Venus, although similar to Earth in size and mass, differs markedly in that it does not have plate tectonics. The boundaries of Earth’s moving surface plates are the primary locations of volcanic activity.

New research by University of Alaska Fairbanks Geophysical Institute research professor Robert Herrick revealed a nearly 1-square-mile volcanic vent that changed in shape and grew over eight months in 1991. Changes on such a scale on Earth are associated with volcanic activity, whether through an eruption at the vent or movement of magma beneath the vent that causes the vent walls to collapse and the vent to expand.

The research was published today in the journal Science.

Herrick studied images taken in the early 1990s during the first two imaging cycles of NASA’s Magellan space probe. Until recently, comparing digital images to find new lava flows took too much time, the paper notes. As a result, few scientists have searched Magellan data for feature formation.

“It is really only in the last decade or so that the Magellan data has been available at full resolution, mosaicked and easily manipulable by an investigator with a typical personal workstation,” Herrick said.

The new research focused on an area containing two of Venus’ largest volcanoes, Ozza and Maat Mons.

“Ozza and Maat Mons are comparable in volume to Earth’s largest volcanoes but have lower slopes and thus are more spread out,” Herrick said.

Maat Mons contains the expanded vent that indicates volcanic activity.

Herrick compared a Magellan image from mid-February 1991 with a mid-October 1991 image and noticed a change to a vent on the north side of a domed shield volcano that is part of the Maat Mons volcano.

The vent had grown from a circular formation of just under 1 square mile to an irregular shape of about 1.5 square miles.

The later image indicates that the vent’s walls became shorter, perhaps only a few hundred feet high, and that the vent was nearly filled to its rim. The researchers speculate that a lava lake formed in the vent during the eight months between the images, though whether the contents were liquid or cooled and solidified isn’t known.

The researchers offer one caveat: a nonvolcanic, earthquake-triggered collapse of the vent’s walls might have caused the expansion. They note, however, that vent collapses of this scale on Earth’s volcanoes have always been accompanied by nearby volcanic eruptions; magma withdraws from beneath the vent because it is going somewhere else.

The surface of Venus is geologically young, especially compared to all the other rocky bodies except Earth and Jupiter’s moon Io, Herrick said.

“However, the estimates of how often eruptions might occur on Venus have been speculative, ranging from several large eruptions per year to one such eruption every several or even tens of years,” he said.

Herrick contrasts the lack of information about Venusian volcanism with what is known about Jupiter’s moon Io and about Mars.

“Io is so active that multiple ongoing eruptions have been imaged every time we’ve observed it,” he said.

On a geological time scale, relatively young lava flows indicate Mars remains volcanically active, Herrick said.

“However, nothing has occurred in the 45 years that we have been observing Mars, and most scientists would say that you’d probably need to watch the surface for a few million years to have a reasonable chance of seeing a new lava flow,” he said.

Herrick’s research adds Venus to the small pool of volcanically active bodies in our solar system.

“We can now say that Venus is presently volcanically active in the sense that there are at least a few eruptions per year,” he said. “We can expect that the upcoming Venus missions will observe new volcanic flows that have occurred since the Magellan mission ended three decades ago, and we should see some activity occurring while the two upcoming orbital missions are collecting images.”

Co-author Scott Hensley of NASA’s Jet Propulsion Laboratory performed the modeling for the research.

Landslides are projected to be a growing concern as climate change produces more extreme rainfall events that can destabilize slopes and trigger these events. Research presented in the session will include investigations of landslide hazards in Puerto Rico, Vermont, Pennsylvania, Michigan, Tennessee, West Virginia, and southern and central Appalachia.

Puerto Rico

After Hurricane Maria in 2017, researchers documented more than 70,000 landslides on the island of Puerto Rico. Geologist Stephen Hughes at the University of Puerto Rico Mayagüez saw a gap in the monitoring and forecasting of landslides on the island, and to fill that gap he started a research and outreach program: Storm-induced Landslide Impact Dynamics on Environment and Society in Puerto Rico (SLIDES-PR). Through partnership with the U.S. Geological Survey, SLIDES-PR has developed a landslide susceptibility map for the island and installed 14 real-time monitoring stations on landslide-prone slopes.

“These are shallow, relatively small landslides, but extremely widespread. It doesn’t matter that it’s a small landslide if it comes through your house,” says Hughes.

The monitoring stations measure soil moisture, pore pressure, and groundwater level, collecting data every five minutes and sending it back to the university every hour. The monitoring network has already saved lives. During Hurricane Fiona in 2022, Hughes was able to use real-time monitoring to warn the town of Naguabo that the soil moisture had crossed the threshold for imminent slope failure, prompting evacuation before a debris flow buried a home.

