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SpaceX is set to launch four people into space Wednesday on a three-day mission that is the first to orbit the Earth with exclusively private citizens on board, as Elon Musk’s company enters the space tourism fray.

The Inspiration4 mission caps a summer that saw billionaires Richard Branson and Jeff Bezos cross the final frontier, on Virgin Galactic and Blue Origin spaceships respectively, a few days apart in July.

The SpaceX flight has been chartered by American billionaire Jared Isaacman, the 38-year-old founder and CEO of payment processing company Shift4 Payment. He is also a seasoned pilot.

The exact price he paid SpaceX hasn’t been disclosed, but it runs into the tens of millions of dollars.

The mission itself is far more ambitious in scope than the few weightless minutes Virgin Galactic and Blue Origin customers can buy.

The SpaceX Crew Dragon will be flying further than the orbit of the International Space Station.

“The risk is not zero,” said Isaacman in an episode of a Netflix documentary about the mission.

“You’re riding a rocket at 17,500 miles (28,000 kilometres) per hour around the Earth. In that kind of environment there’s risks.”

SpaceX has already given no fewer than ten astronauts rides to the ISS on behalf of NASA – but this will be the first time taking non-professional astronauts.

Lift-off is scheduled for Wednesday from 8:00 pm Eastern Time (5:30am IST) from launch pad 39A, at NASA’s Kennedy Center in Florida, from where the Apollo missions to the Moon took off.

‘Are we going to the Moon?’

In addition to Isaacman, who is the mission commander, three non-public figures were selected for the voyage via a process that was first advertised at the Super Bowl in February.

Each crew member was picked to represent a pillar of the mission.

The youngest, Hayley Arceneaux, is a childhood bone cancer survivor, who represents “hope.”

She will become the first person with a prosthetic to go to space.

“Are we going to the Moon?” she asked, when she was offered her spot.

“Apparently people haven’t gone there in decades. I learned that,” she laughed, in the documentary.  

The 29-year-old was picked because she works as a Physician Assistant in Memphis for St. Jude’s Hospital, the charitable beneficiary of Inspiration4.

One of the donors secured the seat of “generosity”: Chris Sembroski, 42, is a former US Air Force veteran who now works in the aviation industry.

The last seat represents “prosperity” and was offered to Sian Proctor, a 51-year-old earth science professor who, in 2009, narrowly missed out on becoming a NASA astronaut.

She will be only the fourth African American woman to go to space.

Months of training

The crew’s training has lasted months and has included experiencing high G force on a centrifuge – a giant arm that rotates rapidly.

They have also gone on parabolic flights to experience weightlessness for a few seconds and completed a high altitude, snowy trek on Mount Rainier in the northwestern United States.

They spent time at the SpaceX base, though the flight itself will be fully autonomous.

Over the three days of orbit, their sleep, heart rate, blood, and cognitive abilities will be analysed.

Tests will be carried out before and after the flight to study the effect of the trip on their body.

The idea is to accumulate data for future missions with private passengers.  

The stated goal of the mission is to make space accessible for more people, although space travel remains for the moment only partially open to a privileged few.

“In all of human history, fewer than 600 humans have reached space,” said Isaacman.

“We are proud that our flight will help influence all those who will travel after us.”


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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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