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101. SIMBIO-SYS: The spectrometer and imagers integrated observatory system for the BepiColombo planetary orbiter

Author

Flamini, E., Capaccioni, F., Colangeli, L., Cremonese, G., Doressoundiram, A., Josset, J.L., Langevin, Y., Debei, S., Capria, M.T., De Sanctis, M.C., Marinangeli, L., Massironi, M., Mazzotta Epifani, E., Naletto, G., Palumbo, P., Eng, P., Roig, J.F., Caporali, A., Da Deppo, V., Erard, S., Federico, C., Forni, O., Sgavetti, M., Filacchione, G., Giacomini, L., Marra, G., Martellato, E., Zusi, M., Cosi, M., Bettanini, C., Calamai, L., Zaccariotto, M., Tommasi, L., Dami, M., Ficai Veltroni, J., Poulet, F., and Hello, Y.

Published
2010
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105. PHEBUS: A double ultraviolet spectrometer to observe Mercury's exosphere

Author

Chassefière, E., Maria, J.-L., Goutail, J.-P., Quémerais, E., Leblanc, F., Okano, S., Yoshikawa, I., Korablev, O., Gnedykh, V., Naletto, G., Nicolosi, P., Pelizzo, M.-G., Correia, J.-J., Gallet, S., Hourtoule, C., Mine, P.-O., Montaron, C., Rouanet, N., Rigal, J.-B., Muramaki, G., Yoshioka, K., Kozlov, O., Kottsov, V., Moisseev, P., Semena, N., Bertaux, J.-L., Capria, M.-Th., Clarke, J., Cremonese, G., Delcourt, D., Doressoundiram, A., Erard, S., Gladstone, R., Grande, M., Hunten, D., Ip, W., Izmodenov, V., Jambon, A., Johnson, R., Kallio, E., Killen, R., Lallement, R., Luhmann, J., Mendillo, M., Milillo, A., Palme, H., Potter, A., Sasaki, S., Slater, D., Sprague, A., Stern, A., and Yan, N.

Published
2010
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109. Semi-Quantitative Identification of Colour Associated Gully Changes Through CaSSIS Band Ratios and Spectral Analysis Techniques

Author

Rangarajan, V, Tornabene, L, Osinski, G, Seelos, F, Conway, Susan J., Dundas, C, Patel, M, Thomas, N, Cremonese, G, Pajola, M, Lucchetti, A, Munaretto, G, Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2021

110. Potential Detection of Exposed Martian Water Ice with Multispectral Images from the 2016 Exomars TGO Colour and Stereo Surface Imaging System (CaSSIS)

Author

Tornabene, L, Becerra, P, Cesar, C, Conway, Susan J., Cremonese, G, Lucchetti, A, Munaretto, G, McEwen, A, Pajola, M, Patel, M, Perry, J, Pommerol, A, Rangarajan, V, Seelos, F, Thomas, N, Wray, J, Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2021

111. Non-Spherical Dust Dynamics of the Ejecta Plume in Support of Dart/liciacube Mission

Author

Ivanovski, S. L., Lucchetti, A., Pajola, M., Rossi, A., Bertini, I., Zanotti, G., Perna, D., Dotto, E., Della Corte, V., Amoroso, M., Pirrotta, S., Lavagna, M., Fahnestock, E. G., Hirabayashi, M., Raducan, S. D., Brucato, J. R., Capannolo, A., Cremonese, G., Gai, I., Ieva, S., Impresario, G., Mazzotta Epifani, E., Meneghin, A., Modenini, D., Simioni, E., Palumbo, P., Poggiali, G., Tortora, P., Zannoni, M., Zinzi, A., Luther, R., Cotugno, B., Di Tana, V., Miglioretti, F., and Simonetti, S.

Published
2021

112. Dynamics of Ejecta in the Didymos-Dimorphos Binary: Sensitivity to the System Parameters

Author

Rossi, A., Tsiganis, K., Gaitanas, M., Lucchetti, A., Ivanovski, S., Raducan, S., Dotto, E., Della Corte, V., Amoroso, M., Pirrotta, S., Bertini, I., Brucato, J. -R., Capannolo, A., Cotugno, B., Cremonese, G., Di Tana, V., Gai, I., Ieva, S., Impresario, G., Lavagna, M., Mazzotta-Epifani, E., Meneghin, A., Miglioretti, F., Modenini, D., Pajola, M., Perna, D., Palumbo, P., Poggiali, G., Simioni, E., Simonetti, S., Tortora, P., Zannoni, M., Zanotti, G., Zinzi, A., and Marzari, F.

Published
2021

113. LICIACube at (65803) Didymos: The Italian Cubesat in Support to the NASA DART Mission

Author

Dotto, E., Della Corte, V., Amoroso, M., Bertini, I., Brucato, J. R. search by orcid, Capannolo, A., Cotugno, B., Cremonese, G., Di Tana, V., Gai, I., Ieva, S., Impresario, G., Ivanovski, S. L., Lavagna, M., Lucchetti, A. search by orcid, Mazzotta Epifani, E., Meneghin, A., Miglioretti, F., Modenini, D., Pajola, M. Palumbo, P., Perna, D., Pirrotta, S., Poggiali, G., Rossi, A., Simioni, E., Simonetti, S., Tortora, P., Zannoni, M., Zanotti, G., Zinzi, A., Cheng, A. F., Rivkin, A. S., Adams, E. Y., Reynolds, E. L., and Fretz, K.

Subjects
Near Earth Asteroids, DART/LICIACube mission
Abstract

DART, the NASA Double Asteroid Redirection Test will be the first mission demonstrating the applicability of the kinetic impactor to change the motion of an asteroid in space and prevent the impact of Earth with a hazardous object. After being launched in 2021, in autumn 2022 the DART spacecraft will impact Dimorphos, the secondary member of the (65803) Didymos binary asteroid. With a mass of 650 kg and an impact velocity of about 6.6 km/s, DART is expected to change the binary orbital period of the 160-m Dimorphos by about 10 minutes, an effect that can be easily measured by ground-based telescopes.

Published
2021

114. Color and multi-angular observations of martian slope streaks

Author

Valantinas, A., Becerra, P., Pommerol, A., Tornabene, L. L., Affolter, L., Cremonese, G., Hauber, E., Mcewen, A. S., Munaretto, G., Pajola, M., Parkes Bowen, A., Patel, M. R., Rangarajan, V. G., Schorghofer, N., and Thomas, N.

Published
2021

115. Rotational Resolved Spectroscopy of the Didymos System, Target of the DART/LICIACube Mission

Author

Ieva, S., Mazzotta Epifani, E., Dotto, E., Perna, D., Brucato, J. R., Poggiali, G., Pajola, M., Lazzarin, M., La Forgia, F., Rossi, A., Palumbo, P., Della Corte, V., Migliorini, A., Zannoni, M., Snodgrass, C., Pravec, P., Granvik, M., Lucchetti, A., Ivanovski, S., Meneghin, A., Amoroso, M., Pirrotta, S., Bertini, I., Capannolo, A., Cotugno, B., Cremonese, G., Di Tana, V., Gai, I., Impresario, G., Lavagna, M., Miglioretti, F., Modenini, D., Simioni, E., Simonetti, S., Tortora, P., Zanotti, G., Zinzi, A., Thomas, C., and Rivkin, A. S.

