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- Breaking Space News: Nov 24 - 30, 2024
Breaking Space News: Nov 24 - 30, 2024
Bittersweet Space News This Week: Declining Global Freshwater, Spaceflight Brain Changes, The Stunning Deep Space 'Sombrero,' and Guitar Nebula, Lasers from Photosynthetic Bacteria, Aliens and Emergent Communication, Trump Administration and Space, Space Debris Mitigation, Mysterious Deep Space Signals, Stars as Spaceships, and More.
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This week we have some stunning images from across the Universe! Commercial Space is picking up pace and so is Research into Dark Matter. Don’t forget to go here for the best reading experience/in case your newsletter gets clipped at the bottom.
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IMAGES
Sombrero Galaxy : Mid-Infrared Instrument (MIRI), James Webb Space Telescope
NASA's James Webb Space Telescope has recently captured an image of the Sombrero Galaxy using its Mid-Infrared Instrument (MIRI), revealing the clumpy distribution of dust in the galaxy's outer ring.
The mid-infrared light highlights the gas and dust involved in star formation within the outer disk of the Sombrero Galaxy. The galaxy's rings generate less than one solar mass of stars per year, which is lower compared to the Milky Way's approximately two solar masses per year, indicating that the Sombrero Galaxy is not a major hub of star formation. The JWST image also shows the presence of polycyclic aromatic hydrocarbons, indicating potential young star-forming regions, although the overall star formation rate remains low.
The Sombrero Galaxy is located about 30 million light-years from Earth in the constellation Virgo. (Credit: NASA, ESA, CSA, STScI)
The James Webb Space Telescope’s MIRI (Mid-Infrared Instrument) reveals the smooth inner disk of the galaxy, while the Hubble Space Telescope’s visible-light image (above) shows the large and extended glow of the central bulge of stars. (Credit: NASA, ESA, CSA, STScI)
'Flame-Throwing' Guitar Nebula : Chandra X-Ray Observatory, Hubble Space Telescope
The Guitar Nebula using NASA's Chandra X-ray Observatory and Hubble Space Telescope: This nebula, located approximately 2,700 light-years from Earth, gets its name from its striking resemblance to a guitar, with a bright pulsar (PSR B2224+65) at the tip of the headstock. The pulsar's high-energy particles create a flame-like filament extending about two light-years, or 12 trillion miles, which has been observed over more than two decades.
The images of the Guitar Nebula are composite, combining data from both Chandra and Hubble. Chandra's X-ray data highlights the high-energy particles emitted by the pulsar, while Hubble's optical observations reveal the surrounding nebula in greater detail. This combination allows scientists to create a "movie" showing the nebula's evolution, providing valuable insights into how pulsars interact with the interstellar medium and the creation of matter and antimatter particles through high-energy radiation. (Credit: X-ray: NASA/CXC/Stanford Univ./M. de Vries et al.; Optical: (Hubble) NASA/ESA/STScI and (Palomar) Hale Telescope/Palomar/CalTech; Image Processing: NASA/CXC/SAO/L. Frattare)
Outline of the guitar shape in the X-ray and optical image. The tip of the guitar is the pulsar, a rapidly rotating neutron star left behind after the collapse of a massive star. As it hurtles through space it is pumping out a flame-like filament of particles and X-ray light that astronomers have captured with Chandra. (Credit: X-ray: NASA/CXC/Stanford Univ./M. de Vries et al.; Optical: (Hubble) NASA/ESA/STScI and (Palomar) Hale Telescope/Palomar/CalTech; Image Processing: NASA/CXC/SAO/L. Frattare)
NGC 2090 : James Webb Space Telescope
The latest Picture of the Month from the James Webb Space Telescope (JWST) showcases the spiral galaxy NGC 2090, located in the constellation Columba. This detailed image, a combination of data from JWST's MIRI and NIRCam instruments, reveals the galaxy's two winding spiral arms and the swirling gas and dust of its disc. NGC 2090, previously studied by the Hubble Space Telescope, is now known to be 40 million light-years away. The near-infrared data from NIRCam highlights the spiral arms with remarkable clarity, while MIRI captures mid-infrared light from carbon-based compounds along the gas and dust strands. (Credit: ESA/Webb, NASA & CSA, A. Leroy)
3D Simulation of Sun's Turbulent Dynamics : NASA
NASA scientists have released a dazzling 3D simulation showcasing the sun's turbulent behavior, revealing intricate flows within its layers. The simulation, powered by the Pleiades supercomputer, uses data from NASA's Solar Dynamics Observatory to visualize the movement of solar plasma. This research aims to decode the sun's complex dynamics, which influence Earth's weather, ocean currents, and space weather. The findings could enhance our understanding of solar phenomena and improve space weather predictions, crucial for protecting satellites and astronauts.
