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A new approach to measuring dark matter density in the Milky Way has been introduced by researchers from The University of Alabama in Huntsville (UAH). The study outlines how gravitational acceleration measurements from pulsars can provide insights into the distribution of dark matter in the galaxy. With an expanded dataset including solitary pulsars, scientists have been able to refine their findings, marking a significant advancement in astrophysical research. The ability to measure accelerations at an unprecedented scale has enabled the team to determine local dark matter density with greater accuracy. The findings suggest that in a volume equivalent to Earth, less than 1 kilogram of dark matter is present, highlighting its rarity despite its dominance in the universe’s total mass.

Use of Solitary Pulsars for Dark Matter Measurement

According to the study published on the arXiv preprint server, earlier research relied on binary millisecond pulsars to measure galactic acceleration. Dr. Sukanya Chakrabarti, Pei-Ling Chan Endowed Chair at UAH, explained to Phys.org that most pulsars exist as solitary objects rather than in pairs. By incorporating solitary pulsars into their methodology, the research team has effectively doubled the sample size available for analysis. This expansion allows for a more precise mapping of the Milky Way’s gravitational field, including its dark matter distribution.

Galactic Wobble and Its Role in Measurement

The study also delves into the effects of the Large Magellanic Cloud (LMC) on the Milky Way. Dr. Chakrabarti told Phys.org that the LMC’s gravitational influence creates an imbalance in the Milky Way, leading to an observable wobble. This asymmetry has now been quantified for the first time through pulsar acceleration data. The impact of this gravitational interaction provides further evidence supporting the study’s findings on dark matter distribution.

Addressing Magnetic Braking in Pulsar Acceleration Analysis

A challenge in previous research was accounting for the spindown effect caused by magnetic braking in pulsars. Dr. Tom Donlon, a postdoctoral associate at UAH, explained to Phys.org that binary pulsars were initially used because their orbits remained unaffected by magnetic braking. The latest study has introduced a method to estimate magnetic braking effects with high accuracy, allowing solitary pulsars to be incorporated into acceleration measurements. This advancement broadens the scope of analysis and strengthens the reliability of the findings.

Future Prospects in Dark Matter Research

With the ability to measure accelerations as small as 10 cm/s per decade, the research team believes that mapping the dark matter distribution in the Milky Way with high precision is now within reach. Dr. Chakrabarti stated to Phys.org that while large accelerations near black holes and the galactic center have been measured in the past, this study marks the first time such small accelerations caused by dark matter have been directly observed. The findings contribute significantly to the ongoing efforts to understand the elusive nature of dark matter and its role in shaping the cosmos.

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NASA’s New Missions Will Map the Sun and the Cosmos

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NASA’s New Missions Will Map the Sun and the Cosmos

Two NASA missions aimed at advancing space research are scheduled for launch aboard a SpaceX Falcon 9 rocket on March 2 from Launch Complex 4E at Vandenberg Space Force Base in California. The spacecraft, PUNCH and SPHEREx, have been designed for separate but complementary scientific objectives. While PUNCH will focus on the dynamics of the Sun’s corona and solar wind, SPHEREx will survey the broader universe using infrared observations. This dual launch, facilitated under NASA’s Launch Services Program, is expected to enhance understanding of cosmic evolution and space weather phenomena.

PUNCH to Study Solar Wind and Space Weather

As reported by Space.com, according to NASA, the Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission consists of four small satellites designed to create three-dimensional images of the Sun’s outer atmosphere. These satellites will use polarized light to track solar events such as coronal mass ejections (CMEs), helping scientists determine their trajectories and potential impacts on Earth. Speaking to Space.com, Nicholeen Viall, PUNCH mission scientist at NASA’s Goddard Space Flight Center, stated that the mission is expected to provide significantly improved resolution compared to previous heliophysics missions like STEREO.

SPHEREx to Map the Universe in Infrared

As per NASA, the Spectro-Photometer for the History of the Universe, Epoch of Reionisation, and Ices Explorer (SPHEREx) will conduct an extensive infrared survey of the entire sky every six months. Unlike the James Webb Space Telescope, which captures highly detailed images of specific regions, SPHEREx is designed to generate broad cosmic maps in 102 wavelengths. In a statement to Space.com, Phil Korngut, SPHEREx instrument scientist at the California Institute of Technology, noted that the data will contribute to research on cosmic inflation, galaxy formation, and the origins of water in planetary systems.

