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Planetary Defense Against Near-Earth Asteroids and Multi-planet Exoplanet Systems
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Studying near-earth asteroids and multi-planet exoplanet systems using open science since 2021.

Asteroid (2977) Chivilikhin Rotation Period: Revisiting a Decade Later

Arushi Nath. 30 January 2026
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Results published in the Minor Planet Bulletin. Volume 53, Number 1, 2026.
The Minor Planet Bulletin (MPB) call list is a key resource for astronomers to identify asteroids that are due for observational campaigns. When (2977) Chivilikhin appeared on the list for its 2025 apparition, I decided to measure its lightcurve again, as its rotation period had last been measured nearly a decade ago. My observations revealed a synodic rotation period of 6.257 ± 0.001 hours with a peak-to-peak amplitude of 0.98 magnitudes. This result aligns perfectly with the 2016 data (6.257 ± 0.0007 hours), showing that the asteroid’s rotation has remained stable.
 Read more 

Extending Exoplanet Ephemerides using N-Body Simulations:  In preparation for the European Space Agency's Ariel Telescope 

 Arushi Nath. 8 October 2025 
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Presenting at 5th ExoClock Annual Meeting in Mard, Spain.
On October 4, 2025, I gave an oral presentation of my year-long research, "Extending Exoplanet Ephemerides through TTV Analysis with NEPTUNE and Ground-Based Observations," at the 5th ExoClock Annual Meeting held at the Polytechnic University of Madrid, Spain. I shared how I performed 100,000+ computer simulations of Transit Timing Variations (TTVs) and combined them with ground based photometry data to extend the orbital ephemerides of exoplanets. The meeting was attended by 100+ scientists and astronomers working on refining exoplanet ephemerides in preparation for the ESA Ariel telescope. Read More

N-body Exoplanet Prediction Using TTV for Unseen Exoplanets (NEPTUNE): Wins Third Grand Award at the International Science and Engineering Fair (ISEF 2025), USA

Arushi Nath. 18 May 2025
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Winning Third Grand Award at 2025 ISEF in Colombus, Ohio
I represented Canada at the 2025 Regeneron International Science and Engineering Fair (ISEF). My project, "NEPTUNE: N-body Exoplanet Prediction Using TTV for Unseen Exoplanets," won the Third Grand Prize in the Physics and Astronomy category. My research combines N-body simulations and Transit Timing Variations (TTVs) to detect unseen exoplanets, improving orbital ephemerides and aiding in the discovery of new planetary companions. This work was validated with Kepler-46b data and continues to expand with contributions to NASA’s TESS and ESA’s ExoClock initiatives. Read more 

Developing Algorithms to Determine Asteroid's Physical Properties: Wins Second Prize Award at the European Union Contest for Young Scientists (EUCYS 2023), Brussels

The 34th European Union Contest for Young Scientists (EUCYS) was held in Brussels, Belgium. It brought together 136 promising young scientists aged 14 to 20, from 36 countries across the EU and beyond for a five-day competition.  I was honored to represent Canada as Winner of the Top Award of the 2023 Canada-Wide Science Fair. My project "Developing Algorithms to Determine Asteroid's Physical Properties and Success of Deflection Missions" won the second prize. I was the youngest contestant and the prize winner.
Read more: https://www.monitormyplanet.com/posts/1393  

 Canada-Wide Science Fair (CWSF) 2023 Best Project Award

Developing Algorithms to Determine Asteroid's Physical Properties and Success of Deflection Missions 
The 2023 Canada-Wide Science Fair (CWSF) organised by Youth Science Canada took place in Edmonton, Alberta, from May 14 to May 19, 2023. It brought together some 396 regional science fair finalists from 7th to 12th grade from across Canada.  My project "Developing algorithms to determine asteroid’s physical properties and success of deflection missionswon the 2023 Best Project Award of the Canada-Wide Science Fair (Innovation). I will now represent Canada at the European Union Contest for Young Scientists (EUCYS) in Brussels in September 2023.
In addition to the Best Project Award, I won 5 more awards:
  • Gold Medal
  • The Actuarial Foundation of Canada Award
  • Excellence in Astronomy Award from the Royal Astronomical Society of Canada
  • Top of the Category Award in Curiosity and Ingenuity
  • Youth Can Innovate Award
I also won the 2022 Best Project Award last year, becoming the first back-to-back best project award winner since 1989-1990 and the youngest ever to do so.

