Interplanetary dust cloud

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The interplanetary dust cloud illuminated and visible as zodiacal light, with its parts the false dawn,[1] gegenschein and the rest of its band, which is visually crossed by the Milky Way, in this composite image of the night sky above the northern and southern hemisphere

The interplanetary dust cloud, or zodiacal cloud (as the source of the zodiacal light), consists of cosmic dust (small particles floating in outer space) that pervades the space between planets within planetary systems, such as the Solar System.[2] This system of particles has been studied for many years in order to understand its nature, origin, and relationship to larger bodies. There are several methods to obtain space dust measurement.

In the Solar System, interplanetary dust particles have a role in

Apollo Program[5] revealed the size distribution of cosmic dust particles bombarding the lunar surface. The ’’Grün’’ distribution of interplanetary dust at 1 AU,[6] describes the flux of cosmic dust
from nm to mm sizes at 1 AU.

The total mass of the interplanetary dust cloud is approximately 3.5×1016 kg, or the mass of an asteroid of radius 15 km (with density of about 2.5 g/cm3).[7] Straddling the zodiac along the ecliptic, this dust cloud is visible as the zodiacal light in a moonless and naturally dark sky and is best seen sunward during astronomical twilight.

The Pioneer spacecraft observations in the 1970s linked the zodiacal light with the interplanetary dust cloud in the Solar System.[8] Also, the VBSDC instrument on the New Horizons probe was designed to detect impacts of the dust from the zodiacal cloud in the Solar System.[9]

Origin

Artist's concept of a view from an exoplanet, with light from an extrasolar interplanetary dust cloud

The sources of interplanetary dust particles (IDPs) include at least: asteroid collisions, cometary activity and collisions in the inner Solar System, Kuiper belt collisions, and interstellar medium grains (Backman, D., 1997). The origins of the zodiacal cloud have long been subject to one of the most heated controversies in the field of astronomy.

It was believed that IDPs had originated from comets or asteroids whose particles had dispersed throughout the extent of the cloud. However, further observations have suggested that Mars

dust storms may be responsible for the zodiacal cloud's formation.[10][2]

Life cycle of a particle

The main physical processes "affecting" (destruction or expulsion mechanisms) interplanetary dust particles are: expulsion by

sublimation
, mutual collisions, and the dynamical effects of planets (Backman, D., 1997).

The lifetimes of these dust particles are very short compared to the lifetime of the Solar System. If one finds grains around a star that is older than about 10,000,000 years, then the grains must have been from recently released fragments of larger objects, i.e. they cannot be leftover grains from the protoplanetary disk (Backman, private communication).[citation needed] Therefore, the grains would be "later-generation" dust. The zodiacal dust in the Solar System is 99.9% later-generation dust and 0.1% intruding interstellar medium dust. All primordial grains from the Solar System's formation were removed long ago.

Particles which are affected primarily by radiation pressure are known as "beta meteoroids". They are generally less than 1.4 × 10−12 g and are pushed outward from the Sun into interstellar space.[11]

Cloud structures

The interplanetary dust cloud has a complex structure (Reach, W., 1997). Apart from a background density, this includes:

Dust collection on Earth

In 1951,

Fred Whipple predicted that micrometeorites smaller than 100 micrometers in diameter might be decelerated on impact with the Earth's upper atmosphere without melting.[12] The modern era of laboratory study of these particles began with the stratospheric collection flights of Donald E. Brownlee and collaborators in the 1970s using balloons and then U-2 aircraft.[13]

Although some of the particles found were similar to the material in present-day meteorite collections, the

nanoporous nature and unequilibrated cosmic-average composition of other particles suggested that they began as fine-grained aggregates of nonvolatile building blocks and cometary ice.[14][15] The interplanetary nature of these particles was later verified by noble gas[16] and solar flare track[17]
observations.

In that context a program for atmospheric collection and curation of these particles was developed at

extraterrestrial material
(not to mention being small astronomical objects in their own right) available for study in laboratories today.

Experiments

Spacecraft that have carried dust detectors include Helios, Pioneer 10, Pioneer 11, Ulysses (heliocentric orbit out to the distance of Jupiter), Galileo (Jupiter Orbiter), Cassini (Saturn orbiter), and New Horizons (see Venetia Burney Student Dust Counter).

Major Review Collections

Collections of review articles on various aspects of interplanetary dust and related fields appeared in the following books:

In 1978 Tony McDonnell edited the book Cosmic Dust[19] which contained chapters[20] on comets along with zodiacal light as indicator of interplanetary dust, meteors, interstellar dust, microparticle studies by sampling techniques, and microparticle studies by space instrumentation. Attention is also given to lunar and planetary impact erosion, aspects of particle dynamics, and acceleration techniques and high-velocity impact processes employed for the laboratory simulation of effects produced by micrometeoroids.

