Three JPL Concepts Picked in Discovery's First Round

Total Page:16

File Type:pdf, Size:1020Kb

Three JPL Concepts Picked in Discovery's First Round OCTOBER Jet Propulsion 2015 Laboratory VOLUME 45 NUMBER 10 Three JPL concepts picked in Discovery’s first round By Franklin O’Donnell JPL’s Discovery Program proposals are (from left) NEOCam, Psyche and VERITAS. Significant good news for JPL ar- would map the planet with a radar “As more and more exoplanets are rived at the end of September when vastly more capable than that on discovered, this information is essen- NASA announced the selection of JPL’s Magellan mission of the ear- tial to predicting whether Earth-sized three mission concepts managed by ly 1990s. The mission would obtain planets are more likely to resemble the Lab for possible development un- global maps of high-resolution radar Earth or Venus.” der the agency’s Discovery Program. imaging and altimetry, and make other Tony Freeman was the VERITAS The three proposals – a Venus or- measurements designed to penetrate capture lead for Step 1. Dave Leh- biter, a mission to a metal asteroid Venus’ thick carbon dioxide atmo- man of JPL is project manager, Scott and a space telescope to search sphere. Hensley is the project scientist, and for more near-Earth asteroids – are JPL planetary scientist Sue Smrek- Leon Alkalai will be the capture lead among five concepts that NASA will ar, VERITAS principal investigator, for Phase A. Lockheed Martin would fund for further concept design stud- said the mission is designed to reveal be the spacecraft contractor. VERI- ies during the coming year. In Sep- Venus’ geologic history, determine TAS stands for Venus Emissivity, Ra- tember 2016, the agency expects to how active it is, and search for the dio Science, InSAR, Topography And pick one or two for final development fingerprints of past and present water. Spectroscopy. for flight. “The overarching question is, ‘How The huge metal asteroid Psyche The Venus orbiter, called VERITAS, Earthlike is Venus?’” said Smrekar. Continued on page 2 2 JPL CONCEPTS PICKED Continued from page 1 is the destination for the second se- Earth – perhaps yielding 10 times NEOCam is being shepherded by the lected JPL proposal. Also known as more near-Earth objects than all dis- Lab’s Astronomy, Physics and Space Universe Psyche, this spacecraft would use covered to date. Technology Directorate (7X). ion propulsion to reach and orbit the NEOCam builds on JPL principal “NEOCam is a solar system mis- 250-kilometer-wide object that circles investigator Amy Mainzer’s previous sion observing solar system objects, the sun in the main asteroid belt be- mission, the Wide-field Infrared Sur- but because of 7X’s involvement with tween Mars and Jupiter. Discovered in vey Explorer, which found 34,000 space telescopes it made sense for 1852, Psyche is unusual for its compo- asteroids and 135 near-Earth objects. us to develop this proposal,” said sition later found to be 90 percent iron The new space telescope would have Roger Lee, deputy manager of 7X’s and nickel, making it the largest metal a larger diameter and would feature a Astrophysics and Heliophysics For- asteroid ever identified. much wider field of view. mulation Office. According to the mission’s princi- Following launch, NEOCam would “All of these proposals have ben- pal investigator, Lindy Elkins-Tanton be stationed at the L1 Lagrange point efited from hard work, innovative so- of Arizona State University in Tempe, between Earth and the sun. That lutions and development approaches Psyche could be the remnant of a location provides a stable, cold en- in many offices across JPL, including massive collision in the early solar vironment allowing the infrared tele- the Foundry and 3X, that contributed “JPL’s representation in these selections is a very strong reflection of the quality of proposal work at the Lab and our success in teaming with science investigators,” said JPL Director Charles Elachi. system that stripped the mantle from a scope to function for many years significant content and technical re- protoplanet then forming, leaving only without the need for cryocoolers. view,” said Kim Reh, deputy manager its metal core. “Everyone wants to know about of 4X’s Solar System Mission Formu- Because the asteroid is so unusual, asteroids hitting Earth,” said Mainzer. lation Office. Elkins-Tanton said her mission con- “NEOCam is designed to settle the Lab Director Charles Elachi added, cept is “truly exploration.” “Nobody issue.” “JPL’s representation in these selec- has ever seen a metal world before,” George Sprague was the NEOCam tions is a very strong reflection of the she added. “We have no idea what it’s Step 1 capture lead. A JPL project quality of proposal work at the Lab going to look like.” manager is expected to be named and our success in teaming with sci- David Oh continues as the capture soon. Ball Aerospace would be the ence