Beech, M. (2010). Atmospheric height by twilight’s glow. Journal of the Royal Astronomical Society of Canada, 104, 147–148.Google Scholar

Powell, C. (2014). Did Cosmos pick the wrong hero. Discover Magazine blog.Google Scholar

Tierie, G. (1932). Cornelis Drebbel (1572–1633). Ph.D. Thesis, University of Leiden (available online).Google Scholar

Huygens, C., The Celestial Worlds Discover’d: Or, Conjectures Concerning the Inhabitants, Plants and Productions of the Worlds in the Planets, London: Timothy Childe, 1698.Google Scholar

Wilkins, J., A Discovery of a New World, or A Discourse tending to prove, that ‘tis Probable there may be another Habitable World in the Moon, with a discourse on the probability of a passage thither, London: J. Gillibrand, 1684.Google Scholar

MacDonald, A., The Long Space Age, New Haven, CT: Yale University Press, 2017.10.12987/yale/9780300219326.001.0001CrossRefGoogle Scholar

Sobester, A., Stratospheric Flight: Aeronautics at the Limit, Springer, 2011.10.1007/978-1-4419-9458-5CrossRefGoogle Scholar

Halley, E. (1693). A discourse concerning the proportional heat of the Sun in all latitudes, with the method of collecting the same, as it was read before the Royal Society in one of their Late Meetings. Philosphical Transactions of the Royal Society, 17, 878–885.10.1098/rstl.1693.0061CrossRefGoogle Scholar

Halley, E. (1686). An estimate of the quantity of vapour raised out of the sea by the warmth of the Sun; derived from an experiment shown before the Royal Society, at one of Their Late Meetings. Philosphical Transactions of the Royal Society, 1686–1692, 16, 366–370, doi:10.1098/rstl.1686.0067Google Scholar

Lorenz, R.D. (2014). The flushing of Ligeia: composition variations across Titan’s seas in a simple hydrological model. Geophysical Research Letters, 41, 5764–5770, doi:10.1002/2014GL061133.CrossRefGoogle Scholar

Halley, E. (1714). A short account of the cause of the saltness of the ocean, and of the several lakes that emit no rivers; with a proposal, by help thereof, to discover the age of the World. Philosphical Transactions of the Royal Society, 29, 296–300, doi:10.1098/rstl.1714.0031.CrossRefGoogle Scholar

Halley, E. (1686). An historical account of the trade winds, and monsoons, observable in the seas between and near the tropicks, with an attempt to assign the phisical cause of the said winds. Philosophical Transactions of the Royal Society, 16(179–191), 153–168.10.1098/rstl.1686.0026CrossRefGoogle Scholar

Hadley, G. (1735). VI. Concerning the cause of the general trade-winds. Philosophical Transactions of the Royal Society, 39(437), 58–62.Google Scholar

Persson, A.O. (2006). Hadley’s principle: understanding and misunderstanding the trade winds. History of Meteorology, 3, 17–42.Google Scholar

Dalrymple, G.B. ( 1994). The Age of the Earth, Stanford, CA: Stanford University Press.Google Scholar

Franklin, B. (1755). Letter to Peter Collinson, dated Philadelphia, August 25, 1755, quoted in Lorenz, R.D., Balme, M.R., Gu, Z., et al. (2016), History and Applications of Dust Devil Studies. Space Science Reviews, 203, 5–37.Google Scholar

Jefferson, T. (1787). Notes on the State of Virginia. London: John Stockdale.Google Scholar

Fleming, J.R., Historical Perspectives on Climate Change, New York: Oxford University Press, 1998.10.1093/oso/9780195078701.001.0001CrossRefGoogle Scholar

Thompson, K. (1980). Forests and climate change in America: some early views. Climatic Change, 3, 47–64.10.1007/BF02423168CrossRefGoogle Scholar

Herschel, W. (1801). Observations tending to investigate the nature of the Sun, in order to find the causes or symptoms of its variable emission of light and heat; with remarks on the use that may possibly be drawn from solar observations. Philosophical Transactions of the Royal Society of London, 91, 265–318.Google Scholar

Hoyt, D.V. & Schatten, K.H. (1997). The Role of the Sun in Climate Change, Oxford: Oxford University Press.CrossRefGoogle Scholar

Wulf, A. (2015). The Invention of Nature: The Adventures of Alexander von Humboldt, the Lost Hero of Science. London: John Murray.Google Scholar

Hamblyn, R. (2011). The Invention of Clouds: How an Amateur Meteorologist Forged the Language of the Skies, London: Pan Macmillan.Google Scholar

Burgess, E. (1837). General remarks on the temperature of the terrestrial globe and the planetary spaces by Baron Fourier. American Journal of Science and Arts, 32, 1–20.Google Scholar

Fleming, J.R. (1999). Joseph Fourier, the ‘greenhouse effect’, and the quest for a universal theory of terrestrial temperatures. Endeavour, 23, 72–75.CrossRefGoogle Scholar

Bard, E. (2004). Greenhouse effect and ice ages: historical perspective. Comptes Rendus Geoscience, 336, 603–638.10.1016/j.crte.2004.02.005CrossRefGoogle Scholar

Smyth, C.P. (1856). Note on the constancy of solar radiation. Monthly Notices of the Royal Astronomical Society, 16, 220.10.1093/mnras/16.9.220CrossRefGoogle Scholar

Piazzi-Smyth, C. (1858). Tenerife, An Astronomer’s Experiment: or, Specialities of a Residence above the Clouds, London: Lovell Reeve.Google Scholar

Baddeley, P.F.H. (1860). Whirlwinds and Dust Storms of India, London: Bell.Google Scholar

Lorenz, R.D., Balme, M.R., Gu, Z., et al. (2016). History and Applications of Dust Devil Studies. Space Science Reviews, 203, 5–37.10.1007/s11214-016-0239-2CrossRefGoogle Scholar

Monmonier, M. (1999). Air Apparent: How Meteorologists Learned to Map, Predict and Dramatize Weather, Chicago: University of Chicago Press,10.7208/chicago/9780226222875.001.0001CrossRefGoogle Scholar

Moore, P. (2015). The Weather Experiment, New York: Farrar.Google Scholar

Holmes, R. (2013). Falling Upwards: How We Took to the Air, New York: Pantheon.Google Scholar

Lequex, J. (2009). Early infrared astronomy. Journal of Astronomical History and Heritage, 12(2), 125–140.CrossRefGoogle Scholar

Tyndall, J. (1861). The Bakerian Lecture: On the absorption and radiation of heat by gases and vapours, and on the physical connexion of radiation, absorption, and conduction. Philosophical Transactions of the Royal Society of London, 151, 1–36.10.1098/rstl.1861.0001CrossRefGoogle Scholar

Foote, Eunice (1856). Article XXL – Circumstances affecting the Heat of the Sun’s Rays, read before the American Association, August 23, 1856. The American Journal of Science and Arts, XXII, 382–383.Google Scholar

Ebelmen, J.J. (1847). Recherches sur la décomposition des roches, Paris: Carilian-Goeury et Vor. Dalmont.Google Scholar

Berner, R. (2012). Jacques-Joseph Ébelmen, the founder of earth system science. Comptes Rendus Geoscience, 344(11), 544–548.10.1016/j.crte.2012.08.001CrossRefGoogle Scholar

Galvez, M.E. & Gaillardet, J. (2012). Historical constraints on the origins of the carbon cycle concept. Comptes Rendus Geoscience, 344(11), 549–567.10.1016/j.crte.2012.10.006CrossRefGoogle Scholar

Murray, J. et al. (1885). Report on the Scientific Results of the Voyage of H.M.S. Challenger during the years 1873–1876, London: Her Majesty’s Stationery Office.Google Scholar

Roemmich, D. et al. (2012). 135 years of global ocean warming between the Challenger Expedition and the Argo Programme. Nature Climate Change, 2, 425–428.10.1038/nclimate1461CrossRefGoogle Scholar

Leitch, W. (1867). God’s Glory in the Heavens, London: Alexander Strahan.Google Scholar

Taylor, H.D. (1895). Mars, A negative optical proof of the absence of seas in Mars. Monthly Notices of the Royal Astronomical Society, 55, 462–474.10.1093/mnras/55.8.462CrossRefGoogle Scholar

Poynting, J.H. (1904). Radiation in the Solar System: its effect on temperature and its pressure on small bodies. Philosophical Transactions of the Royal Society of London, Series A, 202, 525–552.10.1098/rsta.1904.0012CrossRefGoogle Scholar

Earl of Rosse (1871). On the Radiation of Heat from the Moon. No. II. Proceedings of the Royal Society of London, 19, 9–14.10.1098/rspl.1870.0004CrossRefGoogle Scholar

Langley, S.P. (1886). The temperature of the Moon. Science, 7(158) 8–9.10.1126/science.ns-7.152.8CrossRefGoogle ScholarPubMed

Langley, S.P. (1889). The Temperature of the Moon, Third Memoir, National Academy of Sciences Vol. 4 part 2.Google Scholar

Langley, S.P. (1884). Researches on Solar Heat and Its Absorption by the Earth’s Atmosphere: A Report of the Mount Whitney Expedition. US Government Printing Office.Google Scholar

Arrhenius, S. (1896). On the influence of carbonic acid in the air upon the temperature of the ground. The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science, 41(251), 237–276.10.1080/14786449608620846CrossRefGoogle Scholar

Mellard Reade, T. (1879). Chemical Denudation in Relation to Geological Time, London: D. Bogue.Google Scholar

Chamberlin, T.C. (1898). The influence of great epochs of limestone formation upon the constitution of the atmosphere. The Journal of Geology, 6(6), 609–621.10.1086/608185CrossRefGoogle Scholar

Fleming, J. R. (2000). TC Chamberlin, climate change, and cosmogony. Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics, 31(3), 293–308.10.1016/S1355-2198(00)00015-0CrossRefGoogle Scholar

Chamberlin, T.C. (1897). A Group of Hypotheses Bearing on Climatic Changes. Journal of Geology, 5, 653–683.10.1086/607921CrossRefGoogle Scholar

Chamberlin, T.C. (1906). On a possible reversal of deep-sea circulation and its influence on geological climates. Journal of Geology, 14, 363–373.10.1086/621315CrossRefGoogle Scholar

Ekholm, N. (1901). On the variations of the climate of the geological and historical past and their causes. Quarterly Journal of the Royal Meteorological Society, 27, 11–62.10.1002/qj.49702711702CrossRefGoogle Scholar

Walker, G.T. (1923). Correlation in seasonal variations of weather. VIII. A preliminary study of world-weather. Memoirs of the Indian Meteorological Department, 24(Part 4), 75–131.Google Scholar

