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Moonatlas / Curated catalogue 2026.09 · science-0.3.1

Discoveries

Notable lunar observations selected from 80,740 catalogued NASA-IBM model outputs. Each entry is a model prediction over a real lunar observation, promoted by a transparent product rule and given a permanent MOONATLAS id — a selection for exploration, never a scientific ranking or a confirmed feature.

Open any entry on the Moon to see it in its geographic context, or click anywhere on the globe to explore a coordinate of your own. How the science works.

Curated discoveries

97

Craters
48
Polar ice
31
Volcanic / IMP
18

42 held-out test · 55 in-sample

97 of 97

  • Craters

    MM-CR-000009
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    49.645°S 167.460°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    32.87 km
    Confidence
    0.97
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000006

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    83.562°S 60.980°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.995

    prospectivity

    Raw peak
    1.045

    0–1 target scale

    RMSE vs ref.
    0.020

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000001
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateHeld-out test

    4.342°N 33.700°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    9,399 m²
    Tile share
    14.3 %
    Mean softmax
    0.91

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000008
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    37.405°S 170.441°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    31.64 km
    Confidence
    0.95
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000003

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    80.649°S 49.247°E

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.990

    prospectivity

    Raw peak
    1.039

    0–1 target scale

    RMSE vs ref.
    0.031

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000006
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateHeld-out test

    25.660°S 27.621°W

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    7,808 m²
    Tile share
    11.9 %
    Mean softmax
    0.90

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000011
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    45.296°N 138.839°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    29.59 km
    Confidence
    0.99
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000007

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    83.146°S 68.554°E

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.979

    prospectivity

    Raw peak
    1.011

    0–1 target scale

    RMSE vs ref.
    0.023

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000014
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    18.634°N 5.287°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    36,034 m²
    Tile share
    55.0 %
    Mean softmax
    0.99

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000012
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    69.137°N 136.240°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    28.14 km
    Confidence
    1.00
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000010

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    84.409°S 140.049°E

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.917

    prospectivity

    Raw peak
    1.030

    0–1 target scale

    RMSE vs ref.
    0.022

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000017
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    14.887°N 6.465°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    33,086 m²
    Tile share
    50.4 %
    Mean softmax
    0.98

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000013
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    62.254°S 167.922°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    25.30 km
    Confidence
    0.95
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000001

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    81.398°S 41.463°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.838

    prospectivity

    Raw peak
    1.016

    0–1 target scale

    RMSE vs ref.
    0.027

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000011
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateValidation sample

    38.111°N 44.676°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    25,807 m²
    Tile share
    39.4 %
    Mean softmax
    0.99

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000071
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    66.481°S 169.359°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    24.46 km
    Confidence
    0.95
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000004

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    80.812°S 77.541°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.629

    prospectivity

    Raw peak
    1.013

    0–1 target scale

    RMSE vs ref.
    0.031

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000022
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    7.209°N 37.650°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    25,139 m²
    Tile share
    38.4 %
    Mean softmax
    0.97

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000014
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    31.134°S 52.578°E

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    21.23 km
    Confidence
    1.00
    Diameter rank
    Top 0.2%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000012

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    82.500°S 153.057°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.614

    prospectivity

    Raw peak
    1.036

    0–1 target scale

    RMSE vs ref.
    0.023

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000021
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    25.048°N 46.768°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    21,602 m²
    Tile share
    32.9 %
    Mean softmax
    0.96

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000028
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateHeld-out test

    44.488°S 164.762°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    20.50 km
    Confidence
    0.99
    Diameter rank
    Top 0.3%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000011

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    81.194°S 124.474°E

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.610

    prospectivity

    Raw peak
    1.022

    0–1 target scale

    RMSE vs ref.
    0.025

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000024
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    14.782°N 33.856°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    20,528 m²
    Tile share
    31.3 %
    Mean softmax
    0.96

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000057
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    47.961°N 133.998°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    8.47 km
    Confidence
    1.00
    Diameter rank
    Top 3.0%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000027

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    87.112°S 33.603°E

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    1.002

    prospectivity

    Raw peak
    1.041

    0–1 target scale

    RMSE vs ref.
    0.015

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000023
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    7.786°N 6.225°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    16,318 m²
    Tile share
    24.9 %
    Mean softmax
    0.93

