The Hale Telescope is a 5-m reflecting telescope at the Palomar Observatory. Some factors that limit its ability to collect starlight are light pollution, turbulence in the atmosphere, daylight and clouds.
Hubble used, among others, the 100-inch Hooker telescope at Mount Wilson, which could have easily resolved Pluto. The Yerkes observatory managed to (unknowingly) photograph Pluto with only a 40-inch scope, which has about six times less light-gathering ability.
Magnification refers to a telescope's ability to make an object appear larger when viewed through the telescope. It is the degree to which the image of the object is enlarged compared to what is seen with the naked eye.
The ability of a telescope to separate 2 closely spaced stars is called resolving power or angular resolution. This refers to the telescope's ability to distinguish fine details in an image, such as two closely spaced objects.
The size of a reflecting telescope is typically indicated by its aperture, which is the diameter of the primary mirror. Aperture size plays a crucial role in determining the light-gathering ability and resolving power of the telescope.
The Hubble Space Telescope primarily relies on imaging techniques to observe celestial objects, which makes detecting faint exoplanets around distant stars very challenging. Additionally, the telescope's small field of view and limited sensitivity to starlight interference further hinder its ability to directly detect exoplanets. Specialized ground-based observatories and space telescopes like the Kepler Space Telescope are typically used for detecting exoplanets.
diffraction (by a circular apperture)
Hubble used, among others, the 100-inch Hooker telescope at Mount Wilson, which could have easily resolved Pluto. The Yerkes observatory managed to (unknowingly) photograph Pluto with only a 40-inch scope, which has about six times less light-gathering ability.
Magnification refers to a telescope's ability to make an object appear larger when viewed through the telescope. It is the degree to which the image of the object is enlarged compared to what is seen with the naked eye.
By using a Reflective telescope the viewer sees the image of a normal telescope, reflected on a mirror, which is viewed through a microscope, by doing this the telescope doubles it's viewing ability
The ability of a telescope to separate 2 closely spaced stars is called resolving power or angular resolution. This refers to the telescope's ability to distinguish fine details in an image, such as two closely spaced objects.
The "resolving power" of a telescope is a measure of the ability of a telescope to distinguish between two separate objects that appear to be very close together in the sky.
The telescope improved our ability to observe objects in the sky, leading to important discoveries in astronomy. The barometer improved our ability to measure air pressure and predict weather patterns. The microscope improved our ability to see and study tiny organisms and structures. The thermometer improved our ability to measure temperature accurately.
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A telescope would be the ideal instrument to help you see the moon clearly due to its ability to magnify objects in the night sky.
The size of a reflecting telescope is typically indicated by its aperture, which is the diameter of the primary mirror. Aperture size plays a crucial role in determining the light-gathering ability and resolving power of the telescope.
A telescope ray diagram can be used to show how light rays enter and are focused by the lenses or mirrors in a telescope. This helps illustrate how the telescope magnifies distant objects and forms an image for the viewer to see. By analyzing the paths of the light rays in the diagram, one can understand how the optical principles of the telescope work to enhance our ability to observe objects in space.
Please refer to the link below. This will take you to a web site that discusses this. Multiwavelength astronomy is dedicated to observing the various spectrums of radiation emitted. That is called its light gathering ability. The 'aperture size' determines the amount of light (radiation) a telescope gathers This site might help you obtain a more in depth answer imagine.gsfc.nasa.gov IT IS CALLED "LIGHT GRASP" in an optical telescope and "RF GAIN" in a radio-telescope.