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Two NASA astronauts who flew to the International Space Station (ISS) in June aboard Boeing’s faulty Starliner capsule will need to return to Earth on a SpaceX vehicle early next year, NASA officials said on Saturday, deeming issues with Starliner’s propulsion system too risky to carry its first crew home as planned.

Veteran NASA astronauts Butch Wilmore and Sunita Williams, both former military test pilots, became the first crew to ride Starliner on June 5 when they were launched to the ISS for what was expected to be an eight-day test mission.

But Starliner’s propulsion system suffered a series of glitches in the first 24 hours of its flight to the ISS that has so far kept the astronauts on the station for 79 days as Boeing scrambled to investigate the issues.

NASA officials told reporters during a news conference in Houston that Wilmore and Williams, both former military test pilots, are safe and prepared to stay even longer. They will use their extra time to conduct science experiments alongside the station’s other seven astronauts, NASA said.

In a rare reshuffling of NASA’s astronaut operations, the two astronauts are now expected to return in February 2025 on a SpaceX Crew Dragon spacecraft due to launch next month as part of a routine astronaut rotation mission. Two of the Crew Dragon’s four astronaut seats will be kept empty for Wilmore and Williams.

The agency’s decision, tapping Boeing’s top space rival to return the astronauts, is one of NASA’s most consequential in years. Boeing had hoped its Starliner test mission would redeem the troubled program after years of development problems and over $1.6 billion in budget overruns since 2016.

Five of Starliner’s 28 thrusters failed during flight and it sprang several leaks of helium, which is used to pressurize the thrusters. It was still able to dock with the station, a football field-sized laboratory that has housed rotating crews of astronauts for over two decades.

NASA said in a statement Starliner will undock from the ISS without a crew in “early September.” The spacecraft will attempt to return to Earth autonomously, forgoing a core test objective of having a crew present and in control for the return trip.

“I know this is not the decision we had hoped for, but we stand ready to carry out the action’s necessary to support NASA’s decision,” Boeing’s Starliner chief Mark Nappi told employees in an email.

“The focus remains first and foremost on ensuring the safety of the crew and spacecraft,” Nappi said.

Several senior NASA officials and Boeing representatives made the decision during a Saturday morning meeting in Houston.

NASA’s space operations chief Ken Bowersox said agency officials unanimously voted for Crew Dragon to bring the astronauts home. Boeing voted for Starliner, which it said was safe.

Nelson told reporters at a news conference in Houston that he discussed the agency’s decision with Boeing’s new CEO Kelly Ortberg and was confident Boeing would continue its Starliner program. Nelson said he was “100 percent” certain the spacecraft would fly another crew in the future.

“He expressed to me an intention that they will continue to work the problems once Starliner is back safely,” Nelson said of Ortberg.

Boeing struggled for years to develop Starliner, a gumdrop-shaped capsule designed to compete with Crew Dragon as a second US option for sending astronaut crews to and from Earth’s orbit. The company is also struggling with quality issues on production of commercial planes, its most important products.

Starliner failed a 2019 test to launch to the ISS uncrewed, but mostly succeeded in a 2022 do-over attempt where it also encountered thruster problems. Its June mission with its first crew was required before NASA can certify the capsule for routine flights, but now Starliner’s crew certification path is uncertain.

The drawn-out mission has cost Boeing $125 million (roughly Rs. 1,048 crore), securities filings show. The company arranged tests and simulations on Earth to gather data that it has used to try and convince NASA officials that Starliner is safe to fly the crew back home.

But results from that testing raised more difficult engineering questions and ultimately failed to quell NASA officials’ concerns about Starliner’s thrusters and its ability to make a crewed return trip, the most daunting and complex part of the test mission.

“There was just too much uncertainty in the prediction of the thrusters,” NASA’s commercial crew program chief Steve Stich told reporters.

Starliner’s now-uncertain path to receiving a long-sought NASA certification will add to the crises faced by Ortberg, who started this month with the goal to rebuild the planemaker’s reputation after a door panel dramatically blew off a 737 MAX passenger jet in midair in January.

© Thomson Reuters 2024

(This story has not been edited by NDTV staff and is auto-generated from a syndicated feed.)

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Astronomers Spot Nearly Perfect Supernova Remnant of Unknown Size and Distance

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Astronomers Spot Nearly Perfect Supernova Remnant of Unknown Size and Distance

Glowing faintly on the Milky Way’s outskirts, astronomers have found a nearly perfect spherical relic of a supernova, challenging accepted knowledge of stellar explosions. Apart from its terrible symmetry, the orb, G305.4–2.2 or “Telios”—Greek for “perfect”—is confusing in terms of size and distance. Captured on radio pictures from the Australian Square Kilometre Array Pathfinder (ASKAP), the object might be either remarkably young or old. Its remarkable shape raises fundamental questions about how such near-perfect remnants form, especially given the chaotic nature of typical stellar deaths.

