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abhijat | 2 years ago
> New data (Figure 3) at larger heliocentric distances show that the SDC-reported dust f l uxes, out to 55 au, remained higher than current models expected. Each of the three physical phenomena: optical properties and radiation pressure (Arnold et al. 2019); compositional variation between silicates and ice (Grigorieva et al. 2007); and a further reaching than currently identif i ed distribution of dust-producing bodies in the solar system (Fraser et al. 2023), may contribute to the data/model deviation.
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