From Dust to Rocky Planets Workshop
(Astromineralogy Workshop I. 2010)
August 28, 2010, Budapest
The workshop originally titled to "From Dust to Rocky Planets Workshop" (later also named as Astrominerylogy Workhop I.) happened as a satllite meeting of the 20th General Meeting of the International MIneralogical Association (IMA2010).
Location: Konkoly Thege Miklos Astronomical Institute, H-1121 Budapest, Konkoly Thege Miklós út 15-17.
Local Organizing Committee: Péter Ábrahám (Konkoly Observatory), Dániel Apai (Space Telescope Science Institute), Csaba Kiss (Konkoly Observatory), Attila Moór (Konkoly Observatory)
Program:
- 9.00 Registration (at Lecture Hall) / Visit to the Historic Astronomical Library
- 10:00 Welcome by Péter Ábrahám (director of the Konkoly Observatory)
Session I / Chair: Thomas Henning
- 10:10 D. Apai Protoplanetary Disk Evolution and Early Solar System Chronology
- 10:40 N. Sipos Circumstellar environment of young eruptive stars
- 11:00 P. Ábrahám Episodic formation of cometary material in the outburst of a young Sun-like star
- 11:20 Coffee break
Session II / Chair: Thomas Henning
- 11:40 Cs. Kiss Grain growth in cold molecular cores
- 12:00 T. Szalai Dust formation in the ejecta of the Type II-P supernova 2004dj
- 12:20 L. Szucs Stellar-mass-dependent disk structure in coeval planet-forming disks
- 12:40 L. Mosoni Radial probing of mineralogy of circumstellar disks with stellar interferometry
- 13:00 Lunch break in a nearby restaurant (within easy walking distance)
Session III / Chair : Dániel Apai
- 15:00 A. Gucsik Cathodluminescence properties of nanodiamonds in experiment: an application to the astrophysics of the planetary nebula
- 15:30 I. Gyollai Petrographical and micro-Raman study of microdiamonds in ALH-77257 (ureilite) and ALH-78113 (aubrite) samples
- 15:5016:10 Sz. Nagy A micro-Raman spectroscopy study of
-(Mg,Fe)2SiO4 ringwoodite from the shock vein of NWA 5011 meteorite: Constrains to shock conditions
- 16:10 Closing Remarks, P. Ábrahám
Detailed documentation of the workshop can be found here.
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