How social structure influences the way people share money

People around the globe often depend on informal financial arrangements, borrowing and lending money through social networks. Understanding this sheds light on local economies and helps fight poverty.

Now, a study co-authored by an MIT economist illuminates a striking case of informal finance: In East Africa, money moves in very different patterns depending on whether local societies are structured around family units or age-based groups.

That is, while much of the world uses the extended family as a basic social unit, hundreds of millions of people live in societies with stronger age-based cohorts. In these cases, people are initiated into adulthood together and maintain closer social ties with each other than with extended family. That affects their finances, too.

“We found there are major impacts in that social structure really does matter for how people form financial ties,” says Jacob Moscona, an MIT economist and co-author of a newly published paper detailing the results.

He adds: “In age-based societies when someone gets a cash transfer, the money flows in a big way to other members of their age cohort but not to other [younger or older] members of an extended family. And you see the exact opposite pattern in kin-based groups, where money is transferred within the family but not the age cohort.”

This leads to measurable health effects. In kin-based societies, grandparents often share their pension payments with grandchildren. In Uganda, the study reveals, an additional year of pension payments to a senior citizen in a kin-based society reduces the likelihood of child malnourishment by 5.5 percent, compared to an age-based society where payments are less likely to move across generations.

The paper, “Age Set versus Kin: Culture and Financial Ties in East Africa,” is published in the September issue of the American Economic Review. The authors are Moscona, the 3M Career Development Assistant Professor of Economics in MIT’s Department of Economics; and Awa Ambra Seck, an assistant professor at Harvard Business School.

Studying informal financial arrangements has long been an important research domain for economists. MIT Professor Robert Townsend, for one, helped advance this area of scholarship with innovative studies of finances in rural Thailand.

At the same time, the specific matter of analyzing how age-based social groups function, in comparison to the more common kin-based groups, has tended to be addressed more by anthropologists than economists. Among the Maasai people in Northern Kenya, for example, anthropologists have observed that age-group friends have closer ties to each other than anyone apart from a spouse and children. Maasai age-group cohorts frequently share food and lodging, and more extensively than they do even with siblings. The current study adds economic data points to this body of knowledge.

To conduct the research, the scholars first analyzed the Kenyan government’s Hunger Safety Net Program (HSNP), a cash transfer project initiated in 2009 covering 48 locations in Northern Kenya. The program included both age-based and kin-based social groups, allowing for a comparison of its effects.

In age-based societies, the study shows, there was a spillover in spending by HSNP recipients on others in the age cohort, with zero additional cash flows to those in other generations; in kin-based societies, they also found a spillover across generations, but without informal cash flows otherwise.

In Uganda, where both kin-based and age-based societies exist, the researchers studied the national roll-out of the Senior Citizen Grant (SCG) program, initiated in 2011, which consists of a monthly cash transfer to seniors of about $7.50, equivalent to roughly 20 percent of per-capita spending. Similar programs exist or are being rolled out across sub-Saharan Africa, including in regions where age-based organization is common.

Here again, the researchers found financial flows aligned to kin-based and age-based social ties. In particular, they show that the pension program had large positive effects on child nutrition in kin-based households, where ties across generations are strong; the team found zero evidence of these effects in age-based societies.

“These policies had vastly different effects on these two groups, on account of the very different structure of financial ties,” Moscona says.

To Moscona, there are at least two large reasons to evaluate the variation between these financial flows: understanding society more thoroughly and rethinking how to design social programs in these circumstances.

“It’s telling us something about how the world works, that social structure is really important for shaping these [financial] relationships,” Moscona says. “But it also has a big potential impact on policy.”

After all, if a social policy is designed to help limit childhood poverty, or senior poverty, experts will want to know how the informal flow of cash in a society interacts with it. The current study shows that understanding social structure should be a high-order concern for making policies more effective.

