Connect with us

Published

6 months ago

on

The mechanics of hula hooping have been analysed by researchers, uncovering how body shapes and motions influence the ability to keep a hoop spinning against gravity. Insights from the study have raised intriguing questions about body dynamics, energy efficiency, and potential engineering applications. The findings, based on experiments and mathematical modelling, offer new perspectives on an activity often overlooked in scientific research. Key revelations include the role of body curvature and slope in maintaining the hoop’s motion.

Study Details Dynamics of Hula Hooping

According to research published in the Proceedings of the National Academy of Sciences, experiments were conducted using miniature robotic models at New York University’s Applied Mathematics Laboratory. Different shapes, such as cylinders, cones, and hourglasses, were replicated at one-tenth human scale to examine their impact on hula hooping efficiency. Motorised motions were applied to these models, and high-speed cameras captured the behaviour of hoops launched onto the robotic forms.

Findings indicated that successful twirling could be achieved without significant variation based on body cross-section shapes, such as circles or ellipses. However, maintaining the hoop’s height against gravity required specific physical attributes, particularly sloping hips and a curvy waist. These characteristics provided the necessary angles for upward thrust and stability, helping to keep the hoop in motion.

Mathematical Modelling and Broader Applications

Senior researcher and associate professor Leif Ristroph explained in a press release that mathematical models were developed to explain the physical principles observed. These models offered insight into the interaction between body motion and hoop dynamics, which could be extended to applications such as energy harvesting and robotics.

The researchers highlighted that the work bridges a gap in the understanding of a popular activity, while also demonstrating its relevance to technology. Ristroph noted that these findings could lead to improvements in robotic systems used in manufacturing, as well as innovative ways to utilise energy generated by vibrations.

This research sheds light on the science behind hula hooping, offering practical applications while enhancing the understanding of human and mechanical motion.

Catch the latest from the Consumer Electronics Show on Gadgets 360, at our CES 2025 hub.

Related Topics:
Continue Reading

Science

Dead NASA Satellite Relay 2 May Have Caused Mysterious 2024 Radio Burst

Published

3 days ago

on

June 27, 2025

By

Dead NASA Satellite Relay 2 May Have Caused Mysterious 2024 Radio Burst

In June 2024, scientists detected a mysterious, powerful burst of radio waves originating from within our galaxy. At first, they thought it was coming from a pulsar or another undiscovered cosmic object. However, an analysis revealed the origin of the signal was too close to the Earth. Astronomers think it was caused by a long-dead NASA satellite Relay 2, was launched in 1964 but ceased operations in 1967 after its communication systems failed. Yet, nearly 60 years later, it mysteriously emitted a powerful radio signal, the researchers said in a new preprint study, which was posted June 13 to the server arXiv and has not yet been peer-reviewed.

Relay 2: A Silent Satellite Sends a Loud Signal

According to the study, the signal was detected using the Australian Square Kilometre Array Pathfinder (ASKAP) telescope array. These intense flashes typically originate from deep space and can carry more energy in milliseconds than the sun emits over several days.

But this signal, lasting just 30 nanoseconds, was traced back to the vicinity of Earth, too close for ASKAP to focus on clearly. After ruling out cosmic sources, the team traced the pulse to the orbit of Relay 2. Despite having no functioning systems, the satellite somehow emitted the brightest radio flash in the sky at that moment.

Researchers proposed two theories: a micrometeorite impact that created a radio-emitting plasma cloud, or an electrostatic discharge (ESD) caused by charge buildup on the satellite’s aging materials.

New Clues About Spacecraft Behavior and Space Debris

Though both mechanisms could produce similar signals, scientists lean toward electrostatic discharge as the likelier cause. According to space physicists, older spacecraft like Relay 2 may be especially prone to such energy releases due to outdated materials and limited shielding.