A 3D simulation showing the evolution of turbulent flows in the upper layers of the Sun. The more saturated and bright reds represent the most vigorous upward or downward twisting motions. Clear areas represent areas where there are only relatively slow up-flows, with very little twisting. (Credit: NASA/Irina Kitiashvili and Timothy A. Sandstrom)
SCIENCE
Global Freshwater Levels See Sharp Decline, NASA Reports
NASA satellites have revealed a significant and abrupt drop in global freshwater levels since May 2014, indicating that Earth's continents may be entering a persistently drier phase. Measurements from the Gravity Recovery and Climate Experiment (GRACE) satellites show that from 2015 through 2023, the average amount of freshwater stored on land was 290 cubic miles (1,200 cubic kilometers) lower than the average levels from 2002 through 2014. This reduction in freshwater is attributed to a combination of factors, including prolonged droughts, increased reliance on groundwater for agriculture and urban needs, and the effects of global warming.
This map shows the years that terrestrial water storage hit a 22-year minimum (i.e., the land was driest) at each location, based on data from the GRACE and GRACE/FO satellites. A significantly large portion of the global land surface reached this minimum in the nine years since 2015, which happen to be the nine warmest years in the modern temperature record. (Credit: NASA Earth Observatory/Wanmei Liang with data courtesy of Mary Michael O’Neill)
The decline in freshwater levels began with a massive drought in northern and central Brazil, followed by major droughts in regions such as Australasia, South America, North America, Europe, and Africa. Even after the significant El Niño event of 2014-2016, global freshwater levels have not rebounded, with 13 of the world's 30 most intense droughts occurring since January 2015. Scientists suspect that global warming, which leads to more extreme precipitation events and prolonged dry periods, may be contributing to the enduring freshwater depletion.
A render of the GRACE satellites which measure gravity as they orbit the planet to reveal shifting levels of water on the Earth. (Credit: NASA/JPL-Caltech)
This reduction in available water poses significant challenges for farmers and communities, potentially leading to famine, conflicts, poverty, and an increased risk of disease as people turn to contaminated water sources. The findings, published in the journal Surveys in Geophysics underscore the urgent need for sustainable water management practices and further research into the impacts of climate change on freshwater resources.
Research Shows Temporary Cognitive Changes in Space-Traveling Astronauts
NASA scientists have found that while astronauts' cognitive performance is affected during long-duration space missions, the changes are not permanent. Working with 25 astronauts who spent an average of six months on the International Space Station (ISS), researchers discovered that processing speed, working memory, and attention slowed down, but accuracy remained unaffected. These cognitive changes did not persist long-term, suggesting that extended space missions do not lead to significant brain damage. This research provides valuable insights for future deep-space missions, including trips to the moon and Mars. The research was published in the journal Frontiers in Physiology.
NASA's Europa Clipper Begins Scientific Investigations En Route to Jupiter, Instruments Deployed
An artist’s concept of NASA’s Europa Clipper shows the spacecraft in silhouette against Europa’s surface, with the magnetometer boom fully deployed at top and the antennas for the radar instrument extending out from the solar arrays. (Credit: NASA/JPL-Caltech)
NASA's Europa Clipper spacecraft, launched on October 14, 2024, is en route to Jupiter's moon Europa. Recently, the probe successfully deployed two critical science instruments: the magnetometer boom and several radar antennas. These instruments will help scientists study Europa's subsurface ocean by measuring the moon's magnetic field and ice shell thickness. The spacecraft, traveling at 22 miles per second, will perform gravity assists around Mars and Earth before reaching Jupiter in 2030. The mission aims to determine if Europa's ocean has the conditions necessary to support life.
