Browsing by Author "Jones, G. H."

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    The Castalia mission to Main Belt Coment 133P/Elst-Pizarro
    (Elsevier, 2017-09-19) Snodgrass, Colin; Jones, G. H.; Boehnhardt, H.; Gibbings, Alison; Homeister, M.; Andre, N.; Beck, P.; Bentley, M. S.; Bertini, I.; Bowles, Neil E.; Capria, M. T.; Carr, C.; Ceriotti, M.; Coates, A. J.; Della Corte, V.; Donaldson Hanna, Kerri L.; Fitzsimmons, A.; Gutiérrez, P. J.; Hainaut, O. R.; Herique, A.; Hilchenbach, M.; Hsieh, H. H.; Jehin, E.; Karatekin, O.; Kofman, W.; Lara, L. M.; Laudan, K.; Licandro, J.; Lowry, S. C.; Marzari, F.; Masters, A.; Meech, K. J.; Moreno, F.; Morse, A.; Orosei, R.; Pack, A.; Plettemeier, D.; Prialnik, D.; Rotundi, A.; Rubin, M.; Sánchez, Joan-Pau; Sheridan, S.; Trieloff, M.; Winterboer, A.
    We describe Castalia, a proposed mission to rendezvous with a Main Belt Comet (MBC), 133P/Elst-Pizarro. MBCs are a recently discovered population of apparently icy bodies within the main asteroid belt between Mars and Jupiter, which may represent the remnants of the population which supplied the early Earth with water. Castalia will perform the first exploration of this population by characterising 133P in detail, solving the puzzle of the MBC’s activity, and making the first in situ measurements of water in the asteroid belt. In many ways a successor to ESA’s highly successful Rosetta mission, Castalia will allow direct comparison between very different classes of comet, including measuring critical isotope ratios, plasma and dust properties. It will also feature the first radar system to visit a minor body, mapping the ice in the interior. Castalia was proposed, in slightly different versions, to the ESA M4 and M5 calls within the Cosmic Vision programme. We describe the science motivation for the mission, the measurements required to achieve the scientific goals, and the proposed instrument payload and spacecraft to achieve these.
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    Comet interceptor: an ESA mission to a dynamically new solar system object
    (http://www.iafastro.org/events/iac/iac-2020, 2020-10-12) Sánchez, Joan-Pau; Jones, G. H.; Snodgrass, Colin
    While the scientific merits of past comet missions are unquestioned, previously visited comets had all approached the Sun on many occasions and, as a consequence, have also undergone substantial compositional and morphological alterations. Comet Interceptor (Comet-I) was recently selected as ESA’s first fast-track class mission and aims to explore a pristine comet, which will ideally be visiting the inner Solar System for the first time. Comet-I will hitch a ride to a Sun-Earth L2 quasi-halo orbit, as a co-passenger in ESA’s M4 ARIEL’s launch, in 2028. It will then remain there waiting for the right departure conditions to definitively leave the L2 point and intercept a newly discovered comet. Comet-I will be the first mission to be design and, possibly launched, without an identified target. Nevertheless, a Monte Carlo analysis modelling the uncertainties of the long period comet population and the spacecraft transfer capabilities demonstrate the high likelihood of completing the mission within 6 years. A few days before the closest approach Comet-I will release two small independent probes (~30 kg each) into fly-by paths with close approach distances in the order of a few hundred kilometres, while the main spacecraft (~700 kg) will take a safer path (~1000 km) to protect it from the dust environment. Comet-I will thus involve three spacecraft elements working together to ensure a low-risk, bountiful, interdisciplinary scientific return through unprecedented multipoint measurements