z-logo
open-access-imgOpen Access
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

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom