If you were expecting that gossipy bullshyt sorry but this is about science.
Spacecraft will fly through the Sun's atmosphere tomorrow for the first time ever
NASA’s Parker Solar Probe is set to achieve its most dangerous feat yet tomorrow, December 24, 2024. After a six-year journey of spiraling closer to the star at the heart of our solar system, the spacecraft is expected to come within 3.8 million miles of the Sun’s surface.
This tiny distance in cosmic terms lets scientists capture a new type of information, revealing secrets about solar winds, extreme heat, and magnetic fields
Engineers have spent years carefully adjusting Parker’s flight path using multiple Venus gravity assists. These flybys reshape the spacecraft’s orbit and tighten its looping path around the Sun.
“This is one example of NASA’s bold missions, doing something that no one else has ever done before to answer longstanding questions about our universe,” explained Arik Posner, Parker Solar Probe program scientist at NASA Headquarters, describing this mission’s significance.
Ever since the launch in 2018, Parker’s main goal has been to study the Sun’s outer atmosphere, known as the corona. Tomorrow’s approach, often called perihelion, marks a new milestone in that quest.
The probe moves at speeds around 430,000 miles per hour, faster than any other spacecraft. At such high velocity, it can swing around our star without getting swallowed.
Even so, mission managers won’t receive immediate updates once Parker hits its closest point because signals cannot travel through the intense solar environment.
What sets Parker apart is its resilient heat shield. This 4.5-inch-thick carbon-composite barrier enables the spacecraft’s instruments to continue functioning in an environment where temperatures can reach roughly 2,500 degrees Fahrenheit.
Despite the harsh surroundings, the precious science instruments remain near room temperature, thanks to expert engineering by Johns Hopkins University Applied Physics Laboratory (APL).
During every close approach, Parker is pelted by gusts of solar wind and bathed in radiation. Still, it keeps sending back readings about magnetic fields, plasma behavior, and energetic particles.
The probe’s data illuminates reasons behind the corona’s blazing heat, which can climb into the millions of degrees, significantly hotter than the visible surface of the Sun. Such puzzling behavior has fascinated scientists for decades.
Solar wind, a stream of charged particles flowing away from the Sun at speeds topping one million miles per hour, plays a major role in space weather.
By skimming through the corona, Parker records fresh evidence of how these particles speed up and scatter across the solar system.
The answers may help experts forecast disturbances that affect satellites and astronaut safety. Surges of these charged particles can disable communication systems or even disrupt power grids on Earth.
For researchers, big questions remain. How does the solar wind pick up its pace so dramatically? Is there a specific region in the corona that triggers bursts of fast-moving particles?
This is why Parker’s findings are so relevant. Gaining a better understanding of how energetic solar events begin could lead to timelier warnings, giving operators on Earth a heads-up to power down sensitive instruments or adjust satellite orbits.
Spacecraft will fly through the Sun's atmosphere tomorrow for the first time ever
NASA’s Parker Solar Probe is set to achieve its most dangerous feat yet tomorrow, December 24, 2024. After a six-year journey of spiraling closer to the star at the heart of our solar system, the spacecraft is expected to come within 3.8 million miles of the Sun’s surface.
This tiny distance in cosmic terms lets scientists capture a new type of information, revealing secrets about solar winds, extreme heat, and magnetic fields
Engineers have spent years carefully adjusting Parker’s flight path using multiple Venus gravity assists. These flybys reshape the spacecraft’s orbit and tighten its looping path around the Sun.
“This is one example of NASA’s bold missions, doing something that no one else has ever done before to answer longstanding questions about our universe,” explained Arik Posner, Parker Solar Probe program scientist at NASA Headquarters, describing this mission’s significance.
Ever since the launch in 2018, Parker’s main goal has been to study the Sun’s outer atmosphere, known as the corona. Tomorrow’s approach, often called perihelion, marks a new milestone in that quest.
The probe moves at speeds around 430,000 miles per hour, faster than any other spacecraft. At such high velocity, it can swing around our star without getting swallowed.
Even so, mission managers won’t receive immediate updates once Parker hits its closest point because signals cannot travel through the intense solar environment.
What sets Parker apart is its resilient heat shield. This 4.5-inch-thick carbon-composite barrier enables the spacecraft’s instruments to continue functioning in an environment where temperatures can reach roughly 2,500 degrees Fahrenheit.
Despite the harsh surroundings, the precious science instruments remain near room temperature, thanks to expert engineering by Johns Hopkins University Applied Physics Laboratory (APL).
During every close approach, Parker is pelted by gusts of solar wind and bathed in radiation. Still, it keeps sending back readings about magnetic fields, plasma behavior, and energetic particles.
The probe’s data illuminates reasons behind the corona’s blazing heat, which can climb into the millions of degrees, significantly hotter than the visible surface of the Sun. Such puzzling behavior has fascinated scientists for decades.
Solar wind, a stream of charged particles flowing away from the Sun at speeds topping one million miles per hour, plays a major role in space weather.
By skimming through the corona, Parker records fresh evidence of how these particles speed up and scatter across the solar system.
The answers may help experts forecast disturbances that affect satellites and astronaut safety. Surges of these charged particles can disable communication systems or even disrupt power grids on Earth.
For researchers, big questions remain. How does the solar wind pick up its pace so dramatically? Is there a specific region in the corona that triggers bursts of fast-moving particles?
This is why Parker’s findings are so relevant. Gaining a better understanding of how energetic solar events begin could lead to timelier warnings, giving operators on Earth a heads-up to power down sensitive instruments or adjust satellite orbits.
Spacecraft will fly through the Sun's atmosphere tomorrow for the first time ever
After a six-year journey, the Parker Solar Probe will fly through the Sun's atmosphere on December 24, 2024.
www.earth.com