Discovered by Scotsman James Dunlop during his first stint at the Parramatta observatory in southern Australia in August 1828, this starburst planetary nebula located in the constellation Ara contains a Wolf-Rayet star orbited by three gas giants. Each of the six moons orbiting these gas giants is a metal-rich body, which is much further from the system's core than is dictated by traditional models of stellar and planetary formation. Some physicists contend that these moons were originally inner planets from the system's pre-nebular order that were small enough to be knocked into highly elliptical orbits by CD-51 10820's stellar ejecta and ultimately captured by the gas giants. Others have postulated that they are remnants from a single, unstable metal-rich world that was ripped apart and scattered throughout the system during an early, violent period of nebular formation. Both sides have publicly called for a detailed survey of the nebula's distribution of high-metal content asteroids and planetesimals to settle this long-running debate, but unfortunately, there have been few expressions of interest in the project from the freelance cartographer community thus far.