Open AccessMl Driven Prediction of Collision of Milky Way & Andromeda
Author(s) -
A.P. Mittal,
Anusurya,
Deepika Kumar,
G. Vijaya Kumar
Publication year - 2019
Publication title -
international journal of recent technology and engineering
Language(s) - English
Resource type - Journals
ISSN - 2277-3878
DOI - 10.35940/ijrte.a1116.098319
Subject(s) - milky way , galactic center , physics , andromeda , astrophysics , collision , black hole (networking) , galactic plane , supermassive black hole , astronomy , galaxy , computer science , computer network , routing protocol , routing (electronic design automation) , computer security , link state routing protocol
The 3D position of Sun with respect to the galactic center of Milky Way can be used to understand its evolution. After Milky Way collides with Andromeda(M31), the same will hold true. Ensuing sections deal with the implementation of Regressive Analysis to predict the location of Sun in the galactic center after Galactic collision. This model utilizes results of previous studies of black hole mergers to predict the resultant mass of Sagittarius A* and M31’s black hole, which had been found to be (1.49±0.16) × 108 M☉. This mass has been used to calculate the centrifugal force that Sun might experience during and after the galactic collision. The current position, inclination, and velocity of Sun (derived from aforementioned predictions) have been used to predict its distance and inclination after the collision which has been predicted as 63,362.83 ly and 32.75o , from the new galactic center and its plane (97.48% and 96.32% accurate) respectively.