  Using James Webb Space Telescope near-infrared data of the inner Orion
Nebula, \citet{Pearson_McCaughrean_2023} detected 40 Jupiter-Mass Binary
Objects (JuMBOS). These systems are not associated with stars and their
components have masses of giant Jupiter-like planets and separations in the
plane of the sky of order $\sim$100 au. The existence of these wide
free-floating planetary mass binaries was unexpected in our current theories of
star and planet formation. Here we report the radio continuum (6.1 and 10.0
GHz) Karl G.\ Jansky Very Large Array detection of a counterpart to JuMBO\,24.
The radio emission appears to be steady at a level of $\sim$50 $\mu$Jy over
timescales of days and years. We set an upper limit of $\simeq15$~km~s$^{-1}$
to the velocity of the radio source in the plane of the sky. As in the
near-infrared, the radio emission seems to be coming from both components of
the binary.
