• Home
  • Current congress
  • Public Website
  • My papers
  • root
  • browse
  • IAC-22
  • C1
  • IP
  • paper
  • study of orbital mechanics parameter using Laplace transform.

    Paper number

    IAC-22,C1,IP,24,x67210

    Author

    Mr. Bhavesh Dadhich, United States, University of Southern California

    Coauthor

    Mr. Koushik Prasade, India, SRM Institute of Science and Technology

    Coauthor

    Ms. Akshita Swaminathan, United States, University of Southern California

    Coauthor

    Mr. Udhay Venkataswamy Naidu Singuluri, United States

    Year

    2022

    Abstract
    In developing spaceflight, appointment, and disturbed satellite systems, which play an essential role in 
    space missions, it is of considerable significance to find and simulate the relative movement problem 
    between satellites or spacecraft. Orbital parameters are critical for space mission planning. A proper 
    understanding of space orbital mechanics is essential from sending a satellite to space or studying the 
    planets' movements. Newton's orbital mechanics law is primarily being utilized to obtain satellite 
    characteristics in general. However, there is another undiscovered technique in old Vedic writings that 
    yields comparable outcomes. After analyzing the patterns in the texts, they looked like the Laplace 
    function. This work presents a new technique for accurately resolving a deputy (follower) object relative 
    movement equation regarding a chief (leader) object, where both revolve around the central body in 
    elliptical orbits utilizing Laplace transform. This project aims to study orbital mechanics by recreating the 
    orbital equation using Laplace transform with respect to different orbital parameters like true 
    anomaly(Ɵ), eccentricity(e), orbital period(T), etcetera and compare the results with the results of the 
    conventional method. We shall use Kepler's assumptions to obtain our movement equations, which in 
    turn have undergone linearization. This research aims to examine orbital parameters utilizing transform 
    Laplace and compare the findings with the results of conventional techniques. The reason for the 
    computation for orbital parameters should be a simple and less time-consuming procedure. This project 
    aims to study orbital parameters using Laplace transform, and the results will be compared with the 
    results from conventional methods. The motive is to use a simple and less time-consuming process for 
    calculation for orbital parameters. The proposed method could be a convenient and less complex way to 
    calculate orbital parameters. Graph formation, instantaneous value calculation and average value 
    calculation.
    Abstract document

    IAC-22,C1,IP,24,x67210.brief.pdf

    Manuscript document

    (absent)