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STS-75 press kit

NASA · 40 pages · text from the file's own layer

This is NASA's press kit for Space Shuttle mission STS-75, dated February 1996 and later edited by Richard W. Orloff. It covers Columbia's planned 13-day flight carrying the Italian Tethered Satellite System reflight (TSS-1R) and the third United States Microgravity Payload. The kit sets out launch and landing plans, abort modes, the timeline, payload weights, crew duties, the tether's science objectives and investigators, and crew biographies. It does not mention any unidentified objects.

  • p. 2 …The NASA insignia design for space shuttle flights is reserved for use by the astronauts and…
  • p. 3 …Ed Campion Policy/Management 202/358-1778 NASA Headquarters Washington, DC Rob Navias Johnson Space Center…
  • p. 5 …96-27 REFLIGHT OF TETHERED SATELLITE HIGHLIGHTS STS-75 NASA's second Shuttle mission of the…
  • p. 6 …Orloff, 01/2001/Page 6 MEDIA SERVICES INFORMATION NASA Television Transmission NASA television is available through…
  • p. 15 …Orloff, 01/2001/Page 15 TETHERED SATELLITE SYSTEM REFLIGHT (TSS-1R) NASA and ASI long have…
  • p. 16 …Scientific Investigations Of the TSS-1R mission's 12 scientific investigations, NASA will provide six, ASI…
  • p. 18 …Manager Mike Calabrese, Office of Space Science, NASA Headquarters, Washington, DC. Responsible for project management at…
  • p. 22 …Fripp, NASA Langley Research Center, Langley, VA Objective. The speed and the amount of information that…
  • p. 24 …The investigation known as MEPHISTO is a cooperative program between NASA, the French Space Agency and…
  • p. 25 …Richard DeLombard, NASA Lewis Research Center, Cleveland, OH Objective. When the Space Shuttle is in orbit…
  • p. 26 …Sacksteder, NASA Lewis Research Center, Cleveland, OH Objective. On Earth, gravity causes air motion known as…
  • p. 27 …which was formed in 1985 as a NASA Center for the Commercial Development of Space. The…
  • p. 30 …It may not be used to state or imply the endorsement by NASA or by any…
  • p. 31 …Allen (Lieutenant Colonel, USMC) NASA Astronaut BIRTHPLACE AND DATE: Born August 4, 1955, in Philadelphia, PA…
  • p. 32 …Selected by NASA in March 1992, Scott reported to the Johnson Space Center in August 1992…
  • p. 33 …Hoffman was awarded NASA Space Flight Medals in 1985, 1991, 1992 and 1994, NASA Exceptional Service…
  • p. 34 …Satellite System (TSS), a joint project between NASA and the Italian Space Agency. Dr. Hoffman had…
  • p. 35 …Lieutenant Colonel in the Italian Air Force. NASA EXPERIENCE: Cheli reported to the Johnson Space Center…
  • p. 36 …Under agreement between ESA and NASA he joined the NASA astronaut candidates selected in May 1980…
  • p. 37 …Chang-Diaz (Ph.D.) NASA Astronaut BIRTHPLACE AND DATE: Born April 5, 1950, in San Jose…
  • p. 38 …Orloff, 01/2001/Page 38 NASA EXPERIENCE: Selected by NASA in May 1980, Dr. Chang- Diaz…
  • p. 39 …In 1991 he was relocated to the NASA Johnson Space Center to follow the training for…
Edited by Richard W. Orloff, 01/2001/Page 23
Critical Fluid Light Scattering Experiment (Zeno)
Principal Investigator: Dr. Robert Gammon, Institute for Physical Science and Technology,
University of Maryland, College Park, MD
Objective. The Zeno investigation, named for the Greek philosopher, will explore an unusual state of
matter by measuring the density of the element xenon at its critical point, a unique set of conditions when it
is literally on the edge of simultaneously being in a gaseous phase and a liquid phase. More precisely, the
material rapidly changes back and forth from one state to the other so that one is unable to determine the
state of a given volume of material.
Scientists are interested in what happens at the critical point because these phase change phenomena are
common to many different materials. Understanding how matter behaves at the critical point can provide
insight into a variety of physics problems, ranging from state changes in fluids (gas to liquid) to alterations
in the magnetic properties of solids. This knowledge will be valuable in a wide variety of fields, including
liquid crystals, superconductors and even matter fluctuations in the early formation of the universe.
Procedure. Aboard the Shuttle, Zeno will measure properties of xenon a hundred times closer to its critical
point than is possible on Earth. USMP-3 will use a refined procedure for approaching the critical point
temperature more slowly, gradually scanning from one temperature to the next, taking advantage of the
Zeno instrument's sensitivity to minute variations in fluid density that arise in microgravity. This will be
done by shining laser light on a xenon sample and analyzing the resulting light scattering. At controlled
temperatures extremely near the critical temperature, the fluid will be a billion times more compressible
than water but will have similar density. It will change from a vapor clear as glass to a milky white fluid
with a large capacity for absorbing heat, but will transport heat very slowly. Accurate measurements of a
fluid's physical properties when very close to the critical point cannot be made on Earth because gravity
causes the fluid to layer, with respect to density, (vapor on top, liquid below) severely at the temperatures
of most significance. The orbital environment will permit measurements to be made within a few
millionths of a degree of the critical temperature.
The Zeno instrument is contained within two flight modules to isolate electrical noise sources and thermal
loads from the most sensitive optical and electronic subsystems in the light-scattering instrument. A
precision, high-pressure sample cell will hold the xenon sample with a 100-micron- thick fluid layer for the
light-scattering experiment. This cell and a compact, high-performance thermostat are the key elements in
making precision measurements. The main components of the light-scattering system are housed on an
optics bench.
Isothermal Dendritic Growth Experiment (IDGE)
Principal Investigator: Dr. Martin Glicksman,
Rennselaer Polytechnic Institute, Troy, NY
Objective. Metals manufacturing for many industrial and consumer products involves the process of
solidification. Industrial materials research traditionally has tried many different things instead of
developing a clear understanding of the fundamental processes involved. Microgravity research such as
this will lead to manufacturing improvements in metals and alloys that display dendrite formation.
As most molten materials solidify, they form tiny pine tree-shaped crystals called dendrites, from the
ancient Greek for "tree." The size, shape and direction of these crystals dictate the final properties of the
resulting solid material, such as its hardness, its ability to bend without breaking and its electrical
properties. On USMP-2, dendrite researchers were able to observe dendrites in the absence of convection
at extremely small temperature differences below the freezing point, a phenomenon never seen on Earth.
During USMP-3, the experiment will continue to build upon that foundation.

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