None of the nearly 1,900 planets previously discovered and confirmed outside our solar system (called exoplanets) are in the process of formation.
The findings of the scientists, led by University of Arizona graduates Steph Sallum and Kate Follette and including the University of Sydney’s Professor Peter Tuthill, were published recently in Nature.
A star known as LkCa 15, located 450 light years from Earth, has been observed exhibiting all the trappings of an expectant parent: it is surrounded by a vast disc of dust and gas, making an ideal environment for planets to grow from; the dust shows distinct signs of disturbance—something within has eaten away part of the disc.
Co-author of the paper Professor Tuthill said the images provided unambiguous evidence. “This is the first time we’ve imaged a planet that is definitely still in the process of forming.”
The photo provided the proof: “The difficulty had been that when you have indirect evidence, there are always alternate explanations that might fit the data,” Professor Tuthill said.
Researchers are just now being able to image objects that were close to and much fainter than a nearby star, thanks to specialised instruments. These include the Large Binocular Telescope, or LBT—the world’s largest telescope, located on Arizona’s Mount Graham—and the University of Arizona’s Magellan Telescope and its Adaptive Optics System, MagAO, located in Chile.
Capturing sharp images of distant objects was challenging, in large part because of atmospheric turbulence, said Professor Laird Close, Dr Follette’s graduate adviser.
“When you look through the Earth’s atmosphere, what you’re seeing is cold and hot air mixing in a turbulent way that makes stars shimmer,” Professor Close said. “To a big telescope, it’s a fairly dramatic thing; you see a horrible looking image.” The breakthrough was possible because the Large Binocular Telescope was purpose-built, incorporating a novel imaging technique to sharpen the images.
Meanwhile, Professor Close and Dr Follette used Magellan’s adaptive optics system MagAO independently to corroborate the discovery. Using MagAO’s unique ability to work in visible wavelengths, they captured the planet’s ‘hydrogen alpha’ spectral fingerprint, the specific wavelength of light that LkCa 15 and its planets emit as they grow.
When cosmic objects are forming, they get extremely hot, and because they are forming from hydrogen, those objects all glow a deep red. That single shade of red light was emitted by both the planet and the star as they underwent the same growing process, Dr Follette said.
“We were able to separate the light of the faint planet from the light of the much brighter star and to see that they were both growing and glowing in this very distinct shade of red,” she said.
Professor Tuthill said the results were only made possible because of the application of a lot of very advanced new technology to the business of imaging the stars.
“It’s fantastic to see these cutting-edge instruments now enabling us to make such exciting discoveries,” Professor Tuthill said.
University of Sydney School of PhysicsThe University of Sydney School of Physics is the leading physics department in the country, with outstanding staff and students undertaking world-leading teaching and research.
The university’s 100 staff and 150 postgraduate students conduct research across a vast range of interests from nanoparticles to clusters of galaxies and from theoretical modelling to laboratory experiments. With access to supercomputers, modern laboratory facilities and observatories, locally, nationally and internationally, the School of Physics is the premier environment for physics education and research.