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We have developed a model to calculate the emission intensities of variousvibrational transitions of N$_2$ triplet band and Lyman-Birge-Hopfield (LBH)band emissions in the dayglow of Pluto for solar minimum, moderate, and maximumconditions. The calculated overhead intensities of Vegard-Kaplan ($A^3\Sigma_u^+ - X^1\Sigma^+_g $), First Positive ($ B^3\Pi_g - A^3\Sigma^+_u$), Second Positive ($ C^3\Pi_u - B^3\Pi_g $), Wu-Benesch ($W^3\Delta_u -B^3\Pi_g$), Reverse First Positive, and LBH ($a^1\Pi_g$-- $X^1\Sigma^+_g$)bands of N$_2$ are 17 (74), 14.8 (64), 2.4 (10.8), 2.9 (12.7), 2.9 (12.5), and2.3 (10) R, respectively, for solar minimum (maximum) condition. We havepredicted the overhead and limb intensities of VK (150-190 nm) and LBH (120-190nm) bands of N$_2$ on Pluto for the New Horizons (NH) flyby condition that canbe observed by Alice: the ultraviolet imaging spectrograph also know asP-Alice. The predicted limb intensities of VK and LBH bands peak at radialdistance of $ \sim$2000 km with the value of about 5 (13) and 9.5 (22) R forsolar zenith angle 60$ ^\circ $ (0$ ^\circ $), respectively. We have alsocalculated overhead and limp intensities of few prominent transition of COFourth Positive bands for NH flyby condition.

Production of N2 Vegard-Kaplan and Lyman-Birge-Hopfield emissions on Pluto