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Physicists have coaxed a cloud of atoms into having a temperature beyond absolute zero and placed them in a geometric structure that could produce an unknown form of matter

Physicists have coaxed a cloud of atoms into having a temperature beyond absolute zero and placed them in a geometric structure that could produce an unknown form of matter

Thirty-year-old Noland Arbaugh says the Neuralink chip has let him “reconnect with the world”

The next time you snap a selfie, consider thanking an astronomer for your phone’s camera

Judges are only human and can make mistakes, so could an artificial intelligence make better and more efficient decisions?

Judges are only human and can make mistakes, so could an artificial intelligence make better and more efficient decisions?

Billionaire Jared Isaacman wanted to conduct a private Hubble Telescope reboost mission. NASA says 'not yet.'

Zoë Schlanger’s new book The Light Eaters explores the surprising science of plant intelligence.

The waxing Moon reenters the sky as an evening crescent. Pollux and Castor keep it company. The Big Dipper hangs straight down. And can you still catch wintry Capella? The colder your latitude the better your chance.

The post This Week's Sky at a Glance, June 7 – 16 appeared first on Sky & Telescope.

Image: ESA and Vast memorandum signature at ILA

Image: Ahead of World Ocean Day, the Copernicus Sentinel-2 mission takes us over the west of Grand Bahama Island, in the Bahamas.

Through the Artemis Program, NASA will send astronauts to the lunar surface for the first time since 1972. While the challenges remain the same, the equipment has evolved, including the rocket, spacecraft, human landing system (HLS), and space suits. In preparation for Artemis III (planned for September 2026), NASA recently conducted a test where astronauts donned the new space suits developed by Axiom Space and practiced interacting with the hardware that will take them to the Moon.

These new suits, the Axiom Extravehicular Mobility Unit (AxEMU), were developed specifically for the Artemis III mission. The day-long test took place on April 30th at SpaceX headquarters in Hawthorne, California, where astronaut Doug “Wheels” Wheelock and Axiom Space astronaut Peggy Whitson interacted with a full-scale model of the SpaceX Starship Human Landing System (HLS). This was the first time astronauts trained in pressurized spacesuits and conducted mock operations with the HLS hardware.

The Artemis III spacesuit prototype, the AxEMU. Though this prototype uses a dark gray cover material, the final version will likely be all-white when worn by NASA astronauts on the Moon’s surface. Credit: Axiom Space

The test provided valuable feedback on the Starship HLS and the AxEMU spacesuits for NASA and its commercial partners. It also gave astronauts a chance to gauge the suits’ range of motion and to get a feel for the interior of the Starship HLS and its mechanical systems. Said Logan Kennedy, lead for surface activities in NASA’s HLS Program, in a NASA press statement:

“Overall, I was pleased with the astronauts’ operation of the control panel and with their ability to perform the difficult tasks they will have to do before stepping onto the Moon. The test also confirmed that the amount of space available in the airlock, on the deck, and in the elevator, are sufficient for the work our astronauts plan to do.”

The test consisted of Wheelock and Whitson practicing putting on and taking off the spacesuits – which included the suit’s Portable Life Support System (PLSS) – in the Starship HLS‘ full-scale airlock. Since the Artemis III astronauts will need to put the suits on with minimal assistance, this test allowed NASA to test how easily the suits are to get in and out of. The suits were then pressurized and powered up, and Wheelock and Whitson began interacting with the mobility aids (handrails and straps) and control panel in the airlock.

They then walked from the airlock deck to the HLS elevator, which will take the Artemis III astronauts and their equipment to the lunar surface to conduct extravehicular activity (EVA). Though the tasks were routine, they validated the spacesuit design and brought NASA one step closer to achieving its goals through the Artemis Program. As Amit Kshatriya (NASA’s Moon to Mars program manager) expressed:

“With Artemis, NASA is going to the Moon in a whole new way, with international partners and industry partners like Axiom Space and SpaceX. These partners are contributing their expertise and providing integral parts of the deep space architecture that they develop with NASA’s insight and oversight. Integrated tests like this one, with key programs and partners working together, are crucial to ensure systems operate smoothly and are safe and effective for astronauts before they take the next steps on the Moon.”

