Synergies of Robotic Asteroid Redirection Technologies and Human Space Exploration
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Ice& Stone 2020
Ice & Stone 2020 WEEK 34: AUGUST 16-22 Presented by The Earthrise Institute # 34 Authored by Alan Hale This week in history AUGUST 16 17 18 19 20 21 22 AUGUST 16, 1898: DeLisle Stewart at Harvard College Observatory’s Boyden Station in Arequipa, Peru, takes photographs on which Saturn’s outer moon Phoebe is discovered, although the images of Phoebe were not noticed until the following March by William Pickering. Phoebe was the first planetary moon to be discovered via photography, and it and other small planetary moons are discussed in last week’s “Special Topics” presentation. AUGUST 16, 2009: A team of scientists led by Jamie Elsila of the Goddard Space Flight Center in Maryland announces that they have detected the presence of the amino acid glycine in coma samples of Comet 81P/ Wild 2 that were returned to Earth by the Stardust mission 3½ years earlier. Glycine is utilized by life here on Earth, and the presence of it and other organic substances in the solar system’s “small bodies” is discussed in this week’s “Special Topics” presentation. AUGUST 16 17 18 19 20 21 22 AUGUST 17, 1877: Asaph Hall at the U.S. Naval Observatory in Washington, D.C. discovers Mars’ larger, inner moon, Phobos. Mars’ two moons, and the various small moons of the outer planets, are the subject of last week’s “Special Topics” presentation. AUGUST 17, 1989: In its monthly batch of Minor Planet Circulars (MPCs), the IAU’s Minor Planet Center issues MPC 14938, which formally numbers asteroid (4151), later named “Alanhale.” I have used this asteroid as an illustrative example throughout “Ice and Stone 2020” “Special Topics” presentations. -
Lindley Johnson (NASA HQ) – NASA HEOMD – – NASA STMD – Tibor Balint (NASA HQ) – SSERVI – Greg Schmidt (NASA ARC) 19
September 4, 2014: Planetary Science Subcommittee Nancy Chabot, SBAG Chair 11th SBAG Meeting • July 29-31, 2014: Washington, DC • Highlights of SBAG meeting presentations from major projects • Discussion of findings • New steering committee members • Future meetings 1 NEOWISE Reac,va,on • Reac,vated in Dec 2013, NEOWISE is observing, discovering, and characterizing asteroids & comets using 3.4 and 4.6 µm channels • 7239 minor planets observed, including 157 near-Earth objects (NEOs). • 89 discoveries, including 26 NEOs and 3 comets. • NEO discoveries are large, dark • First data delivery from Reac9vaon: March 2015 to IRSA: • hp://irsa.ipac.caltech.edu/Missions/wise.html • All data from prime WISE/NEOWISE mission are publicly available through IRSA and team Comet P/2014 L2 NEOWISE papers; derived physical proper9es heading to PDS Dawn prepares to encounter Ceres PI: Alan Stern (SwRI) New Horizons Status PM: JHU-APL • Spacecraft is healthy & On-Course for Pluto (Radio) § 1.3x more fuel available for KBO Extended (High-E Plasma) NH Payload Mission phase than originally expected • Payload is healthy and well-calibrated § Finishing final Annual Checkout (ACO-8) • First Pluto OpNav Campaign conducted (UV Spectral) § See image below • Enter final Hibernation on Aug 29th (Vis-Color + IR Spectral) • Pluto Encounter begins on 2015-Jan-15 (Low-E Plasma) • Pluto Closest Approach: 2015-Jul-14 (Pan Imager) Intensive searches with ground-based facilities over the past Pluto OpNav Campaign: 2 years have not yet yielded a KBO target for NH. A 194- Cleanly separate Pluto & orbit Hubble program was started in June; below Charon shows the first potentially targetable KBO found. -
Asteroid Retrieval Feasibility Study
Publications 4-2-2012 Asteroid Retrieval Feasibility Study John Brophy California Institute of Technology Fred Culick California Institute of Technology Louis Friedman The Planetary Society Pedro Llanos Embry-Riddle Aeronautical University - Daytona Beach, [email protected] et al. Follow this and additional works at: https://commons.erau.edu/publication Part of the Astrodynamics Commons, Space Vehicles Commons, and the The Sun and the Solar System Commons Scholarly Commons Citation Brophy, J., Culick, F., Friedman, L., Llanos, P., & al., e. (2012). Asteroid Retrieval Feasibility Study. , (). Retrieved from https://commons.erau.edu/publication/893 This Report is brought to you for free and open access by Scholarly Commons. It has been accepted for inclusion in Publications by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. Asteroid Retrieval Feasibility Study 2 April 2012 Prepared for the: Keck Institute for Space Studies California Institute of Technology Jet Propulsion Laboratory Pasadena, California 1 2 Authors and Study Participants NAME Organization E-Mail Signature John Brophy Co-Leader / NASA JPL / Caltech [email protected] Fred Culick Co-Leader / Caltech [email protected] Co -Leader / The Planetary Louis Friedman [email protected] Society Carlton Allen NASA JSC [email protected] David Baughman Naval Postgraduate School [email protected] NASA ARC/Carnegie Mellon Julie Bellerose [email protected] University Bruce Betts The Planetary Society -
