Innumerable Globes Like This One?

Total Page:16

File Type:pdf, Size:1020Kb

Innumerable Globes Like This One? books & arts Innumerable globes like this one? How to Find a formation of the solar system and the observation. Early chapters describe Habitable Planet distribution and redistribution of volatile current methods of observation, which materials provided the Earth with its have predominantly identified large by James Kasting current inventory of water. Tectonic activity worlds orbiting close to their stars. cycles water between the lithosphere and Subsequent chapters discuss the future PRINCETON UNIV. the surface environment, and maintains the of exoplanet research: direct imaging PRESS: 2010. 360PP. carbonate–silicate cycle — a key feedback and spectroscopy could yield evidence £20.95 on greenhouse warming. Solar radiation of habitable conditions and even life. provides energy to warm the planet’s These final chapters bring the book full surface. And the atmosphere — with a circle, linking the information accessible composition continually influenced by through astronomy to the basic stellar, geology, biology and photochemistry — orbital, planetary and atmospheric factors here is a single general space, provides sufficient surface pressure and that determine habitability. “ a single vast immensity which greenhouse warming to keep water in Twe may freely call Void; in it are its liquid form. Kasting explains these innumerable globes like this one on which processes in detail, individually and in Venus (too hot) and Mars we live and grow.” their complex interactions, as he tracks (too cold) are cautionary So wrote the Dominican friar and them across the evolution of the Sun– philosopher Giordano Bruno in De Earth system. tales for worlds aspiring L’infinito Universo et Mondi, in 1584. A If Earth is ‘just right’, Venus (too hot) to habitability. quarter of a century later — ten years after and Mars (too cold) are cautionary tales Bruno was burned at the stake for this and for worlds aspiring to habitability. In other heresies — Galileo made the first the second section, ‘Limits to Planetary The book should appeal to professional telescopic observations of other planets Habitability’, the climate histories of these and armchair scientists alike. Material in our solar system. Today, more than 450 worlds are used to exemplify the processes is presented as if to a class of non- planets have been detected around other that define the inner and outer reaches of specialist undergraduate scientists. A stars. Although these globes are decidedly the ‘continuously habitable zone’. Venus’s modest familiarity with maths, physics unlike the one on which we live and grow, proximity to the sun induced a runaway and chemistry will suffice to unlock most exoplanet astronomers are setting their greenhouse effect that led to the loss of the of the book’s content, and consistent sights on the detection of habitable, and planet’s water, and the development of the attention is paid to explaining more possibly inhabited, worlds. hellish conditions that prevail at its surface challenging concepts in simple terms. In How to Find a Habitable Planet, today. Mars may have begun its history But the book also frequently touches geoscientist and astrobiologist with liquid water at the surface, but the loss on the primary literature — including James Kasting explores the science of its atmosphere over time eliminated the Kasting’s own seminal contributions to behind this emerging phase of exoplanet potential for a strong greenhouse effect; modelling planetary atmospheres — and discovery. A blend of biogeochemistry, essential for keeping the planet warm thereby provides detail for those interested planetary science and astronomy, the book owing to the lower levels of solar radiation in a deeper account of the subject matter. examines the factors and processes that it receives. Given the broad-ranging subject matter yield habitable conditions, and the methods In a prelude to the book’s final section and up-to-date account of the state of that astronomers will use to search for we learn that early searches for inhabited exoplanet science, all but those closest habitable and inhabited worlds beyond our exoplanets will probably focus on stars to the field — and perhaps even many solar system. Kasting’s wealth of first-hand of similar mass to the Sun. Planets in it — will find it difficult not to learn experience — as a researcher focused on around low mass (dim) stars would have something new. the evolution of planetary atmospheres to maintain close orbits to intercept Written in a clear and often and as the chair of NASA’s Exoplanet sufficient radiation to keep warm. As conversational style — and infused Exploration Program Analysis Group — a result, they would become tidally throughout with Kasting’s personal makes for authoritative writing across the locked — like our moon — potentially optimism regarding the existence of, full range of topics covered. causing any volatiles to freeze out on the and our ability to detect, habitable and Following a brief foray into the history permanently dark side of the planet. At inhabited worlds beyond our own — this of thought concerning life on other planets, the opposite end of the spectrum, massive is an informative and worthwhile read for Kasting explores the science of habitability stars emit high-energy radiation that may anyone who looks to the stars and wonders and the methodology of exoplanet be difficult for life to handle. They also if there is anybody out there. ❐ astronomy in three well-integrated sections. burn out quickly, leaving little time for life The interacting factors and processes that to develop. REVIEWED BY TORI M. HOEHLER have endowed the Earth with liquid water The final section, ‘How to Find Another Tori M. Hoehler is in the Exobiology Branch, NASA at the surface — the book’s key metric of Earth’, combines lessons learned in Ames Research Center, Mail Stop 239-4, Moffett habitability — are discussed in the first habitability with the basics of astronomy Field, California 94035, USA. section: ‘Our Habitable Planet Earth’. The to explore the methodology of exoplanet e-mail: [email protected] NATURE GEOSCIENCE | VOL 3 | JULY 2010 | www.nature.com/naturegeoscience 447 © 2010 Macmillan Publishers Limited. All rights reserved.
