The Northern May Ophiuchids is a
poorly known annual meteor shower whose activity
period extends from April, 25 to May, 31, peaking
around May 13 [1]. It is included in the IAU list of
working meteor showers with code 149 NOP. Thus,
the development of a continuous observing campaign
can provide helpful data to increase or knowledge
about this shower. In particular, multi-station events
would be useful to calculate precise orbital data and
different physico-chemical properties of meteoroids
belonging to the NOP stream. Besides, the chemical
nature of these particles of interplanetary matter can be
inferred from the analysis of the emission spectrum
produced when they ablate in the atmosphere. Here we
present the analysis of a NOP fireball recorded in the
framework of the fireball monitoring and spectroscopic
campaign organized by the SPanish Meteor
Network (SPMN)