Katz, R.W. (2002). Sir Gilbert Walker and a connection between El Niño and statistics. Statistical Science, 17, 97–112.CrossRefGoogle Scholar

Stoney, G.J. (1898). Of atmospheres upon planets and satellites. The Astrophysical Journal, 7, 25.10.1086/140435CrossRefGoogle Scholar

Hoinka, K.P. (1997). The tropopause: discovery, definition and demarcation. Meteorologische Zeitschrift, N.F., 6, 281–303.10.1127/metz/6/1997/281CrossRefGoogle Scholar

Dines, W. (1908). The Registering Balloon Ascents in England of July 22–27, 1907, Preliminary Account. Quarterly Journal of the Royal Meteorological Society, 34, 1–5.CrossRefGoogle Scholar

Rotch, A.L. (1897). On obtaining meterological records in the upper air by means of kites and balloons. Proceedings of the American Academy of Arts and Sciences, 32, 245–251.CrossRefGoogle Scholar

Goddard, R.H. (1919). A Method of Reaching Extreme Altitudes, Washington, DC: Smithsonian Institution.10.5479/sil.918318.39088014683783CrossRefGoogle Scholar

Sheehan, W. (1996). The Planet Mars, A History of Observation and Discovery, Tucson, AZ: University of Arizona Press.Google Scholar

Lorenz, R.D. (1997). Did Comas Sola discover Titan’s atmosphere? Astronomy and Geophysics, 38(3) 16–18.CrossRefGoogle Scholar

Lowell, P. (1907). A general method for evaluating the surface-temperature of the planets: with special reference to the temperature of Mars. The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science, 14(79), 161–176.10.1080/14786440709463668CrossRefGoogle Scholar

Poynting, J. (1907). On Prof. Lowell’s method for evaluating the surface-temperatures of the planets; with an attempt to represent the effect of day and night on the temperature of the Earth. The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science, 14(84), 749–760.CrossRefGoogle Scholar

Wallace, A.R. (1907). Is Mars Habitable, London: Macmillan.Google Scholar

Arrhenius, S. (1918). The Destinies of Stars, London: Putnams (translated by J. Fries from the 1915 Swedish publication).Google Scholar

Maunder, E.W. (1913). Are the Planets Inhabited? London: Harper and Brothers.Google Scholar

Pekeris, C. (1933). The Development and Present Status of the Theory of the Heat Balance in the Atmosphere. D.Sc. Thesis, Massachusetts Institute of Technology.Google Scholar

Goody, R. & Yung, Y. (1961). Atmospheric Radiation: Theoretical Basis, Oxford: Oxford University Press.Google Scholar

Simpson, G. (1927). Some studies in terrestrial radiation. Memoirs of the Royal Meteorological Society, 2(16) 69–95.Google Scholar

Simpson, G. (1928). Further studies in terrestrial radiation. Memoirs of the Royal Meteorological Society, 3(21) 1–26.Google Scholar

Simpson, G. (1929). The distribution of terrestrial radiation. Memoirs of the Royal Meteorological Society, 3(23), 53–78.Google Scholar

Abbe, C. (1901). The physical basis of long-range weather forecasts. Monthly Weather Review, 29, 551–561.10.1175/1520-0493(1901)29[551c:TPBOLW]2.0.CO;2CrossRefGoogle Scholar

Milanković, Milutin (1879–1958). From his autobiography with comments by his son, Vasko, and a preface by Andre Berger, European Geophysical Society, Kaltenburg-Lindau, 1995.Google Scholar

Milankovitch, M. (1941). Canon of Insolation and the Ice-Age Problem, Belgrade: Royal Serbian Academy.Google Scholar

Imbrie, J. & Imbrie, K., Ice Ages, Solving the Mystery, Cambridge, MA: Harvard University Press, 1979.10.1007/978-1-349-04699-7CrossRefGoogle Scholar

Richardson, L.F., Weather Prediction by Numerical Process, Cambridge: Cambridge University Press, 1922.Google Scholar

Pettit, E. & Nicholson, S. (1924). Radiation Measures on the Planet Mars. Publications of the Astronomical Society of the Pacific, 36, 269–272.Google Scholar

Sinton, W. (1986). Through the infrared with logbook and lantern slides, a history of infrared astronomy from 1868 to 1960. Publications of the Astronomical Society of the Pacific, 98, 246–251.10.1086/131750CrossRefGoogle Scholar

Harland, D. (2005). Water and the Search for Life on Mars, Springer.Google Scholar

Fleming, J. (2016). Inventing Atmospheric Science: Bjerknes, Rossby, Wexler, and the Foundations of Modern Meteorology, Cambridge, MA: MIT Press.10.7551/mitpress/10250.001.0001CrossRefGoogle Scholar

Flower, W.D. (1936). Sand Devils. Meteorological Office Professional Notes, 5, 1–16. London: His Majesty’s Stationery Office.Google Scholar

Lorenz, R. (2013). The longevity and aspect ratio of dust devils: effects on detection efficiencies and comparison of landed and orbital imaging at Mars. Icarus, 226(1), 964–970.10.1016/j.icarus.2013.06.031CrossRefGoogle Scholar

Courant, R., Friedrichs, K. & Lewy, H. (1928). Über die partiellen Differenzengleichungen der mathematischen Physik. Mathematische Annalen (in German), 100(1), 32–74.10.1007/BF01448839CrossRefGoogle Scholar

Bretz, J. Harlen (1923). The channeled scabland of the Columbia Plateau. Journal of Geology, 31, 617–649.10.1086/623053CrossRefGoogle Scholar

Soennichsen, J. (2008). Bretz’s Flood: The Remarkable Story of a Rebel Geologist and the World’s Greatest Flood, Seattle, WA: Sasquatch Books.Google Scholar

Baker, V.R. & Nummedal, D. (1978). The channeled scabland: a guide to the geomorphology of the Columbia Basin, Washington. Prepared for the Comparative Planetary Geology Field Conference held in the Columbia Basin, June 5–8, 1978, sponsored by Planetary Geology Program, NASA Office of Space Science.Google Scholar

Köppen, W. & Wegener, A. (1924). Die Klimate der Geologischen Vorzeit, Berlin: Borntraeger. An English translation (Climates of the Geological Past) was published in 2015.Google Scholar

Vernadsky, V. (1998). The Biosphere, Annotated Edition, Springer.CrossRefGoogle Scholar

Callendar, G.S. (1938). The artificial production of carbon dioxide and its influence on temperature. Quarterly Journal of the Royal Meteorological Society, 64(275), 223–240.10.1002/qj.49706427503CrossRefGoogle Scholar

Fleming, J.R. (2007). The Callendar Effect, The Life and Work of Guy Stewart Callendar (1898–1964), Boston, MA: American Meteorological Society.Google Scholar

Hawkins, E. & Jones, P. (2013). On Global Temperatures: 75 years after Callendar. Quarterly Journal of the Royal Meteorological Society, 139, 1961–1963.10.1002/qj.2178CrossRefGoogle Scholar

Adams, W.S. & Dunham, T. (1932). Absorption bands in the infra-red spectrum of Venus. Publications of the Astronomical Society of the Pacific, 44, 243–245.10.1086/124235CrossRefGoogle Scholar

Wildt, R. (1940). Note on the surface temperature of Venus. The Astrophysical Journal, 91, 266–268.10.1086/144165CrossRefGoogle Scholar

Jones, H. Spencer (1940). Life on Other Worlds, London: English Universities Press.Google Scholar

Adel, A. & Slipher, V.M. (1934). Concerning the carbon dioxide content of the atmosphere of the planet Venus. Physical Review, 46(3), 240.Google Scholar

Adel, A. & Slipher, V.M. (1934). The constitution of the atmospheres of the giant planets. Physical Review, 46, 902–906.10.1103/PhysRev.46.902CrossRefGoogle Scholar

Livio, M. (2017). Winston Churchill’s essay on alien life found. Nature, 542, 289–291.10.1038/542289aCrossRefGoogle Scholar

Harper, K., Weather by the Numbers: The Genesis of Modern Meteorology, Boston, MA: MIT Press, 2012.Google Scholar

Lewis, J.M. (2003). Ooishi’s observation viewed in the context of jet stream discovery. Bulletin of the American Meteorological Society, 84, 357–369.10.1175/BAMS-84-3-357CrossRefGoogle Scholar

Coen, R. (2014). Fu-go: The Curious History of Japan’s Balloon Bomb Attack on America, Lincoln, NE: University of Nebraska Press.10.2307/j.ctt1d9nmg0CrossRefGoogle Scholar

Drapeau, R.E. (2011). Operation Outward: Britain’s World War II offensive balloons. IEEE Power & Energy Magazine, 9, 94–105.10.1109/MPE.2011.941702CrossRefGoogle Scholar

Sverdrup, H.U. & Munk, W.H. (1947). Wind, Sea and Swell: Theory of Relations for Forecasting, US Navy Hydrographic Office Publication No. 601, 44 pp.Google Scholar

Lorenz, R.D. & Hayes, A.G. (2012). The growth of wind-waves in Titan’s hydrocarbon seas. Icarus, 219(1), 468–475.10.1016/j.icarus.2012.03.002CrossRefGoogle Scholar

Lorenz, R.D., Dooley, J.M., West, J.D. & Fujii, M. (2003). Backyard spectroscopy and photometry of Titan, Uranus and Neptune. Planetary and Space Science, 51(2), 113–125.10.1016/S0032-0633(02)00141-1CrossRefGoogle Scholar

Keiffer, H. et al. The planet Mars: from antiquity to the present, in Keiffer, H. et al. (eds.), Mars, Tucson, AZ: University of Arizona Press, 1986.Google Scholar

Harland, D.M., Water and the Search for Life on Mars, Springer, 2005.Google Scholar

Struve, O. (1952). Proposal for a project of high-precision stellar radial velocity work. The Observatory, 72, 199–200.Google Scholar

Mayer, C.H., McCullough, T.P. & Sloanaker, R.M. (1958). Observations of Venus at 3.15-cm wave length. The Astrophysical Journal, 127, 1.10.1086/146433CrossRefGoogle Scholar

Sinton, W.M. & Strong, J. (1960). Radiometric observations of Venus. The Astrophysical Journal, 131, 470.10.1086/146853CrossRefGoogle Scholar

Pettit, E. & Nicholson, S.B. (1955). Temperatures on the bright and dark sides of Venus. Publications of the Astronomical Society of the Pacific, 67, 293–303.CrossRefGoogle Scholar

Franklin, K.L. (1959). An account of the discovery of Jupiter as a radio source. The Astronomical Journal, 64, 37–39.10.1086/107852CrossRefGoogle Scholar

