Telescope Resolution for AGN Accretion Disk

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Homework Help Overview

The discussion revolves around calculating the necessary telescope size to resolve the accretion disk of an Active Galactic Nucleus (AGN) at specific wavelengths. The problem involves understanding the relationship between distance, diameter, and angular resolution in the context of astrophysics.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants explore the use of the parallax equation and angular resolution formulas to determine the telescope diameter needed for resolution at given wavelengths. There is uncertainty about the appropriateness of the parallax formula in this context.

Discussion Status

Some participants have provided guidance on the calculations, suggesting that the parallax formula may not be necessary and recommending the use of angular extent and diffraction limit equations instead. However, there is still some confusion regarding the interpretation of the diffraction limit factor.

Contextual Notes

The problem is constrained by the specific distances and diameters provided in parsecs, and there is an ongoing discussion about the correct application of formulas related to angular resolution.

wtaylor
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[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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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.
 
Awesome, got it. Thanks a lot.
 
Carefull, the 1.22 factor is the half angle (ie the radius of the source)
 

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