Tuesday, February 24, 2026

 

How competitive gaming on discord fosters social connections



A Japanese Splatoon community reveals how online play has become a social third place



Doshisha University

How online gaming communities act as places for social connections 

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Online gaming spaces illustrate how Discord communities can function as social third places, beyond home and work.

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Credit: Valentin Ottone from Flickr https://www.flickr.com/photos/24450277@N06/3605180954




Human beings are social animals; they need places to relax, connect with others, and feel a sense of belonging beyond the demands of home and work. Traditionally, these ‘third places’ are thought to be limited to cafes, clubs, gardens, and other neighborhood community spots. However, with an increase in digitally shaped life schedules, a new question arises: Do online spaces offer the same social values as offline ones?

Video games and social media are often considered to be isolating or overly competitive among young generations. Yet, for many players, these platforms are more than just entertainment, giving them an opportunity to connect with like-minded people,” explains Assistant Professor Mattias van Ommen from the Faculty of Social Studies at Doshisha University, Japan. While these effects are well-demonstrated in research on Western gaming cultures, the effect of such digital communities remains highly understudied in Asian cultures, especially in Japan where gamers are still often stereotyped as socially awkward young males.

Capturing this issue, researchers at Doshisha University started to explore online gaming communities and their role as a space of social belonging. Together with former Doshisha University student Mr. Ginga Yahanashi, Dr. van Ommen conducted a long-term qualitative study of an online Discord community. The community was called Medimura (pseudonym) and was used by skilled players for the game Splatoon 3. The findings of the study were made available online and published in Volume 11, Issue 4 of the journal Social Media + Society on December 1, 2025.

An in-depth analysis of Medimura reflected that members initially joined primarily to improve their gameplay, but their motivations changed over time. “Participants who initially joined as competitive members eventually stayed back for social reasons, as they started feeling a sense of comfort in their everyday social engagements on Discord,” says Dr. van Ommen. With time, Medimura, which started as a gaming hub, became a place for people to simply spend time together.

The study emphasizes that members carefully balance competitive play with casual conversation. Although matches can be intense, players also joke, chat about daily life, and support one another during stressful moments. Encouraging clear community rules and entry requirements helps in maintaining a safe and respectful environment for people from different social backgrounds interacting on equal ground.

Importantly, the researchers found that the community functions as a ‘third place,’ despite existing entirely online. For most users, Medimura was a space they struggled to find elsewhere, free from strict rules and social pressure usually experienced at work or school. “For some players, the community provided a rare experience where they felt accepted as who they were,” comments Mr. Yahanashi. “For them, this sense of ease and emotional safety was just as important as the game itself.”

In a world where gamers are still often portrayed as socially withdrawn, this study shows that even competitive environments can lead to meaningful relationships. Considering the Japanese cultural context, where casual social interactions can be limited, especially in everyday work and school environments, gaming communities may play an important role in creating safe social spaces where people can relax and ‘be themselves.’

Looking ahead, the researchers hope their study will encourage a broader understanding of digital platforms and their impact on supporting social wellbeing. In a digital age, where offline and online lives continue to coexist, communities like Medimura demonstrate how creative technology can be used to promote social connections, providing a sense of belonging and mutual support.


About Assistant Professor Mattias van Ommen from Doshisha University, Japan
Dr. Mattias van Ommen is an Assistant Professor in the Department of Sociology at Doshisha University, Japan, where he specializes in cultural anthropology and Japanese digital gaming cultures. He completed a Bachelor of Arts in Japan Studies at Leiden University, Netherlands, and holds a Master’s and a PhD in Anthropology earned at the University of Hawaiʻi at Mānoa. He has published on digital games, online communities, and contemporary forms of social interaction, with particular attention to Japanese gaming spaces. His upcoming book on Japanese Final Fantasy XIV communities, Fantastic Intimacy, will be published by Cornell University Press in the late 2026.

Funding information
The authors disclosed receipt of the following financial support for the research, authorship, and/or publication of this article: While the authors received no financial support for the research of this article, this article’s publication—specifically the article processing charge (APC)—was provided by the APC support program of Doshisha University’s Department of Research Planning.

