A new non-convex model of the binary asteroid (809) Lundia obtained with the SAGE modelling technique

Bartczak, P.; Kryszczyńska, A.; Dudziński, G.; Polińska, M.; Colas, F.; Vachier, F.; Marciniak, A.; Pollock, J.; Apostolovska, G.; Santana-Ros, T.; Hirsch, R.; Dimitrow, W.; Murawiecka, M.; Wietrzycka, P.; Nadolny, J.
Referencia bibliográfica

Monthly Notices of the Royal Astronomical Society, Volume 471, Issue 1, p.941-947

Fecha de publicación:
10
2017
Número de autores
15
Número de autores del IAC
1
Número de citas
4
Número de citas referidas
2
Descripción
We present a new non-convex model of the binary asteroid (809) Lundia. A SAGE (Shaping Asteroids with Genetic Evolution) method using disc-integrated photometry only was used for deriving physical parameters of this binary system. The model of (809) Lundia improves former system's pole solution and gives the ecliptic coordinates of the orbit pole - λ = 122°, β = 22°, σ = ±5° - and the orbital period of 15.415 74 ± 0.000 01 h. For scaling our results, we used an effective diameter (Deff) of 9.6 ± 1.1 km obtained from Spitzer observations. The non-convex shape description of the components permitted a refined calculation of the components' volumes, leading to a density estimation of 2.5 ± 0.2 g cm-3 and a macroporosity of 13-23 per cent. The intermediate-scale features of the model may also offer new clues on the components' origin and evolution.