Physical properties of the ESA Rosetta target asteroid (21) Lutetia II. shape and flyby geometry

Astronomy and Astrophysics

Volumn 523, Issue 5, 2010, Pages

  Carry, B ^a,b   Kaasalainen, M ^c   Leyrat, C ^a   Merline, W J ^d   Drummond, J D ^e   Conrad, A ^f   Weaver, H A ^g   Tamblyn, P M ^d   Chapman, C R ^d   Dumas, C ^h   Colas, F ⁱ   Christou, J C ^j   Dotto, E ^k   Perna, D ^a,k,l   Fornasier, S ^a,b   Bernasconi, L ^m   Behrend, R ⁿ   Vachier, F ⁱ   Kryszczynska, A ^o   Polinska, M ^o   Fulchignoni, M ^a,b   Roy, R ^p   Naves, R ^q   Poncy, R ^r   Wiggins, P ^s   more..

^a OBSERVATOIRE DE PARIS   (France)

^b UNIVERSITÉ PARIS DESCARTES   (France)

^c TAMPERE UNIVERSITY OF TECHNOLOGY   (Finland)

^d SOUTHWEST RESEARCH INSTITUTE   (United States)

^e AIR FORCE RESEARCH LABORATORY   (United States)

^f W M KECK OBSERVATORY   (United States)

^g JOHNS HOPKINS UNIVERSITY APPLIED PHYSICS LABORATORY   (United States)

^h EUROPEAN SOUTHERN OBSERVATORY   (Chile)

ⁱ Institut de Mecanique Celeste et de Calcul des ephemerides   (France)

^j GEMINI OBSERVATORY   (United States)

^k INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^l UNIVERSITY OF ROME TOR VERGATA   (Italy)

^m Les Engarouines Observatory   (France)

ⁿ UNIVERSITÉ DE GENÈVE   (Switzerland)

^o ADAM MICKIEWICZ UNIVERSITY   (Poland)

^p Blauvac Observatory   (France)

^q Observatorio Montcabre   (Spain)

^r Le Cres Observatory   (France)

^s Wiggins Observatory   (United States)

more..

Author keywords

asteroids: individual: (21) Lutetia; instrumentation: adaptive optics; methods: observational; minor planets; techniques: high angular resolution

Indexed keywords

INSTRUMENTATION: ADAPTIVE OPTICS; LUTETIA; METHODS:OBSERVATIONAL; MINOR PLANETS; TECHNIQUES: HIGH ANGULAR RESOLUTIONS;

INSTRUMENTS; PHYSICAL PROPERTIES; PLANETS; POLES; SPIN DYNAMICS;

ASTEROIDS;

EID: 78549271137     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015074     Document Type: Article

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