Planet Mars is currently an object of increasing scientific and public inte
rest. Several spacecraft are on their way or planned to be sent to our neig
hbour planet to unravel its secrets. One of the most unknown properties of
planet Mars is whether it possesses a planetary magnetic field of dynamo or
igin. Observed weak surface magnetic herds seem to argue against a currentl
y operating planetary dynamo. However, weak surface fields are also expecte
d if a polarity reversal occurs. We shall discuss arguments in favour and a
gainst the speculation that Mars still operates an active dynamo with the w
eak surface magnetic fields pointing towards an ongoing reversal. As the po
ssible way to validate this speculation we discuss the importance of a sphe
rical harmonic expansion of the Martian magnetic field. The planned NetLand
er project and its anticipated magnetic field measurements are a powerful t
ool to provide at least a low-order spherical harmonic expansion coefficien
t determination of the Martian magnetic field, thereby allowing to study ch
aracteristics of crustal magnetic field anomalies as well as giving clues t
o the question whether Mars is a planet in magnetic transition. (C) 2000 El
sevier Science Ltd. All rights reserved.