Zobrazeno 1 - 10
of 567
pro vyhledávání: '"Fulchignoni M"'
Autor:
Hromakina, T., Birlan, M., Barucci, M. A., Fulchignoni, M., Colas, F., Fornasier, S., Merlin, F., Sonka, A., Anghel, S., Poggiali, G., Belskaya, I., Perna, D., Dotto, E., team, the NEOROCKS
We present new results of the observing program which is a part of the NEOROCKS project aimed to improve knowledge on physical properties of near-Earth Objects (NEOs) for planetary defense. Photometric observations were performed using the 1.2m teles
Externí odkaz:
http://arxiv.org/abs/2302.01165
Autor:
Ieva, S., Dotto, E., Lazzaro, D., Fulvio, D., Perna, D., Epifani, E. Mazzotta, Medeiros, H., Fulchignoni, M.
The majority of basaltic objects in the main belt are dynamically connected to Vesta, the largest differentiated asteroid known. Others, due to their current orbital parameters, cannot be easily dynamically linked to Vesta. This is particularly true
Externí odkaz:
http://arxiv.org/abs/1806.04065
Autor:
Popescu, M., Perna, D., Barucci, M. A., Fornasier, S., Doressoundiram, A., Lantz, C., Merlin, F., Belskaya, I. N., Fulchignoni, M.
In the framework of a 30-night spectroscopic survey of small near-Earth asteroids (NEAs) we present new results regarding the identification of olivine-rich objects. The following NEAs were classified as A-type using visible spectra obtained with 3.6
Externí odkaz:
http://arxiv.org/abs/1803.04486
Publikováno v:
A&A 577, A147 (2015)
Context. The 4th release of the SDSS Moving Object Catalog (SDSSMOC) is presently the largest photometric dataset of asteroids. Up to this point, the release of large asteroid datasets has always been followed by a redefinition of asteroid taxonomy.
Externí odkaz:
http://arxiv.org/abs/1710.01180
Autor:
Bott, N., Perna, D., Deshapriya, J.D.P., Hasselmann, P.H., Barucci, M.A., Domingue, D.L., Dotto, E., Kitazato, K., Matsuoka, M., Palomba, E., Usui, T., Fulchignoni, M.
Publikováno v:
In Planetary and Space Science 15 September 2022 219
Autor:
Praet, A., Barucci, M.A., Clark, B.E., Kaplan, H.H., Simon, A.A., Hamilton, V.E., Emery, J.P., Howell, E.S., Lim, L.F., Zou, X.-D., Li, J.-Y., Reuter, D.C., Merlin, F., Deshapriya, J.D.P., Fornasier, S., Hasselmann, P.H., Poggiali, G., Ferrone, S., Brucato, J.R., Takir, D., Cloutis, E., Connolly, H.C., Jr, Fulchignoni, M., Lauretta, D.S.
Publikováno v:
In Icarus 15 July 2021 363
Autor:
Barucci, M. A., Filacchione, G., Fornasier, S., Raponi, A., Deshapriya, J. D. P., Tosi, F., Feller, C., Ciarniello, M., Sierks, H., Capaccioni, F., Pommerol, A., Massironi, M., Oklay, N., Merlin, F., Vincent, J. -B., Fulchignoni, M., Guilbert-Lepoutre, A., Perna, D., Capria, M. T., Hasselmann, P. H., Rousseau, B., Barbieri, C., Bockelee-Morvan, D., Lamy, P. L., De Sanctis, C., Rodrigo, R., Erard, S., Koschny, D., Leyrat, C., Rickman, H., Drossart, P., Keller, H. U., A'Hearn, M. F., Arnold, G., Bertaux, J. -L., Bertini, I., Cerroni, P., Cremonese, G., Da Deppo, V., Davidsson, B. J. R., El-Maarry, Fonti, S., Fulle, M., Groussin, O., Guttler, C.
Publikováno v:
A&A 595, A102 (2016)
Since the orbital insertion of the Rosetta spacecraft, comet 67P/Churyumov-Gerasimenko (67P/C-G) has been mapped by OSIRIS camera and VIRTIS spectro-imager, producing a huge quantity of images and spectra of the comet's nucleus. The aim of this work
Externí odkaz:
http://arxiv.org/abs/1609.00551
In recent years several small basaltic V-type asteroids have been identified all around the main belt. Most of them are members of the Vesta dynamical family, but an increasingly large number appear to have no link with it. The question that arises i
Externí odkaz:
http://arxiv.org/abs/1510.08776
Autor:
Deshapriya, J.D.P., Barucci, M.A., Bierhaus, E.B., Fornasier, S., Hasselmann, P.H., Merlin, F., Clark, B.E., Praet, A., Fulchignoni, M., Simon, A.A., Hamilton, Victoria E., Cloutis, E.A., Lantz, C., Zou, X.D., Li, J.-Y., Reuter, D.C., Brucato, J.R., Poggiali, G., Daly, R.T., Trang, D., Ferrone, S., DellaGiustina, D.N., Lauretta, D.S.
Publikováno v:
In Icarus 15 March 2021 357
Autor:
Carry, B., Kaasalainen, M., Leyrat, C., Merline, W. J., Drummond, J. D., Conrad, A., Weaver, H. A., Tamblyn, P. M., Chapman, C. R., Dumas, C., Colas, F., Christou, J. C., Dotto, E., Perna, D., Fornasier, S., Bernasconi, L., Behrend, R., Vachier, F., Kryszczynska, A., Polinska, M., Fulchignoni, M., Roy, R., Naves, R., Poncy, R., Wiggins, P.
Aims. We determine the physical properties (spin state and shape) of asteroid (21) Lutetia, target of the ESA Rosetta mission, to help in preparing for observations during the flyby on 2010 July 10 by predicting the orientation of Lutetia as seen fro
Externí odkaz:
http://arxiv.org/abs/1005.5356