investigators.” lead for Psyche, Carol Polanskey is spacecraft contractor for NEOCam. “The Discovery competition re- the project scientist, and a JPL project In addition to the three JPL pro- mains extremely tough,” said Brent manager is expected to be named posals, two mission concepts from Sherwood, manager of 4X’s Solar soon. The spacecraft would be built by NASA’s Goddard Space Flight Center System Mission Formulation Office. JPL, using a power-propulsion chassis were selected in the current Discov- “NASA received 28 proposals this provided by Space Systems Loral. ery Program announcement. time. Congratulations go to the hun- JPL’s third proposal, NEOCam, is VERITAS and Psyche are being dreds of JPLers who supported our the latest project designed to survey developed by JPL’s Solar System Step 1 campaign. Now the hard work potentially hazardous asteroids near Exploration Directorate (4X), while of competing in Step 2 begins.” n 3 Thousands EXOPLANETS discovered since Universe the first finding 20 years ago MARK THE SPOT By Mark Whalen An artist’s rendering of exoplanet 51 Pegasi b, discovered in October 1995. It’s about half the size of Jupiter and orbits its star in about four days. In 1995, a breakthrough for the world of astronomy came when around a sun-like star. This finding, Kepler-452b, brings the total two Swiss scientists announced the discovery of the first planet number of confirmed planets to 1,030. In addition, the Kepler ever found orbiting a sun-like star beyond our solar system. Known team has increased the number of new exoplanet candidates as 51 Pegasi b the planet was a “hot Jupiter,” much larger and by 521 based on their analysis of observations conducted from closer to its parent star than Earth is. May 2009 to May 2013. This raises the number of planet candi- That event ushered in an extraordinarily productive period for dates detected by the Kepler mission to 4,696. planet-finding. Over the past two decades more than 1,800 con- Such candidate exoplanets require follow-up observations firmed exoplanets have been discovered, some much more similar and analysis to verify they are actual planets. Twelve of the new to Earth. Throughout that time, JPL has played a major role in candidates have diameters between one to two times that of both existing discoveries as well as in helping chart the future of Earth, and orbit in their star’s habitable zone. Of these, nine orbit exoplanet exploration. stars that are similar to our sun in size and temperature. JPL’s Spitzer Space Telescope originally was not designed to “The number of planets Kepler has discovered is pretty amaz- study planets around other stars, but one of the mission’s biggest ing,” said Leslie Livesay, JPL’s director for engineering and surprises is its abilities with exoplanets. Thanks to its steady gaze science who previously served as Kepler project manager. “It’s and some clever engineering, it has pioneered the study of atmo- shown us that exoplanets are more abundant than stars. One in spheres and weather on large, gaseous exoplanets. five stars is going to have an Earth analog planet.” Spitzer can help narrow down the sizes of exoplanets too, and NASA’s Exoplanet Exploration Office, which is based at JPL, recently confirmed the closest known rocky planet to Earth, HD leads all planet-seeking study themes across the agency. The 219134b. The infrared observatory also works in tandem with other office coordinates work to define scientific investigations and telescopes that use a planet-hunting technique called microlensing the missions that carry them out, building on each other’s suc- to find some of the most distant exoplanets known. cess. By far the lion’s share of exoplanet discoveries, however, have Looking to the future, JPL is working with NASA’s Goddard been the work of NASA’s Kepler mission. JPL was asked by the Space Flight Center on Wide-Field Infrared Survey Telescope, agency to manage Kepler’s spacecraft development, and contin- or WFIRST, a space-based observatory designed to settle es- ues to support science activities. sential questions in both exoplanet and dark energy research. In its most recent major discovery, in July of this year, Kepler It was the top priority space mission identified in the 2010 confirmed the first near-Earth-size planet in the “habitable zone” Continued on page 5 4 Universe Following the water By Mark Whalen Lujendra Ojha, the former JPL graduate fellow whose research re- Former JPL researcher finds vealed the strongest evidence yet for for water on present-day Mars. evidence of water on Mars today When NASA announced in late Sep- Ojha first noticed puzzling downhill Planitia. Although unrelated to the Mars tember that JPL’s Mars Reconnaissance flows—known as recurring slope lineae, water findings, Smrekar recalls a dedicat- Orbiter provided the strongest evidence often described as possibly related to ed, hardworking but modest researcher.
