National Ocean Worlds Analog Test Facility and Field Station
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The Evolution of Star Habitable Zones
The Evolution of Star Habitable Zones Jeffrey J. Wolynski November 17, 2018 Rockledge, FL 32922 Abstract: It was discovered that planets are older, evolving stars. This means the Circumstellar Habitable Zone collapses and/or shrinks into the star itself, thus evolves as the star evolves. Explanation is provided. The habitable zone of a star is the area where liquid water exists or can exist. Since stars cool down and become water worlds as they evolve, combining their hydrogen with the leftover oxygen in large amounts, it is easy to see what happens. The star is too hot in the beginning to form water, or sustain it, but it can heat up other much colder stars allowing them to pool water on their surfaces from a distance. As the star cools and evolves, the distance it can do this diminishes considerably and its habitable zone shrinks. Blue giants have the largest habitable zones, but they quickly contract because they are so young and are evolving rapidly to cooler, less massive states. What this means is that the time variable for the habitable zones of these objects is quite small. The activity of more evolved stars around blue giants should be short-lived, but interesting to say the least. White stars have smaller habitable zones but are still very large. Orange dwarfs have even smaller habitable zones, as well show a noticeable thinning of the zone as opposed to earlier stages. Red dwarfs have very small external habitable zones and the smallest external habitable zone belongs to only the smallest brown dwarfs, which still have a small amount of heat to radiate the surface of another more evolved star. -
The Evolving Universe and the Origin of Life
Pekka Teerikorpi · Mauri Valtonen · Kirsi Lehto · Harry Lehto · Gene Byrd · Arthur Chernin The Evolving Universe and the Origin of Life The Search for Our Cosmic Roots Second Edition The Evolving Universe and the Origin of Life Pekka Teerikorpi • Mauri Valtonen • Kirsi Lehto • Harry Lehto • Gene Byrd • Arthur Chernin The Evolving Universe and the Origin of Life The Search for Our Cosmic Roots Second Edition 123 Pekka Teerikorpi Mauri Valtonen Department of Physics and Astronomy Department of Physics and Astronomy University of Turku University of Turku Turku, Finland Turku, Finland Kirsi Lehto Harry Lehto Department of Biology Department of Physics and Astronomy University of Turku University of Turku Turku, Finland Turku, Finland Gene Byrd Arthur Chernin Department of Physics and Astronomy Sternberg Astronomical Institute The University of Alabama Moscow University Tuscaloosa, AL, USA Moscow, Russia ISBN 978-3-030-17920-5 ISBN 978-3-030-17921-2 (eBook) https://doi.org/10.1007/978-3-030-17921-2 1st edition: © 2009 Springer Science+Business Media, LLC 2nd edition: © Springer Nature Switzerland AG 2019 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. -
Westminsterresearch the Astrobiology Primer V2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., De La Rubia Leigh, A., Bond
WestminsterResearch http://www.westminster.ac.uk/westminsterresearch The Astrobiology Primer v2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., de la Rubia Leigh, A., Bond, J., Dartnell, L., Goldman, A.D., Lynch, K., Naud, M.-E., Paulino-Lima, I.G., Kelsi, S., Walter-Antonio, M., Abrevaya, X.C., Anderson, R., Arney, G., Atri, D., Azúa-Bustos, A., Bowman, J.S., Brazelton, W.J., Brennecka, G.A., Carns, R., Chopra, A., Colangelo-Lillis, J., Crockett, C.J., DeMarines, J., Frank, E.A., Frantz, C., de la Fuente, E., Galante, D., Glass, J., Gleeson, D., Glein, C.R., Goldblatt, C., Horak, R., Horodyskyj, L., Kaçar, B., Kereszturi, A., Knowles, E., Mayeur, P., McGlynn, S., Miguel, Y., Montgomery, M., Neish, C., Noack, L., Rugheimer, S., Stüeken, E.E., Tamez-Hidalgo, P., Walker, S.I. and Wong, T. This is a copy of the final version of an article published in Astrobiology. August 2016, 16(8): 561-653. doi:10.1089/ast.2015.1460. It is available from the publisher at: https://doi.org/10.1089/ast.2015.1460 © Shawn D. Domagal-Goldman and Katherine E. Wright, et al., 2016; Published by Mary Ann Liebert, Inc. This Open Access article is distributed under the terms of the Creative Commons Attribution Noncommercial License (http://creativecommons.org/licenses/by- nc/4.0/) which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited. The WestminsterResearch online digital archive at the University of Westminster aims to make the research output of the University available to a wider audience. -
