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- W1597081991 abstract "Dust grains represent an important repository of cosmic matter, tracing stages ofstellar evolution in our Galaxy. Three interdisciplinary workshops at ISSI in1997 and 1998 studied dust grains at complementary phases of their life cycle.At these workshops the properties of astronomical interstellar dust grains(ISDG) were compared with in-situ ISDG data and pre-solar grains found inmeteorites. The astronomical dust data yield grain composition and size distri-bution through optical, infrared (IR), and ultraviolet (UV) absorption and emis-sion properties. In contrast, in-situ spacecraft data provide the ISDG mass distri-bution after correction for heliospheric interactions. Precise laboratory studies ofpresolar grains from meteorites yield the composition and origin of the stardustthat parented the ISDGs. Bringing these views together at ISSI provided a newviewpoint of the mass distribution of ISDGs impinging on the Solar System, thegas-to-dust mass ratio and grain composition in the local interstellar cloud, grainformation in stellar atmospheres, destruction in the interstellar medium (ISM),and the composition of pre-solar versus ISDGs.It became clear during the ISSI meetings that relating pre-solar and interstellargrains requires allowance for grain processing in space, including radiative dam-age, alteration, spallation, reheating, and exposure to additional compounds indense interstellar clouds. Ed Anders noted: “There is no real contradictionbetween the meteoritic and astronomical data on grains. The vast majority ofinterstellar grains are reprocessed, homogenized [and fragmented]. The pristinecircumstellar grains are chance survivors of a stochastic process that destroyedall but 10" @default.
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- W1597081991 date "2005-01-01" @default.
- W1597081991 modified "2023-09-23" @default.
- W1597081991 title "Interstellar and presolar grains in the Galaxy and in the Solar System" @default.
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