Lynch, P. (2008). The origins of computer weather prediction and climate modeling. Journal of Computational Physics, 227, 3431–3444.10.1016/j.jcp.2007.02.034CrossRefGoogle Scholar

Charney, J.G., Fjörtoft, R. & Von Neumann, J. (1950). Numerical integration of the barotropic vorticity equation. Tellus A, 2, 237–254.10.3402/tellusa.v2i4.8607CrossRefGoogle Scholar

Phillips, N.A. (1956). The general circulation of the atmosphere: a numerical experiment. Quarterly Journal of the Royal Meteorological Society, 82(352), 123–164.10.1002/qj.49708235202CrossRefGoogle Scholar

Fultz, D. (1949). A preliminary report on experiments with thermally produced lateral mixing in a rotating hemispherical shell of liquid. Journal of Meteorology, 6(1), 17–33.10.1175/1520-0469(1949)006<0017:APROEW>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Riehl, H. & Fultz, D. (1957). Jet stream and long waves in a steady rotating‐dishpan experiment: structure of the circulation. Quarterly Journal of the Royal Meteorological Society, 83(356), 215–231.10.1002/qj.49708335608CrossRefGoogle Scholar

Ghil, M., Read, P. & Smith, L. (2010). Geophysical flows as dynamical systems: the influence of Hide’s experiments. Astronomy & Geophysics, 51(4), 4–28.10.1111/j.1468-4004.2010.51428.xCrossRefGoogle Scholar

Stommel, H. (1961). Thermohaline circulation with two stable regimes of flow. Tellus, 13, 224–241.10.3402/tellusa.v13i2.9491CrossRefGoogle Scholar

Langway, C.C., The History of Early Polar Ice Cores, US Army Cold Regions Research and Engineering Laboratory, ERDC/CRREL TR-08–1, January 2008.CrossRefGoogle Scholar

Sterken, C. (2011). Ernst Julius Opik: Solar variability and climate change. Baltic Astronomy, 20 195–203,Google Scholar

Opik, E. (1952). Ice ages. Irish Astronomical Journal, 2, 71–84.Google Scholar

Opik, E. (1965). Climatic change in cosmic perspective. Icarus, 4, 289–307.CrossRefGoogle Scholar

Wexler, H. (1956). Variations in insolation, general circulation and climate. Tellus A, 8, 480–494.10.3402/tellusa.v8i4.9031CrossRefGoogle Scholar

Shapley, H., Climatic Change, Evidence, Causes and Effects, Cambridge, MA: Harvard University Press, 1953.CrossRefGoogle Scholar

Plass, G.N. (1956). The influence of the 15μ carbon‐dioxide band on the atmospheric infra‐red cooling rate. Quarterly Journal of the Royal Meteorological Society, 82(353), 310–324.CrossRefGoogle Scholar

Plass, G.N. (1956). Effect of carbon dioxide variations on climate. American Journal of Physics, 24(5), 376–387.10.1119/1.1934233CrossRefGoogle Scholar

Weart, S., The Discovery of Global Warming, Cambridge, MA: Harvard University Press, 2008.Google Scholar

Revelle, R. & Suess, H.E. (1957). Carbon dioxide exchange between atmosphere and ocean, and the question of an increase of atmospheric CO₂ during the past decades. Tellus, 9, 18–27.CrossRefGoogle Scholar

Keeling, C.D. (1960). The concentration and isotopic abundances of carbon dioxide in the atmosphere. Tellus, 12(2), 200–203.10.1111/j.2153-3490.1960.tb01300.xCrossRefGoogle Scholar

Strughold, H., The Green and Red Planet, Albuquerque, NM: University of New Mexico Press, 1953.Google Scholar

Cockell, C. (2001). ‘Astrobiology’ and the ethics of new science. Interdisciplinary Science Reviews, 26, 90–96.10.1179/isr.2001.26.2.90CrossRefGoogle Scholar

Spinrad, H., Münch, G. & Kaplan, L.D. (1963). Letter to the Editor: The detection of water vapor on Mars. The Astrophysical Journal, 137, 1319.10.1086/147613CrossRefGoogle Scholar

Kaplan, L.D., Münch, G. & Spinrad, H. (1964). An analysis of the spectrum of Mars. The Astrophysical Journal, 139, 1–15.10.1086/147736CrossRefGoogle Scholar

Latil, P. & Mar, T. (1959). Planetary observations by the multi-balloon technique. New Scientist, 7 May, 1005–1007.Google Scholar

Dollfus, A., Observations of water vapor on Mars and Venus. In The Origin and Evolution of Atmospheres and Oceans, Proceedings of a Conference, held at the Goddard Institute for Space Studies, NASA, New York, April 8–9, 1963. Edited by Brancazio, P.J. & Cameron, A.G.W., New York: Wiley, 1964, p. 257.Google Scholar

House, F.B., Gruber, A., Hunt, G.E. & Mecherikunnel, A.T. (1986). History of satellite missions and measurements of the Earth radiation budget (1957–1984). Reviews of Geophysics, 24(2), 357–377.10.1029/RG024i002p00357CrossRefGoogle Scholar

Wexler, H. (1954). Observing the weather from a satellite vehicle. Journal of the British Interplanetary Society, 13, 269–276.Google Scholar

Sagan, C., The Radiation Balance of Venus. JPL Technical Report 32–34, September 1960.Google Scholar

Kuzmin, A. & Clark, B. (1965). The polarization measurement and the brightness temperature of Venus at 10.6 cm wavelength. The Astronomical Journal, 43, 595–617.Google Scholar

Öpik, E.J. (1961). The aeolosphere and atmosphere of Venus. Journal of Geophysical Research, 66(9), 2807–2819.10.1029/JZ066i009p02807CrossRefGoogle Scholar

Hansen, J.E. & Matsushima, S. (1967). The atmosphere and surface temperature of Venus: a dust insulation model. The Astrophysical Journal, 150, 1139.10.1086/149410CrossRefGoogle Scholar

Samuelson, R.E. (1967). Greenhouse effect in semi-infinite scattering atmospheres: application to Venus. The Astrophysical Journal, 147, 782.10.1086/149053CrossRefGoogle Scholar

Danielson, R.E., Caldwell, J.J. & Larach, D.R. (1973). An inversion in the atmosphere of Titan. Icarus, 20(4), 437–443.10.1016/0019-1035(73)90016-XCrossRefGoogle Scholar

Zellner, B. (1973). The polarization of Titan. Icarus, 18(4), 661–664.CrossRefGoogle Scholar

Hunten, D. (Ed.), The Atmosphere of Titan: A Workshop held at Ames Research Center, July 1973, NASA SP-340.Google Scholar

Kliore, A., Cain, D.L., Levy, G.S., Eshleman, V.R., Fjeldbo, G. & Drake, F.D. (1965). Occultation experiment: results of the first direct measurement of Mars’s atmosphere and ionosphere. Science, 149(3689), 1243–1248.10.1126/science.149.3689.1243CrossRefGoogle Scholar

Fjeldbo, G., Fjeldbo, W.C. & Eshleman, V.R. (1966). Models for the atmosphere of Mars based on the Mariner 4 occultation experiment. Journal of Geophysical Research, 71(9), 2307–2316.10.1029/JZ071i009p02307CrossRefGoogle Scholar

Leighton, R.B. & Murray, B.C. (1966). Behavior of carbon dioxide and other volatiles on Mars. Science, 153(3732), 136–144.10.1126/science.153.3732.136CrossRefGoogle ScholarPubMed

Manabe, S. & Strickler, R.F. (1964). Thermal equilibrium of the atmosphere with a convective adjustment. Journal of the Atmospheric Sciences, 21(4), 361–385.10.1175/1520-0469(1964)021<0361:TEOTAW>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Restoring the Quality of Our Environment. Report of the Environment Pollution Panel, President’s Science Advisory Committee, The White House, November 1965.Google Scholar

Möller, F. (1963). On the influence of changes in the CO₂ concentration in air on the radiation balance of the Earth’s surface and on the climate. Journal of Geophysical Research, 68(13), 3877–3886.10.1029/JZ068i013p03877CrossRefGoogle Scholar

Manabe, S. & Wetherald, R.T. (1967). Thermal equilibrium of the atmosphere with a given distribution of relative humidity. Journal of Atmospheric Sciences, 24, 241–259.10.1175/1520-0469(1967)024<0241:TEOTAW>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Lorenz, E.N. (1963). Deterministic nonperiodic flow. Journal of Atmospheric Sciences, 20(2), 130–148.10.1175/1520-0469(1963)020<0130:DNF>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Gleick, J., Chaos: Making a New Science, New York: Viking, 1987.Google Scholar

Manabe, S. & Bryan, K. (1969). Climate calculations with a combined ocean-atmosphere model. Journal of Atmospheric Science, 26, 786–789.10.1175/1520-0469(1969)026<0786:CCWACO>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Leovy, C. & Mintz, Y. (1969). Numerical simulation of the atmospheric circulation and climate of Mars. Journal of the Atmospheric Sciences, 26(6), 1167–1190.10.1175/1520-0469(1969)026<1167:NSOTAC>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Opik, E. (1965). Climatic change in cosmic perspective. Icarus, 4, 289–307.10.1016/0019-1035(65)90006-0CrossRefGoogle Scholar

Eriksson, E., Air-ocean-icecap interactions in relation to climatic fluctuations and glaciation cycles. In Mitchell, J.M. (Ed.), Causes of Climatic Change. Meteorological Monographs, 8(30), Boston, MA: American Meteorological Society, 1968, pp. 68–92.CrossRefGoogle Scholar

Fritz, S., The heating distribution in the atmosphere and climatic change. In Pfeffer, R. (Ed.), Dynamics of Climate: The Proceedings of a Conference on the Application of Numerical Integration Techniques to the Problem of the General Circulation, October 26–28, 1955, New York: Pergamon Press, 1955, pp. 96–102.Google Scholar

Cobb, W.E. & Wells, H.J. (1970). The electrical conductivity of oceanic air and its correlation to global atmospheric pollution. Journal of the Atmospheric Sciences, 27(5), 814–819.10.1175/1520-0469(1970)027<0814:TECOOA>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Rasool, S.I. & Schneider, S.H. (1971). Atmospheric carbon dioxide and aerosols: effects of large increases on global climate. Science, 173(3992), 138–141.CrossRefGoogle ScholarPubMed

Peterson, T.C., Connolley, W.M & Fleck, J. (2008). The myth of the 1970s global cooling scientific consensus. Bulletin of the American Meteorological Society, 89(9), 1325–1337.10.1175/2008BAMS2370.1CrossRefGoogle Scholar