Monday, November 13, 2017 WHAT DOES IT MEAN to BE HABITABLE? 8:15 A.M. MHRGC Salons ABCD 8:15 A.M. Jang-Condell H. * Welcome C
Monday, November 13, 2017 WHAT DOES IT MEAN TO BE HABITABLE? 8:15 a.m. MHRGC Salons ABCD 8:15 a.m. Jang-Condell H. * Welcome Chair: Stephen Kane 8:30 a.m. Forget F. * Turbet M. Selsis F. Leconte J. Definition and Characterization of the Habitable Zone [#4057] We review the concept of habitable zone (HZ), why it is useful, and how to characterize it. The HZ could be nicknamed the “Hunting Zone” because its primary objective is now to help astronomers plan observations. This has interesting consequences. 9:00 a.m. Rushby A. J. Johnson M. Mills B. J. W. Watson A. J. Claire M. W. Long Term Planetary Habitability and the Carbonate-Silicate Cycle [#4026] We develop a coupled carbonate-silicate and stellar evolution model to investigate the effect of planet size on the operation of the long-term carbon cycle, and determine that larger planets are generally warmer for a given incident flux. 9:20 a.m. Dong C. F. * Huang Z. G. Jin M. Lingam M. Ma Y. J. Toth G. van der Holst B. Airapetian V. Cohen O. Gombosi T. Are “Habitable” Exoplanets Really Habitable? A Perspective from Atmospheric Loss [#4021] We will discuss the impact of exoplanetary space weather on the climate and habitability, which offers fresh insights concerning the habitability of exoplanets, especially those orbiting M-dwarfs, such as Proxima b and the TRAPPIST-1 system. 9:40 a.m. Fisher T. M. * Walker S. I. Desch S. J. Hartnett H. E. Glaser S. Limitations of Primary Productivity on “Aqua Planets:” Implications for Detectability [#4109] While ocean-covered planets have been considered a strong candidate for the search for life, the lack of surface weathering may lead to phosphorus scarcity and low primary productivity, making aqua planet biospheres difficult to detect. -
Stone Aerospace Saves 12 Weeks in Cabling Design by Implementing a Digital Design Process
SUCCESS STORY ® Zuken’s software solution for electrical wiring, control systems and fluid engineering. Stone Aerospace saves 12 weeks in cabling design by implementing a digital design process “We achieved substantial productivity gains because engineers had a very clear picture of what one another were doing, and because of the automated checks performed by the software.“ John Harman, Electrical Engineer, Stone Aerospace ZUKEN - The Partner for Success SUCCESS STORY Stone Aerospace saves 12 weeks in cabling design by implementing a digital design process Stone Aerospace faced the pressure of a tight schedule in designing Results a one-of-a-kind underwater autonomous vehicle (AUV) capable • Elimination of $20,000 in cable of traveling 15km under the Antarctic ice shelf. The AUV acts as a rework and expedited delivery costs testing ground to validate an aircraft-mounted radar system that • Design cycle reduction by 12 weeks will be used in a space mission. The time needed to design the wiring • Ability to view the electrical and harness for the AUV was reduced by around 12 weeks and $20,000 physical design of the entire craft in was saved by using E3.series to automate many aspects of the design a single hierarchical view process, while integrating the logical and physical design on a single • E ective design team collaboration platform. created common nomenclature improving quality and cutting errors The search for life in space aspects such as temperature, depth and water current velocities, and to identify • Automated checks ensured correct Scientists believe that underneath the microbiological communities. connector selections. icy surface of Europa, one of Jupiter’s moons, is a vast ocean thought to be the Cable design challenges most likely location for finding life in our solar system. -
