The Žďár nad Sázavou meteorite fall: Fireball trajectory, photometry, dynamics, fragmentation, orbit, and meteorite recovery
arXiv:1912.11784 · doi:10.1111/maps.13444
Abstract
We report a comprehensive analysis of the instrumentally observed meteorite fall Žďár nad Sázavou, which occurred in the Czech Republic on 9 December 2014 at 16:16:45-54 UT. The original meteoroid with an estimated initial mass of 150 kg entered the atmosphere with a speed of 21.89 km/s and began a luminous trajectory at an altitude of 98.06 km. At the maximum, it reached -15.26 absolute magnitude and terminated after an 9.16 s and 170.5 km long flight at an altitude of 24.71 km with a speed of 4.8 km/s. The average slope of the atmospheric trajectory to the Earth's surface was only 25.66°. Before its collision with Earth, the initial meteoroid orbited the Sun on a moderately eccentric orbit with perihelion near Venus orbit, aphelion in the outer main belt, and low inclination. During the atmospheric entry, the meteoroid severely fragmented at a very low dynamic pressure 0.016 MPa and further multiple fragmentations occurred at 1.4 - 2.5 MPa. Based on our analysis, so far three small meteorites classified as L3.9 ordinary chondrites totaling 87 g have been found almost exactly in the locations predicted for a given mass. Because of very high quality of photographic and radiometric records, taken by the dedicated instruments of the Czech part of the European Fireball Network, Žďár nad Sázavou belongs to the most reliably, accurately, and thoroughly described meteorite falls in history.
arXiv comment35 pages, 23 figures, 4 tables. Accepted to Meteoritics and Planetary Science, December 13, 2019
References in corpus (4)
- Identification of meteorite source regions in the Solar System
- Discovery of a new branch of the Taurid meteoroid stream as a real source of potentially hazardous bodies
- Small Near-Earth Asteroids as a Source of Meteorites
- The January 7, 2015, superbolide over Romania and structural diversity of meter-sized asteroids
Cited by in corpus (13)
- The Global Meteor Network -- Methodology and First Results
- Two Strengths of Ordinary Chondritic Meteoroids as Derived from their Atmospheric Fragmentation Modeling
- Data on 824 fireballs observed by the digital cameras of the European Fireball Network in 2017-2018. I. Description of the network, data reduction procedures, and the catalog
- Data on 824 fireballs observed by the digital cameras of the European Fireball Network in 2017-2018. II. Analysis of orbital and physical properties of centimeter-sized meteoroids
- Direct measurement of decimeter-sized rocky material in the Oort cloud
- FRIPON: A worldwide network to track incoming meteoroids
- Near Earth stream decoherence revisited: the limits of orbital similarity
- Perihelion history and atmospheric survival as primary drivers of the Earth`s meteorite record
- Fireball characteristics derivable from acoustic data
- Comparing the dynamics of Jupiter-family Comets and comet-like fireballs
- Review of synergic meteor observations: linking the results from cameras, ionosondes, infrasound and seismic detectors
- Error dependencies in the space-based CNEOS fireball database
- Statistical significance of meteorite-asteroid pairs using geocentric parameters