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Ten months after launch, NASA’s asteroid-deflecting DART spacecraft neared a planned impact with its target on Monday in a test of the world’s first planetary defense system, designed to prevent a doomsday collision with Earth.

The cube-shaped “impactor” vehicle, roughly the size of a vending machine with two rectangular solar arrays, was on course to fly into the asteroid Dimorphos, about as large as a football stadium, and self-destruct around 7pm EDT (4:30 IST) some 6.8 million miles (11 million km) from Earth.

The mission’s finale will test the ability of a spacecraft to alter an asteroid’s trajectory with sheer kinetic force, plowing into the object at high speed to nudge it astray just enough to keep our planet out of harm’s way.

It marks the world’s first attempt to change the motion of an asteroid, or any celestial body.

DART, launched by a SpaceX rocket in November 2021, has made most of its voyage under the guidance of NASA’s flight directors, with control to be handed over to an autonomous on-board navigation system in the final hours of the journey.

Monday evening’s planned impact is to be monitored in real time from the mission operations center at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Maryland.

DART’s celestial target is an asteroid “moonlet” about 560 feet (170 metres) in diameter that orbits a parent asteroid five times larger called Didymos as part of a binary pair with the same name, the Greek word for twin.

Neither object presents any actual threat to Earth, and NASA scientists said their DART test cannot create a new existential hazard by mistake.

Dimorphos and Didymos are both tiny compared with the cataclysmic Chicxulub asteroid that struck Earth some 66 million years ago, wiping out about three-quarters of the world’s plant and animal species including the dinosaurs.

Smaller asteroids are far more common and pose a greater theoretical concern in the near term, making the Didymos pair suitable test subjects for their size, according to NASA scientists and planetary defense experts.

Also, their relative proximity to Earth and dual-asteroid configuration make them ideal for the first proof-of-concept mission of DART, short for Double Asteroid Redirection Test.

Robotic mission suicide

The mission represents a rare instance in which a NASA spacecraft must ultimately crash to succeed.

The plan is for DART to fly directly into Dimorphos at 15,000 miles per hour (24,000 kph), bumping it hard enough to shift its orbital track closer to its larger companion asteroid.

Cameras on the impactor and on a briefcase-sized mini-spacecraft released from DART days in advance are designed to record the collision and send images back to Earth.

DART’s own camera is expected to return pictures at the rate of one image per second during its final approach, with those images streaming live on NASA TV starting an hour before impact, according to APL.

The DART team said it expects to shorten the orbital track of Dimorphos by 10 minutes but would consider at least 73 seconds a success, proving the exercise as a viable technique to deflect an asteroid on a collision course with Earth – if one were ever discovered. A small nudge to an asteroid millions of miles away could be sufficient to safely reroute it away from the planet.

The test’s outcome will not be known until a new round of ground-based telescope observations of the two asteroids in October. Earlier calculations of the starting location and orbital period of Dimorphos were confirmed during a six-day observation period in July.

DART is the latest of several NASA missions in recent years to explore and interact with asteroids, primordial rocky remnants from the solar system’s formation more than 4.5 billion years ago.

Last year, NASA launched a probe on a voyage to the Trojan asteroid clusters orbiting near Jupiter, while the grab-and-go spacecraft OSIRIS-REx is on its way back to Earth with a sample collected in October 2020 from the asteroid Bennu.

The Dimorphos moonlet is one of the smallest astronomical objects to receive a permanent name and is one of 27,500 known near-Earth asteroids of all sizes tracked by NASA. Although none are known to pose a foreseeable hazard to humankind, NASA estimates that many more asteroids remain undetected in the near-Earth vicinity.

NASA has put the entire cost of the DART project at $330 million (roughly Rs. 2,700 crore), well below that of many of the space agency’s most ambitious science missions.

© Thomson Reuters 2022


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Over 4,300 Koalas Found in Newcastle’s Fringe Forests by Drone Survey

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Over 4,300 Koalas Found in Newcastle’s Fringe Forests by Drone Survey

In a landmark survey, University of Newcastle researchers mapped a previously hidden koala population on the outskirts of Newcastle, NSW. The study estimated about 4,357 koalas across roughly 67,300 hectares of bushland (208 sites). They also found more than 290 koalas in Sugarloaf State Conservation Area, a region with few prior records. Local researcher Daryn McKenny, who grew up nearby and first reported seeing a koala there years ago, contributed his knowledge and sightings to the project. The findings show koalas can survive – and even thrive – in peri-urban forests, underscoring the need to protect these fringe habitats.

Hidden Koalas on Newcastle’s Fringe

According to the study, the survey estimated 4,357 koalas in 208 bushland sites around Newcastle. Lead author Shelby Ryan said that the drone surveys allowed the team to find koalas within minutes in areas that had taken hours on foot. Seven national parks were sampled (about 10% of each) with multiple night surveys, and a statistical model extrapolated these counts across the landscape. Maria National Park had the highest density (about 521 koalas per 3,350 hectares), while fire-affected parks from the 2019-20 fires hosted roughly two-thirds fewer koalas.