Both missions are expected to play a crucial role in expanding current knowledge of space phenomena, with their launch anticipated to provide valuable insights into both solar and cosmic environments.

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SpaceX Falcon 9 Launches Athena Lander, NASA’s Lunar Trailblazer to Moon

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SpaceX Falcon 9 Launches Athena Lander, NASA's Lunar Trailblazer to Moon

A SpaceX Falcon 9 rocket lifted off from Kennedy Space Center on February 26, 2025, carrying the Athena lunar lander and NASA’s Lunar Trailblazer orbiter. The launch, which took place at 7:16 p.m. EST from Launch Complex-39A, marked a significant step in lunar exploration. Athena, developed by Intuitive Machines, is designed to investigate lunar water ice deposits, while Lunar Trailblazer will study similar phenomena from orbit.

Scientific Goals and Technology

As per reports, according to NASA, Athena is equipped with ten scientific instruments, including the Polar Resources Ice Mining Experiment 1 (PRIME-1). The experiment consists of the Regolith Ice Drill for Exploring New Terrain (TRIDENT) and the Mass Spectrometer observing lunar operations (MSolo), both of which will work to extract and analyse samples from beneath the lunar surface. These investigations aim to provide critical data on the presence of water ice, supporting future in-situ resource utilisation (ISRU) efforts.

Lunar Trailblazer, an orbiter developed by NASA, will complement Athena’s findings by mapping water ice deposits across the lunar surface. Scientists have stated that its data will enhance the understanding of lunar ice distribution, particularly in the Mons Mouton region, where Athena is expected to land.

Landing Plans and Exploration Vehicles

Reports indicate that Athena will reach lunar orbit in four to five days and attempt a landing between 1.5 and three days after that. The mission will last approximately ten Earth days. To extend its exploration capabilities, Athena carries two secondary vehicles: MAPP, a rover designed by Lunar Outpost, and Grace, a hopping robot developed by Intuitive Machines. Grace will explore shadowed craters inaccessible to wheeled vehicles, while MAPP will establish a lunar cellular network using the Lunar Surface Communications System (LSCS) developed by Nokia Bell Labs.

Challenges and Expectations

This mission follows Intuitive Machines’ IM-1 mission, which achieved the first soft lunar landing by a private company but encountered a landing issue that affected data transmission. Trent Martin, Senior Vice President of Space Systems at Intuitive Machines, stated to Space.com that improved landing accuracy is a primary focus for IM-2.

NASA’s contract for IM-2 was initially valued at $47 million but increased to $62.5 million due to additional requirements, including temperature data collection. Reports suggest that Athena and Lunar Trailblazer are part of a broader lunar exploration effort, joining missions such as Firefly Aerospace’s Ghost Riders in the Sky and ispace’s Resilience lander, both launched earlier in 2025.

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Scientists Find a New Way To Turn Stale Bread Into Carbon Electrodes

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Scientists Find a New Way To Turn Stale Bread Into Carbon Electrodes

A team of engineers has introduced two innovative techniques for shaping carbon electrodes derived from bread. The methods, which build upon previous research, enable the formation of electrodes in precise and sturdy forms. These advancements could enhance the sustainability of electrode production by utilising stale bread, a commonly wasted food item. The process involves heating bread at high temperatures in an oxygen-free environment, converting it into a carbon-based material suitable for applications such as desalination systems. The research aims to refine this process for potential large-scale production, offering an eco-friendly alternative for carbon electrode manufacturing.

New Techniques for Molding Carbon Electrodes

According to the study published in Royal Society Open Science, the research was conducted by David Bujdos, Zachary Kuzel and Adam Wood from Saint Vincent College and the University of Pittsburgh. The team built upon earlier efforts by Adam Wood, who had previously demonstrated that stale bread could be used to produce carbon electrodes due to its high carbon content.

The latest development introduces two techniques that allow for shaping the electrodes into desired forms. The first method involves compressing bread using a 3D-printed mold before subjecting it to the heating process. This technique enables the formation of precise electrode shapes. In a test, a zigzag mold was used to demonstrate its effectiveness.

The second method requires blending bread with water before shaping it manually. Once formed, the material is dried and carbonised in an oven. While this approach provides less precision, the resulting electrodes are reportedly more durable.

Potential for Sustainable Electrode Production

As per reports, the researchers believe these methods could contribute to the development of a low-cost capacitive desalination system. The aim is to create an environmentally friendly solution that reduces food waste while addressing water purification challenges. Efforts are underway to refine the process and explore possibilities for large-scale implementation.

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