Abscicon 2019 Summary
Summary of AbSciCon (Astrobiology Science Conference) 2019 • AbSciCon 2019 Theme: Understanding and Enabling the Search for Life on Worlds Near and Far • Event Details: • Event Location: Bellevue, WA • Approximate # of attendees: 900 (>3x larger than 2 years ago) • Attendee Demographics: Academia / Researchers / NASA Kate Craft, JHU APL, [email protected] 1 AbSciCon 2019 Topics • Star-planet-planetary system interactions and habitability • Alternative and agnostic biosignatures • Understanding the environments of early Earth • Evidence for early life on Earth • Subsurface habitability and life • Ocean worlds near and far • Characterizing habitable zone exoplanets • Transition of prebiotic chemistry to biology • Energy sources in the environment and metabolic pathways that use that energy • Terrestrial planets orbiting M dwarfs 2 Nature May Present Challenges to Higher- order Life Forms • Earth has special conditions that may skew our view of how common higher-order life is – We have learned that Ocean Worlds are more common than had been thought – Ocean Worlds with frozen crusts are blocked from solar energy, depend on chemical energy from rocks, may limit the biosphere – Ocean Worlds with a deep ocean will have a bottom layer of “ice-VI” that might block water from rock, starving nutrients / chemical energy. – Most Ocean Worlds likely occur around M-dwarf stars like Proxima Centauri. They flare early and push planets in the “habitable zone” through an early Venus phase. Sun-like G-type stars are much more stable. Artist’s conception of Earth- sized planet discovered – Planets orbiting their stars can have large variations in obliquity orbiting Proxima Centauri causing extreme climate change on liquid surfaces. -
Development of Nereid-UI: a Remotely Operated Underwater Vehicle for Oceanographic Access Under Ice
Development of Nereid-UI: A Remotely Operated Underwater Vehicle for Oceanographic Access Under Ice Presented at the 9th Annual Polar Technology Conference, 2-4 April 2013 Louis L. Whitcomb1,2,Andrew D. Bowen1, Dana R. Yoerger1, Christopher German1, James C. Kinsey1, Larry Mayer1,3, Michael V. Jakuba1, Daniel Gomez-Ibanez1, Christopher L. Taylor1, Casey Machado1, Jonathan C. Howland1, Carl Kaiser1, Matthew Heintz1 1Department of Applied Ocean Physics and Engineering, Woods Hole Oceanographic Institution 2Department of Mechanical Engineering, Johns Hopkins University 3Center for Coastal and Ocean Mapping, University of New Hampshire Photo courtesy S. McPhail, NOC Woods Hole Oceanographic Institution World’s largest private ocean research institution ~900 Employees, 143 Scientific Staff $160M Annual Budget • Biology • Chemistry • Geology • Physical Oceanography • Engineering • Marine Policy Deep Ocean Oceanography: The D.S.V. Alvin 4500m Submersible Image Credit: Rod Catenach © WHOI Catenach Credit: Rod Image Crew: 3 = 1 pilot + 2 scientist Depth: 4500m (6,500m soon) Endurance: 6-10 Hours Speed: 1 m/s Mass: 7,000 Kg Length: 7.1m Power: 81 KWH Life Support: 72 Hours x 3 Persons Ph.D. Student James Kinsey Dives: >4,700 (since 1964) Passengers: >14,000 (since 1964) Jason II ROV Specifications: Size: 3.2 x 2.4 x 2.2 m Weight 3,300 kg Depth 6,500 m Power 40 kW (50 Hp) Payload: 120 Kg (1.5 Ton) First Dive: 2002 Dives: >600 Dive Time: >12,500 Hours* Bottom Time: >10,600 Hours* Longest Dive: 139 Hours* Deepest Dive: 6,502 m* Distance: >4,800 km* * As of Feb, 2012 Electric thrusters, twin hydraulic manipulator arms. -
Visionary Counting on Unmanned Vehicles
