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Black Holes

“Unveiling the Secrets of the Sun: NASA’s Parker Solar Probe Reveals the Origins of Solar Storms”

In its closest-ever dive into the Sun’s atmosphere, NASA’s Parker Solar Probe has returned stunning new images and data that bring scientists closer to solving one of the Sun’s biggest mysteries: how the solar wind is born. Captured from just 3.8 million miles away, the footage shows chaotic collisions of solar eruptions, twisting magnetic fields, and the origin zones of the solar wind—phenomena that shape space weather and can disrupt life on Earth. This unprecedented view from inside the corona is helping scientists understand and predict the Sun’s violent behavior like never before.

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NASA’s Parker Solar Probe has captured stunning new images from within the Sun’s atmosphere, revealing the origins of solar storms that can affect Earth. The probe, which flew closer to the Sun than ever before, has helped scientists better understand the Sun’s influence across the solar system.

The newly released images show the corona and solar wind, a constant stream of electrically charged particles from the Sun that rage across the solar system. The solar wind expands throughout the solar system with wide-ranging effects, including generating auroras, stripping planetary atmospheres, and inducing electric currents that can overwhelm power grids and affect communications at Earth.

Understanding the impact of solar wind starts with understanding its origins at the Sun. The WISPR images give scientists a closer look at what happens to the solar wind shortly after it is released from the corona. The images show the important boundary where the Sun’s magnetic field direction switches from northward to southward, called the heliospheric current sheet.

The collision of multiple coronal mass ejections (CMEs), or large outbursts of charged particles, has been captured for the first time in high resolution. “In these images, we’re seeing the CMEs basically piling up on top of one another,” said Angelos Vourlidas, the WISPR instrument scientist at the Johns Hopkins Applied Physics Laboratory.

When CMEs collide, their trajectory can change, making it harder to predict where they’ll end up. Their merger can also accelerate charged particles and mix magnetic fields, which makes the CMEs’ effects potentially more dangerous to astronauts and satellites in space and technology on the ground.

The solar wind was first theorized by preeminent heliophysicist Eugene Parker in 1958. His theories about the solar wind, which were met with criticism at the time, have now been confirmed through Parker Solar Probe’s close-up views of the Sun.

As it spiraled closer to the Sun, Parker Solar Probe helped scientists pinpoint the origin of switchbacks at patches on the visible surface of the Sun where magnetic funnels form. The fast solar wind, which travels at just 220 miles per second, has been shown to be in part powered by these switchbacks, adding to a 50-year-old mystery.

The slow solar wind, which is twice as dense and more variable than fast solar wind, is important to study because its interplay with the fast solar wind can create moderately strong solar storm conditions at Earth sometimes rivaling those from CMEs. Prior to Parker Solar Probe, distant observations suggested there are actually two varieties of slow solar wind, distinguished by the orientation or variability of their magnetic fields.

One type of slow solar wind, called Alfvénic, has small-scale switchbacks. The second type, called non-Alfvénic, doesn’t show these variations in its magnetic field. As it spiraled closer to the Sun, Parker Solar Probe confirmed there are indeed two types.

Its close-up views are also helping scientists differentiate the origins of the two types, which scientists believe are unique. The non-Alfvénic wind may come off features called helmet streamers — large loops connecting active regions where some particles can heat up enough to escape — whereas Alfvénic wind might originate near coronal holes, or dark, cool regions in the corona.

In its current orbit, bringing the spacecraft just 3.8 million miles from the Sun, Parker Solar Probe will continue to gather additional data during its upcoming passes through the corona to help scientists confirm the slow solar wind’s origins. The next pass comes Sept. 15, 2025.

Astrophysics

Harnessing the Power of Black Holes: A Tiny Spacecraft’s Quest to Rewrite Physics

A visionary plan proposes sending a paperclip-sized spacecraft, powered by Earth-based lasers, to a nearby black hole within a century. Led by astrophysicist Cosimo Bambi, the mission would test the limits of general relativity and explore the mysteries of event horizons. While current technology can t yet achieve it, advancements in nanocraft design, laser propulsion, and black hole detection could make the journey possible within decades, potentially rewriting the laws of physics as we know them.

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The possibility of sending a tiny spacecraft to a nearby black hole has sparked excitement among astrophysicists. Cosimo Bambi, an expert on black holes, has outlined the blueprint for such a mission in the journal iScience. If successful, this century-long journey could revolutionize our understanding of physics and the laws governing space and time.

Bambi believes that with advancements in technology, it’s not entirely impossible to achieve this feat. The first challenge lies in finding a black hole close enough to target. Previous knowledge suggests there might be one lurking 20-25 light-years from Earth, but detecting it won’t be easy due to their invisible nature. Instead, scientists study them by observing the effects they have on nearby stars or distortions in light.

New techniques for discovering black holes may lead to finding a nearby one within the next decade. Once identified, the next hurdle is getting there with a spacecraft that can withstand the journey. Bambi proposes using nanocrafts – gram-scale probes consisting of a microchip and light sail – accelerated by Earth-based lasers to a third of the speed of light.

