2012
DOI: 10.1051/0004-6361/201118408
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Determination of binary asteroid orbits with a genetic-based algorithm

Abstract: Aims. Over the past decade, discoveries of multiple and binary asteroid systems have played a significant role in our general understanding of small solar system bodies. Direct observations of satellites of asteroids are rare and difficult since they require the use of already over-subscribed facilities such as adaptive optics (AO) on large 8−10 m class telescopes and the Hubble Space Telescope (HST). The scarcity of data and the long temporal baseline of observations (up to 10 years) significantly complicate … Show more

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Cited by 52 publications
(63 citation statements)
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“…(a) Sheppard et al (2012) only assumed a possible density to derive a size and albedo, none of these values were computed. (b) Two orbital solutions were suggested by Vachier et al (2012), and two different density estimates were derived depending on the orbital solution. Table A.5.…”
Section: Discussionmentioning
confidence: 99%
“…(a) Sheppard et al (2012) only assumed a possible density to derive a size and albedo, none of these values were computed. (b) Two orbital solutions were suggested by Vachier et al (2012), and two different density estimates were derived depending on the orbital solution. Table A.5.…”
Section: Discussionmentioning
confidence: 99%
“…The mass of the Quaoar/Weywot system was first determined to be of 1.6 ± 0.3 × 10 21 kg, and 1.65 ± 0.16 × 10 21 kg, by and Vachier et al (2012), respectively. Recently, Quaoar mass has been determined to be 1.4 ± 0.1 × 10 21 kg from Fraser et al (2013).…”
Section: Classical (50000) Quaoarmentioning
confidence: 99%
“…We classify Isberga as an S-or Sq-type asteroid (in the classification scheme by DeMeo et al 2009), the main class in the inner part of the asteroid belt Carry 2013, 2014). We also use M4AST to determine the degree of space weathering presented by Isberga's surface, following the space weathering model by Brunetto et al (2006), valid for pyroxenes and olivines (see, e.g., Brunetto et al 2007;Vernazza et al 2009;Fulvio et al 2012). In this model, the effect of space weathering is a multiplicative exponential continuum written as Ke (C S /λ) .…”
Section: Surface Compositionmentioning
confidence: 99%