Abstract
High quality new data on the asteroid mass and volume were produced in the last years from both extra-atmospheric instruments and the groundbased high-performance telescopes. This paper presents a synthesis of these resultsin terms of the asteroid density, taking into account several techniques, and the possible correlation of the density through the taxonomic system. The important conclusion is that M-type asteroids seems to have an unexpected low density, which cannot be explained by the present mineralogy assumed by the comparative mineralogy.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