This animation shows how the boom of Europa Clipper’s magnetometer deployed — while the spacecraft was in flight — to its full length of 28 feet (8.5 meters). (Credit: NASA/JPL-Caltech)
Rapid Colonization of Ryugu Asteroid Sample by Earth Microorganisms: Imperial College
An animation of asteroid Ryugu with images from JAXA's Hayabusa2 mission. (Credit: JAXA/University of Tokyo/Kochi University/Rikkyo University/Nagoya University/Chiba Institute of Technology/Meiji University/University of Aizu/AIST)
Scientists at Imperial College London studying a sample from asteroid Ryugu, returned by Japan's Hayabusa2 mission, discovered that it was rapidly colonized by terrestrial microorganisms despite stringent contamination controls. The sample, analyzed under strict laboratory conditions, showed signs of filamentous microorganisms, likely bacteria, which appeared within a week of exposure to Earth's atmosphere. This finding underscores the resilience of Earth-based life and the challenges of preventing contamination in space missions. Enhanced protocols may be necessary for future sample-return missions to ensure the integrity of extraterrestrial materials. The research was published in the journal Meteoritics & Planetary Science
Electron microscope images of sample A0180. (a) A backscattered electron image (BEI) showing a matrix dominated by phyllosilicate with framboidal (fM) and spheroidal (sM) magnetite, dolomite (D), and sulfide (S). Areas containing abundant organic matter (OM) are present. (b) A BEI of rods and filaments (RF) on the surface of the specimen. (c) A secondary electron image (SEI) showing the detailed morphology of filaments with indents denoting individual cells. (d) A SEI of the cavity shown containing an organic rod structure. (e) A BEI showing cluster of rods and filaments around a dolomite grain. A cylindrical mold (MD) is also present. (f) A carbon Kα map of the image shown in e illustrating that filaments are carbon-rich (RF) and showing a C-rich rim on the dolomite grain. (g) A secondary electron image showing highly elongate filaments. (i) A BEI of a dolomite grain surrounded by matrix containing abundant organic matter. A cluster of filaments is also present. Images were obtained on the November 11, 2022 (a–d), November 30, 2022 (g, h), and the January 14, 2023 (e, f). (Credit: Genge et al, 2024)
Images captured by Japan's Hayabusa2 spacecraft show bright S-type rocks that contrast sharply with the darker material composing most of asteroid Ryugu. (Credit: 2020 Tatsumi et al.)
Researchers Develop Space Lasers Using Bacterial Photosynthesis
Researchers are exploring the use of photosynthetic bacteria to develop a new generation of space-borne lasers. The APACE project, led by Heriot-Watt University, aims to replace heavy and complex solar arrays with bacterial photosynthetic structures. This innovative approach could provide a sustainable, low-mass power source for satellites, potentially extending their lifespans and reducing launch costs. Early tests have shown promise, and the project is now moving towards simulated space conditions to further validate the concept.
China Announces Timeline for BeiDou Positioning and Navigation System Upgrade Amid Radar Satellite Launch & Rocket Debut
China is set to develop and deploy its next-generation BeiDou Navigation Satellite System and high-resolution Earth observation system by 2035. Three experimental satellites for this navigation system are slated for launch around 2027. The network deployment will commence around 2029 and is expected to be fully operational by 2035.
One of China’s biggest rockets Chang Zheng 3B/E successfully launched the Beidou-3 G4 payload into the GEO in May 2023. (Credit: via nasaspaceflight.com)
BeiDou, like GPS and other European and Russian systems, supports global civilian applications (driving, aviation, maritime navigation) and sectors (industry, agriculture, finance). It also serves military uses, including precision munitions, UAVs, and battlefield navigation. China currently operates a global BeiDou navigation system consisting of 30 satellites. This system includes 24 satellites in medium Earth orbits, divided into three orbital planes with eight satellites each, excluding backups. Additionally, there are three BeiDou satellites in inclined geosynchronous orbits and three in geostationary orbits, providing comprehensive positioning, navigation, and timing services worldwide. On the other hand, China also plans to retrieve Martian samples around 2031 through its Tianwen 3 mission, aiming to search for life signatures on the red planet.
Meanwhile, on November 24, 2024, China launched a pair of SuperView Neo-2 radar satellites using a Long March 2C rocket from the Jiuquan Satellite Launch Center. These high-resolution synthetic aperture radar (SAR) satellites are part of a larger constellation aimed at enhancing natural resource management, city security, emergency response, and maritime operations.
Additionally, on November 30, 2024, China debuted its first Long March 12 rocket from the newly established Wenchang Commercial Space Launch Site. This two-stage rocket, capable of carrying significant payloads to low Earth orbit (LEO) and sun-synchronous orbit (SSO), marks a milestone in China's efforts to increase its launch frequency and support its lunar exploration plans.
Studying How AI Communicates Could Aid in Talking with Aliens
Researchers propose that studying how AI agents develop their own languages could simplify future communication with extraterrestrial life. This research involves giving AI simple tasks requiring communication, allowing scientists to observe the evolution of AI languages. By studying these emergent languages, scientists aim to gain insights into how languages evolve, potentially aiding in deciphering alien languages. The researchers believe that AI language development mirrors natural language evolution, providing a model for understanding alien communication.
