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The United States will on Wednesday carry a Russian to the International Space Station aboard a SpaceX ship, in a voyage that carries symbolic significance amid the Ukraine war.

Anna Kikina, the only female cosmonaut in service, is part of the Crew-5 mission, which also includes one Japanese and two American astronauts.

Blast-off is set for noon from the Kennedy Space Center, with the weather forecast so far promising.

Two weeks ago, an American astronaut took off on a Russian Soyuz rocket for the orbital platform.

The long-planned astronaut exchange program has been maintained despite soaring tensions between the two countries since Moscow’s invasion of Ukraine in February.

Ensuring the operation of the ISS has become one of the few remaining areas of cooperation between the United States and Russia.

“When you each are flying other’s crew members, you know that you have a huge responsibility that you’re promising to the other country,” NASA associate administrator Kathy Lueders told reporters in a recent press conference.

“At a working level, we really appreciated the constancy in the relationship, even during some really, really tough times geopolitically.”

Fifth female cosmonaut

Kikina, 38 and an engineer by training, will become the fifth Russian female professional cosmonaut to go into space.

“I hope in the near future we have more women in the cosmonaut corps,” the Novosibirsk native told AFP in August.

The Soviet Union put the first woman in space, Valentina Tereshkova, in 1963, nearly 20 years before the first American woman Sally Ride. Since then, America has flown dozens more women.

It will also be the first spaceflight for American astronauts Nicole Mann and Josh Cassada, but the fifth for Japan’s Koichi Wakata.

After a journey of about 30 hours, their ship will dock with the station on Thursday, ready to begin a five-month science mission and relieve the four members of Crew-4, who will stay a few days for handover.

Crew-5’s arrival will bring the total number of astronauts on the ISS to 11, including two other Russians and an American who arrived on the recent Soyuz.

ISS future unclear

Kikina will be the first Russian to fly with Elon Musk’s SpaceX which, along with Boeing, has a “taxi service” contract with NASA.

Musk himself waded into the conflict Thursday by proposing a peace deal that involved re-running, under UN supervision, annexation referendums in Moscow-occupied regions of Ukraine and acknowledging Russian sovereignty over the Crimean peninsula.

The post enraged Ukrainians, including the country’s envoy to Germany, who responded with an expletive.

Tensions between Moscow and Washington have increased considerably in the space field after the announcement of American sanctions against the Russian aerospace industry, in response to the invasion of Ukraine.

Russia thus announced this summer that it wanted to leave the ISS “after 2024” in favor of creating its own station, albeit without setting a precise date.

The director of manned flights at Roscosmos, Sergei Krikaliov, declared Monday he hoped the Russian government agrees to extend participation in the ISS after 2024.

The United States, for its part, wants to continue operating until at least 2030, then transition to commercially run stations.

As things stand, the ISS cannot function without joint cooperation, as the US side is responsible for power and life support and the Russian side for propulsion and maintaining orbit.

Between 2011 — when the Space Shuttle program ended — and SpaceX’s first flight to the ISS in 2020, the United States was dependent on Russia for flying its crew to the station, paying tens of millions of dollars per seat.

The loss of this monopoly represents a significant income reduction for the Russian space program. The current crew exchange program, by contrast, is a barter-based agreement with no exchange of money.


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A Nearby Supernova May End Dark Matter Search, Claims New Study

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A Nearby Supernova May End Dark Matter Search, Claims New Study

The pursuit of understanding dark matter, which comprises 85 percent of the universe’s mass, could take a significant leap forward with a nearby supernova. Researchers at the University of California, Berkeley, led by Associate Professor of Physics Benjamin Safdi, have theorised that the elusive particle known as the axion might be detected within moments of gamma rays being emitted from such an event. Axions, predicted to emerge during the collapse of a massive star’s core into a neutron star, could transform into gamma rays in the presence of intense magnetic fields, offering a potential breakthrough in physics.

Potential Role of Gamma-Ray Telescopes

The study was published in Physical Review Letters and revealed that the gamma rays produced from axions could confirm the particle’s mass and properties if detected. The Fermi Gamma-ray Space Telescope, currently the only gamma-ray observatory in orbit, would need to be pointed directly at the supernova, with the likelihood of this alignment estimated at only 10 percent. A detection would revolutionise dark matter research, while the absence of gamma rays would constrain the range of axion masses, rendering many existing dark matter experiments redundant.

