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 an illustrative 1D radiative-convective equilibrium model (a teaching tool, not a flux-conserving General Circulation Model/GCM) to understand Venus's extreme greenhouse effect. Estimate local surface temperatures from topographic elevation using the VIRA reference profile (primary), compared with a 7.7 K/km linear lapse rate.

🎓 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

Closed-form gray (Eddington) radiative-equilibrium profile with a dry-adiabat convective adjustment β€” an illustrative teaching model, not a flux-conserving GCM

Illustrative model The infrared (greenhouse) optical depth is a tuned knob, not derived from line-by-line radiative transfer. The model does not close the planetary energy budget; its fidelity is reported as RMSE against the VIRA reference profile.

Model Parameters

illustrative 96.5%
illustrative 30
measured 2601 W/m²
measured 0.76
50

Model vs VIRA Profile

Greenhouse diagnostics (illustrative)

Surface Temperature Estimator ℹ️

Estimate local surface temperature from GTDR topographic elevation: VIRA reference profile (primary) compared with a 7.7 K/km linear lapse rate

Radar brightness vs surface temperature ℹ️

Explore how SAR radar-brightness varies with GTDR elevation and VIRA-interpolated surface temperature, per candidate geological category — the Venus highland radar-bright phenomenon as an interpretability aid.

Interpretability aid over candidate regions. SAR backscatter brightness is not calibrated emissivity; brightness also depends on incidence geometry, roughness, slope, latitude and sampling.

Brightness vs elevation (candidate threshold)

Brightness vs VIRA surface temperature

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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Acceptance Rate
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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

πŸ“Š Functions & Usage

Find catalog samples whose SAR+DTM texture signatures resemble one or more reference samples. Pick reference FIDs, optionally restrict the search to a lon/lat region, choose a distance metric (cosine or euclidean) and reference mode (mean centroid or nearest-of-references), and rank candidates. Results can be promoted to annotations for expert review.

πŸŽ“ For Students & General Audience

Pick one or more places on Venus that you find interesting. The computer compares their "texture fingerprint" (how rough, patterned, and high-up they are in radar) against every other place in the catalog, and shows you the ones that look most similar.

Reference Samples β“˜

Region Restriction (optional) β“˜

Draw a Region to Search β“˜

Drag a rectangle on the map to mark an area of interest. The system samples its texture fingerprint and finds catalog samples that look alike β€” no reference FID needed.

Results β“˜

πŸ“Š Functions & Usage

Manage the 13 broad geological categories without mutating the source dataset. Rename and merge categories, split a category by moving specific FIDs to a new one, or reassign a single sample. All changes are persisted as a reversible override layer with an audit log. Re-initialize the catalog to restore the original defaults; individual changes can also be reset (Admin only).

πŸŽ“ For Students & General Audience

This is where experts can rename or combine geological categories (for example, merging two overlapping plains types) without losing the original data. Every change is recorded so it can be reviewed or rolled back later.

Categories β“˜

Category Samples Flags Actions

Operations β“˜

Rename

Merge

Split

Reassign sample

Audit Log