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ice_likelihood
float64
0.800741
1
0.773542
0.9375
0.768378
0.953125
0.8675
0.795417
0.759583
0.9375
0.770081
0.670001
0.700209
0.682708
0.9375
0.682293
0.584168
0.288125
0.439584
0.516088
0.128125
0.523334
0.005417
0.23875
-0.030625
0.21
0.833333
0.557499
0.791619
0.670416
0.400661
0.75147
0.735035
0.884684
0.791666
0.713803
0.817709
0.921875
0.691358
0.670001
0.9375
0.800417
0.763125
0.450416
0.757917
0.601876
0.550834
0.441249
0.284375
0.266875
0.539793
0.19
-0.121875
-0.029375
0.22
0.05375
0.153125
0.28
0.669374
0.325833
0.10875
-0.0175
0.23125
0.21875
-0.02375
0.108125
0.178125
0.36375
0.457499
0.13625
-0.145625
-0.0825
0.229375
0.20125
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-0.1275
0.106875
0.2475
0.350625
0.238125
0.348333
0.18375
0.106875
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-0.09875
0.169375
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-0.143125
-0.148125
-0.27375
0.135
0.362917
0.128125
-0.191875
-0.194375
-0.158125
-0.198125
0.1825
-0.245625
-0.18875
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Hello!

cMars8k is a collection of 8,120 200x200 .jpg images of Martian craters, as well as their corresponding likelihoods of having subsurface ice at a depth of 0-1m.

A short explanation of how the dataset was derived:

  • The THEMIS IR Day Map was used to create this dataset, owing to its lightweight nature and scientific reputability.
  • Robbins & Hynek's 2020 Mars crater database was used to source the geographic coordinates of the craters' (approximate) centers.
  • NASA's SWIM Project 0-1m Ice Consistency map was used to source the likelihood of subsurface ice at the location of each crater.
  • All of these individual datasets were combined together by overlaying them on top of each other inside of QGIS, and then utilizing a python script to mass-export the images.

Data Formatting

As stated, each image is exactly 200x200 pixels and is stored as a .jpg file within cMars8k/images. The ice_likelihood value is a float64 ranging from approximately -0.375 to 1.000, with 1.000 representing an extremely high probability or confirmed presence of subsurface ice.

Accessing Data

This dataset can be accessed via:
!git clone https://huggingface.co/datasets/evans44/cMars8k
or via the Hugging Face API.

Normalization

Many CNNs prefer normalized images as opposed to RGB. The following script loads the images directly from the downloaded folder into a pandas dataframe and performs said action.
!! Note: within metadata.csv, the file_name for each image is in the format images/crater_####, and as such the images directory/folder does not need to be specified when accessing the images.

import pandas as pd
import cv2
from concurrent.futures import ThreadPoolExecutor
import os

# Load metadata
metadata = pd.read_csv("cMars8k/metadata.csv")

IMAGES_DIR = "cMars8k"  # file_name column already includes "images/" prefix

def load_and_normalize(file_name):
    path = os.path.join(IMAGES_DIR, file_name)
    img = cv2.imread(path)                       # loads as BGR, uint8, shape (200, 200, 3)
    img = cv2.cvtColor(img, cv2.COLOR_BGR2RGB)    # convert to RGB
    img = img.astype(np.float32) / 255.0          # normalize to [0, 1]
    return img

with ThreadPoolExecutor(max_workers=8) as executor:
    images = list(executor.map(load_and_normalize, metadata["file_name"]))

df_master = pd.DataFrame({                                # 3 columns:
    "file_name": metadata["file_name"],                   # file_name (over from metadata.csv)
    "image": images,                                      # image: the normalized version of the image
    "ice_prob": metadata["ice_likelihood"]                # ice_prob: probability of ice (over from metadata.csv/ice_likelihood)
})

print("Shape of df_master:")
print(df_master.shape)
print(df_master["image"].iloc[0].shape, df_master["image"].iloc[0].dtype)
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