This approach could prove crucial for humanity's efforts to communicate with alien civilizations, offering a systematic method to decode and understand potential extraterrestrial languages. This interdisciplinary research combines insights from linguistics, AI, and astrobiology, highlighting the potential of AI as a tool for exploring one of humanity's greatest mysteries: the possibility of intelligent extraterrestrial life. Read about the research in detail in this The Conversation article, written by Olaf Lipinski, PhD Student in Artificial Intelligence, University of Southampton
GOVERNANCE
FAA Updates Starship Environmental Review as SpaceX Nears Increased Launches and FCC’s conditional approval Direct-to-Smartphone Service
The U.S. Federal Aviation Administration (FAA) has recently updated its environmental review for SpaceX's Starship vehicle, bringing the company one step closer to increasing its launch rate from Texas. The updated draft environmental assessment examines the impacts of up to 25 launches and landings per year at SpaceX's Starbase test site in Boca Chica, Texas. The FAA has concluded that the proposed increase conforms to prior environmental documentation and does not present significant new environmental impacts. The public comment period for this assessment will run through January 17, 2025, with several public meetings scheduled to gather input.
On Nov. 17, the propellant load test and preflight checkouts were finalized in preparation for Starship's sixth flight test scheduled for Nov. 19. (Credit: SpaceX)
Meanwhile, SpaceX has received conditional approval from the Federal Communications Commission (FCC) for its proposed direct-to-smartphone service. This service aims to provide high-speed internet access directly to users' smartphones without the need for additional hardware. The conditional approval is contingent upon SpaceX meeting certain regulatory requirements and demonstrating that the service will not interfere with other communications systems. The company's plans for increased launch cadence and new communication services are expected to influence the future of space exploration and telecommunications..
Space Tech Expo Panel Addresses Growing Space Debris Challenge, Threat Demands Better Data and Regulation
The growing threat of space debris requires better data, innovation, and regulation, according to experts at the Space Tech Expo Europe in Bremen. Participants, including representatives from Astroscale, Neuraspace, and Look Up Space, emphasized the need for improved sensor capabilities, economic incentives, and new technologies to address the issue. With approximately one million objects between 1 cm and 10 cm orbiting Earth, the risk of collisions is increasing, particularly in low Earth orbit (LEO).
Major orbital fragmentation events since June 2024. (Credit: SpaceNews)
The International Space Station (ISS) has conducted multiple collision avoidance maneuvers, underscoring the urgency. Experts stressed the importance of filling data gaps and enhancing space situational awareness. Additionally, they called for regulatory frameworks to keep pace with the rapid growth in orbital activity, ensuring sustainable space exploration. Collaboration between governments, industry, and international bodies is crucial to developing effective solutions to the space debris problem.
Space Firms Anticipate Shifts in Government Contracting Under New Administration
The incoming Trump administration's close ties to tech billionaires like Elon Musk could disrupt traditional Pentagon procurement practices, according to space and defense industry executives at the Baird Defense & Government Conference in McLean, Virginia. The established defense contractor ecosystem might face competition from newer, tech-focused players as the administration promotes a "cost minus" model, challenging the traditional "cost plus" approach. Vice President-elect JD Vance's background as a venture capitalist, including investments in defense and space tech company Anduril Industries, exemplifies these connections. Experts anticipate more budgets shifting from legacy programs to newer space firms, though significant challenges remain in aligning commercial innovation with military procurement.
Anduril plans to establish a new defense manufacturing facility focused on producing autonomous weapons systems. (Credit: Anduril Industries)
MILITARY
SpaceX Launches Next-Gen US Spy Satellites
On November 30, SpaceX launched its fifth mission for the U.S. National Reconnaissance Office's (NRO) proliferated spy satellite constellation from Vandenberg Space Force Base in California. The Falcon 9 rocket carried an unspecified number of government satellites and 20 Starlink internet satellites. This mission, known as NROL-126, is part of the NRO's strategy to rapidly deploy numerous smaller satellites designed for capability and resilience.
Credit: NRO
The NRO expects to enhance timeliness of access, diversify communications pathways, and improve resilience by delivering data in minutes or even seconds. The Falcon 9's first stage booster successfully landed on a drone ship in the Pacific Ocean, marking the first flight for this particular booster. This launch underscores the growing collaboration between SpaceX and the NRO, as well as the increasing importance of satellite constellations in national security and global communications.
Space Force Awards Raytheon $196.7 Million Contract Extension for GPS System Upgrade
The U.S. Space Force has awarded Raytheon a $196.7 million contract extension for the Global Positioning System Next Generation Operational Control System (OCX), a critical upgrade to the GPS infrastructure. This contract, announced on November 27, aims to deliver the next software upgrade by November 2025. The OCX program, which has faced significant delays, seeks to modernize GPS ground control infrastructure to enhance navigation signal accuracy and cybersecurity for both military and civilian applications. The program has been delayed by approximately seven years, with the original delivery slated for 2018. The Space Force has relied on interim software from Lockheed Martin during this period. The Government Accountability Office has flagged these delays as risks to the GPS enterprise.