In addition to monitoring and forecasting, the SLIDES-PR program has developed guides for residents to understand the warning signs for landslides, what human activities can promote them, and ways to prepare and cope after they happen. At the conference, Anishka Ruiz-Perea will share the science and risk communication work done by SLIDES-PR , and Kiara Cunillera-Cote will present on the development of forecasting thresholds using the data from monitoring stations.

Vermont

In 2019, a hillside in Vermont’s Mt. Mansfield State Forest failed and generated a 12.5-acre landslide with a volume equivalent to 80 Olympic-sized swimming pools. The material formed a dam in Cotton Brook, which eventually carried the influx of sediment to the nearby Waterbury Reservoir.

Smuggler’s Notch, one of the most popular tourist destinations in the state, is a 1,000-foot high mountain gap that has seen major rock slides over several decades, sometimes dropping boulders the size of school buses onto the road below.

“We are convinced, just like many others, that as climate change gets more extreme, we will generate more landslides and more sediment systems,” explains Jonathan Kim of the Vermont Geological Survey, who will present on the many approaches taken to assess, monitor and mitigate landslide hazards in Vermont.

The Vermont Geological Survey has been collaborating with the University of Vermont (Burlington) and Norwich University (Northfield, Vermont) to establish comprehensive tools for monitoring and understanding the risk of landslides in the state. These investigations led to a Federal Emergency Management Agency (FEMA) buyout of a parcel containing a large landslide that posed a threat of additional slope failures in 1999. Rainfall and flooding during Hurricane Irene in 2011 led to slope instability throughout the state, prompting the development of statewide landslide protocols and the formation of a statewide landslide database that can be contributed to by landslide experts and residents.

Pennsylvania

The greater Pittsburgh region experienced record rainfall in February-April of 2018 that triggered more than 200 landslides. Built on clay-rich sedimentary rocks and with steep topography from downcutting by river erosion, southwestern Pennsylvania is one of the more landslide-prone regions in the country. The landslides are small and typically not deadly, affecting residences, roads, streams, and other infrastructure. As a result of the 2018 landslides, one natural gas pipeline ruptured, and the resulting explosion destroyed a house and several other buildings.

“It’s very clear that this was a climatically anomalous circumstance. We had a hugely anomalous amount of rain in February when Pittsburgh would normally be getting snow and the ground would be frozen. The ground wasn’t frozen, and almost all of the precipitation fell as rain. We had shallow soil slides as well as deeper-seated slides that require bigger changes in hydraulic conditions,” explains Helen Delano of the Pennsylvania Geological Survey, who will present about the record landslide year at the conference.

While the scope of damage from the landslides was extensive, an application for FEMA support was denied because the several months of increased landslides were not deemed a single event. When considered as separate events, they did not meet the threshold of damages required to declare a federal disaster. Delano says the record-breaking year has increased awareness at the state level of the need to prepare for landslides. Clean-up from the landslides of 2018 remains ongoing.

Published in Nature Reviews Earth & Environment, the study highlights the connections between surface and groundwater and calls for diversified strategies for managing them both.

“I like to emphasize a lot of solutions and how they can be optimized,” said lead author Bridget Scanlon, a senior research scientist at the UT Bureau of Economic Geology, a research unit of the Jackson School of Geosciences.

The study draws on data from satellites, climate models, monitoring networks and almost 200 scientific papers to analyze the Earth’s water supply, how it’s changing in different regions and what’s driving these changes. The study’s co-authors include almost two dozen water experts from around the world.

According to the research, humans primarily rely on surface water. Globally, it accounts for 75% of irrigation and 83% of municipal and industrial supply annually. However, what we see at the surface is tightly connected to groundwater flow. In the United States, about 50% of annual streamflow starts as groundwater. And globally, surface water that seeps into the ground accounts for about 30% of annual groundwater supplies.

Human intervention can strongly influence the exchange in water between surface and groundwater sources. About 85% of groundwater pumped by humans in the U.S. is considered “captured”from surface water, which leads to declines in streamflow. At the same time, irrigation sourced from surface water can increase groundwater recharge as irrigated water seeps through the ground back to aquifers.

The study cites numerous examples of human activity affecting this flux between surface water and groundwater supplies. For example, surface water irrigation recharged aquifers in the early to mid-1900s in the Northwestern U.S.’ Columbia Plateau and Snake River Plain, while global models show that groundwater pumping has greatly reduced the volume of water going to streams, with 15-21% of global watersheds at risk because of the reduced flows.

