AEROSPACE INDUSTRY
UPDATE
January 2013
McIlvaine Company
The spacecraft and science instrument integration for the Interface Region Imaging Spectrograph (IRIS) – NASA's next Small Explorer (SMEX) Mission – has been completed, and final testing is underway. The instrument has spent time in a cleanroom at the Lockheed Martin Space Systems facility in Sunnyvale, CA.
IRIS was designed and built at the Lockheed Martin Space Systems Advanced Technology Center (ATC) in Palo Alto, Calif., with support from the company’s Civil Space line of business and major partners Smithsonian Astrophysical Observatory, Montana State University, and Stanford University.
NASA’s Ames Research Center, Moffett Field, Calif., is responsible for mission operations and the ground data system. The Norwegian Space Agency will capture the IRIS data with their antennas in Svalbard, inside the Arctic Circle, in northern Norway. The science data will be managed by the Joint Science Operations Center of the Solar Dynamics Observatory, run by Stanford and Lockheed Martin. NASA’s Goddard Space Flight Center in Greenbelt, Md., oversees the SMEX project.
Understanding the interface between the photosphere and corona remains a fundamental challenge in solar and heliospheric science. The IRIS mission will open a window of discovery into this crucial region by tracing the flow of energy and plasma through the chromosphere and transition region into the corona using spectrometry and imaging. Here all but a few percent of the non-radiative energy leaving the Sun is converted to heat and radiation. The remaining few percent create the corona and solar wind. Magnetic fields and plasma exert comparable forces in this region, and IRIS is uniquely suited to provide the observations necessary to pinpoint the physical forces at work in this little understood piece of real estate near the surface of the Sun.
The IRIS observatory, scheduled for launch in April 2013, will fly in a Sun-synchronous polar orbit for continuous solar observations on a two-year mission. It will obtain ultraviolet spectra and images with high resolution (1/3 arcsec) – with a cadence of as little as one second apart – focused on the chromosphere and the transition region. Spectra will cover temperatures from 4,500 to 107 K, with images covering temperatures from 4,500 to 65,000 K.
The NASA SMEX Program is designed to provide frequent, low-cost access to space for heliophysics and astrophysics missions using small to mid-sized spacecraft. The program also seeks to raise public awareness of NASA's space science missions through educational and public outreach activities.
The ATC is the research and development organization of Lockheed Martin Space Systems Company (LMSSC) and creates the technology foundation for the company’s business. In addition, the ATC conducts research into understanding and predicting space weather and the behavior of our Sun, including its impacts on Earth and climate. It has a five-decade-long heritage of space-borne instruments.
LMSSC, a major operating unit of Lockheed Martin Corp., designs and develops, tests, manufactures, and operates a full spectrum of advanced-technology systems for national security and military, civil government, and commercial customers. Chief products include human space flight systems; a full range of remote sensing, navigation, meteorological, and communications satellites and instruments; space observatories and interplanetary spacecraft; laser radar; ballistic missiles; missile defense systems; and nanotechnology research and development.
Headquartered in Bethesda, MD, Lockheed Martin is a global security and aerospace company that is principally engaged in the research, design, development, manufacture, integration, and sustainment of advanced technology systems, products, and services.
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