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Arridge, C. S., Agnor, C. B., André, N., Baines, K. H., Fletcher, L. N., Gautier, D....Zarka, P. (2012). Uranus Pathfinder: exploring the origins and evolution of Ice Giant planets. Experimental Astronomy. 33 (2-3), 753-791

A. C.S. et al.,  "Uranus Pathfinder: exploring the origins and evolution of Ice Giant planets", in Experimental Astronomy, vol. 33, no. 2-3, pp. 753-791, 2012

@article{c.s.2012_1715137076416,
	author = "Arridge, C. S. and Agnor, C. B. and André, N. and Baines, K. H. and Fletcher, L. N. and Gautier, D. and Hofstadter, M. D. and Jones, G. H. and Lamy, L. and Langevin, Y. and Mousis, O. and Nettelmann, N. and Russell, C. T. and Stallard, T. and Tiscareno, M. S. and Tobie, G. and Bacon, A. and Chaloner, C. and Guest, M. and Kemble, S. and Peacocke, L. and Achilleos, N. and Andert, T. P. and Banfield, D. and Barabash, S. and Barthelemy, M. and Bertucci, C. and Brandt, P. and Cecconi, B. and Chakrabarti, S. and Cheng, A. F. and Christensen, U. and Christou, A. and Coates, A. J. and Collinson, G. and Cooper, J. F. and Courtin, R. and Dougherty, M. K. and Ebert, R. W. and Entradas, M. and Fazakerley, A. N. and Fortney, J. J. and Galand, M. and Gustin, J. and Hedman, M. and Helled, R. and Henri, P. and Hess, S. and Holme, R. and Karatekin, O. and Krupp, N. and Leisner, J. and Martin-Torres, J. and Masters, A. and Melin, H. and Miller, S. and Müller-Wodarg, I. and Noyelles, B. and Paranicas, C. and de Pater, I. and Pätzold, M. and Prangé, R. and Quémerais, E. and Roussos, E. and Rymer, A.M. and Sánchez-Lavega, A. and Saur, J. and Sayanagi, K. M. and Schenk, P. and Schubert, G. and Sergis, N. and Sohl, F. and Sittler Jr., E. C. and Teanby, N. A. and Tellmann, S. and Turtle, E.P. and Vinatier, S. and Wahlund, J.-E. and Zarka, P.",
	title = "Uranus Pathfinder: exploring the origins and evolution of Ice Giant planets",
	journal = "Experimental Astronomy",
	year = "2012",
	volume = "33",
	number = "2-3",
	doi = "10.1007/s10686-011-9251-4",
	pages = "753-791",
	url = "https://link.springer.com/article/10.1007%2Fs10686-011-9251-4"
}

TY  - JOUR
TI  - Uranus Pathfinder: exploring the origins and evolution of Ice Giant planets
T2  - Experimental Astronomy
VL  - 33
IS  - 2-3
AU  - Arridge, C. S.
AU  - Agnor, C. B.
AU  - André, N.
AU  - Baines, K. H.
AU  - Fletcher, L. N.
AU  - Gautier, D.
AU  - Hofstadter, M. D.
AU  - Jones, G. H.
AU  - Lamy, L.
AU  - Langevin, Y.
AU  - Mousis, O.
AU  - Nettelmann, N.
AU  - Russell, C. T.
AU  - Stallard, T.
AU  - Tiscareno, M. S.
AU  - Tobie, G.
AU  - Bacon, A.
AU  - Chaloner, C.
AU  - Guest, M.
AU  - Kemble, S.
AU  - Peacocke, L.
AU  - Achilleos, N.
AU  - Andert, T. P.
AU  - Banfield, D.
AU  - Barabash, S.
AU  - Barthelemy, M.
AU  - Bertucci, C.
AU  - Brandt, P.
AU  - Cecconi, B.
AU  - Chakrabarti, S.
AU  - Cheng, A. F.
AU  - Christensen, U.
AU  - Christou, A.
AU  - Coates, A. J.
AU  - Collinson, G.
AU  - Cooper, J. F.
AU  - Courtin, R.
AU  - Dougherty, M. K.
AU  - Ebert, R. W.
AU  - Entradas, M.
AU  - Fazakerley, A. N.
AU  - Fortney, J. J.
AU  - Galand, M.
AU  - Gustin, J.
AU  - Hedman, M.
AU  - Helled, R.
AU  - Henri, P.
AU  - Hess, S.
AU  - Holme, R.
AU  - Karatekin, O.
AU  - Krupp, N.
AU  - Leisner, J.
AU  - Martin-Torres, J.
AU  - Masters, A.
AU  - Melin, H.
AU  - Miller, S.
AU  - Müller-Wodarg, I.
AU  - Noyelles, B.
AU  - Paranicas, C.
AU  - de Pater, I.
AU  - Pätzold, M.
AU  - Prangé, R.
AU  - Quémerais, E.
AU  - Roussos, E.
AU  - Rymer, A.M.
AU  - Sánchez-Lavega, A.
AU  - Saur, J.
AU  - Sayanagi, K. M.
AU  - Schenk, P.
AU  - Schubert, G.
AU  - Sergis, N.
AU  - Sohl, F.
AU  - Sittler Jr., E. C.
AU  - Teanby, N. A.
AU  - Tellmann, S.
AU  - Turtle, E.P.
AU  - Vinatier, S.
AU  - Wahlund, J.-E.
AU  - Zarka, P.
PY  - 2012
SP  - 753-791
SN  - 0922-6435
DO  - 10.1007/s10686-011-9251-4
UR  - https://link.springer.com/article/10.1007%2Fs10686-011-9251-4
AB  - The "Ice Giants" Uranus and Neptune are a different class of planet compared to Jupiter and Saturn. Studying these objects is important for furthering our understanding of the formation and evolution of the planets, and unravelling the fundamental physical and chemical processes in the Solar System. The importance of filling these gaps in our knowledge of the Solar System is particularly acute when trying to apply our understanding to the numerous planetary systems that have been discovered around other stars. The Uranus Pathfinder (UP) mission thus represents the quintessential aspects of the objectives of the European planetary community as expressed in ESA's Cosmic Vision 2015-2025. UP was proposed to the European Space Agency's M3 call for medium-class missions in 2010 and proposed to be the first orbiter of an Ice Giant planet. As the most accessible Ice Giant within the M-class mission envelope Uranus was identified as the mission target. Although not selected for this call the UP mission concept provides a baseline framework for the exploration of Uranus with existing low-cost platforms and underlines the need to develop power sources suitable for the outer Solar System. The UP science case is based around exploring the origins, evolution, and processes at work in Ice Giant planetary systems. Three broad themes were identified: (1) Uranus as an Ice Giant, (2) An Ice Giant planetary system, and (3) An asymmetric magnetosphere. Due to the long interplanetary transfer from Earth to Uranus a significant cruise-phase science theme was also developed. The UP mission concept calls for the use of a Mars Express/Rosetta-type platform to launch on a Soyuz-Fregat in 2021 and entering into an eccentric polar orbit around Uranus in the 2036-2037 timeframe. The science payload has a strong heritage in Europe and beyond and requires no significant technology developments.
ER  -