STS034-10-014 (18-23 Oct. 1989) --- An onboard 35mm camera provides a closeup view of an STS-34 beverage container doubling as an experiment module for a test involving iodine concentration in onboard water. The examination called for the adding of starch to a specimen of Atlantis' fuel-cell produced water. The liquid was then compared against the color chart for determining the degree of iodine content. The experiment was designed by Terry H. Slezak of JSC's Photographic Technology and Television Division.

jsc2023e008494 (Feb. 10, 2023) --- A preflight image of the Exploration Potable Water Dispenser (Exploration PWD) iodine filter. Exploration PWD is a device that dispenses ambient and hot water into crew food and drink bags. The Exploration PWD is an improvement to the International Space Station (ISS) legacy PWD. Successful demonstration of this technology could lead to its adoption for future exploration missions and continued use for the space station crew.

S88-E-5001 (12-04-98) --- Astronaut Jerry L. Ross, mission specialist, discovered incompatible connections involved in one of the STS-88 detailed test objectives (DTO), this one having to do with the crew's drinking water. The proper female counterpart for the connection was later found. DTO 691 is an in-cabin experiment dealing with a low-iodine residual system. Newly developed technology replacing the Galley Iodine Removal System (GIRA) is expected to reduce the concentration of iodine in the Shuttle's potable water system. The photo was taken with an electronic still camera (ESC) at 14:09:17 GMT, Dec. 4.

The heart of a colorimetric solid phase extractor (CSPE) test kit quickly measures the concentration of the biocides silver or iodine in astronauts’ drinking water to determine whether concentrations are safe. When 10 milliliters (ml) of water is drawn through the disk, the disk will turn color (yellow in this picture for iodine) indicating the presence of the biocides. The device could someday be used to test water safety at reservoirs and water treatment plants on Earth. (photo credit: Microanalytical Instrumentation Center, Iowa State University).

S88-E-5002 (12-04-98) --- Astronaut Jerry L. Ross, mission specialist, holds up two incompatible connections involved in one of the STS-88 detailed test objectives (DTO), this one having to do with the crew's drinking water. The proper counterpart was later located and the connection was successfully accomplished. Astronaut James H. Newman, mission specialist, is at left background. DTO 691 is an in cabin experiment dealing with a low-iodine residual system. Newly developed technology replacing the Galley Iodine Removal System (GIRA) is expected to reduce the concentration of iodine in the Shuttle's potable water system. The photo was taken with an electronic still camera (ESC) at 14:09:40 GMT, Dec. 4.

ISS030-E-122089 (6 March 2012) --- NASA astronaut Dan Burbank, Expedition 30 commander, opens a Contingency Water Container-Iodinated (CWC-I) bag in the Kibo laboratory of the International Space Station.

iss055e008298 (April 2, 2018) --- Astronauts Scott Tingle (left) and Ricky Arnold wrap up spacesuit work following a successful spacewalk on March 29, 2018. The duo scrubbed cooling loops, performed the iodination of ion filters and tested the water conductivity inside a pair of U.S. spacesuits.

ISS019-E-014473 (5 May 2009) --- Salt ponds in Nueva Victoria, northern Chile are featured in this image photographed by an Expedition 19 crew member on the International Space Station. This view shows a long alluvial fan, sloping from east to west (left to right) in northern Chile with solar evaporation (or salt) ponds, some brightly colored, near the foot of the fan. The alluvial fan sediments are brown and contrast sharply with tan sediments of the Pampa del Tamarugal, the great hyper arid inner valley of Chile?s northern Atacama Desert. Nitrates and many other minerals are mined in this region. A few extraction pits and ore dumps are visible at bottom right, but most of the shallow diggings (0.5?5 meters deep) of a mine extracting caliche deposits ? a hard, cemented layer in the soil formed by downward movement and redeposition of sodium salts ? lie just outside the picture. Iodine is one of the products from mining; it is first extracted by a process known as heap leaching. Waste liquids from the iodine plants are dried in the tan and brightly colored evaporation ponds to crystallize nitrate salts for collection. Fertilizer production for higher-value crops is the main use for the recovered nitrates, but there are many other uses including the manufacture of pharmaceuticals, explosives, glass, ceramics, water treatment and metallurgical processes.

