Telescope Resolution for AGN Accretion Disk

In summary, an Active Galactic Nucleus (AGN) is a type of galaxy with a supermassive black hole at its center that is fueled by gas and dust in a rotating accretion disk. These disks are typically a few parsecs in diameter and can be best detected at long wavelengths. For a nearby AGN located 3.3x106 parsecs from Earth, with an accretion disk of 2 parsecs in diameter, a telescope with a diameter of 1.22 λ/D would be needed to resolve the disk at a wavelength of 10 μm, and a telescope with a diameter of 1.22 λ/D would be needed to resolve the disk at a wavelength of 21cm.
  • #1
wtaylor
2
0
[SOLVED] Telescope Resolution

Homework Statement


An Active Galactic Nucleus (AGN) is fueled by gas and dust in a rotating
accretion disk that is streaming onto a supermassive black hole in the center of the
galaxy. These accretion disks are typically a few pc in diameter and are best detected
at long wavelengths (to penetrate the dusty envelopes of these galactic centres). One
of the nearest AGNs is 3.3x106 pc from Earth and is powered by an accretion disk
that is 2 pc in diameter.
a) What size telescope would you need to resolve this accretion
disk at a wavelength of 10 μm and also at 21cm?

Homework Equations


p(′′) = 1/D(pc)

θ (") = 2.5 × 10^5 λ/D

The Attempt at a Solution


The only way I can see to find this is to use the parallax equation to find the size of the accretion disk in " and then use the angular resolution formula to find the telescopes diameter using each wavelength. But I am not sure if this will work considering that seems like an improper use of the parallax formula. Could someone give me a hint as to whether I am going in the right direction?
 
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  • #2
You don't need the paralax formula since the distance and diameter are both given in parsec. You just need to work out the angular extent and then use 1.22 lambda/D for the diffraction limit, at 10um telescopes are pretty much diffraction limited.
 
  • #3
Awesome, got it. Thanks alot.
 
  • #4
Carefull, the 1.22 factor is the half angle (ie the radius of the source)
 

1. What is Telescope Resolution?

Telescope resolution refers to the ability of a telescope to distinguish between two closely spaced objects or details in an image. It is a measure of the smallest angular separation that can be resolved by the telescope.

2. How is Telescope Resolution related to AGN Accretion Disk studies?

Telescope resolution is crucial for studying AGN (Active Galactic Nuclei) accretion disks as it allows scientists to observe and analyze the fine details and structures within the disks. Higher resolution telescopes can provide more detailed and accurate data for studying these disks.

3. What factors affect Telescope Resolution for AGN Accretion Disk studies?

The main factors that affect telescope resolution for AGN accretion disk studies are the size and quality of the telescope's primary mirror, atmospheric conditions, and the wavelength of light being observed. Other factors include the telescope's optics, detector technology, and data processing techniques.

4. Can the resolution of a telescope be improved for AGN Accretion Disk studies?

Yes, there are several techniques that can be used to improve the resolution of a telescope for AGN accretion disk studies. These include adaptive optics, which corrects for distortions caused by Earth's atmosphere, and interferometry, which combines the light from multiple telescopes to increase the resolving power.

5. How does Telescope Resolution impact our understanding of AGN Accretion Disks?

The resolution of a telescope plays a critical role in our understanding of AGN accretion disks. Higher resolution allows scientists to observe finer details and structures within the disks, leading to a better understanding of their physical properties and dynamics. It also allows for more accurate measurements of key parameters, such as the mass and accretion rate of the black hole at the center of the disk.

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