COMMERCIAL
China's Landspace Deploys Satellites on Fourth Flight with Enhanced Zhuque-2E
The first Zhuque-2E rocket lifts off from Jiuquan in the Gobi Desert on Nov. 27 (UTC), 2024. (Credit: Landspace)
Blue Arrow Aerospace Technology Corp, a Chinese launch startup, doing business as Landspace, , has successfully placed two satellites into orbit with the enhanced Zhuque-2E rocket on November 27, 2024. The launch, from the Dongfeng Commercial Space Innovation Test Area at Jiuquan Satellite Launch Center, one failure and two successess later, marks the fourth flight of the Zhuque-2 series. The improved rocket features advanced engines and a common bulkhead tank structure, enhancing its payload capacity to 4,000 kg for sun-synchronous orbit.
US NOAA Awards Contract to Slingshot Aerospace for Design of Space Traffic System User Experience
Slingshot Aerospace, a California (U.S.)-based space tracking and analytics company, has has secured a $5.3 million contract from the National Oceanic and Atmospheric Administration’s (NOAA) Office of Space Commerce to design the user experience for the Traffic Coordination System for Space (TraCSS). This next-generation platform aims to modernize U.S. space traffic management for civil and commercial satellites. The 12-month contract includes options for four additional years, potentially bringing the total value to $13.3 million. Slingshot will integrate its proprietary Beacon software to enhance satellite operators' capabilities for real-time information sharing and maneuver coordination. The TraCSS system is expected to be operational by late 2025, ahead of the migration from the Department of Defense’s legacy system.
An instance of Slingshot Aerospace's Beacon space traffic coordination platform, which is providing the foundation for the TraCSS presentation layer. (Credit: Slingshot Aerospace)
ESA Awards $36.5M Contract to Open Cosmos for NanoMagSat Mission
The European Space Agency (ESA) has awarded a contract to Open Cosmos to develop the NanoMagSat mission, which aims to study the Earth's magnetic field and ionosphere. The contract, worth 34.6 million euros ($36.5 million), covers the development, launch, and commissioning of three 16U cubesats. The satellites will operate at an altitude of 545 kilometers, with two in 60-degree inclined orbits and one in a polar orbit. The first satellite is scheduled for launch in late 2027, with the remaining two following in 2028. This mission is part of ESA's Scout program, designed to leverage commercial development processes for cost-effective and agile missions. The data collected will enhance understanding of the Earth's magnetic field and contribute to space weather studies.
NASA Selects SpaceX Falcon Heavy for 2028 Dragonfly Mission to Titan
NASA has selected SpaceX to provide launch services for its Dragonfly mission, a rotorcraft lander designed to explore Saturn's largest moon, Titan. The mission, part of NASA's New Frontiers Program, aims to sample materials and determine surface composition in various geologic settings to advance the search for the building blocks of life. The Dragonfly rotorcraft, powered by a radioisotope thermoelectric generator, will navigate Titan's unique, organic-rich environment, which includes a dense atmosphere and swamp-like surface, for about 2.5 Earth years.
Artist’s concept of Dragonfly soaring over the dunes of Saturn’s moon Titan. (Credit: NASA/Johns Hopkins APL/Steve Gribben)
The $3.35 billion mission is set to launch between July 5-25, 2028, aboard a SpaceX Falcon Heavy rocket from Kennedy Space Center's Launch Complex 39A in Florida. The contract, valued at approximately $256.6 million, covers launch services and other mission-related costs. Dragonfly's scientific payload will investigate the moon's habitability, prebiotic chemistry, and potential signs of past life, making it a groundbreaking step in planetary exploration.
Astroscale Nears Key Design Milestone for OneWeb De-Orbit Mission
The British subsidiary of Japan's Astroscale, is gearing up for a critical design review early next year for its ELSA-M (End-of-Life Services by Astroscale-Multiple) program. This mission aims to capture and de-orbit a defunct OneWeb broadband satellite from low Earth orbit (LEO) in 2026. The 500-kilogram servicer is currently undergoing testing and checkout in a "flatsat" phase, where its components are laid out for evaluation.
The mission is a collaborative effort involving Astroscale, Eutelsat's OneWeb, the UK Space Agency, and the European Space Agency, aiming to make space more sustainable. The servicer will use a capture mechanism compatible with magnetic docking plates on OneWeb's satellites. After finalizing algorithms and completing the design review, Astroscale plans to integrate the subsystems in 2025, with a launch likely in the second quarter of 2026.
