Sharp eye on the sun.

The sun is hotter than anything you can probably imagine, but that may not be the most striking thing about our closest star. The real surprise is that the sun's thin outer atmosphere, or corona, is much, much hotter than the sun's surface.

That's like the air high above a flame being hotter than the flame itself. The temperature should fall as you move away from a heat source.

A new spacecraft called Hinode has just started collecting data that might help explain this solar oddity.

Recently launched through a collaboration involving Japan, Great Britain, and the United States, Hinode can collect two kinds of information about the sun. With a half-meter-wide visible-light telescope, it takes pictures of the sun's surface. It's the largest solar telescope that has ever flown into space.

Hinode also carries an X-ray telescope that detects hot gases in the sun's corona.

Hinode's X-ray telescope can record emissions that range between about 1 million and 4 million kelvins (273.15 kelvins equals 0[degrees]C or 32[degrees]F). This is an unusually wide temperature range for a detector, and it gives Hinode the power to sense the corona's calm, quiet features as well as its hot, explosive ones. Until now, scientists have been unable to study the corona in such detail.

The portrait (shown above) taken by Hinode's X-ray telescope on Oct. 28 shows features called X-ray bright points. These features, it appears, are magnetic loops that trap hot gas.

By monitoring X-ray bright points, scientists hope to better understand how the sun's corona becomes so hot. They should also get a clearer picture of how magnetic fields affect the corona.

Hinode, which means "sunrise" in Japanese, is still undergoing tests. In December, the spacecraft will officially begin a 3-year mission to unravel the sun's secrets.