A proposal to build a far-flung set of radio antennas to measure the cosmos is one of 13 far-out concepts to receive seed funding from the NASA Innovative Advanced Concepts program.
University of Washington astronomer Matthew McQuinn will receive a grant of $175,000 to flesh out his plan for a solar-system-scale interferometer capable of determining cosmological distances with precision that’s an order of magnitude beyond what’s possible today.
The plan would require building and launching a constellation of four radio dishes, each measuring at least several meters (yards) in diameter. The detectors would have to be widely separated, far out in deep space. How far out? “The science gets interesting when they are more than about 10 AU apart,” McQuinn told me in an email. That distance of 10 AU is just a bit less than the width of Jupiter’s orbit.
The detectors would be on the lookout for fast radio bursts that flash from beyond our Milky Way galaxy. By measuring the difference in arrival times at the different detectors, scientists could calculate the distance to the source of a burst with sub-percent precision. “It’s kind of like GPS localizations, but applied to fast radio bursts,” McQuinn explained.
In his proposal, McQuinn says such measurements could lead to new discoveries in fields ranging from gravitational-wave detection to the study of dark matter. McQuinn and a UW colleague, Kyle Boone, lay out the details in a research paper that was published last year in The Astrophysical Journal Letters.