“In these two ways of organizing society, different people are on average more vulnerable,” Moscona says. “In the kin-based groups, because the young and the old share with each other, you don’t see as much inequality across generations. But in age-based groups, the young and the old are left systematically more vulnerable. And in kin-based groups, some entire families are doing much worse than others, while in age-based societies the age sets often cut across lineages or extended families, making them more equal. That’s worth considering if you’re thinking about poverty reduction.”

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What Makes the Atomos Ninja & Shogun Ultra, Ultra? – Videoguys

On this Week’s Videoguys Live, James takes us through what’s new at Atomos and discussing their new products, the Ninja Phone and Shinobi II as well as promotions they are currently running on their ULTRA monitors. Tune in to learn more!

Watch the full webinar below:

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Atomos On Board Monitors / Recorders

Why Go Ultra?

High Frame Rate/Resolution Recording
Ninja Ultra and Shogun Ultra capture RAW inputs up to 8K at 30fps, 6K at 60fps, and 4K at 120fps and 1080 at 240p.​ Ninja can record up to 6k30p, 4k60p and Full HD120p

​Included Codecs
If you’re not sure what codec you’ll need for a particular job, don’t worry we’ve got you covered. We offer a choice of ProRes RAW, ProRes, DNxHR, DNxHD, and 8-bit or 10-bit HEVC (H.265) right out of the box.

Dual record

  • ProRes RAW Recording: Capture in ProRes RAW even if the camera lacks this capability.
  • Camera to Cloud: Enhances collaborative workflows.
  • Dual Recording: Record up to 4K 60p in ProRes RAW and HD 60p in H.265 simultaneously.
  • Auto-Matched Filenames: Compatible with ARRI, Canon, RED, Sony (via SDI), and Nikon Z9 (via HDMI).

Matched camera filenames

  • Dual Recording: Simultaneously record R3D RAW on RED Komodo and 10-bit, 4:2:2 HEVC (H.265) on Atomos.
  • Quick Edits: High-quality, smaller file size clips for easy editing.
  • Auto Conforming: File name matching simplifies the process.

Camera to Cloud

  • Proxy Recording: Now up to 4K 60p to match original files.
  • Efficient: H.265 files are half the size of H.264.
  • Immediate Use: Ideal for social media, sports, and news.
  • Fast Publishing: Quickly reach viewers.

Connectivity for all productions
For Camera to Cloud, streaming and live production, Shogun Ultra has integrated Wi-Fi 6E and GigE. Adding Atomos Connect to Ninja Ultra gives you Wi-Fi 6 and GigE.

Now with NDI 6​
NDI video will look more life-like than ever with the addition of fully native HDR support and 10- bit color depth. Ninja Ultra and Shogun Ultra will support NDI 6 in both send and transmit modes.​


New Products from Atomos means there is a perfect solution for every workflow

Ninja Phone

Now your phone can be a Ninja too!

Turn your smartphone into a high‑end 10‑bit recorder, monitor and streamer for your pro HDMI video camera.

Now available for iPhone 15/16 Pro and 15/16 Pro Max
  • Work with a larger, brighter, world-class monitor
  • The perfect companion for cloud connected workflows straight from the camera
  • Perfect the shot on set with less to fix in the edit
  • Position the monitor to suit your rig
  • Use the intuitive app interface and avoid complex internal camera menus
  • Bypass internal compression and record directly from the sensor
  • A choice of recording formats

Shinobi II

Slimmer. Brighter. Camera control.

The slim, lightweight, high brightness, 5-inch 1500nit HDR monitor that’s perfect for vloggers, creatives and photographers

  • Bright HDR Display: 1500nit peak brightness for outdoor use.​
  • Extensive Camera Control: Manage various cameras and trigger recording from Shinobi II.​
  • Power Options: Charge your camera via USB-C PD port.​
  • User-Friendly Interface: AtomOS 11 touchscreen.​
  • Long Battery Life: All-day usage.​
  • Lightweight & Adaptable: Easily position the monitor.​
  • Secure Connectivity: Unique cable locking system.