Karen Aplin told New Scientist that studying these accidental emissions could help monitor ESD events on today’s small satellites — many of which also lack advanced protection. In an increasingly crowded orbital environment, this detection method may offer a novel tool for evaluating space debris and satellite health.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


Qualcomm May Use Samsung Foundry to Produce Different Variants of Snapdragon Elite 2 SoC for Galaxy S26 Series



Gemini on Android Will Soon Connect to Apps Even If User Disables Activity Logs, Won’t Affect Privacy

Continue Reading

Science

James Webb Telescope Captures First Direct Image of Saturn-Mass Exoplanet

Published

3 days ago

on

June 27, 2025

By

James Webb Telescope Captures First Direct Image of Saturn-Mass Exoplanet

The James Webb Space Telescope (JWST) has captured its first direct image of a newly discovered exoplanet. Astronomers announced that Webb imaged a Saturn-mass planet orbiting the nearby young star TWA 7. Dubbed TWA 7 b, the planet’s mass is only about 0.3 times that of Jupiter – roughly Saturn’s mass – making it the smallest planet ever seen via direct imaging. Most of the nearly 6,000 known exoplanets have been detected indirectly. To spot TWA 7 b, the JWST team used a coronagraph (like a solar eclipse) to block the star’s light and reveal the faint planet.

Detecting a Hidden World

According to the study published in the journal Nature, Webb’s team targeted TWA 7 because its dusty disk is viewed nearly face-on, revealing clear ring structures. They used Webb’s MIRI instrument with a coronagraph to mask the star’s glare. After processing the data, a faint infrared point source appeared roughly 1.5 arcseconds from TWA 7 (about 50 times the Earth–Sun distance).

This source lies in a gap of the star’s second dust ring. Its brightness and color match what theoretical models predict for a young, cold planet roughly Saturn’s mass. The object seems to be carving out the ring gap just as an orbiting planet would. Astronomers ruled out other explanations (like a background star) to confirm the signal is best explained by a planet.

A Step Toward Smaller Worlds

TWA 7 b’s Saturn-like mass makes it about ten times less massive than any exoplanet previously captured in a direct image. Its discovery shows that Webb can now image worlds far smaller than the giant exoplanets seen before. Scientists say the telescope may eventually detect planets as light as 10% of Jupiter’s mass, pushing toward Earth-like size.

This breakthrough “paves the way” to imaging truly terrestrial planets in the future. Astronomers even predict that upcoming observatories could dramatically increase the number of Earth-size planets seen by direct imaging. Next-generation telescopes – on the ground and in space – are being planned with even more powerful coronagraphs to hunt for the first directly photographed Earth analogues.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


Gemini on Android Will Soon Connect to Apps Even If User Disables Activity Logs, Won’t Affect Privacy



How to Delete Emails in Bulk in Gmail Using Different Methods

Related Stories

Continue Reading

Science

James Webb Telescope Detects Methanol and Ethanol Near Young Stars, Hinting at Life’s Origins

Published

3 days ago

on

June 27, 2025

By

James Webb Telescope Detects Methanol and Ethanol Near Young Stars, Hinting at Life’s Origins

In the recent research done by using the James Webb Telescope, in March 2024, scientists found that ethanol and other icy organic compounds near protostars IRAS 2A and IRAS 23385. The findings were published in the JOYS+ program. It can offer insights into the cosmic chemistry that can help in knowing the formation of the planet and the potential for life on it. This also suggests how the building blocks in life can travel in space. The scientists observed alcohol in the orbit of a young star, adding to the understanding of life on Earth.

Methanol and Its Isotopes Detected Around Star HD 100453

As per the recent study conducted by NASA’s JWST, Methanol and its isotopes have been found in gases around the star called HD 100453. It is about 330 light years away from our planet. It has been observed for the first time that scientists have found isotopes of methanol in the shape of a disk. This was reported on June 5, 2025, in the Astrophysical Journal Letters.

Methanol: A Building Block of Life

Methanol acts as a building block for organic compounds like amino acids, which are essential for life. Researchers had found that methanol, but not the rare isotopes, is star-forming structures. These isotopes of methanol give a valuable insight into the ingredients needed for building life on Earth.

HD 100453: A Star Bigger Than the Sun

HD 100453 is larger than the Sun, with more than 1.6 times the mass of the Sun. This signals that methanol and other molecules in the disk exist as gas and farther from the home star, which could be the case when the solar system was quite young. The smaller stars consist of cooler disks, and the molecules are frozen and undetectable.

Link Between Methanol and Comet Chemistry

The researchers found that the ratio of methanol to other organic molecules is similar to that of the comets in the solar system. The findings signal that the ices near the protoplanetary disks clump to form comets filled with organic molecules, which are the result of collisions. This research gives the idea that comets may have played a major role in offering important organic material to the Earth billions of years ago.

Continue Reading

Trending