Behind UCSB astrophysicist Ruth Murray-Clay is an artists animation of a brown dwarf surrounded by a swirling disc of planet-building dust. NASAs Spitzer Space Telescope spotted such a disc around a surprisingly low-mass brown dwarf, or failed star. (Spencer Bruttig photo \/ background courtesy of NASA\/JPL-Caltech) <\/p>\n
By Julie Cohen for the UCSB Office of Public Affairs and Communications | Published on 01.22.2015 2:25 p.m.<\/p>\n
The American Astronomical Society has awarded UC Santa Barbaras Ruth Murray-Clay the 2015 Helen B. Warner Prize for Astronomy for her theoretical studies of star and planet formation. <\/p>\n
Presented annually in recognition of a significant contribution to observational or theoretical astronomy during the five years preceding the award, the Warner Prize is given to an astronomer who is under 36 years of age in the year designated for the award, or within eight years of receiving his or her Ph.D. <\/p>\n
We are proud of Ruth for winning the 2015 Warner Prize, said Philip Pincus, chair of UCSBs Department of Physics, where Murray-Clay is a newly appointed assistant professor. We were delighted for her to join our faculty. She brings a wealth of expertise to UCSB, not only in the area of planet formation, but also in the evolution of their atmospheres and how they migrate. <\/p>\n
I feel very honored to win the Warner Prize, said Murray-Clay. I really like doing this work partly because there are all sorts of different physics involved. What really drew me to this subject is that its about where we came from and how the Earth formed and, by extension, how we came to be. <\/p>\n
The prize committee also cited Murray-Clays substantial contributions to numerous other areas of astrophysics. Her citation states that she has advanced models of planet formation by clarifying the role of gravitational instabilities, illuminating how orbital migration leads to short-period hot Jupiters and exploring photoevaporation of close-in exoplanets. <\/p>\n
According to the AAS, Murray-Clay follows up testable predictions of her theoretical models by delving directly into the observational data. The committee noted that she also has made outstanding contributions to the theoretical interpretation of G2, an ionized gascloud plunging toward the supermassive black hole at the center of the Milky Way. <\/p>\n
In addition to planet and star formation, Murray-Clay is interested in the extrasolar planetary systems recently discovered by NASAs Kepler spacecraft and by ground-based direct imaging. One place where we can really learn a lot about planet formation right now is by studying planets that orbit far from their stars farther than our most distant planet, Neptune, she explained. In particular, there is the first directly imaged planetary system, HR 8799, which has at least four very large planets with very wide separations. We know that this kind of system is the tip of an iceberg. Is it the tip of star formation on a small scale? Or could it be that the processes that we think formed Jupiter and Saturn, our giant planets, actually do work at very large distances and that we havent figured out how yet? <\/p>\n
This is an exciting place to be looking because there are several big direct imaging surveys ramping up now, Murray-Clay continued. So were really going to be able to study these giant planets and their wide separations, which will help us distinguish between different types of models. <\/p>\n
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UCSB Physics Professor Ruth Murray-Clay Awarded Top Astronomy Prize<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" Behind UCSB astrophysicist Ruth Murray-Clay is an artists animation of a brown dwarf surrounded by a swirling disc of planet-building dust. NASAs Spitzer Space Telescope spotted such a disc around a surprisingly low-mass brown dwarf, or failed star. (Spencer Bruttig photo \/ background courtesy of NASA\/JPL-Caltech) By Julie Cohen for the UCSB Office of Public Affairs and Communications | Published on 01.22.2015 2:25 p.m. Continue reading