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The Sun is heading toward solar maximum (which is likely to be about a year away) and as it does‚ there will be more sunspots‚ solar flares and coronal mass ejections. Over the last 24 hours there has been three‚ yes three X-class flares‚ the first peaking at X1.9‚ the second 1.7 and the final one a mighty 6.3. Flares of this magnitude caused radio blackouts‚ disruption to mobile phones and radio transmissions.   The solar cycle is an 11 year recurring pattern of activity that is driven by the Sun’s magnetic field. The cycle begins with solar minimum with low levels of sunspot activity focussed mostly around the polar regions. This is followed by solar maximum with the increased sunspot activity that has migrated toward the lower latitudes. The cycle drives space weather too which is an outflow of charged particles from the Sun. Any increase or outbursts there can be an impact on satellites‚ radio communications and even the climate.  Sunspots captured by NASAs Solar Dynamic Observatory Among the different manifestations of solar activity‚ some of the most powerful are the solar flares. They vary in size and intensity and are caused by a sudden release of magnetic energy. They are powerful emitters of ultraviolet and X-ray radiation and can produce particles energetic enough to be hazardous to astronauts‚ spacecraft and their systems. Teams of scientists study solar flares to help understand their nature and behaviour. Doing so may help to find ways to limit their impact on our technology and space exploration. The most powerful of the flares are the X-class flares.  These X-class flares are classified according to their peak X-ray levels within the 1 to 8 Angstroms (1 angstrom = 10-10 metres). The scale used typically spans from X1-X9 with each letter depicting a tenfold rise in intensity.  An X2 flare for example is twice as intense as an X1 flare and an X3 flare‚ ten times stronger than X2 and so it goes on. On rare occasions‚ flares can exceed X10 but this is a rare event indeed.  Sunspot region 3590‚ which is at a relatively high solar latitude‚ has generated to X-class events. The initial flare reached its peak at X1.9 followed a few hours later by an X1.7 flare. Both of these flares resulted in a brief radio blackout on the day time side of Earth.  It seems that just like busses‚ solar flares are few and far between then three come along all at once (this may be a UK joke so apologies to those based elsewhere). The very same sunspot region 3590 has not let us down as it has done it again. This time‚ it peaked at an impressive X6.3. It is also possible that there is a coronal mass ejection related to this flare but we won’t know for a day or two yet. Whilst the solar maximum may be only a year away‚ it seems the Sun has plenty of poke left in it and we may well be in for quite a year.  Source : Two X-class solar flares only 7 hours apart and X6.3 Solar Flare The post The Sun Gets Feisty‚ Throwing Off Three X-Class Flares Within 24 Hours appeared first on Universe Today.

On Wednesday‚ February 21st‚ at 01:40 p.m. PST (04:40 p.m. EST)‚ an interesting package returned to Earth from space. This was the capsule from the W-1 mission‚ an orbital platform manufactured by California-based Varda Space Industries‚ which landed at the Utah Test and Training Range (UTTR). Even more interesting was the payload‚ which consisted of antiviral drugs grown in the microgravity environment of Low Earth Orbit (LEO). The mission is part of the company’s goal to develop the infrastructure to make LEO more accessible to commercial industries. Founded in 2020 by former SpaceX employees and Silicon Valley venture capitalists‚ Varda is part of a burgeoning space industry (aka. NewSpace) that is taking advantage of the declining cost of sending payloads to space. In particular‚ the company’s vision is to develop pharmaceuticals and other products in space and return them to Earth via their proprietary reentry capsules. Traditionally‚ conducting research in microgravity was something that could only be done by astronauts aboard the International Space Station (ISS). Update #6 on Varda's W-1 Mission: pic.twitter.com/BNBqjbRxvX— Varda Space Industries (@VardaSpace) February 21‚ 2024 With the growing accessibility enabled by reusable rockets and rideshare programs‚ the situation is rapidly changing. Many industries are looking to get in on this trend‚ ranging from biomedical and advanced materials research to manufacturing (to name a few). According to Varda‚ the processing in microgravity dramatically alters buoyancy‚ natural convection‚ sedimentation‚ and phase separation. This has the potential to produce high-quality drugs with more perfect crystalline structures due to the absence of gravitational stresses‚ leading to improved shelf life and effectiveness. There’s also the potential that high-hypersonic flight testing has for the development of vehicle subsystems‚ thermal protective materials‚ navigation‚ communication‚ and sensors. As Varga CEO Will Bruey explained in November last year during an interview with Marketplace: “We manufacture pharmaceuticals in space. Removing gravity allows us to make medicines you otherwise couldn’t on Earth. Gravity is kind of like a parameter. If you put a temperature knob on an oven‚ you create a whole world of new recipes and new food you can create. Similarly‚ if you can change gravity‚ you can also change the chemical process for drug formulations.” The W-1 capsule launched in June 2023 atop a SpaceX Falcon 9 rocket