An ASU astronomer is helping design and build new balloon-borne observatory to explore how stars and solar systems form
A missing link lies in the chain of astronomers' understanding of how stars and planetary systems are born, but a team of scientists and engineers from Arizona State University's School of Earth and Space Exploration is on track to help find it.
"Astronomers have an idea how the Milky Way Galaxy's giant clouds of dust and molecular gas produce stars," SESE astronomer Chris Groppi said. "But we don't have a good idea how these clouds form in the first place."
To discover this is the aim of a newly funded NASA project named GUSTO, which is led by astronomer Christopher Walker of the University of Arizona. The project also involves Johns Hopkins University's Applied Physics Laboratory, NASA’s Jet Propulsion Laboratory, the Massachusetts Institute of Technology, and the Netherlands Institute for Space Research.
GUSTO is short for — take a deep breath — Galactic and Extragalactic Ultra-Long-Duration Balloon-Borne Spectroscopic-Stratospheric Terahertz Observatory.
As its full name suggests, this observatory won't be located on Earth. Instead, it'll soar at high altitude in the atmosphere: about 21 miles up, roughly three times higher than passenger jets typically cruise.
At this altitude the balloon-borne observatory will float above 99 percent of Earth's atmosphere. Effectively, the observatory will be out in space where it can view the universe mostly unimpeded.
Building on NASA's experience with balloon flights launched from Antarctica, the GUSTO project combines a new balloon of advanced design, plus a 30-inch-aperture telescope with two dozen detectors. The detectors cover a spectrum of "colors" that range between thermal infrared (heat radiation) and microwaves.
"This part of the spectrum," Groppi said, "is where we can track characteristic interstellar gases — ionized carbon, oxygen and nitrogen — as they cool off and collapse into clouds that will eventually become stars and probably planetary systems."
The project plans to use GUSTO to scan much of the Milky Way galaxy and all of a small nearby galaxy called the Large Magellanic Cloud. Project astronomers expect that this study will serve as a template to help them understand other galaxies.
"For GUSTO, our role at SESE is to design and build the processing electronics that handle the raw signals coming from the telescope and going to the detectors," Groppi said. GUSTO analyzes the sky in three different "colors." But each color uses eight detectors, so the entire instrument package must handle and process signals involving 24 detectors in all.