Antonika Shapovalova

Young Researcher in Astronomy & Earth Observation
SAR Flood Mapping & Geospatial Modeling
Dual-Enrollment Student, Yavapai Community College
Phi Theta Kappa Honor Society

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Projects

FloodRadar is an applied research project focused on flood detection and evacuation modeling
Awards:

NASA Space Apps Challenge — Global Nominee
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Investigating Exoplanets and Searching for Potential Signatures of Intelligent Life Beyond Earth 2026
A team-based research project focused on analyzing light from exoplanetary systems and investigating potential biosignatures and technosignatures.
Fields: Astrophysics, Astronomy, Data Science
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Detectability of Earth-like Atmospheres 2026
Applied research project focused on ultraviolet transmission spectroscopy and biosignature detectability modeling for Earth-like exoplanet atmospheres
FloodRadar is an applied remote sensing project that integrates multi-sensor SAR imagery with routing algorithms to support evacuation planning during extreme precipitation events. The system processes SAR backscatter data to detect inundated regions and classify low-water crossings using thresholding and machine-learning–based refinement methods to generate flood masks.
These outputs are integrated with OpenStreetMap road networks and OSRM routing to evaluate road accessibility and compute evacuation corridors and shelter accessibility under dynamic hydrological conditions. The project demonstrates an end-to-end workflow for operationalizing satellite data in community-level emergency response.

Awards:
NASA Space Apps Challenge — Global Nominee
This research analyzes physical and orbital characteristics of exoplanetary systems using data from public astronomical catalogs. The study examines planetary radii, equilibrium temperatures, orbital parameters, and atmospheric indicators associated with habitability.
Methods include multivariable correlation analysis, parameter-space mapping, and hypothesis-driven classification of candidate planets. The project develops an analytical framework for prioritizing targets for future spectroscopy-based habitability and technosignature studies.
Detecting atmospheres around Earth-sized exoplanets is a critical step toward identifying potentially habitable worlds, yet such atmospheres produce extremely weak observational signals. This study investigates the detectability of an Earth-like atmosphere using ultraviolet transmission spectroscopy and examines which wavelength ranges provide the strongest atmospheric signatures during planetary transits.
An Earth-like atmospheric model was implemented using realistic altitude profiles of temperature, pressure, and molecular abundances based on terrestrial atmospheric data. Ultraviolet absorption cross sections of key atmospheric species (including oxygen, ozone, nitrogen oxides, and sulfur dioxide), derived from existing laboratory spectroscopic databases, were incorporated
into the model to compute wavelength-dependent absorption of stellar radiation. The cumulative absorption was translated into an effective atmospheric height, representing the apparent increase in planetary radius during transit, while accounting for instrumental spectral resolution and realistic stellar ultraviolet emission.
The results show that atmospheric detectability is strongly wavelength dependent. Ultraviolet wavelengths yield significantly larger transmission signals than longer wavelengths due to efficient absorption by oxygen- and ozone-related features, which dominate the atmospheric signature. Other trace gases contribute smaller effects. The predicted transit depth variations reach several parts per million for an Earth-sized planet, with detectability strongly influenced by host star brightness through its impact on signal-to-noise ratio.
This study demonstrates how Earth serves as a reference system for interpreting exoplanet observations. These findings highlight ultraviolet transmission spectroscopy as a promising approach for future space missions, including concepts such as the Habitable Worlds Observatory, aimed at detecting Earth-like atmospheres and assessing planetary habitability beyond the Solar System.

In addition, the model explicitly evaluates photon budgets and noise sources, enabling quantitative estimates of the observation time required to detect atmospheric signatures at a given signal-to-noise ratio.

Publications

Detecting Exoplanet Atmospheres Using the Habitable Worlds Observatory
June 2026
Authors: A. Shapovalova
Repository: Astrophysics Data System
Bibcode: 2026ASTCS..1100141S
Year: 2026

This study develops a physics-based ultraviolet transmission spectroscopy framework designed to evaluate the detectability of Earth-like atmospheres around Earth-sized exoplanets. The implementation combines realistic atmospheric profiles of temperature, pressure, and molecular abundances with laboratory-measured ultraviolet absorption cross sections for key species, including oxygen, ozone, nitrogen oxides, and sulfur dioxide. Wavelength-dependent molecular absorption is converted into an effective atmospheric height to model the apparent increase in planetary radius during transit, while accounting for instrumental spectral resolution and realistic stellar ultraviolet emission. The resulting framework computes wavelength-dependent transmission signals and transit depth variations, enabling quantitative analysis of which ultraviolet regions provide the strongest atmospheric signatures. The results show that oxygen- and ozone-related absorption produces significantly stronger ultraviolet signals than longer-wavelength observations, with predicted transit depth variations reaching several parts per million for Earth-sized planets. By using Earth as a reference system and incorporating potential atmospheric biosignatures, this work provides a quantitative approach for interpreting exoplanet observations and evaluating the capabilities of future missions such as the Habitable Worlds Observatory in the search for Earth-like atmospheres and potentially habitable worlds.
Detectability of an Earth-like Atmosphere in Ultraviolet Transit Spectroscopy: Effective Atmospheric Height, Transit Depth, and Signal-to-Noise Constraints
January 2026
Authors: A. Shapovalova
Repository: Aerospace Research Central
DOI: https://doi.org/10.2514/6.2026-115779
Year: 2026
Detecting atmospheres around Earth-sized exoplanets is critical for finding habitable worlds, but their observational signals are extremely weak. This study models an Earth-like atmosphere using realistic temperature, pressure, and gas profiles to calculate transit absorption across ultraviolet (UV) wavelengths. The results show that UV transmission spectroscopy yields significantly larger signals than longer wavelengths, driven by strong absorption from oxygen and ozone. While trace gases show smaller effects, the overall transit depth variations reach several parts per million. Ultimately, this research uses Earth as a reference system to demonstrate that UV spectroscopy is a promising approach for future space missions, like the Habitable Worlds Observatory, to assess exoplanet habitability.

