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Oral vaccine prevents recurring UTIs for nine years
Oral vaccine prevents recurring UTIs for nine years
NASA’s DC-8 Completes Final Mission, Set to Retire
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Preparations for Next Moonwalk Simulations Underway (and Underwater) The DC-8 aircraft returned to NASA’s Armstrong Flight Research Center Building 703 in Palmdale, California, on April 1, 2024, after completing its final mission supporting Airborne and Satellite Investigation of Asian Air Quality (ASIA-AQ). The aircraft and crew were welcomed back with a celebratory water salute by the U.S. Air Force Plant 42 Fire Department.NASA/Steve FreemanAfter 37 years of successful airborne science missions, NASA’s DC-8 aircraft completed its final mission and returned to the agency’s Armstrong Flight Research Center Building 703 in Palmdale, California, on April 1.
The DC-8 and crew were welcomed back with a celebratory water salute by the U.S Air Force Plant 42 Fire Department after completing an air quality study, the Airborne and Satellite Investigation of Asian Air Quality, or ASIA-AQ mission. The aircraft is set to retire after concluding operations in May.
As the largest flying science laboratory in the world, the DC-8 has been used to support the agency’s Airborne Science mission since 1987. This unique aircraft was first acquired by NASA in 1985 and collected data for experiments in support of scientific projects serving the world’s scientific community – including scientists, researchers, and students from NASA and other federal, state, academic, and foreign institutions.
The DC-8 will continue its educational legacy as it retires to its new home at Idaho State University in Pocatello, Idaho, where it will be used to train future aircraft technicians by providing real-world experience in the college’s Aircraft Maintenance Technology Program.
For more information about the DC-8 aircraft, visit:
https://www.nasa.gov/centers-and-facilities/armstrong/dc-8-aircraft/
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Australia’s Indigenous people were making pottery over 2000 years ago
Australia’s Indigenous people were making pottery over 2000 years ago
A Neutron Star Merged with a Surprisingly Light Black Hole
Galactic collisions, meteor impacts and even stellar mergers are not uncommon events. neutron stars colliding with black holes however are a little more rare, in fact, until now, we have never observed one. The fourth LIGO-Virgo-KAGRA observing detected gravitational waves from a collision between a black hole and neutron star 650 million light years away. The black hole was tiny though with a mass between 2.5 to 4.5 times that of the Sun.
Neutron stars and black holes have something in common; they are both the remains of a massive star that has reached the end of its life. During the main part of a stars life the inward pull of gravity is balanced by the outward push of the thermonuclear pressure that makes the star shine. The thermonuclear pressure overcomes gravity for low mass stars like the Sun but for more massive stars, gravity wins. The core collapses compressing it into either a neutron star or a black hole (depending on the progenitor star mass) and explodes as a supernova – in the blink of an eye.
In May 2023, as a result of the fourth observing session of the LIGO-Virgo-KAGRA (Laser Interferometer Gravitational Wave Observatory-Virgo Gravitational Wave Interferometer and Kamioka Gravitational Wave Detector) network, gravitational waves were picked up from a merger event. The signal came from an object 1.2 times the mass of the Sun and another slightly more massive object. Further analysis revealed the likelihood that one was a neutron star and the other a low mass black hole. The latter falls into the so called ‘mass gap’, more massive than the most massive neutron star and less massive than the least massive black hole.
Interactions between objects can generate gravitational waves. Before they were detected back in 2015, stellar mass black holes were typically found through X-ray observations. Neutron stars on the other hand, were usually found with radio observations. Between the two, was the mass gap with objects lacking between three and five solar masses.
It has been the subject of debate among scientists with the odd object found which fell within the gap, fuelling debate about its existence. The gap has generally been considered to separate the neutron stars from the black holes and items in this mass group have been scarce. This gravitational wave discovery suggests maybe objects in this gap are not so rare after-all.
One of the challenges of detecting mass gap objects and mergers between them is the sensitivity of detectors. The LIGO team at the University of British Columbia researchers are working hard to improve the coatings used in mirror production. Enhanced performance on future LIGO detectors will further enhance detection capabilities. It’s not just optical equipment that is being developed, infrastructure changes are also being addressed including data analysis software too. Improving sensitivity in all aspects of the gravity wave network is sure to yield results in future runs. However for now, the rest of the first half of the observing run needs analysing with 80 more candidate signals to study.