Recommended publications
  • The Hunt for Exomoons with Kepler (Hek)
    The Astrophysical Journal, 777:134 (17pp), 2013 November 10 doi:10.1088/0004-637X/777/2/134 C 2013. The American Astronomical Society. All rights reserved. Printed in the U.S.A. THE HUNT FOR EXOMOONS WITH KEPLER (HEK). III. THE FIRST SEARCH FOR AN EXOMOON AROUND A HABITABLE-ZONE PLANET∗ D. M. Kipping1,6, D. Forgan2, J. Hartman3, D. Nesvorny´ 4,G.A.´ Bakos3, A. Schmitt7, and L. Buchhave5 1 Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA; [email protected] 2 Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK 3 Department of Astrophysical Sciences, Princeton University, Princeton, NJ 05844, USA 4 Department of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA 5 Niels Bohr Institute, Copenhagen University, Denmark Received 2013 June 4; accepted 2013 September 8; published 2013 October 22 ABSTRACT Kepler-22b is the first transiting planet to have been detected in the habitable zone of its host star. At 2.4 R⊕, Kepler-22b is too large to be considered an Earth analog, but should the planet host a moon large enough to maintain an atmosphere, then the Kepler-22 system may yet possess a telluric world. Aside from being within the habitable zone, the target is attractive due to the availability of previously measured precise radial velocities and low intrinsic photometric noise, which has also enabled asteroseismology studies of the star. For these reasons, Kepler-22b was selected as a target-of-opportunity by the “Hunt for Exomoons with Kepler” (HEK) project. In this work, we conduct a photodynamical search for an exomoon around Kepler-22b leveraging the transits, radial velocities, and asteroseismology plus several new tools developed by the HEK project to improve exomoon searches.
    [Show full text]
  • 2018 Workshop on Autonomy for Future NASA Science Missions
    NOTE: This document was prepared by a team that participated in the 2018 Workshop on Autonomy for Future NASA Science Missions. It is for informational purposes to inform discussions regarding the use of autonomy in notional science missions and does not specify Agency plans or directives. 2018 Workshop on Autonomy for Future NASA Science Missions: Ocean Worlds Design Reference Mission Reports Table of Contents Introduction .................................................................................................................................... 2 The Ocean Worlds Design Reference Mission Report .................................................................... 3 Ocean Worlds Design Reference Mission Report Summary ........................................................ 20 1 NOTE: This document was prepared by a team that participated in the 2018 Workshop on Autonomy for Future NASA Science Missions. It is for informational purposes to inform discussions regarding the use of autonomy in notional science missions and does not specify Agency plans or directives. Introduction Autonomy is changing our world; commercial enterprises and academic institutions are developing and deploying drones, robots, self-driving vehicles and other autonomous capabilities to great effect here on Earth. Autonomous technologies will also play a critical and enabling role in future NASA science missions, and the Agency requires a specific strategy to leverage these advances and infuse them into its missions. To address this need, NASA sponsored the
    [Show full text]
  • Alien Maps of an Ocean-Bearing World