Survey Methods and Conservation Implications

Thermal imaging revealed koalas as yellow hotspots, which were then confirmed by a spotlight to identify the animal. The team used a statistical model accounting for terrain slope, tree coverage, and soil moisture to extrapolate koala numbers across the landscape. University of Newcastle’s Dr. Ryan Witt said that this model can even extend estimates to private or otherwise inaccessible lands that were not directly surveyed.

WWF-Australia – which co-funded the work – hailed the findings as critical for its goal of doubling koala numbers by 2050, noting that accurate abundance estimates are the “holy grail” of koala conservation. 

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NASA F-15 Flights Validate Supersonic Tools for X-59 Quiet Flight Quesst Mission

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NASA F-15 Flights Validate Supersonic Tools for X-59 Quiet Flight Quesst Mission

High above the Mojave Desert, NASA’s two F-15 jets completed a pivotal series of May flights to validate airborne tools essential for the agency’s Quesst mission, aimed at enabling quiet supersonic travel. Flying faster than the speed of sound, the jets replicated the conditions under which NASA’s experimental X-59 aircraft will fly. The campaign tested shockwave sensors, geospatial guidance systems, and schlieren imaging tools designed to detect and visualise the aircraft’s sonic “thump”—a softer alternative to the traditional boom—when the X-59 cruises at Mach 1.4 and above 50,000 feet.

As per NASA’s Armstrong Flight Research Centre, the dual-jet validation effort was led by the SCHAMROQ team, which transformed an F-15D from a combat aircraft into a research platform. Along with an F-15B, the aircraft were used to perform simultaneous flight operations—called dual ship flights—to validate three core systems: a near-field shock-sensing probe, an airborne schlieren photography setup, and a GPS-driven Airborne Location Integrating Geospatial Navigation System (ALIGNS). These efforts collectively confirm the systems’ readiness for X-59 data capture.

Cheng Moua, NASA’s project lead for SCHAMROQ, likened the series to a “graduation exercise”, where all tools were tested in their final configuration. The schlieren system, in particular, demanded intense precision, requiring a high-speed handheld camera to track the X-59’s airflow against the sun’s backdrop while the aircraft flew through a tight 100-foot alignment corridor.

The successful validation shows that NASA’s specialised tools are ready to record the X-59’s sound signature. This is a key step towards establishing that it is conceivable, quantifiable, and repeatable to fly supersonic over land without making too much noise. The information will help determine the future of commercial aviation regulation and technology, making the promise of quicker, quieter flight travel more likely.

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NASA’s Chandra Spots Unexpectedly Strong Jet from Distant Black Hole at Cosmic Noon

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NASA’s Chandra Spots Unexpectedly Strong Jet from Distant Black Hole at Cosmic Noon

A black hole 11.6 billion light years from Earth has unleashed a compelling jet, according to new observations from NASA’s Chandra X-ray Observatory and the National Radio Astronomy Observatory’s Very Large Array (VLA). Seen when the universe was at its early “cosmic noon”, or about 3 billion years after the Big Bang, the jet is visible to telescopes due to its interactions with the dense cosmic microwave background (CMB), a faint glow left over from the universe’s birth. Researchers confirmed two jets from different black holes, their particles racing at up to 99% the speed of light, offering rare insight into early supermassive black hole activity.

Chandra Detects Ultra-Fast Black Hole Jets Using X-Ray Vision and Statistical Relativity Model

As per NASA’s Chandra press release, the jets — from quasars J1405+0415 and J1610+1811 — were detected due to both the Chandra telescope’s sharp X-ray vision and the denser CMB of the early universe. When electrons in the jets collide with the CMB, they emit detectable X-ray signals. These observations were made possible by a statistical method that factors in how relativistic effects brighten jets that are angled toward Earth, solving a decades-old problem in jet detection.

The researchers determined that one jet’s particles were moving between 95 percent and 99 percent the speed of light, while the other reached up to 98 percent. Viewing angles were estimated to be 9 and 11 degrees, respectively. Despite originating from opposite directions, both jets appeared bright — a consequence of Einstein’s special relativity, which causes jets aimed at Earth to visually intensify, masking their actual orientation.

The findings, presented by Jaya Maithil of the Centre for Astrophysics | Harvard & Smithsonian at the 246th meeting of the American Astronomical Society, underline how fast-growing black holes shaped galaxy formation at cosmic noon. The dual detector is an example of how modern statistical models and X-ray measurements can perhaps access the edge of the universe’s most ancient, fiery moments.

These new ideas are informing us about how supermassive black holes work during the peak growth of galaxies. The results, which will be published in The Astrophysical Journal, add to a growing body of evidence suggesting that black hole jets in the most distant reaches of the universe can hold as much, if not more, energy than all the gas in their host galaxies.

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