Connect with us

Published

on

A lunar mission involving a rocket-powered hopper is set to launch later this month. The spacecraft, named Athena, is expected to carry multiple payloads, including ‘Gracie,’ a small robotic explorer developed through a collaboration between Intuitive Machines and NASA. The launch is scheduled to take place from Florida’s Space Coast within a four-day window opening on February 26. If the landing proceeds as planned, Athena will touch down on a plateau approximately 160 kilometres from the Moon’s south pole, a region believed to contain water ice deposits.

Gracie’s Mission Objectives and Design

As reported by space.com, Gracie is designed to perform five controlled hops across the lunar surface using thrusters. The initial hop is expected to reach 20 metres in height, followed by progressively higher leaps, culminating in a descent into a shadowed lunar crater known as Crater H. This crater, located approximately 500 metres from Athena’s landing site, has a depth of around 20 metres.

Trent Martin, Senior Vice President of Space Systems at Intuitive Machines, stated in a NASA press conference that the hopper is intended to operate in extreme conditions, with its final hop aiming to explore the crater floor. Efforts are being made to maintain communication during this phase through Nokia’s Lunar Surface Communication System, which aims to establish the first 4G/LTE network on the Moon.

Scientific Exploration and Data Collection

Gracie is expected to collect data using its onboard instruments. A key feature is the ‘water snooper’ sensor, designed to detect water ice in the surrounding environment. Additionally, the hopper is equipped with cameras, which will provide images of the lunar surface and its movements. The mission is intended to demonstrate alternative exploration methods beyond traditional rover-based designs, with Gracie’s success potentially influencing future lunar exploration strategies.

Additional Payloads on Athena

The Athena lander is set to carry several other payloads. NASA’s Polar Resources Ice Mining Experiment 1 (PRIME-1) will conduct subsurface sampling using a drill capable of reaching depths of one metre. A mass spectrometer will be used to analyse these samples for signs of water and other volatile compounds. Another payload, the Mobile Autonomous Prospecting Platform (MAPP), developed by Lunar Outpost, will explore the lunar surface with high-resolution optical and thermal cameras. A smaller rover known as AstroAnt, developed by the Massachusetts Institute of Technology, will also be deployed from MAPP to collect temperature data.

Expected Landing and Operational Timeline

If Athena’s landing is successful, operations on the Moon are expected to last approximately ten Earth days. The lander and its payloads will function until the lunar night sets in, cutting off solar power. This mission follows the success of Intuitive Machines’ IM-1 mission, which landed the Odysseus spacecraft on the lunar surface in February 2024, marking the first private soft landing on the Moon. Despite minor landing issues, Odysseus provided valuable insights, setting a precedent for future commercial lunar missions.

Additional lunar missions by private companies are currently underway, including Firefly Aerospace’s Blue Ghost and Tokyo-based ispace’s Resilience lander, both launched aboard a Falcon 9 rocket in January. These missions form part of an increasing number of private sector efforts aimed at exploring and utilising lunar resources.

Continue Reading

Science

AMoRE Experiment Sets New Benchmark in Neutrinoless

Published

on

By

AMoRE Experiment Sets New Benchmark in Neutrinoless

The latest phase of the AMoRE (Advanced Mo-based Rare Process Experiment) project has yielded significant findings in the search for neutrinoless double beta decay, a process that could redefine understanding of fundamental particle physics. Conducted at the Yangyang Underground Laboratory in Korea, the study involved the use of molybdate scintillating crystals at extremely low temperatures to detect this elusive nuclear event. While no clear evidence was observed, the research has set a new upper limit on the decay halflife of molybdenum-100, refining the parameters for future experiments in the field.

New Constraints Established

According to the study published in Physical Review Letters, the AMoRE collaboration utilised multiple kilograms of molybdenum-100, a radioactive isotope, in the form of scintillating crystals. The experiment aimed to detect whether two neutrons in a nucleus could decay into two protons without emitting neutrinos, a phenomenon that would confirm the neutrino and antineutrino as identical particles. Detection of this process is considered crucial for exploring matter-antimatter asymmetry in the universe.

In an interview with Phys.org, Yoomin Oh, corresponding author of the study, explained that the neutrino is one of the elementary particles in the Standard Model. It was ‘invented’ by Wolfgang Pauli about a hundred years ago and discovered a couple of decades later than that. He added that while neutrinos are among the most abundant particles, their properties, including mass, remain largely unknown.

Next Phase: AMoRE-II at Yemilab

AMoRE-I achieved the highest sensitivity ever recorded for detecting neutrinoless double beta decay in molybdenum-100, but no definitive signal was found. This outcome has refined the experimental approach, with the next phase, AMoRE-II, currently being developed at Yemilab, a newly constructed underground research facility in Korea.