Published
2021

116. Influence of the body composition on the evolution of ejecta in the Didymos-Dimorphos binary system

Author

Rossi, A., Tsiganis, K., Gaitanas, M., Marzari, F., Lucchetti, A., Ivanovski, S., Raducan, S., Dotto, E., Della Corte, V., Amoroso, M., Pirrotta, S., Bertini, I., Brucato, J. R., Capannolo, A., Cotugno, B., Cremonese, G., Di Tana, V., Gai, I., Ieva, S., Impresario, G., Lavagna, M., Mazzotta-Epifani, E., Meneghin, A., Miglioretti, F., Modenini, D., Pajola, M., Perna, D., Palumbo, P., Poggiali, G., Simioni, E., Simonetti, S., Tortora, P., Zannoni, M., Zanotti, G., and Zinzi, A.

Published
2021

117. Expected geological assessments at Didymos and Dimorphos from DART and LICIACube

Author

Pajola, M., Barnouin, O., Lucchetti, A., Dotto, E., Ernst, C. M., Della Corte, V., Daly, R. T., Poggiali, G., Perna, D., Hirabayashi, M., Ieva, S., Ivanovski, S., Mazzotta Epifani, E., Asphaug, E., Simioni, E., Michel, P., Amoroso, M., Bertini, I., Brucato, J. R., Capannolo, A., Chabot, N., Cheng, A., Cotugno, B., Cremonese, G., Di Tana, V., Fahnestock, E. G., Gai, I., Impresario, G., Lavagna, M., Meneghin, A., Miglioretti, F., Modenini, D., Palumbo, P., Pirrotta, S., Rivkin, A., Rossi, A., Schwartz, S. R., Simonetti, S., Tortora, P., Trigo-Rodriguez, J. M., Zannoni, M., Zanotti, G., and Zinzi, A.

Published
2021

118. Correction to: SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo (Space Science Reviews, (2021), 217, 1, (11), 10.1007/s11214-020-00787-3)

Author

Orsini, S. Livi, S.A. Lichtenegger, H. Barabash, S. Milillo, A. De Angelis, E. Phillips, M. Laky, G. Wieser, M. Olivieri, A. Plainaki, C. Ho, G. Killen, R.M. Slavin, J.A. Wurz, P. Berthelier, J.-J. Dandouras, I. Kallio, E. McKenna-Lawlor, S. Szalai, S. Torkar, K. Vaisberg, O. Allegrini, F. Daglis, I.A. Dong, C. Escoubet, C.P. Fatemi, S. Fränz, M. Ivanovski, S. Krupp, N. Lammer, H. Leblanc, F. Mangano, V. Mura, A. Nilsson, H. Raines, J.M. Rispoli, R. Sarantos, M. Smith, H.T. Szego, K. Aronica, A. Camozzi, F. Di Lellis, A.M. Fremuth, G. Giner, F. Gurnee, R. Hayes, J. Jeszenszky, H. Tominetti, F. Trantham, B. Balaz, J. Baumjohann, W. Brienza, D. Bührke, U. Bush, M.D. Cantatore, M. Cibella, S. Colasanti, L. Cremonese, G. Cremonesi, L. D’Alessandro, M. Delcourt, D. Delva, M. Desai, M. Fama, M. Ferris, M. Fischer, H. Gaggero, A. Gamborino, D. Garnier, P. Gibson, W.C. Goldstein, R. Grande, M. Grishin, V. Haggerty, D. Holmström, M. Horvath, I. Hsieh, K.-C. Jacques, A. Johnson, R.E. Kazakov, A. Kecskemety, K. Krüger, H. Kürbisch, C. Lazzarotto, F. Leblanc, F. Leichtfried, M. Leoni, R. Loose, A. Maschietti, D. Massetti, S. Mattioli, F. Miller, G. Moissenko, D. Morbidini, A. Noschese, R. Nuccilli, F. Nunez, C. Paschalidis, N. Persyn, S. Piazza, D. Oja, M. Ryno, J. Schmidt, W. Scheer, J.A. Shestakov, A. Shuvalov, S. Seki, K. Selci, S. Smith, K. Sordini, R. Svensson, J. Szalai, L. Toublanc, D. Urdiales, C. Varsani, A. Vertolli, N. Wallner, R. Wahlstroem, P. Wilson, P. Zampieri, S.

Subjects
GeneralLiterature_INTRODUCTORYANDSURVEY
Abstract

The original online version of this article was revised because a number of authors had the wrong affiliation number next to their names. © 2021, Springer Nature B.V.

Published
2021

119. Rotational Properties of Binary Asteroid System (65803) Didymos, Target of the DART/LICIACube and HERA Missions

Author

Ieva, S., Mazzotta Epifani, E., Dotto, E., Perna, D., Brucato, J. R. search by orcid, Poggiali, G., Pajola, M., Lazzarin, M., La Forgia, F., Rossi, A., Palumbo, P., Della Corte, V., Migliorini, A., Zannoni, M., Snodgrass, C., Pravec, P., Granvik, M., Lucchetti, A. search by orcid, Ivanovski, S., Meneghin, A. Amoroso, M., Pirrotta, S., Bertini, I., Capannolo, A., Cotugno, B., Cremonese, G., Di Tana, V., Gai, I., Impresario, G., Lavagna, M., Miglioretti, F., Modenini, D., Simioni, E., Simonetti, S., Tortora, P., Zanotti, G., Zinzi, A., Thomas, C., and Rivkin, A. S.

Subjects
Near Earth Asteroids, DART/LICIACube mission, Spectroscopy
Abstract

Near-Earth objects (NEOs), due to their proximity to our planet, represent one of the most accessible bodies in the whole Solar System. Their investigation can provide answers to several pressing questions in modern planetology (regarding, e.g., planetary formation, delivery of water and organics to the early Earth, and emergence of life). Moreover, water and valued minerals stored inside NEOs have already intrigued governments and private companies, allured by the idea of exploiting resources through asteroid mining. However, NEOs can represent a risk for future human civilization, since some of them can be potential impactors. To this purpose, the NASA Double Asteroid Redirection Test (DART) has been approved to be the first demonstration of an hazard mitigation of an asteroid by using a kinetic impactor.

Published
2021

120. Spectroscopic Characterization of the Didymos System, Target of the Kinetic Impactor Dart/liciacube Mission

Author

Ieva, S., Mazzotta Epifani, E., Dotto, E., Perna, D., Brucato, J. R., Poggiali, G., Pajola, M., Lazzarin, M., La Forgia, F., Rossi, A., Palumbo, P., Della Corte, V., Migliorini, A., Zannoni, M., Snodgrass, C., Pravec, P., Granvik, M., Lucchetti, A., Ivanovski, S., Meneghin, A., Amoroso, M., Pirrotta, S., Bertini, I., Capannolo, A., Cotugno, B., Cremonese, G., Di Tana, V., Gai, I., Impresario, G., Lavagna, M., Miglioretti, F., Modenini, D., Simioni, E., Simonetti, S., Tortora, P., Zanotti, G., Zinzi, A., Thomas, C., and Rivkin, A. S.

