Yazılar

NASA’s Parker Solar Probe Makes Closest-Ever Approach to the Sun

/in /tarafından

NASA’s Parker Solar Probe is embarking on a historic mission, attempting the closest-ever approach to the Sun. The spacecraft is plunging into the Sun’s outer atmosphere, known as the corona, enduring extreme temperatures and radiation in a bid to unlock the mysteries of our star.

This daring fly-by will leave the probe out of communication for several days. Scientists will anxiously await a signal, expected at 05:00 GMT on 28 December, to confirm whether the probe has survived the intense conditions. The goal is to deepen our understanding of the Sun’s behavior and how it affects the solar system.

Dr. Nicola Fox, NASA’s head of science, emphasized the importance of firsthand exploration: “For centuries, people have studied the Sun, but you don’t experience the atmosphere of a place until you actually go visit it. And so we can’t really experience the atmosphere of our star unless we fly through it.”

Launched in 2018, the Parker Solar Probe has already completed 21 orbits around the Sun, gradually getting closer with each pass. The Christmas Eve mission is a groundbreaking moment, bringing the probe within 3.8 million miles (6.2 million km) of the Sun’s surface. Though this distance may seem vast, Fox puts it into perspective: “We are 93 million miles away from the Sun, so if I put the Sun and the Earth one metre apart, Parker Solar Probe is just four centimetres from the Sun.”

During its approach, the spacecraft will endure temperatures of 1,400°C (2,552°F) and radiation strong enough to damage its electronics. To protect it, the probe is shielded by a 11.5cm-thick (4.5 inches) carbon-composite heat shield. The spacecraft’s strategy is to fly in and out quickly, racing at an astonishing speed of 430,000 mph (700,000 km/h) — faster than any man-made object in history.

The Parker Solar Probe’s primary mission is to investigate the Sun’s corona, which remains an enigma for scientists. Dr. Jenifer Millard, an astronomer, explains, “The surface of the Sun is about 6,000°C, but the corona reaches millions of degrees — and it’s farther from the Sun. How is the outer atmosphere getting hotter?”

The probe’s journey will also help scientists study solar wind, the constant flow of charged particles from the corona. This space weather can lead to phenomena like auroras, but it can also disrupt power grids, communication systems, and electronics on Earth. “Understanding the Sun and its activity is so important to our everyday lives on Earth,” says Dr. Millard.

As the spacecraft is out of contact with Earth, NASA scientists are anxiously awaiting the return of a signal. Fox admitted to feeling nervous about the probe’s audacious attempt but remains confident in its design. “We really have designed it to withstand all of these brutal conditions. It’s a tough, tough little spacecraft,” she says.

If successful, the Parker Solar Probe will continue its groundbreaking mission, providing valuable insights into the Sun’s behavior and its impact on space weather for years to come.

 

Solar Orbiter Captures Record-Breaking Images of the Sun’s Surface

/in /tarafından

Unveiling the Sun’s Secrets

The Solar Orbiter mission has captured the highest-resolution images of the sun’s surface, offering unprecedented insights into the dynamics of our star. These stunning visuals reveal intricate details of sunspots, plasma movements, and the magnetic fields that govern solar activity, providing scientists with valuable data to further understand solar phenomena.

The images, taken on March 22, 2023, and released this week, were captured using the spacecraft’s Extreme Ultraviolet Imager (EUI) and Polarimetric and Helioseismic Imager (PHI). Positioned 46 million miles from the sun, the Solar Orbiter, a joint mission by the European Space Agency (ESA) and NASA, captured these extraordinary views, marking a significant leap in heliophysics research.

Cutting-Edge Observations

The Solar Orbiter’s PHI instrument produced the sharpest full-surface views of the sun’s photosphere, where temperatures range between 8,132°F and 10,832°F (4,500°C and 6,000°C). These images reveal sunspots, dark regions caused by the sun’s strong magnetic fields, which disrupt convection and make the spots cooler and darker than their surroundings.

The PHI also created detailed magnetic maps, or magnetograms, showing magnetic field concentrations in sunspot areas. A velocity map, or tachogram, highlighted the speed and direction of plasma flows across the surface, with blue regions indicating movement toward the spacecraft and red regions moving away.

Meanwhile, the EUI focused on the sun’s corona, its outermost atmosphere, where temperatures soar to 1.8 million degrees Fahrenheit (1 million degrees Celsius). The corona’s glowing plasma structures, protruding from sunspot regions, were vividly captured, helping scientists probe why this layer is significantly hotter than the surface below.

Each image released by the Solar Orbiter is a mosaic of 25 individual shots, meticulously pieced together due to the spacecraft’s need to rotate while capturing the sun’s entire face.

Complementing Parker Solar Probe

While NASA’s Parker Solar Probe will soon make its closest approach to the sun, coming within 3.86 million miles on December 24, its mission lacks imaging capabilities due to its proximity to extreme heat. Solar Orbiter’s imaging instruments, however, are filling this gap, offering complementary data for scientists studying the sun’s magnetic field, solar winds, and other phenomena.

“The closer we look, the more we see,” said Mark Miesch, a NOAA scientist. “These high-resolution images bring us closer to understanding the sun’s intricate interplay of magnetic fields and plasma flows.”

Solar Activity Peaks

Solar Orbiter’s observations come at an opportune time, as the sun has reached its solar maximum — the peak of activity in its 11-year cycle. During this phase, sunspots proliferate, magnetic poles flip, and solar activity increases, generating phenomena such as flares and coronal mass ejections (CMEs). These events produce space weather that can affect Earth’s power grids, satellites, and communication systems.

The sun’s heightened activity also creates spectacular auroras, with charged particles from CMEs interacting with Earth’s atmosphere to produce the northern and southern lights.

Solar Orbiter’s mission aligns with this dynamic period, allowing scientists to correlate its high-resolution imagery with real-time solar activity.

Paving the Way for Solar Science

With its groundbreaking instruments, Solar Orbiter is helping answer fundamental questions about the sun, such as the origin of solar winds and the reason behind the corona’s extreme temperatures. Together with the Parker Solar Probe, these missions are reshaping our understanding of the sun’s impact on the solar system and Earth.