Thermal evolution and sintering of chondritic planetesimals

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Henke, S ^a   Gail, H P ^a   Trieloff, M ^a   Schwarz, W H ^a   Kleine, T ^b  

^a UNIVERSITY OF HEIDELBERG   (Germany)

^b UNIVERSITY OF MÜNSTER   (Germany)

Author keywords

meteorites meteors meteoroids; minor planets asteroids: general; planets and satellites: physical evolution

Indexed keywords

BASIC PARAMETERS; BEST FIT; BURIAL DEPTHS; CHEMICAL COMPOSITIONS; CHONDRITIC METEORITES; COLD PRESSING; COOLING HISTORY; COOLING PATH; ENERGY TRANSPORT; HEAT-CONDUCTIVITY; HEAT-PRODUCING; HYDROSTATIC EQUILIBRIUM; INTERNAL STRUCTURE; LOW TEMPERATURES; LOW THERMAL CONDUCTIVITY; MEASURED DATA; MINOR PLANETS; NEW MODEL; ORDINARY CHONDRITES; PARENT BODIES; PLANETS AND SATELLITES: PHYSICAL EVOLUTION; POROUS BODIES; POROUS POWDERS; POWDER MATERIAL; POWDER SURFACE; PRESSURE AND TEMPERATURE; RADIOACTIVE NUCLEI; SINTERED MATERIALS; SMALL BODIES; SURFACE LAYERS; THEORETICAL MODELS; THERMAL EVOLUTION; THERMAL MODEL; THRESHOLD TEMPERATURES; TIME-SCALES;

ASTEROIDS; COOLING; GRANULAR MATERIALS; HOT PRESSING; METEORITES; MODELS; PLANETS; POROUS MATERIALS; POWDERS; SATELLITES; SILICATES; SINTERING; THERMOGRAPHY (TEMPERATURE MEASUREMENT);

THERMAL CONDUCTIVITY;

EID: 84855519281     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117177     Document Type: Article

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