Astroscale aims to become the pioneer commercial enterprise to successfully capture and de-orbit a spacecraft. (Credit: Astroscale)
Astroscale's ELSA-M builds on the ELSA-d demonstration, which successfully released and recaptured a small satellite in 2021. However, ELSA-d faced challenges when it lost half its thrusters, preventing a controlled descent. The upcoming ELSA-M mission aims to overcome these hurdles and pave the way for a commercial de-orbit business.
Firefly Announces January Launch for Blue Ghost Lunar Lander
Firefly Aerospace's Blue Ghost lunar lander during development and testing. (Credit: Firefly Aerospace)
Firefly Aerospace has announced a January 2025 launch date for its Blue Ghost lunar lander, marking the company's first lunar mission. The spacecraft, which recently completed environmental testing at NASA's Jet Propulsion Laboratory, will launch on a SpaceX Falcon 9 rocket from Florida. The mission, dubbed "Ghost Riders in the Sky," will carry 10 NASA payloads as part of the Commercial Lunar Payload Services (CLPS) program. The lander is set to touch down near Mons Latreille in Mare Crisium on the moon's northeastern near side. The mission will last approximately 60 days, including a 45-day transit to the moon. Firefly's CEO, Jason Kim, expressed confidence in the team's ability to successfully complete the mission despite the challenges ahead. This follows Firefly's historic achievement in February 2024 when its Odysseus spacecraft became the first private spacecraft to land on the moon, marking the first U.S. moon landing since 1972.
Bulgarian EnduroSat to Integrate 100 Enpulsion Propulsion Systems in Future Satellites
Bulgarian microsatellite specialist EnduroSat has ordered 100 electric propulsion systems from Austria's Enpulsion, responding to the growing demand for larger spacecraft. The propulsion systems will be integrated as standard for satellites measuring 6U and larger, enhancing their capabilities and operational life. The first 30 systems are expected to be delivered within the next year, with some arriving by the end of 2024. This move aligns with the industry trend towards more capable satellites, driven by falling launch prices.
Russia Seeks to Build Spaceports in Algeria, South Africa, Zimbabwe
Russia has offered to build spaceports in several African nations, including Algeria, South Africa, and Zimbabwe, according to Roscosmos head Yury Borisov. The proposal aims to leverage the Earth's rotational velocity near the equator, enhancing payload capacity and reducing fuel requirements for launches.
Today, among the main partners, we can probably name countries such as India, China, Iran. We have big plans with South Africa, with a number of African countries, with Algeria, Zimbabwe, with Indonesia, with Malaysia.
Angara rocket installed on the launch pad in the Vostochny Cosmodrome. (Credit: Roscosmos)
This move is part of Russia's strategy to diversify its services and strengthen cooperation with friendly nations in Africa and Southeast Asia. Recent agreements with African countries for satellite development and space exploration underscore Russia's expanding footprint on the continent.
SPOTLIGHT
Astronomers Trace Mysterious, Record-Breaking Energy Bursts to Binary Star System
Astronomers from the Curtin University (Australia) node of the International Centre for Radio Astronomy Research (ICRAR) have identified the source of a mysterious, long-period radio transient named GLEAM-X J0704-37. Detected in archival data from the Murchison Widefield Array (MWA), this energy burst occurs every three hours and lasts 30-60 seconds, making it the longest-period radio transient ever recorded. A radio transient is a brief burst of radio waves that can last from a fraction of a second to several minutes. The team pinpointed the radio waves to one specific star using the MeerKAT telescope in South Africa and confirmed it was an 'M dwarf' with the SOAR observatory in Chile, located 5,000 light-years away in the Puppis constellation. This finding, however, raised questions as M dwarfs alone couldn't generate the observed energy levels. Their data suggests the M dwarf is in a binary system with a white dwarf, together powering the radio emission.
Associate Professor Natasha Hurley-Walker explained that the discovery was made possible by the less crowded region of space where the transient was found, allowing the team to pinpoint its source. The team used multiple radio telescopes, including the MeerKAT telescope in South Africa and the Southern Astrophysical Research (SOAR) Telescope observatory in Chile, to trace the radio waves to the specific star system. This research was published in the Astrophysical Journal Letters.
Nearby Supernova Could Offer Potential Breakthrough in Dark Matter Discovery
Astrophysicists at the University of California, Berkeley, propose that a nearby supernova could potentially end the long-standing search for dark matter. They suggest that axions, a leading candidate for dark matter, could be detected within seconds of observing gamma rays from such an explosion. During the initial 10 seconds after a massive star collapses into a neutron star, axions would be generated in vast quantities and transformed into high-energy gamma rays by the star's intense magnetic field.