Published
2021

121. Observational constraints to the dynamics of dust particles in the coma of comet 67P/Churyumov–Gerasimenko

Author

Frattin, E, primary, Bertini, I, additional, Ivanovski, S L, additional, Marzari, F, additional, Fulle, M, additional, Zakharov, V V, additional, Moreno, F, additional, Naletto, G, additional, Lazzarin, M, additional, Cambianica, P, additional, Cremonese, G, additional, Ferrari, S, additional, Ferri, F, additional, Güttler, C, additional, La Forgia, F, additional, Lucchetti, A, additional, Pajola, M, additional, Penasa, L, additional, Rotundi, A, additional, Sierks, H, additional, and Tubiana, C, additional

Published
2021
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122. Long-term measurements of the erosion and accretion of dust deposits on comet 67P/Churyumov–Gerasimenko with the OSIRIS instrument

Author

Cambianica, P, primary, Cremonese, G, additional, Fulle, M, additional, Simioni, E, additional, Naletto, G, additional, Pajola, M, additional, Lucchetti, A, additional, Penasa, L, additional, Massironi, M, additional, Frattin, E, additional, Güttler, C, additional, Sierks, H, additional, and Tubiana, C, additional

Published
2021
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125. Spatial variations of the sodium/potassium ratio in Mercury's exosphere uncovered by high-resolution spectroscopy

Author

Doressoundiram, A., Leblanc, F., Foellmi, C., Gicquel, A., Cremonese, G., Donati, J.-F., and Veillet, C.

Subjects
Astronomy -- Environmental aspects, Spectrum analysis -- Environmental aspects, Atmosphere -- Environmental aspects, Earth -- Atmosphere, Earth -- Environmental aspects, Astronomy, Earth sciences
Abstract

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2009.11.020 Byline: A. Doressoundiram (a), F. Leblanc (b), C. Foellmi (c), A. Gicquel (a), G. Cremonese (d), J.-F. Donati (e), C. Veillet (f) Keywords: Mercury, Atmosphere; Abundances, Atmospheres; Spectroscopy Abstract: High-resolution spectroscopy of Mercury has been obtained with two different instruments in 2006: the EMMI instrument at the 3.6-m NTT telescope of ESO La Silla Chile and the ESPADON spectrograph at the 3.6-m CFHT telescope on top of Mauna Kea (Hawaii). The disk of the planet has been scanned for spatial variation of the exospheric species. The large spectral range and high resolution allow simultaneous measurements of the integrated column density of Na and K. We measure Na/K ratio between 80 and 400 with values between 60 and 90 when the telescope was pointed towards the subsolar region of Mercury's disk and much larger value when we looked to other part of the exosphere. Moreover, we observed that the Na and K exospheres display very different spatial distributions. Even if these two species are probably ejected with very similar mechanisms from the surface, their differences in mass and sensitivity to solar pressure acceleration imply very different behavior in Mercury's exosphere. Author Affiliation: (a) LESIA, Observatoire de Paris, F-92195 Meudon Principal Cedex, France (b) LATMOS/IPSL, Universite Versailles Saint Quentin, CNRS, France (c) Laboratoire d'Astrophysique de l'Observatoire de Grenoble, F-38041 Grenoble Cedex 09, France (d) INAF - Osservatorio Astronomico di Padova, Italy (e) CNRS/Universite de Toulouse, LATT/UMR 5572, Observatoire Midi-Pyrenees, F-31400 Toulouse, France (f) Canada-France-Hawaii Telescope Corporation, PO Box 1597, Kamuela, HI 96743, USA Article History: Received 3 March 2009; Revised 7 October 2009; Accepted 15 November 2009 Article Note: (footnote) [star] Based on observations carried out at the European Southern Observatory (ESO), La Silla, Chile, programme id 078.C-0038 and at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

Published
2010

126. Triple F—a comet nucleus sample return mission

Author

Küppers, Michael, Keller, H. U., Kührt, E., A’Hearn, M. F., Altwegg, K., Bertrand, R., Busemann, H., Capria, M. T., Colangeli, L., Davidsson, B., Ehrenfreund, P., Knollenberg, J., Mottola, S., Rathke, A., Weiss, P., Zolensky, M., Akim, E., Basilevsky, A., Galimov, E., Gerasimov, M., Korablev, O., Lomakin, I., Marov, M., Martynov, M., Nazarov, M., Zakharov, A., Zelenyi, L., Aronica, A., Ball, A. J., Barbieri, C., Bar-Nun, A., Benkhoff, J., Biele, J., Biver, N., Blum, J., Bockelée-Morvan, D., Botta, O., Bredehöft, J.-H., Capaccioni, F., Charnley, S., Cloutis, E., Cottin, H., Cremonese, G., Crovisier, J., Crowther, S. A., Epifani, E. M., Esposito, F., Ferrari, A. C., Ferri, F., Fulle, M., Gilmour, J., Goesmann, F., Gortsas, N., Green, S. F., Groussin, O., Grün, E., Gutiérrez, P. J., Hartogh, P., Henkel, T., Hilchenbach, M., Ho, T.-M., Horneck, G., Hviid, S. F., Ip, W.-H., Jäckel, A., Jessberger, E., Kallenbach, R., Kargl, G., Kömle, N. I., Korth, A., Kossacki, K., Krause, C., Krüger, H., Li, Z.-Y., Licandro, J., Lopez-Moreno, J. J., Lowry, S. C., Lyon, I., Magni, G., Mall, U., Mann, I., Markiewicz, W., Martins, Z., Maurette, M., Meierhenrich, U., Mennella, V., Ng, T. C., Nittler, L. R., Palumbo, P., Pätzold, M., Prialnik, D., Rengel, M., Rickman, H., Rodriguez, J., Roll, R., Rost, D., Rotundi, A., Sandford, S., Schönbächler, M., Sierks, H., Srama, R., Stroud, R. M., Szutowicz, S., Tornow, C., Ulamec, S., Wallis, M., Waniak, W., Weissman, P., Wieler, R., Wurz, P., Yung, K. L., and Zarnecki, J. C.

Published
2009
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127. Mars environment and magnetic orbiter model payload

Author

Langlais, B., Leblanc, F., Fouchet, T., Barabash, S., Breuer, D., Chassefière, E., Coates, A., Dehant, V., Forget, F., Lammer, H., Lewis, S., Lopez-Valverde, M., Mandea, M., Menvielle, M., Pais, A., Paetzold, M., Read, P., Sotin, C., Tarits, P., Vennerstrom, S., Branduardi-Raymont, G., Cremonese, G., Merayo, J. G. M., Ott, T., Rème, H., Trotignon, J. G., and Walhund, J. E.

Published
2009
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128. Detection of a southern peak in Mercury's sodium exosphere with the TNG in 2005

Author

Mangano, V., Leblanc, F., Barbieri, C., Massetti, S., Milillo, A., Cremonese, G., and Grava, C.

