(meteorobs) 1972 Draconids [was 2005 Draconids]
Malcolm J. Currie
mjc at star.rl.ac.uk
Wed Jan 26 16:48:35 EST 2005
Thank you to all those who addressed my question about the 1972
Draconids.
On Tue, 25 Jan 2005, Jeff Wilson wrote:
> YORP= ?
This is one of the non-gravitational forces caused by the re-radiation
of heat from a rotating uneven meteoroid (or asteroid), not unlike a
windmill. YORP is an acronym based upon the initials of those who
investigated it. Yarkovsky, O'Keefe, Radzievskii, and Paddack. It's
actually a smaller effect based upon the more widely known and stronger
Yarkovsky effect. Heat accumulated on the day-side of the meteoroid
means the evening side is warmer than the morning side. The excess
radiated heat on the evening sides causes a small radiation pressure to
one side of the particle. Over many orbits this subtle sideways thrust
can amount to a significant deviation from the expected orbit.
Malcolm
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