Goldblatt, C. & Watson, A.J. (2012). The runaway greenhouse: implications for future climate change, geoengineering and planetary atmospheres. Philosophical Transactions of the Royal Society of London A: Mathematical, Physical and Engineering Sciences, 370(1974), 4197–4216.Google ScholarPubMed

Komabayashi, M. (1967). Discrete equilibrium temperatures of a hypothetical planet with the atmosphere and the hydrosphere of a one component–two phase system under constant solar radiation. Journal of the Meteorological Society of Japan, 45, 137–139.10.2151/jmsj1965.45.1_137CrossRefGoogle Scholar

Ingersoll, A.P. (1969). The runaway greenhouse: a history of water on Venus. Journal of the Atmospheric Sciences, 26(6), 1191–1198.2.0.CO;2>CrossRefGoogle Scholar

Rasool, S.I. & de Bergh, C. (1970). The runaway greenhouse and the accumulation of CO₂ in the Venus atmosphere. Nature, 226, 1037–1039.10.1038/2261037a0CrossRefGoogle ScholarPubMed

Lorenz, E. (1970). Climatic change as a mathematical problem, Journal of Applied Meteorology, 9, 325–329.10.1175/1520-0450(1970)009<0325:CCAAMP>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Feagre, A. (1972). An intransitive model of the Earth–atmosphere–ocean system, Journal of Applied Meteorology, 11, 4–6.10.1175/1520-0450(1972)011<0004:AIMOTE>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Pollack, J.B. (1969). A nongray CO₂-H₂O greenhouse model of Venus. Icarus, 10(2), 314–341.10.1016/0019-1035(69)90032-3CrossRefGoogle Scholar

Morrison, D., Cruikshank, D.P. & Murphy, R.E. (1972). Temperatures of Titan and the Galilean satellites at 20 microns. The Astrophysical Journal, 173, L143.10.1086/180934CrossRefGoogle Scholar

Gillett, F.C., Forrest, W.J. & Merrill, K.M. (1973). 8–13 micron observations of Titan. The Astrophysical Journal, 184, L93.10.1086/181296CrossRefGoogle Scholar

Gillett, F.C. (1975). Further observations of the 8–13 micron spectrum of Titan. The Astrophysical Journal, 201, L41–L43.10.1086/181937CrossRefGoogle Scholar

Sagan, C. (1973). The greenhouse of Titan. Icarus, 18(4), 649–656.10.1016/0019-1035(73)90068-7CrossRefGoogle Scholar

Low, F.J. & Rieke, G.H. (1974). Infrared photometry of Titan. The Astrophysical Journal, 190, L143.10.1086/181527CrossRefGoogle Scholar

Murray, B.C., Ward, W.R. & Yeung, S.C. (1973). Periodic insolation variations on Mars. Science, 180(4086), 638–640.10.1126/science.180.4086.638CrossRefGoogle ScholarPubMed

Ward, W.R. (1974). Climatic variations on Mars: 1. Astronomical theory of insolation. Journal of Geophysical Research, 79(24), 3375–3386.10.1029/JC079i024p03375CrossRefGoogle Scholar

Byrne, S. (2009) The polar deposits of Mars. Annual Reviews of Earth and Planetary Science, 37, 8.1–8.26.10.1146/annurev.earth.031208.100101CrossRefGoogle Scholar

Sagan, C. and Mullen, G. (1972). Earth and Mars: evolution of atmospheres and surface temperatures. Science, 177(4043), 52–56.10.1126/science.177.4043.52CrossRefGoogle ScholarPubMed

Henderson-Sellers, A. & Meadows, A.J. (1979). A simplified model for deriving planetary surface temperatures as a function of atmospheric chemical composition. Planetary and Space Science, 27(8), 1095–1099.10.1016/0032-0633(79)90080-1CrossRefGoogle Scholar

Henderson-Sellers, A. & Meadows, A.J. (1976). The evolution of the surface temperature of Mars. Planetary and Space Science, 24(1), 41–44.10.1016/0032-0633(76)90059-3CrossRefGoogle Scholar

Dickinson, R.E. & Cicerone, R.J. (1986). Future global warming from atmospheric trace gases. Nature, 319, 109–115.10.1038/319109a0CrossRefGoogle Scholar

Lovelock, J.E. (1965). A physical basis for life detection experiments. Nature, 207(997), 568–570.10.1038/207568a0CrossRefGoogle ScholarPubMed

Hitchcock, D.R. & Lovelock, J.E. (1967). Life detection by atmospheric analysis. Icarus, 7(1), 149–159.10.1016/0019-1035(67)90059-0CrossRefGoogle Scholar

Lovelock, J.E. (1972). Gaia as seen through the atmosphere. Atmospheric Environment, 6(8), 579–580.10.1016/0004-6981(72)90076-5CrossRefGoogle Scholar

Lovelock, J.E. & Margulis, L. (1974). Atmospheric homeostasis by and for the biosphere: the Gaia hypothesis. Tellus: Series A (Stockholm: International Meteorological Institute), 26(1–2), 2–10.10.3402/tellusa.v26i1-2.9731CrossRefGoogle Scholar

Margulis, L. & Lovelock, J.E. (1974). Biological modulation of the Earth’s atmosphere. Icarus, 21(4), 471–489.10.1016/0019-1035(74)90150-XCrossRefGoogle Scholar

Schwartzman, D., Life, Temperature and The Earth, New York: Columbia University Press, 1999.Google Scholar

Lovelock, J.E., The Ages of Gaia, New York: Norton, 1988.Google Scholar

Lovelock, J.E., Homage to Gaia, Oxford: Oxford University Press, 2001.Google Scholar

Hansen, J.E. & Hovenier, J. (1974). Interpretation of the polarization of Venus. Journal of the Atmospheric Sciences, 31(4), 1137–1160.10.1175/1520-0469(1974)031<1137:IOTPOV>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Gierasch, P.J. (1975). Meridional circulation and the maintenance of the Venus atmospheric rotation. Journal of the Atmospheric Sciences, 32(6), 1038–1044.10.1175/1520-0469(1975)032<1038:MCATMO>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Fels, S.B. & Lindzen, R.S. (1974). The interaction of thermally excited gravity waves with mean flows. Geophysical and Astrophysical Fluid Dynamics, 6(2), 149–191.10.1080/03091927409365793CrossRefGoogle Scholar

Schubert, G. & Whitehead, J.A. (1969). Moving flame experiment with liquid mercury: possible implications for the Venus atmosphere. Science, 163(3862), 71–72.10.1126/science.163.3862.71CrossRefGoogle ScholarPubMed

Kálnay De Rivas, E. (1973). Numerical models of the circulation of the atmosphere of Venus. Journal of the Atmospheric Sciences, 30(5), 763–779.10.1175/1520-0469(1973)030<0763:NMOTCO>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Pollack, J.B., Toon, O.B. & Boese, R. (1980). Greenhouse models of Venus’ high surface temperature, as constrained by Pioneer Venus measurements. Journal of Geophysical Research, 85, A13, 8223–8231.10.1029/JA085iA13p08223CrossRefGoogle Scholar

McCrea, W. (1975). Ice ages and the Galaxy. Nature, 255, 607–609.10.1038/255607a0CrossRefGoogle Scholar

Shapley, H. (1921). Note on a possible factor in changes of geological climate. Journal of Geology, 29, 502–204.10.1086/622806CrossRefGoogle Scholar

Hays, J.D., Imbrie, J. & Shackleton, N.J. (1976). Variations in the Earth’s orbit: pacemaker of the ice ages. Science, 194(4270), 1121–1132.10.1126/science.194.4270.1121CrossRefGoogle ScholarPubMed

Henderson-Sellers, A. (1979). Clouds and the long-term stability of the Earth’s atmosphere and climate. Nature, 279, 786–788.10.1038/279786a0CrossRefGoogle Scholar

Rossow, W.B., Henderson-Sellers, A. & Weinreich, S.K. (1982). Cloud feedback: a stabilizing effect for the early Earth? Science, 217(4566), 1245–1247.10.1126/science.217.4566.1245CrossRefGoogle ScholarPubMed

Hess, S.L., Henry, R.M., Leovy, C.B., Ryan, J.A. & Tillman, J.E. (1977). Meteorological results from the surface of Mars: Viking 1 and 2. Journal of Geophysical Research, 82(28), 4559–4574.10.1029/JS082i028p04559CrossRefGoogle Scholar

Nakamura, Y. & Anderson, D.L. (1979). Martian wind activity detected by a seismometer at Viking lander 2 site. Geophysical Research Letters, 6(6), 499–502.10.1029/GL006i006p00499CrossRefGoogle Scholar

Lorenz, R.D. (1996). Martian surface wind speeds described by the Weibull distribution. Journal of Spacecraft and Rockets, 33(5), 754–756.10.2514/3.26833CrossRefGoogle Scholar

Pollack, J.B., Leovy, C.B., Mintz, Y.H. & Van Camp, W. (1976). Winds on Mars during the Viking season: predictions based on a general circulation model with topography. Geophysical Research Letters, 3(8), 479–482.10.1029/GL003i008p00479CrossRefGoogle Scholar

Wall, S.D. (1981). Analysis of condensates formed at the Viking 2 Lander site: the first winter. Icarus, 47(2), 173–183.10.1016/0019-1035(81)90165-2CrossRefGoogle Scholar

Hansen, J., Johnson, D., Lacis, A., et al. (1981). Climate impact of increasing atmospheric carbon dioxide. Science, 213(4511), 957–966.10.1126/science.213.4511.957CrossRefGoogle ScholarPubMed

Lindzen, R.S., Hou, A.Y. & Farrell, B.F. (1982). The role of convective model choice in calculating the climate impact of doubling CO₂. Journal of the Atmospheric Sciences, 39(6), 1189–1205.10.1175/1520-0469(1982)039<1189:TROCMC>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Schneider, S.H. & Thompson, S.L. (1980). Cosmic conclusions from climatic models: can they be justified? Icarus, 41(3), 456–469.10.1016/0019-1035(80)90229-8CrossRefGoogle Scholar

Hoffert, M.I., Callegari, A.J., Hsieh, C.T. & Ziegler, W. (1981). Liquid water on Mars: an energy balance climate model for CO₂/H₂O atmospheres. Icarus, 47(1), 112–129.10.1016/0019-1035(81)90096-8CrossRefGoogle Scholar

James, P.B. & North, G.R. (1982). The seasonal CO₂ cycle on Mars: an application of an energy balance climate model. Journal of Geophysical Research: Solid Earth, 87(B12), 10271–10283.10.1029/JB087iB12p10271CrossRefGoogle Scholar

Paltridge, G.W. (1975). Global dynamics and climate: a system of minimum entropy exchange. Royal Meteorological Society, Quarterly Journal, 101, 475–484.Google Scholar