Challenges in Catching the Event

For detection, the supernova must occur within the Milky Way or its satellite galaxies—an event averaging once every few decades. The last such occurrence, supernova 1987A, lacked sensitive enough gamma-ray equipment. Safdi emphasised the need for preparedness, proposing a constellation of satellites, named GALAXIS, to ensure 24/7 sky coverage.

Axion’s Theoretical Importance

The axion, supported by theories like quantum chromodynamics (QCD) and string theory, bridges gaps in physics, potentially linking gravity with quantum mechanics. Unlike neutrinos, axions could convert into photons in strong magnetic fields, providing unique signals. Laboratory experiments like ABRACADABRA and ALPHA are also probing for axions, but their sensitivity is limited compared to the scenario of a nearby supernova. Safdi expressed urgency, noting that missing such an event could delay axion detection by decades, underscoring the high stakes of this astrophysical endeavour.

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

Intelligent extraterrestrial civilisations might be utilising stars as massive interstellar vehicles to explore the galaxy, according to a theory proposed by Clement Vidal, a philosopher at Vrije Universiteit Brussel in Belgium. His research suggests that alien species could potentially accelerate their binary star systems to traverse vast cosmic distances. While such a concept is purely hypothetical and unproven, Vidal’s recent paper, which has not undergone peer review, raises intriguing possibilities about advanced extraterrestrial engineering.

Concept of Moving Star Systems

The study was published in the Journal of the British Interplanetary Society. As per a report by LiveScience, the idea revolves around the notion that alien civilisations, instead of building spacecraft for interstellar travel, might manipulate entire star systems to travel across the galaxy. Vidal highlights binary star systems, particularly those involving neutron stars and smaller companion stars, as ideal candidates. Neutron stars, due to their immense gravitational energy, could serve as anchors for devices designed to propel the system by selectively ejecting stellar material.

Vidal explained in the paper that uneven heating or manipulation of magnetic fields on a star’s surface could cause it to eject material in one direction. This process would create a reactionary thrust, propelling the binary system in the opposite direction. The concept provides a way to travel while preserving planetary ecosystems, making it a theoretically viable method for species reliant on their home systems.

Known Examples with High Velocities

Astronomers have identified hypervelocity stars, such as the pulsars PSR J0610-2100 and PSR J2043+1711, which exhibit high accelerations. While their movements are believed to be natural phenomena, Vidal suggests they could be worth further investigation to rule out potential artificial influences.

This theory adds an unconventional angle to the search for intelligent life, expanding possibilities beyond traditional methods of exploration like searching for signals or probes. The research underscores the importance of considering advanced and unconventional methods aliens might employ to navigate the galaxy.

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

NASA’s Hubble Space Telescope has provided new insights into the young star FU Orionis, located in the constellation Orion. Observations have uncovered extreme temperatures in the inner region of its accretion disk, challenging current models of stellar accretion. Using Hubble’s Cosmic Origins Spectrograph and Space Telescope Imaging Spectrograph, astronomers captured far-ultraviolet and near-ultraviolet spectra, revealing the disk’s inner edge to be unexpectedly hot, with temperatures reaching 16,000 kelvins—almost three times the Sun’s surface temperature.

A Star’s Bright Outburst Explained

First observed in 1936, FU Orionis became a hundred times brighter in months and has remained a unique object of study. Unlike typical T Tauri stars, its accretion disk touches the stellar surface due to instabilities. These are caused by the disk’s large mass, interactions with companion stars, or material falling inwards. Lynne Hillenbrand, a co-author from Caltech, in a statement said that the ultraviolet brightness seen exceeded predictions, revealing a highly dynamic interface between the star and its disk.

Implications for Planet Formation

As per a report by NASA, the study holds significant implications for planetary systems forming around such stars. The report further quoted Adolfo Carvalho, lead author of the study, saying that while distant planets in the disk may experience altered chemical compositions due to outbursts, planets forming close to the star could face disruption or destruction. This revised model provides critical insights into the survival of rocky planets in young star systems, he further added.

Future Investigations on FU Orionis

The research team continues to examine spectral emission lines in the collected data, aiming to map gas movement in the star’s inner regions. Hillenbrand noted that FU Orionis offers a unique opportunity to study the mechanisms at play in eruptive young stars. These findings, published in The Astrophysical Journal Letters, showcase the ongoing value of Hubble’s ultraviolet capabilities in advancing stellar science.

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