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000058
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    2.860°S 54.348°E

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.60 km
    Confidence
    1.00
    Diameter rank
    Top 14.8%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000032

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    88.172°S 179.504°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.998

    prospectivity

    Raw peak
    1.022

    0–1 target scale

    RMSE vs ref.
    0.018

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000015
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    36.810°N 46.367°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    7,529 m²
    Tile share
    11.5 %
    Mean softmax
    0.96

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000061
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    26.872°N 132.313°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.30 km
    Confidence
    1.00
    Diameter rank
    Top 17.2%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000023

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    83.304°S 8.828°E

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.997

    prospectivity

    Raw peak
    1.012

    0–1 target scale

    RMSE vs ref.
    0.022

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000013
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    39.665°N 38.406°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    3,458 m²
    Tile share
    5.3 %
    Mean softmax
    0.92

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000062
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    39.574°N 138.307°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    4.04 km
    Confidence
    1.00
    Diameter rank
    Top 11.8%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000038

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    84.419°S 27.327°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.990

    prospectivity

    Raw peak
    1.039

    0–1 target scale

    RMSE vs ref.
    0.018

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000020
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateValidation sample

    8.836°N 17.550°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    3,312 m²
    Tile share
    5.1 %
    Mean softmax
    0.95

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000063
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    33.403°N 138.878°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.50 km
    Confidence
    1.00
    Diameter rank
    Top 15.5%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000036

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    80.528°S 8.583°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.951

    prospectivity

    Raw peak
    1.023

    0–1 target scale

    RMSE vs ref.
    0.024

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000012
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    37.626°N 39.718°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    2,845 m²
    Tile share
    4.3 %
    Mean softmax
    0.94

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000064
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    55.077°S 165.286°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    4.80 km
    Confidence
    1.00
    Diameter rank
    Top 8.4%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000040

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    84.092°S 93.069°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.929

    prospectivity

    Raw peak
    1.026

    0–1 target scale

    RMSE vs ref.
    0.023

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000016
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    9.859°N 25.526°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    2,785 m²
    Tile share
    4.2 %
    Mean softmax
    0.90

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000065
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    28.100°N 139.135°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.71 km
    Confidence
    1.00
    Diameter rank
    Top 14.0%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000039

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    87.185°S 59.036°W

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.887

    prospectivity

    Raw peak
    1.032

    0–1 target scale

    RMSE vs ref.
    0.025

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000018
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    24.540°N 8.067°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    2,748 m²
    Tile share
    4.2 %
    Mean softmax
    0.92

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000068
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceHeld-out test

    58.300°S 170.218°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    9.29 km
    Confidence
    1.00
    Diameter rank
    Top 2.4%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Polar ice

    MM-ICE-000044

    HIGH PROSPECTIVITY REGION

    High prospectivity regionValidation sample

    82.624°S 172.860°E

    SOUTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.779

    prospectivity

    Raw peak
    1.016

    0–1 target scale

    RMSE vs ref.
    0.021

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000019
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    4.487°N 22.908°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    2,538 m²
    Tile share
    3.9 %
    Mean softmax
    0.95

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000060
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    6.883°S 53.878°E

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    4.34 km
    Confidence
    0.99
    Diameter rank
    Top 10.0%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000013

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    82.025°N 146.027°W

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.968

    prospectivity

    Raw peak
    1.008

    0–1 target scale

    RMSE vs ref.
    0.024

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000026
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    17.531°N 16.308°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    2,026 m²
    Tile share
    3.1 %
    Mean softmax
    0.91

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000070
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    74.415°N 131.999°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.03 km
    Confidence
    0.99
    Diameter rank
    Top 19.9%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000016

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    83.342°N 108.198°W

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.837

    prospectivity

    Raw peak
    1.012

    0–1 target scale

    RMSE vs ref.
    0.025

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Volcanic / IMP

    MM-IMP-000025
    IMP CANDIDATE source observation

    IMP CANDIDATE

    IMP candidateTraining sample

    7.355°N 20.944°E

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · IMP segmentation

    Predicted area
    1,808 m²
    Tile share
    2.8 %
    Mean softmax
    0.93

    uncalibrated

    Largest predicted IMP area of its observation group.

