Connect with us

Published

on

After the successful Chandrayaan-3 mission to the Moon, ISRO on Monday announced that India’s first solar mission Aditya-L1 to study the Sun will be launched on September 2 at 11.50 am from Sriharikota spaceport. 

Aditya-L1 spacecraft is designed to provide remote observations of the solar corona and in-situ observations of the solar wind at L1 (Sun-Earth Lagrange point), which is about 1.5 million kilometres from the Earth.

Lagrange Points are positions in space where the gravitational forces of the Sun and the Earth produce enhanced regions of attraction and repulsion. These can be used by spacecraft to reduce fuel consumption needed to remain in position, according to NASA. Lagrange points are named in honor of Italian-French mathematician Josephy-Louis Lagrange.

The Bengaluru-headquartered space agency said in a social media post that the spacecraft — the first space-based Indian observatory to study the Sun — would be launched using a PSLV-C57 rocket.

The Aditya-L1 mission, aimed at studying the Sun from an orbit around the L1, would carry seven payloads to observe the photosphere, chromosphere and the corona — the outermost layers of the Sun — in different wavebands.

Aditya-L1 is a fully indigenous effort with the participation of national institutions, an ISRO official said.

The Bengaluru-based Indian Institute of Astrophysics (IIA) is the lead institute for the development of Visible Emission Line Coronagraph (VELC) payload while Inter-University Centre for Astronomy and Astrophysics, Pune, has developed the Solar Ultraviolet Imaging Telescope (SUIT) payload for the mission.

According to ISRO, VELC aims to collect the data for solving how the temperature of the corona can reach about a million degrees while the Sun’s surface itself stays just over 6000 degrees Centigrade.

Aditya-L1 can provide observations on the corona, and on the solar chromosphere using the UV payload and on the flares using the X-ray payloads. The particle detectors and the magnetometer payload can provide information on charged particles and the magnetic field reaching the halo orbit around L1.

The satellite, developed by U R Rao Satellite Centre here, arrived at ISRO’s spaceport of Sriharikota in Andhra Pradesh, earlier this month.

It is planned to be placed in a halo orbit around the L1 point of the Sun-Earth system.

A satellite placed in the halo orbit around the L1 point has the major advantage of continuously viewing the Sun without any planets obstructing the view or causing eclipses, ISRO noted. “This will provide a greater advantage of observing the solar activities and its effect on space weather in real time,” it said.

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

“The SUITs of Aditya L1 payloads are expected to provide the most crucial information to understand the problem of coronal heating, coronal mass ejection (CME), pre-flare and flare activities and their characteristics, dynamics of space weather, propagation of particle and fields etc,” ISRO said.

The major science objectives of the Aditya-L1 mission are: study of solar upper atmospheric (chromosphere and corona) dynamics; study of chromospheric and coronal heating, physics of the partially ionised 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; and physics of solar corona and its heating mechanism.

Besides, the mission aims to study diagnostics of the coronal and coronal loops plasma: temperature, velocity and density; development, dynamics and origin of 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; and drivers for space weather (origin, composition and dynamics of solar wind).

The instruments of Aditya-L1 are tuned to observe the solar atmosphere, mainly the chromosphere and corona. In-situ instruments will observe the local environment at the L1 point. 

Continue Reading

Science

Newly Confirmed Super-Earth HD 20794 d May Support Life in Habitable Zone

Published

on

By

Newly Confirmed Super-Earth HD 20794 d May Support Life in Habitable Zone

A super-Earth has been confirmed in the habitable zone of a nearby star, raising possibilities for future studies on potentially life-supporting planets. The discovery follows over two decades of observations and has been credited to a team of international researchers. Initially detected two years ago, the planet, named HD 20794 d, is situated 20 light years from Earth and has a mass six times that of Earth. Scientists suggest its orbit places it at an optimal distance from its star to sustain liquid water, a key factor for habitability.

Observational Data Confirms Planet’s Existence

According to a study published in Astronomy & Astrophysics, HD 20794 d was first identified as a possible exoplanet by Dr. Michael Cretignier from the University of Oxford in 2022. Data from the HARPS (High Accuracy Radial Velocity Planet Searcher) spectrograph at the La Silla Observatory in Chile indicated periodic shifts in the light spectrum of the host star, suggesting gravitational influence from an orbiting planet. However, initial findings lacked definitive confirmation due to the faintness of the signal, which led to doubts over whether the anomaly was planetary, instrumental, or caused by stellar activity.

To validate the discovery, data spanning over 20 years from both HARPS and ESPRESSO, an advanced spectrograph also based in Chile, were analysed. As reported by phys.org, Dr. Cretignier said that they have worked on data analysis for years and are gradually analysing and eliminating all possible sources of contamination. The confirmation required advanced processing techniques to separate the planetary signal from background interference.

Implications for Future Space Missions

Dr. Cretignier expressed both excitement and relief upon confirmation of the planet. He stated that great joy was naturally felt when the planet’s existence could be confirmed. Relief was also experienced, as the original signal had been at the edge of the spectrograph’s detection limit, making it difficult at that time to be completely convinced of the signal’s authenticity. He further stated that HD 20794 d’s proximity to Earth makes it a prime candidate for future missions aiming to capture direct images of exoplanets.