Source : New gravitational wave signal helps fill the ‘mass gap’ between neutron stars and black holes
The post A Neutron Star Merged with a Surprisingly Light Black Hole appeared first on Universe Today.
An Eclipse Is a Moment of Solitude—Even When You’re in a Crowd
Even among hundreds of people, experiencing an eclipse is a joyous solitude
Rural Americans Are Dying at Increasingly Higher Rates Than City Dwellers
The urban-rural mortality rate gap in the U.S. is increasing, especially among young women and Native Americans. Limited access to health care could help explain why
The Seven Most Intriguing Worlds to Search for Advanced Civilizations (So Far)
Sometimes, the easy calculations are the most interesting. A recent paper from Balázs Bradák of Kobe University in Japan is a case in point. In it, he takes an admittedly simplistic approach but comes up with seven known exoplanets that could hold the key to the biggest question of them all – are we alone?
Dr. Bradák starts with a simple premise – there is a chance that life on Earth might have started via panspermia. There is also a case that panspermia was intention – an advanced civilization could theoretically have purposefully sent a biological seed ship to our local solar system to spread life here, essentially from scratch.
With those admittedly very large assumptions in place, Dr. Bradák works out a few characteristics about the planets that could have been the starting point for such a civilization. First, he assumes, as much of the astrobiological community does, that for an advanced civilization to arise on a planet, that planet has to be at least partially covered in an ocean.
Sun-like stars aren’t the only potential hosts for habitable planets, as Fraser discusses here.To meet that requirement, the planet has to be both the right size and the right temperature. The two size categories of exoplanets that Dr. Bradák originally selected were “terrestrial” – planets similar to Earth, including so-called “Super-Earths” – and “sub-Neptunes” – planets that are significantly larger than Earth but smaller than the ice giant in the outer fringes of our solar system.
Any such exoplanet also has to be in the habitable zone of its parent star. That alone dramatically narrows the potential field of planetary candidates. For simplicity’s sake, Dr. Bradák also eliminates sub-Neptunes as a potential planetary class. However, one other factor comes into play as well: age.
We know it took around 4.6 billion years for life to evolve to a point where it could theoretically send objects to other star systems – as we have now with Voyager. Since the original planet would also have to have evolved such a civilization, it would be double the time for its minimum age – or 9.2 billion years old.
The idea of panspermia has been around for decades, as Fraser discusses.Dr. Bradák adds some additional argument that lowers the required age of the system – and he also assumes that the planetary system of a star forms at a similar time gap as our planetary system did. The distance to most of these stars is inconsequential on the scale of billions of years, so the travel time for the seed ship was discounted in this calculation.
After all that pruning, Dr. Bradák turned to NASA’s Exoplanet Archive, which currently contains 5271 known exoplanets. Of those 5271, only 7 meet the specified age, size, and habitable zone placement criteria. In other words, according to our current knowledge of exoplanets and how life evolved, only a few planets could potentially have been the starting point for an intentional panspermia campaign.
One planet in particular stands out – Kepler-452 b, which has a star similar to ours and an orbit similar to ours. That system is only 1,400 light years away, relatively close by astronomical standards. If nothing else, it points to that system as a potentially interesting focal point for exoplanet surveys, including assessments of exoplanet atmospheres. However, we’ll likely have to wait for the next generation of grand telescopes.
For now, this was an interesting, though brief, speculative exercise. Astronomers are always looking for exciting things, and this paper contributes to the arguments about why it’s so important to spend time looking in detail at some of the exoplanets we already know about.
Learn More:
B. Bradák – A BOLD AND HASTY SPECULATION ABOUT ADVANCED CIVILIZATION-BEARING PLANETS
APPEARING IN EXOPLANET DATABASES
UT – A Super-Earth (and Possible Earth-Sized) Exoplanet Found in the Habitable Zone
UT – A New Place to Search for Habitable Planets: “The Soot Line.”
UT – Want to Find Life? Compare a Planet to its Neighbors
Lead Image:
Artist’s illustration of a habitable planet.
Credit – Wikipedia / VP8/Vorbis
The post The Seven Most Intriguing Worlds to Search for Advanced Civilizations (So Far) appeared first on Universe Today.
NASA Astronaut Loral O’Hara to Discuss Space Station Mission
After spending six-and-a-half-months aboard the International Space Station, NASA astronaut Loral O’Hara will participate in a news conference at 10:45 a.m. EDT Monday, April 15, at the agency’s Johnson Space Center in Houston.