​Shogun Classic

The versatile, 7-inch workhorse that enables you to monitor, record, and switch all in the one device. It’s the perfect tool for live production, multi-camera shoots, and in-the-field event coverage.
  • 3000nit HDR screen: Zone backlight provides exceptional detail, color, and contrast.
  • Real-time 4K recording: In ProRes, Cinema DNG, and Avid DNx formats
  • High performance HDR: Preview your images in glorious 10-bit HDR
  • 4 x SDI input: For seamless transitions between live video streams
  • 4 x ISO recording: For individual input control and post-production flexibility
  • XLR audio: 2-channel XLR Input and output

Sun Dragon

The world’s first sun spectrum, HDR, waterproof, wireless DMX, 2000 lumen 5-color LED, mount-anywhere, lightweight flexible production and cinema rope light

Zato Connect

Zato Connect is packed with all the features you’d expect from Atomos, and streamlined for speed. A brilliant monitor, essential I/O and onboard recording are just the start of it. Connecting to the cloud with Zato gives you superpowers. That’s because you can capture, edit and post your social media content in the fastest possible way.

Shogun Studio 2

The highly flexible Shogun Studio 2 takes state of the art Atomos multi-channel recording technology and combines it with two premium 7-inch HDR 2000nit high bright touchscreen displays, all in a single 3RU unit. Its unique combination of features makes it perfect for live events, outside broadcast vehicles, production galleries and MCRs, post production facilities, video wall playout, on-set DITs and sports officiating. Connect to practically any SDI or HDMI source including camera channels, PTZ cameras and vision mixers.

SUMO 19SE

A bright (1200nit), HDR touchscreen covering the DCI-P3 (P3) Color Gamut, and able to record Apple ProRes RAW up to 6Kp30. With its rugged and versatile design, the Sumo 19SE is the perfect addition to an on-set video village.

Mars’ missing atmosphere could be hiding in plain sight

Mars wasn’t always the cold desert we see today. There’s increasing evidence that water once flowed on the Red Planet’s surface, billions of years ago. And if there was water, there must also have been a thick atmosphere to keep that water from freezing. But sometime around 3.5 billion years ago, the water dried up, and the air, once heavy with carbon dioxide, dramatically thinned, leaving only the wisp of an atmosphere that clings to the planet today.

Where exactly did Mars’ atmosphere go? This question has been a central mystery of Mars’ 4.6-billion-year history.

For two MIT geologists, the answer may lie in the planet’s clay. In a paper appearing today in Science Advances, they propose that much of Mars’ missing atmosphere could be locked up in the planet’s clay-covered crust.

The team makes the case that, while water was present on Mars, the liquid could have trickled through certain rock types and set off a slow chain of reactions that progressively drew carbon dioxide out of the atmosphere and converted it into methane — a form of carbon that could be stored for eons in the planet’s clay surface.

Similar processes occur in some regions on Earth. The researchers used their knowledge of interactions between rocks and gases on Earth and applied that to how similar processes could play out on Mars. They found that, given how much clay is estimated to cover Mars’ surface, the planet’s clay could hold up to 1.7 bar of carbon dioxide, which would be equivalent to around 80 percent of the planet’s initial, early atmosphere.

It’s possible that this sequestered Martian carbon could one day be recovered and converted into propellant to fuel future missions between Mars and Earth, the researchers propose.

“Based on our findings on Earth, we show that similar processes likely operated on Mars, and that copious amounts of atmospheric CO2 could have transformed to methane and been sequestered in clays,” says study author Oliver Jagoutz, professor of geology in MIT’s Department of Earth, Atmospheric and Planetary Sciences (EAPS). “This methane could still be present and maybe even used as an energy source on Mars in the future.”

The study’s lead author is recent EAPS graduate Joshua Murray PhD ’24.

In the folds

Jagoutz’ group at MIT seeks to identify the geologic processes and interactions that drive the evolution of Earth’s lithosphere — the hard and brittle outer layer that includes the crust and upper mantle, where tectonic plates lie.