Subjects
Planetary meteorology -- Spectra, Planetary meteorology -- Analysis, Weather -- Analysis, Astronomy -- Spectra, Astronomy -- Analysis, Atmosphere -- Analysis, Earth -- Atmosphere, Earth -- Analysis, Astronomy, Earth sciences
Abstract

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2009.01.016 Byline: V. Mangano (a), F. Leblanc (b), C. Barbieri (c), S. Massetti (a), A. Milillo (a), G. Cremonese (d), C. Grava (c) Keywords: Mercury; atmosphere; Spectroscopy Abstract: A long term plan of observations of the sodium exosphere of Mercury began in 2002 by using the high resolution echelle spectrograph SARG and a devoted sodium filter at the 3.5 m Galileo National Telescope (TNG) located in La Palma, Canary Islands. This program is meant to investigate the variations of the sodium exosphere appearance under different conditions of observations, namely Mercury's position along its orbit, phase angle and different solar conditions, as reported by previous observations in August 2002 and August 2003 [Barbieri, C., Verani, S., Cremonese, G., Sprague, A., Mendillo, M., Cosentino, R., Hunten, D., 2004. Planet. Space Sci. 52, 1169-1175; Leblanc, F., Barbieri, C., Cremonese, G., Verani, S., Cosentino, R., Mendillo, M., Sprague, A., Hunten, D., 2006. Icarus 185 (2), 395-402]. Here we present the analysis of data taken in June 29th and 30th and in July 1st 2005, when Mercury's true anomaly angle (TAA) was in the range 124-130[degrees]. The spectra show particularly intense sodium lines with a distinctive peak in emission localized in the southern hemisphere at mid-latitudes. This seems to be a persistent feature related to consecutive favorable IMF conditions inducing localized enhancements of surface sodium density. The comparison with previous data taken by Potter et al. [Potter, A.E., Killen, R.M., Morgan, T.H., 2002. Meteorit. Planet. Sci. 37 (9), 1165-1172] evidences a surprising consistency of the anti-sunward component, which appears to remain constant regardless of the changing illumination and space weather conditions at Mercury. Author Affiliation: (a) INAF-Istituto di Fisica dello Spazio Interplanetario, via Fosso del Cavaliere 100, 00133 Roma, Italy (b) Service d'Aeronomie, IPSL/CNRS, Universite Versailles Saint Quentin, Paris, France (c) Department of Astronomy, University of Padova, vicolo Osservatorio 2, 35122 Padova, Italy (d) INAF-Osservatorio Astronomico di Padova, 35122 Padova, Italy Article History: Received 18 November 2008; Revised 27 January 2009; Accepted 29 January 2009

Published
2009

131. OSIRIS – The Scientific Camera System Onboard Rosetta

Author

Keller, H. U., Barbieri, C., Lamy, P., Rickman, H., Rodrigo, R., Wenzel, K.-P., Sierks, H., A’Hearn, M. F., Angrilli, F., Angulo, M., Bailey, M. E., Barthol, P., Barucci, M. A., Bertaux, J.-L., Bianchini, G., Boit, J.-L., Brown, V., Burns, J. A., Büttner, I., Castro, J. M., Cremonese, G., Curdt, W., Deppo, V. Da, Debei, S., Cecco, M. De, Dohlen, K., Fornasier, S., Fulle, M., Germerott, D., Gliem, F., Guizzo, G. P., Hviid, S. F., Ip, W.-H., Jorda, L., Koschny, D., Kramm, J. R., Kührt, E., Küppers, M., Lara, L. M., Llebaria, A., López, A., López-Jimenez, A., López-Moreno, J., Meller, R., Michalik, H., Michelena, M. D., Müller, R., Naletto, G., Origné, A., Parzianello, G., Pertile, M., Quintana, C., Ragazzoni, R., Ramous, P., Reiche, K.-U., Reina, M., Rodríguez, J., Rousset, G., Sabau, L., Sanz, A., Sivan, J.-P., Stöckner, K., Tabero, J., Telljohann, U., Thomas, N., Timon, V., Tomasch, G., Wittrock, T., and Zaccariotto, M.

Published
2007
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132. LICIACube: the Light Italian Cubesat for Imaging of Asteroids

Author

Dotto, E., Della Corte, V., Amoroso, M., Bertini, I., Brucato, J. R., Capannolo, A., Cotugno, B., Cremonese, G., Di Tana, V., Gai, I., Ieva, S., Impresario, G., Ivanovski, S., Lavagna, M., Lucchetti, A., Mazzotta Epifani, E., Meneghin, A., Miglioretti, F., Modenini, D., Pajola, M., Palumbo, P., Perna, D., Pirrotta, S., Poggiali, G., Rossi, A., Simioni, E., Simonetti, S., Tortora, P., Zannoni, M., Zannotti, G., Zinzi, A., Cheng, A. F., Rivkin, A., Adams, E. Y., Reynolds, E., and Fretz, K.

Subjects
NATURAL HAZARDS, 4342 Emergency management, Astrodynamics, 4328 Risk, 4351 International organizations and natural disasters, 4328 Risk, NATURAL HAZARDS, 4339 Disaster mitigation, NATURAL HAZARDS, 4342 Emergency management, NATURAL HAZARDS, 4351 International organizations and natural disasters, NATURAL HAZARDS, Asteroid impact risk, LICIACube, 4339 Disaster mitigation, Asteroid ejecta dynamics
Abstract

"LICIACube - the Light Italian Cubesat for Imaging of Asteroids" is a CubeSat managed by the Italian Space Agency (ASI), that will be part of the NASA Double Asteroid Redirection Test (DART) mission [2]. DART will be the first mission demonstrating the applicability of the kinetic impactor to change to motion of an asteroid in space and prevent the impact of Earth with a hazardous object. After being launched in summer 2021, the DART spacecraft will impact in autumn 2022 Dimorphos, the secondary member of the (65803) Didymos binary asteroid. With a mass of 650 kg and an impact velocity of about 6.6 km/s, DART is expected to change the binary orbital period of the 160-m Dimorphos by about 10 minutes, an effect that can be easily measured by ground-based telescopes. The design, integration and test of the CubeSat have been assigned by ASI to the aerospace company Argotec, while the LICIACube Ground Segment has a complex architecture based on the Argotec Mission Control Centre, antennas of the NASA Deep Space Network and data archiving and processing, managed at the ASI Space Science Data Center. The LICIACube team includes a wide scientific community, involved in the definition of all the aspects of the mission: trajectory design; navigation analysis (and real-time orbit determination during operations); impact, plume and imaging simulation and modelling, in preparation of a suitable framework for the analysis and interpretation of in-situ data. The scientific team is led by National Institute of Astrophysics (OAR, IAPS, OAA, OAPd, OATs) with the support of IFAC-CNR and University Parthenope of Naples. The team is enriched by University of Bologna, for orbit determination and satellite navigation, and Polytechnic of Milan, for mission analysis and optimization. The major technological mission challenge, i.e. the autonomous targeting and imaging of such a small body during a fast fly-by, to be accomplished with the limited resources of a CubeSat, is affordable thanks to a strong synergy of all the mentioned teams in support of the engineering tasks.

