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NASA on Tuesday celebrated exceeding expectations during a mission to deflect a distant asteroid, in a sci-fi like test of humanity’s ability to stop an incoming cosmic object from devastating life on Earth.

The fridge-sized Double Asteroid Redirection Test (DART) impactor deliberately smashed into the moonlet asteroid Dimorphos on September 26, pushing it into a smaller, faster orbit around its big brother Didymos, NASA chief Bill Nelson announced.

That changed its orbital period by four percent, or 32 minutes — from 11 hour 55 minutes to 11 hours 23 minutes, bettering an expectation of 10 minutes.

“At some point in the future, if we find an asteroid that is threatening to hit Earth, and would be large enough to really do some damage, thank goodness that we will have had this successful test,” Nelson told AFP.

The asteroid pair loop together around our Sun every 2.1 years, and pose no threat to our planet.

But they are ideal for studying the “kinetic impact” method of planetary defense.

DART’s success as a proof-of-concept has made a reality what was once science fiction — notably films such as “Armageddon,” “Deep Impact,” and “Don’t Look Up.”

Never actually photographed before, Dimorphos, which is 530 feet (160 meters) in diameter or roughly the size of a big Egyptian pyramid, appeared as a speck of light around an hour before impact.

Its egg-like shape and craggy, boulder-dotted surface finally came into clear view in the last few moments, as DART raced toward it at roughly 14,500 miles (23,500 kilometres) per hour.

Pseudo-comet 

In the days that followed, astronomers rejoiced in stunning images of matter spreading out thousands of miles — pictures collected by Earth and space telescopes, as well as a tiny companion satellite that traveled to the zone with DART.

Thanks to its temporary new tail, Dimorphos has turned into a man-made comet.

But quantifying just how well the test worked required an analysis of light patterns from ground telescopes, which took a few weeks to become apparent.

The binary asteroid system, which was around 6.8 million miles (11 million kilometres) from Earth at impact, is visible only as a single dot from the ground.

The dot’s brightness changes as Dimorphos passes in front of Didymos, which is significantly bigger at half-a-mile wide.

Four optical telescopes were involved in measuring the orbital period — all in Chile and South Africa — while two US-based radar telescopes helped confirm the finding, said NASA planetary scientist Nancy Chabot.

The test also showed scientists that the asteroid is less like a solid rock, and more like a “rubbish pile” of boulders bound by mutual gravity.

If an asteroid is more solid, the momentum imparted by a spaceship will be limited. But if significant mass is pushed at high velocity in the opposite direction to impact, there will be an additional boost.

“It looks like the recoil from the ejecta blast off the surface was a substantial contributor to the overall push given to the asteroid,” said NASA scientist Tom Statler at a briefing.

The test will serve as an “anchor point” for simulations and calculations about the outcome of future impacts, he added.

Mass extinction

No known asteroid larger than 140 meters (460 feet) in size — big enough to devastate a city — has a significant chance to hit Earth for the next 100 years, according to NASA.

But wait long enough, and it will happen.

The geological record shows, for example, that a six-mile wide asteroid struck Earth 66 million years ago, plunging the world into a long winter that led to the mass extinction of the dinosaurs along with 75 percent of all species.

The agency plans to launch in 2026 a telescope called the Near-Earth Object (NEO) Surveyor to better characterize potentially hazardous 140-meter asteroids and comets that come within 30 million miles.

So far, less than half of the estimated 25,000 NEOs of 140 meters have been discovered.

Kinetic impact with a spaceship is just one way to defend the planet, albeit the only method possible with current technology.

Should an approaching object be detected early, a spaceship could be sent to fly alongside it for long enough to divert its path via using the ship’s gravitational pull, creating a so-called gravity tractor.

Another option would be launching nuclear explosives to redirect or destroy an asteroid.

NASA believes the best way to deploy such weapons would be at a distance, to impart force without blowing the asteroid to smithereens, which could further imperil Earth.


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NASA BioSentinel Studies Space Radiation During Massive Solar Storm Event

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NASA BioSentinel Studies Space Radiation During Massive Solar Storm Event

In May 2024, a remarkable geomagnetic storm, also known as solar storm, impacted Earth, resulting in vibrant auroras that captivated observers worldwide. These stunning natural displays occur when eruptions of solar plasma, known as coronal mass ejections, collide with Earth’s magnetic field. While these events are a visual delight, they also raise significant questions about the impact of solar radiation on humans travelling beyond Earth’s atmosphere.

Exploring Radiation Risks in Space

During this geomagnetic event, NASA’s BioSentinel spacecraft took the opportunity to gather crucial data on solar radiation. This research is vital as NASA  gears up for future missions to the Moon and Mars. As noted by Sergio Santa Maria, who leads the BioSentinel project at NASA’s Ames Research Center, the timing coincided with a solar maximum, which allowed for an in-depth examination of the radiation environment in space.

BioSentinel’s Unique Mission

BioSentinel, a compact satellite roughly the size of a cereal box, is situated over 30 million miles from Earth in a solar orbit. Unlike life on Earth, which is shielded by the planet’s magnetic field, BioSentinel had to endure the full effects of the solar storm. Initial data suggest that although the storm was considerable, it was only associated with a moderate increase in solar radiation, indicating that the immediate threats to life may not be as severe as previously anticipated.

