EPSC Abstracts
Vol. 17, EPSC2024-449, 2024, updated on 03 Jul 2024
https://doi.org/10.5194/epsc2024-449
Europlanet Science Congress 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The recovery of the Matera H5 ordinary chondrite thanks to the observations of the PRISMA fireball network

Dario Barghini1,2, Albino Carbognani3, Daniele Gardiol1, Sara Bertocco4, Matteo Di Carlo5, Mario Di Martino1, Carmelo Falco1, Marco Fenucci6,7, Marco Morelli8, Giovanni Pratesi9,10, Walter Riva1,11, Raffaele Salerno12, Giovanna Maria Stirpe3, Cosimo Antonio Volpicelli1, and the PRISMA team*
Dario Barghini et al.
  • 1INAF - Osservatorio Astrofisico di Torino, Pino Torinese (TO), Italy (dario.barghini@inaf.it)
  • 2Università degli Studi di Torino, Dipartimento di Fisica, Torino, Italy
  • 3INAF – Osservatorio di Astrofisica e Scienze dello Spazio, Bologna, Italy
  • 4INAF – Osservatorio Astronomico di Trieste, Trieste, Italy
  • 5INAF – Osservatorio Astronomico d’Abruzzo, Teramo, Italy
  • 6ESA ESRIN/PDO/NEO Coordination Centre, Frascati (RM), Italy
  • 7Elecnor Deimos, San Pietro Mosezzo (NO), Italy
  • 8Museo Italiano di Scienze Planetarie, Fondazione Parsec, Prato, Italy
  • 9Università di Firenze, Dipartimento di Scienze della Terra, Firenze, Italy
  • 10INAF – Istituto di Astrofisica e Planetologia Spaziali, Roma, Italy
  • 11Osservatorio Astronomico del Righi, Genova, Italy
  • 12Meteo Expert, Cinisello Balsamo (MI), Italy
  • *A full list of authors appears at the end of the abstract

On 14/02/2023 at 17:68:29 UT, three all-sky cameras of the PRISMA network detected a bright bolide (IT20230214) over the regions of Puglia and Basilicata in Southern Italy. The bolide traversed the atmosphere for about 5.3 s, with an entry speed of 16.3 ± 0.1 km/s and at an inclination angle of 56.7° ± 0.3°, reaching a minimum absolute magnitude of -11. Projected on the ground, its trajectory began SW of Bari and ended NE of Matera. From the data collected by the PRISMA network, it was possible to fully characterize the meteoroid, which was determined to have a pre-atmospheric mass of 5 – 21 kg, corresponding to a size of 15 – 24 cm. Its pre-atmospheric orbit was determined to be of asteroidal origin, having a moderate eccentricity of 0.54 ± 0.02, an inclination on the ecliptic plane of 14.5° ± 0.2° and a semi-major axis of 2.10 ± 0.07 AU, with a Tisserand’s parameter of 3.51 ± 0.08. According to a photo-dynamic model, simultaneously fitting for the speed and magnitude data, the residual meteorite mass was determined to be 0.10 ± 0.04 kg (4.4 ± 0.7 cm of size). The area of fall of meteorites was estimated to be located north of Matera, in the Basilicata region. In this contribution, we discuss the analysis of the IT20230214 bolide and, in particular, the finding of the Matera meteorite on 17/03/2023, reported by the brothers Mr. Gianfranco and Pino Losignore in Contrada Rondinelle, in the municipality of Matera. With a total recovered mass of 117.5 g, the Matera meteorite was classified as an H5 ordinary chondrite.

PRISMA team:

M. Albani, A. Andreis, G. Ascione, T. Avoscan, P. Bacci, R. Baldini, A. Balestrero, S. Basso, R. Bellitto, C. Benna, F. Bernardi, M. E. Bertaina, L. Betti, D. Bonino, R. Bonino, K. Boros, M. Bubani, A. Bussi, A. Buzzoni, G. N. Cabizza, E. Cadau, P. Calcidese, C. Carli, T. Carriero, E. Cascone, C. Cattaneo, A. Cellino, P. Colombetti, E. Colombi, G. Colombo, M. Costa, G. Cremonese, D. Cricchio, T. Cuppone, G. D’Agostino, M. D’Elia, M. De Maio, P. Demaria, A. Di Dato, R. Di Luca, F. Federici, D. Fiacchini, M. Forteleoni, A. Frigo, F. Frontera, V. Gagliarducci, T. Gamba, M. Garoni, F. Gasparo, A. Gerardi, G. Giuli, D. Guidetti, G. Interrante, R. Jarre, C. Knapic, M. Lazzarin, S. Lera, G. Leto, D. Licchelli, F. Lippolis, F. Manca, S. Mancuso, F. Mannucci, R. Masi, S. Masiero, P. Mercogliano, S. Meucci, A. Misiano, V. Moggi Cecchi, E. Molinari, J. Monari, M. Montemaggi, M. Montesarchio, G. Monti, P. Morini, A. Nastasi, D. Nieto, A. Novati, V. Orofino, E. Pace, R. Pardini, M. Pavone, A. Pegoraro, S. Pietronave, T. Pisanu, N. Pugno, U. Repetti, M. P. Ricciardi, M. Rigoni, N. Rizzi, M. Romeo, S. Rubinetti, P. Russo, F. Salvati, D. Selvestrel, R. Serra, C. Simoncelli, R. Smareglia, M. Soldi, R. Stanga, F. Strafella, G. Talami, C. Taricco, G. Tigani Sava, M. Tombelli, P. Trivero, G. Umbriaco, C. Vaccaro, R. Vairetti, G. Valente, D. Valeri, G. B. Valsecchi, P. Volpini, R. Zagarella, A. Zollo (an updated list is available at https://www.prisma.inaf.it/index.php/chi-siamo/il-nostro-team/)

How to cite: Barghini, D., Carbognani, A., Gardiol, D., Bertocco, S., Di Carlo, M., Di Martino, M., Falco, C., Fenucci, M., Morelli, M., Pratesi, G., Riva, W., Salerno, R., Stirpe, G. M., and Volpicelli, C. A. and the PRISMA team: The recovery of the Matera H5 ordinary chondrite thanks to the observations of the PRISMA fireball network, Europlanet Science Congress 2024, Berlin, Germany, 8–13 Sep 2024, EPSC2024-449, https://doi.org/10.5194/epsc2024-449, 2024.