Parker Solar Probe
NASA's mission to touch the Sun begins its journey in 2018
We've been studying the Sun from afar for decades, and Parker Solar Probe will finally go where the action is. Our Sun is far more complex than meets the eye: The Sun's atmosphere constantly sends magnetized material outward, enveloping our solar system far beyond the orbit of Pluto and influencing every world along the way. The impact of solar activity on Earth and other worlds are collectively known as space weather, and the key to understanding its origins lies in understanding the Sun itself. NASA and the Johns Hopkins Applied Physics Laboratory's Parker Solar Probe launches in August 2018 to the Sun to make direct measurements of the Sun's corona where outgoing material, known as the solar wind, originates. Though we largely grasp the solar wind's origins on the Sun, we know there is a point – as-yet unobserved – where the solar wind is accelerated to supersonic speeds. Scientists also hope to learn the secret of the corona's enormously high temperatures. The visible surface of the Sun is about 10,000 F – but, for reasons we don't fully understand, the corona is hundreds of times hotter, spiking up to several million degrees F. This is counterintuitive, as the Sun's energy is produced at its core. The spacecraft's instruments should also shed light on the mechanisms at work behind the acceleration of solar energetic particles, which can reach speeds more than half as fast as the speed of light as they rocket away from the Sun. Watch the videos to learn more.
Explore the mysteries of the Sun that Parker Solar Probe will seek to answer.
Learn why Parker Solar Probe won't melt when it flies through the Sun's corona.
The solar wind is a constant stream of charged particles that emanate from the Sun and affect all the planets in the solar system.
Parker Solar Probe uses remote and direct measurements to collect data about the Sun.
Parker Solar Probe was designed and built at the Johns Hopkins University Applied Physics Laboratory.
Credits
Please give credit for this item to:
NASA's Scientific Visualization Studio
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Animators
- Steve Gribben (Johns Hopkins University/APL)
- Brian Monroe (USRA)
- Josh Masters (USRA)
- Michael Lentz (USRA)
- Mary P. Hrybyk-Keith (TRAX International)
- Walt Feimer (KBR Wyle Services, LLC)
- Adriana Manrique Gutierrez (USRA)
- Tom Bridgman (Global Science and Technology, Inc.)
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Producers
- Genna Duberstein (USRA)
- Michael Starobin (KBR Wyle Services, LLC)
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Writer
- Sarah Frazier (ADNET Systems, Inc.)
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Scientist
- Betsy Congdon (Johns Hopkins University/APL)
Release date
This page was originally published on Monday, July 30, 2018.
This page was last updated on Wednesday, May 3, 2023 at 1:46 PM EDT.