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YSM Issue 96.3

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FOCUS<br />

Astronomy<br />

findings to the relatively well-known<br />

composition of Earth, it is plausible to<br />

conclude that Earth, unlike Venus, did<br />

not experience late accretion events that<br />

affected its core temperature to such a<br />

great extent.<br />

While Earth’s large volume of<br />

surface water broke down the crust<br />

and uppermost mantle of the planet to<br />

form tectonic plates, Venus is closer to<br />

the Sun than the Earth, causing Venus<br />

to rapidly lose surface water through<br />

evaporation. This geophysical difference<br />

is significant, as plate tectonics reduce<br />

internal heat. In addition, the researchers<br />

ran a simulation and found that the mean<br />

impact velocities of late accretions on<br />

Venus were larger than those of Earth.<br />

In other words, small celestial bodies<br />

called planetesimals hit Venus harder<br />

and faster. The lower-velocity impacts<br />

on Earth would lead to less core heating<br />

and an inability to sustain the long-lived<br />

volcanic activity seen on Venus. These<br />

key differences are what lends the ‘planet<br />

of beauty’ its distinct, youthful surface.<br />

Future Directions<br />

Marchi and Korenaga hope to use their<br />

model to make predictions and further<br />

explain the mystery of Venus. “This<br />

difference in late accretion by itself may<br />

not explain all the differences [between<br />

Earth and Venus], but it may help to<br />

push it towards the right direction,”<br />

Korenaga said. The collaboration with<br />

Korenaga, who has studied the origin<br />

of life on terrestrial planets for over a<br />

decade, highlights a key link between<br />

late accretion and the early history of<br />

planets. As it did for Venus, late accretion<br />

played a significant role in Earth's early<br />

history and has a lasting impact on its<br />

present surface features, contributing<br />

substantially to the geological record<br />

of the planet. Thus, understanding<br />

late accretions has other far-reaching<br />

implications for related projects.<br />

According to Marchi, these energetic<br />

events could drastically alter the<br />

chemistry of the atmosphere. For<br />

example, large-scale impacts can lead<br />

to the heating of the crust, generating<br />

a hydrothermal system that could serve<br />

as a possible reservoir for microbes to<br />

ABOUT THE<br />

AUTHORS<br />

PHOTOGRAPHY BY MIRANDA SELIN<br />

The members of Jun Korenaga’s lab: from left to right, (top row) Brianna Fernandez, Darius Modirrousta-<br />

Galian, Amy Ferrick, Jun Korrenaga; (bottom row) Steph Larson, Meng Guo, Coral Chen<br />

thrive. “We strive to understand whether<br />

or not these early impacts could have<br />

had anything to do with the origin of life<br />

on Earth,” Marchi said.<br />

Much of Korenaga’s work in the<br />

past has focused on early Earth and<br />

investigating the geophysical catalysts<br />

for life. “The role of late accretion is<br />

important to discuss generally, for<br />

how you can build a habitable planet,”<br />

Korenaga said. He argues that late-stage<br />

cosmic collisions have a large impact on<br />

whether or not a planet can produce life.<br />

In particular, this research helps us better<br />

understand the geological makeup and<br />

formation of planets, a key ingredient for<br />

a given planet's potential to sustain life.<br />

As a planetary scientist, Marchi is<br />

also involved in space missions and is<br />

currently one of the leaders of the Lucy<br />

Mission, a NASA space probe with<br />

the goal of reaching Trojan asteroids<br />

near Jupiter. Recently, there has been<br />

a revival of interest in Venus in space<br />

exploration. NASA selected two future<br />

space missions to explore Venus in the<br />

coming decade, and the European Space<br />

Union has proposed its own mission.<br />

For next steps, the authors hope to<br />

build off of this work and potentially<br />

explore the geophysics of Earth and<br />

Mars, which could hold more mysteries<br />

of their own. “The work for Venus is<br />

definitely not done,” Marchi said. “But<br />

we'll try to push the new idea forward<br />

to make predictions and try to test that<br />

as much as possible—with new missions<br />

as well.” ■<br />

CINDY MEI<br />

DAVID GAETANO<br />

CINDY MEI is a junior in Grace Hopper studying neuroscience. In addition to writing for <strong>YSM</strong>, she serves<br />

as vice president on the Junior Class Council and Yale Math Competitions. She also conducts epilepsy<br />

and Tourette’s syndrome research at the Yale School of Medicine..<br />

DAVID GAETANO is a sophomore in Ezra Stiles studying Mechanical Engineering. In addition to writing<br />

for <strong>YSM</strong>, he is involved in the Yale Undergraduate Aerospace Association.<br />

THE AUTHORS WOULD LIKE TO THANK Simone Marchi and Jun Korenaga for their time and<br />

enthusiasm about their research.<br />

FURTHER READING:<br />

Marchi, S., Walker, R.J., & Canup, R.M. (2020). A compositionally heterogeneous martian mantle due to<br />

late accretion. Science Advances, 6 (7), doi: 10.1126/sciadv.aay2338<br />

24 Yale Scientific Magazine September 2023 www.yalescientific.org

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