The news conference will air live on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media.
Media interested in participating in person must contact the NASA Johnson newsroom no later than 5 p.m. Friday, April 12, by calling 281-483-5111 or emailing: jsccommu@mail.nasa.gov.
Media wishing to participate virtually must contact the newsroom no later than two hours before the start of the event. NASA’s media accreditation policy is available online. Questions may also be submitted on social media by using #AskNASA.
O’Hara launched Sept. 15, 2023, alongside Roscosmos cosmonauts Oleg Kononenko and Nikolai Chub, and returned to Earth April 6 with Roscosmos cosmonaut Oleg Novitskiy and spaceflight participant Marina Vasilevskaya of Belarus. Novitskiy and Vasilevskaya launched with NASA astronaut Tracy C. Dyson to the station aboard the Soyuz MS-25 spacecraft on March 23.
O’Hara completed 204 days in space, 3,264 orbits of the Earth, and 86.5 million miles during her first spaceflight. She witnessed the arrival of eight visiting spacecraft and the departure of seven visiting spacecraft, including both crewed and cargo missions. O’Hara also completed one spacewalk totaling six hours, 42 minutes.
While aboard the orbiting lab, O’Hara conducted dozens of science and technology activities to benefit future exploration in space and life back on Earth. O’Hara is among the first astronauts to participate in CIPHER, or the Complement of Integrated Protocols for Human Exploration Research program, an investigation that studies the psychological and physiological changes humans experience during spaceflight. Collecting data from astronauts on missions of different durations supports the development of ways to protect crew health on long-duration missions to the Moon and Mars.
O’Hara conducted experiments bioprinting cardiac tissues in microgravity which could advance technology for creating replacement organs and tissues for transplant on Earth. She also studied the effects of microgravity on bone marrow mesenchymal stem cells to improve our understanding of the mechanisms behind bone loss and support the development of ways to better protect crew members and people on Earth from its effects.
Get the latest NASA space station news, images, and features on Instagram, Facebook, and X.
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Joshua Finch / Julian Coltre / Claire O’Shea
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / julian.n.coltre@nasa.gov / claire.a.o’shea@nasa.gov
Courtney Beasley
Johnson Space Center, Houston
281-483-5111
courtney.m.beasley@nasa.gov
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What a Swarm of Probes Can Teach Us About Proxima Centauri B
You’ve likely heard of the Breakthrough Starshot (BTS) initiative. BTS aims to send tiny gram-scale, light sail picospacecraft to our neighbour, Proxima Centauri B. In BTS’s scheme, lasers would propel a whole fleet of tiny probes to the potentially water-rich exoplanet.
Now, another company, Space Initiatives Inc., is tackling the idea. NASA has funded them so they can study the idea. What can we expect to learn from the effort?
Proxima b may be a close neighbour in planetary terms. But it’s in a completely different solar system, about four light-years away. That means any probes sent there must travel at relativistic speeds if we want them to arrive in a reasonable amount of time.
That’s why Space Initiatives Inc. proposes such tiny spacecraft. With their small masses, direct lasers can propel them to their destination. That means they must send a swarm of hundreds or even one thousand probes to get valuable scientific results.
This is much different than the architecture that missions usually conform to. Most missions are a single spacecraft, perhaps with a smaller attached probe like the Huygens probe attached to the Cassini spacecraft. How does using a swarm change the mission? What results can we expect?
“We anticipate our innovations would have a profound effect on space exploration.”
Thomas Eubanks, Space Inititatives Inc.A new presentation at the 55th Lunar and Planetary Science Conference (LPSC) in Texas examined the idea. It’s titled “SCIENTIFIC RETURN FROM IN SITU EXPLORATION OF THE PROXIMA B EXOPLANET.” The lead author is T. Marshall Eubanks from Space Initiatives Inc., a start-up developing 50-gram femtosatellites that weigh less than 100 grams (3.5 oz.)
Tiny probes like these can only do flybys. They’re too tiny and low-mass for anything else. When designing a mission like this, the first consideration is whether the probes will operate as a dispersed or coherent swarm. In a dispersed swarm, the probes reach their destination sequentially. In a coherent swarm, the probes are together when they do their flyby. Both architectures have their merits.
In either case, these tiny solar sail probes will be very thin. But thanks to technological advances, they can still gather high-resolution images by working together.