Media contact:
Organization for Research Initiatives & Development
Doshisha University
Kyotanabe, Kyoto 610-0394, JAPAN
E-mail:jt-ura@mail.doshisha.ac.jp

 SPACE/COSMOS

Why some objects in space look like snowmen


Gravitational collapse may explain the origin of contact binaries in the Kuiper Belt, MSU simulation finds




Michigan State University

Kuiper belt image 

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This image was taken by NASA's New Horizons spacecraft on Jan. 1, 2019 during a flyby of Kuiper Belt object 2014 MU69, informally known as Ultima Thule. It is the clearest view yet of this remarkable, ancient object in the far reaches of the solar system – and the first small "KBO" ever explored by a spacecraft.

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Credit: NASA





Astronomers have long debated why so many icy objects in the outer solar system look like snowmen. Michigan State University researchers now have evidence of the surprisingly simple process that could be responsible for their creation.

Far beyond the violent, chaotic asteroid belt between Mars and Jupiter lies what’s known as the Kuiper Belt. There, past Neptune, you’ll find icy, untouched building blocks from the dawn of the solar system, known as planetesimals. About one in 10 of these objects are contact binaries, planetesimals that are shaped like two connected spheres, much like Frosty the Snowman. But just how these objects came to be without the help of a magic silk hat was an open question.

Jackson Barnes, an MSU graduate student, has created the first simulation that reproduces the two-lobed shape naturally with gravitational collapse. His work is published in the Monthly Notices of the Royal Astronomical Society.

Earlier computational models treated colliding objects as fluid blobs that merged into spheres, making it impossible to form these unique shapes. Thanks to MSU’s Institute for Cyber-Enabled Research, or ICER, and its high-performance computing cluster, Barnes’ simulations produce a more realistic environment that allows objects to retain their strength and rest against one another.

Other formation theories involve special events or exotic phenomena that, while possible, aren’t likely to happen on a regular basis.

“If we think 10 percent of planetesimal objects are contact binaries, the process that forms them can’t be rare,” said Earth and Environmental Science Professor Seth Jacobson, senior author on the paper. “Gravitational collapse fits nicely with what we’ve observed.”

Contact binaries were first imaged up close by NASA’s New Horizons spacecraft in January 2019. These images prompted scientists to take another look at other objects in the Kuiper belt, and it turned out that contact binaries accounted for about 10 percent of all planetesimals. These distant objects float mostly undisturbed and safe from collisions in the sparsely populated Kuiper belt.

In the early days of the Milky Way, the galaxy was a disc of dust and gas. Remnants of the galaxy’s formation are found in the Kuiper Belt, including dwarf planets like Pluto, comets and planetesimals.

Planetesimals are the first large planetary objects to form from the disc of dust and pebbles. Much like individual snowflakes that are packed into a snowball, these first planetesimals are aggregates of pebble-sized objects pulled together by gravity from a cloud of tiny materials.

Occasionally as the cloud rotates, it falls inward on itself, ripping the object apart and forming two separate planetesimals that orbit one another. Astronomers observe many binary planetesimals in the Kuiper belt. In Barnes’ simulation, the orbits of these objects spiral inward until the two gently make contact and fuse together while still maintaining their round shapes.

How do these two objects stay together throughout the history of the solar system? Barnes explains they’re simply unlikely to crash into another object. Without a collision, there’s nothing to break them apart. Most binaries aren’t even pocked with craters.

Scientists long suspected that gravitational collapse was responsible for forming these objects, but they couldn’t fully test the idea. Barnes’ model is the first to include the physics needed to reproduce contact binaries.

“We’re able to test this hypothesis for the first time in a legitimate way,” Barnes said. “That’s what’s so exciting about this paper.”

Barnes expects his model will help scientists understand binary systems of three or more objects. The team is also working to create a new simulation that better models the collapse process.

As more NASA missions explore uncharted realms of the solar system, Jacobson and Barnes suspect Frosty may have more distant cousins yet to be found.


Simulation of gravitational collapse [VIDEO] |

Jackson Barnes created this computer simulation showing how a contact binary’s two-lobed shape could be formed by gravitational collapse.

Contact binary example 

Jackson Barnes created this contact binary in a computer simulation showing how the two-lobed shape could be formed by gravitational collapse.

