He received the first ever Malcolm McIntosh Prize for Physical Scientist of the Year in 2000, then the Shaw Prize in Astronomy in 2006, the Gruber Cosmology Prize in 2007 and the Nobel Prize for Physics in 2011—it’s been a satisfying progression for Brian Schmidt, professor of astronomy at the Australian National University, and for Australian science. Schmidt led one of two research teams that determined that the expansion of the Universe is accelerating.
Brian Schmidt, the Malcolm McIntosh Physical Scientist of the Year 2000 and 2011 Physics Nobel Laureate. Credit: ANU
But winning awards does not mean he’s resting on his laurels. Apart from countless invitations to speak, Brian has his hands full with commissioning SkyMapper, a new optical telescope equipped with Australia’s largest digital camera at 268 megapixels. And he’s also involved in two significant new facilities pioneering technology to be used in the Square Kilometre Array (SKA), the world’s largest radio telescope: the Murchison Widefield Array and the Australian SKA Pathfinder. And in his spare time, he’s working on one of the next generation of optical telescopes, the Giant Magellan Telescope. Continue reading Prized astronomer continues to contribute→
RAVE PROJECT MANAGER, FRED WATSON, WITH THE UK SCHMIDT TELESCOPE. CREDIT: SHAUN AMY.
But already, another Australian-led innovation in astronomical instrumentation is providing researchers with the critical information they need to understand the motions of stars within different parts of our galaxy, such as its main body, the bulging core, and the extended halo that surrounds it. Researchers are also searching for evidence of galactic cannibalism—swarms of stars that could be remnants of dwarf galaxies consumed by the Milky Way.
The innovation, called the 6dF instrument, is being used by a multinational consortium, the RAdial Velocity Experiment (RAVE), to measure the radial velocities of more than half a million stars. It is mounted on the Australian National University’s UK Schmidt Telescope at Siding Spring in New South Wales. Radial velocity is movement toward or away from the observer along the light of sight, as distinct from motion across the line of sight. The survey, which began in 2003, will be completed in 2011. Continue reading Profiling and fingerprinting the stars→
On a mountaintop in northern New South Wales sits a new telescope equipped with Australia’s largest digital camera. The Australian National University’s (ANU) SkyMapper facility has been established at Siding Spring Observatory to conduct the most comprehensive optical survey yet of the southern sky.
Fully automated, the telescope is measuring the shape, brightness and spectral type of over a billion stars and galaxies, down to one million times fainter than the eye can see.
SKYMAPPER AT SIDING SPRING, NORTHERN NEW SOUTH WALES. CREDIT: AUSTRALIAN NATIONAL UNIVERSITY.
