JPL Technical Report Server

Infrared Observation of Meteoroid Production by Comet Encke

Show simple item record

dc.contributor.author Reach, W. en_US
dc.contributor.author Sykes, M. en_US
dc.contributor.author Lien, D. en_US
dc.contributor.author Davies, J. en_US
dc.date.accessioned 2004-09-24T17:10:54Z
dc.date.available 2004-09-24T17:10:54Z
dc.date.issued 1999-08 en_US
dc.identifier.citation Nature en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 99-1709 en_US
dc.identifier.uri http://hdl.handle.net/2014/18240
dc.description.abstract Comets lose mass primarily in the form of large particles that form meteoroid streams in the comets orbits. At visible wavelengths, comets often have long dust tails directed away from the Sun, consisting of small dust particles being blown away by solar radiation pressure. en_US
dc.format.extent 357075 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other infrared meteoroid Comet Encke en_US
dc.title Infrared Observation of Meteoroid Production by Comet Encke en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account