https://journals.plos.org/climate/article?id=10.1371/journal.pclm.0000133

*Authors*

Benjamin C. Bromley,
<https://journals.plos.org/climate/article?id=10.1371/journal.pclm.0000133#>
 Sameer H. Khan,
<https://journals.plos.org/climate/article?id=10.1371/journal.pclm.0000133#>
 Scott J. Kenyon
<https://journals.plos.org/climate/article?id=10.1371/journal.pclm.0000133#>


*8 February 2023*
*Citation*: Bromley BC, Khan SH, Kenyon SJ (2023) Dust as a solar shield.
PLOS Clim 2(2): e0000133. https://doi.org/10.1371/journal.pclm.0000133

Abstract

We revisit dust placed near the Earth–Sun L1 Lagrange point as a possible
climate-change mitigation measure. Our calculations include variations in
grain properties and orbit solutions with lunar and planetary
perturbations. To achieve sunlight attenuation of 1.8%, equivalent to about
6 days per year of an obscured Sun, the mass of dust in the scenarios we
consider must exceed 1010 kg. The more promising approaches include using
high-porosity, fluffy grains to increase the extinction efficiency per unit
mass, and launching this material in directed jets from a platform orbiting
at L1. A simpler approach is to ballistically eject dust grains from the
Moon’s surface on a free trajectory toward L1, providing sun shade for
several days or more. Advantages compared to an Earth launch include a
ready reservoir of dust on the lunar surface and less kinetic energy
required to achieve a sun-shielding orbit.

Source: PLOS Climate

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