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Telescopes. Types and how they work

15/04/2026

The online telescope simulations on this page show how a telescope works. We will discover the existing types of telescopes, refracting (Keplerian and Galilean) and reflecting (Newtonian) telescopes, and we will see the working principles of each of them.

STEM OnLine mini dictionary

Chromatic Aberration

Optical defect common in refractors where colors do not focus at the same point, creating colored edges.

Eyepiece

Lens or system of lenses located near the focus that magnifies the image formed by the objective.

Focal Length

Path that light travels from the objective to the point where the sharp image is formed.

Mount

Mechanical system that supports the telescope and allows its movement to point at and track celestial objects.

Opening

Diameter of a telescope’s primary objective, which determines its light-gathering capacity.

Radio Telescope

Specialized antenna that captures radio waves from astronomical sources in space.

Reflecting Telescope

Instrument that uses curved mirrors instead of lenses to collect and focus light.

Refracting Telescope

Type of telescope that uses converging lenses to focus light and form the image.

Resolution

Ability of a telescope to distinguish two objects that are very close to each other in the sky.

Telescope

Optical instrument designed to observe distant objects by collecting electromagnetic radiation.

What is a telescope

A telescope is an optical instrument used to observe and study distant objects in space, such as stars, planets, galaxies and other celestial bodies. Through their design and features, telescopes allow astronomers to gather light and increase the visibility of astronomical objects, revealing details and phenomena that would otherwise be invisible to the naked eye.

How a telescope works

The operation of a telescope is based on the collection and concentration of light from distant objects. Depending on the design, telescopes use lenses or mirrors to capture this light and project it to a focal point, where a magnified image is generated. Once the light is collected, the eyepiece allows detailed observation, magnifying the image to show features that are not visible to the naked eye. This process is essential for studying celestial bodies that would otherwise be too far away or faint to be detected with the human eye.

The size of the telescope is a critical factor in its performance. The larger the diameter of the objective or main mirror, the more light it can collect and, therefore, the higher the quality of the image obtained. Professional telescopes typically have diameters of several meters and are found in astronomical observatories around the world.

Types of telescopes. Refracting telescopes and reflecting telescopes

There are two main types of telescopes: refractors and reflectors. Refracting telescopes use lenses to collect and focus light, while reflecting telescopes employ curved mirrors. Both types have advantages and disadvantages, and their choice depends on the specific observing objectives.

Innovations in modern telescopes

The most advanced telescopes incorporate additional optical systems to correct aberrations and improve image quality, ensuring more accurate and detailed observation. In addition to light collection, many modern telescopes are equipped with advanced instruments and devices to analyze the light received. These include spectrographs to study the chemical composition of objects, digital cameras to capture high-resolution images, and detectors of electromagnetic waves beyond the visible spectrum, such as X-rays and infrared radiation.

Impact of telescopes on modern astronomy

The development of technology has enabled the use of space telescopes, such as the Hubble Space Telescope, which is located outside the Earth’s atmosphere and can capture sharp, detailed images without the distortions caused by the atmosphere. These space telescopes have revolutionized our understanding of the universe and have provided amazing images of distant galaxies and cosmic phenomena.

The study and observation with telescopes have led to important discoveries in astronomy, such as the identification of exoplanets, the measurement of the expansion of the universe, and the understanding of black holes. Telescopes continue to be fundamental tools for astronomers in their search for answers about the origin, evolution and nature of the cosmos.

In summary, the online telescope simulations on this page are very useful for understanding how a telescope works, check them out and you’re sure to like them!

STEM OnLine mini dictionary

Chromatic Aberration

Optical defect common in refractors where colors do not focus at the same point, creating colored edges.

Eyepiece

Lens or system of lenses located near the focus that magnifies the image formed by the objective.

Focal Length

Path that light travels from the objective to the point where the sharp image is formed.

Mount

Mechanical system that supports the telescope and allows its movement to point at and track celestial objects.

Opening

Diameter of a telescope’s primary objective, which determines its light-gathering capacity.

Radio Telescope

Specialized antenna that captures radio waves from astronomical sources in space.

Reflecting Telescope

Instrument that uses curved mirrors instead of lenses to collect and focus light.

Refracting Telescope

Type of telescope that uses converging lenses to focus light and form the image.

Resolution

Ability of a telescope to distinguish two objects that are very close to each other in the sky.

Telescope

Optical instrument designed to observe distant objects by collecting electromagnetic radiation.

Explore the exciting STEM world with our free, online, simulations and accompanying companion courses! With them you’ll be able to experience and learn hands-on. Take this opportunity to immerse yourself in virtual experiences while advancing your education – awaken your scientific curiosity and discover all that the STEM world has to offer!

Telescope simulations

Refracting telescope (Keplerian and Galilean)


This simulation shows us how a refracting telescope works. A telescope that uses only the refraction of a lens is called a refracting telescope. There are two types, the Galilean telescope and the Keplerian telescope. The Galilean telescope or earth telescope consists of a convex objective and a concave eyepiece. The Keplerian telescope has a convex objective and convex eyepiece. Most astronomical telescopes in use today are Keplerian telescopes, whose operation is as we can see in the first of our online telescope simulations..

Reflecting telescope (Newtonian)


This simulation shows us how a reflecting telescope works. The condensation of a telescope is closely related to the size of the objective lens. This leads to a preference for larger telescopes. However, refracting telescopes cannot be made as large as desired. The telescope that solves this problem is the reflecting telescope, which is currently the most widely used telescope for astronomical observation, and whose operation is the one we can observe in this last of our online telescope simulations..

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A telescope is an optical instrument designed to observe very distant objects in space, such as stars, planets, galaxies and other celestial bodies. Its importance lies in its ability to collect and concentrate light, allowing astronomers to detect details that would otherwise be invisible to the naked eye. By gathering light through lenses or mirrors and directing it toward a focal point, the telescope produces an enlarged image that can be examined through the eyepiece. This process makes it possible to study faint or distant objects that the human eye cannot detect on its own. The size of the telescope plays a crucial role: the larger the diameter of the main lens or mirror, the more light it can collect and the better the resulting image. For these reasons, telescopes are fundamental tools for exploring and understanding the universe.
Telescopes work by collecting and concentrating light from distant objects. Depending on their design, they use lenses—refracting telescopes—or curved mirrors—reflecting telescopes—to direct incoming light toward a focal point where an enlarged image is formed. The eyepiece then allows the observer to view this image in detail. A telescope’s performance depends heavily on the size of its main lens or mirror: a larger diameter means more light can be gathered, resulting in clearer and more detailed images. Modern telescopes include additional optical systems to correct aberrations and enhance image quality. They also incorporate advanced instruments such as spectrographs, digital cameras and detectors capable of capturing electromagnetic radiation beyond visible light, including X‑rays and infrared. These innovations have greatly expanded astronomers’ ability to study the universe with precision.
Because the larger the main lens or mirror, the more light the telescope can collect. Objects in space are extremely far away and often very faint, so a bigger telescope helps capture clearer and brighter images. That’s why professional telescopes have mirrors several meters wide and are installed in observatories.
Refracting telescopes use lenses to gather and focus light, while reflecting telescopes use curved mirrors. Both allow us to observe space, but they work in different ways. The choice between them depends on the type of observation and the characteristics needed in the image.
Because they operate outside Earth’s atmosphere, which distorts light and reduces image quality. A space telescope, like the Hubble, can capture much sharper and more detailed images. Thanks to these instruments, astronomers have made major discoveries about distant galaxies, exoplanets and many other cosmic phenomena.

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