Paltridge, G.W. (1978). The steady-state format of global climate. Quarterly Journal of the Royal Meteorological Society, 104(442), 927–945.Google Scholar

Lorenz, E.N., Generation of available potential energy and the intensity of the general circulation. In Pfeffer, H. (ed.) Dynamics of Climate: Proceedings of a Conference. Symposium Publications Division, Pergamon Press, 1960.Google Scholar

Hoffert, M.I., Callegari, A.J., Hsieh, C.T. & Ziegler, W. (1981). Liquid water on Mars: an energy balance climate model for CO₂/H₂O atmospheres. Icarus, 47(1), 112–129.10.1016/0019-1035(81)90096-8CrossRefGoogle Scholar

James, P.B. & North, G.R. (1982). The seasonal CO₂ cycle on Mars: an application of an energy balance climate model. Journal of Geophysical Research: Solid Earth, 87(B12), 10271–10283.10.1029/JB087iB12p10271CrossRefGoogle Scholar

François, L.M., Walker, J.C.G. & Kuhn, W.R. (1990). A numerical simulation of climate changes during the obliquity cycle on Mars. Journal of Geophysical Research: Solid Earth, 95(B9), 14761–14778.10.1029/JB095iB09p14761CrossRefGoogle ScholarPubMed

Jaffe, W., Caldwell, J. & Owen, T. (1980). Radius and brightness temperature observations of Titan at centimeter wavelengths by the Very Large Array. The Astrophysical Journal, 242, 806–811.10.1086/158515CrossRefGoogle Scholar

Lindal, G.F., Wood, G.E., Hotz, H.B., et al. (1983). The atmosphere of Titan: an analysis of the Voyager 1 radio occultation measurements. Icarus, 53(2), 348–363. (Gunnar Fjeldbo at Stanford University, who had been part of the team executing the Mariner 4 experiment at Mars, had changed his name to Gunnar Lindal.)10.1016/0019-1035(83)90155-0CrossRefGoogle Scholar

Hunten, D.M.. In Gehrels, T. and Matthews, M. Shapley (eds.), Saturn, Tucson, AZ: University of Arizona Press, 1984.Google Scholar

Samuelson, R.E. (1983). Radiative equilibrium model of Titan’s atmosphere. Icarus, 53(2), 364–387.10.1016/0019-1035(83)90156-2CrossRefGoogle Scholar

Pollack, J.B., Kasting, J.F., Richardson, S.M. & Poliakoff, K. (1987). The case for a wet, warm climate on early Mars. Icarus, 71(2), 203–224.10.1016/0019-1035(87)90147-3CrossRefGoogle ScholarPubMed

Squyres, S.W. & Carr, M.H. (1986). Geomorphic evidence for the distribution of ground ice on Mars. Science, 231(4735), 249–252.10.1126/science.231.4735.249CrossRefGoogle ScholarPubMed

Clow, G.D. (1987). Generation of liquid water on Mars through the melting of a dusty snowpack. Icarus, 72(1), 95–127.10.1016/0019-1035(87)90123-0CrossRefGoogle Scholar

Carr, M.H. (1979). Formation of Martian flood features by release of water from confined aquifers. Journal of Geophysical Research, 84(13), 2995–3007.10.1029/JB084iB06p02995CrossRefGoogle Scholar

Clifford, S.M. (1993). A model for the hydrologic and climatic behavior of water on Mars. Journal of Geophysical Research, 98(E6), 10–973.CrossRefGoogle Scholar

Parker, T.J., Saunders, R.S. & Schneeberger, D.M. (1989). Transitional morphology in West Deuteronilus Mensae, Mars: implications for modification of the lowland/upland boundary. Icarus, 82(1), 111–145.10.1016/0019-1035(89)90027-4CrossRefGoogle Scholar

Baker, V.R., Strom, R.G., Gulick, V.C., Kargel, J.S. & Komatsu, G. (1991). Ancient oceans, ice sheets and the hydrological cycle on Mars. Nature, 352, 589–594.10.1038/352589a0CrossRefGoogle Scholar

Carr, M. (1987). Water on Mars. Nature, 326(6108), 30–35.10.1038/326030a0CrossRefGoogle Scholar

Carr, M., Water on Mars, Oxford: Oxford University Press, 1996.10.1093/oso/9780195099386.001.0001CrossRefGoogle Scholar

Esposito, L.W. (1984). Sulfur dioxide: episodic injection shows evidence for active Venus volcanism. Science, 223(4640), 1072–1074.10.1126/science.223.4640.1072CrossRefGoogle ScholarPubMed

Marov, M. & Grinspoon, D., The Planet Venus, New Haven, CT: Yale University Press, 1998.Google Scholar

Moroz, V. (2001). Spectra and spacecraft. Planetary and Space Science, 49, 173–190.10.1016/S0032-0633(00)00130-6CrossRefGoogle Scholar

Krasnopolsky, V.A. (2006). Chemical composition of Venus atmosphere and clouds: some unsolved problems. Planetary and Space Science, 54(13), 1352–1359.10.1016/j.pss.2006.04.019CrossRefGoogle Scholar

Sagdeev, R.Z., et al. (1986). Overview of VEGA Venus balloon in situ meteorological measurements. Science, 231, 1411–1414.10.1126/science.231.4744.1411CrossRefGoogle ScholarPubMed

Crisp, D., Ingersoll, A.P., Hildebrand, C.E. & Preston, R.A. (1990). VEGA balloon meteorological measurements. Advances in Space Research, 10(5), 109–124.10.1016/0273-1177(90)90172-VCrossRefGoogle Scholar

Kasting, J.F., Pollack, J.B. & Ackerman, T.P. (1984). Response of Earth’s atmosphere to increases in solar flux and implications for loss of water from Venus. Icarus, 57(3), 335–355.10.1016/0019-1035(84)90122-2CrossRefGoogle ScholarPubMed

Watson, A.J., Donahue, T.M. & Kuhn, W.R. (1984). Temperatures in a runaway greenhouse on the evolving Venus: implications for water loss. Earth and Planetary Science Letters, 68(1), 1–6.10.1016/0012-821X(84)90135-3CrossRefGoogle Scholar

Donahue, T.M., Hoffman, J.H, Hodges, R.R. & Watson, A.J. (1982). Venus was wet: a measurement of the ratio of deuterium to hydrogen. Science, 216(4546), 630–633.10.1126/science.216.4546.630CrossRefGoogle Scholar

Kasting, J.F. & Pollack, J.B. (1983). Loss of water from Venus. I. Hydrodynamic escape of hydrogen. Icarus, 53(3), 479–508.10.1016/0019-1035(83)90212-9CrossRefGoogle Scholar

Grinspoon, D.H. (1987). Was Venus wet? Deuterium reconsidered. Science, 238(4834), 1702–1704.10.1126/science.238.4834.1702CrossRefGoogle ScholarPubMed

Watson, A.J. & Lovelock, J.E. (1983). Biological homeostasis of the global environment: the parable of Daisyworld. Tellus B, 35(4), 284–289.10.3402/tellusb.v35i4.14616CrossRefGoogle Scholar

Wood, A.J., Ackland, G.J., Dyke, J.G., Williams, H.T. & Lenton, T. M. (2008). Daisyworld: a review. Reviews of Geophysics, 46(1) RG1001.10.1029/2006RG000217CrossRefGoogle Scholar

Koeslag, J.H., Saunders, P.T. & Wessels, J.A. (1997). Glucose homeostasis with infinite gain: further lessons from the Daisyworld parable? Journal of Endocrinology, 154(2), 187–192.10.1677/joe.0.1540187CrossRefGoogle ScholarPubMed

Walker, J.C.G., Hays, P.B. & Kasting, J.F. (1981). A negative feedback mechanism for the long-term stabilization of Earth’s surface temperature. Journal of Geophysical Research: Oceans, 86(C10), 9776–9782.10.1029/JC086iC10p09776CrossRefGoogle Scholar

Turco, R.P., Toon, O.B., Ackerman, T.P., Pollack, J.B. & Sagan, C. (1983). Nuclear winter: global consequences of multiple nuclear explosions. Science, 222(4630), 1283–1292.10.1126/science.222.4630.1283CrossRefGoogle Scholar

McKay, C.P., Pollack, J. B. & Courtin, R. (1989). The thermal structure of Titan’s atmosphere. Icarus, 80(1), 23–53.10.1016/0019-1035(89)90160-7CrossRefGoogle ScholarPubMed

Lemmon, M.T., Karkoschka, E. & Tomasko, M. (1993). Titan’s rotation: surface feature observed. Icarus, 103, 329–332.10.1006/icar.1993.1074CrossRefGoogle Scholar

McKay, C.P., Pollack, J.B. & Courtin, R. (1991). The greenhouse and antigreenhouse effects on Titan. Science, 253(5024), 1118–1121.10.1126/science.11538492CrossRefGoogle ScholarPubMed

Thatcher, M., Speech to United Nations General Assembly (Global Environment), November 8, 1989.Google Scholar

Robinson, T.D. & Catling, D.C. (2014). Common 0.1-bar tropopause in thick atmospheres set by pressure-dependent infrared transparency. Nature Geoscience, 7(1), 12–15.10.1038/ngeo2020CrossRefGoogle Scholar

Hillier, J., Helfenstein, P., Verbiscer, A., et al. (1990). Voyager disk-integrated photometry of Triton. Science, 250(4979), 419–421.10.1126/science.250.4979.419CrossRefGoogle ScholarPubMed

Tyler, G.L., Sweetnam, D.N., Anderson, J.D., et al. (1989). Voyager radio science observations of Neptune and Triton. Science, 246(4936), 1466–1473.CrossRefGoogle ScholarPubMed

Hansen, C.J. & Paige, D.A. (1992). A thermal model for the seasonal nitrogen cycle on Triton. Icarus, 99(2), 273–288.10.1016/0019-1035(92)90146-XCrossRefGoogle Scholar

Zalucha, A.M. & Michaels, T.I. (2013). A 3D general circulation model for Pluto and Triton with fixed volatile abundance and simplified surface forcing. Icarus, 223(2), 819–831.10.1016/j.icarus.2013.01.026CrossRefGoogle Scholar

Stansberry, J.A., Pisano, D.J. & Yelle, R.V. (1996). The emissivity of volatile ices on Triton and Pluto. Planetary and Space Science, 44(9), 945–955.10.1016/0032-0633(96)00001-3CrossRefGoogle Scholar

Stansberry, J.A. & Yelle, R.V. (1999). Emissivity and the fate of Pluto’s atmosphere. Icarus, 141(2), 299–306.10.1006/icar.1999.6169CrossRefGoogle Scholar

