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EPSC2015-691, 2015 European Planetary Science Congress 2015 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2015

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EPSC2015-691, 2015 European Planetary Science Congress 2015 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2015 EPSC Abstracts Vol. 10, EPSC2015-691, 2015 European Planetary Science Congress 2015 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2015 A Survey for Extreme Shape Hilda Asteroids P. Lacerda (1), V. Ali-Lagoa (2), J. Licandro (2), N. Peixinho (3) (1) Max Planck Institute for Solar System Research, Göttingen, Germany; ([email protected]) (2) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain; (3) Unidad de Astronomía, Fac. de Ciencias Básicas, Universidad de Antofagasta, Antofagasta, Chile Abstract ●● ● ●● ●● H13 ●●●●●● ●●● ● ● ● ●●● H12 We will present results of a survey of Hilda asteroids ●● ●● ● ●●● ● H11 to look for extreme shape objects. We used WISE ●●●●● ● ● ● H10 [1, 2] sparse IR photometry to identify objects with ●● ● ●● ● ● H09 high photometric variability in different bands. Highly Extreme ●●●● ●● ● ● H08 variable candidates were targeted by densely sampled, Variability ● ●● ● ● ● ● ● H07 Hildas follow-up ground-based photometry. ●● ●● ●● ● H06 Similar strategies were successfully used to iden- ●●●●● ●●●● ● H05 ● ●● ● ● ●●● ● ● ● H04 tify extreme shape objects among Jovian Trojans [3] ● ●● ● ● ● ● ● ● ● H03 (see Fig. 1) and Kuiper belt objects [4]. These surveys ●●●● ● ●●●● ● ●● ● ● H02 found high intrinsic abundances of highly variable ob- ●● ● ● ● ● ● ● ● ●● H01 Trojan jects in both population and led to the discovery of ■ ■ ■■■ Trojan 29314 contact binaries. Contact Binaries ■■ ■ ■ Trojan 17365 Contact binaries and extreme shape objects are use- -0.5 0.0 0.5 1.0 ful as they permit useful bulk density estimates [5, 6] Relative photometric variability which in the long run can be used to, e.g., trace dif- from sparse measurements ferences in the bulk composition of different popula- tions. Repeated variability observations of candidate Figure 1: WISE sparse photometry of highly vari- contact binaries among Hilda asteroids will be used to able Hilda asteroids (red circles; each row represents measure their obliquity, which may shed light on how a Hilda asteroid, labeled H01-H13, and show relative these objects formed [7]. photometry along the x-axis). Also shown is similar sparse photometry from [3] (black squares) that led to the discovery of Trojan contact binaries 29314 and Acknowledgements 17365. P. L. wishes to thank the Royal Society for support in [6] Lacerda, P., McNeill, A. & Peixinho, N. 2014, MNRAS, the form of a Newton Fellowship. 437, 3824 [7] Lacerda, P. 2011, Astron. J., 142, 90 References [1] Wright, E. L., et al. 2010, Astron. J., 140, 1868 [2] Mainzer, A., et al. 2011, Astroph. J., 731, 53 [3] Mann, R. K., Jewitt, D. & Lacerda, P. 2007, Astron. J., 134, 1133 [4] Sheppard, S. S. & Jewitt, D. C. 2004, Astron. J., 127, 3023 [5] Lacerda, P. & Jewitt, D. C. 2007, Astron. J., 133, 1393.
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