  • Craters

    MM-CR-000067
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    9.611°N 136.392°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.93 km
    Confidence
    0.97
    Diameter rank
    Top 12.5%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000017

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    85.295°N 52.514°W

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.814

    prospectivity

    Raw peak
    1.024

    0–1 target scale

    RMSE vs ref.
    0.031

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000059
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    22.221°S 53.689°E

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.24 km
    Confidence
    0.96
    Diameter rank
    Top 17.7%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000015

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    81.818°N 132.378°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.798

    prospectivity

    Raw peak
    1.014

    0–1 target scale

    RMSE vs ref.
    0.031

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000073
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    73.589°S 168.527°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.79 km
    Confidence
    0.96
    Diameter rank
    Top 13.5%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000014

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    83.915°N 173.734°W

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.748

    prospectivity

    Raw peak
    1.029

    0–1 target scale

    RMSE vs ref.
    0.027

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000069
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    58.736°N 131.680°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    4.69 km
    Confidence
    0.95
    Diameter rank
    Top 8.8%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000018

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    87.966°N 178.885°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.718

    prospectivity

    Raw peak
    1.020

    0–1 target scale

    RMSE vs ref.
    0.034

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000072
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    64.195°N 136.035°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.28 km
    Confidence
    0.95
    Diameter rank
    Top 17.4%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000020

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    82.249°N 11.528°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.693

    prospectivity

    Raw peak
    1.019

    0–1 target scale

    RMSE vs ref.
    0.035

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000066
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsHeld-out test

    19.040°N 137.760°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    6.25 km
    Confidence
    0.93
    Diameter rank
    Top 5.4%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Polar ice

    MM-ICE-000019

    HIGH PROSPECTIVITY REGION

    High prospectivity regionHeld-out test

    80.140°N 66.350°W

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.686

    prospectivity

    Raw peak
    1.025

    0–1 target scale

    RMSE vs ref.
    0.031

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000037
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateTraining sample

    12.437°N 101.048°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    40.21 km
    Confidence
    0.99
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000033

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    83.789°N 64.675°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.993

    prospectivity

    Raw peak
    1.018

    0–1 target scale

    RMSE vs ref.
    0.025

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000035
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateValidation sample

    7.982°S 33.445°E

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    39.24 km
    Confidence
    1.00
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000029

    HIGH PROSPECTIVITY REGION

    High prospectivity regionValidation sample

    85.748°N 96.517°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.984

    prospectivity

    Raw peak
    1.026

    0–1 target scale

    RMSE vs ref.
    0.030

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000033
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateTraining sample

    69.094°N 159.551°E

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    38.60 km
    Confidence
    0.94
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000041

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    86.724°N 42.553°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.961

    prospectivity

    Raw peak
    1.021

    0–1 target scale

    RMSE vs ref.
    0.030

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000050
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateTraining sample

    15.259°N 160.185°E

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    38.08 km
    Confidence
    0.97
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000021

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    80.823°N 173.279°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.921

    prospectivity

    Raw peak
    1.019

    0–1 target scale

    RMSE vs ref.
    0.031

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000049
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateTraining sample

    43.220°N 88.767°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    37.35 km
    Confidence
    1.00
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000043

    HIGH PROSPECTIVITY REGION

    High prospectivity regionValidation sample

    83.285°N 13.758°W

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.645

    prospectivity

    Raw peak
    1.031

    0–1 target scale

    RMSE vs ref.
    0.036

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000046
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateTraining sample

    2.611°N 160.330°E

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    36.04 km
    Confidence
    0.94
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000042

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    80.764°N 53.659°E

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.617

    prospectivity

    Raw peak
    1.012

    0–1 target scale

    RMSE vs ref.
    0.030

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000034
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateTraining sample

    71.172°N 105.144°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    35.54 km
    Confidence
    0.99
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Polar ice

    MM-ICE-000037

    HIGH PROSPECTIVITY REGION

    High prospectivity regionTraining sample

    80.169°N 124.596°W

    NORTH POLAR REGION

    NASA-IBM LFM · polar ice prospectivity

    Raw P90
    0.597

    prospectivity

    Raw peak
    1.023

    0–1 target scale

    RMSE vs ref.
    0.029

    MOONATLAS derived

    Highest raw P90 prospectivity of its polar area.

