Images

Large cracks parallel to the shoreline are still visible on the Kamokuna delta, indicating instability. The view is to the northeast.

Lava is transported to the Kamokuna ocean entry, its plume is visible in the distance, via a lava tube. The trace of an active lava tube is often identifiable by a line of fume, as seen here for the episode 61g lava tube above the Pūlama pali.

A close-up of one of several streams of lava entering the ocean at the front of the Kamokuna lava delta on Kīlauea's south flank. The billowy white plume formed by the interaction of hot lava and seawater may look harmless, but it is a mixture of superheated steam, hydrochloric acid, and tiny shards of volcanic glass—all of which should be avoided.

Tectonic Features of World with Subduction Zones Highlighted. (modified from This Dynamic Planet)

Lava continues to enter the ocean at Kamokuna, where a lava delta about 19 acres in size has been built. The gravel emergency access road is visible on both sides of the surface flow that cut it. The view is to the southwest.

A breakout from the episode 61g vent at the head of the lava tube on November 21 sent lava streaming downslope. That breakout was still active when observed on November 29 and had traveled about 1.3 km (0.8 miles), partly surrounding Pu‘u Halulu, a tephra cone formed in 1983 at the start of the Pu‘u ‘Ō‘ō eruption.

Kīlauea's summit lava lake in Halema‘uma‘u is about 255 m (~840 ft) long (left to right in the image) and 195 m (~640 ft) wide. From this perspective, magma rises into the lake near its north edge (upper left) and circulates to the south, where it sinks all along the south margin of the lake.

This map shows recent changes to Kīlauea's East Rift Zone lava flow field. The area of the active flow field as of November 3 is shown in pink, while widening and advancement of the active flow as of November 29 is shown in red. The new flow branch east of Pu‘u ‘Ō‘ō started from a breakout at the episode 61g vent on November 21.

Graphic shows an east to west cut-away of Mount St. Helens with an interpreted model of seismic wave speeds under the volcano and earthquakes from 2008-2016. The colors of the model represent changes in seismic p-wave velocities from tomographic studies (Waite and Moran, 2009; doi:10.1016/j.jvolgeores.2009.02.009).

The largest spatter bombs traveled the farthest, perhaps aided by momentum, landing on the trail between the Halema‘uma‘u parking area and overlook. Upon landing, these bombs splatted to form complexly shaped bomb fragments connected by thick strands and masses of Pele's hair.

This VIDEO CLIP shows a cloud of ash and spatter being thrown from the summit lava lake during today's explosive event. The images were captured by an HVO webcam located on the rim of Halema‘uma‘u Crater, just above the rockfall area. Spatter falling onto the crater rim is a reminder of the hazards that exist in this area, which has been closed since 2008.

HVO scientists visited the rim of Halema‘uma‘u this afternoon (11/28) to collect samples of tephra and check for equipment damage. This view, taken on the approach to the Halema‘uma‘u, shows the tephra deposit on the crater rim. New spatter is seen as dark lumps scattered across the center of the image on top of older brown-colored Pele's hair.

This view shows the main body of the tephra deposit, which comprises the dark fragments scattered from the foreground to the web camera in the background (the HTcam thermal webcam). The rim of Halema‘uma‘u is to the right; the closed overlook is behind the photographer.

The larger spatter bombs bounced after hitting, leaving divots in the layer of Pele's hair that blankets the area, as seen here. These bombs are the diameter of large dinner plates.

VIDEO CLIP captured by HVO webcam: At 11:59 a.m., a rockfall from the south wall of Halema‘uma‘u Crater triggered a small explosive event in the summit lava lake. The explosion threw spatter (fragments of molten lava) onto the rim of the crater, mostly to the west of the former visitor overlook.

Only a relatively small amount of spatter reached the rim of Halema‘uma‘u, compared to the thick, continuous layer of spatter seen here on the intermediate ledge midway between the lava lake and the Halema‘uma‘u Crater rim.

A clear evening provided good views of the lava lake within Halema‘uma‘u Crater at the summit of Kīlauea Volcano. Spattering was active along the south margin (left side) of the lava lake, with the gas plume drifting to the southwest (upper left).

This close-up view of the lava lake surface on the south side of the lake shows a typical spreading zone. In this image, the crustal plates on both sides of the incandescent line are migrating to the south (toward the lower left corner of the photo), but the crust on the left side is moving more rapidly to the south than the crust on the right.

A slightly wider view of the lake surface, encompassing the photo at left. The lake surface is migrating to the south (lower left corner of image), towards the spatter source visible in the lava lake photo above.

HVO geologists hiked across the 61g flow field to investigate this breakout at the base of the pali on Kīlauea Volcano's south flank. Toes of active pāhoehoe lava were slowly advancing on top of older ‘A‘ā and pāhoehoe flows erupted earlier this year.

A close-up view showing the ropy texture that forms on the surface of pāhoehoe lava.