Published
2020

133. Multidisciplinary Analysis of Lermontov Crater on Mercury

Author

PAJOLA, MAURIZIO, LUCCHETTI, ALICE, Semenzato, A., Munaretto, G., POGGIALI, GIOVANNI, Galluzzi, V., Cremonese, G., BRUCATO, John Robert, Palumbo, P., and Massironi, M.

Abstract

We present the geological, age determination, and spectrophotometric analysis of the Lermontov Crater on Mercury.

Published
2020

134. Physical characterization of NEOs with a CubeSat: LICIACube at (65803) Didymos

Author

Dotto, E., Della Corte, V., Amoroso, M., Bertini, I., Brucato, J., Capannolo, A., Cremonese, G., Cotugno, B., Di Tana, V., Gai, I., Ieva, S., Impresario, G., Ivanovski, S. L., Lavagna, M., Lucchetti, A., Mazzotta Epifani, E., Meneghin, A., Miglioretti, F., Modenini, D., Pajola, Palumbo, M., Perna, D., Pirrotta, S., Poggiali, G., Rossi, A., Simioni, E., Simonetti, S., Tortora, P., Zannoni, M., Zanotti, G., Zinzi, A., Cheng, A. F., Rivkin, A. S., Adams, E. Y., Reynolds, E. L., and Fretz, K

Subjects
Astrodynamics, Near Earth Asteroid, Asteroid impact risk, LICIACube, Asteroid ejecta dynamics
Abstract

The study of Near-Earth Objects (NEOs) has opened new frontiers in planetary sciences in the last decades due to the fact that their proximity makes them the most accessible bodies in our solar system. Their investigation can offer the answers to several hot topics in modern planetology (e.g. planetary formation, delivery of water and organics on early Earth, emergence of life). Furthermore, NEOs represent a risk for future human civilization, since some of them can be potential impactors. For all these reasons, the characterization of NEO physical properties is an essential topic in planetary sciences, from both ground and space. In this context, the NASA Double Asteroid Redirection Test (DART) will be the first mission demonstrating the applicability of the kinetic impactor to change to motion of an asteroid in space and prevent the impact of Earth with a hazardous object [1]. "LICIACube - the Light Italian Cubesat for Imaging of Asteroids"[2] - is managed by the Italian Space Agency (ASI) and will be part of the DART mission. LICIACube will be equipped with two optical cameras: LEIA (Liciacube Explorer Imaging for Asteroid), a catadioptric camera composed of two reflective elements and three refractive elements with a FoV of ± 2.06° on the sensor diagonal, and LUKE (Liciacube Unit Key Explorer), a camera with a RGB Bayer pattern filter designed for a deep of field from 400 m to infinity. After the release from the DART spacecraft, LICIACube will be autonomously guided to a fast fly-by with the target, reaching a minimum distance of about 55 km, and will acquire several images of the target impact and non-impact sides, as well as of the plume produced by the DART impact, with the aim: i) to document the DART impact's effects on Dimorphos, the secondary member of the Didymos binary system, ii) to characterize the shape of the target, and iii) to perform dedicated scientific investigations on it. Acknowledgements: We acknowledge financial support from Agenzia Spaziale Italiana (ASI, contract No. 2019-31-HH.0 CUP F84I190012600). . Cheng, A. F., et al., Plan. Space Sci., Vol. 157, pp. 104-115, 2018. . Dotto, E., et al., Plan. Space Sci., 2020, accepted.

Published
2020

137. Surface-Exosphere-Magnetosphere System Of Mercury

Author

Milillo, A., Wurz, P., Orsini, S., Delcourt, D., Kallio, E., KILLEN, R. M., Lammer, H., Massetti, S., Mura, A., Barabash, S., Cremonese, G., Daglis, I. A., De Angelis, E., Di Lellis, A. M., Livi, S., Mangano, V., and Torkar, K.

Published
2005
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138. Observations of Mercury's exosphere: Spatial distributions and variations of its Na component during August 8, 9 and 10, 2003

Author

Leblanc, F., Barbieri, C., Cremonese, G., Verani, S., Cosentino, R., Mendillo, M., Sprague, A., and Hunten, D.

Subjects
Mercury (Planet) -- Environmental aspects, Solar wind -- Properties, Magnetosphere -- Composition, Magnetosphere -- Properties, Sodium -- Properties, Sodium -- Distribution, Planets -- Atmosphere, Planets -- Composition, Planets -- Properties, Company distribution practices, Astronomy, Earth sciences
Abstract

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2006.08.006 Byline: F. Leblanc (a), C. Barbieri (b), G. Cremonese (c), S. Verani (b), R. Cosentino (d), M. Mendillo (e), A. Sprague (f), D. Hunten (f) Keywords: Mercury; atmosphere; Spectroscopy; Magnetospheres; Solar wind Abstract: Following the observations of August 2002 [Barbieri, C., Verani, S., Cremonese, G., Sprague, A., Mendillo, M., Cosentino, R., Hunten, D., 2004. Planet. Space Sci. 52, 1169-1175], the high resolution spectrograph of the 3.5-m Galileo National Telescope (TNG) has been used to obtain several spatially resolved spectra of Mercury's Na-D on the evenings of 8, 9 and 10 August 2003. The resolution of the spectrograph was 115,000, the slit dimensions were 0.4.sup.a[sup.3]x27.sup.a[sup.3]. With respect to Paper I, the planet was in a fairly similar orbital configuration, being at a geocentric distance of approximately 1 AU, and having a True Anomaly Angle (TAA) from 163[degrees]-168[degrees] instead of 171[degrees]-174[degrees]. We present here a significantly larger set of observations and discuss several important features regarding the formation of Mercury's sodium exosphere, in particular the role of photon stimulated and thermal desorptions, as well as of the solar wind sputtering and micro-meteoroid vaporization. Thanks to the very good seeing of these observations, we also report and discuss the origins and variations of equatorial structures in Mercury's early morning sodium exosphere. Author Affiliation: (a) Service d'Aeronomie du CNRS, Route des gatines, BP 3, 91371 Verrieres-Le-Buisson, France (b) Department of Astronomy, University of Padova, I-35122 Padova, Italy (c) Astronomical Observatory of Padova, INAF, I-35122 Padova, Italy (d) Telescopio Nazionale Galileo, INAF, 38700 Santa Cruz de La Palma, TF, Spain (e) Center for Space Physics, Boston University, MA 02215, USA (f) Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA Article History: Received 7 March 2006; Revised 2 August 2006

Published
2006

139. Release of neutral sodium atoms from the surface of Mercury induced by meteoroid impacts

Author

Cremonese, G., Bruno, M., Mangano, V., Marchi, S., and Milillo, A.

