The landscapes in the Bohemian Massif are mostly dominated by rolling hills. North of the river Danube the topography is characterized by gentle valleys and broad, flat ridges and hilltops. The highest peaks on the Czech-Austrian borderline are the Plöckenstein (Plechý, 1,378 m) and Sternstein (1,125 m). The bedrock of acid gneiss and granite is weathered to brown soil (cambisols). In flat areas and valleys the groundwater had more influence on soil formation; in such places gley soils may be found too.
The internal tectonic structure of the Bohemian Massif was formed during the Variscan Orogeny. The Variscan Orogeny was a phase of mountain building and accretion of terranes that resulted from the closing of the Rheic Ocean when the two paleocontinents Gondwana (in the south) and Laurussia (in the north) collided. Most of the Bohemian Massif is often supposed to belong to a terrane called Cadomia or Armorica, which also included the terranes of the Armorican Massif in western France. This supposedly formed a microcontinent that became sandwiched between the large continental masses north and south. The result of the Variscan Orogeny was that almost all continental mass became united in a supercontinent called Pangaea. From the Permian period onward the Variscan mountain belt eroded and became partly covered by younger sediments, with the exception of Variscan massifs like the Bohemian Massif.
The basement rocks and terranes of the Bohemian Massif are tectonically part of three main structural zones, which differ in metamorphic degrees, lithologies and tectonic styles. This tectonic subdivision was formed during the Variscan Orogeny.
The Moldanubian Zone forms the central parts of the massif and has generally a higher grade than the Saxothuringian Zone. It includes the Teplá-Barrandian Terrane, which is assumed to have been a small microcontinent.
The southeast of the massif forms a third unit, the Moravo-Silesian Zone. This zone includes the Brunovistulian Block, an allochthonous unit thrusted over the Moravo-Silesian crystalline rocks. Contradictionary to most parts of the Bohemian Massif, the Brunovistulian was originally part of or close to the southern part of Laurussia.
Unlike other Variscan massifs in Central Europe the Bohemian Massif is not very rich in ores. The Harz Mountains further north in Germany, which are geologically part of the Rhenohercynian Zone, have more ore deposits. On the other hand, the Bohemian massif has many quarries where granite, granodiorite and diorite are won for use as decorative building stone.
^Finger et al. (2000) linked the Brunovistulian terrane with "Avalonia" (i.e. the southern part of Laurussia)
Finger, F.; Hanžl, P., Pin, C.; von Quadt, A. & Steyrer, H.P.; 2000: The Brunovistulian: Avalonian Precambrian sequence at the eastern Bohemian Massif: speculations on palinsplastic reconstruction, in: Franke, W.; Haak, V.; Oncken, O. & Tanner, D. (eds.): Orogenic Processes: Quantification and Modelling in the Variscan Belt, Geological Society of London Special Publication 179, pp 103-113.
Kossmat, F.; 1927: Gliederung des varistischen Gebirgsbaues, Abhandlungen des Sächsischen Geologischen Landesamtes 1, pp. 1–39.
Linnemann, U.; Romer, R.L.; Pin, C.; Aleksandrowski, P.; Buła, Z.; Geisler, T.; Kachlik, V.; Krzemińska, E.; Mazur, S.;Motuza, G.; Murphy, J.B.; Nance, R.D.; Pisarevsky, S.A.; Schulz, B.; Ulrich, J.; Wiszniewska, J.; Żaba, J. & Zeh, A.; 2008a: Chapter 2: Precambrian, in: McCann, T. (ed.): The Geology of Central Europe, The Geological Society, ISBN1-86239-246-3.
Linnemann, U.; D'Lemos, R.; Dorst, K.; Jeffries, T.; Gerdes, A.; Romer, R.L.; Samson, S.D. & Strachan, R.A.; 2008b: Chapter 3: Cadomian tectonics, in: McCann, T. (ed.): The Geology of Central Europe, The Geological Society, ISBN1-86239-246-3.
Linnemann, U.; Gerdes, A.; Drost, K. & Buschmann, B.; 2007: The Continuum between Cadomian orogenesis and opening of the Rheic Ocean: Constraints from LA-ICP-MS U-Pb Zircon dating and analysis of plate tectonic setting (Saxo-Thuringian Zone, northeastern Bohemian Massif, Germany, in: Linnemann, U.; Nance, R.D.; Kraft, P. & Zulauf, G. (eds.): The evolution of the Rheic Ocean, from Avalonian-Cadomian Active Margin to Alleghenian-Variscan Collision, Geological Society of America Special Paper 423, pp 61–96.