What are the two main types of optical telescopes and how are they different?
The two major types of optical telescopes are
Despite being Earth-based, the twin telescopes at the Keck Observatory can see farther into space than the famous Hubble Telescope. This means that around a quarter of the observations made by U.S. astronomers are achieved using Keck, and it is considered the most scientifically productive of all land telescopes.
Optical telescopes collect visible light. The three main types are reflecting telescopes, refracting telescopes, and catadioptric telescopes.
X-ray and gamma ray telescopes detect very short wavelength of light and look at the sun, stars and supernovas. Reflecting telescopes see visible light and they see things way out in space. Refracting telescopes detect visible light; they see things out in space but not as far as reflecting telescopes.
Most telescopes will fall into one of three categories: refractors (which use lenses to bend light into focus), reflectors (which use mirrors that reflect light into focus), and catadioptric or compound scopes, (which use a combination of both lenses and mirrors).
Some telescopes are classified by the task they perform; for example Solar telescopes are all designs that look at the Sun, Dobsonian telescopes are designed to be low cost and portable, Aerial telescopes overcame the optical shortcomings of 17th-century objective lenses, etc.
There are three primary types of optical telescope: Refractors ( Dioptrics) which use lenses, Reflectors ( Catoptrics) which use mirrors, and Combined Lens-Mirror Systems ( Catadioptrics) which use lenses and mirrors in combination (for example the Maksutov telescope and the Schmidt camera).
The telescope you want has two essentials: high-quality optics and a steady, smoothly working mount. And all other things being equal, big scopes show more and are easier to use than small ones, as we'll see below. But don't overlook portability and convenience — the best scope for you is the one you'll actually use.
Name | Space agency | Observing location |
---|---|---|
Astron | IKI | Earth orbit (2,000–200,000 km) |
Hubble Space Telescope | NASA & ESA | Earth orbit (586.47–610.44 km) |
Broad Band X-ray Telescope / Astro 1 | NASA | Earth orbit (500 km) |
Extreme Ultraviolet Explorer (EUVE) | NASA | Earth orbit (515–527 km) |
The three main types of telescopes are refracting telescopes, reflecting telescopes, and catadioptric telescopes. There are many variations and hybrid designs for each type.
What is the difference between visible light telescope and infrared telescope?
Infrared telescopes do not differ significantly from reflecting telescopes designed to observe in the visible region of the electromagnetic spectrum. The main difference between the two types is in the physical location of the infrared telescope, since infrared photons have lower energies than those of visible light.
Radio telescopes have to be much larger than optical telescopes because the wavelengths of radio waves are so much larger than the wavelengths of visible light. Radio wavelengths are between λ ≈ 3 km to λ ≈ 1 cm, while visible light wavelengths are between λ ≈ 4 x 10-7m (violet) and λ ≈ 7 x 10-7m (red).
Types of astronomy
In the past century or so, astronomy has been broadly split into two camps — observational astronomy (using telescopes and cameras to collect data about the night sky) and theoretical astronomy (using that data to analyze, model and theorize about how objects and phenomena work).
(i) Astronomical telescopes are used for viewing distant stars and planets whereas terrestrial telescopes are used for viewing distant objects on earth. (ii) The final image in the astronomical telescope is inverted whereas that in the terrestrial telescope is erect.
To reiterate: Telescopes come in two basic flavors—those with a high plus eyepiece lens, and those with a high minus eyepiece lens. High-plus-eyepiece telescopes are called astronomical (or Keplerian) telescopes; and high-minus-eyepiece telescopes are called Galilean (or terrestrial) telescopes.
Refractors generally have the edge over reflectors for a quality image, both from the standpoint of lens/mirror quality and precision optical mountings, and lack of central obscurations. Equally important in a choice of telescope type is the focal length and the resulting field of view.
The mirrors or lenses in a telescope are called the “optics.” Really powerful telescopes can see very dim things and things that are really far away. To do that, the optics—be they mirrors or lenses—have to be really big. The bigger the mirrors or lenses, the more light the telescope can gather.
Its most common form is the Newtonian reflector (invented by Isaac Newton), with a specially curved concave (dish-shaped) primary mirror at the bottom end of the telescope.
- Refractor Telescopes.
- Reflector Telescopes.
- Dobsonian Telescopes.
- Maksutov-Cassegrain Telescopes.
Great Observatories, a semiformal grouping of four U.S. satellite observatories that had separate origins: the Hubble Space Telescope, the Compton Gamma Ray Observatory, the Chandra X-ray Observatory, and the Spitzer Space Telescope.
What are the famous optical telescopes?
Name/Observatory | Aperture m | Site and/or Observatory |
---|---|---|
Keck 2 | 10 m | Mauna Kea Observatory, Hawaii |
Hobby-Eberly Telescope (HET) | 9.2 m | McDonald Observatory, Texas |
Subaru (JNLT) | 8.2 m | Mauna Kea Observatory, Hawaii |
VLT 1 (Antu) | 8.2 m | Paranal Observatory, Chile |
Reflecting Telescopes
They do not require as much light to form a clear image as refracting telescopes, and so a small reflecting telescope can form a clear image of things that are very far out in space. Today, the vast majority of telescopes used in research are reflecting telescopes and not refracting telescopes.
telescope, device used to form magnified images of distant objects. The telescope is undoubtedly the most important investigative tool in astronomy. It provides a means of collecting and analyzing radiation from celestial objects, even those in the far reaches of the universe.
