The magnetic field of Mercury was measured on two fly-bys of the plane
t by the Mariner 10 space-craft. The presence of a field at Mercury is
interesting for what it implies for both the internal and external so
urces of field. The internal field of the planet is almost certainly g
enerated by an internal dynamo although there remain many puzzles as t
o how a dynamo is sustained given expectations of the thermal history
of Mercury. The external sources of field are associated with the sola
r wind interaction with the planet. There is a magnetospheric cavity f
ormed about the planet in the solar wind. It seems likely that magneto
spheric phenomena such as substorms and pulsations like those that occ
ur in the terrestrial environment occur in the Mercury magnetosphere.
This fact not only tests our understanding of these processes at Earth
but also carries strong implications that there is continual electrom
agnetic processing of the outer layers of the planet by magnetospheric
processes. (C) 1997 Elsevier Science Ltd.