The Universe is continually radiating a wealth of information to Earth, sending signals in wide-spectrum of light. However, not all of these messages reach the ground. Because our planet's atmosphere blocks most radiation coming in from space, humans need to launch telescopes beyond it to get a complete cosmic picture.
Many of the Universe's messages are transmitted in infrared light, which our sky heavily filters. Infrared waves are too long for our eyes to see, but our nerves feel them as heat. In space, any object that has a temperature above zero Kelvin (- 459.67 degrees Fahrenheit, or -273.15 degrees Celsius) radiates in the infrared.
The Spitzer Space Telescope (SST), formerly the Space Infrared Telescope Facility (SIRTF) is an infrared space observatory launched in 2003. It is the fourth and final of the NASA Great Observatories program.
Spitzer is the largest infrared telescope ever launched into space. The Spitzer satellite carries a 0.85-meter telescope and three cryogenically-cooled science instruments. The science instruments are very sensitive, allowing astronomers to peer into regions of the Universe hidden from optical telescopes.
Hot dust. Much of deep space is filled with vast, dense clouds of gas and dust which block our view of visible light.
Fortunately, infrared light can penetrate the clouds of dust and gas, allowing us to see into the centers of galaxies and uncover stars and planetary systems forming.
Cool stars. Infrared light also reveals cooler objects across the Universe. Some of which are smaller stars too dim to be seen in visible light, planets around other stars, and giant clouds of molecules. In fact, many organic and inorganic molecules in space are seen best in infrared light.