telescope glimpses population freefloating planets

Our observations pointed an elderly, ailing telescope with blurred vision at one the most densely crowded parts of the sky, where there are already thousands of bright stars that vary in brightness, and thousands of asteroids that skim across our field. These signals are extremely difficult to find. Roughly one out of every million stars in our Galaxy is visibly affected by microlensing at any given time, but only a few percent of these are expected to be caused by planets. This produces a short burst in brightness that can last from hours to a few days. Predicted by Albert Einstein 85 years ago as a consequence of his General Theory of Relativity, microlensing describes how the light from a background star can be temporarily magnified by the presence of other stars in the foreground. Such planets may perhaps have originally formed around a host star before being ejected by the gravitational tug of other, heavier planets in the system. These new events do not show an accompanying longer signal that might be expected from a host star, suggesting that these new events may be free-floating planets. However, the four shortest events are new discoveries that are consistent with planets of similar masses to Earth. Many of these had been previously seen in data obtained simultaneously from the ground.

The study team found 27 short-duration candidate microlensing signals that varied over timescales of between an hour and 10 days.

The study, led by Dr Iain McDonald of The University of Manchester, UK, (now based at the, UK) used data obtained in 2016 during the K2 mission phase of NASA’s Kepler Space Telescope.ĭuring this two-month campaign, Kepler monitored a crowded field of millions of stars near the centre of our Galaxy every 30 minutes in order to find rare gravitational microlensing events. The results include four new discoveries that are consistent with planets of similar masses to Earth, published today in Monthly Notices of the Royal Astronomical Society. Tantalising evidence has been uncovered for a mysterious population of ’free-floating’ planets which may be alone in deep space, unbound to any host star. Abstract: The Extremely Large Telescopes currently under construction have a collecting area that is. The delivered image quality approaches Gemini’s diffraction limit, with an average measured full-width at half-maximum (FHWM) of 0.09 arcsecond. Their Ks measurements of the Galactic globular cluster NGC 1851 are combined with HST photometry and the resulting color-magnitude diagram demonstrates that the ground-based data is of an unprecedented depth and precision for crowded field observations. It also illustrates the remarkable potential of MCAO-equipped Extremely Large Telescopes of the future. Their data present the most accurate and deepest near-infrared photometry from the ground of a crowded field. However, Paolo Turri (University of Victoria, Canada) and colleagues have used the Gemini Multi-conjugate adaptive optics System (GeMS) with the Gemini South Adaptive Optics Imager (GSAOI) to do just that. 30 September 2015: Expecting to resolve stars deep into the crowded field of a globular cluster is a tall order for ground-based telescopes.

Telescope glimpses population freefloating planets