2001 Eberhard Grün, Bo Gustafson, Stan Dermott, and Hugo Fechtig published the book Interplanetary Dust.[21] Topics covered[22] are: historical perspectives; cometary dust; near-Earth environment; meteoroids and meteors; properties of interplanetary dust, information from collected samples; in situ measurements of cosmic dust; numerical modeling of the Zodiacal Cloud structure; synthesis of observations; instrumentation; physical processes; optical properties of interplanetary dust; orbital evolution of interplanetary dust; circumplanetary dust, observations and simple physics; interstellar dust and circumstellar dust disks.

2019 Rafael Rodrigo, Jürgen Blum, Hsiang-Wen Hsu, Detlef V. Koschny, Anny-Chantal Levasseur-Regourd, Jesús Martín-Pintado, Veerle J. Sterken, and Andrew Westphal collected reviews in the book Cosmic Dust from the Laboratory to the Stars.[23] Included are discussions[24] of dust in various environments: from planetary atmospheres and airless bodies over interplanetary dust, meteoroids, comet dust and emissions from active moons to interstellar dust and protoplanetary disks. Diverse research techniques and results, including in-situ measurement, remote observation, laboratory experiments and modelling, and analysis of returned samples are discussed.

Rings of dust

First ever panorama image of the dust ring of Venus's orbital space, imaged by Parker Solar Probe.

Interplanetary dust has been found to form rings of dust in the orbital space of Mercury and Venus.

proto-planetary disc and then itself, the Solar planetary system, formed.[26]

See also

References

  1. ^ "False Dawn". www.eso.org. Retrieved 14 February 2017.
  2. ^
    EurekAlert!
    . NASA. 12 March 2019. Retrieved 12 March 2019.
  3. ^ Levasseur-Regourd, A.C., 1996
  4. ^ Backman, D., 1997
  5. Bibcode:1979LPSC...10.1649M
    . Retrieved 3 February 2022.
  6. doi:10.1016/0019-1035(85)90121-6
    . Retrieved 23 January 2022.
  7. PMID 11543198
    .
  8. ^ Hannter; et al. (1976). "Pioneer 10 observations of zodiacal light brightness near the ecliptic - Changes with heliocentric distance".
  9. S2CID 17522966
    . Retrieved 17 September 2022.
  10. ^ Shekhtman, Svetlana (8 March 2021). "Serendipitous Juno Detections Shatter Ideas About Zodiacal Light". NASA. Retrieved 8 May 2022. While there is good evidence now that Mars, the dustiest planet we know of, is the source of the zodiacal light, Jørgensen and his colleagues cannot yet explain how the dust could have escaped the grip of Martian gravity.
  11. ^ "Micrometeorite Background". GENESIS Discovery 5 Mission. Caltech. Archived from the original on 26 August 2007. Retrieved 4 August 2008.
  12. PMID 16578350
    .
  13. Bibcode:1978prpl.conf..134B
    .
  14. ^ Fraundorf, P.; Brownlee, D. E. & Walker, R. M. (1982) [1st pub. 1986]. "Laboratory studies of interplanetary dust". In Wilkening, L. (ed.). Comets. University of Arizona Press. pp. 383–409.
  15. Bibcode:1986NASCP2403...55W
    .
  16. PMID 17748271
    .
  17. S2CID 27703897
    .
  18. ^ "Cosmic Dust". NASA – Johnson Space Center program, Cosmic Dust Lab. 6 January 2016. Retrieved 14 March 2016.
  19. ISBN 0-471-99512-6
    . Retrieved 22 January 2022.
  20. Bibcode:1978codu.book.....M
    . Retrieved 5 February 2022.
  21. ISBN 978-3-540-42067-5
    . Retrieved 5 February 2022.
  22. ISBN 978-3-642-62647-0
    . Retrieved 5 February 2022.
  23. ISBN 978-94-024-2009-8
    . Retrieved 5 February 2022.
  24. ^ "Cosmic Dust from the Laboratory to the Stars". Retrieved 5 February 2022.
  25. ^ a b Garner, Rob (12 March 2019). "What Scientists Found After Sifting Through Dust in the Solar System". NASA. Retrieved 21 January 2023.
  26. ^ Rehm, Jeremy (15 April 2021). "Parker Solar Probe Captures First Complete View of Venus Orbital Dust Ring". JHUAPL. Retrieved 21 January 2023.

Further reading

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