Recommended publications
  • Snowball Earth: a Thin-Ice Solution with Flowing Sea Glaciers’’ by David Pollard and James F
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 111, C09016, doi:10.1029/2005JC003411, 2006 Click Here for Full Article Comment on ‘‘Snowball Earth: A thin-ice solution with flowing sea glaciers’’ by David Pollard and James F. Kasting Stephen G. Warren1,2 and Richard E. Brandt1 Received 22 November 2005; revised 22 May 2006; accepted 9 June 2006; published 14 September 2006. Citation: Warren, S. G., and R. E. Brandt (2006), Comment on ‘‘Snowball Earth: A thin-ice solution with flowing sea glaciers’’ by David Pollard and James F. Kasting, J. Geophys. Res., 111, C09016, doi:10.1029/2005JC003411. 1. Introduction 2. Choices of Model Variables That Favor [1] Pollard and Kasting [2005] (hereinafter referred to as Thin Ice PK) have coupled an energy-balance climate model to an 2.1. Albedo of Cold Glacier Ice ice-shelf flow model, to investigate the Snowball Earth [2] As sea glaciers flowed equatorward into the tropical episodes of the Neoproterozoic, 600–800 million years region of net sublimation, their surface snow and subsurface ago, when the ocean apparently froze all the way to the firn would sublimate away, exposing bare glacier ice to equator [Hoffman and Schrag, 2002]. PK’s particular con- the atmosphere and solar radiation. This ice would be cern was to investigate the possibility that over a wide freshwater (meteoric) ice, which originated from compres- equatorial band where sublimation exceeded snowfall, the sion of snow, so it would contain numerous bubbles, giving bare ice may have been thin enough to permit transmission a high albedo. The albedo of cold (nonmelting) glacier ice of sunlight to the water below, providing an extensive exposed by sublimation (Antarctic ‘‘blue ice’’) has been refugium for the photosynthetic eukaryotes that survived measured as 0.55–0.65 in four experiments in the Atlantic the Snowball events.