Adaptation of Scientific Goals

Originally intended to study yeast in space, BioSentinel has shifted its focus to understanding the broader implications of deep space conditions. The spacecraft’s biosensor instruments continue to provide valuable insights into the radiation environment in space. Santa Maria pointed out that despite the completion of the biological aspect of the mission, BioSentinel still holds significant scientific relevance, demonstrating its capability for future long-duration missions.

Conclusion: The Importance of Ongoing Research

The spectacular auroras that light up the night sky serve as a reminder of the unseen forces governing our solar system. As NASA and its collaborators seek to deepen their understanding of space environments, the data collected by missions like BioSentinel is essential. This research not only enhances our knowledge of solar radiation but also informs the safety and success of future human explorations beyond Earth.

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This Strange Fisht Can Taste Using Its Crab-Like Legs, Says Study

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This Strange Fisht Can Taste Using Its Crab-Like Legs, Says Study

The northern sea robin (Prionotus carolinus) is an intriguing marine species known for its remarkable adaptations. Unlike most fish, this species employs its six leg-like appendages to navigate the ocean floor. This ability allows it not only to move but also to explore the sea bed in search of food. While this capability was long known in the scientific community, another strange use case of its leg was recently discovered.

Sensory Capabilities of Sea Robins

Recent studies have illuminated how these legs function as sensory organs. Researchers observed that the northern sea robin is capable of detecting buried prey through chemical cues released into the water. Using its shovel-like feet, the fish can unearth hidden food sources, demonstrating a unique blend of mobility and sensory detection.

Research Collaboration and Findings

A collaborative research effort involving developmental biologist David Kingsley from Stanford University and molecular biologist Nicholas Bellono from Harvard University examined the sea robin’s sensory adaptations. The study was published in the journal Current Biology. Their experiments placed the fish in environments with buried mussels and amino-acid capsules. The results confirmed the fish’s efficiency in locating and retrieving these hidden items, thanks to the specialized bumps on its legs, known as papillae, which house taste receptors.

Evolutionary Insights into Adaptation

The evolutionary background of the northern sea robin reveals an intriguing narrative. An evolutionary analysis of various sea robin species indicated that while the legs initially developed for locomotion, their sensory capabilities evolved later. The researchers identified the tbx3a gene as a key factor in the development of these legs, and using CRISPR technology, they demonstrated that altering this gene can impact both leg formation and sensory function.

Conclusion: Implications of the Research

The findings from this research not only enhance our understanding of the northern sea robin but also provide broader insights into how species adapt over time. By exploring the genetic and evolutionary pathways that led to such unique adaptations, scientists can better understand the complexities of marine life and the evolutionary processes that shape it.

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This Is How the Earth Might Escape Eventual Death After the Sun Explodes

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This Is How the Earth Might Escape Eventual Death After the Sun Explodes

A planetary system anchored by a white dwarf star, located approximately 4,000 light-years away, provides astronomers with insights into what could happen to our Sun and Earth in about 8 billion years. This scenario unfolds if the Earth survives the Sun’s transformation into a red giant, expected to occur in 5 to 6 billion years. During this phase, the Sun will expand, potentially engulfing Mercury, Venus, and possibly Earth before shrinking into a white dwarf.

The Potential for Earth’s Survival

One scenario for Earth’s survival involves its migration to an orbit similar to Mars or beyond, resulting in a radiation-battered yet frozen world orbiting a burnt-out star, as per a study published in the journal Nature Astronomy. The newly discovered system reveals a white dwarf with half the mass of the Sun and an Earth-sized planet in a wider orbit, showcasing what a surviving Earth might resemble.

Keming Zhang, a researcher from the University of California, San Diego, highlighted that there is no consensus on whether Earth could escape being swallowed by the red giant Sun. This system stands out because it also contains a massive companion, likely a brown dwarf, which is a stellar body that fails to ignite nuclear fusion.

The Discovery Process

The planetary system was identified through a microlensing event, where the gravitational influence of a body distorts the light from a more distant source. Observations of this event, dubbed KMT-2020-BLG-0414, were conducted using the Korea Microlensing Telescope Network. The investigation continued with the Keck telescopes in Hawaii, ultimately confirming the nature of the central star as a white dwarf based on the absence of light expected from a main sequence star.

Future Habitable Possibilities

While this discovery suggests that Earth could escape destruction, it raises questions about the potential for life to persist on our planet. Jessica Lu, an astronomer at UC Berkeley, noted that while Earth may avoid being engulfed, it might not remain habitable during the Sun’s red giant phase. The habitable zone will shift beyond Earth’s orbit, with Zhang suggesting that humanity might need to consider migrating to the moons of Jupiter or Saturn, which could become viable ocean worlds as the Sun expands.

Conclusion

This research illustrates the significance of microlensing in exploring planetary systems. The upcoming Nancy Grace Roman Telescope, set for launch in 2027, is expected to enhance our ability to discover and study exoplanets, potentially unveiling more unique configurations in the cosmos.

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