Patents

FloodRadar: SAR-Based Automated Flood Detection and Safe Routing System
November 2025
Application Number: 63/922,936
Inventor: Antonika Shapovalova
Filing Date: November 21, 2025
Status: Patent Pending
A provisional patent application filed with the USPTO.
The invention introduces an automated framework for flood detection and safe evacuation routing using multi-sensor SAR satellite imagery, hydrological data, and machine-learning classification. The system identifies flood extent, evaluates road accessibility, and computes optimized evacuation paths under real-world disaster constraints.
Status: Patent Pending (US 63/922,936).

Public Scientific Presentations

2026 CURIC Symposium at Elgin Community College
April 27, 2026
Colorado-Wyoming Junior Academy of Science 68th Annual Science and Engineering Symposium
April 18, 2026
AIAA Region 3 Student Conference
University of Michigan, Ann Arbor, Michigan
April 10–11, 2026
Exoplanet Atmospheres 2026 (AASTCS 11)
Hilton Denver City Center - Denver, CO
March 16–20, 2026
The Zodiac Signs and How They Are Defined
Elgin Community College — Elgin, IL
November 11, 2025
Synthetic Aperture Radar (SAR): Principles and ApplicationsNorthwest Suburban Astronomers (NSA) — Harper College, Illinois
November 7, 2025

Awards

NASA International Space Apps Challenge 2025 - Global Nominee
Oct 2025
NASA Space Grant Consortium Award
State Science Fair 
Mar 2026
U.S. Naval Science Award
Office of Naval Research
Mar 2026
Mathematical Olympiads for Elementary and Middle Schools
Top 2% Scorer
National
2026
National Award -  Continental Mathematics League (CML)
Top 1% Nationally 
National
2026
National Award - Math League
National
April 2026
6th Place MATHCOUNTS 
State 
Mar 2026
28th Place Mathematical Kangaroo Competition 2026
National
Mar 2026
1st Place – Physics & Astronomy
State Science Fair
Mar 2026
WEST Inc. Special Award
State Science Fair
Mar 2026
Phi Theta Kappa (PTK) — International Honor Society
Inducted based on outstanding academic achievement (Elgin Community College)
Mar 2026
AMC 8
Score: 20/25, One Point Below National Top 5% Honor Roll Cutoff
National
Jan 2026
Naval Science Award - Office of Naval Research (U.S. Navy)
Senior Division - Southeast Regional Science Fair
Regional
Jan 2026
Regional Science Fair
First Place - Physics & Astronomy
Regional
Jan 2026
Midwest Middle & High School Chinese Speech Contest - 3rd Place
Regional
Spring 2024, 2025

Experience

Member - Phi Theta Kappa Honor Society
GPA: 3.88
Status: Dual-Enrollment
Illinois, USA
2024-2026
Elgin Community College
Calculus with Analytic Geometry
Biology for Contemporary Society
College Algebra
Trigonometry
English Composition
Astronomy
Principles of Sociology
2026- Present
Arizona, USA
Status: Dual-Enrollment
Yavapai Community College
Current Classes
2021–Present
Illinois, USA
GPA: 3.96
Wyoming, USA
At Vero Homeschooling, I study an advanced curriculum that allows me to strengthen core academic skills while progressing at an accelerated pace. My coursework emphasizes math, science, and problem-solving. I enjoy developing independent learning strategies and consistently maintain strong academic performance.

Education

GPA: N/A
2022–2024
Illinois, USA
During middle school, I focused on building a strong academic foundation through advanced coursework, especially in math and science. I enjoy problem-solving and connecting concepts across subjects
Illinois Science Assessment (Grade 7)
Exemplary (Level 4), Top 1–3% in Illinois
MAP Growth (Math)
99th percentile
MAP Growth (Reading)
95th percentile
Standardized Assessments:
2017–2022
Illinois, USA
Programs:
Advanced Mathematics Enrichment Program, Summer 2022

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Illinois Science Assessment (Grade 7)
Exemplary (Level 4), Top 1–3% in Illinois
MAP Growth (Math)
99th percentile
MAP Growth (Reading)
95th percentile
Standardized Assessments:
Barbara B. Rose Elementary School (Grades K–5)

Additional University-Level Coursework

Rice University - AdvPHY1x: Topics in AP Physics
February 2025
Verified online university-level courseworkRICEdX / edX - Non-credit; not equivalent to on-campus enrollment
Delft University of Technology - PUCH1x: Pre-University Chemistry
April 2025
Verified online university-level coursework DelftX / edX - Non-credit; not equivalent to on-campus enrollment
Rice University  - Introduction to Biology: Ecology, Evolution & Biodiversity
Jun 2025
Online university-level coursework Coursera - Non-credit; not equivalent to on-campus enrollment

Skills

Media

Only 13, Carpentersville girl already a seasoned student at Elgin Community College

14-year-old invited to present planetary research at Denver conference

Wyoming Space Grant Alumna Makes Waves with NASA-recognized Projects

Chicago Tribune

Laramie’s Antonika Shapovalova, age 14, making waves with NASA-recognized projects

Laramie's Antonika Shapovalova, age 14, is making waves with NASA-recognized projects

Wyoming Public Media

Chicago Tribune

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