    [Show full text]
  • Habitable Zone
    How to Find a Habitable Planet James Kasting Department of Geosciences Penn State University The search for other habitable worlds is ancient “There are infinite worlds both like and unlike this world of ours...”--- Epicurus (c. 300 BCE) (died painfully 269 BCE) “… false and "There are countless suns and damnable ...” countless earths …” G. Galilei (b. 1564) Giordano Bruno (b. 1584) in De L'infinito Universo E Mondi From Mike Devirian, (life imprisonment JPL (burned at the stake in Campo 1633) dei Fiore, Rome, 1600) • Even today, opinions differ widely as to whether other Earth-like planets exist… The Gaia hypothesis First presented in the 1970s by James Lovelock 1979 1988 http://www.ecolo.org/lovelock Gaia—The Greek goddess • According to this hypothesis, life creates and maintains conditions for its own existence by stabilizing Earth’s climate and other aspects of the Earth system • If this idea is correct, then only planets that are already inhabited would be habitable http://www.paleothea.com/Majors.html The Medea and Rare Earth hypotheses Peter Ward 2009 2000 Medea hypothesis: Life is harmful to the Earth! Rare Earth hypothesis: Complex life (animals, including humans) is rare in the universe The latest addition to this literature Me My new book (Princeton University Press, 2010) • As you will see, I am more optimistic than either Peter Ward or Jim Lovelock Talk outline • Introduction (which you heard already) • Part 1: What makes Earth unique, and what is life? • Part 2: Can we find Earth-like planets around other stars, and can
    [Show full text]
  • NASA Astrobiology Institute 2018 Annual Science Report
    A National Aeronautics and Space Administration 2018 Annual Science Report Table of Contents 2018 at the NAI 1 NAI 2018 Teams 2 2018 Team Reports The Evolution of Prebiotic Chemical Complexity and the Organic Inventory 6 of Protoplanetary Disk and Primordial Planets Lead Institution: NASA Ames Research Center Reliving the Past: Experimental Evolution of Major Transitions 18 Lead Institution: Georgia Institute of Technology Origin and Evolution of Organics and Water in Planetary Systems 34 Lead Institution: NASA Goddard Space Flight Center Icy Worlds: Astrobiology at the Water-Rock Interface and Beyond 46 Lead Institution: NASA Jet Propulsion Laboratory Habitability of Hydrocarbon Worlds: Titan and Beyond 60 Lead Institution: NASA Jet Propulsion Laboratory The Origins of Molecules in Diverse Space and Planetary Environments 72 and Their Intramolecular Isotope Signatures Lead Institution: Pennsylvania State University ENIGMA: Evolution of Nanomachines in Geospheres and Microbial Ancestors 80 Lead Institution: Rutgers University Changing Planetary Environments and the Fingerprints of Life 88 Lead Institution: SETI Institute Alternative Earths 100 Lead Institution: University of California, Riverside Rock Powered Life 120 Lead Institution: University of Colorado Boulder NASA Astrobiology Institute iii Annual Report 2018 2018 at the NAI In 2018, the NASA Astrobiology Program announced a plan to transition to a new structure of Research Coordination Networks, RCNs, and simultaneously planned the termination of the NASA Astrobiology Institute
    [Show full text]
  • The Lick-Carnegie Exoplanet Survey: a 3.1 M Earth Planet in The
    The Lick-Carnegie Exoplanet Survey: A 3.1 M⊕ Planet in the Habitable Zone of the Nearby M3V Star Gliese 581 Steven S. Vogt1, R. Paul Butler2, E. J. Rivera1, N. Haghighipour3, Gregory W. Henry4, and Michael H. Williamson4 Received ; accepted arXiv:1009.5733v1 [astro-ph.EP] 29 Sep 2010 1UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 2Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015-1305 3Institute for Astronomy and NASA Astrobiology Institute, University of Hawaii-Manoa, Honolulu, HI 96822 4Tennessee State University, Center of Excellence in Information Systems, 3500 John A. Merritt Blvd., Box 9501, Nashville, TN. 37209-1561 –2– ABSTRACT We present 11 years of HIRES precision radial velocities (RV) of the nearby M3V star Gliese 581, combining our data set of 122 precision RVs with an ex- isting published 4.3-year set of 119 HARPS precision RVs. The velocity set now indicates 6 companions in Keplerian motion around this star. Differential photometry indicates a likely stellar rotation period of ∼ 94 days and reveals no significant periodic variability at any of the Keplerian periods, supporting planetary orbital motion as the cause of all the radial velocity variations. The combined data set strongly confirms the 5.37-day, 12.9-day, 3.15-day, and 67-day planets previously announced by Bonfils et al. (2005), Udry et al. (2007), and Mayor et al. (2009). The observations also indicate a 5th planet in the system, GJ 581f, a minimum-mass 7.0 M⊕ planet orbiting in a 0.758 AU orbit of period 433 days and a 6th planet, GJ 581g, a minimum-mass 3.1 M⊕ planet orbiting at 0.146 AU with a period of 36.6 days.
