Space Telescope Imaging Spectrograph
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The Space Telescope Imaging Spectrograph (STIS) is a special tool used to study objects in space, installed on the Hubble Space Telescope. It was created by aerospace engineer Bruce Woodgate at the Goddard Space Flight Center. The STIS worked from 1997 until a problem in 2004, but it was fixed and started working again in 2009.
The STIS was put on the Hubble Space Telescope in 1997 during a space mission called STS-82. It replaced two older instruments and was expected to work for five years. Even though it stopped working in 2004, it kept going for two extra years before astronauts fixed it during another mission, STS-125, in 2009.
One of the most exciting things the STIS helped discover was the first ever look at the atmosphere of a planet outside our solar system, called HD 209458b. Astronauts worked hard to repair the instrument, and it started exploring the universe once more.
Design
The Space Telescope Imaging Spectrograph (STIS) is a special tool that works like both a spectrograph and a camera. It mainly looks at ultraviolet light.
STIS uses three big detector arrays. The first one is a charge-coupled device that sees visible and near-infrared light. The other two detectors look at different kinds of ultraviolet light.
Timeline
- February 14, 1997 โ STIS was installed (STS-82).
- In 2001, it started using new parts after some old parts stopped working.
- On August 3, 2004, STIS stopped working because of a problem with its power.
- In 2009, STIS was fixed up again (STS-125).
- As of 2022, STIS is still working using its backup parts and all its cameras.
Selected discoveries and observations
The Space Telescope Imaging Spectrograph helped scientists learn many new things between 1997 and 2017. It studied 20 galaxies to look for black holes, examined the space between galaxies, and watched stars and star systems.
Some of its important work included studying the air around a planet outside our solar system, spotting a dusty disk around the star Beta Pictoris, watching huge stars in the Tarantula Nebula, and seeing the remains of the star explosion Supernova 1987A. It also looked at flows of material from very active galaxies.
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