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Terminology

Space Telescope Imaging Spectrograph

Illustration — STIS under construction, 1996 • Illustration — STIS camera images Saturn aurora • Illustration — STIS images the Fomalhaut system (January 8, 2013) (NASA). • Illustration — Ultraviolet image of Jupiter's aurora; the bright spot at far left is the end of field line to Io; spots at bottom lead to Ganymede and Europa. The Space Telescope Imaging Spectrograph (STIS) is a spectrograph, also with a camera mode, installed on the Hubble Space Telescope. Aerospace engineer Bruce Woodgate of the Goddard Space Flight Center was the principal investigator and creator of the STIS. It operated continuously from 1997 until a power supply failure in August 2004.

Also recorded as STIS

Space Telescope Imaging Spectrograph

Illustrates cumulative absorption spectra observed by Hubble. A beam of light coming to Earth from a distant quasar passes through numerous intervening gas clouds in galaxies and in intergalactic space. These clouds of primeval hydrogen subtract specific colors from the beam. The resulting "absorption spectrum," recorded by Hubbles Space Telescope Imaging Spectrograph (STIS) is used to determine t

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Illustration — STIS under construction, 1996 • Illustration — STIS camera images Saturn aurora • Illustration — STIS images the Fomalhaut system (January 8, 2013) (NASA). • Illustration — Ultraviolet image of Jupiter's aurora; the bright spot at far left is the end of field line to Io; spots at bottom lead to Ganymede and Europa. The Space Telescope Imaging Spectrograph (STIS) is a spectrograph, also with a camera mode, installed on the Hubble Space Telescope. Aerospace engineer Bruce Woodgate of the Goddard Space Flight Center was the principal investigator and creator of the STIS. It operated continuously from 1997 until a power supply failure in August 2004.

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wikidata · Q933358 · wikipedia · Space Telescope Imaging Spectrograph

In this article

  1. 01Origins and development
  2. 02Notes, references and evidence

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