SystemOnline
Craters
CRATER CANDIDATE
9.611°N 136.392°W · FARSIDE · NORTHERN HEMISPHERE
- DiameterEstimated diameter
- 3.93 km
- ConfidenceModel confidence
- 0.97
- Diameter rankDiameter rank
- Top 12.5%
MOONATLAS derived
The NASA-IBM LFM crater detection model predicts a crater candidate about 3.9 km across with confidence 0.97. It is a model detection, not a reference catalog entry. No Robbins (2019) reference crater matched this detection under the IoU ≥ 0.5 rule; that does not make it a new or previously unknown crater.
Why MOONATLAS selected this
Unmatched with Robbins
No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater. 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.
M1201022087CE · 85 predicted boxes · 132 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
- 0.973
- DIAMETERAI prediction · NASA-IBM LFM
- 3.932 km
- REFERENCE MATCHMOONATLAS derived metric
- No
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
- M1201022087CE_r7528_c1112.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-m1201022087ce-r7528-c1112#32
- 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.