The image below shows 247 probes forming an array as they fly by Proxima b. Together, they have the light-collecting area of a three-meter telescope. This arrangement should enable sub-arc-second resolutions at optical wavelengths. Spectroscopy should be equally as fine.
“While both erosion by the Interstellar Medium (ISM) and image smearing will degrade imaging, we anticipate these systems will enable sub-arcsecond resolution imaging and spectroscopy of the target planet,” the authors write.
This image from the presentation shows how the probe swarm would arrive at Proxima b. (Note that the planned swarm dispersion is much smaller than is indicated here.) Image Credit: Eubanks et al. 2024.These tiny spacecraft could do some course correction, but not much. So, getting the navigation right is critical. Unfortunately, our data on Proxima b’s orbit is not as well-understood as the planets in our own Solar System. It all comes down to ephemeris.
Ephemeris tables show the trajectory of planets and other objects in space. But in Proxima b’s case, the ephemeris error is potentially quite large.
Added to that is the distance. If the probes can travel at 20% of light speed, reaching the planet will take over 21 years. The authors calculate that if they can restrict Proxima b’s ephemeris error to 100,000 km and send 1,000 probes, at least one will come within 1,000 km of the planet. “Meeting this ephemeris error goal will require improved astrometry of the Proxima system,” the authors write.
The probes would perform science observations on their way to Proxima b. As they travel, the swarm would have dozens or even hundreds of opportunities to use microlensing to study stellar objects. A stellar mass microlensing event requiring one month on Earth would only take one hour.
“It is now possible to predict lensing events for nearby stars; BTS probe observations of dozens or hundreds of predicted microlensing events by nearby stars will offer both a means of observing these systems and a novel means of interstellar navigation,” the authors explain.
The swarm would be only the third mission to leave our Solar System. The Voyage spacecraft left the heliosphere, but only inadvertently. So, the swarm could observe the interstellar medium (ISM) during its 20+ year journey. One of the questions we have about the local ISM concerns clouds. We only have poor data on the nature of these clouds, and scientists aren’t certain if our Solar System is in the Local Interstellar Cloud (LIC.)
“In situ observation of the properties of these clouds will be a primary scientific goal for mission science during the long interstellar voyage,” the researchers write.
There are clouds in the ISM near our Solar System. But we don’t know much about them, including if our Solar System is in the LIC or if it’s leaving it. Image Credit: Interstellar Probe/JHUAPLOpportunistic science during the voyage is great, but arrival at Proxima b is the meat of the mission. One day before the probes arrive, they would still be 35 AU away. At that point, the mission could begin imaging. Proxima b would still only be several pixels across, but it’s enough to see any visible moons.
“At this point, it would be worth turning some probes to face forward and begin imaging the Proxima system to search for undiscovered planets, moons and asteroids in the system, and to begin a Proxima b approach video,” the researchers explain.
Upon arrival at Proxima Centauri b, a one-meter aperture telescope 6,000 km away from the planet could attain a six-meter resolution on the surface. That’s an idealistic number, as not all of the planet’s surface could be imaged at that resolution. PCb is also tidally locked to its star, meaning one side is in darkness. Because of that, the mission should be designed to gather low-light and infrared images of the night side. “Night-side illumination imagery might also be the most conclusive technosignature from an initial Proxima mission,” the authors write.
As probes pass through Proxima b’s shadow, they could use the light from the star to perform spectroscopy. Probes passing behind Proxima b could use the Earth laser system for spectrometry, and if the probes are in a coherent swarm, they could use the lasers from pairs of probes on either side of the planet.
“Transmission spectroscopy, which for Proxima b cannot be done from Earth,” the researchers explain, “will likely provide the best means of determining the existence of a biology or even a technological society on Proxima b through the search for the spectral lines of biomarkers and technomarkers.”
As humanity’s first mission to Proxima Centauri b, the swarm would face some hurdles and uncertainties. But in a coherent swarm architecture, the mission could also be almost too successful. “A BTS mission, especially with a coherent swarm, may collect more data than can be returned to Earth,” the authors write. If the data returned has to be selected autonomously by the swarm itself, that could be more demanding than deciding what data to collect in the first place.
Scientists have many questions about Proxima Centauri b. Should the swarm ever be launched, any amount of data it returns will be valuable. Even though it’ll take over four years for the data to be sent back to Earth.