Credit

Michigan State University Jacobson Lab




New Horizons video [VIDEO] 

This short movie shows the view of Kuiper Belt object 2014 MU69 (nicknamed Ultima Thule) as seen by NASA's New Horizons spacecraft from Dec. 7, 2018 to Jan. 1, 2019. During the approach, Ultima Thule transforms from a faint dot 20 million miles (31 million kilometers) away, indistinguishable from thousands of background stars, to a newly revealed world unlike any seen before, from a range of 5,000 miles (8,000 kilometers). The sequence consists of actual New Horizons images, taken at discrete intervals during the approach, supplemented with computer-generated intermediate frames in order to make a smooth movie. Time slows down during the movie to show clearly both the slow initial phases of the approach and the very rapid final stages. The final image is a parting crescent view of Ultima Thule, taken 10 minutes after closest approach occurred at 12:33 a.m. EST on Jan. 1.

Credit

NASA


STEM IS DEI

PhD student maps mysterious upper atmosphere of Uranus for the first time


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Northumbria University

Paola Tiranti of Northumbria University 

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Paola Tiranti of Northumbria University

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Credit: Northumbria University/Barry Pells




A Northumbria University PhD student has led an international team of astronomers in creating the first-ever three-dimensional map of Uranus's upper atmosphere, revealing how the ice giant's unusual magnetic field shapes spectacular auroras high above the planet's clouds.

 

Using the James Webb Space Telescope, led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency), Paola Tiranti and her colleagues observed Uranus for nearly a full rotation, detecting the faint glow from molecules up to 5,000 kilometres above the cloud tops.

 

The observations provide the most detailed picture yet of where the planet's auroras form and how energy moves through its atmosphere.

 

The study, published today (19 Feb) in Geophysical Research Letters, also confirms that Uranus's upper atmosphere has continued to cool over the past thirty years – a trend that has been surprising scientists for over three decades.

 

Auroras occur when energetic particles become trapped in a planet's magnetic field and strike the upper atmosphere, releasing energy that creates a signature glow.

 

Using Webb's Near-Infrared Spectrograph, the team mapped out the temperature and density of ions in Uranus's ionosphere, a region where the atmosphere becomes ionised and interacts strongly with the planet's magnetic field.

 

The measurements revealed that temperatures peak between 3,000 and 4,000 kilometres above the cloud tops, whilst ion densities reach their maximum around 1,000 kilometres.

 

Speaking about the findings, lead author Paola Tiranti said: “This is the first time we've been able to see Uranus's upper atmosphere in three dimensions. With Webb's sensitivity, we can trace how energy moves upward through the planet's atmosphere and even see the influence of its lopsided magnetic field.”

 

Uranus's magnetosphere is one of the strangest in the Solar System. Unlike Earth, where the magnetic field is relatively aligned with the planet's rotation axis, Uranus's magnetic field is tilted by nearly 60 degrees and offset from the planet's centre. This means its auroras sweep across the surface in complex ways.

 

The Webb observations detected two bright auroral bands near Uranus's magnetic poles, together with a distinct depletion in emission and ion density between them – a feature likely linked to how magnetic field lines guide charged particles through the atmosphere. Similar darkened regions have been seen at Jupiter, where magnetic field geometry controls particle flow.

 

Webb's data also confirmed that Uranus's upper atmosphere is still cooling, extending a trend that began in the early 1990s. The team measured an average temperature of around 426 kelvins (about 150 degrees Celsius), lower than values recorded by ground-based telescopes or previous spacecraft observations.

 

Understanding why Uranus is cooling, despite being so far from the Sun, could provide crucial insights into how ice giant planets regulate their atmospheric temperature.

 

Paola Tiranti said: “By revealing Uranus's vertical structure in such detail, Webb is helping us understand the energy balance of the ice giants. This is a crucial step towards characterising giant planets beyond our Solar System.”

 

The study is based on data from JWST General Observer programme 5073, led by Dr Henrik Melin of Northumbria University, which used the telescope's Integral Field Unit on 19 January 2025 to observe Uranus for 15 hours.

 

Planetary scientists from Northumbria University's Solar and Space Physics peak of research excellence have been involved in a number of research projects using data from Webb, specifically exploring the upper atmospheres of our solar system's giant gas planets – Jupiter, Saturn, Uranus and Neptune.

 

 

The James Webb Space Telescope is the world's premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

  

Uranus (January 2025)

Credit

ESA/Webb, NASA, CSA, STScI, P. Tiranti, H. Melin, M. Zamani (ESA/Webb)

Paola Tiranti of Northumbria University

Credit

Northumbria University/Barry Pells