Kathryn Volk
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Gnc 2021 Abstract Book
GNC 2021 ABSTRACT BOOK Contents GNC Posters ................................................................................................................................................... 7 Poster 01: A Software Defined Radio Galileo and GPS SW receiver for real-time on-board Navigation for space missions ................................................................................................................................................. 7 Poster 02: JUICE Navigation camera design .................................................................................................... 9 Poster 03: PRESENTATION AND PERFORMANCES OF MULTI-CONSTELLATION GNSS ORBITAL NAVIGATION LIBRARY BOLERO ........................................................................................................................................... 10 Poster 05: EROSS Project - GNC architecture design for autonomous robotic On-Orbit Servicing .............. 12 Poster 06: Performance assessment of a multispectral sensor for relative navigation ............................... 14 Poster 07: Validation of Astrix 1090A IMU for interplanetary and landing missions ................................... 16 Poster 08: High Performance Control System Architecture with an Output Regulation Theory-based Controller and Two-Stage Optimal Observer for the Fine Pointing of Large Scientific Satellites ................. 18 Poster 09: Development of High-Precision GPSR Applicable to GEO and GTO-to-GEO Transfer ................. 20 Poster 10: P4COM: ESA Pointing Error Engineering -
A Deep Search for Additional Satellites Around the Dwarf Planet
Search for Additional Satellites around Haumea A Preprint typeset using LTEX style emulateapj v. 01/23/15 A DEEP SEARCH FOR ADDITIONAL SATELLITES AROUND THE DWARF PLANET HAUMEA Luke D. Burkhart1,2, Darin Ragozzine1,3,4, Michael E. Brown5 Search for Additional Satellites around Haumea ABSTRACT Haumea is a dwarf planet with two known satellites, an unusually high spin rate, and a large collisional family, making it one of the most interesting objects in the outer solar system. A fully self-consistent formation scenario responsible for the satellite and family formation is still elusive, but some processes predict the initial formation of many small moons, similar to the small moons recently discovered around Pluto. Deep searches for regular satellites around KBOs are difficult due to observational limitations, but Haumea is one of the few for which sufficient data exist. We analyze Hubble Space Telescope (HST) observations, focusing on a ten-consecutive-orbit sequence obtained in July 2010, to search for new very small satellites. To maximize the search depth, we implement and validate a non-linear shift-and-stack method. No additional satellites of Haumea are found, but by implanting and recovering artificial sources, we characterize our sensitivity. At distances between 10,000 km and 350,000 km from Haumea, satellites with radii as small as 10 km are ruled out, assuming∼ an albedo∼ (p 0.7) similar to Haumea. We also rule out satellites larger∼ than &40 km in most of the Hill sphere using≃ other HST data. This search method rules out objects similar in size to the small moons of Pluto. -
Curriculum Vitae: Dr
Curriculum Vitae: Dr. Yanga R. “Yan” Fernandez´ UniversityofCentralFlorida Ph: +1-407-8232325 Department of Physics Fax: +1-407-8235112 4000 Central Florida Blvd. Email: [email protected] Orlando, FL 32816-2385 U.S.A. Website: physics.ucf.edu/∼yfernandez/ Education University of Maryland, College Park, Ph.D. Astronomy, 1999 Dissertation: Physical Properties of Cometary Nuclei University of Maryland, College Park, M.S. Astronomy, 1995 California Institute of Technology, B.S. with Honors, Astronomy, 1993 Professional Experience and Appointments 2019 - present Professor, Department of Physics, University of Central Florida 2016 - present Associate Scientist, Florida Space Institute, University of Central Florida 2011 - 2019 Associate Professor, Department of Physics, University of Central Florida 2005 - 2011 Assistant Professor, Department of Physics, University of Central Florida 2002 - 2005 SIRTF/Spitzer Fellow, Institute