Back To Projects

Using Machine Learning to identify the Habitability of Exoplanets from TESS Transit Data

Eve B.

With so many new tools and methods to detect exoplanets, it is time to start determining which are deserving of more research in the hunt for other habitable planets.


With so many new tools and methods to detect exoplanets, it is time to start determining which are deserving of more research in the hunt for other habitable planets. We began our research with exoplanets that are similar to Earth as the most likely to house life. We used transit measurements such as an exoplanet's size, temperature, and relative distance from its star as well as machine learning to develop two models: one to predict if an object of interest was an exoplanet and another to cluster our data to determine its similarity to Earth. We achieved an 88.7% accuracy for the first model, and our clustering algorithm found interesting results when compared to a graph showing the principal components of the data. We found that our Earth data point fell right on the origin of our 2 dimensional PCA graph and was placed in our largest cluster. Both of our models showed that machine learning can be useful in the search for habitable exoplanets and is deserving of more research.

Explore More!

Eve B.
Tomer Arnon
MS Engineering at Stanford

Related Projects

Predictive Analysis of Aircraft Engine Lifespan: Leveraging Neural Networks on NASA's C-MAPSS Dataset

This research paper explores the application of neural networks for predictive maintenance of aircraft engines, focusing on the estimation of their Remaining Useful Life (RUL).
Sambhav A.
Mentored by
Findings Provided by a Machine Learning Clustering Model of Stellar Kinematics in Star Clusters Can be Used to Identify Runaway Stars

The need for developing a machine learning model that can detect these runaway stars is established in this research as it attempts to expand the domain of astrophysics to help astrophysicists understand tidal tail formation and the theoretical dark matter subhalos’ effects on celestial bodies.
Roneet D.
Mentored by Tony Rodriguez
Using Deep Learning to Predict the Half-Lives of Isotopes Given Proton and Neutron Count

This study explores using deep learning regression models to predict superheavy isotopes' half-lives based on proton and neutron counts, finding that additional complexity in input variables and model architecture may be necessary to improve prediction accuracy.
Akilan P.
Mentored by Erick Ruiz