    Alien Maps of an Ocean-Bearing World The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Cowan, Nicolas B., Eric Agol, Victoria S. Meadows, Tyler Robinson, Timothy A. Livengood, Drake Deming, Carey M. Lisse, et al. 2009. Alien maps of an ocean-bearing world. Astrophysical Journal 700(2): 915-923. Published Version doi: 10.1088/0004-637X/700/2/915 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:4341699 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#OAP Accepted for publication in ApJ A Preprint typeset using LTEX style emulateapj v. 10/09/06 ALIEN MAPS OF AN OCEAN-BEARING WORLD Nicolas B. Cowan1, Eric Agol, Victoria S. Meadows2, Tyler Robinson2, Astronomy Department and Astrobiology Program, University of Washington, Box 351580, Seattle, WA 98195 Timothy A. Livengood3, Drake Deming2, NASA Goddard Space Flight Center, Greenbelt, MD 20771 Carey M. Lisse, Johns Hopkins University Applied Physics Laboratory, SD/SRE, MP3-E167, 11100 Johns Hopkins Road, Laurel, MD 20723 Michael F. A’Hearn, Dennis D. Wellnitz, Department of Astronomy, University of Maryland, College Park MD 20742 Sara Seager, Department of Earth, Atmospheric, and Planetary Sciences, Dept of Physics, Massachusetts Institute of Technology, 77 Massachusetts Ave. 54-1626, MA 02139 David Charbonneau, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 and the EPOXI Team Accepted for publication in ApJ ABSTRACT When Earth-mass extrasolar planets first become detectable, one challenge will be to determine which of these worlds harbor liquid water, a widely used criterion for habitability.
    [Show full text]
  • Planets of the Solar System
    Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter.
    [Show full text]
  • Evolutionary Argument Against Naturalism?” International ​ Journal for Philosophy of Religion 69.3 (2010): 193–204
    1 On Plantinga on Belief in Naturalism1 Troy Cross Introduction Naturalism, according to Alvin Plantinga, is the thesis “that there is no such person as God or anything at all like God” (2011b, 435; see also, 2002a, 1; 2011a, vix), and one ​ ​ could be forgiven for thinking that what Plantinga calls his “Evolutionary Argument Against Naturalism”, or “EAAN”, which he has refined and defended for over two decades, is an argument against that thesis (1991, 1993, 2002a, 2002b, 2011a, 2011b). But that would be a mistake. The conclusion of the EAAN is not about the truth of ​ ​ naturalism but about the rationality of believing naturalism to be true: it is that one cannot ​ ​ rationally and reflectively believe that contemporary evolutionary theory is correct about our origins while also believing that neither God nor anything like God exists.2 The difference between truth and rational belief is important here. Consider Moore’s paradoxical sentence: “I don’t believe it’s raining but as a matter of fact it is” (Moore, 209). Nothing prevents that sentence, or others like it, from being true. If you 1 For instructive conversations on this topic I am indebted to John Bang, George Bealer, Mark Bedau, Eliyah Cohen, Bryan Cross, Augie Faller, Emma Handte, Elad Gilo, Nick Gigliotti, John Hare, Jordan Horowitz, Paul Hovda, Alexander Pruss, Margaret Scharle, Derek Schiller, Mackenzie Sullivan, and Carol Voeller. I also wish to thank audiences at Reed College and the University of Nebraska Omaha where I presented early versions of some of this material. Anthony Nguyen gave me many helpful comments on a draft.
