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Autor:
S. Ieva (1), E. Dotto (1), E. Mazzotta Epifani (1), D. Perna (1, A. Rossi (3), A. Di Paola (1), A. Giunta (1), M. Micheli (1, E. Perozzi (5), R. Speziali (1), M. Lazzarin (6), I. Bertini (6), P. Ochner (6), V. Petropoulou (6), D. Lazzaro (7), P. Arcoverde (7), H. Medeiros (7), F. Monteiro (7)
Publikováno v:
European Planetary Science Congress 2018, Berlin, Germany, 16-21 September 2018
info:cnr-pdr/source/autori:S. Ieva (1), E. Dotto (1), E. Mazzotta Epifani (1), D. Perna (1,2), A. Rossi (3), A. Di Paola (1), A. Giunta (1), M. Micheli (1,4), E. Perozzi (5), R. Speziali (1), M. Lazzarin (6), I. Bertini (6), P. Ochner (6), V. Petropoulou (6), D. Lazzaro (7), P. Arcoverde (7), H. Medeiros (7), F. Monteiro (7)/congresso_nome:European Planetary Science Congress 2018/congresso_luogo:Berlin, Germany/congresso_data:16-21 September 2018/anno:2018/pagina_da:/pagina_a:/intervallo_pagine
info:cnr-pdr/source/autori:S. Ieva (1), E. Dotto (1), E. Mazzotta Epifani (1), D. Perna (1,2), A. Rossi (3), A. Di Paola (1), A. Giunta (1), M. Micheli (1,4), E. Perozzi (5), R. Speziali (1), M. Lazzarin (6), I. Bertini (6), P. Ochner (6), V. Petropoulou (6), D. Lazzaro (7), P. Arcoverde (7), H. Medeiros (7), F. Monteiro (7)/congresso_nome:European Planetary Science Congress 2018/congresso_luogo:Berlin, Germany/congresso_data:16-21 September 2018/anno:2018/pagina_da:/pagina_a:/intervallo_pagine
More than 85% of the 18,000 NEOs discovered up to now lack a physical characterization. The situation is even more dramatic for the small NEO population (D < 300 m). We conducted photometric observations for a large collection of uncharacterized NEOs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=cnr_________::dc44ba051f8a6333d7aab54a8e6c78e2
https://publications.cnr.it/doc/425188
https://publications.cnr.it/doc/425188