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ISRO will perform the final manoeuvre on Saturday to inject Aditya-L1 spacecraft — the first space-based Indian observatory to study the Sun — into its final destination orbit, some 1.5 million kilometres from the Earth. According to ISRO officials, the spacecraft will be placed in a halo orbit around Lagrange point 1 (L1) of the Sun-Earth system, about 1.5 million km from the Earth. The L1 point is about one per cent of the total distance between the Earth and the Sun.

A satellite in a halo orbit around the L1 point has the major advantage of continuously viewing the Sun without any occultations/eclipses, they said, adding, this will provide a greater advantage in observing solar activities and its effect on space weather in real time.

“This manoeuvre (at around 4pm on Saturday) will bind the Aditya-L1 to a halo orbit around L1. If we don’t do this, there is a possibility that it will continue its journey, maybe towards the Sun,” an ISRO official told PTI on Friday.

The Polar Satellite Launch Vehicle (PSLV-C57) launched the Aditya-L1 spacecraft from the second launch pad of Satish Dhawan Space Centre (SDSC), Sriharikota, on September 2 last year.

After a flight duration of 63 minutes and 20 seconds, it was successfully injected into an elliptical orbit of 235×19500 km around the Earth.

The spacecraft underwent a series of manoeuvres thereafter and headed Sun-Earth Lagrange Point 1(L1), having escaped the Earth’s sphere of influence.

The spacecraft carries seven payloads to observe the photosphere, chromosphere and the outermost layers of the Sun (the corona) using electromagnetic and particle and magnetic field detectors.

“Using the special vantage point L1, four payloads directly view the Sun and the remaining three payloads carry out in-situ studies of particles and fields at the Lagrange point L1, thus providing important scientific studies of the propagatory effect of solar dynamics in the interplanetary medium,” according to the space agency.

The suits of Aditya L1 payloads are expected to provide the “most crucial information” to understand the problem of coronal heating, coronal mass ejection, pre-flare and flare activities and their characteristics, dynamics of space weather, and propagation of particles and fields, officials said.

The major science objectives of the Aditya-L1 mission are:

  • Study of the Solar upper atmospheric (chromosphere and corona) dynamics.
  • Study of chromosphere and coronal heating, physics of the partially ionized plasma, initiation of the coronal mass ejections, and flares.
  • Observe the in-situ particle and plasma environment, providing data for the study of particle dynamics from the Sun.
  • Physics of the solar corona and its heating mechanism.
  • Diagnostics of the coronal and coronal loops plasma: Temperature, velocity and density.
  • Development, dynamics and origin of coronal mass ejections (CMEs).
  • Identify the sequence of processes that occur at multiple layers (chromosphere, base and extended corona) which eventually leads to solar eruptive events.
  • Magnetic field topology and magnetic field measurements in the solar corona.
  • Drivers for space weather (origin, composition and dynamics of solar wind).

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New Method Controls Synchronisation in Spin Hall Nano-Oscillators Using Spin Waves

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New Method Controls Synchronisation in Spin Hall Nano-Oscillators Using Spin Waves

A recent breakthrough in spintronic technology has demonstrated how phase-tunable synchronisation can be achieved in spin Hall nano-oscillators (SHNOs). These nanoscale devices generate high-frequency microwave signals by converting direct current into spin wave auto-oscillations. The ability to control synchronisation between SHNOs is expected to improve applications in telecommunications, neuromorphic computing, and optimisation hardware. The study, conducted by researchers at the University of Gothenburg in Sweden and Tohoku University in Japan, highlights the role of propagating spin waves in enabling phase information transfer between SHNOs.

Phase Control Through Spin Waves

According to the study published in Nature Physics, experimental evidence has confirmed that spin-wave-mediated mutual synchronisation between SHNOs is possible. Unlike earlier systems that relied on nearest-neighbor interactions, the use of propagating spin waves has allowed long-range, one-to-one coupling. Akash Kumar, the first author of the study, explained to Phys.org that this research was motivated by previous findings on propagating spin waves in SHNOs. The team utilised optimised thin-film materials, specifically W/CoFeB/MgO, to facilitate this coupling.

Experimental Validation and Potential Applications

The study’s findings were supported by electrical measurements and advanced microscopy techniques. High-frequency spectrum analysers were used to detect phase-tuned synchronisation, while phase-resolved Brillouin light scattering (μ-BLS) microscopy provided direct visualisation of oscillator phase alignment. Victor H. González, a graduate student and co-author of the study, confirmed the results through micromagnetic simulations. Kumar stated that the ability to transfer phase information between SHNOs has significant implications for Ising machines, which are used for combinatorial optimisation tasks. Future research will focus on scaling the system and incorporating voltage gating to enhance control and energy efficiency in spintronic devices.