    [Show full text]
  • VERITAS – a Discovery-Class Venus Surface Geology and Geophysics Mission Anthony Freeman, Suzanne E
    VERITAS – a Discovery-class Venus surface geology and geophysics mission Anthony Freeman, Suzanne E. Joern Helbert Erwan Mazarico Smrekar, Scott Hensley, Mark German Aerospace Center (DLR) NASA Goddard Space Flight Center Wallace, Christophe Sotin, Murray Institutefor Planetary Research Planetary Geodynamics Lab Darrach, Peter Xaypraseuth Rutherfordstrasse 2, 8800 Greenbelt Rd. Jet Propulsion Laboratory, 12489 Berlin, Germany Greenbelt, MD 20771 California Institute of Technology +49-30-67055-319, 301 614-6504, 4800 Oak Grove Dr. [email protected] [email protected] Pasadena, CA 91109 818-354-1887 [email protected] Abstract— Our understanding of solar system evolution is spacecraft adapted for the environment at Venus, and to follow limited by a great unanswered question: How Earthlike is the old adage – keep it simple. The mission has only two Venus? We know that these “twin” planets formed with instruments, and VISAR for example has only one mode of similar bulk composition and size. Yet the evolutionary path operation. The VEM instrument is a simple pushbroom imager Venus followed has diverged from Earth’s, in losing its surface with no moving parts. Gravity science is carried out using the water and becoming hotter than Mercury. What led to this? spacecraft’s fixed-antenna telecom system. No new The answer has profound implications for how terrestrial technologies are used. Onboard processing of the radar data planets become habitable and the potential for life in the using a COTS space-qualified processor reduces data volume universe. to levels commensurate with downlink rates for other NASA planetary orbiters, so no heroics are required to get the data Prior Venus missions discovered that its surface (like Earth’s) back.
    [Show full text]
  • Lockheed Martin to Help NASA Uncover Mysteries of Venus with VERITAS and DAVINCI+ Spacecraft
    Lockheed Martin to Help NASA Uncover Mysteries of Venus with VERITAS and DAVINCI+ Spacecraft June 2, 2021 Lockheed Martin has a major role in NASA's long-anticipated return to Venus DENVER, June 2, 2021 /PRNewswire/ -- To learn more about how terrestrial planets evolve over time, NASA selected the VERITAS and DAVINCI+ missions for its Discovery Program, both bound for Venus. Lockheed Martin will design, build and operate both spacecraft. The missions will launch in 2026 and 2030 respectively, and will combine to study Venus' dense atmosphere, topography and geologic processes in great depth. Both missions will aim to discover how Venus – which may have been the first potentially habitable planet in our solar system – became inhospitable to life. They represent NASA's return to Earth's sister planet after more than three decades. "We're very grateful for this opportunity to work with NASA and the missions' principal investigators to fully understand how rocky planets evolved and what it means for our planet, Earth," said Lisa Callahan, vice president and general manager of Lockheed Martin's Commercial Civil Space business. "Our team who designed these two spacecraft to study Venus in unprecedented detail – and yield answers to its greatest mysteries – is beyond excited!" The operations and science for DAVINCI+ – which stands for Deep Atmosphere Venus Investigation of Noble Gases, Chemistry and Imaging Plus – will be managed by NASA's Goddard Space Flight Center in Greenbelt, Maryland. VERITAS – which stands for Venus Emissivity, Radio Science, InSAR, Topography & Spectroscopy – will have its science and operations managed by NASA's Jet Propulsion Laboratory in Southern California.
    [Show full text]
  • Licensing Department of Land Management
    Town of Southampton Licensing Licensing Review Board Phone: (631) 702-1826 Department of Land Management Fax (631) 287-5754 Bulgin & Associates Inc License Number: 000511-0 Licensee - David E Bulgin & Jeffrey Gagliotti Expires: 02/12/2022 Climbers Tree Care Specialist Inc License Number: L002198 Licensee - Alex R Verdugo Expires: 07/10/2021 CW Arborists Ltd License Number: L002378 Licensee - Michael S Gaines Expires: 09/09/2022 Domiano Pools Inc. D/B/A Pool Fection License Number: 002770-0 Licensee - Joseph P Domiano Jr. Expires: 03/11/2022 East End Centro-Vac Inc. P O Box 412 License Number: 000358-0 Licensee - Dennis V. Finnerty Expires: 03/11/2022 Ecoshield Pest Control of NYC License Number: L005737 Licensee - Ermir Hasija Expires: 10/08/2021 EmPower CES, LLC License Number: L002063 Licensee - David G Schieren Expires: 07/08/2022 Field Stone Dirt Works Corp. License Number: L005874 Licensee - Louis Russo Expires: 06/10/2022 Fire Sprinkler Associates Inc License Number: L001682 Licensee - Mark Mausser Expires: 05/13/2022 Four Seasons Solar Products LLC License Number: L000230 Licensee - Joseph Segreti Expires: 07/08/2022 Green Team USA LLC D/B/A Green Team LI License Number: L005839 Licensee - Jay B Best Expires: 03/11/2022 Harald G. Steudte License Number: L990112 Licensee - Expires: 08/14/2021 Heatco, Inc License Number: L001776 Licensee - Dennis Valenti Expires: 08/12/2022 Hopping Tree Care License Number: L004995 Licensee - John N Hopping Expires: 06/12/2021 J Tortorella Heating & Gas Specialists Inc License Number: L002120 Licensee - John Tortorella Expires: 06/10/2022 Joseph W. Labrozzi Sr. LLC License Number: L005636 Licensee - Joseph W.