Johnsen, S.J., Clausen, H.B., Dansgaard, W., et al. (1992). Irregular glacial interstadials recorded in a new Greenland ice core. Nature, 359(6393), 311–313.10.1038/359311a0CrossRefGoogle Scholar

Petit, J.R., Jouzel, J., Raynaud, D., et al. (1999). Climate and atmospheric history of the past 420,000 years from the Vostok ice core, Antarctica. Nature, 399(6735), 429–436.10.1038/20859CrossRefGoogle Scholar

Hong, S., Candelone, J.P., Patterson, C.C. & Boutron, C.F. (1994). Greenland ice evidence of hemispheric lead pollution two millennia ago by Greek and Roman civilizations. Science, 265(5180), 1841–1843.10.1126/science.265.5180.1841CrossRefGoogle ScholarPubMed

Dansgaard, W., Johnsen, S.J., Clausen, H.B., et al. (1993). Evidence for general instability of past climate from a 250-kyr ice-core record. Nature, 364(6434), 218–220.10.1038/364218a0CrossRefGoogle Scholar

Alley, R.B. & MacAyeal, D.R. (1994). Ice-rafted debris associated with binge/purge oscillations of the Laurentide Ice Sheet. Paleoceanography, 9(4), 503–511.10.1029/94PA01008CrossRefGoogle Scholar

Heinrich, H. (1988). Origin and consequences of cyclic ice rafting in the northeast Atlantic Ocean during the past 130,000 years. Quaternary Research, 29(2), 142–152.10.1016/0033-5894(88)90057-9CrossRefGoogle Scholar

Rahmstorf, S. (1994). Rapid climate transitions in a coupled ocean–atmosphere model. Nature, 372(6501), 82–85.CrossRefGoogle Scholar

Ganopolski, A., Rahmstorf, S., Petoukhov, V. & Claussen, M. (1998). Simulation of modern and glacial climates with a coupled global model of intermediate complexity. Nature, 391(6665), 351–356.10.1038/34839CrossRefGoogle Scholar

Ganopolski, A. & Rahmstorf, S. (2001). Rapid changes of glacial climate simulated in a coupled climate model. Nature, 409(6817), 153–158.10.1038/35051500CrossRefGoogle Scholar

Yung, Y.L., Allen, M. & Pinto, J.P. (1984). Photochemistry of the atmosphere of Titan: comparison between model and observations. The Astrophysical Journal Supplement Series, 55, 465–506.10.1086/190963CrossRefGoogle ScholarPubMed

Yung, Y.L. & Pinto, J.P. (1978). Primitive atmosphere and implications for the formation of channels on Mars. Nature, 273(5665), 730–732.10.1038/273730a0CrossRefGoogle Scholar

Flasar, F.M. (1983). Oceans on Titan? Science, 221(4605), 55–57.CrossRefGoogle ScholarPubMed

Lunine, J.I., Stevenson, D.J. & Yung, Y.L. (1983). Ethane ocean on Titan. Science, 222(4629), 1229–1230.10.1126/science.222.4629.1229CrossRefGoogle ScholarPubMed

Stevenson, D.J. & Potter, B.E. (1986). Titan’s latitudinal temperature distribution and seasonal cycle. Geophysical Research Letters, 13(2), 93–96.10.1029/GL013i002p00093CrossRefGoogle Scholar

McKay, C.P., Pollack, J.B., Lunine, J.I. & Courtin, R. (1993). Coupled atmosphere–ocean models of Titan’s past. Icarus, 102(1), 88–98.10.1006/icar.1993.1034CrossRefGoogle ScholarPubMed

Lunine, J.I. & Rizk, B. (1989). Thermal evolution of Titan’s atmosphere. Icarus, 80(2), 370–389.10.1016/0019-1035(89)90147-4CrossRefGoogle Scholar

McKay, C.P., Toon, O.B. & Kasting, J.F. (1991). Making Mars habitable. Nature, 352(6335), 489–496.10.1038/352489a0CrossRefGoogle ScholarPubMed

McKay, C.P. (1982). Terraforming Mars. Journal of the British Interplanetary Society, 35, 427–433.Google Scholar

Dickinson, R.E. & Cicerone, R.J. (1986). Future global warming from atmospheric trace gases. Nature, 319, 109–115.10.1038/319109a0CrossRefGoogle Scholar

Bougher, S.W., Hunten, D.M. & Phillips, R.J. (Eds.) (1997). Venus II: Geology, Geophysics, Atmosphere, and Solar Wind Environment. Tucson, AZ: University of Arizona Press.Google Scholar

Esposito, L.W., Stofan, E.R. & Cravens, T.E. (Eds.) (2013). Exploring Venus as a Terrestrial Planet, AGU Geophysical Monograph 176. John Wiley & Sons.Google Scholar

Sleep, N.H., Zahnle, K.J., Kasting, J.F. & Morowitz, H.J. (1989). Annihilation of ecosystems by large asteroid impacts on the early Earth. Nature, 342(6246), 139.10.1038/342139a0CrossRefGoogle ScholarPubMed

Abe, Y. & Matsui, T. (1988). Evolution of an impact-generated H₂O–CO₂ atmosphere and formation of a hot proto-ocean on Earth. Journal of the Atmospheric Sciences, 45(21), 3081–3101.10.1175/1520-0469(1988)045<3081:EOAIGH>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Zahnle, K.J., Kasting, J.F. & Pollack, J.B. (1988). Evolution of a steam atmosphere during Earth’s accretion. Icarus, 74(1), 62–97.10.1016/0019-1035(88)90031-0CrossRefGoogle ScholarPubMed

Hamano, K., Abe, Y. & Genda, H. (2013). Emergence of two types of terrestrial planet on solidification of magma ocean. Nature, 497(7451), 607.10.1038/nature12163CrossRefGoogle ScholarPubMed

Kasting, J.F., Whitmire, D.P. & Reynolds, R.T. (1993). Habitable zones around main sequence stars. Icarus, 101(1), 108–128.10.1006/icar.1993.1010CrossRefGoogle ScholarPubMed

Pierazzo, E., Kring, D.A. & Melosh, H.J. (1998). Hydrocode simulation of the Chicxulub impact event and the production of climatically active gases, Journal of Geophysical Research, 103, 28607–28625.10.1029/98JE02496CrossRefGoogle Scholar

Bullock, M.A. & Grinspoon, D.H. (1996). The stability of climate on Venus. Journal of Geophysical Research: Planets, 101(E3), 7521–7529.10.1029/95JE03862CrossRefGoogle Scholar

Taylor, F. & Grinspoon, D. (2009). Climate evolution of Venus. Journal of Geophysical Research: Planets, 114(E9).CrossRefGoogle Scholar

Hashimoto, G.L., Abe, Y. & Sasaki, S. (1997). CO₂ amount on Venus constrained by a criterion of topographic‐greenhouse instability. Geophysical Research Letters, 24(3), 289–292.10.1029/96GL04006CrossRefGoogle Scholar

Klose, K.B., Wood, J.A. & Hashimoto, A. (1992). Mineral equilibria and the high radar reflectivity of Venus mountaintops. Journal of Geophysical Research: Planets, 97(E10), 16353–16369.10.1029/92JE01865CrossRefGoogle Scholar

Bullock, M.A. & Grinspoon, D.H. (2001). The recent evolution of climate on Venus. Icarus, 150(1), 19–37.10.1006/icar.2000.6570CrossRefGoogle Scholar

Solomon, S.C., Bullock, M.A. & Grinspoon, D.H. (1999). Climate change as a regulator of tectonics on Venus. Science, 286(5437), 87–90.10.1126/science.286.5437.87CrossRefGoogle ScholarPubMed

Anderson, F.S. & Smrekar, S.E. (1999). Tectonic effects of climate change on Venus. Journal of Geophysical Research: Planets, 104(E12), 30743–30756.10.1029/1999JE001082CrossRefGoogle Scholar

Phillips, R. J., Bullock, M.A. & Hauck, S.A. (2001). Climate and interior coupled evolution on Venus. Geophysical Research Letters, 28(9), 1779–1782.10.1029/2000GL011821CrossRefGoogle Scholar

Hoffman, P.F., Kaufman, A.J., Halverson, G.P. & Schrag, D.P. (1998). A Neoproterozoic snowball Earth. Science, 281(5381), 1342–1346.10.1126/science.281.5381.1342CrossRefGoogle ScholarPubMed

Hoffman, P.F. & Schrag, D.P. (2000). Snowball Earth. Scientific American, 282(1), 68–75.10.1038/scientificamerican0100-68CrossRefGoogle Scholar

Kirschvink, J.L., Late Proterozoic low-latitude global glaciation: the snowball Earth. In Schopf, J. et al. (Eds.), The Proterozoid Biosphere: A Multidisciplinary Study, Cambridge: Cambridge University Press, 1992.Google Scholar

Lorenz, R.D., McKay, C.P. & Lunine, J.I. (1997). Photochemically driven collapse of Titan’s atmosphere. Science, 275(5300), 642–644.10.1126/science.275.5300.642CrossRefGoogle ScholarPubMed

Lorenz, R.D., McKay, C.P. & Lunine, J.I. (1999). Analytic investigation of climate stability on Titan: sensitivity to volatile inventory. Planetary and Space Science, 47(12), 1503–1515.10.1016/S0032-0633(99)00038-0CrossRefGoogle ScholarPubMed

Conway, E.M., Exploration and Engineering: The Jet Propulsion Laboratory and the Quest for Mars, Baltimore, MD: Johns Hopkins University Press, 2015.Google Scholar

Morton, O., Mapping Mars: Science, Imagination and the Birth of a World, New York: Picador, 2002.Google Scholar

Malin, M.C. & Edgett, K.S. (2000). Evidence for recent groundwater seepage and surface runoff on Mars. Science, 288(5475), 2330–2335.10.1126/science.288.5475.2330CrossRefGoogle ScholarPubMed

Del Genio, A.D., Zhou, W. & Eichler, T.P. (1993). Equatorial superrotation in a slowly rotating GCM: implications for Titan and Venus. Icarus, 101(1), 1–17.10.1006/icar.1993.1001CrossRefGoogle Scholar

Hourdin, F., Talagrand, O., Sadourny, R., et al. (1995). Numerical simulation of the general circulation of the atmosphere of Titan. Icarus, 117(2), 358–374.10.1006/icar.1995.1162CrossRefGoogle ScholarPubMed

Forget, F. & Pierrehumbert, R.T. (1997). Warming early Mars with carbon dioxide clouds that scatter infrared radiation. Science, 278(5341), 1273–1276.10.1126/science.278.5341.1273CrossRefGoogle ScholarPubMed

