This Solar Satellite Will Shed Light on the Inner Workings of the Sun

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The Sun actually gets hotter as you travel away from its surface, jumping from 6,000 K there to over 1,000,000 K a few million kilometers above in the corona. This effect contributes to solar flares that can damage earthbound electronics and we have no idea how it does this. But NASA is about to find out thanks to the IRIS (Interface Region Imaging Spectrograph) spacecraft that just launched from Vandenberg Air Force Base today.


The two-year IRIS project is part of NASA's Small Explorer (SMEX) mission that has studied everything from mesospheric ice aeronomy to the interstellar boundaries of our galaxy. IRIS itself is designed to study how heat and energy propagate through the Sun's lower atmosphere using an ultraviolet telescope and an imaging spectrograph.

"This is the first time we'll be directly observing this region since the 1970s," Joe Davila, IRIS project scientist at NASA's Goddard Space Flight Center, said in a press statement. "We're excited to bring this new set of observations to bear on the continued question of how the corona gets so hot."

The Lockheed Martin Solar and Astrophysics Lab teamed with NASA Ames—as well as the Smithsonian, and a trio of universities—-to produce the $120 million spacecraft. It measures approximately seven feet long by 12 feet wide with its solar panel array deployed and weighs 440 pounds. Its only equipment are the 8-inch ultraviolet telescope and imaging spectrograph. While the relatively-small diameter of the telescope will only allow researchers to image 1 percent of the Sun's surface at a time, it will also resolve objects down to 150 miles, providing an unprecedented close-up view of our home star like an astronomical microscope, the perfect complement to NASA's Solar Dynamics Observatory (SDO).

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In line with its severe focus, the IRIS will only record data in the 5000 K to 65,000 K temperature range that exists between the photosphere (the sun's surface), and chromosphere/transition region (the start of the Sun's atmosphere). It will record spectra readings every second and snap images every five using a quartet of identical 13 µm-pixel CCDs. When processed by a supercomputer running state-of-the-art 3D numerical modeling back on Earth, researchers will be able to trace the path of energy through the Sun's lower atmosphere.


“The interpretation of the IRIS spectra is a major effort coordinated by the IRIS science team that will utilize the full extent of the power of the most advanced computational resources in the world," explained Alan Title, the IRIS principal investigator at the Advanced Technology Center (ATC) Solar and Astrophysics Laboratory. "It is this new capability, along with development of state of the art codes and numerical models by the University of Oslo that captures the complexities of this region, which make the IRIS mission possible. Without these important elements we would be unable to fully interpret the IRIS spectra.” Assuming all goes as planned with today's launch, IRIS' first results should be available in the coming weeks.

[NASA 1, 2 - Wikipedia - Space Flight 101 - Lockheed Martin]




The Corona might be hotter, but there's less energy there than on the surface (ie, the particles in the Corona are super energetic by themselves, but there's very few of them).

Common explanations for the Corona are they picked up excess energy at the surface by random chance (Temperature is just a statistical measurement; and statistics do allow for wide, but few, variations) or that the magnetic field agitates the corona a lot.