Astrophysical plasma

Short description: Plasma outside of the Solar System

Lagoon Nebula is a large, low-density cloud of partially ionized gas.[1]

Astrophysical plasma is plasma outside of the Solar System. It is studied as part of astrophysics and is commonly observed in space.[2] The accepted view of scientists is that much of the baryonic matter in the universe exists in this state.[3]

When matter becomes sufficiently hot and energetic, it becomes ionized and forms a plasma.[clarification needed] This process breaks matter into its constituent particles which includes negatively charged electrons and positively charged ions.[4] These electrically charged particles are susceptible to influences by local electromagnetic fields. This includes strong fields generated by stars, and weak fields which exist in star forming regions, in interstellar space, and in intergalactic space.[5] Similarly, electric fields are observed in some stellar astrophysical phenomena.

Astrophysical plasma is often differentiated from space plasma, which typically refers to the plasma of the Sun, the solar wind, and the ionospheres and magnetospheres of the Earth and other planets.[6][7][8][9][10][11][12]

## Contents

* 1 Terminology
* 2 Observing and studying astrophysical plasma
* 3 Possible related phenomena
* 4 Early history
* 5 In popular culture
* 6 References
* 7 External links

## Terminology

Although gas and plasma are distinct states of matter, the term gas is frequently used by astronomers to refer to any astrophysical fluid that is in either the gas or plasma state of matter. The term ionized gas specifically refers to plasma.[13]

## Observing and studying astrophysical plasma

Plasmas in stars can both generate and interact with magnetic fields, resulting in a variety of dynamic astrophysical phenomena. These phenomena are sometimes observed in spectra due to the Zeeman effect. Other forms of astrophysical plasmas can be influenced by preexisting weak magnetic fields, whose interactions may only be determined directly by polarimetry or other indirect methods.[5] In particular, the intergalactic medium, the interstellar medium, the interplanetary medium and solar winds consist of diffuse plasmas.

## Possible related phenomena

Scientists are interested in active galactic nuclei because such astrophysical plasmas could be directly related to the plasmas studied in laboratories.[14] Many of these phenomena seemingly exhibit an array of complex magnetohydrodynamic behaviors, such as turbulence and instabilities.[2]

In Big Bang cosmology, the entire universe was in a plasma state prior to recombination.[15]

## Early history

Norwegian explorer and physicist Kristian Birkeland predicted that space is filled with plasma. He wrote in 1913:

> It seems to be a natural consequence of our points of view to assume that the whole of space is filled with electrons and flying electric ions of all kinds. We have assumed that each stellar system through its evolution throws off electric corpuscles into space.

Birkeland assumed that most of the mass in the universe should be found in "empty" space.[16]

## In popular culture

The 1959 album Space Songs contains the song Why Does the Sun Shine?,[17] which incorrectly refers to the Sun as "a mass of incandescent gas." In 1993, They Might Be Giants released a cover version of this song in an EP entitled Why Does the Sun Shine? (The Sun Is a Mass of Incandescent Gas).[18] The album Here Comes Science was released by They Might be Giants in 2009. Here Comes Science includes a recording of this song immediately followed by the song Why Does the Sun Really Shine? (The Sun is a Miasma of Incandescent Plasma) that correctly refers to the Sun as plasma.[19]