as part of the company’s eight dedicated rideshare mission (Transporter-8). It spent the next eight months integrated with a Rocket Lab Photon spacecraft (the upper stage of the Electron rocket) that provided the capsule with power‚ propulsion‚ and navigation. Meanwhile‚ it developed a drug known as Ritonavir‚ an antiviral medication used to treat HIV and hepatitis C. Said Rocketlab CEO Peter Beck in a company statement: “This mission was a phenomenal feat and impressive display of teamwork between the Rocket Lab and Varda teams to develop a unique and highly capable spacecraft‚ successfully demonstrate in-space manufacturing and bring back the capsule and finished pharmaceutical product – all on the first attempt‚” Varda Space’s off-Earth manufacturing capsule is evaluated by recovery personnel at the desert floor of the Utah Test and Training Range (UTTR). Credit: Varda Space/John Kraus Now that the capsule has returned home‚ Varda will transport it back to their facilities in Los Angeles for post-mission analysis while the drug is shipped to their commercial partner. The company is also gearing up for its second launch‚ which will take place this summer and also rely on a Photon spacecraft. As Varda posted on their X page: “The Ritonavir vials onboard the spacecraft will be shipped to our collaborators Improved Pharma for post-flight characterization. Additionally‚ data collected throughout the entirety of the capsule’s flight — including a portion where we reached hypersonic speeds — will be shared with the Air Force and NASA under a contract Varda has with those agencies.” Further Reading: Varda Space Industries The post A Capsule With Antiviral Drugs Grown in Space Returns to Earth appeared first on Universe Today.

I can remember seeing images of SN1987A as it developed back in 1987. It was the explosion of a star‚ a supernova in the Large Magellanic Cloud. Over the decades that followed‚ it was closely monitored in particular the expanding debris cloud. Predictions suggested there may be a neutron star or even a black hole at the core but the resolution of the telescopes was insufficient to pick anything up. Now we have the James Webb Space Telescope and using its more powerful technology‚ signs of a neutron star have been detected.  Supernova are among the most spectacular and intense explosions in the Universe that signal the end of a massive star’s life. They emit vast amounts of energy and radiation and at the moment of explosion‚ their light can exceed that of all the stars in the host galaxy put together.  There are the type II supernova and it is this type of phenomenon that brought 1987A to our skies.  1987A occurred in the Large Magellanic Cloud which is approximately 160‚000 light years away and was first observed in February 1987.  It continued to brighten until its luminosity peaked three months later in May. It even became visible to the naked eye‚ the first since Kepler’s Supernova of 1604. Before the visible light signals were detected‚ three observatories detected short bursts of neutrinos. The bursts were attributed to the supernova and they gave insight into the events leading up to the collapse. Since the event‚ astronomers have been searching for its existence.  Part of the SMASH dataset showing an unprecedented wide-angle view of the Large Magellanic Cloud. Image Credit: CTIO/NOIRLab/NSF/AURA/SMASH/D. Nidever (Montana State University) Acknowledgment: Image processing: Travis Rector (University of Alaska Anchorage)‚ Mahdi Zamani &; Davide de Martin Observations of similar objects‚ like the supernova remnant in Taurus‚ the Crab Nebula ‚ revealed a neutron star at the core of the debris field.  In the years that followed astronomers hunted for evidence but no direct evidence had been found. The James Webb Space Telescope was focussed onto the 1987A remnant in July 2022‚ making it one of the earliest objects observed by Webb. The team used the Medium Resolution Spectrograph (MRS) mode of the Mid-Infrared instrument (MIRI). It was a tool that had been partly developed by the team that were hunting for the 1987A neutron star. MIRI was a wonderful tool that could simultaneously image an object whilst it was obtaining its spectrum! This allowed observers the ability to detect spectroscopic variations across the object while analysing the Doppler shift at various points to assess velocity at each position. Artist impression of the James Webb Space Telescope The team found a strong signal due to ionised argon that seemed to originate from a region around the site of the original 1987A event. Using Webb’s Near-Infrared Spectrograph (NIRSpec) they observed shorter wavelengths and detected even more ionised elements including five times ionised argon (this mean the argon atoms have lost five of their eighteen electrons). For these to be created‚ they required highly energetic photons and these had to come from somewhere.  The conclusion is that their must be some source of high-energy radiation in the centre of the 1987A remnant. Of all the options discussed in their paper‚ lead author Claes Fransson of Stockholm University hints that only a few of the scenarios are likely but they all involve a young energetic neutron star. More observations are now required to follow up on this and probe the heart of the 1987A supernova remnant to see if the neutron star can finally be visually identified.  Source : Webb Finds Evidence for Neutron Star at Heart of Young Supernova Remnant The post Finally! Webb Finds a Neutron Star from Supernova 1987A appeared first on Universe Today.