The development of future astronomical observatories is driven by a combination of factors, including the increased demand for space exploration, advancements in telescope technology, and the growing interest in astrobiology.

The ELT is designed to study the formation and evolution of galaxies, as well as other fundamental questions in astronomy, such as the nature of dark matter and dark energy.

Infrared telescopes are expected to play a significant role in future space-based observatories due to their ability to penetrate dust and gas, allowing astronomers to study obscured regions of the universe.

Adaptive optics technology corrects for atmospheric turbulence, which can distort images obtained from ground-based telescopes, resulting in improved image quality and higher resolution.

The development of future astronomical observatories faces several challenges, including the high cost of construction and operation, the need for specialized expertise and training, and the limited availability of suitable observing sites.

The JWST is designed to study the early universe, including the formation of the first galaxies, as well as other fundamental questions in astronomy, such as the evolution of stars and galaxies.

AI has the potential to revolutionize astronomical observatories by automating data processing and analysis, improving image quality and resolution, and increasing observing efficiency.

The SKA is designed to study the formation and evolution of galaxies, as well as other fundamental questions in astronomy, such as the nature of dark matter and dark energy.

ELTs face several limitations, including their high cost of construction and operation, limited field of view, and susceptibility to atmospheric turbulence.

Adaptive optics technology corrects for atmospheric turbulence, which can distort images obtained from ground-based telescopes, resulting in improved image quality and higher resolution.

AI has the potential to revolutionize astronomical observatories by automating data processing and analysis, improving image quality and resolution, and increasing observing efficiency.

The SKA is designed to study the formation and evolution of galaxies, as well as other fundamental questions in astronomy, such as the nature of dark matter and dark energy.

ELTs face several limitations, including their high cost of construction and operation, limited field of view, and susceptibility to atmospheric turbulence.

Adaptive optics technology corrects for atmospheric turbulence, which can distort images obtained from ground-based telescopes, resulting in improved image quality and higher resolution.

AI has the potential to revolutionize astronomical observatories by automating data processing and analysis, improving image quality and resolution, and increasing observing efficiency.