An artist's concept of a highly magnetized neutron star. According to current theory, axions would be created in the hot interior of the neutron star. UC Berkeley astrophysicists say that the strong magnetic field of the star will transform these axions into gamma rays that can be detected from Earth, pinpointing the mass of the axion. (Credit: Casey Reed, courtesy of Penn State CC BY-NC 3.0)
After a hot, compact neutron star forms from the collapsed iron core of a massive star, axions should be produced in immense quantities for about 10 seconds. Some of these axions (a, red dotted line) will be converted into gamma rays in the intense magnetic field of the star. A fleet of gamma-ray telescopes around Earth could detect these gamma rays, confirming the existence of axions and pinpointing the mass. (Credit: Benjamin Safdi, UC Berkeley)
Supernovae are powerful explosions that occur at the end of a star's life cycle, often resulting in neutron stars, which are dense stellar remnants composed primarily of neutrons. The challenge lies in the rarity of nearby supernovae and the need for precise alignment of the Fermi Gamma-ray Space Telescope. The last nearby supernova, 1987A, was not detected with sufficient sensitivity, but modern telescopes could change that. A successful detection would pinpoint the axion's mass, while a lack of detection would narrow down the search parameters significantly. The research was published in the journal Physical Review Letters.
An artist's animation of cosmic dust re-forming or growing rapidly in the wake of powerful blast waves from supernova 1987A. (Image credit: NASA/SOFIA/Symbolic Pictures/The Casadonte Group)
Unusual Dwarf Galaxy Grouping Challenges Standard Dark Matter Model
Astronomers from Yonsei University in Seoul, South Korea, and other institutions have discovered a rare group of five star-forming dwarf galaxies, designated D1 to D5, aligned in a near-straight line about 117 million light-years away. This discovery, based on data from the Sloan Digital Sky Survey (SDSS), challenges the cold dark matter (CDM) theory, which predicts disordered galaxy groupings. The galaxies share a common rotational direction, suggesting they formed from the same gas clump. Dwarf galaxy D2 is the most massive member with a stellar mass of 275 million solar masses, while D4 is the least massive at 14.7 million solar masses. The group's dynamical mass is estimated at 60.2 billion solar masses. Dynamical mass is a measure of the total mass within a system that influences the motion of objects within it. It includes not only the visible matter, like stars and gas, but also dark matter, which is inferred from the gravitational effects it has on visible objects.
D1, D2 and D5 have a common direction of rotation, challenging predictions made by the conventional cold dark matter (CMD) model. The g − r − z combined color image cut-out of the system obtained from the Legacy survey viewer page. The five member dwarf galaxies are designated, with their redshift information. (Credit: Paudel et al., 2024)
This observation supports the warm dark matter (WDM) theory, which proposes that dark matter particles are less massive and move faster than those in the CDM model. The discovery, made using data from the Dark Energy Spectroscopic Instrument (DESI), could provide new insights into galaxy formation and the nature of dark matter. Study lead author Sanjaya Paudel of Yonsei University in South Korea noted, "Why do they have the same rotation? They must have a connection with each other — that would be a very strong question that cannot be explained by the ΛCDM model." The research paper was published in The Astrophysical Journal Letters.
New Theory Proposes Hypervelocity Stars as Alien-Propelled Objects
A new paper is exploring the possibility that the fastest-moving stars in the galaxy, known as hypervelocity stars, could be propelled by advanced extraterrestrial civilizations. Clement Vidal, a philosopher at Vrije Universiteit Brussels, suggests that these stars might be part of binary systems where one star is a neutron star and the other a low-mass companion. By manipulating the companion star, an advanced civilization could create thrust, moving the entire system across the galaxy. The idea involves using powerful magnetic fields or gravitational interactions to transfer angular momentum, thereby propelling the binary star system.
The top panels show the Binary Stellar Engine (BSE) in different configurations, with the top being the direction of travel. (a) The BSE is in acceleration mode. (b) the BSE is steering to the left. (c) the BSE is decelerating. (d) is a side view that shows changes in the orbital plane by asymmetric heating of the companion, which creates a lifting force in relation to the orbital plane. The binary separation is not to scale. (Credit: Vidal et al. 2024)
Artist’s impression of a so-called “Black Widow” pulsar PSR B1957+20 (seen in the background) through the cloud of gas enveloping its brown dwarf star companion. (Credit: Dr. Mark A. Garlick; Dunlap Institute for Astronomy & Astrophysics, University of Toronto)
This concept, termed the "Spider Stellar Engine," proposes that such civilizations could use their stars as natural spaceships. Hypervelocity stars travel at speeds of several hundred kilometers per second, far exceeding typical stellar velocities. The "Spider Stellar Engine" could provide a novel perspective on interstellar travel and challenge traditional notions of alien life and technological capabilities. While the idea remains speculative and unproven, it opens new avenues for understanding the potential reach and influence of advanced civilizations in the cosmos.
