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NASA’s DART spacecraft successfully slammed into a distant asteroid at hypersonic speed on Monday in the world’s first test of a planetary defense system, designed to prevent a potential doomsday meteorite collision with Earth.

Humanity’s first attempt to alter the motion of an asteroid or any celestial body played out in a NASA webcast from the mission operations center outside Washington, DC, 10 months after DART was launched.

The livestream showed images taken by DART’s camera as the cube-shaped “impactor” vehicle, no bigger than a vending machine with two rectangular solar arrays, streaked into the asteroid Dimorphos, about the size of a football stadium, at 7:14 pm EDT (23:14 GMT) some 6.8 million miles (11 million km) from Earth.

The $330 million (roughly Rs. 2,683 crore) mission, some seven years in development, was devised to determine if a spacecraft is capable of changing the trajectory of an asteroid through sheer kinetic force, nudging it off course just enough to keep Earth out of harm’s way.

Whether the experiment succeeded beyond accomplishing its intended impact will not be known until further ground-based telescope observations of the asteroid next month. But NASA officials hailed the immediate outcome of Monday’s test, saying the spacecraft achieved its purpose.

“NASA works for the benefit of humanity, so for us it’s the ultimate fulfillment of our mission to do something like this – a technology demonstration that, who knows, some day could save our home,” NASA Deputy Administrator Pam Melroy, a retired astronaut, said minutes after the impact.

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

Monday evening’s bullseye impact was monitored in near real time from the mission operations center at the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland.

Cheers erupted from the control room as second-by-second images of the target asteroid, captured by DART’s onboard camera, grew larger and ultimately filled the TV screen of NASA’s live webcast just before the signal was lost, confirming the spacecraft had crashed into Dimorphos.

DART’s celestial target was an oblong asteroid “moonlet” about 560 feet (170 meters) 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 could not create a new 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 present 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. A Dimorphos-sized asteroid, while not capable of posing a planet-wide threat, could level a major city with a direct hit.

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

Robotic suicide mission

The mission represented a rare instance in which a NASA spacecraft had to crash to succeed. DART flew directly into Dimorphos at 15,000 miles per hour (24,000 kph), creating the force scientists hope will be enough to shift its orbital track closer to the parent asteroid.

APL engineers said the spacecraft was presumably smashed to bits and left a small impact crater in the boulder-strewn surface of the asteroid.

The DART team said it expects to shorten the orbital path 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 nudge to an asteroid millions of miles away years in advance could be sufficient to safely reroute it.

Earlier calculations of the starting location and orbital period of Dimorphos were made during a six-day observation period in July and will be compared with post-impact measurements made in October to determine whether the asteroid budged and by how much.

Monday’s test also was observed by a camera mounted on a briefcase-sized mini-spacecraft released from DART days in advance, as well as by ground-based observatories and the Hubble and Webb space telescopes, but images from those were not immediately available.

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.

© Thomson Reuters 2022


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Juno Mission Sheds Light on Jupiter’s Storms and Volcanic Activity on Io

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Juno Mission Sheds Light on Jupiter’s Storms and Volcanic Activity on Io

NASA’s Juno mission has discovered a world of cyclones at Jupiter’s north Jovian pole, a region of cooler stratospheric haze. The cyclones drift to the pole through a process the researchers refer to as “beta drift” via JunoCam and Jovian Infrared Aurora Mapper. The cyclones oscillate around their centres and can drift clockwise around the pole. Juno has also been making recurring flybys of the innermost Jovian moon, Io, revealing evidence of subterranean magma flows below its surface. These cooling flows could explain how Io’s volcanoes erupt, as about 10% of the moon’s subsurface has these flows.

Juno Spots Colliding Jupiter Cyclones and Magma Beneath Io’s Surface

As per the data presented by NASA at the European Geosciences Union General Assembly on April 29, Juno has observed a large central cyclone over 1,800 miles wide, encircled by eight slightly smaller cyclones. These weather systems, blowing at speeds over 100 miles per hour, interact through a phenomenon called beta drifts — similar to Earth’s cyclones but progressing to Jupiter’s pole.

Once enabled, researchers could visualise both visible and thermal activity in Jupiter’s atmosphere. The cyclones stabilise one another and slowly push in the same direction around the pole—in a clockwise direction, as the researchers noted. Jupiter’s cyclones differ from those on Earth since they do not weaken over time at the poles, when the planet has a different atmospheric makeup.

