What limits the ability to directly image distant objects with telescopes?

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Discussion Overview

The discussion revolves around the limitations of telescopes in directly imaging distant objects, such as planets in other galaxies. It addresses theoretical and practical challenges related to resolution, signal detection, and environmental factors affecting observations.

Discussion Character

  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions whether light collection is the primary issue in imaging distant objects.
  • Another participant identifies two main limits: resolution, which is dependent on the diameter of the telescope mirror, and signal limit, which relates to the telescope's area and the noise in the detector over time.
  • A participant notes that ground-based telescopes face additional challenges due to the presence of local and astronomical light sources, which can wash out faint images during long integrations.
  • It is mentioned that even space-based telescopes are ultimately limited by zodiacal light, which is light reflecting off dust in the solar system.

Areas of Agreement / Disagreement

Participants present multiple competing views regarding the limits of telescopes, with no consensus reached on which factor is the most significant or how they interact.

Contextual Notes

Participants discuss various factors affecting telescope performance, including resolution and environmental light interference, but do not resolve the complexities of these interactions or their implications for imaging distant objects.

Holocene
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Why can't a telescope be built that has the capability of directly imaging extremely far away objects...say a planet in another galaxy?

Is light collection the issue?
 
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There are two limits.
1, Resolution - this depends only the diameter of the mirror ( assuming you are in space - on Earth you are limited by the atmosphere). The largest current telescopes would resolve the largest nearby stars.
To resolve stars in nearby galaxies would require telescope appertures the size of the Earth.

2, Signal limit - this depends on the area of the telescope and the noise in the detector * the length of the observation. We can detect quasars (very bright galaxies) out to pretty much the edge of the observable universe. The only limit for individual stars would be the size of the telescope and how long you are prepared to observe for.
 
For ground-based telescopes, there is an additional issue in seeing faint objects. The sky itself is not totally dark, due to the diffusion of local and astronomical light sources. So, if you're integrating for a long time to try to see an extremely faint object, tou'll evetually end up with an image that's totally washed out.
 
Even for space based telescopes the ultimate limit is probably zodiacal light. This is light reflecting off dust left arounf in the solar system.
 

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