In 1995, Caltech researchers at the Institute’s Palomar Observatory first observed what appeared to be a brown dwarf orbiting Gliese 229 – a red dwarf star located about 19 light-years from Earth. Since then, this brown dwarf (Gliese 229 B) has mystified astronomers because it appeared too dim for its mass. With 70 times the mass of Jupiter, it should have been brighter than what telescopes had observed. However, a Caltech-led international team of astronomers recently solved the mystery by determining that the brown dwarf is a pair of closely orbiting twins! The study was led by Jerry W. Xuan, a graduate student in Caltech’s Department of Astronomy working with Dimitri Mawet, the David Morrisroe Professor of Astronomy. They were joined by an international team from institutes and universities around the world, including the National Research Council of Canada Herzberg, the European Southern Observatory (ESO), the European Space Agency (ESA), the Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), the Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), the Max Planck Institute for Astronomy (MPIA) and Extraterrestrial Physics (MPE), and NASA’s Jet Propulsion Laboratory (JPL). Their study, which appeared in Nature, was funded by NASA and the Heising-Simons Foundation. The study team responsible for discovering Gliese 229 B in 1995 included several co-authors on this latest study, including Rebecca Oppenheimer, a Caltech graduate student at the time (now an astrophysicist at the American Museum of Natural History); Shri Kulkarni, the George Ellery Hale Professor of Astronomy and Planetary Science; Keith Matthews, an instrument specialist at Caltech; and other colleagues. At the time, their findings indicated that Gliese 229 B had methane in its atmosphere, which is typical of gas giants but not stars. These findings constituted the first confirmed detection of a brown dwarf, a class of cool star-like objects that constitute the “missing link” between gas giants and stars that had been predicted about 30 years prior. “Seeing the first object smaller than a star orbiting another sun was exhilarating,” said Oppenheimer in a Caltech news release, “It started a cottage industry of people seeking oddballs like it back then, but it remained an enigma for decades.” “Gliese 229 B was considered the poster-child brown dwarf,” added Xuan. “And now we know we were wrong all along about the nature of the object. It’s not one but two. We just weren’t able to probe separations this close until now.” Hundreds of observations have been conducted since Gliese 229 B was discovered nearly 30 years ago, but its dimness remained a mystery to astronomers. While scientists suspected Gliese 229 B might be twins, the two brown dwarfs would have to be very close to each other to evade notice for almost three decades. To confirm this theory, the team relied on the GRAVITY interferometer on the ESO’s Very Large Telescope in Chile to spatially resolve the two brown dwarfs. They then used the CRyogenic high-resolution InfraRed Echelle Spectrograph (CRIRES+) instrument to detect their distinct spectral signatures and measure their Doppler shift. Their results showed that Gliese 229 B consists of two brown dwarfs (Gliese 229 Ba and Gliese 229 Bb) about 38 and 34 times the mass of Jupiter, that orbit each other with a period of 12 days and a separation of 16 times the distance between Earth and the Moon. The observed brightness levels also match what is expected for two small brown dwarfs in this mass range. “This discovery that Gliese 229 B is binary not only resolves the recent tension observed between its mass and luminosity but also significantly deepens our understanding of brown dwarfs, which straddle the line between stars and giant planets,” said Mawet, a senior research scientist at NASA JPL. The discovery of this duo raises new questions about how tight-knit brown dwarfs form and suggests similar binaries may be out there and waiting to be found. An artist’s conception of looking back at Sol from the binary brown dwarf system WISE 1049-5319, 6.5 light years distant. Credit: Janella Williams, Penn State University Some theories suggest that brown dwarf pairs could form within a star’s protoplanetary disk that fragments into two seeds of brown dwarfs that become gravitationally bound after a close encounter. The same mechanism might lead to closely orbiting exoplanet binaries, though all of this remains to be seen. In the meantime, said Oppenheimer, this discovery is a very exciting development. “These two worlds whipping around each other are actually smaller in radius than Jupiter,” she said. “They’d look quite strange in our night sky if we had something like them in our own solar system. This is the most exciting and fascinating discovery in substellar astrophysics in decades.” In the future, Xuan and his colleagues plan to search for more brown dwarf binaries using existing and next-generation instruments. This includes the Keck Planet Imager and Characterizer (KPIC) and the Keck Observatory’s High-resolution Infrared SPectrograph for Exoplanet Characterization (HISPEC). A team led by Mawet developed the former, while the latter is currently under construction at Caltech and other laboratories by teams also led by Mawet. A separate independent study that appeared in The Astrophysical Journal Letters was led by Sam Whitebook and Tim Brandt, a Caltech graduate student and an associate astronomer at the Space Telescope Science Institute in Baltimore (respectively). Their findings also concluded that Gliese 229 B is a pair of tightly-orbiting brown dwarfs. Further Reading: Caltech, Nature The post Astronomers Solve the Mystery of the Famed Brown Dwarf That is Too Bright: It’s Twins! appeared first on Universe Today.

