Feasibility of meteor surveying from a Venus orbiter

The fireball of November 24, 1970, as the most probable source of the Ischgl meteorite

“…In order to gather extensive data on the orbits of solar system small bodies and fireball trajectories and their behaviors, photographic all-sky camera networks have been established worldwide since the mid-20th century (Bland et al, 2012;Ceplecha & Rajchl, 1965;Colas et al, 2020;Devillepoix et al, 2020;Halliday et al, 1978;Howie et al, 2017;Trigo-Rodrıǵuez et al, 2006;Whipple, 1938). Subsequently, a posibility of meteor detection has been discussed or even integrated also within the broader scoped surveys on the Earth and beyond including the Vera C. Rubin Observatory, previously referred to as the Large Synoptic Survey Telescope (LSST), Mini-EUSO telescope on board the ISS, high-power large-aperture (HPLA) radars such as the European Incoherent Scatter facility EISCAT, the global network of robotic astronomical observatories BOOTES, and EnVision mission to Venus developed by the European Space Agency (Bektešević et al, 2018;Castro-Tirado, 2023;Christou & Gritsevich, 2024;Coleman et al, 2023;Hu et al, 2023;Kero et al, 2019;Pellinen-Wannberg et al, 1998;Räbinä et al, 2016;Vinković et al, 2016;Vinković & Gritsevich, 2020). Of particular interest are relatively rare meteorite-producing events (Boaca et al, 2022;Brown et al, 2013;Gritsevich, 2008a;Peña-Asensio et al, 2023;Sansom, Gritsevich, et al, 2019;Wetherill & ReVelle, 1981), as their identification and subsequent analysis may allow rapid recovery of unique extraterrestrial samples in unweathered conditions while also providing clues to their dynamic origin (Dmitriev et al, 2015;Jansen-Sturgeon et al, 2019;Kyrylenko et al, 2023;Peña-Asensio et al, 2021;Trigo-Rodrıǵuez et al, 2015).…”