The nucleosynthesis of 31P in stars of 30 M model with solar metallicity is investigated using the MESA (Modules for Experiments in Stellar Astrophysics) stellar evolution code. Mass loss mechanisms are included in the evolution of the star with no rotation. The mass loss mechanism used is one constructed by MESA. The paper is divided into two parts. The first part deals with the investigations of the main reactions involved in the production and destruction of 31P. The site for the nucleosynthesis of 31P is also suggested. In the second part of the paper we compare the results of our production of 31P to other papers whenever possible and discuss the need to add new reactions to the network. We also explore the possible mechanisms for the distribution of 31P to the galaxy.

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