Guinevere Planitia
Guinevere Planitia is an expansive lowland region of Venus that lies east of Beta Regio and west of Eistla Regio (quadrangle V-30). These low-lying plains, particularly in the western portion, are characterized by apparent volcanic source vents and broad regions of bright, dark, and mottled deposits. They are the only break in an equatorially connected zone of highlands and tectonic zones. The types, numbers, and patterns of mapped tectonic features and small volcanic landforms in the region provide important detail in the interpretation and evolution of venusian landscape. 
By using Pioneer Venus, Goldstone, and Arecibo data, these regions have been interpreted as widespread superposed flows that originated from the source vents. Fracture zones and lineament belt segments that have been identified are said to represent the Beta-Eistla deformation zones of the region. "Magellan" SAR images have revealed that most of these surface units are composed of volcanic land forms. There is also Seymour crater that is associated with extensive crater outflow deposits.
Q313
Venus
CEL
Q2900039
Beta Regio
LOC
Q54810259
quadrangle V-30
UNK
Q279148
Pioneer Venus
Concept
Q618630
Goldstone
MISC
Q102327045
Arecibo
LOC
Q842427
superposed
Concept
Q1826413
lineament belt
Concept
Q466932
"Magellan" SAR
MISC
Q1158958
Guinevere Planitia
LOC
-30^^http://www.w3.org/2001/XMLSchema#decimal
-30
NUMBER
located on astronomical body
located on astronomical body
located on astronomical body