Infrared Observation of Meteoroid Production by Comet Encke

Reach, W.; Sykes,  M.; Lien,  D.; Davies,  J.

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