For the first time, astronomers¹ have directly observed the mysterious dark companion in a binary² star（双子星） system that has puzzled skywatchers since the 19th century. Using an instrument developed at the University of Michigan, scientists have taken close-up pictures of Epsilon Aurigae during its eclipse, which happens every 27 years. "Close up" in this case is a relative term, but the images zoom³ in enough to show the shape of the dark object's shadow.

"Seeing is believing," said John Monnier, an associate professor in the U-M Department of Astronomy who is an author of a paper about the research findings published in the April 8 edition of Nature. Researchers from the University of Denver and Georgia State University were involved as well.

Epsilon Aurigae is the fifth brightest star in the northern constellation⁴（星座，荟萃） Auriga. For more than 175 years, astronomers have known it is dimmer than it should be, given its mass. They also noticed its brightness dip for more than a year every few decades. They surmised⁵（猜测，推测） that it was a binary system（二进制） in which one companion was invisible. But what type of object was the companion?

Because astronomers hadn't observed much light from it, the prevailing⁶（一般的，流行的） theory labeled it a smaller star orbited edge-on by a thick disk of dust. The theory held that the disk's orbit must be in precisely⁷ the same plane as the dark object's orbit around the brighter star, and all of this had to be occurring in the same plane as Earth's vantage point（有利位置，优势） . This would be an unlikely alignment⁸（结盟，队列） , but it explained observations.

The new images show that this is indeed the case. A geometrically thin, dark, dense⁹, but partially¹⁰ translucent¹¹（透明的） cloud can be seen passing in front of Epsilon Aurigae.

"This really shows that the basic paradigm¹²（范例，词形变化表） was right, despite the slim probability," Monnier said. "It kind of blows my mind that we could capture this. There's no other system like this known. On top of that, it seems to be in a rare phase of stellar life. And it happens to be so close to us. It's extremely fortuitous（意外的，偶然的） ."

The disk appears much flatter than recent modeling from the Spitzer Space Telescope suggests, Monnier said.

"It's really flat as a pancake," he said.

Monnier led the creation of the Michigan Infra-Red Combiner (MIRC) instrument that was used to produce these images. MIRC uses a process called "interferometry（干扰量度法） " to combine the light entering four telescopes at the CHARA array at Georgia State University and amplify¹³ it so that it seems to be coming through a device 100 times larger than the Hubble Space Telescope.

MIRC allowed astronomers to see the shape and surface characteristics of stars for the first time. Previously¹⁴, stars were mere¹⁵ points of light even with the largest telescopes.

"Interferometry has made high resolution imaging of distant objects a reality," said Fabien Baron¹⁶, a post-doctoral researcher in the Department of Astronomy who helped with the imaging in this study. "It most probably will solve many mysteries but also raise many new questions."