Affiliation:
1. Faculty of Science, Technology, Engineering & Mathematics, School of Physical Sciences, Walton Hall, Open University, Milton Keynes MK7 6AA, UK
Abstract
Colin Pillinger was a larger-than-life planetary scientist with an infectious enthusiasm for science. He was a founding member of the Planetary and Space Sciences Research Institute at the Open University in Milton Keynes. He was a mass spectroscopist who applied these techniques with great success to the study of extraterrestrial rock samples from both meteorites and the Moon. He helped identify a class of meteorite found on Earth that originated from Mars. In turn, this led to leadership of the Beagle 2 Mars lander project, which was designed to take scientific instruments to Mars in order to search for evidence of past life. Against all odds, the landing on Mars was successful, but communication with the lander was never established. Colin was a brilliant innovator, both in his science and in adopting a somewhat unconventional approach to funding the ambitious Beagle 2 project. He enjoyed the fact that, even though it was possible to purchase off-the-shelf instrumentation, the truly creative aspect of his analytic method was in the details of how it was applied, for which the rule book was still being written. Throughout his career he continued to ride the wave of new developments and was always keen to push the limits. He was a brilliant communicator, always full of engaging enthusiasm.
Reference82 articles.
1. Identification of the Beagle 2 lander on Mars
2. Effects of darkening processes on surfaces of airless bodies
3. Gancet J. et al. 2019 Lunar Volatiles Mobile Instrumentation (LUVMI) Project results. In Proc. 70th Int. Astronautical Congress (IAC) 21–25 October 2019 Washington DC USA. Copyright ©2019 by the International Astronautical Federation (IAF). All rights reserved. IAC-19-A3.2C.6.
4. Mossbauer spectroscopy of Apollo 11 samples;Housley R. M.;Proc. Apollo 11 Lunar Sci. Conf., Houston, Texas, 5–8 January 1970,1970
5. Isotopic Composition of Nitrogen: Implications for the Past History of Mars' Atmosphere