Despite their inherent connection, surface water and groundwater are frequently regulated and managed as separate resources. According to the researchers, future water resilience depends on recognizing that surface water and groundwater behave as a single resource — and acting on that knowledge.

The study describes different ways for managing water through both natural and engineered solutions that can help increase water supplies, reduce demand, store water and transport it. According to Scanlon, one of the best ways to adapt to increasing climate extremes is storing water during wet times and drawing on it in times of drought.

“We have droughts and we have floods,” she said. “We are trying to manage those extremes and a way to do that is to store water.”

Annually, the world stores about 7,000-8,300 cubic kilometers, or about two Lake Michigan’s worth of water, in surface reservoirs. The researchers said it was important to continue developing groundwater supplies, too, because they are more resilient than surface reservoirs during long-term droughts. Managed aquifer recharge can help cities build up their groundwater supplies by collecting surface water and diverting it underground into aquifers. Globally, about 10,000 cubic kilometers of water is stored this way each year.

“This type of integrated research, linking surface and groundwater, is exactly what is needed to develop lasting solutions to issues such as fresh water use,” said Scott Tinker, the director of the Bureau of Economic Geology. “Too often studies are done in isolation, and well-intended applications have unintended outcomes.”

Matthew Rodell, a hydrologist at NASA Goddard Space Flight Center who was not involved in the study, said that the paper offers a useful compendium of research results and potential solutions for managing water supplies while also keeping water quality — a characteristic that’s more difficult to monitor remotely than quantity — in mind.

“Water quality is one of the next targets in terms of being able to manage water resources,” he said. “I like that this was incorporated as well.”

To avoid a bottleneck of bots, a team of MIT engineers is designing a kit of universal robotic parts that an astronaut could easily mix and match to rapidly configure different robot “species” to fit various missions on the moon. Once a mission is completed, a robot can be disassembled and its parts used to configure a new robot to meet a different task.

The team calls the system WORMS, for the Walking Oligomeric Robotic Mobility System. The system’s parts include worm-inspired robotic limbs that an astronaut can easily snap onto a base, and that work together as a walking robot. Depending on the mission, parts can be configured to build, for instance, large “pack” bots capable of carrying heavy solar panels up a hill. The same parts could be reconfigured into six-legged spider bots that can be lowered into a lava tube to drill for frozen water.

“You could imagine a shed on the moon with shelves of worms,” says team leader George Lordos, a PhD candidate and graduate instructor in MIT’s Department of Aeronautics and Astronautics (AeroAstro), in reference to the independent, articulated robots that carry their own motors, sensors, computer, and battery. “Astronauts could go into the shed, pick the worms they need, along with the right shoes, body, sensors and tools, and they could snap everything together, then disassemble it to make a new one. The design is flexible, sustainable, and cost-effective.”

Lordos’ team has built and demonstrated a six-legged WORMS robot. Last week, they presented their results at IEEE’s Aerospace Conference, where they also received the conference’s Best Paper Award.

MIT team members include Michael J. Brown, Kir Latyshev, Aileen Liao, Sharmi Shah, Cesar Meza, Brooke Bensche, Cynthia Cao, Yang Chen, Alex S. Miller, Aditya Mehrotra, Jacob Rodriguez, Anna Mokkapati, Tomas Cantu, Katherina Sapozhnikov, Jessica Rutledge, David Trumper, Sangbae Kim, Olivier de Weck, Jeffrey Hoffman, along with Aleks Siemenn, Cormac O’Neill, Diego Rivero, Fiona Lin, Hanfei Cui, Isabella Golemme, John Zhang, Jolie Bercow, Prajwal Mahesh, Stephanie Howe, and Zeyad Al Awwad, as well as Chiara Rissola of Carnegie Mellon University and Wendell Chun of the University of Denver.

Animal instincts

WORMS was conceived in 2022 as an answer to NASA’s Breakthrough, Innovative and Game-changing (BIG) Idea Challenge — an annual competition for university students to design, develop, and demonstrate a game-changing idea. In 2022, NASA challenged students to develop robotic systems that can move across extreme terrain, without the use of wheels.

A team from MIT’s Space Resources Workshop took up the challenge, aiming specifically for a lunar robot design that could navigate the extreme terrain of the moon’s South Pole — a landscape that is marked by thick, fluffy dust; steep, rocky slopes; and deep lava tubes. The environment also hosts “permanently shadowed” regions that could contain frozen water, which, if accessible, would be essential for sustaining astronauts.