    [Show full text]
  • NASA's Mars Global Surveyor May Be at Mission's End 21 November 2006
    NASA's Mars Global Surveyor May Be at Mission's End 21 November 2006 explanations for the radio silence. "Realistically, we have run through the most likely possibilities for re-establishing communication, and we are facing the likelihood that the amazing flow of scientific observations from Mars Global Surveyor is over," said Fuk Li, Mars Exploration Program manager at NASA's Jet Propulsion Laboratory (JPL), Pasadena, Calif. "We are not giving up hope, though." Efforts to regain contact with the spacecraft and determine what has happened to it will continue. NASA's newest Mars spacecraft, the Mars Reconnaissance Orbiter, pointed its cameras towards Mars Global Surveyor on Monday. "We NASA's Mars Global Surveyor. have looked for Mars Global Surveyor with the star tracker, the context camera and the high-resolution camera on Mars Reconnaissance Orbiter," said Doug McCuistion, Mars Exploration Program NASA's Mars Global Surveyor has likely finished director at NASA Headquarters. "Preliminary its operating career. The orbiter has not analysis of the images did not show any definitive communicated with Earth since Nov. 2. Preliminary sightings of a spacecraft." indications are that a solar panel became difficult to pivot, raising the possibility that the spacecraft The next possibility for learning more about Mars may no longer be able to generate enough power Global Surveyor's status is a plan to send it a to communicate. command to use a transmitter that could be heard by one of NASA's Mars Exploration Rovers later "Mars Global Surveyor has surpassed all this week. expectations," said Michael Meyer, NASA's lead scientist for Mars exploration at NASA Mars Global Surveyor launched on Nov.
    [Show full text]
  • A 4565 Myr Old Andesite from an Extinct Chondritic Protoplanet
    A 4565 Myr old andesite from an extinct chondritic protoplanet. Jean-Alix Barrata*, Marc Chaussidonb, Akira Yamaguchic, Pierre Beckd, Johan Villeneuvee, David J. Byrnee, Michael W. Broadleye, Bernard Martye a Univ Brest, Institut Universitaire Européen de la Mer (IUEM), UMR 6539, Place Nicolas Copernic, F- 29280 Plouzané, France ;b Université de Paris, Institut de pHysique du globe de Paris, CNRS, F-75005 Paris;c National Institute of Polar ResearcH, Tokyo, 190-8518, Japan ;dUniversite Grenoble Alpes, CNRS, Institut de Planetologie et d’Astrophysique de Grenoble (IPAG), Saint-Martin d’Heres, France;e Université de Lorraine, CNRS, CRPG, F-54000 Nancy, France. *Corresponding autHor Jean-Alix Barrat Email: [email protected] Abstract The age of iron meteorites implies that accretion of protoplanets began during the first millions of years of the solar system. Due to the Heat generated by 26Al decay, many early protoplanets were fully differentiated, with an igneous crust produced during the cooling of a magma ocean, and the segregation at depth of a metallic core. The formation and nature of the primordial crust generated during the early stages of melting is poorly understood, due in part to the scarcity of available samples. The newly discovered meteorite Erg CHecH 002 (EC 002) originates from one sucH primitive igneous crust, and has an andesite bulk composition. It derives from the partial melting of a non-carbonaceous chondritic reservoir, witH no depletion in alkalis relative to the sun’s photosphere, and at a high melting rate of around 25%. Moreover, EC 002 is to date, the oldest known piece of an igneous crust witH a 26Al-26Mg crystallization age of 4565.0 Myr.
