The formation and evolution of Titan's winter polar vortex.

Nature communications 8:1 (2017) 1586-1586

Authors:

NA Teanby, B Bézard, S Vinatier, M Sylvestre, CA Nixon, PGJ Irwin, RJ de Kok, SB Calcutt, FM Flasar

Abstract:

Saturn's largest moon Titan has a substantial nitrogen-methane atmosphere, with strong seasonal effects, including formation of winter polar vortices. Following Titan's 2009 northern spring equinox, peak solar heating moved to the northern hemisphere, initiating south-polar subsidence and winter polar vortex formation. Throughout 2010-2011, strengthening subsidence produced a mesospheric hot-spot and caused extreme enrichment of photochemically produced trace gases. However, in 2012 unexpected and rapid mesospheric cooling was observed. Here we show extreme trace gas enrichment within the polar vortex dramatically increases mesospheric long-wave radiative cooling efficiency, causing unusually cold temperatures 2-6 years post-equinox. The long time-frame to reach a stable vortex configuration results from the high infrared opacity of Titan's trace gases and the relatively long atmospheric radiative time constant. Winter polar hot-spots have been observed on other planets, but detection of post-equinox cooling is so far unique to Titan.

Ammonia in Jupiter's Troposphere From High-Resolution 5 mu m Spectroscopy

GEOPHYSICAL RESEARCH LETTERS 44:21 (2017) 10838-10844

Authors:

RS Giles, LN Fletcher, PGJ Irwin, GS Orton, JA Sinclair

Linking the climate and thermal phase curve of 55 Cancri e

The Astrophysical Journal: an international review of astronomy and astronomical physics American Astronomical Society (2017)

Authors:

M Hammond, RT Pierrehumbert

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.

The formation and evolution of Titan's winter polar vortex.

Nature Communications Nature Publishing Group 8:1 (2017) 1586

Authors:

NA Teanby, B Bézard, S Vinatier, M Sylvestre, CA Nixon, Patrick GJ Irwin, RJ de Kok, Simon B Calcutt, FM Flasar

Abstract:

Saturn's largest moon Titan has a substantial nitrogen-methane atmosphere, with strong seasonal effects, including formation of winter polar vortices. Following Titan's 2009 northern spring equinox, peak solar heating moved to the northern hemisphere, initiating south-polar subsidence and winter polar vortex formation. Throughout 2010-2011, strengthening subsidence produced a mesospheric hot-spot and caused extreme enrichment of photochemically produced trace gases. However, in 2012 unexpected and rapid mesospheric cooling was observed. Here we show extreme trace gas enrichment within the polar vortex dramatically increases mesospheric long-wave radiative cooling efficiency, causing unusually cold temperatures 2-6 years post-equinox. The long time-frame to reach a stable vortex configuration results from the high infrared opacity of Titan's trace gases and the relatively long atmospheric radiative time constant. Winter polar hot-spots have been observed on other planets, but detection of post-equinox cooling is so far unique to Titan.