
NASA's Parker Probe Captures Closest-Ever Image Of The Sun
NASA's Parker Probe captured the first-ever images from inside a solar eruption, offering vital clues about space weather and its effects on Earth
The Sun, Earth's most powerful energy source, has long been a subject of awe and concern due to its sheer scale and volatile nature. Now, NASA's Parker Solar Probe has delivered astonishing new images that provide a close-up look inside the Sun's atmosphere; images as mesmerising as they are menacing.
Closest Flyby Reveals Intense Solar Activity
On December 24, 2024, the Parker Solar Probe made its closest-ever approach to the Sun, reaching just 3.8 million miles from its surface. During this moment, the onboard WISPR camera (Wide-field Imager for Parker Solar Probe) captured a live eruption of a Coronal Mass Ejection (CME).
This marks the first time scientists have directly recorded such a violent solar event from within, rather than simulating it through models.
Deadly Solar Waves Observed First-Hand
Within the CME, scientists observed Kelvin-Helmholtz Instabilities—swirling, wave-like patterns formed by the collision of solar flows. Once considered purely theoretical or seen only in simulations, these dangerous waveforms have now been witnessed in real solar conditions.
Unprecedented Footage From Inside the Corona
NASA released a video showing the Sun's corona from the probe's perspective.
According to Angelos Vourlidas from Johns Hopkins University, USA, the footage shows CMEs colliding and merging, giving researchers insight into how space weather forms and evolves.
NASA's Dr Nicky Fox added, 'We are finally seeing where Earth's space weather begins".
Against All Odds: The Probe Survives Extreme Heat
Despite temperatures above 1,300°C and intense radiation, the Parker Probe emerged undamaged. NASA engineers regard this survival as a historic feat in space engineering.
What's Next For Parker?
The probe's next flyby is set for September 15, 2025, where it will venture even closer to the Sun. Scientists are optimistic that this mission will help decode the origin of solar winds, which are critical in understanding and forecasting space weather.
Why This Matters For Earth
Space weather caused by CMEs can disrupt satellites, GPS systems, radio signals, and even power grids on Earth. These new findings will help scientists build better early-warning systems, protecting both astronauts and everyday technologies on Earth.
view comments
First Published:
July 12, 2025, 14:06 IST
Disclaimer: Comments reflect users' views, not News18's. Please keep discussions respectful and constructive. Abusive, defamatory, or illegal comments will be removed. News18 may disable any comment at its discretion. By posting, you agree to our Terms of Use and Privacy Policy.
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles


Time of India
an hour ago
- Time of India
Astronomers discover blazing Betelgeuse has companion star
This is an AI generated image. Used for representation purpose only. Since at least the time of the ancient Egyptians, people across the world have gazed up in awe at Betelgeuse , one of the brightest stars blazing in the night sky. Now astronomers have discovered that this red supergiant , known to many as the hunter's shoulder in the Orion constellation , is being orbited by a much smaller companion star , a study said on Monday. It is not the first time Betelgeuse has surprised stargazers. Seemingly out of nowhere, the giant star dramatically dimmed for five months between 2019 and 2020, leading some scientists to suggest it could soon die in an epic supernova explosion. Further observations revealed that this event -- known as the " Great Dimming " -- was actually caused by material ejected from the surface that cooled part of the star, creating a dust cloud that blocked its light. by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Swelling and internal bleeding in the brain, help this baby Donate For Health Donate Now Undo But scientists could still not explain why Betelgeuse's brightness changes regularly, both on a 400-day cycle and another that lasts nearly six years. In a paper titled "A Buddy for Betelgeuse" published in December, some researchers theorised that the longer variation could be caused by a hidden small star orbiting the behemoth. Astronomers using the Gemini North telescope in Hawaii have now discovered this elusive companion, according to a new study in The Astrophysical Journal Letters. - Little buddy - This companion has a mass around 1.5 times greater than our Sun, the research estimated. That means it is dwarfed by Betelgeuse, which is 1,000 times bigger than the Sun. The companion star is around four times the distance from Betelgeuse as the Earth is from the Sun, which is quite close for a stellar companion. The discovery is the first time such a close companion star has been detected orbiting a supergiant, according to a statement from the US research centre NOIRLab, which operates the Gemini Observatory. Betelgeuse is more than 10,000 times brighter than the Sun, its blinding light making spotting anything nearby difficult. Steve Howell, a NASA scientist who led the research team, said previous "papers that predicted Betelgeuse's companion believed that no one would likely ever be able to image it". However the Gemini North telescope was able to spot the much smaller, dimmer star using a technique called speckle imaging. This involves assembling many images taken with short exposure times to overcome the distortions that Earth's atmosphere causes ground-bound telescopes. According to Greek myth, the giant hunter Orion claimed he would kill all the world's beasts, so Earth goddess Gaia sent a scorpion to kill him. God king Zeus then turned both Orion and the scorpion -- Scorpius -- into constellations. Earlier, ancient Egyptians included Betelgeuse in the constellation Osiris, their god of the dead. Even earlier, research has suggested that Indigenous Australians included Betelgeuse in their own constellations -- and had noticed the star's varying brightness.


