Kepler telescope glimpses population of free-floating planets

Tantalising evidence has been found for a mysterious "free-floating", or unbound, population of planets. Four new discoveries, which are consistent with Earth-sized planets, were published in Monthly Notices of the Royal Astronomical Society. Iain McDonald, now at the Open University in the UK, was the study's leader. The data used for the study were obtained during NASA's K2 mission phase of its Kepler Space Telescope. Kepler observed a dense field of millions stars close to the center of our Galaxy for two months in order to detect rare gravitational microlensing phenomena. The team discovered 27 candidate microlensing signals with short durations that varied in time between one hour and 10 days. Many of these signals were previously observed in ground data. The four shortest events, however, are new discoveries consistent with similar-sized planets to Earth. These new events don't show the accompanying longer signal expected from a star. This suggests that they may be free-floating, or even planetary events. These planets could have formed originally around a star, before being ejected from the gravitational pull of heavier planets in this system. Microlensing was predicted by Albert Einstein 85 year ago, as a result of his General Theory of Relativity. It describes how light from a background star can temporarily be magnified by other stars in its foreground. This causes a brief burst of brightness that can last for hours or days. One out of every million stars of our Galaxy is visible affected by microlensing, though only a small percentage of these can be attributed to planets. Kepler was not intended to search for planets with microlensing or to study dense star fields in the inner Galaxy. To find signals in the Kepler data, new data reduction techniques were needed. Iain writes: "These signals can be extremely difficult to locate." We pointed an elderly telescope with blurred vision to one of the most densely populated parts of the sky. There are thousands of bright stars, each with a different brightness, as well as thousands of asteroids, which skim across the field. We try to find tiny brightenings that are characteristic of planets from this cacophony. Unfortunately, we only have one chance at seeing a signal before it disappears. It's as simple as searching for a single flash of a firefly on a motorway median using a handheld cellphone. Eamonn Kerins from the University of Manchester comments that Kepler has done what it was never intended to, providing more tentative evidence for the existence of a free-floating population of planets. It now passes the baton to other missions, which will be looking for such signals. These signals are so rare that Einstein thought they would never be observed. It is exciting that the ESA Euclid mission, which will be joining this mission as an additional science activity, could also participate in it. Future missions like the NASA Nancy Grace Roman Space Telescope and possibly the ESA Euclid will focus on confirmation of the existence and nature free-floating planets. Both of these missions will be optimized to search for microlensing signal.

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