  Using XMM Newton data, we investigate the nature of the X-ray emission in the
radio relic 1253+275 in the Coma cluster. We determine the conditions of the
cluster gas to check current models of relic formation, and we set constraints
on the intracluster magnetic field. Both imaging and spectral analysis are
performed, and the X-ray emission is compared with the radio emission. We found
that the emission is of thermal origin and is connected to the sub-group around
NGC 4839. The best-fit gas temperature in the region of the relic and in its
vicinity is in the range 2.8 - 4.0 keV, comparable to the temperature of the
NGC 4839 sub-group. We do not detect any high temperature gas, resulting from a
possible shock in the region of the Coma relic. We therefore suggest that the
main source of energy for particles radiating in the radio relic is likely to
be turbulence. From the X-ray data, we can also set a flux upper limit of 3.2 x
10e-13 erg/cm^2 s, in the 0.3 - 10 keV energy range, to the non-thermal
emission in the relic region. This leads to a magnetic field B > 1.05 microG.