At this pace, the craft could reach a black hole 20-25 light-years away in about 70 years, with data gathering taking another two decades to get back to Earth. This would make the total mission duration around 80-100 years. Upon reaching the black hole, researchers can run experiments to answer pressing questions like: does it truly have an event horizon? Do the rules of physics change near a black hole? And does Einstein’s theory of general relativity hold under extreme conditions?

Bambi acknowledges that creating such a spacecraft is currently beyond our capabilities and would require significant advancements in technology. However, with advancements in funding and technological progress over the next 30 years, he believes it may be possible to make this vision a reality.

As Bambi notes, people once thought detecting gravitational waves or observing black hole shadows was impossible, but we achieved those milestones within a century. This work highlights the power of human ingenuity and our relentless pursuit of understanding the universe’s secrets.

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Astrophysics

A Star’s Second Act: Uncovering the Secrets of Black Hole Encounters

This is the first confirmed case of a star that survived an encounter with a supermassive black hole and came back for more. This discovery upends conventional wisdom about such tidal disruption events and suggests that these spectacular flares may be just the opening act in a longer, more complex story.

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The discovery of a star that survived an encounter with a supermassive black hole and came back for more has left astronomers stunned. For decades, scientists have observed spectacular flares caused by stars falling onto these cosmic monsters, only to be destroyed in the process. However, a team of researchers from Tel Aviv University has made a groundbreaking finding: one such flare, named AT 2022dbl, was repeated nearly two years after its initial occurrence, suggesting that at least part of the star survived.

Led by Dr. Lydia Makrygianni and Prof. Iair Arcavi, the study published in the Astrophysical Journal Letters reveals that this flare might not have been a full stellar disruption as previously thought. Instead, it could be a result of the partial destruction of the star, with much of its material surviving to come back for a second, nearly identical passage.

The implications of this finding are significant. If future flares from the same location occur at regular intervals, it would suggest that these events might not be one-off occurrences but rather part of a more complex and dynamic process. “This discovery upends conventional wisdom about such tidal disruption events,” says Prof. Arcavi. “We’ll have to re-write our interpretation of these flares and what they can teach us about the monsters lying in the centers of galaxies.”

The study’s findings also challenge long-held assumptions about black holes, which are notoriously difficult to study due to their complete darkness. By observing the aftermath of a star’s encounter with a supermassive black hole, scientists have gained valuable insights into these enigmatic objects.

As researchers continue to investigate this phenomenon, they may uncover even more secrets about the complex interactions between stars and supermassive black holes. The question now is: will we see a third flare after two more years, in early 2026?

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Black Holes

Radar on NASA’s Europa Clipper Mission Successfully Conducts First Big Test

NASA’s Europa Clipper spacecraft just aced a key radar test while flying past Mars, proving its ability to detect structures beneath planetary surfaces—something that couldn’t be tested on Earth. The radar, known as REASON, will eventually be used to explore Europa, an icy moon of Jupiter believed to harbor a subsurface ocean.

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The NASA Europa Clipper mission has achieved a significant milestone by successfully testing its Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) instrument during a flyby of Mars in March. The test, which was impossible to conduct on Earth due to the scale and complexity of the radar system, aimed to determine the radar’s readiness for the mission at Jupiter’s moon Europa.

The REASON instrument, which will “see” into Europa’s icy shell, may have pockets of water inside, uses two pairs of slender antennas that jut out from the solar arrays, spanning a distance of about 58 feet (17.6 meters). This unusual radar setup for an interplanetary spacecraft was designed to catch as much light as possible at Europa, which receives only about 1/25th the sunlight as Earth.

During the Mars flyby, REASON sent and received radio waves for about 40 minutes, collecting a wealth of data that will help scientists understand how the ice may capture materials from the ocean and transfer them to the surface of the moon. The instrument’s performance was deemed successful, with engineers able to collect 60 gigabytes of rich data.

The Europa Clipper mission’s primary goal is to determine the thickness of the ice shell on Europa and its interactions with the ocean below. The REASON radar will play a crucial role in achieving this objective, providing scientists with valuable insights into the moon’s composition and geology. With the success of the REASON test, the mission is now one step closer to unlocking the secrets of Jupiter’s icy moon and potentially discovering habitable worlds beyond our planet.

The Europa Clipper spacecraft is currently on its journey to reach Europa, which will take approximately 1.8 billion miles (2.9 billion kilometers) and include a gravity assist using Earth in 2026. The mission is managed by Caltech, led by NASA’s Jet Propulsion Laboratory, and includes partners such as the Johns Hopkins Applied Physics Laboratory and NASA’s Science Mission Directorate.

As scientists continue to analyze the data from the REASON test, they are exercising their skills and preparing for the detailed exploration of Europa that will take place in the future. The mission has the potential to revolutionize our understanding of the solar system and provide new insights into the astrobiological potential of habitable worlds beyond Earth.

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