The Artemis program involves impressive technological advancements in robotics, communications, spacecraft, and advanced habitats, all of which are clearly necessary for such an ambitious endeavour. But the mission also requires updated spacesuits. Those spacesuits are critical to mission success, and the Italian luxury fashion house Prada is adding their knowledge and experience to the design. More than 50 years have passed since the last human walked on the Moon. Entirely new technologies have been available since then, though spacesuits don’t look like they’ve changed that much, at least on the surface. But Axiom Space, the NASA contractor creating the new spacesuits, says they’ve redefined spacesuit development—and they’ve done it with help from Prada. “We’re blending engineering, science and art.”Russel Ralston, Axiom Space’s Executive Vice President of Extravehicular Activity. It’s tempting to dismiss Prada as just a fashion brand. But according to the two companies, Prada has “expertise on high-performance materials, features, and sewing techniques,” that are critical to the new spacesuit. “This is a groundbreaking partnership,” said Russel Ralston, Axiom Space’s Executive Vice President of Extravehicular Activity. “We’re blending engineering, science and art.” “Our elite teams have redefined spacesuit development, establishing new pathways to innovative solutions and applying a state-of-the-art design approach for the AxEMU,” said Matt Ondler, the President of Axiom Space. “We have broken the mold. The Axiom Space-Prada partnership has set a new foundational model for cross-industry collaboration, further expanding what’s possible in commercial space.” The AxEMU is impressive. It’s a single architecture that can be adapted for missions to the lunar surface and to Low-Earth Orbit. It can accommodate a wide range of body sizes from the first to the 99th percentile and is more flexible due to innovative soft and hard joints. This provides greater flexibility and allows more precise geological and scientific work while maximizing astronaut comfort. The AxEMU spacesuit includes custom gloves made in-house, featuring several advancements over the gloves currently in use. Image Credit: Axiom Space/Prada According to Axiom, the AxEMU is more reliable than previous suits and built-in redundancies provide increased safety for astronauts. If something fails, those redundancies allow astronauts to return to a spacecraft or habitat, where another benefit of the suit comes into play. The new suit is designed to be maintained in orbit. Artemis aims to explore the Moon’s polar regions, where temperatures plummet to as low as -238°C (-396°F) in permanently shadowed craters. AxEMU can keep astronauts alive for two hours in those temperatures, and they will be able to perform spacewalks for eight hours. This infographic highlights some of AxEMU’s components and capabilities. The suit features biometric monitoring, in-suit athlete-level nutrition, and 4G/LTE communications. Image Credit: Axiom Space/Prada AxEMU employs an innovative regenerative carbon dioxide scrubbing system. This is an improvement over other suits, which employed lithium hydroxide (LiOH) canisters to absorb CO2 and had to be replaced after each use. While many of the suit’s improvements are strictly technological, Prada contributed to its overall design. Both Prada and Axiom Space praise their ongoing partnership. Lorenzo Bertelli is the Prada Group’s Chief Marketing Officer and Head of Corporate Social Responsibility. Bertelli said, “Going beyond our limits is one of the company’s values that perfectly reflects the spirit of the Prada brand and my parents’ vision. I’m very proud of the result we’re showing today, which is just the first step in a long-term collaboration with Axiom Space. We’ve shared our expertise on high-performance materials, features, and sewing techniques, and we learned a lot. I’m sure we’ll continue to explore new challenges, broaden our horizons, and build new scenarios together.” “We are pioneering a new era in space exploration where partnerships are imperative to the commercialization of space,” said Ralston. “Partnerships build a strong, cohesive team, enabling industry experts to provide cutting-edge technology, specialized products and services to drive innovation. For the first time, we are leveraging expertise in other industries to craft a better solution for space.” New visor coatings on the AxEMU give astronauts improved vision. Image Credit: Axiom Space/Prada. From gloves to boots to electronics and visor coatings and everything in between, the AxEMU is an improvement over previous suits. Over the past two years, Axiom Space has been iteratively improving the design with an eye on the scheduled moon landing in 2026. They’ve tested the suit extensively with astronauts and with simulations in state-of-the-art facilities at SpaceX, NASA, and in-house. They also tested the suit underwater to simulate the lunar environment with an unoccupied spacesuit at NASA’s Neutral Buoyancy Laboratory (NBL) and reduced gravity simulations at NASA’s Johnson Space Center. AxEMU is nearing its final testing stage. In 2025, it will enter its critical design testing phase. If all goes well, Artemis astronauts will wear them when they set foot on the Moon in 2026. The post The Artemis Astronauts are Getting New Spacesuits With Some Help From Prada appeared first on Universe Today.

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