  We describe the main features of a new and updated version of the program
PArthENoPE, which computes the abundances of light elements produced during Big
Bang Nucleosynthesis. As the previous first release in 2008, the new one,
PArthENoPE 2.0, will be soon publicly available and distributed from the code
site, http://parthenope.na.infn.it. Apart from minor changes, which will be
also detailed, the main improvements are as follows. The powerful, but not
freely accessible, NAG routines have been substituted by ODEPACK libraries,
without any significant loss in precision. Moreover, we have developed a
Graphical User Interface (GUI) which allows a friendly use of the code and a
simpler implementation of running for grids of input parameters. Finally, we
report the results of PArthENoPE 2.0 for a minimal BBN scenario with free
radiation energy density.
