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demo/tile_102057/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:704f635471e1f86f4ccbed821c050033693427e2403d3951fe72a267d4218fb5
+size 15207561

demo/tile_102057/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 102057,
+ "role": "mare",
+ "lat": 47.8759,
+ "lon": -25.9272,
+ "unit": "Im2",
+ "gt_age_ga": 3.4,
+ "pos_text": "long=25\u00b055'38.03\"W, lat=47\u00b052'33.21\"N",
+ "reference_closed_book": "The scene is very dark (albedo 0.15) and very smooth \u2014 local relief ~200 m, roughness ~50 m \u2014 while the Clementine UV/VIS ratio (~0.43) reads as a near-neutral ratio color. Regional crater statistics date the adjacent mapped basalts to roughly 3.4 Ga, within the Imbrian. The Basin Massif Unit (Ibm) forms the foundational structural element here, representing the ancient crustal response to large-scale impact events prior to subsequent volcanic infilling. I see the Upper Mare Unit (Im2) clearly overlying these massifs, which leads me to conclude that mare volcanism occurred after the initial formation of the basin's topographic highs. Within the vicinity of the crater Cavendish, the superposition of the Crater Unit (pNc) across both the volcanic flows and the underlying massifs provides a clear stratigraphic sequence where impact cratering represents the most recent geological"
+}

demo/tile_103725/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:a7635c3d03a295f4ecc77ba4af5f690b66fda428d833fb9a3a2df9eaf8254f30
+size 15207561

demo/tile_103725/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 103725,
+ "role": "mare",
+ "lat": 57.8801,
+ "lon": -23.3945,
+ "unit": "Em",
+ "gt_age_ga": 3.5,
+ "pos_text": "long=23\u00b023'40.31\"W, lat=57\u00b052'48.26\"N",
+ "reference_closed_book": "The scene is very dark (albedo 0.15) and very smooth \u2014 local relief ~200 m, roughness ~50 m \u2014 while the Clementine UV/VIS ratio (~0.44) reads as a near-neutral ratio color. Regional crater statistics date the adjacent mapped basalts to roughly 3.5 Ga, within the Imbrian. The Imbrium Apenninus Formation Unit (Iiap) serves as the foundational basement here, underlying both the Basin Massif Unit (Nbm) and the Upper Mare Unit (Im2). I view the relationship between these layers as a clear sequence of volcanic resurfacing, where the Nbm was emplaced over the ancient Iiap before being subsequently buried by the Im2. This superposition indicates that the Upper Mare Unit represents the most recent major event in this area, effectively capping the older, more complex terrain. While the presence of the small satellite feature Herigonius B provides a useful"
+}

demo/tile_127989/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:b6085ed57361b605f435232580d82dc43ad4a5ea9e7c8ea7c5c565ef09637b1f
+size 15207561

demo/tile_127989/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 127989,
+ "role": "highland",
+ "lat": 3.4129,
+ "lon": 12.9076,
+ "unit": "Ip",
+ "gt_age_ga": 3.8,
+ "pos_text": "long=12\u00b054'27.17\"E, lat=3\u00b024'46.40\"N",
+ "reference_closed_book": "The scene is bright (albedo 0.29) and smooth \u2014 local relief ~1200 m, roughness ~300 m \u2014 while the Clementine UV/VIS ratio (~0.45) reads as a near-neutral ratio color. The Imbrium Apenninus Formation Unit (Iiap) serves as the foundational basement here, underlying all subsequent volcanic activity within the vicinity of Newton. I see the Mare Unit (Em) and Upper Mare Unit (Im2) overlying this older formation, which clearly indicates a period of post-Imbrian volcanism that flooded the pre-existing terrain. The Basin Massif Unit (Nbm) appears to be contemporaneous with or slightly younger than the Iiap, suggesting its structural development was tied to the massive impact event that created the Imbrium basin. Finally, the Crater Unit (pNc) cross-cuts every other visible layer, leading me to conclude that impact cratering represents the most"
+}

demo/tile_131356/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:85a8228a0595da4ab8f4f677a40d432a47b2bb40cda93e47fcba18ddb23d15a2
+size 15207561

demo/tile_131356/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 131356,
+ "role": "mare",
+ "lat": 6.1918,
+ "lon": 17.973,
+ "unit": "Im2",
+ "gt_age_ga": 3.8,
+ "pos_text": "long=17\u00b058'22.66\"E, lat=6\u00b011'30.57\"N",
+ "reference_closed_book": "The scene is very dark (albedo 0.15) and smooth \u2014 local relief ~1400 m, roughness ~300 m \u2014 while the Clementine UV/VIS ratio (~0.53) reads as a blue-shifted (higher-Ti, fresher) ratio color. Regional crater statistics date the adjacent mapped basalts to roughly 3.6 Ga, i.e. the Imbrian. The Imbrium Apenninus Formation Unit (Iiap) serves as the foundational basement for this landscape within Mare Humorum, representing the oldest crustal component visible here. I see subsequent volcanic activity evidenced by the Mare Unit (Em), which clearly overlies this ancient formation and marks a period of significant basaltic flooding. The Basin Massif Unit (Nbm) appears to be contemporaneous with or slightly younger than the Em, likely formed through localized uplift during the same era of basin-related volcanism. Finally, the Crater Unit ("
+}

