Rain dust

The leaves of this Schefflera show the dust stains of a rain dust (near Paris, France)

Rain dust or snow dust, traditionally known as muddy rain, red rain, or coloured rain, is a variety of rain (or any other form of precipitation) which contains enough desert dust for the dust to be visible without using a microscope.


The rain dust phenomenon was studied by Italian scientist Giuseppe Maria Giovene (1753–1837), who managed to correctly explain the phenomenon as early as 1803. On 7 March 1803, rain dust fell over Southern Italy's region Apulia. At that time, people believed that the rain was caused by the explosions of Italy's volcanoes Mount Vesuvius or Etna, or that it was due to the transport of matter coming from the sea floor and raised by vapor. Giuseppe Maria Giovene brilliantly managed to relate the phenomenon to the wind which occurred prior to the rain event, and he came to the conclusion that the sand had come from Africa and that it had been pushed by the wind coming from south-east.[1][2]


Rain dust is common in the Western and Southern Merranean, where the dust supply comes from the atmospheric depressions going through the northern part of North Africa. The main sources of desert dust reach the Iberian Peninsula and the Balearic Islands in the form of dust transported by wind or rain from the Sahara, Atlas Mountains in Morocco and Central Algeria.[3]

Mud rains are relatively frequent and had been increasing in early 1990s in the Merranean Basin.[4]

It also occurs in arid desert regions of North America such as west Texas or Arizona. It occasionally happens in the grasslands as it did in Bexar County, Texas on March 18, 2008.

It may also occur in some regions of Southern Italy (sand coming from North Africa), but it is a very rare phenomenon.

Dust composition[]

The rain dust is very alkaline.[3] Some of the large particles contain mixtures of chemicals such as sulfate and sea salt (chiefly with sodium, chlorine and magnesium). Major minerals in order of decreasing abundance are: illite, quartz, smectite, palygorskite, kaolinite, calcite, dolomite and feldspars.[3] In Majorca a study finds that the size, by volume, 89% of the particles from rain dust fraction corresponded to silt (between 0.002 mm and 0.063 mm) and that there was virtually no clay sized particles (less than 0.29%).[5]


Blood/red rain[]

Rain dust is the most common cause of blood rain.

Red rain is however not always rain dust, see for example the Red rain in Kerala.

See also[]


  1. ^ elogio-storico, pag. 20
  2. ^ pioggia-rossa
  3. ^ a b c Avila, Anna; Queralt-Mitjans, Ignasi; Alarcón, Marta (1997). "Mineralogical composition of African dust delivered by red rains over northeastern Spain". Journal of Geophysical Research. 102: 21977. Bibcode:1997JGR...10221977A. doi:10.1029/97JD00485.
  4. ^ Sala, José Quereda; Cantos, Jorge Olcina; Chiva, Enrique Montón (1996). "Red dust rain within the Spanish Merranean area". Climatic Change. 32 (2): 215. Bibcode:1996ClCh...32..215S. doi:10.1007/BF00143711.
  5. ^ Fornós, Joan J., Crespí, Damià; Fiol, Lluís (1997). "Aspectes mineralogics i texturals de la pols procedent de les pluges de 1ang a les IIles Balears: la seva importancia en alguns processos geologics recents". Boll. Soc. Hist. Nat. Balears. 40: 114–122.CS1 maint: Multiple names: authors list (link)
  6. ^ Papastefanou, C; Manolopoulou, M; Stoulos, S; Ioannidou, A; Gerasopoulos, E (2001). "Coloured rain dust from Sahara Desert is still radioactive". Journal of Environmental Radioactivity. 55 (1): 109–112. doi:10.1016/S0265-931X(00)00182-X. PMID 11381550.