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91̽»¨
Juno Jupiter image

Simon Calcutt

Emeritus

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary atmosphere observation analysis
  • Solar system
  • Space instrumentation
  • Planetary surfaces
simon.calcutt@physics.ox.ac.uk
Telephone: 01865 (2)72916
Atmospheric Physics Clarendon Laboratory, room 308
  • About
  • Publications

The formation and evolution of Titan’s winter polar vortex

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

Authors:

Nicholas A Teanby, Bruno Bézard, Sandrine Vinatier, Melody Sylvestre, Conor A Nixon, Patrick GJ Irwin, Remco J de Kok, Simon B Calcutt, F Michael 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.

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.

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

The DREAMS experiment flown on the ExoMars 2016 mission for the study of Martian environment during the dust storm season

2017 IEEE International Workshop on Metrology for AeroSpace (MetroAeroSpace) IEEE (2017) 249-255

Authors:

C Bettanini, F Esposito, S Debei, C Molfese, A Aboudan, GP Guizzo, E Friso, V Mennella, R Molinaro, S Silvestro, R Mugnuolo, A-M Harri, F Montmessin, Colin Wilson, I Arruego Rodriguez, S Abbaki, V Apestigue, G Bellucci, J-J Berthelier, O Karatekin, G Landis, R Lorenz, J Martinez, D Moehlmann

Abstract:

The DREAMS (Dust characterization, Risk assessment and Environment Analyser on the Martian Surface) experiment on Schiaparelli lander of ExoMars 2016 mission was an autonomous meteorological station designed to completely characterize the Martian atmosphere on surface, acquiring data not only on temperature, pressure, humidity, wind speed and direction, but also on solar irradiance, dust opacity and atmospheric electrification, to measure for the first time key parameters linked to hazard conditions for future manned explorations. Although with very limited mass and energy resources, DREAMS would be able to operate autonomously for at least two Martian days (sols) after landing in a very harsh environment as it was supposed to land on Mars during the dust storm season (October 2016 in Meridiani Planum) relying on its own power supply. ExoMars mission was successfully launched on 14th March 2016 and Schiaparelli entered the Mars atmosphere on October 20th beginning its `six minutes of terror' journey to the surface. Unfortunately, some unexpected behavior during the parachuted descent caused an unrecoverable critical condition in navigation system of the lander driving to a destructive crash on the surface. The adverse sequence of events at 4 km altitude triggered the transition of the lander in surface operative mode, commanding switch on the DREAMS instrument, which was therefore able to correctly power on and send back housekeeping data. This proved the nominal performance of all DREAMS hardware before touchdown demonstrating the highest TRL of the unit for future missions. This paper describes this experiment in terms of scientific goals, design, performances, testing and operational capabilities with an overview of in flight performances and available mission data.

Composite infrared spectrometer (CIRS) on Cassini: publisher's note.

Applied Optics Optica Publishing Group 56:21 (2017) 5897

Authors:

DE Jennings, FM Flasar, VG Kunde, CA Nixon, ME Segura, PN Romani, N Gorius, S Albright, JC Brasunas, RC Carlson, AA Mamoutkine, E Guandique, MS Kaelberer, S Aslam, RK Achterberg, GL Bjoraker, CM Anderson, V Cottini, JC Pearl, MD Smith, BE Hesman, RD Barney, S Calcutt, TJ Vellacott, LJ Spilker, SG Edgington, SM Brooks, P Ade, PJ Schinder, A Coustenis, R Courtin, G Michel, R Fettig, S Pilorz, C Ferrari

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