They are too big and heavy for it to be possible to launch them into space.
No they are not bigger then radio telescopes at all.
Locating a radio telescope near a radio station is generally not a good idea due to potential interference from the radio station's broadcasts. Radio telescopes are extremely sensitive to electromagnetic signals, and the noise from a nearby station could disrupt observations and data collection. Ideally, radio telescopes should be placed in remote areas with minimal man-made radio frequency interference to ensure accurate and clear readings of celestial objects.
They are optical telescopes.
Radio Telescope Arrays
---False
Some other types of telescopes used by astronomers to observe stars include radio telescopes, which detect radio waves emitted by stars, and space telescopes like the Hubble Space Telescope, which is specifically designed for observations in space without the distortion caused by Earth's atmosphere. Astronomers also use infrared telescopes to study stars emitting infrared radiation, providing valuable insights into their composition and temperature.
Optical telescopes are placed high to avoid having to look through the thickest part of the atmosphere. Radio telescopes are place in valleys to avoid the effects of man-made electrical noise in the telescope.
Radio telescopes and Keck telescopes differ primarily in the type of electromagnetic radiation they observe. Radio telescopes detect radio waves emitted by celestial objects, allowing astronomers to study phenomena like pulsars and cosmic microwave background radiation. In contrast, the Keck telescopes, which are optical/infrared telescopes located in Hawaii, observe visible and infrared light, enabling detailed imaging and spectroscopy of stars, galaxies, and other astronomical features. This distinction in wavelength leads to different techniques and instruments used in their respective observations.
Astronomers use radio telescopes, infrared telescopes, and space-based telescopes to map the shape of the Milky Way. They measure the positions and motions of stars, gas, and dust to create a three-dimensional map of our galaxy.
That is because radio waves pass through clouds so radio astronomers do not have to wait for a clear sky.
The three basic categories of astronomical observation are optical, radio, and space-based. Optical observations involve using telescopes to detect visible light; radio observations involve detecting radio waves from celestial objects; space-based observations are done using telescopes and satellites positioned outside Earth's atmosphere to observe different wavelengths of light.
Astronomers use telescopes to study stars and planets by capturing light from these celestial objects and analyzing it. They can gather data on the properties of stars and planets, such as their temperature, composition, and distance from Earth, to deepen our understanding of the universe. Telescopes come in various forms, such as optical telescopes, radio telescopes, and space telescopes like the Hubble Space Telescope.
Astronomers are least likely to use optical telescopes for investigating galaxies that are very distant or obscured by interstellar dust, as these telescopes primarily detect visible light. Instead, they often rely on radio, infrared, or X-ray telescopes, which can penetrate dust and reveal more information about such galaxies. Optical observations are still valuable, but their limitations make them less effective for certain types of galaxy studies.
Most telescopes collect and focus light from distant objects in space, such as stars, planets, and galaxies. This focused light is then magnified and analyzed by astronomers to study and make observations about the universe.
Astronomers should observe radio waves if they want to capture images twenty-four hours a day quickly and cheaply. Radio waves can penetrate clouds and atmospheric disturbances, allowing for continuous observations regardless of weather conditions or time of day. Additionally, radio telescopes require less complex technology and can be built at a lower cost compared to optical telescopes, making them a practical choice for frequent imaging.
Ratio telescopes, often referred to as radio telescopes, are used to study the structure of the Milky Way galaxy because they can detect radio waves emitted by celestial objects, allowing for observations through interstellar dust that obscures optical wavelengths. This capability enables astronomers to map the distribution of hydrogen gas and other components of the galaxy, revealing its spiral structure and dynamics. Additionally, radio telescopes can capture data from various wavelengths, providing a more comprehensive understanding of the galaxy's morphology and behavior.
Radio telescopes extend the sense of sight by detecting and measuring radio waves emitted by celestial objects in space. This allows astronomers to observe objects and phenomena that are not visible with optical telescopes.