Venus Geological Sample Catalog

Magellan SAR Texture Analysis & ML Classification | by Henrik Hargitai & Viktor Somogyi for HUN-REN / European Space Agency (ESA) β“˜ β“˜
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Initialize Catalog

This will load 1947 geological samples, extract SAR texture features, and train classification models. This may take a few minutes on first run.

🌡️ Venus Atmospheric Explorer

An interactive exploration tool for Venus atmospheric physics. Visualize the VIRA (Venus International Reference Atmosphere) standard profile validated against real Venera/VeGa probe measurements. Experiment with a simplified 1D radiative-convective equilibrium model to understand Venus's extreme greenhouse effect. Estimate local surface temperatures from topographic elevation using the near-adiabatic lapse rate. This is an educational and exploratory tool β€” not a replacement for full General Circulation Models (GCMs).

🎓 For Students & General Audience

Venus is the hottest planet in our Solar System β€” even hotter than Mercury, despite being farther from the Sun. This is because Venus has an incredibly thick atmosphere made of carbon dioxide (CO₂) that traps heat like a giant greenhouse. The surface temperature is about 462°C (hot enough to melt lead!), and the atmospheric pressure is 92 times that of Earth. This tab lets you explore real data from spacecraft that visited Venus and experiment with a climate model to understand why Venus is so extreme.

VIRA Reference Atmosphere ℹ️

Standard Venus atmospheric profile with Venera/VeGa probe validation data

Temperature Profile

Pressure Profile

Atmospheric Structure & Composition ℹ️

Atmospheric Composition

Density Profile

1D Radiative-Convective Model ℹ️

Adjust atmospheric parameters and run the equilibrium model

Model Parameters

96.5%
30
2601 W/m²
0.76
50

Model vs VIRA Profile

Energy Budget

Surface Temperature Estimator ℹ️

Estimate local surface temperature from GTDR topographic elevation using the adiabatic lapse rate

Venus vs Earth Comparison ℹ️

📊 Candidate Object Annotation Lab

This tab provides an interactive annotation tool for creating, reviewing, and exporting bounding box and polygon annotations on Venus SAR imagery. Use it to: (1) auto-generate annotations from existing geological samples, (2) detect candidate objects from the spatial prediction pipeline with NMS deduplication, (3) manually draw new bounding boxes or polygons, (4) review and validate candidates in a structured queue. The system produces candidate structures for expert review — not definitive detections. All annotations include source tracking, status workflow (draft/reviewed/accepted/rejected), and append-only audit logging for reproducibility.

🎓 For Students & General Audience

Scientists need to mark and label geological features on Venus radar images — just like drawing rectangles or outlines around craters and volcanoes. This tool helps by automatically suggesting where features might be, then letting experts confirm or correct those suggestions. Think of it like a smart highlighter that finds interesting spots, and then a scientist checks each one. The validated data can then be exported to train even smarter AI models!

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Total Annotations
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Pending Review
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Accepted
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Rejected
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Retrain Ready
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Candidate Accuracy
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ID Category Source Status Conf. By

Selected Annotation

Click an annotation in the list or on the canvas to view details.

Annotation Statistics