Space Telescope Imaging Spectrograph (STIS)

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Overview

Ball Aerospace designed and built the Space Telescope Imaging Spectrograph (STIS) to enhance the capabilities of two first-generation Hubble Space Telescope instruments: the Goddard High Resolution Spectrograph and the Faint Object Spectrograph. STIS was installed aboard Hubble during the second servicing mission in February 1997.

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A Ball Aerospace team helped NASA prepare for the SM4 STIS repair activity. This image show an astronaut practicing the repair under water.

STIS captured images along its narrow entrance slit, which blocked extraneous light and generated the spectra of many locations simultaneously. The instrument’s observations are helping scientists understand the origins, properties, and dynamics of galaxies, stars, and the interstellar medium.

Astronauts installed Ball Aerospace’s improved power supply during Servicing Mission 4. The repairs were deep within the instrument and included several blind operations performed by the astronaut.  STIS operated nearly three years beyond its five-year design life, until its power-supply wore out in 2004.

Ball Aerospace worked with NASA to develop a simple repair process that would not compromise any performance characteristics of the instrument.

Programs

CALIPSO

CloudSat

Deep Impact/EPOXI

EFV

ERBS

GDPAA

GFO-2

GMI

HiRISE

Hubble Space Telescope

ICESat

James Webb Space Telescope

Joint Strike Fighter

Kepler

MASINT/AGI

Mast-Mounted Sight

Mk 20 Camera

MTI

NPP

Operational Land Imager

Orbital Express NextSat

OSSE

QuickBird

QuikSCAT

SBSS

SBUV/2

Seasparrow

Spitzer

STP-SIV

WISE

WorldView-1

WorldView-2