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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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NASA Hubble Space Telescope Helps Confirm the First Solitary Black Hole

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NASA Hubble Space Telescope Helps Confirm the First Solitary Black Hole

For the first time, the existence of a lone black hole has been confirmed by scientists. This black hole has no star orbiting it. According to the statement by Kailash Sahu, astronomer at the Space Telescope Science Institute in Baltimore, “it’s the only one so far”. The discovery made headlines in the year 2022, when Sahu and his Team claimed a dark object was moving through the constellation Sagittarius. However, another team of researchers disputed the claims by identifying the object as a neutron star.

About the Discovery

This discovery came into the light three years ago. All the stellar-mass black holes are accompanied by stars that betray their presence and race around an invisible star, along with three times the sun’s mass. Such a procedure indicates the presence of black holes rather than a neutron star.

On the contrary, the solitary black holes are expected to be common, but are very hard to find. Likewise, the one in Sagittarius was identified while passing through the dim background star and additionally shifting its position due to the black hole’s gravity. Recently, Sahu’s efforts were reported in the Astrophysical Journal, about the new observations from NASA’s Hubble Space Telescope, confirming the presence of a lone black hole in Sagittarious.

Black Hole Key Findings

Although the passage occurred first in the year 2011, the original discovery relied on the Hubble measurements from the year 2011 to 2017. However, the new data has been gained from the Hubble observations from the year 2021 to 2022, accompanied by the data received from the Gaia Spacecraft.

How Big is a Black Hole?

The ideal size of this lone black home is seven times as huge as the sun. In recent observations, a different team of scientists revisited the project and identified the size as massive as six times that of the sun. The theories of the scientists match with that of Sahu’s observation.

The research continues for detecting the black holes in Sagittarius. Located at a distance of 5,000 light years away from Earth, this solitary black hole is yet to be observed from different aspects. The astronomer, Sahu, hopes to find more lone black holes with the effective use of the Nancy Grace Roman Space Telescope, which is set to launch in the year 2027.

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Mars’ Carbonate Mystery and Ancient Atmosphere Deciphered

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Mars’ Carbonate Mystery and Ancient Atmosphere Deciphered

The evolution of Mars and its ancient atmosphere has been a prominent research topic for scientists. NASA’s Curiosity Mars rover could potentially be the ultimate solution for the temperature and other details about the planet. As per the assumptions made by the researchers, Mars’s atmosphere was crafted with a thick layer of carbon dioxide whereas the surface comprised liquid water. Likewise, the presence of carbonate minerals on the planet would be the result of a potential reaction between water, carbon dioxide, and Martian rocks, researchers say.

Presence of Siderite Detected

Recently reported in the April paper of Science, the presence of siderite has been discovered within the sulfate-rich rocky layers of Mount Sharp on Mars. The discovery was made at three of Curiosity’s drill sites.

According to the lead author and Associate Professor at the University of Calgary, Canada, Benjamin Tutolo, “The discovery of abundant siderite in Gale Crater represents both a surprising and important breakthrough in our understanding of the geologic and atmospheric evolution of Mars”.

About the Drilling Process

To achieve an understanding of the chemical and mineral makeup at the surface of Mars, Curiosity drills three to four centimeters down into the subsurface. Further, the powdered rock samples are then dropped into the CheMin instrument. This instrument analyses the rocks and soil via X-ray diffraction. The CheMin instrument is driven by NASA’s Ames Research Centre in California’s Silicon Valley.

The data analysis of the discovery was conducted by scientists at the Astromaterials Research and Exploration Science (ARES) Division at NASA Johnson Space Center in Houston.

Potential Findings and Atmosphere at Mars

The discovery of this carbonate mineral could potentially be hiding other minerals beneath the surface, in near-infrared satellite analysis. The possible presence of carbonates in sulfate-rich layers across Mars may result in the amount of carbon dioxide, which will be ideal to support the liquid water and create conditions warm enough to sustain water. Also, the scientists doubt the existence of other carbonates, or maybe they might have vanished from space.

To Conclude

The missions and analyses are still undergoing, and they will continue the research in the future. The findings can be confirmed post-research on the sulfate-rice area on the red planet. As the findings arrive, they will help us understand the transformation of the planet and will offer clarity on the ancient atmosphere.

Note: Curiosity is a part of NASA’s Mars Exploration Program (MEP) portfolio. It was built by NASA’s Jet Propulsion Laboratory, managed by Caltech in Pasadena, California. The mission is successfully led by JPL on behalf of NASA’s Science Mission Directorate in Washington.

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JWST Might Have Revealed New Signs of Alien Life on Nearby Exoplanet

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JWST Might Have Revealed New Signs of Alien Life on Nearby Exoplanet

Scientists discovered suitable biosignature gases for alien life on planet K2-18b. On K2-18b, NASA’s James Webb Space Telescope (JWST) noticed dimethyl sulfide (DMS), a chemical primarily produced by living creatures on Earth. Notably, the exoplanet is nine times the size of our planet and exists in the habitable zone of its planetary system. As exoplanets pass in front of their home stars, the team probes planetary atmospheres using JWST’s Mid-Infrared Instrument (MIRI). Based on its size and other properties, astronomers think K2-18b is a “Hycean” world—that is, one with a large liquid-water ocean and a hydrogen-rich atmosphere.

Although the researchers estimate concentrations of more than 10 parts per million by volume on Earth, they are less than one part per billion. However, further research is required to confirm and expand on their findings.

NASA’s Webb Telescope Finds Possible Life Signs on Exoplanet K2-18b

According to a new study, which was published in The Astrophysical Journal Letters, chemical proof of life on the far-off exoplanet K2-18b has come from NASA’s James Webb Space Telescope. Rare on other planets or moons, these signals, which point to the presence of dimethyl sulfide and dimethyl disulfide, are found in marine plants and bacteria on Earth.

Because K2-18b boasts a hydrogen-rich atmosphere and a planet-wide ocean, researchers classify it as a “hycean world.” Methane and carbon dioxide, found in the planet’s atmosphere in 2023, were the first carbon-based compounds found in the habitable zone of an exoplanet. Though the levels had minimal statistical significance, the researchers also found likely DMS signals, therefore confounding DMS diagnosis. The results underline the possibilities of life on exoplanets.

JWST Data Hints at High Sulfur Levels on Exoplanet, Life or Not

MIRI observations from the JWST expose features in planetary atmospheres that point to DMS or DMDS helping to explain them. Scientists estimate that atmospheric DMS and DMDS levels could be substantially greater than on Earth, that is, above 10 parts per million. Differentiating DMS from DMDS requires more data. Scientists want to investigate undiscovered chemical processes involving no living entities able to generate DMS and DMDS from nothing.

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