The upcoming phase will involve a significantly larger quantity of molybdenum-based crystal detectors and an upgraded low-temperature detection system. The AMoRE collaboration aims to achieve an even lower background environment, enhancing the sensitivity of the experiment. Data collection for AMoRE-II is expected to begin within the next year, with researchers hoping to uncover new insights into the nature of neutrinos.

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.


Assassin’s Creed Shadows Hits 2 Millions Players, Surpasses Launches of Assassin’s Creed Origins, Odyssey



Den of Thieves 2: Pantera OTT Release Date: When and Where to Watch it Online?

Continue Reading

Science

Did black hole radiation shape the universe?

Published

on

By

Did black hole radiation shape the universe?

A theoretical form of radiation first proposed by Stephen Hawking may have played a role in shaping the universe after the Big Bang, as suggested by recent research. The phenomenon is known as Hawking radiation. It was introduced in the 1970s when Hawking theorised that black holes could emit radiation despite their widely accepted nature as objects that absorb all matter. The study suggests that primordial black holes which are believed to have existed in the early universe, may have released intense radiation. This emission could have influenced cosmic structures in ways previously unaccounted for.

Findings from the Study

According to the study published in the Journal of Cosmology and Astroparticle Physics, a phase may have occurred in the early universe where primordial black holes dominated the energy density before evaporating through Hawking radiation. The researchers state that ultra-light primordial black holes could have rapidly gained prominence during expansion, leaving behind observable effects. The research suggests that the impact of these black holes was powerful enough to influence the formation of galaxies and cosmic structures.

Examining the Role of Hawking Radiation

The study builds on Hawking’s work. He merged aspects of quantum mechanics and general relativity. Black holes were once thought to trap everything indefinitely. The Hawking’s theory introduced the possibility of radiation emission. It is reported that larger black holes radiate at an extremely low rate, making detection with existing technology impossible. The focus shifts to smaller primordial black holes, estimated to be less than 100 tons in mass, as their radiation levels could have shaped the universe’s early structure.

Potential Implications of the Research

The study explores the possibility of Hawking relics which are stable particles resulting from the evaporation of black holes. If these particles are detected, it could provide insights into the cosmic radiation budget and the formation of atomic nuclei. The research suggests that primordial black holes must have evaporated before certain cosmic events to align with existing atomic models. While Hawking relics have not been directly observed, future technological advancements may allow for their detection. The findings open avenues for understanding black hole physics and the universe’s evolution.

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.


Aghathiyaa Tamil Fantasy Thriller Now Streaming on Sun NXT



Assassin’s Creed Shadows Hits 2 Millions Players, Surpasses Launches of Assassin’s Creed Origins, Odyssey

Related Stories

Continue Reading

Science

Artemis II Orion Service Module Secured for Launch at Kennedy Space Center

Published

on

By

Artemis II Orion Service Module Secured for Launch at Kennedy Space Center

NASA’s Artemis II Orion spacecraft has gone through a critical step in its preparation for launch. Three spacecraft adapter jettison fairings have been installed on the service module inside the Neil A. Armstrong Operations and Checkout Building at the Kennedy Space Center in Florida. This installation was completed on March 19, 2025. It plays an important role in protecting the spacecraft during its ascent. The fairings shield the solar array wings from extreme conditions such as heat and wind while also helping to distribute the force generated by the Space Launch System (SLS) rocket. Once the spacecraft reaches space, the panels will detach, which will reduce the overall mass and allow the solar wings to deploy.

Structural Enhancements for Launch Readiness

According to NASA, the European-built service module is a key component of the Orion spacecraft. It provides power, propulsion and life support for the mission. Four solar array wings were fitted earlier in March, forming an important part of the module’s design. The newly added fairing panels are essential for safeguarding these components during launch. Their primary function is to resist the intense vibrations and aerothermal forces experienced during liftoff. Once the spacecraft exits Earth’s atmosphere, the fairings will separate, ensuring the solar arrays can function as intended.

Mission Details and Crew Objectives

The Artemis II mission will be NASA’s first crewed flight under the Artemis programme. The spacecraft will carry four astronauts. This includes NASA’s Reid Wiseman, Victor Glover and Christina Koch, along with Canadian Space Agency astronaut Jeremy Hansen. They will gp on a 10-day mission to orbit the Moon, testing the spacecraft’s capabilities before future deep-space missions. The service module will supply oxygen, water and temperature control to support the crew during their journey.

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.


Zakir Khan’s Delulu Express Stand-Up Special Now Streaming on Prime Video



Nothing Explains Why It Used UFS 2.2 Storage in Phone 3a and Phone 3a Pro

Related Stories

Continue Reading

Trending