For more information on my project visit: https://www.monitormyplanet.com/posts/1393

Research on " Citizen Science for NASA Double Asteroid Redirection Test (DART) Mission" Presented at the 2023 Planetary Defense Conference, UNOOSA, Vienna

Arushi Nath. 15 April 2023
The 8th Planetary Defense Conference was held at the United Nations Office for Outer Space Affairs (UNOOSA) in Vienna, Austria, from 3 - 7 April 2023.  I was thrilled that my research abstract, "Citizen Science for NASA DART Mission: How I Used Robotic Telescopes, Open-Data, Python, and Maths to Study the Didymos System Before and After the Impact," was accepted as an in-person poster presentation at the Conference. Two years I gave an oral presentation of research on asteroid Apophis via webcam as the 2021  Planetary Defense Conference was held virtually. This year I presented my citizen science work on planetary defense using robotic telescopes and open data, in particular on the characterization of Near-Earth Objects (NEOs) and measuring the impact of the NASA Double Asteroids Redirection Test (DART) Mission.

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Lunar and Planetary Science Conference (LPSC) 2023 Poster Presentation

(My Research Poster in 20 threaded tweets)
Strengthening Planetary Defense: Developing Algorithms to Determine the Physical Properties of Asteroids using Robotic Telescopes and Applying them to Measure the Impact of NASA’s DART Asteroid Deflection Mission

The pace of discovery of near-earth asteroids outpaces current abilities to analyze them. Knowledge of an asteroid's physical properties is essential to deflect them. I developed open-source algorithms that combine images from robotic telescopes and open data to determine asteroids' size, rotation, and strength. I took observations of the Didymos binary asteroid, and my algorithm determined it to be 850m wide, with a 2.26-hour rotation period and rubble pile strength. I measured a 35-minute decrease in the mutual orbital period after impact by the 2022 NASA DART Mission. External sources validated the findings. Every citizen scientist is now a planetary defender.

https://lpsc2023.ipostersessions.com/default.aspx?s=95-60-E2-17-9B-F9-00-E5-DE-30-39-F3-57-70-5D-0C&guestview=true

Publication: Finding Unknown Asteroids to Strengthen Planetary Defence

Arushi Nath. Journal of the Royal Astronomical Society of Canada. Volume 117.  February 2023.

 The success of the NASA Double Asteroid Redirection Test (DART) Mission in slamming a kinetic impactor on moonlet Dimorphos of asteroid Didymos on 2022 September 26 and changing its orbit has put the planetary defence on world news. The challenge of planetary defence intrigues me. Roughly 66 million years ago, an asteroid at least 10–kilometres wide may have led to the extinction of dinosaurs. If humans do not want to suffer the same fate, then we need to be well-informed and prepared to handle any threats of an asteroid colliding with Earth.

https://www.rasc.ca/sites/default/files/publications/jrasc2023-feb-hr.pdf

iTelescope.net Webinar: Asteroid Science with Remote Telescope with a focus on DART Mission

Arushi Nath. 30 November 2022.
Citizen science and robotic telescopes have brought astronomy to everyone, from school kids to backyard astronomers and those staying in rural areas with dark skies to city dwellers living under a light cloud. For the past two years, Arushi Nath, age 13, has been using robotic telescopes, open datasets, python algorithms, and middle school maths to undertake research on near-earth asteroids. Astrometry-related observations helped her identify asteroids, provide information about their celestial location, and predict their future locations. Photometry involved taking images of the asteroid to find its magnitude. Longer observations yield a change in magnitude, which makes it possible to find the rotational period. For binary asteroids, she uses light curves to find the moonlet’s orbital period. As with all her research, she makes her datasets and methodology open source to reach out to other youths and citizen scientists.

https://hotpoprobot.com/2022/11/24/webinar-asteroid-science-with-remote-telescope/

Strengthening Planetary Defense: Detecting Unknown Asteroids using Open Data, Math, and Python

I took images from 4 telescopes located at different latitudes to get full sky coverage. I wrote Python algorithms to query European Space Agency’s GAIA and NASA’s Horizon sky catalogues to find all known stars and asteroids. Mean, standard deviation, and histograms created masks to remove known objects. The remaining objects were classified as possible asteroid candidates.
I detected 3 ‘preliminary’ asteroids. Using the telescope's focal length and celestial location, my algorithm’s plate-solving ability determined its Right Ascension and Declination. I reported this information by creating a Minor Planet Center report for my images. I have made my code and methodology open-source to crowdsource planetary defense.