Images of "circumstellar" disks circling young stars as seen by the Atacama Large Millimeter Array (ALMA). (Credit:听ALMA, ESO/NAOJ/NRAO, S. Andrews et al.; NRAO/AUI/NSF, S. Dagnello)
This story was adapted from a version published by the University of California, Santa Cruz. .
The NASA Astrobiology Program has awarded a five-year, $5 million grant to an interdisciplinary consortium to trace the volatile elements that form the atmospheres of planets, establishing a scientific foundation for detecting the signatures of life on other planets.听
Meredith MacGregor, an assistant professor in the Department听of Astrophysical and Planetary Sciences (APS) and the Center for Astrophysics and Space Astronomy (CASA) at 抖阴旅行射 Boulder, will lead the university's听efforts on the project. Her research will explore the connections between planets, their host stars and the disks of gas and dust that surround young stars鈥攊ncluding how planets inherit their atmospheres from disks and how bursts of energy from stars can make alien worlds less hospitable for life.
Meredith MacGregor
鈥淓nergy from stars can ionize and even erode the atmosphere of a planet, turning a habitable world into a barren wasteland,鈥� MacGregor said. 鈥淚n this project, we hope to better understand how this happens and how many worlds could be affected.鈥�
Natalie Batalha, professor of astronomy and astrophysics at the University of California, Santa Cruz, will lead the overall consortium, one of eight new research teams selected by NASA to inaugurate its (ICAR) program. The consortium also includes researchers at the University of Hawaii at Manoa, University of Kansas and NASA Ames Research Center.
鈥淲e want to understand the physical processes that impact planetary atmospheres,鈥� Batalha said. 鈥淲e must understand those physical processes and their effects in the absence of life so that we will be able to recognize the signs of life when we see them.鈥�
For Batalha鈥檚 team, that means 鈥渇ollowing the volatiles,鈥� tracing the path of the volatile elements like carbon and oxygen that make up a planet鈥檚 atmosphere. That path goes from star-forming clouds into protoplanetary disks, to the building blocks of planets and eventually into planets themselves, where volatile elements can move between the surface, atmosphere and interior, and even be lost to space.
The researchers will address four fundamental science questions: What is the inventory of volatiles in planetary building blocks? What are a planet鈥檚 external sources and sinks of volatiles (in other words, where do they come from and where do they go)? How are volatiles distributed between a planet鈥檚 interior, surface and atmosphere? And what can atmospheric observations tell us about the volatile inventories and chemistries of exoplanets?
MacGregor will lead analysis of circumstellar disk observations using the Atacama Large Millimeter/submillimeter Array (ALMA) combined with other ground-based observatories. She will also coordinate multi-wavelength observing campaigns to explore the properties of and mechanisms behind stellar flaring in order to better understand how these events can damage planetary atmospheres over time.
