A filament extends from the binary system toward the lower left and points toward the spot of light representing the candidate planet. Models suggest that the planet and binary system are a mere 300,000 years old, with the planet having a mass of about 2 to 3 Jupiters. Future observations to look for the planet's continued runaway motion and spectral signatures should be able to confirm the nature of this object. While this and other tantalizing discoveries of extrasolar planetary objects and protoplanetary disks don't seem to offer direct examples of solar systems like our own , they do strongly hint that planet formation is a varied and common process. TMR-1 likely just a background star.
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