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Near Earth Objects (NEOs) Statistical Analysis Project

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Overview

This project explores Near Earth Objects (NEOs), particularly asteroids, to assess their potential hazard to Earth through data-driven statistical analysis. Using publicly available datasets and Python-based tools, we analyze orbital and physical properties of asteroids and apply logistic regression to model their hazard classification.

Objectives

  • Data Collection & Cleaning: Acquire NEO data, clean it using Excel Power Query and Python.
  • Exploratory Data Analysis (EDA): Analyze variable distributions, correlations, and patterns.
  • Statistical Analysis: Examine how size, orbit, and type relate to hazard potential.
  • Logistic Regression: Train a model to classify whether an asteroid is potentially hazardous.
  • Insights & Conclusion: Summarize findings and their implications for planetary defense.

Getting Started

  1. Clone the Repository

    git clone https://github.com/HaiderPhys21/NEO_statAnalysis.git
    
    
  2. Install Dependencies

    pip install -r requirements.txt
  3. Run the Analysis Explore Jupyter notebooks in the notebooks/ directory, which walk through:

    • Data cleaning
    • EDA
    • Logistic regression modeling

Repository Structure

NEO_statAnalysis/
├── data/             # Input data files (optional or downloadable)
├── notebooks/        # Jupyter notebooks with analysis steps
├── requirements.txt  # Python dependencies
├── LICENSE
└── README.md

Citation

If you use this project in your research, please cite it using the Zenodo DOI (after publishing to Zenodo).

License

This project is licensed under the MIT License.


Created by Syed Haider Ali

About

Conducted statistical analysis of Hazardous Near-Earth Asteroids (NEAs) to identify key parameters contributing to their hazard potential. Developed and implemented a Machine Learning Model to model the impact of different parameters on NEA hazard potential, leading to more accurate predictions of future asteroid impacts.

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