Advantages of radio telescopes
Radio telescopes can be used in the daytime as well as at night. Radio waves are unaffected by the dust particles in space. Light waves are scattered by these dust particles and so never make it to Earth for detection.
Hubble, the observatory, is the first major optical telescope to be placed in space, the ultimate mountaintop. Above the distortion of the atmosphere, far far above rain clouds and light pollution, Hubble has an unobstructed view of the universe.
Two examples of a space telescope would be an optical telescope and a refracting telescope. Two examples of a space probe would be Chandra X-ray Observatory and the swift.
The James Webb Space Telescope – also called JWST or Webb – is NASA's largest and most powerful space science telescope.
The two most important properties of a telescope are its light-collecting area and its angular resolution. A telescopes light-collecting area tells us how much total light it can collect at one time.
IR telescopes can be much smaller than radio telescopes to have the same resolving power. IR telescopes have lower resolving powers than those of optical telescopes of the same size.
Infrared waves have longer wavelengths than visible light and can pass through dense regions of gas and dust in space with less scattering and absorption.
What is the difference between infrared and ultraviolet?
What is the difference between Ultraviolet (UV) and Infrared (IR) Infrared is the heat you feel in the sun and UV is the burn you get in the sun. Ultraviolet radiation is more energetic than infrared. But “hotter” is a somewhat informal term.
The wavelengths of radio waves range from a few millimeters (tenths of inches) to hundreds of kilometers (hundreds of miles). Visible light, for comparison, has wavelengths in the 400 to 700 nanometer range, about 5,000 times shorter than the shortest wavelength radio waves.
Visible light has a wavelength that ranges from 380 nm – 750 nm on the electromagnetic spectrum while infrared light is just beyond it, ranging from 700 nm – 1 mm, the start of the non-visible portion of the spectrum. As a result, infrared cannot be seen except with special equipment like a security camera.
The different types of radiation are defined by the the amount of energy found in the photons. Radio waves have photons with low energies, microwave photons have a little more energy than radio waves, infrared photons have still more, then visible, ultraviolet, X-rays, and, the most energetic of all, gamma-rays.
Types of Galaxies
Astronomers classify galaxies into three major categories: elliptical, spiral and irregular. These galaxies span a wide range of sizes, from dwarf galaxies containing as few as 100 million stars to giant galaxies with more than a trillion stars.
There are two basic types of telescopes, refractors and reflectors. The part of the telescope that gathers the light, called the objective, determines the type of telescope. A refractor telescope uses a glass lens as its objective.
In our Solar System, astronomers often divide the planets into two groups — the inner planets and the outer planets. The inner planets are closer to the Sun and are smaller and rockier. The outer planets are further away, larger and made up mostly of gas.
In an astronomical telescope, The eyepiece has greater power while a smaller aperture. and, the objective has lower power with a longer aperture so, by using 4 as objective and L3 are eyepiece, the best possible magnification, m=PP=310=3.
The three main types of telescopes are refracting telescopes, reflecting telescopes, and catadioptric telescopes.
The two important properties of a telescope are light-gathering power (light bucket) and resolving power. Light bucket improves out ability to see distant or faint objects and is proportional to the square of the radius of the primary mirror.
What is the difference between optical telescopes and other telescopes?
A radio telescope is designed to detect radio waves from distant sources, while an optical telescope is designed to detect visible light (and sometimes UV or IR radiation).
(i) Astronomical telescopes are used for viewing distant stars and planets whereas terrestrial telescopes are used for viewing distant objects on earth. (ii) The final image in the astronomical telescope is inverted whereas that in the terrestrial telescope is erect.
To reiterate: Telescopes come in two basic flavors—those with a high plus eyepiece lens, and those with a high minus eyepiece lens. High-plus-eyepiece telescopes are called astronomical (or Keplerian) telescopes; and high-minus-eyepiece telescopes are called Galilean (or terrestrial) telescopes.
Refractor telescopes utilize specialized lenses that make them a favorite for deep space objects like galaxies and nebulae. In contrast, reflector telescopes are more popular with larger and brighter objects like the Moon and planets because they use mirrors that provide more sensitivity to all wavelengths.
There are three main types of telescopes commonly available to amateur astronomers: refractors, reflectors, and Schmidt-Cassegrains (here is a nice description of the difference between a refractor and a reflector).
The focal length of a lens depends on the curvature of the lens surface. A basic refracting telescope consists of two lenses. The larger, primary lens is called the objective, while the second lens, the eyepiece, is used to view the image produced by the objective.
Both types are used to gather and focus electromagnetic radiation to be observed by human eyes or recorded on photographs or in computers. In both cases, the image formed at the focus is viewed with a small magnifying lens called an eyepiece.
The telescope is undoubtedly the most important investigative tool in astronomy. It provides a means of collecting and analyzing radiation from celestial objects, even those in the far reaches of the universe.
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