Subjects
Astronomy, Earth sciences
Abstract

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2005.03.022 Byline: G. Cremonese (a), M. Bruno (a), V. Mangano (b)(c), S. Marchi (d), A. Milillo (c) Keywords: Mercury; surface; Impact processes; Abundances; atmospheric Abstract: Meteoroid impact has been shown to be a source of sodium, and most likely of other elements, on the Moon. The same process could be also relevant for Mercury. In this work we calculate the vapor and neutral Na production rates on Mercury due to the impacts of meteoroids in the radius range of 10.sup.-8-10.sup.-1 m. We limit our calculations to this size range, because meteoroids with radius larger than 10.sup.-1 m have not to be found important for the daily production of the exosphere. This work is based on a new dynamical model of the meteoroid flux at the heliocentric distance of Mercury, regarding objects in the size range 10.sup.-2-10.sup.-1 m. This size range, never investigated before, is not affected by nongravitational forces, such as the Poynting-Robertson effect, which is dominant for particles smaller than 10.sup.-2 m. In order to evaluate the release of neutral sodium atoms also for smaller meteoroids we have used the distribution reported by M.J. Cintala [1992. Impact-induced thermal effects in the lunar and mercurian regoliths. J. Geophys. Res. 97, 947-973] calculated for particle size range 10.sup.-8-10.sup.-3 m. We have extrapolated this distribution up to 10.sup.-2 m and we have based the impact calculations on a new surface composition assuming 90% plagioclase and 10% pyroxene. The results of our model are that (i) the total mass of vapor produced by the impact of meteoroids in the size range 10.sup.-8-10.sup.-1 m is 4.752x10.sup.8g per year, and (ii) the production rate of neutral sodium atoms is 1.5x10.sup.22 s.sup.-1. Author Affiliation: (a) INAF Osservatorio Aastronomico Padova, Padova 35122, Italy (b) CISAS, Universita' di Padova, Padova, Italy (c) INAF, IFSI, Roma, Italy (d) Dipartimento di Astronomia, Universita' di Padova, Padova, Italy Article History: Received 16 September 2004; Revised 14 March 2005