This photograph shows activities during the International Microgravity Laboratory-1 (IML-1) mission (STS-42) in the Payload Operations Control Center (POCC) at the Marshall Space Flight Center. The IML-1 mission was the first in a series of Shuttle flights dedicated to fundamental materials and life sciences research. The mission was to explore, in depth, the complex effects of weightlessness on living organisms and materials processing. The crew conducted experiments on the human nervous system's adaptation to low gravity and the effects on other life forms such as shrimp eggs, lentil seedlings, fruit fly eggs, and bacteria. Low gravity materials processing experiments included crystal growth from a variety of substances such as enzymes, mercury, iodine, and virus. The International space science research organizations that participated in this mission were: The U.S. National Aeronautics and Space Administration, the European Space Agency, the Canadian Space Agency, the French National Center for Space Studies, the German Space Agency, and the National Space Development Agency of Japan. The POCC was the air/ground communication charnel used between the astronauts aboard the Spacelab and scientists, researchers, and ground control teams during the Spacelab missions. The facility made instantaneous video and audio communications possible for scientists on the ground to follow the progress and to send direct commands of their research almost as if they were in space with the crew.

This photograph shows activities during the International Microgravity Laboratory-1 (IML-1) mission (STS-42) in the Payload Operations Control Center (POCC) at the Marshall Space Flight Center. Members of the Fluid Experiment System (FES) group monitor the progress of their experiment through video at the POCC. The IML-1 mission was the first in a series of Shuttle flights dedicated to fundamental materials and life sciences research. The mission was to explore, in depth, the complex effects of weightlessness on living organisms and materials processing. The crew conducted experiments on the human nervous system's adaptation to low gravity and the effects on other life forms such as shrimp eggs, lentil seedlings, fruit fly eggs, and bacteria. Low gravity materials processing experiments included crystal growth from a variety of substances such as enzymes, mercury, iodine, and virus. The International space science research organizations that participated in this mission were: The U.S. National Aeronautics and Space Administion, the European Space Agency, the Canadian Space Agency, the French National Center for Space Studies, the German Space Agency, and the National Space Development Agency of Japan. The POCC was the air/ground communication charnel used between astronauts aboard the Spacelab and scientists, researchers, and ground control teams during the Spacelab missions. The facility made instantaneous video and audio communications possible for scientists on the ground to follow the progress and to send direct commands of their research almost as if they were in space with the crew.

Engineers at the National Aeronautics and Space Administration (NASA) Lewis Research Center inspect the nitrogen baffle in the interior of the 22.5-foot diameter dome at the Space Power Chambers. In 1961 NASA Lewis management decided to convert the Altitude Wind Tunnel into two large test chambers and renamed the facility the Space Power Chambers. The conversion, which took over two years, included removing the tunnel’s drive fan, exhaust scoop, and turning vanes from the east end and inserting bulkheads to seal off the new chambers within the tunnel. The eastern section of the tunnel became a vacuum chamber capable of simulating 100 miles altitude. In 1962 NASA management decided to use the new vacuum chamber exclusively to study the second-stage rocket. This required significant modifications to the new tank and extensive test equipment to create a space environment. The Lewis test engineers sought to subject the Centaur to long durations in conditions that would replicate those encountered during its missions in space. The chamber was already capable of creating the vacuum of space, but the test engineers also wanted to simulate the cryogenic temperatures and solar radiation found in space. Six panels of 500-watt tungsten-iodine lamps were arranged around the Centaur to simulate the effect of the Sun’s heat. A large copper cold wall with its interior coated with heat-absorbing black paint was created specifically for these tests and assembled around the Centaur. The 42-foot-high wall had vertical ribs filled with liquid nitrogen which produced the low temperatures.