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A new robotic system capable of planetary exploration through tethered jumping has been developed by researchers at the Robotics and Mechanisms Laboratory (RoMeLa) at the University of California, Los Angeles (UCLA). The robot, named SPLITTER (Space and Planetary Limbed Intelligent Tether Technology Exploration Robot), has been designed as a modular, multi-robot system composed of two quadrupedal robots connected by a tether. The system, expected to be presented at the IEEE Aerospace Conference (AeroConf) 2025, has been designed to navigate low-gravity environments such as the moon and asteroids. Reports indicate that the robotic system can perform successive jumps while collecting scientific data, providing an alternative to conventional planetary rovers and drones.

SPLITTER’s Design and Capabilities

According to the study published on the arXiv preprint server, SPLITTER consists of two Hemi-SPLITTER robots connected by a tether, forming a dumbbell-like structure. The tether enables mobility and stability during mid-air travel, eliminating the need for additional attitude control mechanisms such as gas thrusters or reaction wheels. The system has been designed to dynamically alter its inertia by adjusting limb positions and tether length, ensuring stability during flight. The development of SPLITTER was driven by the limitations of traditional planetary rovers, which are often slow and cumbersome, and the impracticality of drones due to the absence of atmospheric conditions on celestial bodies like the moon and asteroids.

Mechanism Behind SPLITTER’s Motion

Reports suggest that SPLITTER incorporates an inertial morphing mechanism based on a Model Predictive Controller (MPC) to regulate its orientation during mid-air movements. The concept is based on the Tennis Racket Theorem, also known as the Dzhanibekov effect, which describes how objects with asymmetric inertia undergo spontaneous rotational flips. Yusuke Tanaka, lead author of the study, told Tech Xplore that the technique allows aggressive stabilization of the robot’s mid-air flight through controlled inertia adjustments. It has been suggested that this method significantly enhances the efficiency of planetary exploration by ensuring stability without relying on external force mechanisms.

Potential Applications and Future Research

The research team has indicated that SPLITTER could be deployed in planetary exploration missions as a swarm of robots, allowing extensive and unstructured terrain to be efficiently traversed. The tether mechanism could also enable one unit to explore craters or caves while the other remains anchored, providing support. Dennis Hong, director of RoMeLa and principal investigator of the project, told Tech Xplore that ongoing research is focusing on improving the hardware, including new actuators and sensing mechanisms. Future studies are expected to further validate the inertial morphing mechanism through high-fidelity simulations, with the long-term goal of enhancing SPLITTER’s capabilities for real-world space applications.

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IIT Madras and ISRO Unveil IRIS, India’s First Aerospace-Grade Semiconductor

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IIT Madras and ISRO Unveil IRIS, India’s First Aerospace-Grade Semiconductor

The Indian Institute of Technology Madras (IIT Madras) and the Indian Space Research Organisation (ISRO) have successfully developed and booted an aerospace-grade semiconductor chip, marking a significant step towards self-reliance in space technology. The chip, named ‘IRIS’ (Indigenous RISCV Controller for Space Applications), has been designed based on the SHAKTI processor and is intended for use in IoT and compute systems. The project aligns with India’s efforts to reduce dependence on foreign semiconductor technology and is part of a broader initiative to strengthen indigenous capabilities in space applications.

Development and Testing of the IRIS Chip

According to reports, the ISRO Inertial Systems Unit (IISU) in Thiruvananthapuram collaborated with IIT Madras to define the specifications and develop the chip. The design incorporates fault-tolerant internal memories to improve reliability and includes custom functional and peripheral interface modules such as CORDIC, WATCHDOG Timers, and advanced serial buses. Testing of the semiconductor was conducted to ensure its suitability for space missions, with rigorous software and hardware evaluations carried out before finalising the chip.

Complete Indigenous Fabrication and Assembly

Professor V. Kamakoti, Director of IIT Madras, stated to India Today that the entire development process, including chip design, fabrication, packaging, motherboard assembly, and software booting, was carried out within India. The project is part of the ‘Digital India RISC-V’ initiative (DIRV), which supports domestic development of microprocessor-based products with high security standards.

ISRO and Industry Support for Indigenous Innovation

ISRO Chairman Dr. V Narayanan expressed satisfaction over the development of the IRIS Controller, highlighting its contribution to India’s ‘Make in India’ initiative. Kamaljeet Singh, Director General of the Semiconductor Laboratory (SCL) Chandigarh, mentioned that SCL remains committed to collaborating with academia and startups to further India’s self-reliance in niche semiconductor products.

