The Indian Institute of Astrophysics (IIA) is a premier research institution in India that has made significant contributions to cometary modeling and simulations.

Cometary modeling and simulations aim to understand the physical processes responsible for cometary activity, such as the sublimation of ices and the formation of jets and tails.

Smoothed particle hydrodynamics (SPH) is a numerical technique that is well-suited for modeling the dynamics of cometary comae and tails due to its ability to handle large deformations and discontinuities.

COMET (COmetary Modeling and Simulation Toolkit) is an open-source software package developed by Indian researchers for simulating the dynamics and evolution of comets.

Dr. J.N. Goswami is a renowned Indian scientist who has made significant contributions to cometary modeling and simulations, including the development of COMET.

Studying cometary activity helps scientists understand the composition and structure of comets, which provides insights into their formation and evolution in the early solar system.

ISRO's Deep Space Mission, also known as the Chandrayaan-2 mission, successfully studied the comet 67P/Churyumov-Gerasimenko in 2018.

COMET (COmetary Modeling and Simulation Toolkit) was used to study the comet 67P/Churyumov-Gerasimenko during ISRO's Deep Space Mission.

The Indian Institute of Astrophysics (IIA) is involved in the development of the COMET software package.

The primary objective of the COMET software package is to understand cometary activity, including the sublimation of ices and the formation of jets and tails.

The COMET software package employs the smoothed particle hydrodynamics (SPH) technique for simulating cometary dynamics.

Dr. J.N. Goswami led the development of the COMET software package.

The Physical Research Laboratory (PRL) is involved in the study of cometary comae and tails.

The primary focus of the research on cometary comae and tails at the Physical Research Laboratory is studying the dynamics of cometary tails.

Dr. R. Rajamohan is known for his contributions to the study of cometary comae and tails at the Physical Research Laboratory.