Venkataramani, KumarKumarVenkataramaniGanesh, ShashikiranShashikiranGaneshRai, ArchitaArchitaRaiHus�rik, MarekMarekHus�rikBaliyan, K. S.K. S.BaliyanJoshi, U. C.U. C.Joshi2025-08-312025-08-312019-05-0110.3847/1538-3881/ab0f262-s2.0-85067379405http://repository.iitgn.ac.in/handle/IITG2025/23297The asteroid 2014 JO25, considered to be potentially hazardous by the Minor Planet Center, was spectroscopically followed during its close-Earth encounter on 2017 April 19 and 20. The spectra of the asteroid were taken with the low-resolution spectrograph (LISA), mounted on the 1.2 m telescope at the Mount Abu Infrared Observatory, India. Coming from a region close to the Hungaria population of asteroids, this asteroid follows a comet-like orbit with a relatively high inclination and large eccentricity. Hence, we carried out optical spectroscopic observations of the asteroid to look for comet-like molecular emissions or outbursts. However, the asteroid showed a featureless spectrum, devoid of any comet-like features. The light curve of the asteroid was analyzed using V-band magnitudes derived from the spectra and the most likely solution for the rotation of the asteroid was obtained. The absolute magnitude H and the slope parameter G were determined for the asteroid in the V filter band using the IAU accepted standard two-parameter H-G model. A peculiar, rarely found result from these observations is its phase bluing trend. The relative B-V color index seems to decrease with increasing phase angle, which indicates a phase bluing trend. Such trends have seldom been reported in the literature. However, phase reddening in asteroids is very common. The asymmetry parameter g and the single-scattering albedo w were estimated for the asteroid by fitting the Hapke phase function to the observed data. The asteroid shows a relatively large value for the single-scattering albedo and a highly back-scattering surface.truemethods: observational | minor planets, asteroids: individual (2014 JO25) | techniques: spectroscopic | telescopesArticlehttps://iopscience.iop.org/article/10.3847/1538-3881/ab0f26/pdfMay 20191199arJournal1