Asteroids are much 'redder' than meteorites (which come from asteroids); the accepted explanation is 'space weathering', though the actual processes and timescales involved have remained controversial. Vernazza et al. report observations of two young asteroid families, revealing that 'space weathering' must be a very rapid process, which favours solar wind implantation as the main mechanism; they further demonstrate an apparent weathering dependence on olivine abundance.
Solar wind as the origin of rapid reddening of asteroid surfaces
Rossi A;
2009
Abstract
Asteroids are much 'redder' than meteorites (which come from asteroids); the accepted explanation is 'space weathering', though the actual processes and timescales involved have remained controversial. Vernazza et al. report observations of two young asteroid families, revealing that 'space weathering' must be a very rapid process, which favours solar wind implantation as the main mechanism; they further demonstrate an apparent weathering dependence on olivine abundance.File in questo prodotto:
File | Dimensione | Formato | |
---|---|---|---|
prod_44308-doc_3011.pdf
solo utenti autorizzati
Descrizione: Solar wind as the origin of rapid reddening of asteroid surfaces
Tipologia:
Versione Editoriale (PDF)
Dimensione
191.02 kB
Formato
Adobe PDF
|
191.02 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.