Scientists have discovered what they believe to be a new planet, the closest one ever detected outside our solar system. It is a small, rocky planet not unlike our own, orbiting the sun’s closest stellar neighbor.
Astronomers have long suspected that the star Proxima Centauri would be home to a planet, but proof had been elusive. Dim red dwarf stars such as Proxima have been found to host billions of small, closely orbiting planets throughout the galaxy. Now a study published Wednesday in the journal Nature provides the best evidence yet for a tantalizingly close target on which to seek alien life.
“It’s so inspiring, it’s our closest star,” Lisa Kaltenegger, a Cornell astronomer who wasn’t involved in the new study, told The Washington Post. “A planet next door. How much more inspiring can it get?” Located about 4.25 light years from the sun, Proxima is less famous than the Alpha Centauri binary star system it hangs around with. But while Alpha Centauri is made up of two rather sun-like stars, Proxima is actually closer. It used to be that scientists were far more interested in stars like our own sun than in dim little dwarves like Proxima, but the times are changing – these types of stars are far more common in the galaxy, and scientists now believe they might be just as capable of hosting life as more familiar looking suns.
The proposed planet comes to light not long after a would-be-world orbiting Alpha Centauri B was determined to be nothing but a fluke in the data. Scientists know that most stars in the galaxy harbor planets, but we’ve had difficulty finding our closest companions in the cosmos.
Proxima b will no doubt be dubbed “Earthlike” by many, but let’s not jump the gun. Here’s what we know: The planet, based on statistical analysis of the behavior of its star, is quite likely to exist. Beyond that, we know very little.
Proxima b orbits its parent star every 11 days. Because of the method used to detect it, we don’t actually know how massive the planet candidate is – but we can say with confidence that it’s at least 1.3 times as massive as the Earth. It’s just over 4 million miles away from its cool, tiny red dwarf of a star (much closer than we are to our own sun), so it is blasted with enough radiation to maintain a balmy surface temperature of around minus 40 degrees Fahrenheit.
Based on what we know about the planets that form around red dwarf stars, it’s probably rocky – like Earth, Venus and Mars – and is likely tidally locked, meaning that one face of the planet constantly stares at the sun while the other half is left in darkness.
To call a planet “Earthlike,” scientists have to show that a planet is likely to be rocky and capable of holding liquid water. If Proxima b has an atmosphere – a question unlikely to be answered anytime soon – then it could have a temperature quite close to Earth’s, meaning it would at least be capable of maintaining liquid water on its surface.
Even if Proxima b has (or once had) an atmosphere and held water, the evolution of life is far from guaranteed. For one thing, we’re working with a sample size of one (the Earth) and have no idea how common the spark of life really is – even on planets that have all the same ingredients as the ones found at home.
Then there’s Proxima itself: Known as a flare star, the red devil lashes huge flares of radiation out into space every few hours.
Anything that evolved on a nearby planet would have to live deep underground or underwater to survive – unless it evolved some level of protection from radiation that scientists on Earth can scarcely imagine.
The discovery of this planet, be it Earthlike or not, has been a long time coming. Led by Guillem Anglada-Escude from Queen Mary University of London, 31 scientists from eight different countries spent several months collecting data on Proxima. They were looking to build on previous indications of planetary presence, studying the “wiggle” in the star’s light that would be caused by the seesaw gravitational pull between it and an orbiting planet (this is known as the Doppler method). Such a wiggle had been seen before, but the signal wasn’t strong enough to prove a planet was there.
Anglada-Escude and his colleagues applied for several months of observation time on the European Southern Observatory’s HARPS (High Accuracy Radial velocity Planet Searcher) spectrograph, allowing them to collect 54 nights worth of data on this telltale stellar wiggle.
“There had previously been claims of other planets, so we had to be really careful here,” Anglada-Escude said during an embargoed news briefing held by Nature on Tuesday. The data from those 54 nights made a pretty strong case for the presence of a planet, but “it wasn’t enough.” The researchers weren’t satisfied until they combined their data with the older signals, the ones that hadn’t made enough of a case on their own.
“And then the [statistical] significance goes sky high,” he said.
Others agree that while the planet has yet to be confirmed using direct observational methods, the researchers have likely found something special. ESO astronomer Henri Boffin, who previously worked as HARPS’s instrument scientist but wasn’t involved in the new research, told The Post that Proxima b’s signal looked to be about three times as strong as that of Alpha Centauri Bb, the “planet” that turned out to be nothing but noise.
“It is quite amazing that our closest stellar neighbor would harbor a low-mass planet,” Boffin said. “Even if this is not so surprising after all, as it now seems established that the vast majority of stars host at least one planet, it is still nice to have apparently found the closest to us.”
Courtsey : Wasington Post