THE ASTRO MISSIONS

ULTRAVIOLET IMAGING TELESCOPE


Astro-Artist's
Astro-1 Mission on orbit (artist's concept)


BACKGROUND

The Ultraviolet Imaging Telescope, one of the three ultraviolet telescopes of the Astro Observatory, flew on Space Shuttle missions in December 1990 and March 1995. It was designed, built, and operated by a team led by Theodore P. Stecher at Goddard Space Flight Center.

UIT was proposed in 1978 as part of a program to fly small ("university-class") scientific experiments on the Spacelab modules attached to the Space Shuttle. At that time, NASA anticipated that there would be about 3 Shuttle/Spacelab missions each year dedicated to astrophysics experiments (out of an envisioned 20 or so missions annually). By late 1985, the Astro UV telescopes had been approved for six missions. At the time of the Challenger accident in January 1986, Astro-1 was in the Shuttle Columbia payload bay ready for the launch to follow the Challenger mission. In the aftermath of the accident and in the face of the rapidly escalating costs of the Shuttle itself, the Spacelab astrophysics program was drastically reduced. Of the 200 experiments proposed in 1978, only the four telescopes of the Astro-1 mission were actually flown.

UIT was a 38-cm Cassegrain telescope carrying two ultraviolet cameras with 40 arc-minute diameter fields of view (150 times larger than the field of the Hubble Space Telescope). The cameras operated in the "far-UV" (120-200 nm) and "mid-UV" (200-320 nm) spectral ranges, respectively, and carried a total of 12 filters. They employed dual-stage, magnetically focussed image intensifiers with very strong long-wavelength rejection to provide pure UV response. Images produced by phosphors at the output of the intensifiers were recorded on film. (At the time UIT was approved, there were no proven electronic detectors capable of covering the required large, 2048x2048 pixel field of view.) Fine guidance was accomplished with an articulated secondary mirror controlled by a signal from an externally mounted 15-cm star tracker containing a CCD detector. Final resolution for point sources was typically 2.7 arc-seconds FWHM. A cutaway drawing of the UIT design is shown below.

During the two Astro missions, UIT returned a total of 1570 data frames of 250 different astronomical targets.

The Astro UV payload consisted of UIT, the Hopkins Ultraviolet Telescope (HUT), and the Wisconsin Ultraviolet Photo-Polarimeter Experiment (WUPPE). HUT was a far-ultraviolet spectrometer (Johns Hopkins University, led by A. F. Davidsen). WUPPE was a UV spectro-polarimeter (University of Wisconsin, led by A. D. Code). These three instruments were co-aligned and mounted on the Spacelab Instrument Pointing System. They were operated simultaneously on a given target by crew members from the Shuttle aft flight deck.

For Astro-1 (STS-35, 1990, Shuttle Columbia) the Broad-Band X-Ray Telescope (BBXRT, P. Serlemitsos, Goddard Space Flight Center) was operated independently on a separate pointing system. Astro-1 compiled a NASA record for delays: 33 different assigned launch dates over 8 years, 12 complete target timelines planned (each 8 days long at 1 second resolution), and 4 scrubs within 6 hours of launch.

On Astro-2 (STS-67, 1995, Shuttle Endeavour), the UV telescopes flew alone. Astro-2 was the first NASA mission to have an active Internet home page and logged over 2.5 million hits from over 200,000 people during its 15 day duration.

A list of over 140 publications based on data from the UIT can be found here.

MISSION IMAGES

[Click for Full Size]

UIT Design
  		Vacuum-Tank Testing
(HUT)
  		UV Instruments
On Pallet
 
Co-Mounted UV
Telescopes
  		Astro-1 Payload
On Pallets
  		Astro-1 Patch
 
Rollback Of Astro
Rollout Of HST
  		Astro-1 & HST On
Launch Pads
  		On The Launch Pad
 
Astro-1 Launch
  		UIT On Orbit
  		Astro-1 Crew
 
Lunch
  		Moon Rising Over
Earth's Limb
  		Orion Rising
(Daylight)
 
Astro-2 Patch
  		Astro-2 Launch
  		Main Engines At Launch
 
Astro-2 Crew
  		Astro-2 Payload
On Orbit
  		Payload Into Shadow
 
Stars over the Limb
  		Aft Flight Deck
(Instrument Control)
  		Running the Instruments
 
Orbiting Target Book
  		Payload Operations Control
Center (Huntsville, AL)
  		Over the Andes
 
Disappointment Reach
(Australia)
  		Nepal
  		Oahu
 
Low Pressure System
  		Sunset
  		The Dreaded Exercycle
 
Landing Practice
  		Landing (Edwards
Air Force Base)
 

SCIENCE IMAGES

[Far-Ultraviolet Unless Noted;
Click for Full Size]

Moon (Far-UV, Optical)
  		Cygnus Loop
(Supernova Remnant)
  		Crab Nebula 4 Bands
(Supernova Remnant)
 
NGC 6752
(Globular Cluster)
  		Omega Centauri
(Globular Cluster)
  		Omega Centauri
(Center)
 
UIT Fields in the
Large Magellanic Cloud
  		3 Views of
30 Doradus (LMC)
  		Small Magellanic Cloud
Mosaic
 
M31 (Andromeda Spiral)
Center and SW Disk
(Mid-UV Mosaic)
  		M33 (Spiral; UV/Optical
Comparison, 4 Bands)
  		M33
UV/Optical Superposition
 
M74 (Spiral;
Mid-UV, Optical)
  		M51 (Spiral;
Far-UV, H-alpha)
  		M51 (Far-UV, H-alpha
Color Map)
 
M101 (Spiral
Galaxy)
  		M101 (Far-UV,
Optical)
  		M101 (Far-UV,
H-alpha)
 
M81 (Spiral;
Mid-UV, Optical)
  		M81 (Far-UV,
Mid-UV, Optical)
  		NGC 1317 (Sa Galaxy
With Nuclear Ring)
 
NGC 1399/1404
(E Galaxies)
  		M83 (Barred Spiral;
Mid-UV With
UIT Rocket Prototype)
  		Irregular & Dwarf
Galaxies
 
NGC 4736 (Spiral
With Interior Ring)
  		3 Spiral Galaxies
  		M82 (Starburst Galaxy
With Galactic Wind)
 
Cen A: Post-Merger
Starburst Ring
 
LINKS

Last modified July 2024 by R. W. O'Connell

Presentation copyright © 2002-2024 Robert W. O'Connell. All rights reserved. Image sources: NASA archives; Ultraviolet Imaging Telescope Team (T. P. Stecher, Goddard Space Flight Center); Hopkins Ultraviolet Telescope Team (A. F. Davidsen, Johns Hopkins University). Launch pad photo of HST/WFC3 Science Oversight Committee copyright © 1999, J. A. Frogel.