Publication Year 2016
Acceptance in OA@INAF 2021-02-26T16:24:19Z
Title Geology of the Victoria quadrangle (H02), Mercury
Authors GALLUZZI, VALENTINA; GUZZETTA, Laura Giovanna; Ferranti, Luigi; DI ACHILLE, Gaetano; Rothery, David Alan; et al.
DOI 10.1080/17445647.2016.1193777
Handle http://hdl.handle.net/20.500.12386/30653
Journal JOURNAL OF MAPS
Number 12 H01 - Borealis Geologic Map of the Victoria Quadrangle (H02), Mercury 60° Geologic Units Borea 65° Smooth plains material 1 1 2 3 4 1,5 sp H05 - Hokusai H04 - Raditladi H03 - Shakespeare H02 - Victoria Smooth and sparsely cratered planar surfaces confined to pools found within crater materials. Galluzzi V. , Guzzetta L. , Ferranti L. , Di Achille G. , Rothery D. A. , Palumbo P. 30° Apollonia Liguria Caduceata Aurora Smooth plains material–northern spn Smooth and sparsely cratered planar surfaces confined to the high-northern latitudes. 1 INAF, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy; 22.5° Intermediate plains material 2 H10 - Derain H09 - Eminescu H08 - Tolstoj H07 - Beethoven H06 - Kuiper imp DiSTAR, Università degli Studi di Napoli "Federico II", Naples, Italy; 0° Pieria Solitudo Criophori Phoethontas Solitudo Lycaonis Tricrena Smooth undulating to planar surfaces, more densely cratered than the smooth plains. 3 INAF, Osservatorio Astronomico di Teramo, Teramo, Italy; -22.5° Intercrater plains material 4 72° 144° 216° 288° icp 2 Department of Physical Sciences, The Open University, Milton Keynes, UK; ° Rough or gently rolling, densely cratered surfaces, encompassing also distal crater materials. 70 60 H14 - Debussy H13 - Neruda H12 - Michelangelo H11 - Discovery ° 5 3 270° 300° 330° 0° 30° spn Dipartimento di Scienze e Tecnologie, Università degli Studi di Napoli "Parthenope", Naples, Italy. Cyllene Solitudo Persephones Solitudo Promethei Solitudo Hermae -30° Trismegisti -65° 90° 270° Crater Materials icp H15 - Bach Australia Crater material–well preserved cfs -60° c3 180° Fresh craters with a sharp rim, textured ejecta blanket and pristine or sparsely cratered floor. 2 1:3,000,000 ° c2 80° 350 Crater material–degraded c2 spn M c3 Degraded craters with a subdued rim and a moderately cratered smooth to hummocky floor. on spn te ve Crater material–heavily degraded c3 rd c1 i c3 Correlation of Map Units Heavily degraded craters with a subdued or discontinuous rim and a hummocky, densely cratered floor. 290° 340° cfs Crater floor material–smooth c3 cfs 60° Crater Materials Geologic Units Very smooth, planar and sparsely cratered crater floor surfaces. c1 spn c1 60° c1 300 30° spn c1 ° 3 c3 c3 present Crater floor material–hummocky c3 cfh cfh cfs Rough or gently rolling, moderately cratered crater floor surfaces. c3 cfs 310° 320° c1 c2 in c3 ed cfs + b cfh c1 A c3 c2 Kuiperian cfh icp c3 + cfs Surface Features cfs c3 cfs cfs c3 cfh cfs R c1 c3 u c2 c3 be icp cfs Hollow cluster n c3 c3 cfh c1 1 Ga c3 s cfs cfh cfs cfs cfs + c2 cfh c2 c2 + + c2 c3 Secondary crater chain/cluster c2 + cfh c2 c2 c3 + c3 c2 + c1 cfs cfh cfs cfs cfh c2 cfs c1 cfh c3 Geologic Contacts cfs c1 2 Ga c2 cfh c1 + cfh + c3 Mansurian cfs c3
