Asteroid phase curves from ATLAS dual-band photometry
نویسندگان
چکیده
Asteroid phase curves are used to derive fundamental physical properties through the determination of absolute magnitude H. The upcoming visible Legacy Survey Space and Time (LSST) mid-infrared Near-Earth Object Surveillance Mission (NEOSM) surveys rely on these magnitudes colours albedos millions asteroids. Furthermore, shape reflects their surface compositions, allowing for conclusions taxonomy. We asteroid from dual-band photometry acquired by Terrestrial-impact Last Alert System telescopes. Using Bayesian parameter inference, we retrieve slope parameters 127,012 94,777 asteroids in photometric $H, G_1, G_2$- G^*_{12}$-systems. taxonomic complexes separate observed $G_1, G_2$-distributions, correlating with mean visual albedo. This allows differentiating X-complex into P-, M-, E-complexes using as alternative albedo measurements. Further, misclassifications spectrophotometric datasets well interlopers dynamical families reveal themselves G_2$-space. G^*_{12}$-model applied serendipitous observations is unable resolve target G_2$ coefficients show wavelength-dependency majority complexes. Serendipitous allow reliable curve a large number To ensure that suited colour computations, it imperative future densely cover opposition effects curves, minimizing uncertainty offer an accessible dimension classification.
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ژورنال
عنوان ژورنال: Icarus
سال: 2021
ISSN: ['0019-1035', '1090-2643']
DOI: https://doi.org/10.1016/j.icarus.2020.114094