Lightsail 2 Set to Launch in June “We Are Go for Launch!” Said Planetary Society CEO Bill Nye
Lightsail 2 set to launch in June “We are go for launch!” said Planetary Society CEO Bill Nye. Funded by space enthusiasts, LightSail 2 aims to accomplish the 1st-ever, controlled solar sail flight in Earth orbit next month. Writing at the Planetary Society’s blog, Jason Davis this week (May 13, 2019) described the upcoming challenge of the launch of LightSail 2, a little spacecraft literally powered by sunbeams and dear to the hearts of many. He wrote: Weighing just 5 kilograms, the loaf-of-bread-sized spacecraft, known as a CubeSat, is scheduled to lift A one-unit CubeSat measures 10 centimeters per side. off on June 22, 2019, aboard a SpaceX Falcon Heavy LightSail is a three-unit CubeSat measuring 10 by 10 by 30 rocket from Kennedy Space Center, Florida. Once in centimetres. Here, an early LightSail model sits next to a space, LightSail 2 will deploy a boxing ring-sized solar loaf of bread for size comparison. sail and attempt to raise its orbit using the gentle push from solar photons. It’s the culmination of a 10-year project with an origin story linked to the three scientist-engineers who founded The Planetary Society in 1980. Indeed, although the Lightsail 2 project itself is 10 years old, the idea for lightsail or solar sail spacecraft goes back decades, at least. Carl Sagan – who was one of those Planetary Society founders -- popularized the idea for our time. Now the mantle for popularizing lightsails, and helping to bring the dream many steps closer to reality, has been passed to Bill Nye, the current CEO of the Planetary Society. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Asteroid Retrieval Feasibility Study
Asteroid Retrieval Feasibility Study 2 April 2012 Prepared for the: Keck Institute for Space Studies California Institute of Technology Jet Propulsion Laboratory Pasadena, California 1 2 Authors and Study Participants NAME Organization E-Mail Signature John Brophy Co-Leader / NASA JPL / Caltech [email protected] Fred Culick Co-Leader / Caltech [email protected] Co -Leader / The Planetary Louis Friedman [email protected] Society Carlton Allen NASA JSC [email protected] David Baughman Naval Postgraduate School [email protected] NASA ARC/Carnegie Mellon Julie Bellerose [email protected] University Bruce Betts The Planetary Society [email protected] Mike Brown Caltech [email protected] Michael Busch UCLA [email protected] John Casani NASA JPL [email protected] Marcello Coradini ESA [email protected] John Dankanich NASA GRC [email protected] Paul Dimotakis Caltech [email protected] Harvard -Smithsonian Center for Martin Elvis [email protected] Astrophysics Ian Garrick-Bethel UCSC [email protected] Bob Gershman NASA JPL [email protected] Florida Institute for Human and Tom Jones [email protected] Machine Cognition Damon Landau NASA JPL [email protected] Chris Lewicki Arkyd Astronautics [email protected] John Lewis University of Arizona [email protected] Pedro Llanos USC [email protected] Mark Lupisella NASA GSFC [email protected] Dan Mazanek NASA LaRC [email protected] Prakhar Mehrotra Caltech [email protected] -
Copernic Agent Search Results
Copernic Agent Search Results Search: sonofusion (The exact phrase) Found: 1626 result(s) on _Full.Search Date: 7/17/2010 5:51:35 AM 1. New sonofusion experiment produces results without external neutron source Mar 2009 - ...Rensselaer Polytechnic Institute New sonofusion experiment produces results without...results in 2004, suggesting that "sonofusion" may be a viable approach to producing...technique, which has been dubbed "sonofusion," produces a shock wave t http://www.eurekalert.org/pub_releases/2006-01/rpi-nse012706.php 93% 2. Bubbles feel the heat http://physicsworld.com/cws/article/news/21654 92% 3. Directory:Sonofusion - PESWiki Directory of technologies and resources relating to sonofusion, also known as bubble fusion, which involves room temperature fusion using sound frequencies " ... http://peswiki.com/index.php/Directory:Sonofusion 92% 4. Evidence bubbles over to support tabletop nuclear fusion device The researchers believe the new evidence shows that "sonofusion" generates nuclear reactions by creating tiny bubbles that implode with tremendous force. http://news.uns.purdue.edu/html4ever/2004/0400302.Taleyarkhan.fusion.html 92% 5. Research Uses Sonofusion to Generate Temperatures Hot Enough For Fusion - The Tech Mar 2009 - ...Article Tools E-Mail Print Write the Editor Research Uses Sonofusion to Generate Temperatures Hot Enough For Fusion By Kenneth Chang...tabletop. Putterman's approach is to use sound waves, called sonofusion or bubble fusion, to expand and col http://tech.mit.edu/V127/N7/long5.html 92% 6. Roger Stringham Sonofusion Jets Sonofusion is a developing alternate energy technology that has the potential to replace polluting hydrocarbons which include fossil fuels. The economics for sonofusion appear feasible now with its application to heating large structures. -