Wheelock and Whitson tested the agility of the spacesuits by conducting movements and tasks similar to those necessary during lunar surface exploration on Artemis missions. Credit: SpaceX

Putting the spacesuits through rigorous testing is necessary since the Artemis III mission will include EVAs in space and on the lunar surface. The four-person crew will launch aboard an Orion spacecraft atop NASA’s Space Launch System (SLS) while the Starship HLS launches separately and refuels in orbit. The Orion spacecraft will rendezvous and dock with the HLS in lunar orbit; two astronauts will transfer aboard and then take the HLS to and from the lunar surface. The AxEMU suits are designed to provide greater flexibility and accommodate a wider range of astronauts.

This is in keeping with NASA’s commitment to diversity, equity, and inclusion in its astronaut corps. Despite delays, things are undeniably coming together for Artemis III!

Further Reading: NASA

The post Astronauts are Practicing Lunar Operations in New Space Suits appeared first on Universe Today.

Boeing's Starliner Crew Flight Test faced down thruster glitches and helium leaks to reach the International Space Station on June 6. Why all the glitches and is NASA worried?

Made with narrowband filters,

Similar craters are found on Earth and the Moon, and are the product of volcanic, tectonic or even fluvial activity.

Red dwarf stars, also known as M-dwarfs, dominate the Milky Way’s stellar population. They can last for 100 billion years or longer. Since these long-lived stars make up the bulk of the stars in our galaxy, it stands to reason that they host the most planets.

Astronomers examined one red dwarf star named SPECULOOS-3, a Jupiter-sized star about 55 light-years away, and found an Earth-sized exoplanet orbiting it. It’s an excellent candidate for further study with the James Webb Space Telescope.

SPECULOOS stands for the Search for habitable Planets EClipsing ULtra-cOOl Stars. It’s a European Southern Observatory effort that searches for terrestrial planets orbiting cool stars like red dwarfs. (Its odd name is an homage to a Belgian sweet biscuit.) Its goal is to find planets that are good targets for spectroscopy with the JWST and the ELT.

The new planet is named SPECULOOS-3b, and its discovery was presented in a recent paper in Nature Astronomy. The paper is titled “Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3.” The lead author is Michaël Gillon from the Astrobiology Research Unit, Université de Liège, Belgium.

SPECULOOS is an automated search using four telescopes around the world: one at the Paranal Observatory in Chile, one at the Teide Observatory in Tenerife, one at the La Silla Observatory in Chile, and one at the Oukaïmden Observatory in Morocco. The project is searching 1,000 ultra-cool stars and brown dwarfs for terrestrial planets.

One of the problems in detecting planets around these stars is their low luminosity. Since they’re so dim, transiting exoplanets are difficult to detect, making their planetary populations difficult to characterize and study. So far, astronomers have found only one planetary system around one of these stars, and it’s rather well-known: the TRAPPIST-1 system. When it began, the SPECULOOS program expected to find at least one dozen systems similar to TRAPPIST-1.

“We designed SPECULOOS specifically to explore nearby ultra-cool dwarf stars in search of rocky planets,” lead author Gillon said. “With the SPECULOOS prototype and the crucial help of the NASA Spitzer Space Telescope, we discovered the famous TRAPPIST-1 system. That was an excellent start!”

The dimness of these stars can’t be understated. “Though this particular red dwarf is more than a thousand times dimmer than the Sun, its planet orbits much, much closer than the Earth, heating up the planetary surface,” said co-author Catherine Clark, a postdoctoral researcher at NASA’s JPL in Southern California.

The new planet is an Earth-sized world that orbits its star in only 17 hours. The star has a spectral type M6.5, and it delivers 16.5 more solar irradiation to its planet than the Sun does to Earth. That may sound surprising since the star is much cooler than the Sun. The Sun’s surface temperature is 5,772 K (5,500 C), while SPECULOOS-3’s temperature is only 2,900 K (2,627 C.) But SPECULOOS 3 bombards the planet with radiation due to the small distance separating them.

Since the irradiation is largely infrared and the star is only Jupiter-sized, it makes the planet an exceptional candidate for follow up observations, which is exactly what the SPECULOOS program is all about. The SPECULOOS Program 1 has found about 365 temperate, Earth-sized targets for further study with the JWST.

This chart shows the classifications by spectral type for main sequence stars according to the Harvard classification. Image Credit: By Pablo Carlos Budassi – Own work, CC BY-SA 4.0, https://commons.wikimedia.org/w/index.php?curid=92588077

The SPECULOOS-3 system is about 6.6 billion years old. Its luminosity, mass and radius are 0.084%, 10.1% and 12.3% of those of the Sun. “Just slightly larger than TRAPPIST-1, SPECULOOS-3 is the second-smallest main sequence star found to host a transiting planet,” the authors explain in their paper.

