The Hubble Space Telescope is primarily designed to observe distant objects in the universe, including galaxies, stars, and nebulae, in order to study their properties and evolution.

The Hubble Space Telescope was launched on April 24, 1990, from the Kennedy Space Center in Florida.

The Hubble Space Telescope is approximately 13 meters (43 feet) long and 4 meters (13 feet) in diameter.

The main mirror of the Hubble Space Telescope is made of beryllium, which is a lightweight and strong metal.

The Hubble Space Telescope weighs approximately 11,000 kilograms (24,000 pounds).

There have been five servicing missions conducted on the Hubble Space Telescope, the last one being in 2009.

The Wide Field Camera 3 (WFC3) is the primary instrument on the Hubble Space Telescope used to study exoplanets.

The Hubble Space Telescope is not capable of directly imaging exoplanets due to their small size and distance from Earth.

51 Pegasi b was the first exoplanet discovered by the Hubble Space Telescope in 1995.

51 Pegasi b has a mass of approximately 0.5 Jupiter masses.

51 Pegasi b has an orbital period of approximately 4 days.

As of 2023, the Hubble Space Telescope has discovered over 2,000 exoplanets.

HD 80606 b is the first exoplanet discovered to have a retrograde orbit around its star.

Exoplanets discovered by the Hubble Space Telescope are located outside our solar system.

The Hubble Space Telescope's discoveries of exoplanets have had a profound impact on our understanding of the universe, confirming the existence of exoplanets, providing valuable information about their properties, and helping us understand the formation and evolution of planetary systems.