  We present observations of the disintegrating long-period comet C/2019 J2
(Palomar) taken to determine the nature of the object and the cause of its
demise. The data are consistent with break-up of a sub-kilometer nucleus into a
debris cloud of mass or order 1e9 kg, peaking on UT 2019 May 24+/-$12. This is
56 days before perihelion and at a heliocentric distance of 1.9 AU. We consider
potential mechanisms of disintegration. Tidal disruption is ruled-out, because
the comet has not passed within the Roche sphere of any planet. Impact
disruption is implausible, because the comet orbit is highly inclined
(inclination 105.1 deg) and disruption occurred far above the ecliptic, where
asteroids are rare. The back-pressure generated by sublimation (0.02 to 0.4
N/m2) is orders of magnitude smaller than the reported compressive strength (30
to 150 N/m2) of cometary material and, therefore, is of no importance. The
depletion of volatiles by sublimation occurs too slowly to render the nucleus
inactive on the timescale of infall. However, we find that the e-folding
timescale for spin-up of the nucleus by the action of sublimation torques is
shorter than the infall time, provided the nucleus radius is smaller than 0.4
km. Thus, the disintegration of C/2019 J2 is tentatively interpreted as the
rotational disruption of a sub-kilometer nucleus caused by outgassing torques.
