In our solar system, the largest planets are dominated by the gas giants located in the outer solar system. And in exoplanetary systems, large planets seem to be the norm based on our improving detection capabilities. One reason may be due to the fact that the larger planets have more mass and can accrete gas in disks which ultimately form planetary systems. This week, we welcome Sivan Ginzburg, a Postdoctoral Researcher and 51 Pegasi b Fellow working in theoretical #astrophysics from the Department of Astronomy at #Berkeley (@ucberkeley). He also has research interests in planetary formation and evolution. Please join us TODAY, Friday 31 May 2019, from 12-1 PM in @UCLA ’s Geology Building for his talk titled: ‘Accretion and Final Mass of Gas Giants’. Image Credit: NASA/JPL/UniverseToday #nasa #astro #cosmos #DTLA #education #EPSS #exoplanets #explore #GasGiants #Jupiter #LosAngeles #Neptune #origins #outreach #pizza #planet #physics #SantaMonica #Saturn #sky #solarsystem #space #UCBerkeley #UCLA #universe #universetoday #Uranus (at Institute for Planets & Exoplanets - IPLEX) https://www.instagram.com/p/ByInWFWgq_J/?igshid=oxzyyj84yadi















