Apollo Telescope Mount

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Apollo Telescope Mount
Apollo Telescope Mount picture.jpg
Image of the ATM with solar panels extending
Organization NASA Edit this on Wikidata
First light 1973 Edit this on Wikidata
Telescope style Optical telescope
Solar telescope
Space telescope Edit this on Wikidata
Solar array for the ATM (could also power other Skylab systems)
Illustration of the telescope cluster and solar array deployment

The Apollo Telescope Mount, or ATM, was a solar observatory attached to Skylab, the first American space station.

The ATM was manually operated by the astronauts aboard Skylab from 1973–74, yielding data principally as exposed photographic film that was returned to Earth with the crew. The film magazines had to be changed out by the crew during spacewalks.

The ATM was designed and construction was managed at NASA's Marshall Space Flight Center.[1] It included eight major observational instruments, along with several lesser experiments. The ATM made observations at a variety of wavelengths, including X-Rays, Ultraviolet, and Visible light.

As of 2006, the original exposures were on file (and accessible to interested parties) at the Naval Research Laboratory in Washington, D.C.

Design[edit]

The ATM was actively cooled to maintain the temperature of the instruments within a certain range.[2] Pointing was done with the help of the Skylab computer, which could be commanded from the space station by astronauts or by communication link from Earth.[3]

Sun facing end with entrance for light of multiple instruments
A side view of the instrument cluster without its enclosure
ATM assembly

History[edit]

Astronaut Paul J. Weitz at the telescope's command and display (C&D) console inside Skylab during the mission (June 1973)[4]

The ATM was one of the projects that came out of the late 1960s Apollo Applications Program, which studied a wide variety of ways to use the infrastructure developed for the Apollo program in the 1970s. Among these concepts were various extended-stay lunar missions, a permanent lunar base, long-duration space missions, a number of large observatories, and eventually the "wet workshop" space station.

In the case of the ATM, the initial idea was to mount the instrumentation in a deployable unit attached to the Service Module,[5] this was then changed to use a modified Apollo Lunar Module[6] to house controls, observation instruments and recording systems, while the lunar descent stage was replaced with a large solar telescope and solar panels to power it all. After launch, it would be met in orbit by a three-crew Apollo CSM who would operate it and retrieve data before returning to Earth. As many of the other concepts were dropped, eventually only the space station and ATM remained "on the books". The plans then changed to launch the ATM and have it connect to Skylab in orbit. Both spacecraft would then be operated by the Skylab crews.

With the cancellation of the later Apollo landing missions providing a Saturn V, the wet workshop concept was no longer needed. Instead, the plans were changed to orbit an expanded, dry version of the station. The ATM would now be launched attached to the station, as the Saturn V had enough power to launch them both at the same time. This change saved the Skylab program when a problem during launch destroyed one of the workshop solar panels and prevented the other from automatically deploying. The windmill-like arrays on the ATM, which fed power to both the ATM and the station, remained undamaged due to the protection within the launch shroud, and provided enough power for manned operations until the one remaining workshop array could be deployed during the first manned mission.

There were additional astronomical and Earth observation experiments aboard Skylab. During development, the ATM was subjected to thermal vacuum testing.[7]

Instruments[edit]

Image of the ATM taken showing some of the instrument covers

There were 8 major solar studies instruments on the mount.[8][9] Combined, they could observe the Sun in light wavelengths from 2 to 7000 Å (angstroms), which corresponds to soft X-ray, ultraviolet, and visible light.[9]

Same instruments by designation:

The X-Ray instruments included:[10]

  • S-054
  • S-056
  • S-020 (X-ray and extreme ultraviolet camera)[11]

UV instruments included:[12]

  • S-082A (Extreme ultraviolet spectroheliograph)
  • S-082B (Ultraviolet spectroheliometer)
  • S-055 (Ultraviolet spectrograph)

Hydrogen alpha and coronograph:

  • H-alpha no. 1
  • H-alpha no. 2
  • S-052 (a Coronagraph)

Also, experiment S149 was attached to one of the ATM solar panels.[13]

Film canisters[edit]

Six ATM experiments used film to record data, and over the course of the missions over 150,000 successful exposures were recorded.[14] The film canister had to be manually retrieved on manned spacewalks to the instruments during the missions.[14] The film canisters were returned to Earth aboard the Apollo capsules when each mission ended, and were among the heaviest items that had to be returned at the end of each mission.[15] The heaviest canisters weighed 40 kg (88.1 lb) and could hold up to 16,000 frames of film.[15]

Over the course of operations almost 30 canisters were loaded and utilized, and then returned to Earth.[16]

Results[edit]

Solar prominence recorded by Skylab on August 21, 1973[17]
This shows an extreme ultraviolet view of the sun (the Apollo Telescope Mount SO82A Experiment) taken during Skylab 3, with the Earth added for scale. On the right, an image of the Sun shows helium emissions; an image on the left displays emissions from iron

Experiments[edit]

The instruments were used for various types of observations including pre-planned experiements, including a set of student experiments. This is a chart describing an example of this:

Chart for the ED 24 experiment[18]

S-54 X-Ray Spectrographic Telesope[edit]

Skylab S-54 instrument, 1970

Legacy[edit]

A backup ATM spar (instruments were mounted to this) was restored at put on display in 2015 at the Steven F. Udvar-Hazy Center in Chantilly, Virginia, US.[19] The restoration involved repairing some Kapton layers that had degraded after 4 decades.[20]

See also[edit]

References[edit]

  1. ^ "NASM Space Artifacts: Apollo Telescope Mount". Web.archive.org. 2006-09-16. Archived from the original on September 16, 2006. Retrieved 2016-02-27.
  2. ^ "Apollo Telescope Mount". wwwsolar.nrl.navy.mil. Retrieved 2018-07-10.
  3. ^ "Apollo Telescope Mount". wwwsolar.nrl.navy.mil. Retrieved 2018-07-10.
  4. ^ [1]
  5. ^ [2]
  6. ^ [3]
  7. ^ APOLLO TELESCOPE MOUNT THERMAL SYSTEMS UNIT THERMAL VACUUM TEST
  8. ^ a b "0101909 - H-Alpha #1 Telescope - Skylab Apollo Telescope Mount". Mix.msfc.nasa.gov. 1973-01-01. Retrieved 2016-02-27.
  9. ^ a b c d e f g "ch4". History.nasa.gov. 1973-05-14. Retrieved 2016-02-27.
  10. ^ [https://history.nasa.gov/SP-402/ch4.htm
  11. ^ [https://history.nasa.gov/SP-402/ch4.htm
  12. ^ [https://history.nasa.gov/SP-402/ch4.htm
  13. ^ [4]
  14. ^ a b "ch4". history.nasa.gov. Retrieved 2017-01-09.
  15. ^ a b [5]
  16. ^ "ch4". history.nasa.gov. Retrieved 2018-07-10.
  17. ^ "7461522 - A Solar Prominence Taken by the Skylab Telescope". Mix.msfc.nasa.gov. 1973-08-21. Retrieved 2016-02-27.
  18. ^ [6]
  19. ^ "Restoring the Apollo Telescope Mount". National Air and Space Museum. 2015-12-10. Retrieved 2018-07-12.
  20. ^ "Restoring the Apollo Telescope Mount". National Air and Space Museum. 2015-12-10. Retrieved 2018-07-12.