    [Show full text]
  • Habitability Models for Astrobiology
    Astrobiology, 21, 8. (August, 2021) DOI: 10.1089/ast.2020.2342 Habitability Models for Astrobiology Abel Méndez, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Edgard G. Rivera-Valentín, Lunar and Planetary Institute, USRA, Houston, Texas, USA Dirk Schulze-Makuch, Center for Astronomy and Astrophysics, Technische Universität Berlin, Berlin, Germany; German Research Centre for Geosciences, Section Geomicrobiology, Potsdam, Germany; Leibniz-Institute of Freshwater Ecology and Inland Fisheries, Stechlin, Germany. Justin Filiberto, Lunar and Planetary Institute, USRA, Houston, Texas, USA Ramses M. Ramírez, University of Central Florida, Department of Physics, Orlando, Florida, USA; Space Science Institute, Boulder, Colorado, USA. Tana E. Wood, USDA Forest Service International Institute of Tropical Forestry, San Juan, Puerto Rico, USA Alfonso Dávila, NASA Ames Research Center, Moffett Field, California, USA Chris McKay, NASA Ames Research Center, Moffett Field, California, USA Kevin N. Ortiz Ceballos, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Marcos Jusino-Maldonado, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Nicole J. Torres-Santiago, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA Guillermo Nery, Planetary Habitability Laboratory, University of Puerto Rico at Arecibo, Puerto Rico, USA René Heller, Max Planck Institute for Solar System Research; Institute for Astrophysics,
    [Show full text]
  • Planets Galore
    physicsworld.com Feature: Exoplanets Detlev van Ravenswaay/Science Photo Library Planets galore With almost 1700 planets beyond our solar system having been discovered, climatologists are beginning to sketch out what these alien worlds might look like, as David Appell reports And so you must confess Jupiters, black Jupiters or puffy Jupiters; there are David Appell is a That sky and earth and sun and all that comes to be hot Neptunes and mini-Neptunes; exo-Earths, science writer living Are not unique but rather countless examples of a super-Earths and eyeball Earths. There are planets in Salem, Oregon, class. that orbit pulsars, or dim red dwarf stars, or binary US, www. Lucretius, Roman poet and philosopher, from star systems. davidappell.com De Rerum Natura, Book II Astronomers are in heaven and planetary scien- tists have an entirely new zoo to explore. “This is the The only thing more astonishing than their diver- best time to be an exoplanetary astronomer,” says sity is their number. We’re talking exoplanets exoplanetary astronomer Jason Wright of Pennsyl- – planets around stars other than our Sun. And vania State University. “Things have really exploded they’re being discovered in Star Trek quantities: recently.” Proving the point is that a third of all 1692 as this article goes to press, and another 3845 abstracts at a recent meeting of the American Astro- unconfirmed candidates. nomical Society were related to exoplanets. The menagerie includes planets that are pink, This explosion is largely thanks to the Kepler space blue, brown or black. Some have been labelled hot observatory.
    [Show full text]
  • THE GEOCHEMICAL NEWS Quarterly Newsletter of the Geochemical Society
    THE GEOCHEMICAL NEWS Quarterly Newsletter of The Geochemical Society NUMBER 100 ISSN 0016-7010 JULY 1999 Digging for the Roots of Geochemistry 9th V.M. Goldschmidt Conference In this issue: Harvard University Cambridge, MA, U. S. A. August 22-27, 1999 Van der Weijden Retires..................................7 Digging for the Roots of Geochemistry..........10 Contact: In Memoriam - Werner Stumm......................16 When Did The Earth’s Atmosphere Become Stein B. Jacobsen Department of Earth and Planetary Sciences Oxic? A Reply.....................................20 Harvard University Meetings Calendar .........................................23 Cambridge MA 02138 U.S.A. GS Special Publications..................................26 Phone: 617-495-5233 GS Membership Application .........................27 Fax: 617-496-4387 E-mail: [email protected] (see page 5 for more information) 2 The Geochemical News #100, July 1999 THE GEOCHEMICAL SOCIETY The Geochemical Society is a nonprofit scientific society founded to encourage the application of chemistry to the solution of geologi- cal and cosmological problems. Membership is international and diverse in background, encompassing such fields as organic geochem- istry, high and low-temperature geochemistry, petrology, meteorit- ics, fluid-rock interaction, and isotope geochemistry. The Society produces a Special Publications Series, The Geochemical News OFFICERS - 1999 (this quarterly newsletter), the Reviews in Mineralogy and Geochem- istry Series (jointly with the Mineralogical Association of America), PRESIDENT Michael J. Drake, University of Arizona and the journal Geochimica et Cosmochimica Acta (jointly with the Meteoritical Society); grants the V.M. Goldschmidt, F.W. Clarke VICE PRESIDENT and Clair C. Patterson Awards, and, jointly with the European Michael F. Hochella, Jr., Virginia Polytechnic Institute Association of Geochemistry, the Geochemistry Fellows title; spon- sors the V.M.
