Activity in Geminid Parent (3200) Phaethon
David Jewitt, Jing Li

TL;DR
This study observed a sudden brightening of asteroid Phaethon near perihelion, indicating impulsive dust release likely caused by thermal fracture, suggesting Phaethon acts as a rock comet contributing to the Geminid stream.
Contribution
First direct evidence of impulsive dust ejection from Phaethon near perihelion, supporting its role as a rock comet rather than a traditional icy comet.
Findings
Detected a twofold brightening of Phaethon near perihelion.
Estimated dust mass ejected is about 2.5x10^8 kg.
Impulsive dust release could replenish the Geminid stream over time.
Abstract
The asteroid (3200) Phaethon is widely recognized as the parent of the Geminid meteoroid stream. However, it has never shown evidence for on-going mass loss or for any form of comet-like activity that would indicate the continued replenishment of the stream. Following an alert by Battams and Watson (2009), we used NASA's STEREO-A spacecraft to image Phaethon near perihelion, in the period UT 2009 June 17 - 22, when the heliocentric distance was near 0.14 AU. The resulting photometry shows an unexpected brightening, by a factor of two, starting UT 2009 June 20.2+/-0.2, which we interpret as an impulsive release of dust particles from Phaethon. If the density is near 2500 kg/m^3, then the emitted dust particles must have a combined mass of ~2.5x10^8 a1 kg, where a1 is the particle radius in millimeters. Assuming a1 = 1, this is approximately 10^-4 of the Geminid stream mass and to…
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