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 |