There has always been a fascination about the universe, a sense of intrigue and wonder in the endless twinkling stars and swirling galaxies that have been painted across the heavens above, but how are we meant to close the gap between our reality and the vastness of space? The way in which we do so has been through a single invention that has enabled us to peer further into space than ever before and reveal the cosmic secrets of the Universe before us. The telescope has been the answer.
At its core is a telescope: a piece of equipment that brings a distant object up close and sharp, a window on the cosmos. It works by collecting light with its primary components.
The telescope itself is a multifaceted world, with each type of instrument tailored to different kinds of observation.
Getting from the selection of a celestial object to the bright glow of its magnified image is a process of detail and precision:
It would be difficult to overstate the importance of the telescope to astronomy. No other instrument has allowed us to make so many new discoveries. It has enabled us to tabulate our growing inventory of exoplanets. It has allowed us to peer back into the very onset of time at the edges of our visible Universe. It has enabled us to detect supernovae at the edge of the observable Universe. It has allowed us to probe and map the external galaxies that surround us. Even though we build bigger and better telescopes every day, the next frontier of astronomical discovery goes far beyond simply expanding the physical capabilities of our instruments. In the hands of our modern astronomers, telescopes are more than just instruments – they are torches. They illuminate the path to answers about where we came from and the architectural design of the Universe.
Even the modern behemoth observatories and spaceborne telescopes that today are dwarfing their forebears trace their ancestry back to this simple yet highly effective design. Every hurdle in its development – every refinement of optics and mechanics, every addition to the scrubbing arsenal – has helped to reveal a little more of the heavens to our puzzled eyes.
Lenses are the heart of many types of telescopes, and especially of the type of telescope called a refracting telescope designed to focus light entering through a lens. Lenses bend (or refract) the light rays – the photons – that pass through them in such a way that the light rays come together (converge) to a focus at a point. If that point is behind the lens, all the light rays caring about a particular point in space – a star, say – are focused onto the back of the lens. There they converge into an image, as small as an atom and with no thickness at all – in a sense, a mathematical point. If the focus lies in front of the lens, light from different parts of the celestial body align at different distances in front of the lens, thus forming their own point image in three-dimensional space. The light is focused, but now it forms a tiny, speckless point that is not located behind the lens but rather another pea-sized point, now in front of the lens. Brilliant. Viewing the delicate Saturnian rings or the far-off diffuse light from a newly born star, titanic lenses are quietly at work, gathering the beauty and glare of the Universe, converging them into manageable mathematical points, and bringing them down to the size of a single photon.
Telescopes in astronomy has been on a remarkable intellectual journey over the lifespan of this wonder tool. From crude spherical mirrors to perfect paraboloids, perhaps in the future we will succeed in making an ‘aristotelian’ telescope – or in conjunction with optical illusions, a mirror that never appears catenary! Indeed, a telescope is a mirror, a reflection of all our efforts to find our place in the Universe. What’s on the other side of the telescope? It’s our yearning to know.
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