At the same time, exploring Io with Juno has made another discovery: that beneath the surface of the moon lie hidden flows of magma. By pairing infrared and microwave data, scientists picked up warm lava from a large eruption on Dec. 27, 2024. The volcano remained active through Juno’s next flyby in March and is expected to erupt again in May. These discoveries mark the most energetic volcanic eruption ever observed on Io.

The detection of subsurface magma confirms Io’s surface is constantly being renewed. Scientists calculate that 10% of the moon’s interior contains slowly cooling lava. These lava flows help transport heat from Io’s interior to the surface.

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New Study Uncovers Shadowy Origins of Universe’s Most Luminous Phenomena

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New Study Uncovers Shadowy Origins of Universe’s Most Luminous Phenomena

Some of the brightest lights in the universe shine from some of its darkest corners — so-called supermassive black holes. Invisible to the human eye, these high-energy powerhouses light up the cosmos with emissions that are detected by space telescopes. Thousands of such light sources have been discovered with NASA’s Fermi Gamma-ray Space Telescope, which has been observing since 2008. These aren’t just stars — they are active galactic nuclei (AGN) where large gravitational forces fling matter around black holes, creating intense radiation blasts all across the electromagnetic spectrum.

Blazars and AGN Jets Reveal How Black Holes Shape and Light Up the Universe

As per NASA’s report ,observational data, black holes lurk at the centres of most galaxies and are hundreds of thousands to billions of times the mass of the sun. In AGN, gas and dust fall into an inward-spiralling disk. Second, the disks experience friction and magnetic forces that produce light from radio to gamma rays. About one in ten AGN produce powerful jets of particles that move at nearly the speed of light, and it’s still a mystery to scientists how material so close to the event horizon is accelerated in the jets.

, the type of AGN observed depends on its orientation relative to Earth. Radio galaxies shoot their jets sideways, while blazars aim them nearly straight at us, making them appear especially bright in gamma rays. Fermi’s sky surveys show that more than half of the thousands of gamma-ray sources it has recorded are blazars, giving researchers vital clues about the energetic mechanics behind these cosmic light shows.

AGN are more than just bright; scientists are attracted to them for what they tell us about cosmic history. AGN existed in the early universe and were probably important in modulating galaxy evolution. Astrophysicists will use observations and analyses of the conditions directly around these black holes to learn more about the structure and history of the universe itself.

The paradox is acute: black holes are famous for eating up all the light and matter they can latch onto, but they lie behind some of the most luminous phenomena seen in space. Through missions like Fermi, scientists are adjusting the picture of the universe, in which some of its darkest origins can sparkle the most.

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NASA’s Psyche Mission Encounters Pressure Drop, Backup Systems on Standby

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NASA’s Psyche Mission Encounters Pressure Drop, Backup Systems on Standby

The Psyche mission by NASA has gained a small success in its journey to the asteroid belt. Spacecraft used solar electric propulsion to pass through into space easily. This led to a decrease in fuel pressure. The scientists are finding the reason behind this issue to make sure the mission stays as it was planned. Xenon gas is used in the propulsion to eject the electric thrusters. This in turn allows Psyche to move into space efficiently at far distances.

Unexpected Pressure Drop Halts Thruster Firing

As per physics.org, it was studied that Psyche detected a sudden decrease in the pressure of xenon gas, which dropped from 36 psi to 26 psi, on April 1, 2025. According to its programming by NASA, the spacecraft shut down the thrusters automatically to avoid any risk. Spacecraft design allows it to handle the anomalies safely with precautions. Scientists are analysing the data driven by telemetry, to understand the reason behind this pressure drop.

Backup Systems Ready if Needed

The design of the spacecraft has been designed redundantly. Psyche has two identical fuel lines, and the team can access backup when needed. The team has put all the activities at halt till the examination of the system. This limited period hiatus of the mission allowed the spacecraft’s planned course of action till the middle of June at least. This buffer will allow the researchers enough time to detect the issue with no impact on the mission.

Mission Progress Remains on Track

The spacecraft is at a distance of around 238 million kms away from the Earth. After the launch of the spacecraft from Kennedy Space Center in October 2023, thruster operations began in May 2024. There is a flexibility in the design to carry out the mission with ease, after knowing the minor changes or hanging on that is required to do during this long expedition to the asteroid belt.

Next Steps: A Mars Flyby and Beyond

Further, Psyche will be on track for a Mars flyby in 2026. This will help the spacecraft to move ahead till the final point, the metal-rich asteroid Psyche which is placed between Mars and Jupiter. This will begin orbiting the asteroid in 2029.

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