c1 + cfs c3 cfh
+ + cfs
Contact, certain c2 cfs +
c2 + C
+
+ c2 c2 + ar c2 c1 n c2 c3 cfs cfh cfs eg c3 + i cfs Contact, approximate c3 cfs e cfs cfs R cfs c3
cfh + u + + + c2 p cfs c3 cfs e + c3 s nanska 3 Ga c2 Boz cfh c3
c3 c1 + ira cfs c3 j +
cfh mat c3 c3
Linear Features c2 cfs cfs c1 c3 Na c3 + cfh c2 cfh c2 c3
cfs c3 cfh c3 + Duc
Crest of crater rim (diam. > 20 km) cfs cio c2 cfh +
cfs + Calorian S c3 sp sp h c2 c3 c2 spn 50° A o c2 cfs + le le c1 imp i m cfs cfs 50° 4 Ga Tolstojan
Crest of small crater rim (diam. > 5 km) c c1 icp h imp c1 + spn
em imp cfh + c2 cfs c2 c2 c3 cfs Pre-Tolstojan sp imp c2 cfs cfs c2 Crest of subdued or buried crater c2 c2 cfh c2
S + + tra c3 c2 cfs cfs c2 cfs
vi c2 c3 c2 c3 Irregular pit n c1 + imp sk cfs c3 icp
y cfh c2
sp + V cfs c2 +
c3 + c3 c1 Grieg c1 cfs cfh i cfs c1 + c c2 cfs t cfs cfh c1 imp cfh o
c2 c3 r + c3 + cfs Thrust–certain (lobate scarp, high relief ridge) c1 i c3 c3 c3 a
cfs cfs + c3 + cfh V c2 cfs R c2
y cfh + u as c2 cfs c3 cfs p cfh c2 cfs Thrust–uncertain (lobate scarp, high relief ridge) a cfh c2 es icp cfs c2 cfs c2 + c3 cfs c3 c2 cfs + cfh cfh c1 cfs imp c3 cfs c3 c3 c2 cfs c2 c3 c3 cfh cfh c3 c3 c2 Contractional fault–certain c2 c3 cfs cfs + c3 + c3 c3 cfh c1 c1 cfs c3 cfs c3 c3 c3 c2 cfs cfh c3 c1 c3 cfs c3 Contractional fault–uncertain c1 c2 c3 cfs cfh cfs c3 + c1 cfh c3 imp cfs na cfs c3 cfs cfs c3 cfs icp ua c2 cfs r J c3 c3 c3 So Wrinkle ridge c3 cfs c2 c3 imp c3 cfs c2 cfs + cfh cfs c2 cfs c2 cfs cfs c2 cfs
c2 cfs kas + cfs Baranaus cfh
c2 cfs c2 + cfs c3 c2 c2 c3 c3 c2 cfh c2 cfs cfs c3 c3 c2 c2 c2 + cfs
40° c1 cfs c2 c2 + c2 cfs c2 cfs + c3 cfh Monet 40° c2 + cfh cfs cfs cfs c3 cfh c1 cfh c3 c3 c2 n+ a c3 + c3 eduan + Enh c1 cfs cfh c3 c3 cfs cfs c2 +
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+ + a spn + c3 ar c3 cfs + cfh L cfs eg arr c1 c2 cfh ch cfs
+ c3 oc cfs c2 c3 E c2 cfs h c1 cfs + imp a c1 cfs + + icp c2 + + + c2 c3 c2 cfh cfs + c3 + c3 cfs c3 + c3 c2 c3 c3 c1 + cfs c2 c3 icp cfs c1 + c2 c2 cfh c1 + c2
icp c1 c3 cfs c3 cfs + cfs
cfs + c2 cfh cfh c1 c2 c3 cfs c2 c3 cfs c2 cfs c3 c1 cfs cfs cfh cfh cfs c2 c3
cfh + c3 + c2 cfh cfs+ c2
c2 cfs c2 c2 + cfh cfh c3 c3 cfh + c3 c2 c2
cfs c2 cfs c3 icp c1 c3 c2 + c2 cfs c3 c3 cfh cfs
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icp cfs + cfh
c1 + c2 c3 c1 + +
cfs c2 cfs cfs cfs c2 cfs +
cfh
