Text Size
OpNom:
Overview | Description | Applications | Operations | Results | Publications | Imagery
Experiment OverviewData from the Capillary Channel Flow (CCF) experiment will help to innovate solutions to transporting liquids (such as fuels, low temperature liquids like liquid nitrogen and water) in microgravity. By understanding capillary fluid flow rates in microgravity, hardware can be developed for "pumping" liquids from one reservoir to another without the need for a pump with moving parts. The reduced cost, weight, and improved reliability of such equipment make this a particularly attractive technology for NASA.
Principal Investigator(s)
Developer(s)
Information Pending
National Aeronautics and Space Administration (NASA)
Sponsoring OrganizationHuman Exploration and Operations Mission Directorate (HEOMD)
Research BenefitsInformation Pending
ISS Expedition Duration:September 2010 - September 2013
Expeditions Assigned25/26,27/28,29/30,33/34,35/36
Previous ISS MissionsISS Expedition 25/26 was the first operation of CCF in microgravity.
Capillary Channel Flow (CCF) is a versatile experiment for studying a critical variety of inertial-capillary dominated flows key to spacecraft systems that cannot be studied on the ground. The results of CCF will help innovate existing and inspire new applications in the portion of the aerospace community that is challenged by the containment, storage, and handling of large liquid inventories (fuels, cryogens, and water) aboard spacecraft. The results will be immediately useful for the design, testing, and instrumentation for verification and validation of liquid management systems of current orbiting, design stage, and advanced spacecraft envisioned for future lunar and Mars missions. The results will also be used to improve life support system design, phase separation, and enhance current system reliability.
Since hydrostatic pressure is absent in microgravity, technologies for liquid management in space use capillary forces to position and transport liquids. On Earth, the effect of capillary forces is limited to a few millimeters. In space, these forces still affect free surfaces that extend over meters. For the application of open channels in propellant tanks of spacecraft, design knowledge of the limitations of open capillary channel flow is a requirement.
To enable design of spacecraft tanks that can supply gas-free propellant to spacecraft thrusters, directly through capillary vanes, significantly reducing cost and weight, while improving reliability. Technologies for liquid management in space use capillary forces to position and transport liquids, since the hydrostatic pressure is absent which gives the liquid a defined surface and enables easy withdrawal from the tank bottom. But the effect of capillary forces is limited on Earth to a few millimeters. In space these forces affect free surfaces that extend over meters. For the application of open channels in propellant tanks of spacecrafts, design knowledge of these limitations are a requirement, predicated with a bubble free liquid restriction prior to entering the thrusters.
Earth ApplicationsTechnologies for liquid management in space use capillary forces to position and transport liquids, since the hydrostatic pressure is absent which gives the liquid a defined surface and enables easy withdrawal from the tank bottom. But the effect of capillary forces is limited on Earth to a few millimeters. In space these forces affect free surfaces that extend over meters. For the application of open channels in propellant tanks of spacecrafts, design knowledge of these limitations are a requirement, predicated with a bubble free liquid restriction prior to entering the thrusters.
Forced liquid flows through open capillary channels with free liquid surfaces will be investigated in the Microgravity Science Glovebox (MSG) onboard ISS. In open capillary channels, if a certain critical flow rate is exceeded, the flow becomes unsteady, the surfaces collapse, and gas ingestion occurs at the outlet. From a fluid mechanical point of view, a characteristic critical velocity must exist at which the steady subcritical flow turns into an unsteady supercritical flow, which involves the collapse of the free surfaces. To find this velocity and the location of collapse of the free surface, the surface profile must be measured with great accuracy. Furthermore, the local flow velocity must be known at dedicated points of the channel.
Operational ProtocolsThe crew involvement is limited to installation of the CCF hardware in the MSG work volume and exchange of experiment units between sessions.
CCF experimental unit and electrical subsystem, image courtesy of Glenn Research Center.