The Hindu
3 hours ago
- The Hindu
Telescopes spot start of planet formation in Orion
When rocky worlds like the earth began to form, dust in the young Solar System was first heated until it vaporised and then cooled so that the very first, refractory (i.e. heat-loving) minerals could crystallise. Catching that moment in another star system would show astronomers exactly how planet formation begins — but no one had seen it before. A new study in Nature this month has reported just such an event. By examining the star HOPS‑315 in Orion, whose protoplanetary disc is tilted just enough for someone on or near the earth to peer deeper within, researchers from France, the Netherlands, Sweden, Taiwan, and the US observed raw rock vapour cool and crystallise. The protoplanetary disc is a flat, rotating pancake-shaped mass of gas and dust that surrounds a newborn star. Inside it, dust grains bump together, stick, and gradually grow into rocks, planets, moons, and other bodies while the gas creates atmospheres and influences the planets' long-term orbits. The observations themselves were conducted by the NASA James Webb Space Telescope and the Atacama Large Millimeter/sub‑millimeter Array (ALMA) observatory in Chile. In 2023, the team used the NIRSpec and MIRI integral‑field spectrographs onboard the telescope to collect sharp energy readings across a range of frequencies. Eight months later, ALMA observed the same system for signs of carbon monoxide, silicon monoxide and sulphur monoxide. Together, the telescope traced warm gas and dust only a few stellar radii from the star while ALMA mapped cooler gas farther out. The telescope's data contained evidence of a strong band of silicon monoxide gas at around 470 K as well as crystalline silicates. Both lay within 2.2 AU of the star — well inside Mercury's orbit if this were in the solar system. (1 AU equals the earth-sun distance.) The team also ran computer simulations, which predicted that around 1 AU from the star, temperatures hovered around 1,300 K, which is the temperature at which dust just begins to evaporate. The study's energy readings matched the prediction: that interstellar grains must have vaporised there, releasing silicon monoxide gas that then cooled and re-condensed into fresh shards of crystals. According to the study, the relative quantities of crystals of forsterite, enstatite, and tentative silica were reminiscent of inclusions — i.e. minerals trapped inside minerals — that have been found in primitive meteorites on the earth, meaning that a similar condensation chemistry is under way around the star. The ALMA data also revealed no slow silicon monoxide at the star's position whereas the Webb telescope's data was blueshifted by around 10 km/s. Together, they indicate that the minerals lay inside the rising disc atmosphere, the thin upper layer of gas and dust above the mid‑plane of the protoplanetary disc, rather than in the material pouring out of the star. Thus the study has reported the first evidence of solid matter condensing out of rock vapour around a star, a.k.a. the first step of planet formation.


Economic Times
3 hours ago
- Economic Times
Jupiter's moon Europa is not what it looks like; shocking revelations from new study break scientists' decades-old beliefs
A recent study revealed several new observations about the hidden chemistry of the icy interior of Jupiter's moon Europa, challenging scientists' long-held beliefs. Jupiter's moon Europa has been a subject of deep study for scientists, which has led to several observations over decades. A study that was carried out recently revealed many fresh observations about the hidden chemistry of the icy moon's interior, which challenge the long-held beliefs of scientists. According to the latest observations made by the James Webb Space Telescope, it was revealed that Europa's frozen surface is a dynamic world that's far from frozen in time. The findings came as a surprise to scientists who had pictured Europa's frozen surface as a still and silent shell for decades. "We think that the surface is fairly porous and warm enough in some areas to allow the ice to recrystallize rapidly," Richard Cartwright, a spectroscopist at Johns Hopkins University's Applied Physics Laboratory and lead author of the new study, said in a statement, according to What's even more intriguing is what this surface activity tells us about Europa's subsurface ocean. The geologic activity and constant exchange between the surface and the subsurface make 'chaos terrains.' These are areas where ice blocks have broken apart, moved, and refrozen. These regions are especially valuable because they might offer direct access to what's happening inside Europa's interior. The latest study focused on two regions in Europa's southern hemisphere: Tara Regio and Powys Regio. Tara Regio stands out as one of the moon's most intriguing areas. According to observations from the JWST, crystalline ice exists both on Europa's surface and deeper below, challenging previous assumptions about how ice is distributed there. Scientists can have access to valuable insights pertaining to Europa's chemistry as well as its potential for habitability, they explained in the paper, by measuring the spectral properties of these "chaos" regions using remotely sensed data. The paper was published on May 28, 2025, in The Planetary Science Journal."Our data showed strong indications that what we are seeing must be sourced from the interior, perhaps from a subsurface ocean nearly 20 miles (30 kilometers) beneath Europa's thick icy shell," Ujjwal Raut, program manager at the Southwest Research Institute and co-author of the study, said in the statement, understand how water freezes on Europa, Ujjwal Raut and his team carried out laboratory experiments. The surface is constantly bombarded on Europa by charged particles from ice structure on Europa is disrupted by the intense radiation, which is not the case on Earth, where ice naturally forms a hexagonal crystal structure. The radiation on Europa causes the ice to become what's known as amorphous ice. It is a disordered, noncrystalline experiments were crucial, as they played a key role in demonstrating how the ice changes over time. By studying the manner in which ice transforms between different states, scientists can learn more about the moon's surface dynamics. The observations through the experiments, combined with fresh data from JWST, add to a set of findings showing that a vast, hidden liquid ocean lies beneath Europa's icy shell."In this same region […] we see a lot of other unusual things, including the best evidence for sodium chloride, like table salt, probably originating from its interior ocean," Cartwright said. "We also see some of the strongest evidence for CO2 and hydrogen peroxide on Europa. The chemistry in this location is really strange and exciting," he regions, marked by fractured surface features, may point to geologic activity pushing material up from beneath Europa's icy shell.