Yung, Y.L., Nair, H. & Gerstell, M.F. (1997). CO₂ greenhouse in the early Martian atmosphere: SO₂ inhibits condensation. Icarus, 130(1), 222–224.10.1006/icar.1997.5808CrossRefGoogle ScholarPubMed

Head, J.W., Hiesinger, H., Ivanov, M.A., et al. (1999). Possible ancient oceans on Mars: evidence from Mars Orbiter Laser Altimeter data. Science, 286(5447), 2134–2137.10.1126/science.286.5447.2134CrossRefGoogle ScholarPubMed

Smith, D.E., Zuber, M.T. & Neumann, G.A. (2001). Seasonal variations of snow depth on Mars. Science, 294(5549), 2141–2146.10.1126/science.1066556CrossRefGoogle ScholarPubMed

Ivanov, A.B. & Muhleman, D.O. (2001). Cloud reflection observations: results from the Mars Orbiter Laser Altimeter. Icarus, 154(1), 190–206.10.1006/icar.2001.6686CrossRefGoogle Scholar

McKay, D.S., Gibson, E.K., Thomas-Keprta, K.L., et al. (1996). Search for past life on Mars: possible relic biogenic activity in Martian meteorite ALH84001. Science, 273(5277), 924–930.10.1126/science.273.5277.924CrossRefGoogle ScholarPubMed

Thomas-Keprta, K.L., Bazylinski, D.A., Kirschvink, J.L., et al. (2000). Elongated prismatic magnetite crystals in ALH84001 carbonate globules: potential Martian magnetofossils. Geochimica et Cosmochimica Acta, 64(23), 4049–4081.10.1016/S0016-7037(00)00481-6CrossRefGoogle ScholarPubMed

Connerney, J.E.P., Acuna, M.H., Wasilewski, P.J., et al. (1999). Magnetic lineations in the ancient crust of Mars. Science, 284(5415), 794–798.10.1126/science.284.5415.794CrossRefGoogle ScholarPubMed

Allen, D.A. & Crawford, J.W. (1984). Cloud structure on the dark side of Venus. Nature, 307, 222–224.10.1038/307222a0CrossRefGoogle Scholar

Crisp, D., Allen, D.A., Grinspoon, D.H. & Pollack, J.B. (1991). The dark side of Venus: near-infrared images and spectra from the Anglo-Australian Observatory. Science, 253(5025), 1263–1266.10.1126/science.11538493CrossRefGoogle ScholarPubMed

Lemmon, M.T., Karkoschka, E. & Tomasko, M. (1993). Titan’s rotation: surface feature observed. Icarus, 103(2), 329–332.10.1006/icar.1993.1074CrossRefGoogle Scholar

Smith, P.H., Lemmon, M.T., Lorenz, R.D., et al. (1996). Titan’s surface, revealed by HST imaging. Icarus, 119(2), 336–349.10.1006/icar.1996.0023CrossRefGoogle Scholar

Lorenz, R.D., Lemmon, M.T., Smith, P.H. & Lockwood, G.W. (1999). Seasonal change on Titan observed with the Hubble Space Telescope WFPC-2. Icarus, 142(2), 391–401.10.1006/icar.1999.6225CrossRefGoogle Scholar

Griffith, C.A., Owen, T., Miller, G.A. & Geballe, T. (1998). Transient clouds in Titan’s lower atmosphere. Nature, 395(6702), 575–578.10.1038/26920CrossRefGoogle ScholarPubMed

Griffith, C.A., Hall, J.L. & Geballe, T.R. (2000). Detection of daily clouds on Titan. Science, 290(5491), 509–513.10.1126/science.290.5491.509CrossRefGoogle ScholarPubMed

Lorenz, R. & Mitton, J., Lifting Titan’s Veil, Cambridge: Cambridge University Press, 2002.Google Scholar

Brown, M.E., Bouchez, A.H. & Griffith, C.A. (2002). Direct detection of variable tropospheric clouds near Titan’s south pole. Nature, 420(6917), 795–797.10.1038/nature01302CrossRefGoogle ScholarPubMed

Roe, H.G., De Pater, I., Macintosh, B.A. & McKay, C.P. (2002). Titan’s clouds from Gemini and Keck adaptive optics imaging. The Astrophysical Journal, 581(2), 1399.10.1086/344403CrossRefGoogle Scholar

Lorenz, R.D., Griffith, C.A., Lunine, J.I., McKay, C.P. & Rennò, N.O. (2005). Convective plumes and the scarcity of Titan’s clouds. Geophysical Research Letters, 32(1) L01201.10.1029/2004GL021415CrossRefGoogle Scholar

Roe, H.G., Brown, M.E., Schaller, E.L., Bouchez, A.H. & Trujillo, C.A. (2005). Geographic control of Titan’s mid-latitude clouds. Science, 310(5747), 477–479.10.1126/science.1116760CrossRefGoogle ScholarPubMed

Harland, D.M. & Lorenz, R.D., Space Systems Failures, Springer, 2006.Google Scholar

Boynton, W.V., Bailey, S.H., Hamara, D.K, et al. (2001). Thermal and evolved gas analyzer: part of the Mars volatile and climate surveyor integrated payload. Journal of Geophysical Research: Planets, 106(E8), 17683–17698.10.1029/1999JE001153CrossRefGoogle Scholar

Nye, J.F., Durham, W.B., Schenk, P.M. & Moore, J.M. (2000). The instability of a south polar cap on Mars composed of carbon dioxide. Icarus, 144(2), 449–455.CrossRefGoogle Scholar

Lorenz, R.D., Young, E.F. & Lemmon, M.T. (2001). Titan’s smile and collar: HST observations of seasonal change 1994–2000. Geophysical Research Letters, 28(23), 4453–4456.10.1029/2001GL013728CrossRefGoogle Scholar

Lorenz, R.D., Lemmon, M.T. & Smith, P.H. (2006). Seasonal evolution of Titan’s dark polar hood: midsummer disappearance observed by the Hubble Space Telescope. Monthly Notices of the Royal Astronomical Society, 369(4), 1683–1687.10.1111/j.1365-2966.2006.10405.xCrossRefGoogle Scholar

Yung, Y.L. (1987). An update of nitrile photochemistry on Titan. Icarus, 72(2), 468–472.10.1016/0019-1035(87)90186-2CrossRefGoogle ScholarPubMed

Samuelson, R.E., Nath, N.R. & Borysow, A. (1997). Gaseous abundances and methane supersaturation in Titan’s troposphere. Planetary and Space Science, 45(8), 959–980.10.1016/S0032-0633(97)00090-1CrossRefGoogle Scholar

Samuelson, R.E. & Mayo, L.A. (1997). Steady-state model for methane condensation in Titan’s troposphere. Planetary and Space Science, 45(8), 949–958.10.1016/S0032-0633(97)00089-5CrossRefGoogle Scholar

Lorenz, R.D., Lunine, J.I., Withers, P.G. & McKay, C.P. (2001). Titan, Mars and Earth: entropy production by latitudinal heat transport. Geophysical Research Letters, 28(3), 415–418.CrossRefGoogle Scholar

Kleidon, A. & Lorenz, R.D.. Non-equilibrium Thermodynamics and the Production of Entropy: Life, Earth, and Beyond. Springer Science & Business Media, 2005.10.1007/b12042CrossRefGoogle Scholar

Dewar, R. (2003). Information theory explanation of the fluctuation theorem, maximum entropy production and self-organized criticality in non-equilibrium stationary states. Journal of Physics A: Mathematical and General, 36(3), 631.10.1088/0305-4470/36/3/303CrossRefGoogle Scholar

Goody, R. (2007). Maximum entropy production in climate theory. Journal of the Atmospheric Sciences, 64(7), 2735–2739.10.1175/JAS3967.1CrossRefGoogle Scholar

Jupp, T.E. & Cox, P.M. (2010). MEP and planetary climates: insights from a two-box climate model containing atmospheric dynamics. Philosophical Transactions of the Royal Society B: Biological Sciences, 365(1545), 1355–1365.10.1098/rstb.2009.0297CrossRefGoogle ScholarPubMed

Shimokawa, S. & Ozawa, H. (2001). On the thermodynamics of the oceanic general circulation: entropy increase rate of an open dissipative system and its surroundings. Tellus A, 53(2), 266–277.10.3402/tellusa.v53i2.12185CrossRefGoogle Scholar

Hoffman, N. (2000). White Mars: a new model for Mars’ surface and atmosphere based on CO₂. Icarus, 146(2), 326–342.10.1006/icar.2000.6398CrossRefGoogle Scholar

Lanagan, P.D., McEwen, A.S., Keszthelyi, L.P. & Thordarson, T. (2001). Rootless cones on Mars indicating the presence of shallow equatorial ground ice in recent times. Geophysical Research Letters, 28(12), 2365–2367.10.1029/2001GL012932CrossRefGoogle Scholar

Malin, M.C., Caplinger, M.A. & Davis, S.D. (2001). Observational evidence for an active surface reservoir of solid carbon dioxide on Mars. Science, 294(5549), 2146–2148.10.1126/science.1066416CrossRefGoogle ScholarPubMed

Byrne, S. & Ingersoll, A.P. (2003). A sublimation model for Martian south polar ice features. Science, 299(5609), 1051–1053.10.1126/science.1080148CrossRefGoogle ScholarPubMed

Byrne, S. (2009). The polar deposits of Mars. Annual Review of Earth and Planetary Sciences, 37, 535–560.10.1146/annurev.earth.031208.100101CrossRefGoogle Scholar

Boynton, W.V., et al. (2002). Distribution of hydrogen in the near surface of Mars: evidence for subsurface ice deposits. Science, 297(5578), 81–85.10.1126/science.1073722CrossRefGoogle ScholarPubMed

Feldman, W.C., Boynton, W.V., Tokar, R.L., et al. (2002). Global distribution of neutrons from Mars: results from Mars Odyssey. Science, 297(5578), 75–78.10.1126/science.1073541CrossRefGoogle ScholarPubMed

Pillinger, C.T., with Sims, M.R. & Clemmet, S., The Guide to Beagle 2. London: Faber and Faber, 2003.Google Scholar

Head, J.W., Neukum, G., Jaumann, R., et al. (2005). Tropical to mid-latitude snow and ice accumulation, flow and glaciation on Mars. Nature, 434(7031), 346–351.10.1038/nature03359CrossRefGoogle ScholarPubMed

Formisano, V., Atreya, S., Encrenaz, T., Ignatiev, N. & Giuranna, M. (2004). Detection of methane in the atmosphere of Mars. Science, 306(5702), 1758–1761.10.1126/science.1101732CrossRefGoogle ScholarPubMed

Mumma, M.J., Villanueva, G.L., Novak, R.E., et al. (2009). Strong release of methane on Mars in northern summer 2003. Science, 323(5917), 1041–1045.10.1126/science.1165243CrossRefGoogle ScholarPubMed

