Balloon-borne astronomy experiment X-Calibur racing to hit wind window

September 14, 2013 by Diana Lutz
Balloon-borne astronomy experiment X-Calibur racing to hit wind window
The X-ray telescope InFOCuS in the NASA hangar at the Fort Sumner Municipal Airport. An X-ray mirror (the object in the background, left, that looks like a jet engine intake) concentrates X-rays onto the WUSTL polarimeter, situated directly behind Matthias Beilicke (left) and Fabian Kislat.

In a few days, a balloon-borne telescope sensitive to the polarization of high-energy "hard" X-rays will ascend to the edge of the atmosphere above Fort Sumner, N.M., to stare fixedly at black holes and other exotic astronomical objects.

When X-Calibur, as the polarimeter is called, looks to the skies, it will see things that have never been seen before because it is looking at characteristics of high-energy light that astronomers are just beginning to explore.

X-Calibur differs from other instruments in that it can measure the degree and direction of X-rays, which provide information not available in other ways. For example, when it looks at and their outflows, it will be able tos study how black holes devour matter and grow.

"Whenever you look at the at a different , you see something completely different," said Henric Krawczynski, PhD, professor of physics in Arts & Sciences at Washington University in St. Louis and principal investigator of the X-Calibur experiment.

The beauty of balloon flights is that they can be used to test new instruments like X-Calibur at relatively low cost, but the drama of them is that the experiment flies at the mercy of the wind.

X-Calibur, like other experiments flown from NASA's Columbia Scientific Balloon Facility in Fort Sumner, has to catch a ride on what is called a stratospheric turnaround event.

This video is not supported by your browser at this time.
Matthias Beilicke, PhD, research assistant professor of physics, and Fabian Kislat, PhD, postdoctoral research associate in physics, assemble an X-ray polarimeter named X-Calibur that was designed at Washington University in St. Louis and built in a hangar in Fort Sumner, N.M. If all goes well, the instrument, now installed aboard a pointing telescope called InFOCuS, will be carried aloft by balloon in the coming week. (Video shot by Beilicke and edited by Tom Malkowicz of WUSTL Video Services.)

At mid-latitudes, stratospheric winds reverse direction twice each year: in the early spring and in late summer. When this happens, the winds are generally slow and small cells form where they go in circles. Balloons launched in these windows don't fly far away and may actually circle back toward the launch area.

"This way you can put it in the air for 30 hours, if you're lucky," Krawczynski said. If they miss the stratospheric turnaround, however, the balloon flight could be cut short. When balloons drift outside the allowed operational area, flight safety officers fire guillotines that separate the parachute from the , dropping the payload.

What could possibly go wrong?

The WUSTL polarimeter will be carried aloft by an X-ray pointing , called InFOCuS, that was designed and built by NASA's Goddard Space Flight Center.

A team of 15 people is working 12-hour days—essentially living in the NASA hangar at Fort Sumner—to make sure the telescope will be ready on time to catch the favorable winds.

One crucial task is to make sure the X-rays are concentrated on the center of the polarimeter, which is 8 meters from the mirror. The two components have to be aligned within one-sixtieth of a degree or the X-rays either won't hit the collimator at the center of the polarimeter or they'll hit it off-axis, both of which impact the results, Krawczynski said.

"The X-rays are hitting the collimator but a bit off to one side. We still need to tilt the mirror by half an arc-minute or so to focus the beam on the center of the collimator," he said.

Everything else has to be carefully checked out as well. A reaction wheel that has worked for 25 years has suddenly started to wobble and must be replaced. And difficulties arose when the telescope was rotated through 90 degrees in the NASA hangar that hadn't been apparent when it was rotated through 30 degrees in the lab.

But in fact, Krawczynski isn't so much worried as excited. "When something doesn't work, we have to troubleshoot and try to figure out what to do. It's detective work, which is fun," he said.

"I'm pretty confident we'll make the window for these turnaround flights," he said during a brief return to St. Louis. "It looks like we'll be ready in the middle of the window, but maybe we can make up a few days' time."

Explore further: Balloon-based experiment to measure gamma rays 6,500 light years distant

Related Stories

Krawczynski group receives NASA grant to spy on black holes

January 6, 2012

( -- Henric Krawczynski, PhD, professor of physics in Arts & Sciences at Washington University in St. Louis, is a big-game hunter of the astrophysical variety — he hunts celestial beasts, not beasts of the ...

Super-TIGER lying low for the Southern Hemisphere winter

February 8, 2013

(—Late Friday, Feb. 2, an overcast day in St. Louis, the twitter feed for the Super-TIGER cosmic ray experiment burst into life, as the Super-TIGER team received word that NASA's Columbia Scientific Balloon Facility, ...

Recommended for you

Hubble captures a galactic waltz

November 26, 2015

This curious galaxy—only known by the seemingly random jumble of letters and numbers 2MASX J16270254+4328340—has been captured by the NASA/ESA Hubble Space Telescope dancing the crazed dance of a galactic merger. The ...

The hottest white dwarf in the Galaxy

November 25, 2015

Astronomers at the Universities of Tübingen and Potsdam have identified the hottest white dwarf ever discovered in our Galaxy. With a temperature of 250,000 degrees Celsius, this dying star at the outskirts of the Milky ...

A blue, neptune-size exoplanet around a red dwarf star

November 25, 2015

A team of astronomers have used the LCOGT network to detect light scattered by tiny particles (called Rayleigh scattering), through the atmosphere of a Neptune-size transiting exoplanet. This suggests a blue sky on this world ...


Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.