Luke Jerram's Mars

26 July 2021, 12.00 AM - 1 August 2021, 12.00 AM

Wills Memorial Building

The School of Earth Sciences supports Luke Jerram's 'Mars' exhibition at the University of Bristol (26 July to Friday 30 July) by showcasing some of its fabulous scientists who study Mars and other planetary systems. Find out more below.

The exhibition is open to the public 31st July and 1st August. Book a place via eventbrite.

Dr Anna Horleston 

Anna is a planetary seismologist and currently works on the NASA Insight Mission. InSight is a Mars Lander that launched on May 5th 2018 and arrived on Mars on November 26th 2018. It deployed a seismic station on the surface of Mars, containing both broadband and short period sensors. The mission is looking for tectonic and impact events and aims to determine the structure of Mars and improve our understanding of planetary formation. Anna is currently co-lead of the MarsQuake Service and spend my days analysing the data that is retruned each day and helping produce and manage the catalogue of marsquakes. More about Anna, her research, and passion for science communication and talking space with the public or in schools can be found here.

Dr Jessica Irving

Dr Bob Myhill

Dr Nick Teanby 

Nick researches the application of geophysical techniques to solve planetary science problems. He says: "Sometimes you just have to go with the exploration and see where it takes you. If we could predict everything beforehand it would be a lot less fun." Nick studies the atmospheres of Titan, Saturn, Jupiter, Uranus, Neptune, and Mars using both space-based and ground-based instruments such as Cassini, ExoMars Trace Gas Orbiter, the Atacama Large Millimeter/sub-millimeter Array, and Herschel. Like Anna, Nick also supports the NASA's InSight mission to Mars. Nick's honest summary of how he became a planetary scientist, is journey and his passion is worth a read forand you can find out about his research projects and publications: here.

Dr Melody Silvestre

Melody studies the atmosphere of Titan, Saturn's biggest moon. Titan's atmosphere has unique characteristics in the Solar System. It is the only atmosphere detected around a moon. It also the only place where a cycle analogous to Earth's water cycle has been observed: evaporation from Titan's methane seas forms methane clouds, which gives birth to methane rains which form methane rivers which go back into the methane seas. Titan's atmosphere also features a very complex chemistry. As the different gases react further together, they form more and more complex organics and eventually solid particles in suspension in the atmosphere, known as hazes. These hazes are responsible for the nearly uniform yellow/orange appearance of Titan. More about Melody's work: here.

Dr Tim Tompkinson

Tim studies the extraterrestrial formation of alteration minerals within Martian meteorites. These hydrous mineral assemblages provide an opportunity to gain key insights into the past Martian fluid reservoirs (hydrosphere) and the ancient atmosphere of Mars. He builds on previous investigations by employing a new radioisotopic dating program and geochemical characterization. More about his projects and publications: here.

Dr James Wookey

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