Two different telescopes observed the planetary transits around the star in 2021 and 2022 over eight nights. “Visual inspection of the 2021 and 2022 light curves showed some transit-like structures that motivated future intensive monitoring of the star,” the authors explain. The star was re-observed in 2023.

This figure from the study shows the transit of SPECULOOS-3b around its dim, cool star. Image Credit: Gillon et al. 2024.

The researchers determined that SPECULOOS-3b is about the same size as Earth, about 96% of our planet’s radius. But the planet’s density and mass are so far unconstrained. “Nevertheless,” the authors write in their paper, “several factors strongly suggest a rocky composition.”

There are two empirical reasons why the planet is likely rocky, though. The first is that its radius is on the rocky side of the radius gap. The second is that “all of the known Earth-sized planets in the NASA exoplanet archive have masses that imply rocky compositions,” Gillon and his co-authors explain.

This figure from the research compares SPECULOOS-3b to other transiting terrestrial exoplanets with less than 1.6 Earth radii. All of these planets are also cool enough to have rocky daysides rather than molten daysides. The shaded green area highlights planetary radii most similar to Earth’s (0.9–1.1R). Image Credit: Gillon et al. 2024.

But the big question concerns the planet’s potential atmosphere.

“From a theoretical point of view, the intense extreme ultraviolet emission of low-mass stars during their early lives makes it unlikely that such a small planet on such a short orbit could have maintained a substantial envelope of hydrogen.” the authors explain.

Red dwarfs are known to emit extreme radiation that strips away planetary atmospheres. However, there is some evidence that some planets can hold on to their atmospheres despite intense radiation, as with the recently discovered TIC365102760 b. Only time and more observations can tell us if the planet has an atmosphere and what type it has.

The researchers watched closely to see if there was a second planet around the star but didn’t find one. They also examined the planet spectroscopically with ground-based facilities. But we’ll have to wait for the JWST to examine the planet before we can really understand its atmosphere. The two most likely types of atmospheres for hot rocky planets are CO2-dominated and H2O-dominated.

The JWST will be able to examine SPECULOOS-3b with emission spectroscopy. This means it can examine the light the planet is emitting rather than just the light from the star as it passes through the atmosphere, which is called transmission spectroscopy. Emission spectroscopy is unaffected by irregular stellar behaviour, which red dwarfs are known to exhibit. JWST emission spectroscopy can also help determine the surface mineralogy if there’s no atmosphere. There’s a potential wealth of information waiting to be uncovered.

“We’re making great strides in our study of planets orbiting other stars,” said Steve B. Howell, one of the planet’s discoverers at NASA Ames Research Center. “We have now reached the stage where we can detect and study Earth-sized exoplanets in detail. The next step will be to determine whether any of them are habitable or even inhabited.”

The post An Earth-sized Exoplanet Found Orbiting a Jupiter-Sized Star appeared first on Universe Today.

NASA has awarded contracts to six companies to supply liquid nitrogen and liquid oxygen in support of operations at agency centers and facilities across the United States. The indefinite-delivery/fixed-price contract runs from Monday, July 1, 2024, through June 30, 2029.

The awards and approximate maximum contract values are:

• Air Products and Chemicals Inc., Allentown, Pennsylvania, $36.9 million
• Airgas USA LLC (South), Kennesaw, Georgia, $4.7 million
• Airgas USA LLC (Central), Tulsa, Oklahoma, $5.1 million
• Linde Inc., Danbury, Connecticut, $42.2 million
• Matheson Tri-Gas Inc., Warren, New Jersey, $1.8 million  
• Messer LLC, Bridgewater, New Jersey, $62.3 million

The total maximum delivery of liquid nitrogen, which NASA uses for pneumatic actuation, purging and inerting, pressurization, and cooling, will be about 656.8 tons, 30.4 million gallons, and 740,000 liters. The total maximum delivery of liquid oxygen, which is used as an oxidizer in cryogenic rocket engines, will be about 2.1 million gallons and 243,000 tons.

