
The surface of this vesicle has broken so that you can see through to the other side.
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Walk just around the corner from stop 1 and you'll see a really huge vesicle! While lava is still very hot and fluid, gas bubbles form and work their way toward the lava surface. If you look at an active lava flow you can watch bubbles rise to the surface, then POP! with a spray of molten droplets as gas escapes from the flow.
Often the surface of the lava flow cools and hardens first, forming a crust with still-flowing lava beneath it. In this case, gas rises but is trapped beneath the crusty roof. As more and more bubbles are trapped by the roof, they grow together to form a really big bubble like the one you see here.
Compare this mega-vesicle at Sunset Crater with the one forming
just beneath the roof of this lava tube in Hawaii. Even though the
lava has long-since hardened at Sunset Crater, you can easily see
that the processes forming these two bubbles are very similar.
Step up to take a closer look at the
roofs in these photos you'll see something that looks like stalactites
found in limestone caves. These solidifies lava drips provide another
reminder that the trail you are walking on was once a 1000°C-plus
molten lava flow.

Mega-vesicle seen from the Bonito Lava Flow trail.
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This image shows the thin, crusty roof above a lava tube. Click
here to view Pu`u`O`o, an active cinder cone. |
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