Back to Search
Start Over
A new mechanism for chondrule formation: Radiative heating by hot planetesimals.
- Source :
-
ICARUS . Mar2016, Vol. 267, p364-367. 4p. - Publication Year :
- 2016
-
Abstract
- We propose that chondrules are formed by radiative heating of pre-existing dust clumps during close fly-bys of planetesimals with incandescent lava at their surfaces. We show that the required temperatures and cooling rates are easily achieved in this scenario and discuss how it is consistent with bulk aspects of chondritic meteorites, including complementarity and the co-mingling of FeO-poor and FeO-rich chondrules. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 00191035
- Volume :
- 267
- Database :
- Academic Search Index
- Journal :
- ICARUS
- Publication Type :
- Academic Journal
- Accession number :
- 112629867
- Full Text :
- https://doi.org/10.1016/j.icarus.2015.11.026