The commodities will support current and future aerospace flight, simulation, research, development, testing, and other operations at the following NASA centers and facilities: Ames Research Center in California’s Silicon Valley; Glenn Research Center in Cleveland and Neil Armstrong Test Facility in Sandusky, Ohio; Goddard Space Flight Center in Greenbelt, Maryland; Jet Propulsion Laboratory in Southern California; Johnson Space Center in Houston and White Sands Test Facility in Las Cruces, New Mexico; Kennedy Space Center in Florida; Langley Research Center in Hampton, Virginia; Marshall Space Flight Center in Huntsville, Alabama; Michoud Assembly Facility in New Orleans; and Stennis Space Center in Bay St. Louis, Mississippi.

For more information about NASA programs and missions, visit:

https://www.nasa.gov

-end-

Abbey Donaldson
Headquarters, Washington
202-358-1600
abbey.a.donaldson@nasa.gov  

Despite being extraordinarily difficult to detect for the first time, gravitational waves can be found using plenty of different techniques. The now-famous first detection at LIGO in 2015 was just one of the various ways scientists had been looking. A new paper from researchers from Europe and the US proposes how scientists might be able to detect some more by tracking the exact position of the upcoming Uranus Orbiter and Probe (UOP).

Initially suggested by NASA’s Planetary Science and Astrobiology Decadal Survey, UOP will be the first mission to Uranus since Voyager visited the system in 1986. When it finally arrives in 2044, after a 2031 launch date, it will be almost 60 years since humanity last had an up-close look at the Uranian system.

But 13 years in transit sure is a long time. Part of that time will be spent getting a gravitational boost from Jupiter, but most will be spent coasting between planetary bodies. And that much time spent in between planets is what the paper’s authors want to utilize to do non-Uranian science.

Fraser has long been a proponent of returning to Uranus, as he explains here.

Gravitational waves can disrupt the fabric of space-time, causing discernible distortions, especially over long distances. If the instruments in question are sensitive enough, the massive distance between UOP and the Earth would be a viable way to detect them.

This isn’t the first time using the distance between a spacecraft and Earth has been considered for detecting gravitational waves. Pioneer 11, Cassini, and a triangulation of Galileo, Ulysses, and Mars Orbiter all had entertained suggestions of being utilized for gravitational wave detection while on their journey to their final destinations. However, the equipment they were designed with was not sensitive enough to pick up the minute fluctuations required for an actual detection.

UOP will have the added advantages of decades of improved equipment, especially communications and timing electronics, which are critical to any gravitational wave detection. It also benefits that we’ve already officially detected a gravitational wave, so we know at least what to look for.

Long distance communication is hard, as Fraser explains in this video, but it’s also key to capturing data on gravitational waves.

The underlying mechanism is simple enough – consistently track the exact established position of UOP during its 13-year cruise to Uranus and cross-reference any anomalies in its position against what could be expected from known causes. These include the gravitational pull of some of the planets, or even asteroids, and solar radiation pressure on the spacecraft itself. As the authors note, some or even all of these could impact the spacecraft’s exact position; for the calculations to work effectively to find gravitational waves, better accounting for what, if any, impact they have must be completed.

But there is another potentially scientifically interesting cause of slight positional drift for the UOP: ultra-light dark matter. In theory, UOP could be used to test or even directly detect a form of dark matter known as ultra-light dark matter if it happens to exist in the solar system. Theorists have numerous models showing how it would work if it did exist. UOP could also use the same sort of exact positional calculation to contribute to that scientific research.

Best of all, UOP can do all this with literally no change to its primary functional mission – exploring the Uranian system. All that would have to be changed about the mission would be to update Earth with consistent positional data about once every 10 seconds for the duration of the 13-year trip to UOP’s final destination. Suppose there’s a chance that those more frequent check-ins with home could help detect gravitational waves or potentially dark matter. In that case, it seems well worth the consideration of the UOP mission planners – but it remains to be seen whether it will be included or not. The paper’s authors have made a persuasive argument about why it should be.

Learn More:
Zwick et al. – Bridging the micro-Hz gravitational wave gap via Doppler tracking with the Uranus Orbiter and Probe Mission: Massive black hole binaries, early universe signals and ultra-light dark matter
UT – It’s Time to Go Back to Uranus. What Questions do Scientists Have About the Ice Giants?
UT – We Could SCATTER CubeSats Around Uranus To Track How It Changes
UT – What Mission Could Detect Oceans at Uranus’ Moons?

Lead Image:
Proposed Uranus orbiter mission.
Credit – NASA Decadal Survey

The post A Mission to Uranus Could Also be a Gravitational Wave Detector appeared first on Universe Today.