SystemOnline
Craters
CRATER CANDIDATE
26.872°N 132.313°W · FARSIDE · NORTHERN HEMISPHERE
- DiameterEstimated diameter
- 3.30 km
- ConfidenceModel confidence
- 1.00
- Diameter rankDiameter rank
- Top 17.2%
MOONATLAS derived
The NASA-IBM LFM crater detection model predicts a crater candidate about 3.3 km across with confidence 1.00. It is a model detection, not a reference catalog entry.
Why MOONATLAS selected this
High confidence
Confidence ≥ 0.99 and at least 3 km across. Product curation over model outputs, not a scientific ranking.
Dataset split
Held out of training and tuning, so this sample is the kind used to evaluate the model. That is evaluation provenance, not physical importance.
M1112693892CE · 97 predicted boxes · 152 Robbins (2019) reference boxes
A model detection on one analyzed tile, not a catalogued crater and not a unique physical crater: SomBench tiles overlap, so the same crater can be detected on more than one tile.
Model outputs
- CONFIDENCEAI prediction · NASA-IBM LFM
- 1.000
- DIAMETERAI prediction · NASA-IBM LFM
- 3.299 km
- REFERENCE MATCHMOONATLAS derived metric
- Yes
Provenance
- Model
- NASA-IBM Lunar Foundation Model
- Task
- Crater detection on LROC WAC imagery
- Checkpoint
- WAC_ni_lfm_ps8_lora_s46.ckpt
- Dataset
- sombench-wac-crater-detection
- Split
- Held-out test
- Source
- M1112693892CE_r14184_c872.tif
- Processing
- science-0.3.1
- Data origin
- Real model output
Scientific details
- Model id
- lfm-crater-detection
- Model revision
- f09ebeae2099
- Reference
- robbins-2019
- Object id
- wac-m1112693892ce-r14184-c872#0
- Catalogued
- 2026-09-17
Values are model output as produced, or MOONATLAS derived metrics computed from it; reference annotations are shown separately and never mixed into predictions. How MOONATLAS works.