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Parker Solar Probe

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Encyclopedia of Astrobiology

Definition

Parker Solar Probe is a NASA mission designed to investigate the fundamental plasma physics of the near-Sun plasma environment by flying into its outermost atmosphere known as the corona, a region which has never been explored before. It will perform the closest-ever in situ and remote sensing observations of the coronal and solar wind plasma as close as 9.8 solar radii (Rs) from the center of the Sun (0.045 A.U).

History

The idea of the Parker Solar Probe mission dates back to the 1958 Simpson Committee Report which proposed several space missions including “a solar probe to pass inside the orbit of Mercury to study the particles and fields in the vicinity of Mercury.” The concept of this mission, originally called “Solar Probe” has been revised many times over more than five decades, nevertheless its main objective has always been a close encounter with the Sun.

It is only until 2014 that “Solar Probe” mission was confirmed and started to be developed as part of NASA’s...

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Abbreviations

PSP:

Parker Solar Probe

A.U.:

Astronomical Unit

Rs:

Solar Radii

WISPR:

Wide-field Imager for Solar Probe

SWEAP:

Solar Wind Electrons Alphas and Protons

ISIS:

Integrated Science Investigation of the Sun energetic particle

SPC:

Solar Probe Cup

SPAN:

Solar Probe ANalyzers

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Correspondence to Olivier Witasse .

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Hadid, L.Z., Witasse, O. (2022). Parker Solar Probe. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_5557-1

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_5557-1

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  • Print ISBN: 978-3-642-27833-4

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