As they mulled over ways to navigate the moon’s polar terrain, the students took inspiration from animals. In their initial brainstorming, they noted certain animals could conceptually be suited to certain missions: A spider could drop down and explore a lava tube, a line of elephants could carry heavy equipment while supporting each other down a steep slope, and a goat, tethered to an ox, could help lead the larger animal up the side of a hill as it transports an array of solar panels.

“As we were thinking of these animal inspirations, we realized that one of the simplest animals, the worm, makes similar movements as an arm, or a leg, or a backbone, or a tail,” says deputy team leader and AeroAstro graduate student Michael Brown. “And then the lightbulb went off: We could build all these animal-inspired robots using worm-like appendages.'”

Snap on, snap off

Lordos, who is of Greek descent, helped coin WORMS, and chose the letter “O” to stand for “oligomeric,” which in Greek signifies “a few parts.”

“Our idea was that, with just a few parts, combined in different ways, you could mix and match and get all these different robots,” says AeroAstro undergraduate Brooke Bensche.

The system’s main parts include the appendage, or worm, which can be attached to a body, or chassis, via a “universal interface block” that snaps the two parts together through a twist-and-lock mechanism. The parts can be disconnected with a small tool that releases the block’s spring-loaded pins.

Appendages and bodies can also snap into accessories such as a “shoe,” which the team engineered in the shape of a wok, and a LiDAR system that can map the surroundings to help a robot navigate.

“In future iterations we hope to add more snap-on sensors and tools, such as winches, balance sensors, and drills,” says AeroAstro undergraduate Jacob Rodriguez.

The team developed software that can be tailored to coordinate multiple appendages. As a proof of concept, the team built a six-legged robot about the size of a go-cart. In the lab, they showed that once assembled, the robot’s independent limbs worked to walk over level ground. The team also showed that they could quickly assemble and disassemble the robot in the field, on a desert site in California.

In its first generation, each WORMS appendage measures about 1 meter long and weighs about 20 pounds. In the moon’s gravity, which is about one-sixth that of Earth’s, each limb would weigh about 3 pounds, which an astronaut could easily handle to build or disassemble a robot in the field. The team has planned out the specs for a larger generation with longer and slightly heavier appendages. These bigger parts could be snapped together to build “pack” bots, capable of transporting heavy payloads.

“There are many buzz words that are used to describe effective systems for future space exploration: modular, reconfigurable, adaptable, flexible, cross-cutting, et cetera,” says Kevin Kempton, an engineer at NASA’s Langley Research Center, who served as a judge for the 2022 BIG Idea Challenge. “The MIT WORMS concept incorporates all these qualities and more.”

This research was supported, in part, by NASA, MIT, the Massachusetts Space Grant, the National Science Foundation, and the Fannie and John Hertz Foundation.

Video: https://youtu.be/U72lmSXEVkM

Massive stars race through their lifecycles, and only some of them go through a brief Wolf-Rayet phase before going supernova, making Webb’s detailed observations of this rare phase valuable to astronomers. Wolf-Rayet stars are in the process of casting off their outer layers, resulting in their characteristic halos of gas and dust. The star WR 124 is 30 times the mass of the Sun and has shed 10 Suns’ worth of material — so far. As the ejected gas moves away from the star and cools, cosmic dust forms and glows in the infrared light detectable by Webb.

The origin of cosmic dust that can survive a supernova blast and contribute to the universe’s overall “dust budget” is of great interest to astronomers for multiple reasons. Dust is integral to the workings of the universe: It shelters forming stars, gathers together to help form planets, and serves as a platform for molecules to form and clump together — including the building blocks of life on Earth. Despite the many essential roles that dust plays, there is still more dust in the universe than astronomers’ current dust-formation theories can explain. The universe is operating with a dust budget surplus.

Webb opens up new possibilities for studying details in cosmic dust, which is best observed in infrared wavelengths of light. Webb’s Near-Infrared Camera (NIRCam) balances the brightness of WR 124’s stellar core and the knotty details in the fainter surrounding gas. The telescope’s Mid-Infrared Instrument (MIRI) reveals the clumpy structure of the gas and dust nebula of the ejected material now surrounding the star. Before Webb, dust-loving astronomers simply did not have enough detailed information to explore questions of dust production in environments like WR 124, and whether the dust grains were large and bountiful enough to survive the supernova and become a significant contribution to the overall dust budget. Now those questions can be investigated with real data.

Stars like WR 124 also serve as an analog to help astronomers understand a crucial period in the early history of the universe. Similar dying stars first seeded the young universe with heavy elements forged in their cores — elements that are now common in the current era, including on Earth.

Webb’s detailed image of WR 124 preserves forever a brief, turbulent time of transformation, and promises future discoveries that will reveal the long-shrouded mysteries of cosmic dust.