An artist’s conception of a violent flare erupting from the red dwarf star Proxima Centauri. Such flares can obliterate the atmospheres of nearby planets. Credit: NRAO/S. Dagnello.Scientists don’t know how hot the planet is. They’re not certain if it even has liquid water. It looks like the planet is just over one Earth mass and has a slightly higher radius. But those measurements are uncertain. Scientists are also uncertain about its composition. The star it orbits is a flare star, which means the planet could be subjected to extremely powerful bursts of radiation. That’s a lot of uncertainty.
But it’s the nearest exoplanet, the only one we could feasibly reach in a realistic amount of time. That alone makes it a desirable target.
There’s no final plan for a mission like this. It’s largely conceptual. But the technology to do it is coming along. NASA has funded a mission study, so it definitely has merit.
“Fortunately, we don’t have to wait until mid-century to make practical progress – we can explore and test swarming techniques now in a simulated environment, which is what we propose to do in this work,” said report lead author Thomas Eubanks from Space Initiatives Inc. “We anticipate our innovations would have a profound effect on space exploration, complementing existing techniques and enabling entirely new types of missions, for example, picospacecraft swarms covering all of cislunar space or instrumenting an entire planetary magnetosphere.”
Eubanks also points out how a swarm of probes could investigate interstellar objects that pass through our inner Solar System, like Oumuamua.
But the main mission would be the one to Proxima Centauri b. According to Eubanks, that would happen sometime in the third quarter of this century.
The post What a Swarm of Probes Can Teach Us About Proxima Centauri B appeared first on Universe Today.
One of the biggest mysteries of cosmology may finally be solved
One of the biggest mysteries of cosmology may finally be solved
Recycle Your Eclipse Glasses to Share the Awe with Others
The nonprofit Astronomers Without Borders is collecting gently used eclipse glasses through Warby Parker and other sites to enable people to see future eclipses
Are you languishing in life? Here’s how to find your purpose again
Are you languishing in life? Here’s how to find your purpose again
New NASA Strategy Envisions Sustainable Future for Space Operations
To address a rapidly changing space operating environment and ensure its preservation for generations to come, NASA released the first part of its integrated Space Sustainability Strategy, on Tuesday advancing the agency’s role as a global leader on this crucial issue.
“The release of this strategy marks true progress for NASA on space sustainability,” said NASA Deputy Administrator Pam Melroy. “Space is busy – and only getting busier. If we want to make sure that critical parts of space are preserved so that our children and grandchildren can continue to use them for the benefit of humanity, the time to act is now. NASA is making sure that we’re aligning our resources to support sustainable activity for us and for all.”
For decades, NASA has served as a proactive leader for responsible and sustainable space operations. Entities across the agency develop best practices, analytic tools, and technologies widely adopted by operators around the world. The new strategy seeks to integrate those efforts through a whole-of-agency approach – allowing NASA to focus its resources on the most pressing issues. To facilitate that integration, NASA will appoint a new director of space sustainability to coordinate activities across the agency.
Key aspects of our approach include providing global leadership in space sustainability, supporting equitable access to space, and ensuring NASA’s missions and operations enhance space sustainability.
Space environments currently are seeing the rapid emergence of commercial capabilities, many of them championed by NASA. These capabilities include increased low Earth orbit satellite activity and plans for the use of satellite constellations, autonomous spacecraft, and commercial space destinations. However, this increased activity also has generated challenges, such as an operating environment more crowded with spacecraft and increased debris. Understanding the risks and benefits associated with this growth is crucial for space sustainability.
Developed under the leadership of a crossagency advisory board, the space sustainability strategy focuses on advancements NASA can make toward measuring and assessing space sustainability in Earth orbit, identifying cost-effective ways to meet sustainability targets, incentivizing the adoption of sustainable practices through technology and policy development, and increasing efforts to share and receive information with the rest of the global space community.
NASA’s approach to space sustainability recognizes four operational domains: Earth, Earth orbit, the orbital area near and around the Moon known as cislunar space, and deep space, including other celestial bodies. The first volume of the strategy focuses on sustainability in Earth orbit. NASA plans to produce additional volumes focusing on the other domains.
Learn more about the Space Sustainability Strategy at:
https://www.nasa.gov/spacesustainability
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Amber Jacobson / Rob Margetta
Headquarters, Washington
202-358-1600
amber.c.jacobson@nasa.gov / robert.j.margetta@nasa.gov