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Geologic History of the Lavinia Planitia/Lada Terra Region, Venus: Results of Mapping in the V-55, V-61, and V-56 Quadrangles

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Geologic History of the Lavinia Planitia/Lada Terra Region, Venus: Results of Mapping in the V-55, V-61, and V-56 Quadrangles Lunar and Planetary Science XXXVIII (2007) 1032.pdf GEOLOGIC HISTORY OF THE LAVINIA PLANITIA/LADA TERRA REGION, VENUS: RESULTS OF MAPPING IN THE V-55, V-61, AND V-56 QUADRANGLES. M. A. Ivanov1,2 and J. W. Head2, 1Vernadsky Institute, RAS, Moscow 119991, Russia, [email protected]; 2Brown University, Providence, RI 02912, USA. Introduction: Lada Terra (V-61 and V-56 quadran- (thousands of km long, hundreds of km wide, a couple of gles) is a region of midlands (0-2 km above mean plane- km in amplitude), an elongated depression, and a topog- tary radius, MPR) at high southern latitudes (~300-90oE, raphic ridge, concentrically outline the swell of Lada 55-80oS). It is dominated by a large dome-shaped struc- from the north and east. ture, a swell, and hosts numerous coronae (e.g. Quet- Regional geology: Units, structures, and their zalpetlatl and Boala [1,2]), and large complexes of lava stratigraphic relationships. In our mapping, we used flows, fluctuses (e.g. Mylitta and Cavillaca [3,4]). Belts traditional methods of unit definition [12,13] appropri- of fractures and graben interconnect many coronae in ately modified for radar data [14]. On the basis of these Lada Terra [5]. The vast lowland of Lavinia Planitia approaches [14-18], we defined units and mapped rela- (~330-0oE, 25-55oS, V-55 quadrangle) is adjacent to tions between them and tectonic structures using F/C1- Lada Terra from the north. Deformational belts of ridges MIDR’s, images and altimetry data. All three mapped and grooves and vast moderately deformed plains char- quadrangles display similar sets of material and tectonic acterize the floor of Lavinia Planitia [6,7]. The pattern of units. Consistent age relationships among them allow deformation, topography, and gravity signature are con- stratigraphic correlations of the units in the broad sistent with mantle downwelling under Lavinia Planitia mapped region. The oldest unit is Tessera. It has a [8] and with mantle upwelling in the region of Lada unique pattern of deformation consisting of intersecting Terra [9,10]. Thus, Lada Terra and Lavinia Planitia ap- ridges and grooves [19-22, 7] and is consistently em- parently represent contrasting geodynamic provinces. bayed by less deformed materials. The major occur- Their close proximity suggests a genetically related his- rences of tessera in the area of our mapping are Alpha tory [4]. We studied these regions in detail through geo- Tessera (to the east of Lavinia Planitia, V-55) and Co- logical mapping at 1:5 M scale under the USGS plane- comama Tessera (to the east of the Lada swell, V-56). tary mapping program (combined area of the quadran- Densely lineated plains (pdl) form the oldest plains unit. gles V-55 [11], V-61, map in edit, and V-56, map in pro- Its surface is cut by densely packed lineaments (some of gress). The main goal of our study was to reconstruct the them are fractures). Material of densely lineated plains major episodes of geologic history of Lada and Lavinia embays tessera where these units are in contact. Ridged and establish the timing and sequence of events during plains (pr) are commonly deformed by broad (5-10 km formation and evolution of these regions. wide) ridges tens of kilometers long. The ridges are ar- Topographic configuration of Lavinia Planitia and ranged in linear belts and predominantly occur on the Lada Terra. Lavinia Planitia is a large lowland basin a floor of Lavinia Planitia (V-55). Both emplacement and few thousand km across, and is as deep as ~1.5 km be- deformation of ridged plains postdate deformation of the low MPR. The general distribution of topography in unit pdl. Abundant small (a few km) shield-like features Lavinia Planitia is asymmetric with the deepest portion characterize Shield plains (psh). The unit occurs prefer- of the basin toward its southern edge. Toward the north entially within Lavinia Planitia where it embays ridged and northwest, the elevation changes ~1 km over a dis- plains. Psh is significantly less widespread within the tance of ~1800 km while at the southern and eastern elevated portion of Lada Terra (V-61) but is abundant margins the same change in elevation occurs over a dis- around Cocomama Tessera (V-56). Regional plains (rp) tance of ~500 km. Deformational belts on the floor of the form the most widespread unit with a morphologically basin form a radial pattern and topographically represent smooth and homogeneous surface, which is typically cut elevated zones several hundred meters high. The most by wrinkle ridges. Sources of the plains are not obvious. prominent belts are concentrated in the deepest area of There are two units of regional plains. The lower unit