    [Show full text]
  • Comparative Planetary Climate Studies a White Paper for the Planetary Sciences Decadal Survey
    Comparative Planetary Climate Studies A White Paper for the Planetary Sciences Decadal Survey David Grinspoon, Denver Museum of Nature & Science Mark Bullock, Southwest Research Institute James Kasting, Penn State University Janet Luhmann, University of California, Berkeley Peter Read, Oxford University Scot Rafkin, Southwest Research Institute Sanjay Limaye, University of Wisconsin Kevin McGouldrick, Denver Museum of Nature & Science Gordon Chin, NASA/Goddard Space Flight Center Samuel Gulkis, Jet Propulsion Laboratory Feng Tian, LASP, CU-Boulder Eric Chassefiere, CNRS Hakan Svedhem, ESTEC Kevin Baines, Jet Propulsion Laboratory 1 Introduction With a broad scientific consensus on the reality of anthropogenic climate change [1], and the recognized need for more research on the consequent magnitude, mechanisms and potential for future societal disruption, NASA’s crucial and highly visible role in our understanding of the Earth system has become increasingly clear. Much of the attention and discussion of this has focused on the obvious importance of remote sensing observations from Earth orbit and the further development of NASA-supported Earth science modeling efforts. It is the purpose of this White Paper to draw attention to, and summarize, the important role that planetary exploration, and research with a comparative planetology focus, have played and should continue to play in our understanding of climate, and climate change, on Earth. Venus is Earth’s closest planetary neighbor, and a near twin in terms of overall properties such as mass and size. Their bulk densities and inventories of carbon and nitrogen are similar, suggesting similar primordial volatile inventories. Mars, Earth’s next nearest neighbor, has surface conditions most closely resembling Earth’s and a wide range of meteorological and geological phenomena that are recognizable as variations on familiar terrestrial themes.
    [Show full text]
  • Comparative Planetary Climate Studies a White Paper for the Planetary Sciences Decadal Survey
    Comparative Planetary Climate Studies A White Paper for the Planetary Sciences Decadal Survey David Grinspoon, Denver Museum of Nature & Science Mark Bullock, Southwest Research Institute James Kasting, Penn State University Janet Luhmann, University of California, Berkeley Peter Read, Oxford University Scot Rafkin, Southwest Research Institute Sanjay Limaye, University of Wisconsin Kevin McGouldrick, Denver Museum of Nature & Science Gordon Chin, NASA/Goddard Space Flight Center Samuel Gulkis, Jet Propulsion Laboratory Feng Tian, LASP, CU-Boulder Eric Chassefiere, CNRS Hakan Svedhem, ESTEC Vikki Meadows, University of Washington 1 Introduction With a broad scientific consensus on the reality of anthropogenic climate change [1], and the recognized need for more research on the consequent magnitude, mechanisms and potential for future societal disruption, NASA’s crucial and highly visible role in our understanding of the Earth system has become increasingly clear. Much of the attention and discussion of this has focused on the obvious importance of remote sensing observations from Earth orbit and the further development of NASA-supported Earth science modeling efforts. It is the purpose of this White Paper to draw attention to, and summarize, the important role that planetary exploration, and research with a comparative planetology focus, have played and should continue to play in our understanding of climate, and climate change, on Earth. Venus is Earth’s closest planetary neighbor, and a near twin in terms of overall properties such as mass and size. Their bulk densities and inventories of carbon and nitrogen are similar, suggesting similar primordial volatile inventories. Mars, Earth’s next nearest neighbor, has surface conditions most closely resembling Earth’s and a wide range of meteorological and geological phenomena that are recognizable as variations on familiar terrestrial themes.
