A new dwarf planet has been identified on the fringes of our solar system. Designated 2015 RR245, the object's size hasn't been confirmed just yet, but its discoverers estimate it to have a diameter of 700 km (435 miles) and one of the largest known orbits of a dwarf planet, circling the Sun once every 700 years.

The object was first spotted back in February by the Canada-France-Hawaii Telescope in Hawaii, in images taken in September last year as part of the Outer Solar System Origins Survey (OSSOS). The survey is an ongoing collaboration between dozens of scientists at institutions from eight countries, studying the objects orbiting beyond Neptune to help piece together our solar system's turbulent past. Tens of thousands of smaller objects are estimated to lie out there, left over from the upheaval caused by the giant planets moving away from the Sun and settling into their current orbits.

"But almost all of these icy worlds are painfully small and faint," says Michele Bannister of the University of Victoria, in British Columbia. "It's really exciting to find one that's large and bright enough that we can study it in detail."

Measuring in at around half the size of Makemake, RR245 is much smaller than other known dwarf planets in the neighborhood, but still meets the International Astronomical Union's (IAU) criteria of that category: namely, it's in orbit around the Sun, it has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a nearly round shape, and, unlike regular planets, it hasn't cleared the neighbourhood around its orbit, and it isn't a satellite.