Nature magnifying glass discloses unanticipated transitional mass exoplanets. Astronomers have discovered a contemporary exoplanet that could change the existing theory of planet formation. A mass that is between Neptune and Saturn and its position beyond the snow line of its host star, an unknown world of this magnitude was presumed to be exceptional.
Aparna Bhattacharya, a postdoctoral researcher from the University of Maryland and her team made a discovery which was declared recently. Utilizing the Near-Infrared Camera, second generation (NIRC2) apparatus on the 10-meter Keck II telescope of the W. M. Keck Observatory on Maunakea, Hawaii and the Wide Field Camera 3 (WFC3) instrument on the Hubble Space Telescope, the researchers captured synchronous high intent images of the exoplanet, named OGLE-2012-BLG-0950Lb, permitting them to condition its mass.
Bhattacharya exclaimed that they were startled to observe the mass exuding right in the center of the forecast transitional mammoth planet mass gap; it was like finding an oasis in the center of exoplanet desert.
Co-author David Bennett, a senior research scientist at the University of Maryland and GSFC said that he was extremely pleased with the swiftness with which Aparna finished her analysis. She had to advance some contemporary methods to inspect the data, a kind of analysis that had never been executed earlier.
In a supernatural turn of events alternative team of astronomers issued a statistical analysis at mostly the same time depicting that such sub-Saturn mass planets do exist after all.