Shape modeling technique KOALA validated by ESA Rosetta at (21) Lutetia

Planetary and Space Science

Volumn 66, Issue 1, 2012, Pages 200-212

  Carry, B ^a   Kaasalainen, M ^b   Merline, W J ^c   Muller T G ^d   Jorda, L ^e   Drummond, J D ^f   Berthier, J ^g   O'Rourke, L ^a   Urech, J ^h   Kuppers M ^a   Conrad, A ⁱ   Tamblyn, P ^c   Dumas, C ^j   Sierks, H ^k  

^a EUROPEAN SPACE AGENCY   (Spain)

^b TAMPERE UNIVERSITY OF TECHNOLOGY   (Finland)

^c SOUTHWEST RESEARCH INSTITUTE   (United States)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e AIX MARSEILLE UNIVERSITÉ   (France)

^f AIR FORCE RESEARCH LABORATORY   (United States)

^g Institut de Mecanique Celeste et de Calcul des ephemerides   (France)

^h CHARLES UNIVERSITY   (Czech Republic)

ⁱ MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^j EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^k MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

more..

Author keywords

(21) Lutetia; Asteroid; Disk resolved imaging; KOALA; Rosetta

Indexed keywords

ADAPTIVE OPTICS; ASTEROIDS; EARTH (PLANET); GRAVITATION; PHYSICAL PROPERTIES; SOLAR RADIATION; SPACE RESEARCH; TEMPERATURE MEASUREMENT;

GROUND-BASED OBSERVATIONS; HIGH SPATIAL RESOLUTION IMAGES; KOALA; LUTETIA; NON-GRAVITATIONAL FORCE; RADIOMETRIC TECHNIQUES; ROSETTA; THERMAL INFRARED DATA;

INTERPLANETARY FLIGHT;

EID: 84861189510     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pss.2011.12.018     Document Type: Article

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