Abstract
Astronomers have been trying to update the biography of the Sun for decades, at the same time trying to confirm our models for its internal structure. Like the Earth - of which we can sample directly less than 0.2% of its total depth - most of the interior of the Sun is hidden from direct view. Except for neutrinos from the solar core, we receive direct information from a surface layer of gas whose depth is only 0.05% of the radius of the Sun.
Astronomers, faced with the same challenge that geophysicists had tackled before us to probe the deep interior of the Earth, turned to the rule book of geoseismology. For the Sun, we could apply the principles of global helioseismology and eventually time-distance seismology, using the intrinsic vibrations of the Sun caused by sound waves propagating in the solar interior. Much of this was possible with telescopes on the Earth's surface because of the very high signal-to-noise and surface spatial sampling possible for solar observations. But when it came to extending this technique to the stars, through asteroseismology, it was necessary not to toss out the rule book, but to toss it upwards, into space.
Canada's first space telescope, called MOST, was one of the pioneers, later joined by the French CoRoT space mission and eventually NASA's Kepler satellite. These instruments are the most sophisticated stellar lightmeters ever built, and launching them into space launched a revolution in ultraprecise photometry of stars and exoplanets. That in turn launched a revolution in our ability to seismically probe distant stars, and to put our own Sun in better context by studying the interiors of other suns. Not just 'middle-aged' suns like our own, but senior suns, and teen suns, and baby suns, and even suns still in the womb.
Even for our own Sun, the seismic data are driving the physics, so we need to include what used to be considered third-order effects lost in the noise, if we're to match the eigenfrequencies to their current measured accuracies.
Join me on a lunchtime voyage through space and time, where the guide book contains the principles of time series analysis and mathematical inversion, to see how far we have come in only a decade, and the exciting frontiers that are ahead of us.
Biography
Jaymie Matthews is an astrophysical “gossip columnist” who unveils the hidden lifestyles of stars by eavesdropping on “the music of the spheres.” His version of an interstellar iPod is Canada’s first space telescope, MOST (Microvariability & Oscillations of STars), which detects vibrations in the light of ringing stars too subtle to be seen by the largest telescopes on Earth. MOST also makes Prof. Matthews an “astro-paparazzo” by helping him spy on planets around other stars that might be homes for alien celebrities. Celebrities? Maybe not beings like the fictional Vulcans, but even the discovery of extraterrestrial microbes on another world would qualify those microbes as news makers of the century.
Prof. Matthews leads the Canadian Space Agency’s MOST project, and is a Professor of Astrophysics in the Department of Physics & Astronomy at the University of British Columbia. He also serves on the Executive Science Team for BRITE Constellation (BRIght Target Explorer – a Canadian–Austrian–Polish space satellite mission to monitor the brightest stars in the night sky) and on the Executive Council for NASA’s Kepler satellite mission hunting for Earth-sized planets in the Habitable Zones of their parent stars. He is a frequent invited speaker around the world, from Prague to Porto, Moscow to Mmbatho (South Africa), Santiago to the Sunshine Coast.
Last year, he was the Jacob Bronowski Memorial Lecturer at the University of Toronto. (Carl Sagan was the inaugural Bronowski Lecturer.) In 2006, Prof. Matthews was appointed an Officer of the Order of Canada.
