Category: DTM Seminar

Spectrograph of 2004 Parkfield CA earthquake -- taken from http://geophysics.eas.gatech.edu/people/zpeng/EQ_Music/#part1_1

Spectrograph of 2004 Parkfield CA earthquake — taken from http://geophysics.eas.gatech.edu/people/zpeng/EQ_Music/#part1_1

Today’s DTM Seminar speaker was Prof. Zhigang Peng from GA Tech‘s Earth and Atmospheric Sciences Dept. He talked about a kind of earthquake (he called “tremors”) that is triggered when the seismic waves from another larger earthquake pass by. The relationship between earthquake duration and strength (as measured by the seismic moment) for these tremor quakes is apparently much different than for normal earthquakes, suggesting they result from different geophysical mechanisms.

The part of the talk that stuck out most for me was when Prof. Peng played the “sound” of an earthquake, generated by speeding up the seismic vibrations from measured earthquakes. This “earthquake music” is available on his website, but I have posted one such recording below. Apparently, different kinds of earthquakes make different sounds, and so these recordings can be used to tease out information about the quakes.

Sound of the 2004 Parkfield CA earthquake

“Triggered Tectonic Tremor and Interaction of Large Earthquakes”

  • July 30th, 2013
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Figure 2 from Cuk & Stewart (2012) showing the range of model outcomes for different impact conditions.

Figure 2 from Cuk & Stewart (2012) showing the range of model outcomes for different impact conditions.

In Friday’s DTM seminar, Sarah Stewart-Mukhopadhyay of Harvard gave a fascinating talk on the origin of the Moon and the effects of large impacts on the Earth’s volatile inventory.

Lots of evidence (geochemical and astronomical) say that the the Moon originated in a large impact between the proto-Earth and a roughly Mars-sized rogue planet (often called Theia). This explanation accounts for many of peculiarities of the Earth-Moon system, EXCEPT that geochemical data says that Earth and Moon probably formed out of the same material. Old models of the Moon’s formation showed that Moon should have formed mostly out of the impactor, Theia, which (like all other solar system planets) was probably compositionally distinct from the Earth. So the Moon SHOULDN’T be Earth’s compositional twin.

Instead, Stewart and Cuk suggested that the pre-impact Earth was spinning much faster than previously assumed, with a day that lasted about 2 hours, and so enough material from the proto-Earth could have been launched by the impact to make the Moon mostly out of the proto-Earth. Once the Moon formed, Stewart and Cuk suggested it could interact gravitationally with the Earth and the Sun to reduce the Earth-Moon angular momentum and bring it into line with what we see today, removing the one big objection to their fast-spinning proto-Earth idea.

In the last part of her talk, Stewart discussed what such large impacts might do to the gases trapped inside the young Earth. Contrary to popular thought, she suggested that these large impacts actually might NOT melt most of the Earth’s outermost layers, and so the Earth could retain in its interior much of the nebular gas that it was born with.

This idea could help explain geochemical data that suggest gas trapped in different parts of the Earth’s interior currently have different isotopic compositions and would mean that the Earth retains geochemical scars from its adolescence once thought completely erased by the violence of the early solar system.

“New Ideas about the Origin of the Earth and Moon”

  • July 27th, 2013
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