A topographic map of the surface of Venus shows the large highland areas Ishtar Terra, Aphrodite Terra and Lada Terra that have occasionally been described as "continents", plus various other smaller regions such as Beta Regio. Are these "continents" likely to have existed before the global resurfacing event, or is the topography of the planet likely to have been completely altered?
Ishtar Terra belongs to the tessera type of terrain, "one of the most tectonically deformed types of terrain on Venus", representing ~7.3 % of Venus' surface (Ivanov & Head 2011, Global geological map of Venus). Tessera are "dated" (relatively, from stratigraphic relationships) from the Fortunian, the oldest period:
The most important features of the Fortunian are large tessera-bearing crustal plateaus (e.g., Fortuna, Ovda, etc.) that form a specific class of first-order (a few thousands of kilometers across) highs on Venus [...] The lowest stratigraphic position of tessera and its relative abundance show that this unit is of extreme importance as a probable ‘window’ into the geological past of Venus.
Stratigraphy of defined and mapped geologic units on Venus. The visible geologic history of Venus consists of the Fortunian, Guineverian, and Atlian Periods. The major portion of the surface of Venus (about 70%) was resurfaced during the Guineverian Period. See text for discussion. T is the mean model absolute age of the surface
The globally observed stratigraphic relationships among the tectonic and volcanic units that make up the absolute majority (~96%) of the surface of Venus divide the observable portion of its geologic history into three different episodes, each with a specific style of resurfacing. These are as follows: (1) Global tectonic regime, when tectonic resurfacing dominated. Exposed occurrences of these units comprise about 20% of the surface of Venus. (2) Global volcanic regime, when volcanism was the most important process of resurfacing and resurfaced about 60% of Venus. (3) Network rifting-volcanism regime, when both tectonic and volcanic activities were about equally important. During this regime, about 14% of the surface of Venus was modified.
So, to summarize, "continent-like" (tessera) terrains like Ishtar Terra have existed for a long (yet unknown) time, and have survived the resurfacing from volcanism that covers most of the surface today. But they are themselves considered to represent a (tectonic) resurfacing process that has affected older (and unknown) pre-Fortunian terrains.
A global correlation chart that shows the three major regimes of resurfacing on Venus: global tectonic regime, global volcanic regime, and Network-rifting-volcanism regime.
Wiki describes the global resurfacing event as follows :-
NASA's Magellan spacecraft mission discovered that Venus has a geologically young surface with a relatively uniform age of 500±200 Ma (million years). The age of Venus was revealed by the observation of over 900 impact craters on the surface of the planet. These impact craters are nearly uniformly distributed over the surface of Venus and less than 10% have been modified by plains of volcanism or deformation. These observations indicate that a catastrophic resurfacing event took place on Venus around 500 Ma, and was followed by a dramatic decline in resurfacing rate.
In the same paragraph :-
Based on its surface features, it appears that Venus is tectonically and convectively alive but has a lithosphere that is static.
(Some emphasis on 'lithosphere is static')
The above paragraph makes it less likely that the Venusian 'Continents' could have existed before the resurfacing event, but we cannot be sure that the same rules applied before the event.
I also found this website that says that doesn't really say anything about 'continent'-like things before the resurfacing event, but it says that the event might have :
"turned off" any plate tectonics on the planet, completely solidifying the crust into a single surface.
This means that any further resurfacing events would be unlikely.
Couldn't find any papers on the same though.