Krasnopolsky, V.A., Maillard, J.P. & Owen, T.C. (2004). Detection of methane in the Martian atmosphere: evidence for life? Icarus, 172(2), 537–547.10.1016/j.icarus.2004.07.004CrossRefGoogle Scholar

Zahnle, K., Freedman, R.S. & Catling, D.C. (2011). Is there methane on Mars? Icarus, 212(2), 493–503.CrossRefGoogle Scholar

Lefevre, F. & Forget, F. (2009). Observed variations of methane on Mars unexplained by known atmospheric chemistry and physics. Nature, 460(7256), 720–723.10.1038/nature08228CrossRefGoogle Scholar

Pavlov, A.A., Kasting, J.F., Brown, L.L., Rages, K.A. & Freedman, R. (2000). Greenhouse warming by CH₄ in the atmosphere of early Earth. Journal of Geophysical Research: Planets, 105(E5), 11981–11990.10.1029/1999JE001134CrossRefGoogle ScholarPubMed

Trainer, M.G., Pavlov, A.A., DeWitt, H.L., et al. (2006). Organic haze on Titan and the early Earth. Proceedings of the National Academy of Sciences, 103(48), 18035–18042.10.1073/pnas.0608561103CrossRefGoogle ScholarPubMed

Kass, D.M., Schofield, J.T., Michaels, T.I., et al. (2003). Analysis of atmospheric mesoscale models for entry, descent, and landing. Journal of Geophysical Research: Planets, 108(E12).10.1029/2003JE002065CrossRefGoogle Scholar

Squyres, S.W., Arvidson, R.E., Bell, J.F., et al. (2004). The Opportunity Rover’s Athena science investigation at Meridiani Planum, Mars. Science, 306(5702), 1698–1703.10.1126/science.1106171CrossRefGoogle ScholarPubMed

Morris, R.V., Ruff, S.W., Gellert, R., et al. (2010). Identification of carbonate-rich outcrops on Mars by the Spirit rover. Science, 329(5990), 421–424.10.1126/science.1189667CrossRefGoogle ScholarPubMed

Ruff, S.W., Farmer, J.D., Calvin, W.M., et al. (2011). Characteristics, distribution, origin, and significance of opaline silica observed by the Spirit rover in Gusev crater, Mars. Journal of Geophysical Research: Planets, 116(E7), doi:10.1029/2010JE003767.CrossRefGoogle Scholar

Lorenz, R.D. (2009). Power law of dust devil diameters on Earth and Mars. Icarus, 203, 683–684.10.1016/j.icarus.2009.06.029CrossRefGoogle Scholar

Lorenz, R.D. & Reiss, D. (2014). Solar panel clearing events, dust devil tracks, and in-situ vortex detections on Mars. Icarus, 248, 162–164.10.1016/j.icarus.2014.10.034CrossRefGoogle ScholarPubMed

Lemmon, M.T., Wolff, M.J., Bell, J.F., et al. (2015). Dust aerosol, clouds, and the atmospheric optical depth record over 5 Mars years of the Mars Exploration Rover mission. Icarus, 251, 96–111.10.1016/j.icarus.2014.03.029CrossRefGoogle Scholar

Lorenz, R.D., Lemmon, M.T. & Smith, P.H. (2006). Seasonal evolution of Titan’s dark polar hood: midsummer disappearance observed by the Hubble Space Telescope. Monthly Notices of the Royal Astronomical Society, 369(4), 1683–1687.10.1111/j.1365-2966.2006.10405.xCrossRefGoogle Scholar

Lorenz, R.D., Smith, P.H. & Lemmon, M.T. (2004). Seasonal change in Titan’s haze 1992–2002 from Hubble Space Telescope observations. Geophysical Research Letters, 31(10).10.1029/2004GL019864CrossRefGoogle Scholar

Marten, A., Hidayat, T., Biraud, Y. & Moreno, R. (2002). New millimeter heterodyne observations of Titan: vertical distributions of nitriles HCN, HC₃N, CH₃CN, and the isotopic ratio ¹⁵N/¹⁴N in its atmosphere. Icarus, 158(2), 532–544.10.1006/icar.2002.6897CrossRefGoogle Scholar

Rannou, P., Hourdin, F. & McKay, C.P. (2002). A wind origin for Titan’s haze structure. Nature, 418(6900), 853–856.10.1038/nature00961CrossRefGoogle ScholarPubMed

Kostiuk, T., Livengood, T.A., Hewagama, T., et al. (2005). Titan’s stratospheric zonal wind, temperature, and ethane abundance a year prior to Huygens insertion. Geophysical Research Letters, 32(22), doi:10.1029/2005GL023897.CrossRefGoogle Scholar

Tokano, T. & Neubauer, F.M. (2002). Tidal winds on Titan caused by Saturn. Icarus, 158(2), 499–515.10.1006/icar.2002.6883CrossRefGoogle Scholar

Tokano, T., Molina-Cuberos, G.J., Lammer, H. & Stumptner, W. (2001). Modelling of thunderclouds and lightning generation on Titan. Planetary and Space Science, 49(6), 539–560.10.1016/S0032-0633(00)00170-7CrossRefGoogle Scholar

Lorenz, R.D. (2000). The weather on Titan. Science, 290(5491), 467–468.10.1126/science.290.5491.467CrossRefGoogle ScholarPubMed

Lorenz, R.D., Griffith, C.A., Lunine, J.I., McKay, C.P. & Rennò, N.O. (2005). Convective plumes and the scarcity of Titan’s clouds. Geophysical Research Letters, 32(1), doi:10.1029/2004GL021415/.CrossRefGoogle Scholar

Awal, M. & Lunine, J.I. (1994). Moist convective clouds in Titan’s atmosphere. Geophysical Research Letters, 21(23), 2491–2494.10.1029/94GL01707CrossRefGoogle Scholar

Ou, H.W. (2001). Possible bounds on the Earth’s surface temperature: from the perspective of a conceptual global-mean model. Journal of Climate, 14(13), 2976–2988.10.1175/1520-0442(2001)014<2976:PBOTES>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Rosing, M.T., Bird, D.K., Sleep, N.H. & Bjerrum, C.J. (2010). No climate paradox under the faint early Sun. Nature, 464(7289), 744–747.10.1038/nature08955CrossRefGoogle ScholarPubMed

Goldblatt, C. & Zahnle, K. (2011). Faint young Sun paradox remains. Nature, 474(7349), E1.10.1038/nature09961CrossRefGoogle Scholar

Goldblatt, C. & Zahnle, K. (2011). Clouds and the faint young Sun paradox. Climate of the Past, 7, 203–220.10.5194/cp-7-203-2011CrossRefGoogle Scholar

Pierrehumbert, R.T. (1995). Thermostats, radiator fins, and the local runaway greenhouse. Journal of the Atmospheric Sciences, 52(10), 1784–1806.10.1175/1520-0469(1995)052<1784:TRFATL>2.0.CO;22.0.CO;2>CrossRefGoogle Scholar

Lindzen, R.S., Chou, M.D. & Hou, A.Y. (2001). Does the Earth have an adaptive infrared iris? Bulletin of the American Meteorological Society, 82(3), 417–432.10.1175/1520-0477(2001)082<0417:DTEHAA>2.3.CO;22.3.CO;2>CrossRefGoogle Scholar

Rondanelli, R. & Lindzen, R.S. (2010). Can thin cirrus clouds in the tropics provide a solution to the faint young Sun paradox? Journal of Geophysical Research: Atmospheres, 115(D2).10.1029/2009JD012050CrossRefGoogle Scholar

Hartmann, D.L. & Michelsen, M.L. (2002). No evidence for iris. Bulletin of the American Meteorological Society, 83(2), 249–254.2.3.CO;2>CrossRefGoogle Scholar

Roderick, M.L. & Farquhar, G.D. (2002). The cause of decreased pan evaporation over the past 50 years. Science, 298(5597), 1410–1411.10.1126/science.1075390-aCrossRefGoogle ScholarPubMed

Ohmura, A. & Wild, M. (2002). Is the hydrological cycle accelerating? Science, 298, 1345–1346.10.1126/science.1078972CrossRefGoogle Scholar

Brutsaert, W. & Parlange, M.B. (1998). Hydrologic cycle explains the evaporation paradox. Nature, 396(6706), 30.10.1038/23845CrossRefGoogle Scholar

Travis, D.J., Carleton, A.M. & Lauritsen, R.G. (2002). Climatology: contrails reduce daily temperature range. Nature, 418(6898), 601–601.10.1038/418601aCrossRefGoogle Scholar

Kalkstein, A.J. & Balling, R.C. (2004). Impact of unusually clear weather on United States daily temperature range following 9/11/2001. Climate Research, 26(1), 1–4.10.3354/cr026001CrossRefGoogle Scholar

Dietmüller, S., Ponater, M., Sausen, R., Hoinka, K.P. & Pechtl, S. (2008). Contrails, natural clouds, and diurnal temperature range. Journal of Climate, 21(19), 5061–5075.10.1175/2008JCLI2255.1CrossRefGoogle Scholar

Porco, C.C., Baker, E., Barbara, J., et al. (2005). Imaging of Titan from the Cassini spacecraft. Nature, 434(7030), 159–168.10.1038/nature03436CrossRefGoogle ScholarPubMed

Turtle, E.P., Perry, J.E., McEwen, A.S., et al. (2009). Cassini imaging of Titan’s high‐latitude lakes, clouds, and south‐polar surface changes. Geophysical Research Letters, 36(2), doi/10.1029/2008GL036186.CrossRefGoogle Scholar

Griffith, C.A., Penteado, P., Baines, K., et al. (2005). The evolution of Titan’s mid-latitude clouds. Science, 310(5747), 474–477.10.1126/science.1117702CrossRefGoogle ScholarPubMed

Elachi, C., et al. (2005). Cassini radar views the surface of Titan. Science, 308(5724), 970–974.10.1126/science.1109919CrossRefGoogle ScholarPubMed

Lorenz, R.D., Lopes, R.M., Paganelli, F., et al. (2008). Fluvial channels on Titan: initial Cassini RADAR observations. Planetary and Space Science, 56(8), 1132–1144.10.1016/j.pss.2008.02.009CrossRefGoogle Scholar

Lorenz, R. and Mitton, J., Titan Unveiled, Princeton University Press, 2008 (revised edition 2010).Google Scholar

Tomasko, M.G., Archinal, B. & Becker, T. (2005). Rain, winds and haze during the Huygens probe’s descent to Titan’s surface. Nature, 438(7069), 765–778.10.1038/nature04126CrossRefGoogle ScholarPubMed