demo/tile_131658/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:344c66735f72f16c98b43faeb290b83df14845177b4539c5eeaa2c8edc5f11b8
+size 15207561

demo/tile_131658/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 131658,
+ "role": "highland",
+ "lat": -5.4797,
+ "lon": 18.3951,
+ "unit": "Nt",
+ "gt_age_ga": 3.8,
+ "pos_text": "long=18\u00b023'42.24\"E, lat=5\u00b028'46.97\"S",
+ "reference_closed_book": "The scene is bright (albedo 0.29) and moderately rugged \u2014 local relief ~1500 m, roughness ~400 m \u2014 while the Clementine UV/VIS ratio (~0.53) reads as a blue-shifted (higher-Ti, fresher) ratio color. The Basin Massif Unit (Nbm) forms the foundational structural element here, representing the oldest crustal component visible beneath more recent volcanic flows. I see the Upper Mare Unit (Im2) clearly overlying this massif, which leads me to conclude that widespread mare volcanism occurred after the initial formation of the basin's topographic highs. The Plains Unit (Ip) appears to partially bury both the Nbm and the Im2, suggesting a later period of plains emplacement that post-dates the primary volcanic flooding. Finally, the Crater Unit (Nc) cross-cuts all underlying layers, marking the most recent phase of impact-driven modification in this area near"
+}

demo/tile_73525/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:8ebf4e53ca9be39bb252101f732328230ae9c83d3f08ea98b2789d7ec76ec86d
+size 15207561

demo/tile_73525/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 73525,
+ "role": "highland",
+ "lat": -24.3765,
+ "lon": -68.9832,
+ "unit": "Ioho",
+ "gt_age_ga": 3.4,
+ "pos_text": "long=68\u00b058'59.47\"W, lat=24\u00b022'35.38\"S",
+ "reference_closed_book": "The scene is bright (albedo 0.28) and smooth \u2014 local relief ~1500 m, roughness ~350 m \u2014 while the Clementine UV/VIS ratio (~0.36) reads as a red-shifted (lower-Ti, more mature) ratio color. The Inner Facies Unit of the Orientale Hevelius Formation dominates this landscape, representing the massive ejecta blanket deposited during the formation of the Orientale basin. I view these deposits as the primary product of the multi-ring impact event that shaped the southwestern highlands, where the sheer volume of material excavated and redistributed across the region created this complex stratigraphy. Near the satellite feature Lippmann R, the surface texture reflects the intense energy of that impact, which fundamentally restructured the local crustal architecture through widespread excavation and subsequent deposition."
+}

demo/tile_90313/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:1f2c9d4cfdd5cad1495811cd16324b8bb16e7357ec9ecd87aff288eeda6f87d5
+size 15207561

demo/tile_90313/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 90313,
+ "role": "mare",
+ "lat": 15.6402,
+ "lon": -43.6562,
+ "unit": "Em",
+ "gt_age_ga": 3.5,
+ "pos_text": "long=43\u00b039'22.17\"W, lat=15\u00b038'24.77\"N",
+ "reference_closed_book": "The scene is very dark (albedo 0.13) and very smooth \u2014 local relief ~200 m, roughness ~50 m \u2014 while the Clementine UV/VIS ratio (~0.48) reads as a near-neutral ratio color. Regional crater statistics date the adjacent mapped basalts to roughly 3.5 Ga, within the Imbrian. The Imbrium Apenninus Formation Unit (Iiap) serves as the foundational basement here, underlying both the Basin Massif Unit (Nbm) and the Upper Mare Unit (Im2). I view the relationship between these layers as a clear progression of volcanic resurfacing, where the Nbm was emplaced atop the older Iiap before being eventually buried by the more recent Im2 flows. This sequence of superposition allows me to reconstruct a history beginning with the massive impact event that formed the Imbrium basin, followed by subsequent mass wasting and volcanism. While I am confident in this relative"
+}

demo/tile_92835/inputs.pt

@@ -0,0 +1,3 @@
+version https://git-lfs.github.com/spec/v1
+oid sha256:abde26fa11565ec7c55997d0ddaddf75cc9fd63b7d35e83449a5d4d0cf2edd02
+size 15207561

demo/tile_92835/meta.json

@@ -0,0 +1,10 @@
+{
+ "full_idx": 92835,
+ "role": "mare",
+ "lat": 19.5307,
+ "lon": -39.8571,
+ "unit": "Im2",
+ "gt_age_ga": 3.5,
+ "pos_text": "long=39\u00b051'25.57\"W, lat=19\u00b031'50.62\"N",
+ "reference_closed_book": "The scene is very dark (albedo 0.15) and very smooth \u2014 local relief ~200 m, roughness ~50 m \u2014 while the Clementine UV/VIS ratio (~0.44) reads as a near-neutral ratio color. Regional crater statistics date the adjacent mapped basalts to roughly 3.4 Ga, within the Imbrian. The Basin Massif Unit (Ibm) forms the foundational structural element here, representing the ancient crustal response to large-scale impact events prior to subsequent volcanic infilling. I see the Upper Mare Unit (Im2) clearly overlying these massifs, which leads me to conclude that mare volcanism occurred after the initial formation of the basin's topographic highs. Within the vicinity of the crater Cavendish, the superposition of the Crater Unit (Nc) across both the volcanic flows and the underlying massifs provides a clear stratigraphic sequence where impact cratering represents the most recent geological process"
+}