CASTAway: An asteroid main belt tour and survey.

Advances in Space Research Elsevier 62:8 (2017) 1998-2025

Authors:

Neil E Bowles, C Snodgrass, JP Sanchez, Jessica A Arnold, P Eccleston, T Andert, A Probst, G Naletto, AC Vandaele, de de Leon, A Nathues, IR Thomas, N Thomas, L Jorda, V da Deppo, H Haack, SF Green, B Carry, Kerri L Donaldson Hanna, J Leif Jorgensen, A Kereszturi, FE DeMeo, JK Davies, Fraser Clarke, K Kinch, A Guilbert-Lepoutre, J Agarwal, AS Rivkin, P Pravec, S Fornasier, M Gravnik, RH Jones, N Murdoch, KH Joy, Matthias Tecza, Jennifer M Barnes, J Licandro, BT Greenhagen, Simon B Calcutt, Charlotte M Marriner, Tristram J Warren, I Tosh

Abstract:

CASTAway is a mission concept to explore our Solar System’s main asteroid belt. Asteroids and comets provide a window into the formation and evolution of our Solar System and the composition of these objects can be inferred from space-based remote sensing using spectroscopic techniques. Variations in composition across the asteroid populations provide a tracer for the dynamical evolution of the Solar System. The mission combines a long-range (point source) telescopic survey of over 10,000 objects, targeted close encounters with 10 – 20 asteroids and serendipitous searches to constrain the distribution of smaller (e.g. 10 m) size objects into a single concept. With a carefully targeted trajectory that loops through the asteroid belt, CASTAway would provide a comprehensive survey of the main belt at multiple scales. The scientific payload comprises a 50 cm diameter telescope that includes an integrated low-resolution (R = 30 – 100) spectrometer and visible context imager, a thermal (e.g. 6 – 16 μm) imager for use during the flybys, and modified star tracker cameras to detect small (~10 m) asteroids. The CASTAway spacecraft and payload have high levels of technology readiness and are designed to fit within the programmatic and cost caps for a European Space Agency medium class mission, whilst delivering a significant increase in knowledge of our Solar System.

New constraints on Ganymede's hydrogen corona: Analysis of Lyman- α emissions observed by HST/STIS between 1998 and 2014

Planetary and Space Science 148 (2017) C

Authors:

J Alday, L Roth, N Ivchenko, KD Retherford, TM Becker, P Molyneux, J Saur

Was Planet 9 captured in the Sun’s natal star-forming region?

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 472:1 (2017) L75-L79

Authors:

Richard J Parker, Tim Lichtenberg, Sascha P Quanz

Comparison of the GOSAT TANSO-FTS TIR CH4 volume mixing ratio vertical profiles with those measured by ACE-FTS, ESA MIPAS, IMK-IAA MIPAS, and 16 NDACC stations

Atmospheric Measurement Techniques Copernicus Publications 10:10 (2017) 3697-3718

Authors:

Kevin S Olsen, Kimberly Strong, Kaley A Walker, Chris D Boone, Piera Raspollini, Johannes Plieninger, Whitney Bader, Stephanie Conway, Michel Grutter, James W Hannigan, Frank Hase, Nicholas Jones, Martine de Mazière, Justus Notholt, Matthias Schneider, Dan Smale, Ralf Sussmann, Naoko Saitoh

Seismic Coupling of Short-Period Wind Noise Through Mars' Regolith for NASA's InSight Lander

SPACE SCIENCE REVIEWS 211:1-4 (2017) 485-500

Authors:

NA Teanby, J Stevanovic, J Wookey, N Murdoch, J Hurley, R Myhill, NE Bowles, SB Calcutt, WT Pike