A mirror instead of and objective lens (:
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Reflecting telescopes use mirrors to gather and focus light, while refracting telescopes use lenses. Reflecting telescopes tend to be more compact and easier to support larger apertures, making them popular for professional astronomical research. Additionally, reflecting telescopes are less affected by chromatic aberration compared to refracting telescopes.
Most optical telescopes used by professional astronomers are located on mountains or remote locations away from city lights to minimize light pollution and atmospheric disturbances. Some observatories, such as those in Chile and Hawaii, are known for having excellent observing conditions due to high altitudes and clear skies. Telescopes are also placed in space, like the Hubble Space Telescope, to avoid atmospheric interference.
A disadvantage of having a telescope in space is the high cost involved in building, launching, and maintaining it. Additionally, servicing the telescope in space is much more complex and limited compared to telescopes on Earth. Lastly, space telescopes are vulnerable to space debris and solar radiation which can potentially damage their delicate instruments.
Scientists often build telescopes on top of mountains or in deserts where the air is clearer and there is less light pollution. This helps to minimize atmospheric interference and optimize the visibility of celestial objects.
to increase the resolution of the telescope system. By having multiple telescopes spread out, the system can simulate a larger telescope, which allows for more detailed observations of celestial objects. Additionally, this setup improves the sensitivity of the telescope array, enabling it to detect fainter signals.
Telescopes used for astronomy typically do not need to make the image right-side up because it doesn't affect the data or observations collected. In fact, having an inverted image is actually common in many optical systems due to the way the lenses bend and focus light. Telescopes prioritize light-gathering ability and image quality for observing celestial objects, rather than the orientation of the image.