One night this September, scientists working at the old municipal airport in the desert town of Fort Sumner, N.M., picked up the InFOCuS X-ray telescope with a crane, carried it to the open doors of a hanger and pointed it at the starry sky overhead.
They were testing the system the telescope uses to find a target star and hold it in its sights so that the telescope and its onboard X-ray polarimeter X-Calibur could be declared flight-ready and queued for launch into the stratosphere.
There are roughly 100 thousand million stars in the Milky Way galaxy. How does InFOCuS find and point at one of them?
Every two seconds one of the three star cameras aboard the telescope takes an image of the sky, analyzes the image to find the stars in it, and compares the pattern of stars to those in its onboard star catalog. When it finds a match, it translates the center of the image it took into true celestial coordinates, and commands heavy brass reaction wheels and sliders to slew the telescope from those coordinates to those of its target star.
The star trackers work from a “seed” position provided by a magnetometer, a sun/moon sensor and three widely separated GPS units, which in turn listen to seven satellites. Together these systems provide coarse position information that narrows the search for the star trackers, which take over fine positioning once they have their bearings.
Balloon rise over Fort Sumner
Read our previous story ‘Balloon Rise over Fort Sumner’ about the giant balloon that will carry aloft X-Calibur, a cutting-edge telescope.
As the target object moves across the sky the telescope follows its motion with arc-second accuracy, typically to a few thousandths of a degree, or a spot more than 100 times smaller than the diameter of the moon. Ground-based telescopes can track with sub-arc-second accuracy, but then again they are not slowly spinning at an altitude of 120,000 feet, rocked by thin stratospheric winds.
Once it is declared flight-ready, InFOCuS will carry aloft a new detector sensitive to polarized X rays shed by exotic celestial bodies, such as the ultrafast outflows of mass-accreting black holes. If this trial flight is successful, the detector will fly in winter of 2016-2017 from Antarctica. Balloons taking advantage of slow stratospheric winds above the New Mexican desert can stay aloft only for one day, but those carried by the polar vortex over the frozen continent can remain at float altitude for a month or more.
Armchair observers can watch near-real-time video of the X-Calibur launch on the Columbia Scientific Balloon Facility’s website. While the balloon is aloft, it will be tracked on a Google Earth map. Click early and often. The balloon is now second in line for launch.
Washington University in St. Louis, led by Henric Krawczynski, is in charge of the X-ray polarimeter and overall mission. NASA’s Goddard Space Flight Center, led by Scott Barthelmy, is responsible for the gondola, X-ray telescope and the pointing system. The X-ray mirror and star trackers were contributed by Nagoya University in Japan. The stratospheric balloon that will carry the experiment to the edge of the atmosphere was made by Raven Aerostar, and launched by the experienced team at NASA’s Columbia Scientific Balloon Facility, based in Palestine, Texas.