory apply to cosmology
it combines quantum mechanics and relativity to explain fundamental forces, dark energy, and the Universe’s evolution.
36
What role does dark energy play in cosmic expansion
it causes the accelerated expansion of the Universe, driving the Big Freeze scenario.
37
What evidence supports the Big Freeze as the most likely scenario
Observations of dark energy and the Universe’s accelerating expansion.
38
Why do we sometimes not see broad lines in accreting AGN
Broad line regions can be obscured by the dusty torus depending on the viewing angle.
39
What two galaxy properties did Hubble compare to discover the expansion of the Universe
he compared the recession velocity and distance of galaxies to determine the relationship described by Hubble’s Law.
40
How does redshift indicate the Universe has expanded
a redshift of 10% implies the Universe has expanded by 10% since the light left the galaxy.
41
Where did the Big Bang happen
it occurred everywhere in the Universe as space itself expanded
42
Why do we still observe the CMB today
The CMB’s photons have been traveling through space, reaching us as faint microwave radiation.
43
How do we study protogalaxies despite their age
By observing light that has taken billions of years to travel to us, we see these galaxies as they were in the distant past.
44
Why is it a challenge to explain 1.5 billion solar mass black holes only 600 million years after the Big Bang
bc black holes of this size would require rapid growth unlikely to occur through stellar mass black hole mergers alone.
45
How does the Event Horizon Telescope (EHT) capture images of black holes
it uses light from the accretion disk bent around the black hole’s event horizon to create images of the shadow.
46
What is spaghettification
A phenomenon where tidal forces near a black hole stretch objects into long, thin shapes.
47
How are black holes detected
Through accretion disk emissions, gravitational interactions, and X-ray or infrared observations.
48
Antimatter
consists of particles with opposite charges and quantum numbers to their matter counterparts. positron is the antimatter of the electron
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