By Daniel Clery
Astronomers are staring at a nearby star in hopes of seeing a giant baby of a planet pass across its face, perhaps accompanied by dust clouds, rings, or newborn moons. Last week, the newest and tiniest telescope joined the vigil, when the French-built PicSat rode into orbit on an Indian rocket. It will be able to continuously monitor the star, β Pictoris, until chances of seeing the once-in-20-year transit event diminish in a few months’ time. “We can’t miss this. We would be kicking ourselves,” says astronomer Matthew Kenworthy of Leiden University in the Netherlands.
Astronomers have seen thousands of exoplanets transit, or cross the face of their stars, eclipsing a fraction of their light. But β Pictoris, a bright star just 63 light-years away, is special. It is a natural laboratory for how solar systems form because it is only 24 million years old—the “equivalent of a baby of a few weeks,” says Sylvestre Lacour of the Paris Observatory.
In 1984, astronomers observed a disk of gas and dust around it, the first protoplanetary disk to be seen. The disk, viewed nearly edge on, was warped and had gaps, a sign of planets in the making. But it wasn’t until 2009 that researchers spied the faint glow of a hot, young giant planet, 10 times the mass of Jupiter, in a roughly 20-year orbit. Now dubbed β Pictoris b, it is one of only a handful of exoplanets to be imaged directly.
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