NASA’s Interface Region Imaging Spectrograph (IRIS) spacecraft launched at 10:27 p.m. EDT Wednesday, June 26 from Vandenberg Air Force Base, Calif. Its primary goal is to understand how heat and energy move through the lower levels of the solar atmosphere.
IRIS is designed to study the Sun’s “interface region” – an area just above the Sun’s surface that once seemed so uninteresting it earned the title “ignorosphere.”
The interface region, between the Sun’s photosphere and corona, powers its dynamic million-degree atmosphere and drives the solar wind. The interface region also is where most of the Sun’s ultraviolet light is generated. In other words, when you get a sunburn blame the interface region!
IRIS carries a single instrument: an ultraviolet telescope combined with an imaging spectrograph. The telescope was built at the Smithsonian Astrophysical Observatory, and several SAO scientists are involved in post-launch commissioning and calibrations.
The telescope’s primary mirror has a diameter of about eight inches. While it will only be able to see about one percent of the sun at a time, it will be able to resolve that image to show features as small as 150 miles across – slightly larger than the state of Connecticut. Therefore it will complement missions like NASA’s Solar Dynamics Observatory, which capture images of the whole sun simultaneously.
Initially all operations of the IRIS satellite will be done from the Lockheed Martin Solar and Astrophysics Laboratory in Palo Alto, Calif., but after a few months some spacecraft operations will be controlled remotely from SAO’s Solar Mission Operations room.
IRIS is a class of spacecraft called a Small Explorer, which NASA defines as costing less than $120 million. IRIS weighs 440 pounds. It is approximately 7 feet (2.1 meters) long and, with its solar panels extended, is a little over 12 feet (3.7 meters) across
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