4–8 Nov 2024
VIC
Europe/Vienna timezone

Infrasound detections of the OSIRIS-REx Sample Return Capsule re-entry

7 Nov 2024, 15:50
25m
M2 (VIC)

M2

VIC

Wagramer Strasse 5, Vienna, Austria
oral Sources and Scientific Applications Sources and Scientific Applications

Description

On 24 September 2023, NASA's OSIRIS-REx mission achieved a significant milestone by successfully returning particles from a nearby asteroid to Earth via a Sample Return Capsule (SRC). The SRC generated shock waves as it entered the atmosphere, traversing California, Nevada and Utah before landing at the Utah Test and Training Range (UTTR). Since SRCs are well-characterized objects with known parameters, their re-entries can be leveraged towards studying meteor phenomena, characterizing high-altitude shock wave dynamics, improving entry and propagation models, and advancing global monitoring efforts. Under desirable conditions, SRCs generate infrasound which can be detected by microbarometers. We deployed ground-based and balloon-borne infrasound sensors in Nevada and Utah to capture the signals as a function of distance from the trajectory and from different parts of the trail. We will present signal characteristics at different stations, and how these might relate to SRC altitude and point(s) along the trajectory. These findings not only hold promise for enhancing future observational campaigns on Earth but also offer valuable perspectives into the detection and characterization of shock wave signatures on extraterrestrial bodies with atmospheres, including Mars, Titan, and Venus.

SNL is managed and operated by NTESS under DOE NNSA contract DE-NA0003525.

E-mail [email protected]

Primary authors

Daniel Bowman (Sandia National Laboratories) Dr Elizabeth Silber (Sandia National Laboratories (SNL))

Presentation materials