Visionary Counting on Unmanned Vehicles By Rich Tuttle Bill Stone, the founder of Stone Aerospace, has a vision—several visions, in fact—and unmanned vehicles play a part in a number of them. His Austin, Texas-based company developed and built the DEPTHX robot that last May conducted the first comprehensive exploration of the world’s deepest sink hole, El Zacaton in Mexico. It brought back enough data to keep scientists enthralled for some time. An unmanned system based on DEPTHX (DEep Phreatic—meaning underwater cave—THermal eXplorer) will be tested in Antarctica beginning next year to help determine the suitability of such a device to meet, in about 20 years, what’s been called the ultimate robotic challenge: exploring the ice- covered ocean of Europa, a moon of Jupiter. Scientists believe there’s a high probability of detecting the first life off Earth in that remote and ancient sea. That's one vision. The challenges would fill a book: melting through many kilometers of ice just to get to the ocean, for instance. That will be addressed in the Antarctica experiments. But DEPTHX does seem to have demonstrated the possibility of clearing two other key hurdles—surviving in a three-dimensional, unexplored environment without external navigation aids; and carrying out science experiments autonomously. DEPTHX's abilities are two generations beyond those of the Spirit and Opportunity rovers on Mars right now, Stone says in an interview. Every move of the Mars vehicles is based on a carefully prepared script. But, Stone says, “in the case of Europa, it can’t be that way.” The computer brain of a Europa probe would have to be wired to achieve “global” objectives, he says. -
Ocean Worlds : May 21–23, 2018, Houston, Texas
Program Ocean Worlds May 21–23, 2018 • Houston, Texas Organizers Lunar and Planetary Institute Universities Space Research Association Convener Louise Prockter Lunar and Planetary Institute Science Organizing Committee Julie Castillo NASA Jet Propulsion Laboratory Christopher German Wood Hole Oceanographic Institution Jonathan Kay Lunar and Planetary Institute Marc Neveu NASA Headquarters Beth Orcutt Bigelow Laboratory for Ocean Sciences Paul Schenk Lunar and Planetary Institute Christophe Sotin NASA Jet Propulsion Laboratory Hajime Yano Japan Aerospace Exploration Agency Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Abstracts for this meeting are available via the meeting website at www.hou.usra.edu/meetings/oceanworlds2018/ Abstracts can be cited as Author A. B. and Author C. D. (2018) Title of abstract. In Ocean Worlds, Abstract #XXXX. LPI Contribution No. 2085, Lunar and Planetary Institute, Houston. Guide to Sessions Monday, May 21, 2018 1:00 p.m. Lecture Hall Opening Session: Setting the Framework 5:30 p.m. Great Room Poster Session Tuesday, May 22, 2018 8:30 a.m. Lecture Hall Session I 12:45p.m. Great Room Poster Viewing Tuesday, May 22, 2018 1:30 p.m. Lecture Hall Session II Wednesday, May 23, 2018 8:30 a.m. Lecture Hall Session III 1:00 p.m. Lecture Hall Session IV Program Monday, May 21, 2018 OPENING SESSION: SETTING THE FRAMEWORK 1:00 p.m. Lecture Hall Chair: Christopher German 1:00 p.m. German C. R. * Prockter L. * Opening Remarks 1:15 p.m. Hand K. P. * Ocean Worlds of the Outer Solar System [#6042] I will provide an overview of why we think we know ocean worlds exist, what we know about the physical and chemical conditions that likely persist on these worlds, and how we may proceed in our search for biosignatures on these worlds. -
The Kepler Revolution Observations and Satellite Inferences of the Kepler Space Telescope Will Soon Run out of Fuel and End Its Mission
VOL. 99 • NO. 10 • OCT 2018 Models That Forecast Wildfires Recording the Roar of a Hurricane Earth & Space Science News How Much Snow Is in the World? The Honors and Recognition Committee is pleased to announce the recipients of this year’s Union Medals, Awards, and Prizes honors.agu.org Earth & Space Science News Contents OCTOBER 2018 PROJECT UPDATE VOLUME 99, ISSUE 10 20 Seismic Sensors Record a Hurricane’s Roar Newly installed infrasound sensors at a Global Seismographic Network station on Puerto Rico recorded the sounds of Hurricane Maria passing overhead. PROJECT UPDATE 26 How Can We Find Out How Much Snow Is in the World? In Colorado forests, NASA scientists and a multinational team of researchers test the limits of satellite remote sensing for measuring the water content of snow. 30 OPINION Global Water Clarity: COVER 14 Continuing a Century- Long Monitoring An approach that combines field