Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-12-20
Astronomy and Astrophysics
Astrophysics
12 pages; includes 1 figure, 1 table; accepted by ApJ Letters
Scientific paper
10.1086/339363
Silicate dust grains in the interstellar medium are known to be mostly amorphous, yet crystalline silicate grains have been observed in many long-period comets and in protoplanetary disks. Annealing of amorphous silicate grains into crystalline grains requires temperatures > 1000 K, but exposure of dust grains in comets to such high temperatures is incompatible with the generally low temperatures experienced by comets. This has led to the proposal of models in which dust grains were thermally processed near the protoSun, then underwent considerable radial transport until they reached the gas giant planet region where the long-period comets originated. We hypothesize instead that silicate dust grains were annealed in situ, by shock waves triggered by gravitational instabilities. We assume a shock speed of 5 km/s, a plausible value for shocks driven by gravitational instabilities. We calculate the peak temperatures of micron and submicron amorphous pyroxene grains of chondritic composition under conditions typical in protoplanetary disks at 5 - 10 AU. Our results also apply to chondritic amorphous olivine grains. We show that {\it in situ} thermal annealing of submicron and micron-sized silicate dust grains can occur, obviating the need for large-scale radial transport.
Desch Steven J.
Harker David E.
No associations
LandOfFree
Annealing of Silicate Dust by Nebular Shocks at 10 AU does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Annealing of Silicate Dust by Nebular Shocks at 10 AU, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Annealing of Silicate Dust by Nebular Shocks at 10 AU will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-313881