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James Webb Telescope to Study Potentially Hazardous Asteroid 2024 YR4

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James Webb Telescope to Study Potentially Hazardous Asteroid 2024 YR4

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James Webb Telescope to Study Potentially Hazardous Asteroid 2024 YR4

The James Webb Space Telescope (JWST) has been allocated emergency observation time to study asteroid 2024 YR4, which has been classified as potentially hazardous. The space rock was identified in December 2024 and has been placed on the asteroid watch list due to its estimated 2.3% chance of colliding with Earth in December 2032. The emergency decision has been made to improve the accuracy of its size estimation, which is currently based on ground-based observations. Scientists believe that a more precise measurement of its dimensions will provide better insight into the potential risk it poses.

Infrared Observations to Determine True Size

According to reports, the European Space Agency (ESA), the asteroid has an estimated width of 55 metres, but this figure is uncertain due to limitations in ground-based telescopic observations. The asteroid’s brightness has been used to approximate its size, though its actual dimensions may vary significantly depending on surface reflectivity. If the surface is highly reflective, the asteroid could be as small as 40 metres. If it is less reflective, its true size could be as large as 90 metres, significantly altering the potential impact risk assessment.

JWST has been selected for this task due to its ability to capture infrared emissions, which can provide a more accurate measurement of the asteroid’s size and surface composition. Unlike ground telescopes, which rely on reflected sunlight, JWST’s infrared capabilities will detect heat emitted by the asteroid, offering a clearer picture of its actual dimensions. The updated information will play a crucial role in refining impact probability models and informing future planetary defence strategies.

Scheduled Observations and Data Availability

Observations using JWST are planned for March and May. The first session will coincide with the asteroid reaching peak brightness, while the second will take place as it moves away from the Sun. These observations will be conducted using four hours of JWST’s director’s discretionary time, a reserve allocation used for urgent scientific inquiries.

The data collected during these observations will be publicly released once processed. ESA has highlighted the significance of this research, stating that refining the size estimation of 2024 YR4 is essential for determining its potential impact consequences. The results will contribute to ongoing research into near-Earth objects and planetary defence strategies.

Previous Impacts and Potential Consequences

Historical events have demonstrated the damage that asteroids of this size can cause. The Tunguska event of 1908, which flattened an estimated 80 million trees over a vast area of Siberia, is believed to have been caused by an asteroid of similar dimensions. While an impact from 2024 YR4 would not cause mass extinction, the regional consequences could be severe.

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Increased Seismic Activity at Mount Spurr Raises Eruption Concerns

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Increased Seismic Activity at Mount Spurr Raises Eruption Concerns

An increase in seismic activity has been recorded at Mount Spurr, a stratovolcano located 124 kilometres west of Anchorage, Alaska. Over the past ten months, small earthquakes have been detected, with a noticeable rise in activity observed in recent weeks. Reports indicate that the earthquakes, which were initially concentrated near the summit, have shifted towards Crater Peak, a side vent that previously erupted in 1992 and 1953. Scientists suggest that this could signal the movement of magma beneath the volcano, potentially leading to an eruption. The likelihood of an eruption occurring at Crater Peak has been estimated at 50 percent, while the chances of an eruption at the volcano’s main crater remain low.

Potential Eruption Scenarios at Mount Spurr

According to the Alaska Volcano Observatory (AVO), the ongoing seismic activity could either lead to an eruption or subside without significant volcanic activity. Matt Haney, Scientist-in-Charge at AVO, told Live Science that the earthquake pattern has intensified, with tremors now concentrated in an area approximately 3 kilometres down the slope. This shift aligns with previous eruptions from Crater Peak, which ejected ash plumes reaching 20,000 metres into the atmosphere. Despite similarities to past events, volcanic unrest observed in 2004 and 2005 did not result in an eruption, demonstrating that increased seismicity does not always lead to an explosive event.

Possible Impact of an Eruption

If an eruption occurs, hazards such as pyroclastic flows, lahars, and ashfall could impact surrounding areas. While no communities are directly in the path of potential lahars or pyroclastic flows, disruptions to air travel could be significant. The 1992 eruption of Crater Peak led to the temporary closure of Anchorage’s airport and covered parts of the city in ash. Given the current volume of air traffic passing through Alaska, a similar event could cause major disruptions to transcontinental flights. Scientists are monitoring the situation closely, particularly for signs of prolonged seismic tremors, which could indicate that an eruption is imminent.

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