The Kepler Revolution observations and satellite inferences of The Kepler Space Telescope will soon run out of fuel and end its mission. Here are nine Secchi depth could transform how we assess fundamental discoveries about planets aided by Kepler, one for each year since its water clarity across the globe and pinpoint launch. key changes over the past century. Earth & Space Science News Eos.org // 1 Contents DEPARTMENTS Senior Vice President, Marketing, Communications, and Digital Media Dana Davis Rehm: AGU, Washington, D. C., USA; [email protected] Editors Christina M. S. Cohen Wendy S. Gordon Carol A. Stein California Institute Ecologia Consulting, Department of Earth and of Technology, Pasadena, Austin, Texas, USA; Environmental Sciences, Calif., USA; wendy@ecologiaconsulting University of Illinois at cohen@srl .caltech.edu .com Chicago, Chicago, Ill., José D. -
Geometric Control Theory and Its Application To
GEOMETRIC CONTROL THEORY AND ITS APPLICATION TO UNDERWATER VEHICLES A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN OCEAN & RESOURCES ENGINEERING DECEMBER 2008 By Ryan N. Smith Dissertation Committee: Monique Chyba, Chairperson Song K. Choi R. Cengiz Ertekin Geno Pawlak George R. Wilkens We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Ocean & Resources Engineering. DISSERTATION COMMITTEE —————————————— Chairperson —————————————— —————————————— —————————————— —————————————— —————————————— ii c 2008, Ryan Neal Smith. All rights reserved. iii To Neal iv Acknowledgments Of this entire dissertation, this single section has proven to be the most painful and difficult to write. Of course, after committing two-hundred and some odd pages to the discussion of my research over the last five years, I have few words left for the one section that will probably be read the most of any other in this dissertation. Additionally, recounting the memories of all the love and support which I have received from so many people brings tears to my eyes every time I have tried to work on this section. My cup runneth over. I have written this acknowledgments section one hundred forty-three times; yes, I have been counting. I can not simply list every person who has participated in the success of this work, as the list would be longer than the dissertation itself. So, I must restrict myself to acknowledging only those whom have truly made this all possible, and at times, very worthwhile. -
Design and Deployment of a 3D Autonomous Subterranean Submarine Exploration Vehicle
DESIGN AND DEPLOYMENT OF A 3D AUTONOMOUS SUBTERRANEAN SUBMARINE EXPLORATION VEHICLE William C. Stone, Stone Aerospace / PSC, Inc. 3511 Caldwell Lane, Del Valle, TX 78617, Ph: (512) 247-6385, [email protected] ABSTRACT likely include the following components: The NASA Deep Phreatic Thermal Explorer • the parent spacecraft, which will remain in orbit (DEPTHX) project is developing a fully autonomous either about Jupiter or about Europa and which will underwater vehicle intended as a prototype of primarily serve as a data relay back to Earth from the the Europa lander third stage that will search for Lander. microbial life beneath the ice cap of that Jovian • the Lander, which will be a 3-stage device: moon. DEPTHX has two principal objectives: First, to develop and test in an appropriate environment Stage 1: the physical landing system that will contain the ability for an un-tethered robot to explore into propulsion systems, power, and data relay systems to unknown 3D territory, to make a map of what it sees, communicate with the orbiter, and which will control and to use that map to return home; and second, to and carry out the descent and automated landing on demonstrate that science autonomy behaviors can the moon. identify likely zones for the existence of microbial life, to command an autonomous maneuvering Stage 2: the “cryobot” second stage, which will melt platform to move to those locations, conduct localized a hole through up to ten kilometers of ice cap before searches, and to autonomously collect microbial reaching the sub-surface liquid ocean. Although the life in an aqueous environment.