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Towards Greener Nights: Exploring AI-Driven Solutions for Light Pollution Management

Paras Varshney, Niral Desai, Uzair Ahmed

TL;DR

This work tackles light pollution by building predictive pipelines that estimate night-sky brightness (limiting magnitude) across space and time using a fusion of Globe at Night and GaN-MN datasets. The approach integrates spatio-temporal context via KNN-derived features, text representations with DeBERTa v3 embeddings, and TF-IDF with PCA, evaluated through multi-fold cross-validation and ensemble learning (XGBoost, LightGBM, RandomForest). The study reports a Mean F1-Score of up to $0.81883$ on the leaderboard, with LightGBM selected as the primary engine for its balance of speed and accuracy, supported by a rigorous comparison against CatBoost and DeBERTa-based variants. The resulting framework offers actionable insights for targeting lighting interventions, reducing sky glow, and informing policy and urban planning to mitigate ecological, energy, and human health impacts, while providing a data-rich basis for ongoing monitoring of nocturnal luminosity. $F1 = 2 \cdot \frac{\text{Precision} \cdot \text{Recall}}{\text{Precision} + \text{Recall}}$ is employed as the core evaluation metric to ensure balanced performance.

Abstract

This research endeavors to address the pervasive issue of light pollution through an interdisciplinary approach, leveraging data science and machine learning techniques. By analyzing extensive datasets and research findings, we aim to develop predictive models capable of estimating the degree of sky glow observed in various locations and times. Our research seeks to inform evidence-based interventions and promote responsible outdoor lighting practices to mitigate the adverse impacts of light pollution on ecosystems, energy consumption, and human well-being.

Towards Greener Nights: Exploring AI-Driven Solutions for Light Pollution Management

TL;DR

This work tackles light pollution by building predictive pipelines that estimate night-sky brightness (limiting magnitude) across space and time using a fusion of Globe at Night and GaN-MN datasets. The approach integrates spatio-temporal context via KNN-derived features, text representations with DeBERTa v3 embeddings, and TF-IDF with PCA, evaluated through multi-fold cross-validation and ensemble learning (XGBoost, LightGBM, RandomForest). The study reports a Mean F1-Score of up to on the leaderboard, with LightGBM selected as the primary engine for its balance of speed and accuracy, supported by a rigorous comparison against CatBoost and DeBERTa-based variants. The resulting framework offers actionable insights for targeting lighting interventions, reducing sky glow, and informing policy and urban planning to mitigate ecological, energy, and human health impacts, while providing a data-rich basis for ongoing monitoring of nocturnal luminosity. is employed as the core evaluation metric to ensure balanced performance.

Abstract

This research endeavors to address the pervasive issue of light pollution through an interdisciplinary approach, leveraging data science and machine learning techniques. By analyzing extensive datasets and research findings, we aim to develop predictive models capable of estimating the degree of sky glow observed in various locations and times. Our research seeks to inform evidence-based interventions and promote responsible outdoor lighting practices to mitigate the adverse impacts of light pollution on ecosystems, energy consumption, and human well-being.
Paper Structure (19 sections, 1 equation, 9 figures, 1 table)

This paper contains 19 sections, 1 equation, 9 figures, 1 table.

Figures (9)

  • Figure 1: The 6th Street Bridge in Los Angeles before (left) and after (right) the LED conversion (Bureau of Street Lighting)
  • Figure 2: The image illustrating different components of light pollution. Courtesy Anezka Gocova, in The Night Issue (2013) b4
  • Figure 3: Map of North America’s artificial sky brightness, as a ratio to the natural sky brightness. (Falchi et al, 2016) b3
  • Figure 4: Average annual change of various features in contrast of limiting magnitude
  • Figure 5: Numerical Features Correlations with Target
  • ...and 4 more figures