Mass – Radius Relationship in Extrasolar Planets
| dc.contributor.author | Santana, M. | |
| dc.contributor.author | Santos, N. | |
| dc.contributor.author | Bezzeghoud, Mourad | |
| dc.contributor.author | Caldeira, Bento | |
| dc.date.accessioned | 2012-01-17T12:54:33Z | |
| dc.date.available | 2012-01-17T12:54:33Z | |
| dc.date.issued | 2011 | |
| dc.description.abstract | The increasing number of Extrasolar planets observed in the last years makes important to define, as soon as possible, a mass – radius relationship, and so, we adjusted an planetary constitution independent experimental equation. Using the latest database of Extrasolar planets, a bi-logarithmic graphic was plotted that represents the mass - radius relationship where we adjusted a polynomial equation, which better suited the sample of Extrasolar planets at current time. | por |
| dc.identifier.authoremail | nd | |
| dc.identifier.authoremail | nd | |
| dc.identifier.authoremail | mourad@uevora.pt | |
| dc.identifier.authoremail | bafcc@uevora.pt | |
| dc.identifier.local | Évora | |
| dc.identifier.scientificarea | 243 | por |
| dc.identifier.sharewith | FIS | por |
| dc.identifier.uri | http://hdl.handle.net/10174/3682 | |
| dc.identifier.withinvitedoralpresentation | nao | por |
| dc.identifier.withoralpresentation | nao | por |
| dc.identifier.withposter | sim | por |
| dc.language.iso | eng | por |
| dc.publisher | PGUE2011- Fifth Meeting of Post-Graduation in Physics and Earth Sciences of University of Évora | por |
| dc.rights | openAccess | por |
| dc.subject | Extrasolar planets | por |
| dc.subject | mass - radius relationship | por |
| dc.title | Mass – Radius Relationship in Extrasolar Planets | por |
| dc.type | lecture | por |
| degois.publication.issue | 5 | por |
| degois.publication.location | Évora | por |
| degois.publication.title | Fifth Meeting of Post-Graduation in Physics and Earth Sciences of University of Évora | por |