+ + imp imp + c2 c2 c2 c2 c3 cfh c3 + cfs c3 cfh +
c2 c2 c3 + c2 + cfs
cfh cfs c1 + c2 + c3 c2 cfs cfh cfh
cfh + cfh c3 c3 c2 cfh +
+ c3 c2 cfs + + + cfs cfh c1 c2 cfs c3 c2 c2
cfs cfs cfs cfs c2 c2 + 30° cfs cfh c2 c3 cfs + c2 c3 c2 Gluckcfs cfh cfs c2 c1 30° + c2 c3 + cfs c3 cfh c2 A cfs cfh c3 c2 c2 c3 +
c2 ks cfh c3 c2 cfs
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v cfs n c2 + + R cfh cfs c2 c2 cfs d c2 c3
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cfh c3 c3 cfh Jobim cfh c3 + c2 cfs cfs cfs c3 c3 cfs c2 cfs c1 c2 cfs + + cfs
+ cfh c2 + cfs c2 cfh c2 c3 c3 icp c2 c3 + c3
c2 c2 c2 + c3 c3 cfs c2 + + cfs cfs c2 + ck c3 cfs c1 c2 c3 n c3
c2 cfs c2 c2 + cfh + i
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cfs cfs cfh la c2 + imp 27 cfh c3 cfs + + V cfs °
0 c2 c3 + c2 + c3 60 ° c2 c2 cfs cfs c3 + + 3 cfs c3 c2 + + cfh cfh c2 cfs cfs c2 c2 cfh imp + c3
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cfh + cfs
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cfs cfs +
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c1 cfh cfs c3 cfh c3 cfh c1 c2 c3 cfs + cfs + c3 cfs c2 +
icp c1 +
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c1 + c1 risc
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+ c3 + + c3
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c1 cfs c3 c3 n
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c2 'ing cfs s a c2 + cfh c2 u d +
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8 + 50 0 + cfs + 3 ° cfh c1 c2 c2 c3 cfs c3 c2 c2 cfs cfh cfs c1 c3 cfs cfs c1 cfs cfs cfs +
c2 Praxi c3 c2 Geddes + c2 tele c2
s cfs c2 c3 + c2 + c3 c2 c2 c3
cfs + c1 + c3 cfs c3 c2 c3 c3 cfs cfs cfh
cfs cfh cfs c2
cfs + + c2 + c3 c1 c2 cfs cfs +
c3 c2 c2 + c3 c1 c3 cfs cfs c3 i c3 cfs -Ch c1 c3 en c2 c2 c1 i W cfs cfs s'a +
cfs imp cfs T ° 2 + 90° c1 340 cfh c3 cfh c3 c1 c3 + cfh c2 Wren c1 c1 c2 icp
cfh + c1 cfs c2 c1 c2 cfs icp cfh + c3 c3 c2 cfs cfs c2 + c1 cfh c1 c3 cfh Coordinate System c2 c3 cfs cfh c2 cfh cfs 300° c2 + cfs 330° Feature Nomenclature cfh c3 + cfs cfs Projection: Lambert conformal conic c3 c2 c3 c3 c1 c2 c1 cfs cfs Central meridian: 315°E
Duccio Craters + Aurora Albedo features 310° 320° Standard parallel 1: 30°N Standard parallel 2: 58°N Victoria Rupes Lobate scarps (rupes) and high-relief ridges (dorsa) 65°N Sphere radius: 2440 km From the Gazetteer of Planetary Nomenclature of the International Astronomical Union (IAU) 60°N
Basemaps 50°N 40°N Top-right Mercury globe: mdis_v3_color_1000_750_430_665mpp 30°N Central main map: mdis_v8_750nm_250mpp 22.5°N Basemaps credits: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington -500 km -400 km -300 km -200 km -100 km 0 100 km 200 km 300 km 400 km 500 km
© Journal of Maps, 2016