    [Show full text]
  • Life on Venus, and How to Explore Venus with High-Temperature Electronics Carl-Mikael Zetterling [email protected]
    Life on Venus, and How to Explore Venus with High-Temperature Electronics Carl-Mikael Zetterling [email protected] www.WorkingonVenus.se Outline Life on Venus (phosphine in the clouds) Previous missions to Venus Life on Venus (photos from the ground) High temperature electronics Future missions to Venus, including Working on Venus (KTH Project 2014 - 2018) www.WorkingonVenus.se 3 Phosphine gas in the cloud decks of Venus Trace amounts of phosphine (20 ppb, PH3) seen by the ALMA and JCMT telescopes, with millimetre wave spectral detection 4 Phosphine gas in the cloud decks of Venus 5 Phosphine gas in the cloud decks of Venus https://www.nature.com/articles/s41550-020-1174-4 https://arxiv.org/pdf/2009.06499.pdf https://www.nytimes.com/2020/09/14/science/venus-life- clouds.html?smtyp=cur&smid=fb-nytimesfindings https://www.scientificamerican.com/article/is-there-life-on- venus-these-missions-could-find-it/ 6 Did NASA detect phosphine 1978? Pioneer 13 Large Probe Neutral Mass Spectrometer (LNMS) https://www.livescience.com/life-on-venus-pioneer-13.html 7 Why Venus? From Wikimedia Commons, the free media repository Our closest planet, but least known Similar to earth in size and core, has an atmosphere Volcanoes Interesting for climate modeling Venus Long-life Surface Package (ultimate limit of global warming) C. Wilson, C.-M. Zetterling, W. T. Pike IAC-17-A3.5.5, Paper 41353 arXiv:1611.03365v1 www.WorkingonVenus.se 8 Venus Atmosphere 96% CO2 (Also sulphuric acids) Pressure of 92 bar (equivalent to 1000 m water) Temperature 460 °C From Wikimedia Commons, the free media repository Difficult to explore Life is not likely www.WorkingonVenus.se 9 Previous Missions Venera 1 – 16 (1961 – 1983) USSR Mariner 2 (1962) NASA, USA Pioneer (1978 – 1992) NASA, USA Magellan (1989) NASA, USA Venus Express (2005 - ) ESA, Europa From Wikimedia Commons, the free media repository Akatsuki (2010) JAXA, Japan www.WorkingonVenus.se 10 Steps to lunar and planetary exploration: 1.
    [Show full text]
  • Origin of Water Ice in the Solar System 309
    Lunine: Origin of Water Ice in the Solar System 309 Origin of Water Ice in the Solar System Jonathan I. Lunine Lunar and Planetary Laboratory The origin and early distribution of water ice and more volatile compounds in the outer solar system is considered. The origin of water ice during planetary formation is at least twofold: It condenses beyond a certain distance from the proto-Sun — no more than 5 AU but perhaps as close as 2 AU — and it falls in from the surrounding molecular cloud. Because some of the infalling water ice is not sublimated in the ambient disk, complete mixing between these two sources was not achieved, and at least two populations of icy planetesimals may have been present in the protoplanetary disk. Added to this is a third reservoir of water ice planetesimals representing material chemically processed and then condensed in satellite-forming disks around giant planets. Water of hydration in silicates inward of the condensation front might be a sepa- rate source, if the hydration occurred directly from the nebular disk and not later in the parent bodies. The differences among these reservoirs of icy planetesimals ought to be reflected in diverse composition and abundance of trapped or condensed species more volatile than the water ice matrix, although radial mixing may have erased most of the differences. Possible sources of water for Earth are diverse, and include Mars-sized hydrated bodies in the asteroid belt, smaller “asteroidal” bodies, water adsorbed into dry silicate grains in the nebula, and comets. These different sources may be distinguished by their deuterium-to-hydrogen ratio, and by pre- dictions on the relative amounts of water (and isotopic compositional differences) between Earth and Mars.
    [Show full text]