  • Craters

    MM-CR-000047
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Large candidateTraining sample

    53.909°N 87.406°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    33.52 km
    Confidence
    0.96
    Diameter rank
    Top 0.1%

    MOONATLAS derived

    Largest confident detections of the analyzed tiles.

  • Craters

    MM-CR-000074
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceTraining sample

    61.690°N 88.941°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    4.41 km
    Confidence
    1.00
    Diameter rank
    Top 9.8%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000076
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceTraining sample

    4.635°N 102.870°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.20 km
    Confidence
    1.00
    Diameter rank
    Top 18.1%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000077
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceTraining sample

    17.044°S 143.850°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.13 km
    Confidence
    1.00
    Diameter rank
    Top 18.8%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000078
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceValidation sample

    5.418°S 29.628°E

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.08 km
    Confidence
    1.00
    Diameter rank
    Top 19.3%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000079
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceTraining sample

    25.889°N 87.514°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.35 km
    Confidence
    1.00
    Diameter rank
    Top 16.7%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000080
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceTraining sample

    35.066°N 88.909°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.31 km
    Confidence
    1.00
    Diameter rank
    Top 17.1%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000082
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceTraining sample

    17.089°N 103.136°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.38 km
    Confidence
    1.00
    Diameter rank
    Top 16.5%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000083
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    High confidenceTraining sample

    1.059°S 78.307°E

    NEARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.30 km
    Confidence
    1.00
    Diameter rank
    Top 17.2%

    MOONATLAS derived

    Confidence ≥ 0.99 and at least 3 km across.

  • Craters

    MM-CR-000085
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsTraining sample

    32.660°N 107.062°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.94 km
    Confidence
    1.00
    Diameter rank
    Top 12.4%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Craters

    MM-CR-000075
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsTraining sample

    49.788°N 85.493°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.25 km
    Confidence
    0.99
    Diameter rank
    Top 17.7%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Craters

    MM-CR-000088
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsTraining sample

    6.082°N 162.779°E

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.88 km
    Confidence
    0.99
    Diameter rank
    Top 12.8%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Craters

    MM-CR-000087
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsTraining sample

    67.006°S 144.453°W

    FARSIDE · SOUTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.62 km
    Confidence
    0.99
    Diameter rank
    Top 14.7%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Craters

    MM-CR-000089
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsTraining sample

    22.054°N 85.875°W

    NEARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.04 km
    Confidence
    0.99
    Diameter rank
    Top 19.7%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Craters

    MM-CR-000084
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsValidation sample

    39.459°N 103.704°E

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    3.03 km
    Confidence
    0.99
    Diameter rank
    Top 19.9%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Craters

    MM-CR-000081
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsValidation sample

    52.864°N 101.184°E

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    6.03 km
    Confidence
    0.98
    Diameter rank
    Top 5.8%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

  • Craters

    MM-CR-000086
    CRATER CANDIDATE source observation

    CRATER CANDIDATE

    Unmatched with RobbinsTraining sample

    21.742°N 105.419°W

    FARSIDE · NORTHERN HEMISPHERE

    NASA-IBM LFM · WAC crater detection

    Diameter
    7.57 km
    Confidence
    0.98
    Diameter rank
    Top 3.8%

    MOONATLAS derived

    No Robbins (2019) reference crater matched under the IoU ≥ 0.5 rule. It does not mean a new or previously unknown crater.

Held-out test and in-sample

Every entry is a genuine lunar observation and a genuine model output. The badge describes evaluation provenance only: held-out test samples were not used to train or tune the downstream task, so they are the ones evaluation uses; training and validation samples are in-sample, published for coverage and exploration and never quoted as independent evidence of model performance.

Selection rules

Craters enter as large candidates, high-confidence candidates or candidates unmatched with the Robbins (2019) reference. Unmatched means no reference crater matched under the configured IoU ≥ 0.5 criterion. It does not imply a newly discovered or previously unknown crater.

What the values mean

Ice prospectivity is an unconstrained regression against a 0–1 expert target, not a probability of ice. IMP mean softmax is uncalibrated, and an IMP candidate is not an active volcano. Crater counts are model detections: overlapping tiles detect the same crater more than once.