Lavinia Planitia. (rp1) has relatively low radar backscatter and usually The major portion of Lada Terra is within the 0-2 km makes up the floor of the lowlands surrounding Lada interval (midlands). The largest topographic feature of Terra. Sometimes it occurs in stratigraphic windows on Lada Terra is a broad (~1000 km across) symmetric the slopes of the Lada swell. The upper unit (rp2) has a swell, the summit of which reaches an elevation of ~3.5 higher radar albedo and, sometimes, lobate boundaries. km. The overall topographic shape of the Lada swell Both units of regional plains embay shields plains. Lo- resembles that of other dome-shaped rises on Venus bate and digitate boundaries (Lobate plains, pl) morpho- (e.g., Beta, Eistla Regiones). In contrast to these areas, logically smooth surfaces (Smooth plains, ps), and clus- which are topped by large volcanoes, the Lada swell ters of small shields (Shield clusters, sc) similar to those hosts nested Quetzalpetlatl and Boala Coronae and lacks of shield plains characterize units that are younger than large volcanoes. Two regional-scale topographic features Lunar and Planetary Science XXXVIII (2007) 1032.pdf regional plains. These units preferentially occur on (lobate plains) and young extensional deformation (rift slopes of the Lada swell (V-61 and 56). zones). The summit area of the swell (Quetzalpetlatl and There are two types, scales, and ages of contractional Boala Coronae) and the Tarbell/Jord Coronae complex features in the map area. The older are ridges and arches within the rift of Kalaipahoa Linea are the most impor- that deform ridged plains (unit pr). Regional plains em- tant sources of young volcanism. Young lava flows flow bay these structures. The northern rim of Quetzalpetlatl down the regional slopes of the swell and the steeper Corona is morphologically similar to a typical ridge southern and eastern edges of the Lavinia basin [11,23]. belt, and is related to the evolution of the corona. Re- Magellan gravity data [24,25] show that the Lada swell gional plains embay the rim at its southern end. Thus, is characterized by high values of both vertical gravity formation of the rim predates emplacement of regional acceleration (up to 120 mGal) and geoid height (up to plains. The younger contractional features are wrinkle 40 m). These features together strongly suggest that the ridges that form a regional network that deform regional central portion of Lada Terra represents a region of plains and other older units and are embayed by smooth mantle upwelling. The stratigraphic position of the most and lobate plains. abundant units in Lada Terra means that much of the Numerous fractures and graben in the region studied volcanism associated with the upwelling largely post- are typically collected in zones of extensional structures dated the subsidence in Lavinia Planitia. (groove belts and rift zones). Groove belts preferentially Thus, the geologic history of the region of Lavinia occur on the floor of Lavinia Planitia (V-55) where they Planitia and Lada Terra appears to consist of two major cut ridges of the unit pr and are embayed by shield plains phases. The earlier phase corresponds to formation of and regional plains. Rift zones are concentrated in Lada the vast basin in Lavinia. During the phase of broad Terra and appear to be contemporaneous with the updoming, massive volcanism and extensional tectonics youngest plains units (pl, ps, and sc). The largest of them occurred in Lada Terra largely postdating the formation is a rift-like zone of Kalaipahoa Linea (V-61) that out- of Lavinia. The close geographic position of the low- lines the Lada swell from the north. Another rift-like lying Lavinia Planitia and elevated Lada Terra, their zone is within the V-56 quadrangle. It consists of a chain overall topographic configuration, and general sequence of coronae interconnected by graben and outlines the of events in these regions are consistent with and sug- swell from the east. Within both zones there are promi- gest a genetically linked evolution of these provinces nent sources (coronae) from which emanate the youngest [4]. In this model, the downwelling in Lavinia occurred volcanic flows (e.g. Mylitta Fluctus). together with upwelling under Lada, initiating the Discussion and conclusions The V-55, V-61, and V- younger geologic activity within Lada Terra. 56 quadrangles cover a region that consists of two prov- inces, Lavinia Planitia and Lada Terra, contrasting in References: 1) Stofan, E. R. et al., JGR, 97, 13347, 1992, topography, gravity, and overall geologic history. De- 2) Crumpler, L. S. and J. Aubele, Volcanism on Venus, in: formational zones of ridge and groove belts that form the Encycl. of Volcanoes, 727, 2000, 3) Roberts, K.M., et al., JGR, bottom of the general stratigraphic column populate the 97, 15991, 1992, 4) Magee, K. P. and J. W. Head, JGR, 100, 1527, 1995, 5) Baer, G. et al., JGR, 99, 8355, 1994, 6) floor of Lavinia Planitia.
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