In 2023, he and Murray focused on a type of surface clay mineral called smectite, which is known to be a highly effective trap for carbon. Within a single grain of smectite are a multitude of folds, within which carbon can sit undisturbed for billions of years. They showed that smectite on Earth was likely a product of tectonic activity, and that, once exposed at the surface, the clay minerals acted to draw down and store enough carbon dioxide from the atmosphere to cool the planet over millions of years.

Soon after the team reported their results, Jagoutz happened to look at a map of the surface of Mars and realized that much of that planet’s surface was covered in the same smectite clays. Could the clays have had a similar carbon-trapping effect on Mars, and if so, how much carbon could the clays hold?

“We know this process happens, and it is well-documented on Earth. And these rocks and clays exist on Mars,” Jagoutz says. “So, we wanted to try and connect the dots.”

“Every nook and cranny”

Unlike on Earth, where smectite is a consequence of continental plates shifting and uplifting to bring rocks from the mantle to the surface, there is no such tectonic activity on Mars. The team looked for ways in which the clays could have formed on Mars, based on what scientists know of the planet’s history and composition.

For instance, some remote measurements of Mars’ surface suggest that at least part of the planet’s crust contains ultramafic igneous rocks, similar to those that produce smectites through weathering on Earth. Other observations reveal geologic patterns similar to terrestrial rivers and tributaries, where water could have flowed and reacted with the underlying rock.

Jagoutz and Murray wondered whether water could have reacted with Mars’ deep ultramafic rocks in a way that would produce the clays that cover the surface today. They developed a simple model of rock chemistry, based on what is known of how igneous rocks interact with their environment on Earth.

They applied this model to Mars, where scientists believe the crust is mostly made up of igneous rock that is rich in the mineral olivine. The team used the model to estimate the changes that olivine-rich rock might undergo, assuming that water existed on the surface for at least a billion years, and the atmosphere was thick with carbon dioxide.

“At this time in Mars’ history, we think CO2 is everywhere, in every nook and cranny, and water percolating through the rocks is full of CO2 too,” Murray says.

Over about a billion years, water trickling through the crust would have slowly reacted with olivine — a mineral that is rich in a reduced form of iron. Oxygen molecules in water would have bound to the iron, releasing hydrogen as a result and forming the red oxidized iron which gives the planet its iconic color. This free hydrogen would then have combined with carbon dioxide in the water, to form methane. As this reaction progressed over time, olivine would have slowly transformed into another type of iron-rich rock known as serpentine, which then continued to react with water to form smectite.

“These smectite clays have so much capacity to store carbon,” Murray says. “So then we used existing knowledge of how these minerals are stored in clays on Earth, and extrapolate to say, if the Martian surface has this much clay in it, how much methane can you store in those clays?”

He and Jagoutz found that if Mars is covered in a layer of smectite that is 1,100 meters deep, this amount of clay could store a huge amount of methane, equivalent to most of the carbon dioxide in the atmosphere that is thought to have disappeared since the planet dried up.

“We find that estimates of global clay volumes on Mars are consistent with a significant fraction of Mars’ initial CO2 being sequestered as organic compounds within the clay-rich crust,” Murray says. “In some ways, Mars’ missing atmosphere could be hiding in plain sight.”

“Where the CO2 went from an early, thicker atmosphere is a fundamental question in the history of the Mars atmosphere, its climate, and the habitability by microbes,” says Bruce Jakosky, professor emeritus of geology at the University of Colorado and principal investigator on the Mars Atmosphere and Volatile Evolution (MAVEN) mission, which has been orbiting and studying Mars’ upper atmosphere since 2014. Jakosky was not involved with the current study. “Murray and Jagoutz examine the chemical interaction of rocks with the atmosphere as a means of removing CO2. At the high end of our estimates of how much weathering has occurred, this could be a major process in removing CO2 from Mars’ early atmosphere.”

This work was supported, in part, by the National Science Foundation.

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