1 Statement of Kathryn C. Thornton Professor and Associate Dean School of Engineering and Applied Science University of Virginia
Statement of Kathryn C. Thornton Professor and Associate Dean School of Engineering and Applied Science University of Virginia before the Committee on Science and Technology Subcommittee on Space and Aeronautics U.S. House of Representatives April 3, 2008 Chairman Udall, Ranking Member Feeney, and members of the subcommittee, thank you for inviting me to appear before you today. My name is Kathryn Thornton and I am a Professor and Associate Dean in the School of Engineering and Applied Science at the University of Virginia. I appear here this morning not in my faculty role but as an organizer and co-chair of an independent workshop entitled Examining the Vision: Balancing Exploration and Science held last February at Stanford University. The workshop was co-hosted by Stanford University Department of Aeronautics and Astronautics, and The Planetary Society. Other organizers were co-chair Professor G. Scott Hubbard from Stanford University, Dr. Louis Friedman of The Planetary Society, and Dr. Wesley T. Huntress, Jr., of the Carnegie Institution of Washington. The post- workshop joint communiqué and a partial list of participants are attached. The intent of the workshop was to critically examine the current implementation of the Vision for Space Exploration as announced by President Bush in January 2004, especially to help prepare for a new Administration’s consideration of its broad space program goals and plans. The Vision for Space Exploration in its original plan was a major redirection of the human space flight program with an accompanying emphasis on scientific exploration. Whatever changes might be made in its implementation in the next Administration, we wanted to identify, highlight and support the best parts of the current concept. -
Hydrated Minerals on Asteroids: the Astronomical Record
Hydrated Minerals on Asteroids: The Astronomical Record A. S. Rivkin, E. S. Howell, F. Vilas, and L. A. Lebofsky March 28, 2002 Corresponding Author: Andrew Rivkin MIT 54-418 77 Massachusetts Ave. Cambridge MA, 02139 [email protected] 1 1 Abstract Knowledge of the hydrated mineral inventory on the asteroids is important for deducing the origin of Earth’s water, interpreting the meteorite record, and unraveling the processes occurring during the earliest times in solar system history. Reflectance spectroscopy shows absorption features in both the 0.6-0.8 and 2.5-3.5 pm regions, which are diagnostic of or associated with hydrated minerals. Observations in those regions show that hydrated minerals are common in the mid-asteroid belt, and can be found in unex- pected spectral groupings, as well. Asteroid groups formerly associated with mineralogies assumed to have high temperature formation, such as MAand E-class asteroids, have been observed to have hydration features in their reflectance spectra. Some asteroids have apparently been heated to several hundred degrees Celsius, enough to destroy some fraction of their phyllosili- cates. Others have rotational variation suggesting that heating was uneven. We summarize this work, and present the astronomical evidence for water- and hydroxyl-bearing minerals on asteroids. 2 Introduction Extraterrestrial water and water-bearing minerals are of great importance both for understanding the formation and evolution of the solar system and for supporting future human activities in space. The presence of water is thought to be one of the necessary conditions for the formation of life as 2 we know it. -
Planetary Report