Published
2005

140. FRIPON: a worldwide network to track incoming meteoroids

Author

Colas, F., primary, Zanda, B., additional, Bouley, S., additional, Jeanne, S., additional, Malgoyre, A., additional, Birlan, M., additional, Blanpain, C., additional, Gattacceca, J., additional, Jorda, L., additional, Lecubin, J., additional, Marmo, C., additional, Rault, J. L., additional, Vaubaillon, J., additional, Vernazza, P., additional, Yohia, C., additional, Gardiol, D., additional, Nedelcu, A., additional, Poppe, B., additional, Rowe, J., additional, Forcier, M., additional, Koschny, D., additional, Trigo-Rodriguez, J. M., additional, Lamy, H., additional, Behrend, R., additional, Ferrière, L., additional, Barghini, D., additional, Buzzoni, A., additional, Carbognani, A., additional, Di Carlo, M., additional, Di Martino, M., additional, Knapic, C., additional, Londero, E., additional, Pratesi, G., additional, Rasetti, S., additional, Riva, W., additional, Stirpe, G. M., additional, Valsecchi, G. B., additional, Volpicelli, C. A., additional, Zorba, S., additional, Coward, D., additional, Drolshagen, E., additional, Drolshagen, G., additional, Hernandez, O., additional, Jehin, E., additional, Jobin, M., additional, King, A., additional, Nitschelm, C., additional, Ott, T., additional, Sanchez-Lavega, A., additional, Toni, A., additional, Abraham, P., additional, Affaticati, F., additional, Albani, M., additional, Andreis, A., additional, Andrieu, T., additional, Anghel, S., additional, Antaluca, E., additional, Antier, K., additional, Appéré, T., additional, Armand, A., additional, Ascione, G., additional, Audureau, Y., additional, Auxepaules, G., additional, Avoscan, T., additional, Baba Aissa, D., additional, Bacci, P., additional, Bǎdescu, O., additional, Baldini, R., additional, Baldo, R., additional, Balestrero, A., additional, Baratoux, D., additional, Barbotin, E., additional, Bardy, M., additional, Basso, S., additional, Bautista, O., additional, Bayle, L. D., additional, Beck, P., additional, Bellitto, R., additional, Belluso, R., additional, Benna, C., additional, Benammi, M., additional, Beneteau, E., additional, Benkhaldoun, Z., additional, Bergamini, P., additional, Bernardi, F., additional, Bertaina, M. E., additional, Bessin, P., additional, Betti, L., additional, Bettonvil, F., additional, Bihel, D., additional, Birnbaum, C., additional, Blagoi, O., additional, Blouri, E., additional, Boacă, I., additional, Boatǎ, R., additional, Bobiet, B., additional, Bonino, R., additional, Boros, K., additional, Bouchet, E., additional, Borgeot, V., additional, Bouchez, E., additional, Boust, D., additional, Boudon, V., additional, Bouman, T., additional, Bourget, P., additional, Brandenburg, S., additional, Bramond, Ph., additional, Braun, E., additional, Bussi, A., additional, Cacault, P., additional, Caillier, B., additional, Calegaro, A., additional, Camargo, J., additional, Caminade, S., additional, Campana, A. P. C., additional, Campbell-Burns, P., additional, Canal-Domingo, R., additional, Carell, O., additional, Carreau, S., additional, Cascone, E., additional, Cattaneo, C., additional, Cauhape, P., additional, Cavier, P., additional, Celestin, S., additional, Cellino, A., additional, Champenois, M., additional, Chennaoui Aoudjehane, H., additional, Chevrier, S., additional, Cholvy, P., additional, Chomier, L., additional, Christou, A., additional, Cricchio, D., additional, Coadou, P., additional, Cocaign, J. Y., additional, Cochard, F., additional, Cointin, S., additional, Colombi, E., additional, Colque Saavedra, J. P., additional, Corp, L., additional, Costa, M., additional, Costard, F., additional, Cottier, M., additional, Cournoyer, P., additional, Coustal, E., additional, Cremonese, G., additional, Cristea, O., additional, Cuzon, J. C., additional, D’Agostino, G., additional, Daiffallah, K., additional, Dǎnescu, C., additional, Dardon, A., additional, Dasse, T., additional, Davadan, C., additional, Debs, V., additional, Defaix, J. P., additional, Deleflie, F., additional, D’Elia, M., additional, De Luca, P., additional, De Maria, P., additional, Deverchère, P., additional, Devillepoix, H., additional, Dias, A., additional, Di Dato, A., additional, Di Luca, R., additional, Dominici, F. M., additional, Drouard, A., additional, Dumont, J. L., additional, Dupouy, P., additional, Duvignac, L., additional, Egal, A., additional, Erasmus, N., additional, Esseiva, N., additional, Ebel, A., additional, Eisengarten, B., additional, Federici, F., additional, Feral, S., additional, Ferrant, G., additional, Ferreol, E., additional, Finitzer, P., additional, Foucault, A., additional, Francois, P., additional, Frîncu, M., additional, Froger, J. L., additional, Gaborit, F., additional, Gagliarducci, V., additional, Galard, J., additional, Gardavot, A., additional, Garmier, M., additional, Garnung, M., additional, Gautier, B., additional, Gendre, B., additional, Gerard, D., additional, Gerardi, A., additional, Godet, J. P., additional, Grandchamps, A., additional, Grouiez, B., additional, Groult, S., additional, Guidetti, D., additional, Giuli, G., additional, Hello, Y., additional, Henry, X., additional, Herbreteau, G., additional, Herpin, M., additional, Hewins, P., additional, Hillairet, J. J., additional, Horak, J., additional, Hueso, R., additional, Huet, E., additional, Huet, S., additional, Hyaumé, F., additional, Interrante, G., additional, Isselin, Y., additional, Jeangeorges, Y., additional, Janeux, P., additional, Jeanneret, P., additional, Jobse, K., additional, Jouin, S., additional, Jouvard, J. M., additional, Joy, K., additional, Julien, J. F., additional, Kacerek, R., additional, Kaire, M., additional, Kempf, M., additional, Krier, C., additional, Kwon, M. K., additional, Lacassagne, L., additional, Lachat, D., additional, Lagain, A., additional, Laisné, E., additional, Lanchares, V., additional, Laskar, J., additional, Lazzarin, M., additional, Leblanc, M., additional, Lebreton, J. P., additional, Lecomte, J., additional, Le Dû, P., additional, Lelong, F., additional, Lera, S., additional, Leoni, J. F., additional, Le-Pichon, A., additional, Le-Poupon, P., additional, Leroy, A., additional, Leto, G., additional, Levansuu, A., additional, Lewin, E., additional, Lienard, A., additional, Licchelli, D., additional, Locatelli, H., additional, Loehle, S., additional, Loizeau, D., additional, Luciani, L., additional, Maignan, M., additional, Manca, F., additional, Mancuso, S., additional, Mandon, E., additional, Mangold, N., additional, Mannucci, F., additional, Maquet, L., additional, Marant, D., additional, Marchal, Y., additional, Marin, J. L., additional, Martin-Brisset, J. C., additional, Martin, D., additional, Mathieu, D., additional, Maury, A., additional, Mespoulet, N., additional, Meyer, F., additional, Meyer, J. Y., additional, Meza, E., additional, Moggi Cecchi, V., additional, Moiroud, J. J., additional, Millan, M., additional, Montesarchio, M., additional, Misiano, A., additional, Molinari, E., additional, Molau, S., additional, Monari, J., additional, Monflier, B., additional, Monkos, A., additional, Montemaggi, M., additional, Monti, G., additional, Moreau, R., additional, Morin, J., additional, Mourgues, R., additional, Mousis, O., additional, Nablanc, C., additional, Nastasi, A., additional, Niacşu, L., additional, Notez, P., additional, Ory, M., additional, Pace, E., additional, Paganelli, M. A., additional, Pagola, A., additional, Pajuelo, M., additional, Palacián, J. F., additional, Pallier, G., additional, Paraschiv, P., additional, Pardini, R., additional, Pavone, M., additional, Pavy, G., additional, Payen, G., additional, Pegoraro, A., additional, Peña-Asensio, E., additional, Perez, L., additional, Pérez-Hoyos, S., additional, Perlerin, V., additional, Peyrot, A., additional, Peth, F., additional, Pic, V., additional, Pietronave, S., additional, Pilger, C., additional, Piquel, M., additional, Pisanu, T., additional, Poppe, M., additional, Portois, L., additional, Prezeau, J. F., additional, Pugno, N., additional, Quantin, C., additional, Quitté, G., additional, Rambaux, N., additional, Ravier, E., additional, Repetti, U., additional, Ribas, S., additional, Richard, C., additional, Richard, D., additional, Rigoni, M., additional, Rivet, J. P., additional, Rizzi, N., additional, Rochain, S., additional, Rojas, J.F., additional, Romeo, M., additional, Rotaru, M., additional, Rotger, M., additional, Rougier, P., additional, Rousselot, P., additional, Rousset, J., additional, Rousseu, D., additional, Rubiera, O., additional, Rudawska, R., additional, Rudelle, J., additional, Ruguet, J.P., additional, Russo, P., additional, Sales, S., additional, Sauzereau, O., additional, Salvati, F., additional, Schieffer, M., additional, Schreiner, D., additional, Scribano, Y., additional, Selvestrel, D., additional, Serra, R., additional, Shengold, L., additional, Shuttleworth, A., additional, Smareglia, R., additional, Sohy, S., additional, Soldi, M., additional, Stanga, R., additional, Steinhausser, A., additional, Strafella, F., additional, Sylla Mbaye, S., additional, Smedley, A. R. D., additional, Tagger, M., additional, Tanga, P., additional, Taricco, C., additional, Teng, J. P., additional, Tercu, J. O., additional, Thizy, O., additional, Thomas, J. P., additional, Tombelli, M., additional, Trangosi, R., additional, Tregon, B., additional, Trivero, P., additional, Tukkers, A., additional, Turcu, V., additional, Umbriaco, G., additional, Unda-Sanzana, E., additional, Vairetti, R., additional, Valenzuela, M., additional, Valente, G., additional, Varennes, G., additional, Vauclair, S., additional, Vergne, J., additional, Verlinden, M., additional, Vidal-Alaiz, M., additional, Vieira-Martins, R., additional, Viel, A., additional, Vîntdevarǎ, D. C., additional, Vinogradoff, V., additional, Volpini, P., additional, Wendling, M., additional, Wilhelm, P., additional, Wohlgemuth, K., additional, Yanguas, P., additional, Zagarella, R., additional, and Zollo, A., additional

Published
2020
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141. Cavezzo, the first Italian meteorite recovered by the PRISMA fireball network. Orbit, trajectory, and strewn-field

