Characterizing the Daytime Sextantids Meteor Shower and Unveiling the Nature of the Phaethon-Geminid Stream Complex
Y. Kipreos, Margaret Campbell-Brown, P. Brown, D. Vida

TL;DR
This study characterizes the Daytime Sextantids meteor shower, revealing its physical properties, orbit, and possible common origin with asteroid 2005 UD and the Phaethon-Geminid Stream Complex, through optical and radar data analysis.
Contribution
It introduces a novel convex hull approach for isolating stream orbits and provides new insights into the origin and physical characteristics of the DSX meteor shower.
Findings
DSX meteors ablate similarly to Geminids, indicating high density.
Peak flux of DSX is approximately 20 meteors per hour.
Estimated stream mass is about 10^16 grams, too large for recent formation from 2005 UD.
Abstract
The Daytime Sextantids meteor shower, part of the Phaethon-Geminid Stream Complex (PGC), is closely related to the Geminids, currently the strongest meteor shower visible at the Earth. The DSX share a similar orbit to asteroid 2005 UD, but the nature of the association remains unclear. From optical data we find that DSX meteors ablate similarly to Geminids, suggesting that they are also high density and consistent with a common origin. From radar data we have isolated 19,007 DSX orbits through application of a novel convex hull approach to determine stream membership. We find at the peak the mean semi-major axis is near 1 AU, eccentricity is 0.86 and that both decrease as a function of solar longitude. The inclination averages 25 degrees at the peak but increases over time. Noticeable DSX activity extends from solar longitude 173-196 with a flux plateau between 186 -…
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