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Telescopes and their Uses
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Schmidt-Cassegrain Telescope
Design: A combination of a spherical mirror and a correcting lens (Schmidt plate). Functionality: Compact design that is popular with amateur astronomers and combines the benefits of refractors and reflectors. Examples of discoveries: Widely used in astrophotography and deep-sky observation.
Adaptive Optics Telescope
Design: Telescopes with systems to reduce the effects of atmospheric distortion. Functionality: Measures the distortions in wavefront and compensates for them in real-time by adjusting mirrors. Examples of discoveries: Detailed observations of stars and galaxies at high angular resolution.
Refracting Telescope
Design: Uses lenses to form an image, with the primary lens being the objective lens. Functionality: Light is bent (refracted) to bring it to a focal point to create an image. Examples of discoveries: Planets' moons, details on planetary surfaces.
Interferometer
Design: Consists of two or more telescopes that combine their signals. Functionality: Increases effective resolution using the principle of interference. Examples of discoveries: The diameter of stars, fine details of celestial objects.
Gamma-Ray Telescope
Design: Detect high-energy gamma rays from cosmic sources. Functionality: Uses detectors like scintillation counters or spark chambers to convert gamma rays into light or an electrical signal. Examples of discoveries: Gamma-ray bursts, pulsars, high-energy particle acceleration in various phenomena.
Space Telescope
Design: A telescope located outside Earth's atmosphere, in space. Functionality: Avoids atmospheric distortion and light pollution enabling clearer and more detailed images. Examples of discoveries: Age and size of the Universe (Hubble Space Telescope), exoplanet atmospheres.
Reflecting Telescope
Design: Employs a single or a combination of curved mirrors that reflect light to form an image. Functionality: Light is gathered and focused using reflective surfaces, usually a parabolic primary mirror. Examples of discoveries: Deep-sky objects like nebulae and galaxies.
Radio Telescope
Design: Essentially a large dish antenna, which detects radio waves from astronomical radio sources. Functionality: Radio waves are focused onto a receiver using a large, parabolic reflector. Examples of discoveries: Cosmic microwave background radiation, mapping of gas clouds in galaxies.
X-ray Telescope
Design: Uses low-angle reflections from nested mirrors to focus X-ray photons from celestial objects. Functionality: Due to X-rays being absorbed by the Earth's atmosphere, these telescopes are placed in space. Examples of discoveries: Black holes, neutron stars, coronae of stars.
Solar Telescope
Design: Specifically designed for observing the Sun. Often has a narrow band filter to allow detailed observations of the solar atmosphere. Functionality: Filter out most of the sunlight to prevent damage to the observer’s eyes and instruments. Examples of discoveries: Solar flares, sunspots, solar granulation.
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