## References

1. ↑ "Sneak Preview of Survey Telescope Treasure Trove". ESO Press Release. http://www.eso.org/public/news/eso1403/.
2. ↑ 2.0 2.1 "Study sheds light on turbulence in astrophysical plasmas: Theoretical analysis uncovers new mechanisms in plasma turbulence". MIT News. December 2017. https://news.mit.edu/2017/study-uncovers-new-mechanisms-astrophysical-plasma-turbulence-1201.
3. ↑ Chiuderi, C.; Velli, M. (2015). "Particle Orbit Theory". Basics of Plasma Astrophysics. UNITEXT for Physics. p. 17. doi:10.1007/978-88-470-5280-2_2. ISBN 978-88-470-5280-2. Bibcode: 2015bps..book.....C.
4. ↑ IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version:  (2006-) "Ionization". doi:10.1351/goldbook.I03183
5. ↑ 5.0 5.1 Lazarian, A.; Boldyrev, S.; Forest, C.; Sarff, P. (2009). "Understanding of the role of magnetic fields: Galactic perspective". Astro2010: The Astronomy and Astrophysics Decadal Survey 2010: 175. Bibcode: 2009astro2010S.175L.
6. ↑ "Space Physics Textbook". 2006-11-26. http://www.oulu.fi/~spaceweb/textbook/.
7. ↑ "The Solar Physics and Space Plasma Research Centre (SP2RC)". MIT News. http://sp2rc.group.shef.ac.uk/.
8. ↑ Owens, Mathew J.; Forsyth, Robert J. (2003). "The Heliospheric Magnetic Field" (in en). Living Reviews in Solar Physics 10 (1): 5. doi:10.12942/lrsp-2013-5. ISSN 2367-3648. Bibcode: 2013LRSP...10....5O.
9. ↑ Nagy, Andrew F.; Balogh, André; Thomas E. Cravens; Mendillo, Michael; Mueller-Woodarg, Ingo (2008). Comparative Aeronomy. Springer. pp. 1–2. ISBN 978-0-387-87824-9.
10. ↑ Ratcliffe, John Ashworth (1972). An Introduction to the Ionosphere and Magnetosphere. CUP Archive. ISBN 978-0-521-08341-6. https://archive.org/details/introductiontoio0000ratc.
11. ↑ NASA Study Using Cluster Reveals New Insights Into Solar Wind, NASA, Greenbelt, 2012, p.1
12. ↑ Cade III, William B.; Christina Chan-Park (2015). "The Origin of "Space Weather"". Space Weather 13 (2): 99. doi:10.1002/2014SW001141. Bibcode: 2015SpWea..13...99C.
13. ↑ Schaffner, David; Kostadinova, Evdokya; Kuranz, Carolyn; Mordijck, Saskia; Rachmeler, Laurel; Thakur, Saikat Chakraborty; Abler, Mel (2023). "Just Say Plasma". Bulletin of the American Astronomical Society 55 (3): 357. doi:10.3847/25c2cfeb.5c4f5de5. Bibcode: 2023BAAS...55c.357S. https://baas.aas.org/pub/2023n3i357/release/1.
14. ↑ Berkowitz, Rachel (April 2018). "Lab experiments mimic the origin and growth of astrophysical magnetic fields". Physics Today 71 (4): 20–22. doi:10.1063/PT.3.3891. Bibcode: 2018PhT....71d..20B.
15. ↑ Peebles, P. J. E. (1968). "Recombination of the Primeval Plasma". Astrophysical Journal 153: 1. doi:10.1086/149628. Bibcode: 1968ApJ...153....1P.
16. ↑ Birkeland, Kristian (1908). The Norwegian Aurora Polaris Expedition 1902–1903. New York and Christiania (now Oslo): H. Aschehoug & Co. p. 720. https://archive.org/details/norwegianaurorap01chririch. out-of-print, full text online.
17. ↑ Tom Glazer and Dottie Evans (1959). "Why Does the Sun Shine?". Space Songs. Lyrics by Hy Zaret; music by Lou Singer. Motivation Records.`{{cite AV media}}`: CS1 maint: others in cite AV media (notes) (link)
18. ↑ They Might Be Giants (1993). Why Does the Sun Shine? (The Sun Is a Mass of Incandescent Gas (Audio recording). Elektra.
19. ↑ They Might Be Giant (2009). "Why Does the Sun Really Shine? (The Sun Is a Miasma of Incandescent Plasma)". Here Comes Science (Audio recording). Idlewild/Disney.

## External links

* "US / Russia Collaboration in Plasma Astrophysics"

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