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Japan’s First Space Launch of 2025 Sends Michibiki 6 Navigation Satellite into Orbit

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Japan’s First Space Launch of 2025 Sends Michibiki 6 Navigation Satellite into Orbit

Japan successfully launched a navigation satellite on Sunday, marking the country’s first space mission of 2025. The H3 rocket lifted off from Tanegashima Space Center at 3:30 a.m. EST carrying the Michibiki 6 satellite. The launch vehicle, developed by the Japan Aerospace Exploration Agency (JAXA) and Mitsubishi Heavy Industries, placed the 4,900-kilogram spacecraft into a geostationary transfer orbit 29 minutes after liftoff. The satellite is set to enhance Japan’s Quasi-Zenith Satellite System (QZSS), which has been operational since November 2018.

Michibiki 6 to Strengthen Japan’s Navigation System

According to space.com, Michibiki 6 is expected to improve satellite-based navigation services in Japan and nearby regions. As said in a statement by Japan officials, the QZSS, designed to work alongside the United States’ Global Positioning System (GPS), enhances positioning accuracy, particularly in urban and mountainous areas where GPS signals may be obstructed. The system’s expansion aims to provide better location services across Asia-Oceania, reinforcing Japan’s capabilities in satellite positioning.

H3 Rocket Gains Momentum After Initial Failure

The H3 rocket used for this mission is Japan’s next-generation launch vehicle, intended to replace the aging H-2A series. This was the fifth flight of the H3, which initially failed during its maiden launch in March 2023, resulting in the loss of an Earth observation satellite. Since then, all subsequent missions have been completed without issue.

Japan’s Expanding Space Initiatives

Japan has been steadily advancing its space program, focusing on satellite navigation, communications, and deep-space exploration. Future launches are expected to strengthen the nation’s technological presence in space, with plans to expand collaborations in both commercial and scientific ventures.

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Mind-Controlling Fungus That Turns Spiders into Zombies Found in Ireland

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Mind-Controlling Fungus That Turns Spiders into Zombies Found in Ireland

A newly identified fungus that infects and manipulates spiders has been discovered in Northern Ireland. Found in a former Victorian gunpowder store on the grounds of a ruined Irish castle, this fungus takes control of cave spiders, leading them out of their usual hiding spots before killing them and using their bodies to release spores. The fungus, which resembles the species known to infect ants, was first observed during the filming of a nature documentary in 2021. Scientists later confirmed it as an entirely new species.

Named in Honour of Sir David Attenborough

According to a study published in Fungal Systematics and Evolution, the fungus has been named Gibellula attenboroughiiin recognition of British naturalist Sir David Attenborough. It was initially found on a dead orb-weaving cave spider, a species that typically resides in caves and dark man-made structures like cellars and old storerooms. Following this initial discovery, more infected spiders were located in caves across Ireland. The infected spiders were observed in open spaces rather than concealed within their usual lairs, suggesting that the fungus influences their behaviour before killing them.

How the Fungus Infects and Controls Spiders

Study lead author Harry Evans, an emeritus fellow at the Centre for Agriculture and Bioscience International (CABI), explained to Live Science that the fungus penetrates the spider’s body, infecting its hemocoel—the cavity containing its blood-like fluid. Once inside, it secretes toxins to kill the host before producing antibiotics that preserve the corpse. When conditions such as humidity levels are suitable, the fungus grows structures on the spider’s body to release spores into the air.

Potential for Medicinal Applications

Beyond its ability to manipulate spiders, the fungus is being studied for potential medicinal properties. Evans noted that its antibiotic-producing capabilities could lead to new medical discoveries. Scientists have extracted its DNA to confirm that it is a previously unidentified species. While it has only been found in Ireland so far, researchers suspect that similar fungi may exist in other regions, including Wales.

Hidden Diversity of Parasitic Fungi

The study highlighted the likelihood of many more undiscovered fungal species, particularly parasitic ones. Researchers estimate that the fungal kingdom could contain up to 20 million species, with only a small fraction currently identified. Initially, the new species was to be named Gibellula bangbangus, referencing the gunpowder store where it was first found, but the decision was later made to name it after Attenborough instead.

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