Tadpole and Lava Tube

An irregularly shaped depression may be a volcanic vent
An irregularly shaped depression, resembling a tadpole (center left), which is part of a sinuous chain of pits. The black arrow indicates the beginning of the pit chain that trends to the southeast. This feature is about 8 km long and 600 m deep, and is located in the mare northwest of Gruithuisen crater. Color shaded-relief depicts elevation from NAC DTM PITVENT; higher elevations are red and white, lower elevations are blue and purple; north is up [NASA/GSFC/Arizona State University].

Today's feature is an irregularly shaped, steep-walled mare depression that looks a bit like a tadpole; it is about 8 km long and located at the northwest end of a 60-km long, sinuous chain of pits northwest of Gruithuisen crater (315.901°E, 35.284°N). The pit chain was one of the first and most spectacular candidates proposed for an intact lunar lava tube (i.e., one with uncollapsed segments). This depression may be the source vent for the lava flows that host the pit chain (see image below).

Volcanic vents tend to be sub-circular or elongate, like today's feature, which is roughly 600 m deep and has steep inner walls (~35° slopes). Similarly sized and shaped features include examples near Sulpicius Gallus crater and the Orientale basin. Dark, low-albedo, materials surrounding the Sulpicius Gallus and Orientale features suggest formation through explosive pyroclastic eruptions; however, further exploration is still needed to confirm this interpretation.

Tadpole vent and pit chain are likely parts of a lava tube
WAC context image of the maria northwest of Gruithuisen crater. The irregularly shaped depression heads the northwest end of a sinuous chain of pits (white arrows) and may be the source region for some of the lava flows to the southeast [NASA/GSFC/Arizona State University].

Collapse pits, with sharp and nearly vertical walls, like the one in the Marius Hills (shown in a previous post) suggest fairly recent collapse of ancient lava tubes. The chain of pits near Gruithuisen, however, has more subdued topography, and likely formed earlier in the history of the Moon (perhaps more than 1 or 2 billion years ago).

Intact lava tubes have long been thought to be important to future exploration. Many have speculated that uncollapsed portions of lava tubes could be used to shield explorers from harmful radiation, as well as provide a relatively warm and stable environment that is buffered from the large temperature variations at the surface. Many hope that uncollapsed lava tubes will be located near volcanic materials that can be used in construction or energy-generation processes. However, we still have not explored inside any lava tubes on another planet, though many engineers and scientists are currently working to enable such activities. In the meantime, LROC images combined with other data sets, can be used to search for additional lava tube candidates.

Explore today's tadpole-shaped vent in more detail (LROC NAC M1103837710):

Continue Reading about this facsinating lava tube candidate and the sinuous pit chain, or explore the Sulpicius Gallus vent and Orientale Basin vent in more detail!

Even more to explore:

Collapsing Tube

Pyroclastic Excavation

Pyroclastic Trails 

Mare Pit Topography!

Published by J. Stopar on 29 August 2014