Search for Activity in 3200 Phaethon
Author(s) -
Henry H. Hsieh,
David Jewitt
Publication year - 2005
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/429250
Subject(s) - physics , asteroid , meteoroid , meteor (satellite) , astrophysics , coma (optics) , meteor shower , fraction (chemistry) , astronomy , astrobiology , chemistry , organic chemistry
We present deep optical imaging of Geminid meteor stream parent 3200 Phaethon taken in search of low-level cometary activity (i.e., coma or dust trail). Although no unambiguous cometary behavior was observed, we find an upper limit on the object's cometary mass-loss rate of ˙ Mlim 0:01 kg s 1 . The corresponding active fraction (the fraction of the surface area that could consist of freely sublimating water ice) is f 7 ;10 6 , at least 2 orders of magnitude smaller than other known comets. Subject headinggs: comets: general — meteors, meteoroids — minor planets, asteroids
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