The PLANETARY REPORT Volume XXX Number 3 May/June 2010 Why Go Into Space? From The Editor On the Cover: This dazzling, visible-light portrait of the Orion nebula was his 30th anniversary year has had me looking taken by the European Southern Observatory’s new Visible Tback to the beginning of The Planetary Soci- and Infrared Survey Telescope for Astronomy (VISTA). Most of ety, while our LightSail program keeps pulling the light from the spectacular clouds comes from hydrogen gas glowing under the fierce ultraviolet glare of the hot young my thoughts to the future. In 1980, The Planetary Society launched while stars at center. The region above Orion’s center is obscured Carl Sagan was presenting his personal view of by clouds of dust. Image: ESO/J. Emerson/VISTA & R. Gendler, the universe on television screens around the with thanks to the Cambridge Astronomical Survey Unit world. There’s no question that our organization’s success is linked directly to the phenomenon that Background: was Cosmos. To honor that connection, in 2005, It’s easy to forget—as we deal with the day-to-day challenges we created the Cosmos Award for Outstanding of life—that we live on a planet whose normal geologic Public Presentation of Science. The first recipi- activity can trump our most important plans. Here, lava ent was filmmaker James Cameron (who’s had spews out of a mountain on March 21, 2010, in the region a rather big success of his own lately). This February, we presented The Planetary of Iceland’s Eyjafjallajökull volcano. -
Required Deflection Impulses As a Function of Time Before Impact for Earth-Impacting Asteroids
Icarus 347 (2020) 113792 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Required deflection impulses as a function of time before impact for Earth-impacting asteroids Sarah Greenstreet a,b,<, Ed Lu a, Mike Loucks a,c, John Carrico a,c, Tatiana Kichkaylo a, Mario Juri¢ b a Asteroid Institute, 20 Sunnyside Ave, Suite 427, Mill Valley, CA 94941, USA b Department of Astronomy and the DIRAC Institute, University of Washington, 3910 15th Avenue, NE, Seattle, WA 98195, USA c Space Exploration Engineering LLC, 687 Chinook Way, Friday Harbor, WA 98250, USA ARTICLEINFO ABSTRACT Keywords: For any asteroid on an impact trajectory, the amount of time prior to impact a deflection can be implemented Asteroids can drastically change the amount of deflection impulse required. In this study we use the precision cloud- Dynamics based asteroid orbit propagation and targeting capabilities of the Asteroid Institute's Asteroid Decision Analysis and Mapping (ADAM) platform to investigate the distribution of deflection 훥푣 required to divert asteroids on Earth-impacting trajectories (Chesley and Spahr, 2004) as a function of time prior to impact for 10,000 synthetic impacting asteroids. We target a miss distance of one Earth radius above the surface of the Earth and calculate the distribution of deflection 훥푣 required if applied 10, 20, 30, 40, and 50 years prior to impact. We find that the median required deflection impulse decreases as approximately t*1 for increasing time before impact (Ahrens and Harris, 1992), where the median required 훥푣 is 1.4 cm/s, 0.76 cm/s, 0.55 cm/s, 0.46 cm/s, and 0.38 cm/s for 10, 20, 30, 40, & 50 years before impact, respectively. -
ABSTRACT Title of Dissertation: WATER in the EARLY SOLAR
ABSTRACT Title of Dissertation: WATER IN THE EARLY SOLAR SYSTEM: INFRARED STUDIES OF AQUEOUSLY ALTERED AND MINIMALLY PROCESSED ASTEROIDS Margaret M. McAdam, Doctor of Philosophy, 2017. Dissertation directed by: Professor Jessica M. Sunshine, Department of Astronomy This thesis investigates connections between low albedo asteroids and carbonaceous chondrite meteorites using spectroscopy. Meteorites and asteroids preserve information about the early solar system including accretion processes and parent body processes active on asteroids at these early times. One process of interest is aqueous alteration. This is the chemical reaction between coaccreted water and silicates producing hydrated minerals. Some carbonaceous chondrites have experienced extensive interactions with water through this process. Since these meteorites and their parent bodies formed close to the beginning of the Solar System, these asteroids and meteorites may provide clues to the distribution, abundance and timing of water in the Solar nebula at these times. Chapter 2 of this thesis investigates the relationships between extensively aqueously altered meteorites and their visible, near and mid-infrared spectral features in a coordinated spectral-mineralogical study. Aqueous alteration is a parent body process where initially accreted anhydrous minerals are converted into hydrated minerals in the presence of coaccreted water. Using samples of meteorites with known bulk properties, it is possible to directly connect changes in mineralogy caused by aqueous alteration with spectral features. Spectral features in the mid-infrared are found to change continuously with increasing amount of hydrated minerals or degree of alteration. Building on this result, the degrees of alteration of asteroids are estimated in a survey of new asteroid data obtained from SOFIA and IRTF as well as archived the Spitzer Space Telescope data.