Astronomers Find Rarely Symmetrical Supernova Remnant in Milky Way Outskirts

As per a recent study published on the preprint server arXiv and accepted by Publications of the Astronomical Society of Australia, Telios was detected during the Evolutionary Map of the Universe project. Most supernova remnants (SNRs) have spheroidal shapes, none close to the smooth circular extremity of this record-holding SNR. “This object is circularly symmetric, indicating that it is one of the most circular galactic SNRs ever seen,” the authors mentioned.

Telios’ unusual symmetry is paired with extremely low brightness, making it difficult to pinpoint its distance or dimensions. Ranging from 45.6 to 156.5, it lets astronomers pin down that it could be anywhere from 7,170 to 25,101 light-years away from us. Its position below the galactic plane, in the thin disc of the galaxy where very few stars live, adds another layer of complexity. Its symmetric shape indicates a recently born neutron star, albeit with fainter light, supporting two other possibilities: an old, slowing-down neutron star or a young one that hasn’t lost its initial shape.

Though the source of Telios is yet unknown, astronomers choose Type Ia supernovae, explosions from less massive stars with a more constant force. Starting from more massive red giants, these are not as far-off or as lovely in quality as core-collapse supernovae. That notion is called into doubt, though, by the absence of a recognised parent star. Although the Type Ia scenario was recommended without direct data, the writers actively argued for more high-resolution studies.

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Planet Moving Backwards Found in Binary Star System Nu Octantis

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Planet Moving Backwards Found in Binary Star System Nu Octantis

A binary star system is a pair of stars gravitationally bound and orbiting a common centre of mass. In 2004, David Ramm at the University of Canterbury in New Zealand spotted a mysterious repeating signal while observing the motion of a pair of stars in a system called Nu Octantis. The signal hinted that a massive planet, twice Jupiter’s size, might exist in that system. In a new study, a small group of astronomers used improved measuring devices to confirm the planet’s existence and explain how the system can remain stable.

Retrograde motion of the planet

According to the study, new data from the HARPS spectrograph at the European Southern Observatory, the main star in the system is a sub-giant. The smaller star, a white dwarf, and the planet both orbit the larger star. But, oddly enough, they go around the star in opposite directions. These reversed trajectories reduce the risk of gravitational disruption and make the system stable.

The planet’s signal has remained consistent for more than 20 years, which strongly suggests it is not caused by stellar activity. According to Man Hoi Lee, co-author of the study, researchers are pretty sure about the planet’s existence. This highlights how long-term stability in the data supports the existence of this strange planet with a tight but stable path through the binary system.

Origin of the planet

There are two possibilities: the planet either used to orbit both stars at once but then radically shifted trajectory when one of the two stars became a white dwarf, or it was formed from the mass that the star ejected as it transformed into a white dwarf. Future observations and a lot more mathematical modelling may be able to pinpoint which of these scenarios is more likely to have occurred, but both are rather novel.

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Quantum Tech Could Finally Let Astronomers Snap Direct Images of Earth-Like Exoplanets

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Quantum Tech Could Finally Let Astronomers Snap Direct Images of Earth-Like Exoplanets

A team of U.S.-based astronomers is building a new kind of coronagraph — one powered by quantum mechanics — that could enable direct imaging of Earth-like exoplanets previously considered too faint or too close to their host stars to detect. Traditional telescopes have advanced since Galileo’s time, with instruments like the James Webb Space Telescope (JWST) now capable of analysing distant planetary atmospheres. But even these devices generally are not able to capture images of planets and asteroids that orbit nearby bright stars, as their light is frequently drowned out. Now, a breakthrough could be in sight.

Quantum-Sensitive Coronagraph May Revolutionize Exoplanet Imaging With Sub-Diffraction Precision

As per a recent Space.com report, researchers from the University of Arizona and the University of Maryland have developed a “quantum-sensitive” coronagraph that filters starlight before it reaches the telescope’s detector. By exploiting differences in the spatial modes of photons — how light waves behave in space — the device physically separates planetary light from overwhelming stellar glare. “This method routes photons to different regions before they even hit the sensor,” one co-author explained, emphasising its superiority to digital image processing.

This experimental device uses a “spatial mode sorter”, a series of precision-crafted optical phase masks that redirect light waves from exoplanets, allowing astronomers to view them below the diffraction limit. Normally, achieving this resolution would require telescopes too massive for current spaceflight capabilities. But quantum engineering may bypass that need altogether, provided that light purity — known as mode fidelity — reaches the stringent 1-in-a-billion requirement needed to block star photons while preserving exoplanet signals.

In lab tests, researchers successfully simulated star-planet systems and demonstrated that their system could resolve a dim, Earth-like planet even when positioned one-tenth the distance modern coronagraphs can handle. At higher star-to-planet contrast ratios — up to 1,000:1 — the device maintained accuracy within a few percentage points of theoretical limits, showcasing its potential for space-based observatories.

The technology could augment missions like NASA’s upcoming Habitable Worlds Observatory, designed to detect biosignatures on exoplanets. While scientists caution that the method isn’t a standalone solution, they believe it could dramatically expand the toolkit for planetary discovery. The findings were published on April 22 in Optica.

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