    [Show full text]
  • Carbon Dioxide on the Early Earth
    CARBON DIOXIDE ON THE EARLY EARTH JAMES C. G. WALKER Space Physics Research Laboratory, Department of Atmospheric and Oceanic Science, The University of Michigan, Ann Arbor, MI 48109, U.S.A. (Received 6 September; in revised form 10 December, 1985) Abstract. This paper uses arguments of geochemical mass balance to arrive at an estimate of the partial pressure of carbon dioxide in the terrestrial atmosphere very early in earth history. It appears that this partial pressure could have been as large as 10 bars. This large estimate depends on two key considerations. First, volatiles were driven out of the interior of the earth during the course of earth accretion or very shortly thereafter. This early degassing was a consequence of rapid accretion, which gave the young earth a hot and rapidly convecting interior. Second, the early earth lacked extensive, stable continental plat- forms on which carbon could be stored in the form of carbonate minerals for geologically significant periods of time. In the absence of continental platforms on the early earth, the earth's carbon must have been either in the atmosphere or ocean or in the form of shortlived sedimentary deposits on ephemeral sea floor. 1. Introduction A widely accepted scenario for the origin of the atmospheres of the inner planets holds that they were released from the planetary interiors rapidly and very early in the history of the solar system. As a completely separate matter it is also widely believed that the early earth lacked extensive, stable continental platforms. The implication of these two hypotheses for the history of carbon dioxide in earth's ocean and at- mosphere has not previously been explored.
    [Show full text]
  • Sulfate Aerosol Hazes and SO2 Gas As Constraints on Rocky Exoplanets’ Surface Liquid Water
    Draft version December 26, 2019 Typeset using LATEX twocolumn style in AASTeX62 Sulfate Aerosol Hazes and SO2 Gas as Constraints on Rocky Exoplanets' Surface Liquid Water Kaitlyn Loftus,1 Robin D. Wordsworth,1, 2 and Caroline V. Morley3 1Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02140, USA 2Harvard Paulson School of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02140, USA 3Department of Astronomy, University of Texas at Austin, Austin, TX 78712, USA ABSTRACT Despite surface liquid water's importance to habitability, observationally diagnosing its presence or absence on exoplanets is still an open problem. Inspired within the Solar System by the differing sulfur cycles on Venus and Earth, we investigate thick sulfate (H2SO4 {H2O) aerosol haze and high trace mixing ratios of SO2 gas as observable atmospheric features whose sustained existence is linked to the near-absence of surface liquid water. We examine the fundamentals of the sulfur cycle on a rocky planet with an ocean and an atmosphere in which the dominant forms of sulfur are SO2 gas and H2SO4 {H2O aerosols (as on Earth and Venus). We build a simple but robust model of the wet, oxidized sulfur cycle to determine the critical amounts of sulfur in the atmosphere-ocean system required for detectable levels of SO2 and a detectable haze layer. We demonstrate that for physically realistic ocean pH values (pH & 6) and conservative assumptions on volcanic outgassing, chemistry, and aerosol microphysics, surface liquid water reservoirs with greater than 10−3 Earth oceans are incompatible with a sustained observable H2SO4 {H2O haze layer and sustained observable levels of SO2.
    [Show full text]
  • Pinning Down the Habitable Zones of Different Stars
    Pinning Down the Habitable Zones of Professor James Kasting Different Stars PINNING DOWN THE HABITABLE ZONES OF DIFFERENT STARS One of life’s greatest mysteries is whether or not we are alone in the Universe. One way to find planets that could support life is by working out whether they lie in the ‘habitable zone’ of their parent star – a distance at which liquid water might exist on the surface. Professor Jim Kasting at Penn State University has been studying stars and the boundaries of their habitable zones for decades. More recently, he has been looking into how these boundaries can change with a phenomenon called climate limit cycling, which might occur on certain planets. The Habitable Zone most likely rocky planets within the habitable zones of their host stars. But exactly how Finding extra-terrestrial planets that may be we know whether or not water can exist on able to support life is one of the biggest goals a planet is a complicated question, with a in astronomy. Since life as we know it relies rich history. on water to survive, one of the requirements for finding potentially habitable worlds is Over twenty years ago, in 1993, Professor that liquid water must be able to exist on the Jim Kasting and his colleagues came up with planets’ surface. Life could exist on planets a model to place restrictions on where the with subsurface water, as well, but it would habitable zone could be for certain planets. be difficult to detect remotely, and so is of ‘I derived estimates for the boundaries of less interest to astronomers.
    [Show full text]