Laboratory study of the bidirectional reflectance of powdered surfaces: On the asymmetry parameter of asteroid photometric data

被引:36
作者
Kamei, A [1 ]
Nakamura, AM [1 ]
机构
[1] Kobe Univ, Grad Sch Sci & Technol, Nada Ku, Kobe, Hyogo 6578501, Japan
关键词
photometry; regoliths; surfaces; asteroids;
D O I
10.1006/icar.2002.6818
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We performed laboratory experiments on the bidirectional reflectance of powdered surfaces of dunite, graphite, and Allende (CV3) and Gao (H5) meteorites. The particle size of each sample varied from tens to hundreds of micrometers. The absolute bidirectional reflectance was determined for two ranges of phase angle: from 2degrees to 80degrees at 0degrees angle of incidence and from 2degrees to 155degrees at 75degrees angle of incidence. The phase angle was incremented every 1degrees in between 2degrees and 5degrees and every 10degrees between 10degrees and 150degrees. We determined the Hapke parameters and found that the values of the asymmetry parameter retrieved for most of the samples were positive when the coverage of the phase angle was wide, 2degrees to 155degrees, although the values derived from remote sensing instruments on asteroid flyby missions have been negative or nearly zero. Among our sample surfaces, only those of graphite, Allende, and Gao, with particle sizes of hundreds micrometers show negative or nearly zero values. The single-scattering albedos determined for the Gao samples are comparable to the values of S-class asteroids, while those for the Allende samples are much larger than those of C-class asteroids. (C) 2002 Elsevier Science (USA).
引用
收藏
页码:551 / 561
页数:11
相关论文
共 21 条
[1]   NEAR photometry of asteroid 253 Mathilde [J].
Clark, BE ;
Veverka, J ;
Helfenstein, P ;
Thomas, PC ;
Bell, JF ;
Harch, A ;
Robinson, MS ;
Murchie, SL ;
McFadden, LA ;
Chapman, CR .
ICARUS, 1999, 140 (01) :53-65
[2]   LIMB DARKENING OF METEORITES AND ASTEROIDS [J].
FRENCH, LM ;
VEVERKA, J .
ICARUS, 1983, 54 (01) :38-47
[4]  
Hapke B., 1993, THEORY REFLECTANCE E
[5]   PHASE-RELATIONS OF HIGH ALBEDO ASTEROIDS - THE UNUSUAL OPPOSITION BRIGHTENING OF 44-NYSA AND 64-ANGELINA [J].
HARRIS, AW ;
YOUNG, JW ;
CONTREIRAS, L ;
DOCKWEILER, T ;
BELKORA, L ;
SALO, H ;
HARRIS, WD ;
BOWELL, E ;
POUTANEN, M ;
BINZEL, RP ;
THOLEN, DJ ;
WANG, SC .
ICARUS, 1989, 81 (02) :365-374
[6]   Scattering of light by individual particles and the implications for models of planetary surfaces [J].
Hartman, B ;
Domingue, D .
ICARUS, 1998, 131 (02) :421-448
[7]   Submillimeter-scale topography of the lunar regolith [J].
Helfenstein, P ;
Shepard, MK .
ICARUS, 1999, 141 (01) :107-131
[8]   The lunar opposition effect: A test of alternative models [J].
Helfenstein, P ;
Veverka, J ;
Hillier, J .
ICARUS, 1997, 128 (01) :2-14
[9]   Galileo photometry of asteroid 243 Ida [J].
Helfenstein, P ;
Veverka, J ;
Thomas, PC ;
Simonelli, DP ;
Klaasen, K ;
Johnson, TV ;
Fanale, F ;
Granahan, J ;
McEwen, AS ;
Belton, M ;
Chapman, C .
ICARUS, 1996, 120 (01) :48-65
[10]   GALILEO PHOTOMETRY OF ASTEROID 951-GASPRA [J].
HELFENSTEIN, P ;
VEVERKA, J ;
THOMAS, PC ;
SIMONELLI, DP ;
LEE, P ;
KLAASEN, K ;
JOHNSON, TV ;
BRENEMAN, H ;
HEAD, JW ;
MURCHIE, S ;
FANALE, F ;
ROBINSON, M ;
CLARK, B ;
GRANAHAN, J ;
GARBEIL, H ;
MCEWEN, AS ;
KIRK, RL ;
DAVIES, M ;
NEUKUM, G ;
MOTTOLA, S ;
WAGNER, R ;
BELTON, M ;
CHAPMAN, C ;
PILCHER, C .
ICARUS, 1994, 107 (01) :37-60