Author

Gardiol, D, primary, Barghini, D, additional, Buzzoni, A, additional, Carbognani, A, additional, Di Carlo, M, additional, Di Martino, M, additional, Knapic, C, additional, Londero, E, additional, Pratesi, G, additional, Rasetti, S, additional, Riva, W, additional, Salerno, R, additional, Stirpe, G M, additional, Valsecchi, G B, additional, Volpicelli, C A, additional, Zorba, S, additional, Colas, F, additional, Zanda, B, additional, Bouley, S, additional, Jeanne, S, additional, Malgoyre, A, additional, Birlan, M, additional, Blanpain, C, additional, Gattacceca, J, additional, Lecubin, J, additional, Marmo, C, additional, Rault, J L, additional, Vaubaillon, J, additional, Vernazza, P, additional, Affaticati, F, additional, Albani, M, additional, Andreis, A, additional, Ascione, G, additional, Avoscan, T, additional, Bacci, P, additional, Baldini, R, additional, Balestrero, A, additional, Basso, S, additional, Bellitto, R, additional, Belluso, M, additional, Benna, C, additional, Bernardi, F, additional, Bertaina, M E, additional, Betti, L, additional, Bonino, R, additional, Boros, K, additional, Bussi, A, additional, Carli, C, additional, Carriero, T, additional, Cascone, E, additional, Cattaneo, C, additional, Cellino, A, additional, Colombetti, P, additional, Colombi, E, additional, Costa, M, additional, Cremonese, G, additional, Cricchio, D, additional, D’Agostino, G, additional, D’Elia, M, additional, De Maio, M, additional, Demaria, P, additional, Di Dato, A, additional, Di Luca, R, additional, Federici, F, additional, Gagliarducci, V, additional, Gerardi, A, additional, Giuli, G, additional, Guidetti, D, additional, Interrante, G, additional, Lazzarin, M, additional, Lera, S, additional, Leto, G, additional, Licchelli, D, additional, Lippolis, F, additional, Manca, F, additional, Mancuso, S, additional, Mannucci, F, additional, Masi, R, additional, Masiero, S, additional, Meucci, S, additional, Misiano, A, additional, Moggi Cecchi, V, additional, Molinari, E, additional, Monari, J, additional, Montemaggi, M, additional, Montesarchio, M, additional, Monti, G, additional, Morini, P, additional, Nastasi, A, additional, Pace, E, additional, Pardini, R, additional, Pavone, M, additional, Pegoraro, A, additional, Pietronave, S, additional, Pisanu, T, additional, Pugno, N, additional, Repetti, U, additional, Rigoni, M, additional, Rizzi, N, additional, Romeni, C, additional, Romeo, M, additional, Rubinetti, S, additional, Russo, P, additional, Salvati, F, additional, Selvestrel, D, additional, Serra, R, additional, Simoncelli, C, additional, Smareglia, R, additional, Soldi, M, additional, Stanga, R, additional, Strafella, F, additional, Suvieri, M, additional, Taricco, C, additional, Tigani Sava, G, additional, Tombelli, M, additional, Trivero, P, additional, Umbriaco, G, additional, Vairetti, R, additional, Valente, G, additional, Volpini, P, additional, Zagarella, R, additional, and Zollo, A, additional

Published
2020
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143. CUBES: the Cassegrain U-band Efficient Spectrograph

Author

Evans, Christopher J., Bryant, Julia J., Motohara, Kentaro, Cristiani, S., Alcalá, J. M., Alencar, S. H. P., Balashev, S., Bastian, N., Barbuy, B., Battino, U., Calcines, A., Calderone, G., Cambianica, P., Carini, R., Carter, B., Cassisi, S., Castilho, B., Cescutti, G., Christlieb, N., Cirami, R., Coretti, I., Cooke, R. J., Covino, S., Cremonese, G., Cunha, K., Cupani, G., da Silva, A., De Caprio, V., De Cia, A., Dekker, H., D'Elia, V., de Silva, G., Diaz, M. P., Di Marcantonio, P., D'Auria, D., D'Odorico, V., Fitzsimmons, A., Ernandes, H., Evans, C., Franchini, M., Genoni, M., Gänsicke, B., Giribaldi, R. E., Gneiding, C., Grazian, A., Hansen, C. J., La Forgia, F., Landoni, M., Lazzarin, M., Lunney, D., Maciel, W. J., Marcolino, W., Marconi, M., Migliorini, A., Miller, C., Noterdaeme, P., Opitom, C., Pariani, G., Pilecki, B., Piranomonte, S., Quirrenbach, A., Redaelli, E. M. A., Pereira, C., Randich, S., Rossi, S., Sanchez-Janssen, R., Seifert, W., Smiljanic, R., Snodgrass, C., Stilz, I., Stürmer, J., Vanzella, E., Ventura, P., Verducci, O., Waring, C., Watson, S., Wells, M., Wright, D., Zafar, T., and Zanutta, A.

Published
2022
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144. OSIRIS: The Scientific Camera System Onboard Rosetta

Author

Keller, H. U., primary, Barbieri, C., additional, Lamy, P., additional, Rickman, H., additional, Rodrigo, R., additional, Wenzel, K. -P., additional, Sierks, H., additional, A’Hearn, M. F., additional, Angrilli, F., additional, Angulo, M., additional, Bailey, M. E., additional, Barthol, P., additional, Barucci, M. A., additional, Bertaux, J.-L., additional, Bianchini, G., additional, Boit, J.-L., additional, Brown, V., additional, Burns, J. A., additional, Büttner, I., additional, Castro, J. M., additional, Cremonese, G., additional, Curdt, W., additional, Deppo, V. Da, additional, Debei, S., additional, Cecco, M. De, additional, Dohlen, K., additional, Fornasier, S., additional, Fulle, M., additional, Germerott, D., additional, Gliem, F., additional, Guizzo, G. P., additional, Hviid, S. F., additional, Ip, W.-H., additional, Jorda, L., additional, Koschny, D., additional, Kramm, J. R., additional, Kührt, E., additional, Küppers, M., additional, Lara, L. M., additional, Llebaria, A., additional, López, A., additional, López-Jimenez, A., additional, López-Moreno, J., additional, Meller, R., additional, Michalik, H., additional, Michelena, M. D., additional, Müller, R., additional, Naletto, G., additional, Origné, A., additional, Parzianello, G., additional, Pertile, M., additional, Quintana, C., additional, Ragazzoni, R., additional, Ramous, P., additional, Reiche, K.-U., additional, Reina, M., additional, Rodríguez, J., additional, Rousset, G., additional, Sabau, L., additional, Sanz, A., additional, Sivan, J.-P., additional, Stöckner, K., additional, Tabero, J., additional, Telljohann, U., additional, Thomas, N., additional, Timon, V., additional, Tomasch, G., additional, and Wittrock, T., additional

Published
2009
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149. Dust Environment Model of the Interstellar Comet 2I/Borisov

Author

Cremonese, G., primary, Fulle, M., additional, Cambianica, P., additional, Munaretto, G., additional, Capria, M. T., additional, Forgia, F. La, additional, Lazzarin, M., additional, Migliorini, A., additional, Boschin, W., additional, Milani, G., additional, Aletti, A., additional, Arlic, G., additional, Bacci, P., additional, Bacci, R., additional, Bryssinck, E., additional, Carosati, D., additional, Castellano, D., additional, Buzzi, L., additional, Rubbo, S. Di, additional, Facchini, M., additional, Guido, E., additional, Kugel, F., additional, Ligustri, R., additional, Maestripieri, M., additional, Mantero, A., additional, Nicolas, J., additional, Ochner, P., additional, Perrella, C., additional, Trabatti, R., additional, and Valvasori, A., additional

Published
2020
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150. Time evolution of dust deposits in the Hapi region of comet 67P/Churyumov-Gerasimenko

Author

Cambianica, P., primary, Fulle, M., additional, Cremonese, G., additional, Simioni, E., additional, Naletto, G., additional, Massironi, M., additional, Penasa, L., additional, Lucchetti, A., additional, Pajola, M., additional, Bertini, I., additional, Bodewits, D., additional, Ceccarelli, C., additional, Ferri, F., additional, Fornasier, S., additional, Frattin, E., additional, Güttler, C., additional, Gutiérrez, P. J., additional, Keller, H. U., additional, Kührt, E., additional, Küppers, M., additional, La Forgia, F., additional, Lazzarin, M., additional, Marzari, F., additional, Mottola, S., additional, Sierks, H., additional, Toth, I., additional, Tubiana, C., additional, and Vincent, J.-B., additional

Published
2020
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