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Learn about the history of telescopes and the function of refracting and reflecting optical telescopes.
Astronomy comes from the Greek words “astron” meaning ‘star’ and “nomos” meaning ‘law.’ It is the study of everything that exists beyond the Earth. It is really all about the study of light. Whether you are doing research, or just gazing up at the night sky, everything that you learn comes in the form of light. On a clear dark night, there is a lot to see! Long ago, astronomers used to try to document it all with the naked eye. But the human eye is not good at seeing details of dim and distant objects. There is much we cannot see with our eyes alone.
A is a tool that makes far off things look up-close and bright. The invention of the first telescope is a little sketchy. Most people believe that Galileo Galilei invented the first telescope in 1609. But people knew how to build telescopes before that. We just do not have any evidence before Galileo. The earliest telescopes we know of were made in 1608 by various optical craftsmen in the Netherlands. One of them, Hans Lippershey, publicized his design well enough that news reached Galileo in Italy in 1609. When Galileo heard of the existence of a telescope, he built his own. Within a year he had improved Lippershey’s design. And his name became associated with the first telescope. Galileo’s used his telescope to make observations of Jupiter’s largest moons.
In 1923, Edwin Hubble used the most powerful telescope on Earth at the time to look at the Andromeda Galaxy. He is the person after whom the famous space telescope is named. Astronomers knew that the Andromeda Galaxy was made up of stars. But it was Hubble who was able to measure how far away it is. Astronomers had already figured out the rough size of the Milky Way. Hubble used that data to calculate that the Andromeda Galaxy was at least ten times further away than the edge of our galaxy. This discovery led to further observations that helped astronomers find other galaxies. It also helped to expand our ideas about the Universe.
How Do Telescopes Work?
So how exactly do telescopes work? Let's consider a basic telescope. If you were looking to buy a telescope, a knowledgeable friend might tell you that there are two basic designs. There are refracting telescopes (refractors) and reflecting telescopes (reflectors).
Refracting telescopes are the long, tube-shaped telescopes which you might imagine Galileo using. Refractors use lenses to refract (bend) incoming light through a tube to a focal point. Refractors typically have two lenses. The objective lens is the lens at the front of the telescope through which the light passes. The eyepiece or lens is the lens, which magnifies the image.
Reflecting telescopes use mirrors instead of lenses to light to a focal point. Reflectors have two mirrors. The primary mirror is the big curved mirror at the back that starts to focus the light. The secondary mirror is the smaller mirror at the front that redirects the light towards your eye. Reflectors also have eyepiece lenses.
It's not really fair to say which type of telescope is 'better’. They both have their advantages and disadvantages. It depends on what you want to look at. Whether you want to take pictures, if you want portability, etc. Most modern observatories, which are buildings containing telescopes, use reflectors. This is because their telescopes are so huge! Their size allows for a lot of light to pass through them/ For telescopes that size, the weight of the lenses and the length of the tube makes refractors impractical.
There are two other important aspects of telescopes. These are the aperture and focal length (see above). The aperture of the telescope is the diameter of the opening on the front. The bigger the aperture the greater the amount of light that can enter the telescope. The pupil in your eye is your body's aperture. It can only open a few millimetres. Optical telescopes rarely have apertures smaller than 8 cm. Large telescopes in observatories can have apertures that are greater than 10 m in diameter! Since the dimmest objects in the universe do not give us a lot of light to work with, we need telescopes with big apertures to collect enough light from the object to see them!
Focal length is the length from the aperture to the focal point in the telescope. The longer the focal length, the smaller the patch of sky you can see. The upside is that longer focal lengths allow for greater possible magnification. Focal length is another advantage for reflectors. Since refractors bend light down their tube, the tube has to be at least as long as the focal length. Reflectors, on the other hand, use mirrors to reflect light. This means that they can be shorter than their focal length. The light still travels the full focal length, but the tube itself does not need to be as long. The eyepiece is near the focal point of the primary mirror to magnify the image.
Therefore, you might be thinking that every telescope should have the biggest aperture and longest focal length possible. Aside from limitations such as cost and storage space, there are other reasons why this is not a good idea. First, for anyone who studies our solar system, aperture really is not that important. Most of the planets are visible using even the smallest telescopes. Objects like the Moon are so bright that too large an aperture may be an issue. Secondly, even smaller-sized telescopes, such as ones with apertures of 20 cm, are capable of seeing hundreds of galaxies and nebulae, some of which are almost a hundred million light-years away! Galaxies are large systems of stars, gases and dust and nebulae are interstellar clouds of dust and hydrogen gas. It can actually help to use low magnification for these types of objects. Objects, such as star clusters and galaxies can be too large to 'zoom in' on. The Andromeda Galaxy, for example, appears to be larger than the full moon in the night sky!