Astronomers at the University of California, Berkeley, have discovered unusual, Earth-sized dark ovals in the polar haze of Jupiter, visible only in ultraviolet light. These ovals, appearing more frequently at the south pole, are thought to be caused by magnetically driven vortices in Jupiter's ionosphere. The dark UV ovals, embedded in layers of stratospheric haze, absorb more UV light than their surroundings, making them appear dark in Hubble Space Telescope images. This discovery, reported in the journal Nature Astronomy, suggests that unusual processes are occurring in Jupiter's strong magnetic field, propagating down to the poles and deep into the atmosphere. The findings offer new insights into Jupiter's atmospheric dynamics and the planet's powerful magnetic field.
An artificially colored view of Jupiter observed in ultraviolet light. In addition to the Great Red Spot, which appears blue, another oval feature can be seen in the brown hood or cap of hydrocarbon haze at Jupiter's south pole. The oval, an area of concentrated haze, is possibly the result of mixing generated by a vortex higher up in the planet's ionosphere. The edge of the north polar hood is visible at the top. (Credit: Troy Tsubota and Michael Wong, UC Berkeley)
UV Dark Oval (UDO) in the south polar hood of Jupiter. Main image, 225 nm (R), 275 nm (G) and 343 nm (B) data were used for the composite. The bands were balanced to maximize the visibility of the dark oval. a), NUDO observed by Cassini in 2000, showing the main auroral oval (dashed) and the 60° N planetocentric latitude circle (solid). b), Steps in data preparation and analysis (Methods). (Credit: Tsubota et al, 2024; Panel a reproduced with permission from Porco, et al, 2003)
Advanced Simulations Propose New Model for Origins of Martian Moons
A simulation of the paths of fragments of an asteroid ripped apart by Mars' gravity. (Credit: NASA Ames/Durham University)
Astronomers at NASA and Durham University have proposed a new theory for the formation of Mars's moons, Phobos and Deimos, using supercomputer simulations. The study suggests that an asteroid passing near Mars could have been ripped apart by the planet's strong gravitational pull, creating rocky fragments that eventually formed the moons. This new model challenges the previous theories that suggested the moons were either captured asteroids or formed from a giant impact on Mars. The simulations revealed that the debris from the disrupted asteroid would coalesce over time, leading to the formation of the two moons. The research was published in the journal Icarus.
New Theory Explains Zebra Pattern in Crab Nebula Pulses
This Hubble image offers the most detailed view of the Crab Nebula, one of the most studied astronomical objects. It’s the largest image ever taken with Hubble's WFPC2 camera, assembled from 24 exposures, and represents the highest resolution image of the nebula. (Credit: NASA, ESA and Allison Loll/Jeff Hester (Arizona State University). Acknowledgement: Davide De Martin (ESA/Hubble))
A theoretical astrophysicist from the University of Kansas, Mikhail Medvedev, has proposed a solution to the nearly two-decade-old mystery of the Crab Nebula's "zebra" pattern. This pattern, observed in high-frequency radio pulses from the Crab Pulsar, features unusual band spacing in the electromagnetic spectrum. Medvedev's study, recently published in Physical Review Letters, uses wave optics to gauge the density of the pulsar's plasma. By analyzing the fringe pattern in the electromagnetic pulses, he established a method to understand the plasma density variations caused by the neutron star's magnetic field. This breakthrough provides insights into the unique high-frequency interpulse, ranging between 5 and 30 gigahertz, and its stability and high polarization. The findings could help unravel other astronomical puzzles and enhance our understanding of neutron stars.
Medvedev modeled wave diffraction off a circular reflecting region with radially varying index of refraction outside of it to better understand the Crab Nebula’s zebra pattern. (Credit: Mikhail Medvedev)
This composite image of the Crab Nebula combines data from four different telescopes: X-rays from Chandra X-ray Observatory (blue), optical light from Hubble Space Telescope (red), infrared light from Spitzer Space Telescope (yellow), and radio waves from Very Large Array (purple). (Credit: X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Infrared: NASA/JPL/Caltech; Radio: NSF/NRAO/VLA; Ultraviolet: ESA/XMM-Newton)
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