Despite its placement in the habitable zone, the planet’s elliptical orbit raises questions about its suitability for life. Its changing distance from the star moves it between the inner and outer edges of the habitable zone, potentially subjecting it to extreme temperature variations.

Potential for Further Study

HD 20794 d is expected to be a focal point for upcoming projects like the Extremely Large Telescope, the Habitable Worlds Observatory, and the Large Interferometer For Exoplanets (LIFE). These instruments aim to study exoplanet atmospheres in search of biosignatures that could indicate life.

Continue Reading

Science

El Capitan Is Now the Fastest Supercomputer on the Planet

Published

on

By

El Capitan Is Now the Fastest Supercomputer on the Planet

The world’s most powerful supercomputer, El Capitan, has been officially launched at the Lawrence Livermore National Laboratory (LLNL) in California. Built at a cost of $600 million, the system has been designed to manage highly classified national security tasks. The primary objective of the supercomputer is to ensure the security and reliability of the U.S. nuclear stockpile in the absence of underground testing, which has been prohibited since 1992. Research in high-energy-density physics, material discovery, nuclear data analysis, and weapons design will be conducted, along with other classified operations.

Performance and Capabilities

According to reports, El Capitan became the fastest supercomputer globally after achieving 1.742 exaFLOPS in the High-Performance Linpack (HPL) benchmark. The system has a peak performance of 2.746 exaFLOPS, making it the third machine ever to reach exascale computing speeds. The measurement, taken in floating-point operations per second (FLOPS), represents the ability of the supercomputer to perform one quintillion (10^18) calculations per second.

As reported by space.com, the second-fastest supercomputer, Frontier, located at Oak Ridge National Laboratory in Illinois, has recorded a standard performance of 1.353 exaFLOPS, with a peak of 2.056 exaFLOPS. El Capitan’s significant advancement marks a leap in computational capabilities within high-performance computing.

Technical Specifications

As reported by The Next Platform, El Capitan is powered by over 11 million processing and graphics cores distributed across 44,544 AMD MI300A accelerated processing units. These units incorporate AMD EPYC Genoa CPUs, AMD CDNA3 GPUs, and shared computing memory. Each processing unit includes 128 gigabytes of high-bandwidth memory, designed to optimise computational efficiency while minimising power consumption.

Development and Commissioning

Reports indicate that construction of El Capitan began in May 2023, with the system going online in November 2024. The official dedication took place on January 9, 2025. The supercomputer was commissioned by the U.S. Department of Energy’s CORAL-2 program as a successor to the Sierra supercomputer, which was deployed in 2018 and currently ranks 14th in the latest Top500 list of most powerful supercomputers.

With El Capitan’s full-scale deployment, advancements in national security research and computational science are expected to reach unprecedented levels.

Continue Reading

Science

ISRO Dismisses Glitch Reports in SpaDeX Docking, Confirms Mission Progress

Published

on

By

ISRO Dismisses Glitch Reports in SpaDeX Docking, Confirms Mission Progress

The Indian Space Research Organisation (ISRO) has dismissed reports suggesting issues in its maiden space docking mission, SpaDeX. On February 8, ISRO Chairman and Secretary, Department of Space, V Narayanan, clarified that no technical faults had been encountered in the docking process. He stated that the mission was progressing systematically and that further experiments were planned. His remarks were made during the 15th Biennial Edition of the Aero India International Seminar in Bengaluru, scheduled from February 10 to 14. The docking of satellites under SpaDeX was carried out successfully on January 16, with post-docking control enabling the satellites to function as a single entity.

Successful Docking and Mission Details

As reported by The Indian Express, according to ISRO, SpaDeX achieved a significant milestone by docking two satellites in orbit, with docking precision confirmed through manoeuvres. The agency reported that post-docking stability was achieved, with the satellites operating as a unified structure. The mission also involved injecting the NVS-02 navigation satellite into a Geosynchronous Transfer Orbit (GTO).

ISRO detailed the docking procedure, stating in a post on X (formerly Twitter) that the satellites were manoeuvred from a 15-metre distance to a 3-metre hold point before initiating capture. The docking process was completed with retraction and rigidisation for structural stability. With this development, India became the fourth country globally to achieve space docking.

Challenges in Orbit Raising Operations

Despite the successful docking, ISRO issued an update on February 2 indicating that attempts to raise the satellite’s orbit had encountered difficulties. The agency explained that the oxidiser valves, crucial for thruster ignition, had failed to open, preventing orbital repositioning. The issue remains under analysis as ISRO assesses possible solutions.

The SpaDeX mission was launched on December 30, 2024, using the PSLV C60 rocket, which deployed two small satellites, SDX01 and SDX02, into a 475-kilometre orbit. The mission serves as a demonstration of in-space docking capabilities, aiming to advance cost-effective space technology for future applications.

Continue Reading

Trending