for Astronomy, University of Hawai‘i 1999 - 2002 Scientific Researcher, Institute for Astronomy, University of Hawai‘i Honors and Awards • Asteroid (12225) Yanfernandez named in honor. • International Astronomical Union membership, awarded 2012. • SIRTF/Spitzer Fellowship, 2002-2005. • UCF Scroll & Quill Society membership, awarded 2017. External Funding • As PI, 16 grants totalling $1,337K. • As Co-PI or Co-I, 14 grants totalling $531K to YRF. Impact Indicators (as of April 22, 2021) • Google Scholar lists nearly 5500 citations all-time of refereed and unrefereed work. https://scholar.google.com/citations?user=wPjufFkAAAAJ&hl=en. • Astrophysics Data System has recorded about 3600 citations all-time of refereed and unrefereed work. https://tinyurl.com/mufdrktx. Y.R.Fern´andez CV April 2021 1 • Web of Science (WoS) has recorded over 3000 citations all-time of refereed work that is included in WoS. -
Exploring Connections Between Neos and Meteoroid Streams
Observers Meeting NEOCC observations with the ESA OGS, VLT, and LBT Marco Micheli ([email protected]) NEO Statistics ~ 13 700 known NEOs …of which… ~ 510 (4 %) have impact solutions (VIs) in the next century (according to NEODyS and Sentry) However… of those VIs: Only ~2 % have more than one apparition ~90 % are lost! We need to find a way to improve these numbers by: Prevent the new ones from being lost “Recover” some of the lost ones How to do it There are basically three ways to deal with this problem: Extend the observed arc at the discovery apparition Attempt wide-field recoveries at the next apparition Try to locate precovery observations in existing archives These goals can be achieved using: Large aperture telescopes Wide-field imagers Large repositories of astronomical images The observational network ~ 100 collaborators worldwide Plus all of you who More than a dozen telescopes with helped us over the various apertures years with your A wide range of observing techniques observations (astrometry, lightcurves, visual and IR Thank you! colors, spectroscopy, polarimetry, …) ESA Optical Ground Station (OGS) A 1.0 meter ESA telescope in Tenerife, Canary Islands. Originally designed for satellite optical communication experiments. We have 4 to 8 nights per month, around new Moon. ESA Optical Ground Station (OGS) Follow-up activities The OGS is one of the few follow-up facilities that can reach magnitude 22. In 2015 we have: Observed ~250 NEO observed (~20 per run) ~10-15 NEO candidates targeted every night (>50 % turn out to be -
Instrumental Methods for Professional and Amateur
Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, Francois Colas, Alain Klotz, Christophe Pellier, Jean-Marc Petit, Philippe Rousselot, et al. To cite this version: Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, et al.. Instru- mental Methods for Professional and Amateur Collaborations in Planetary Astronomy. Experimental Astronomy, Springer Link, 2014, 38 (1-2), pp.91-191. 10.1007/s10686-014-9379-0. hal-00833466 HAL Id: hal-00833466 https://hal.archives-ouvertes.fr/hal-00833466 Submitted on 3 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy O. Mousis, R. Hueso, J.-P. Beaulieu, S. Bouley, B. Carry, F. Colas, A. Klotz, C. Pellier, J.-M. Petit, P. Rousselot, M. Ali-Dib, W. Beisker, M. Birlan, C. Buil, A. Delsanti, E. Frappa, H. B. Hammel, A.-C. Levasseur-Regourd, G. S. Orton, A. Sanchez-Lavega,´ A. Santerne, P. Tanga, J. Vaubaillon, B. Zanda, D. Baratoux, T. Bohm,¨ V. Boudon, A. Bouquet, L. Buzzi, J.-L. Dauvergne, A. -
Asteroid Precovery. a Citizen-Science Project Using the Virtual Observatory
Highlights of Spanish Astrophysics VII, Proceedings of the X Scientific Meeting of the Spanish Astronomical Society held on July 9 - 13, 2012, in Valencia, Spain. J. C. Guirado, L.M. Lara, V. Quilis, and J. Gorgas (eds.) Asteroid precovery. A citizen-science project using the Virtual Observatory Carlos Rodrigo1;2, Enrique Solano1;2, and Rebeca Pulido1;2 1 Dpt. Astrofisica, CAB (INTA-CSIC), ESAC Campus. P.O. Box 78. 28691 Villanueva de la Ca~nada,Madrid, Spain 2 Spanish Virtual Observatory (SVO) Abstract Precovery is the process of finding an astronomical object in archive data taken before the discovery of the object. The Virtual Observatory project makes it much easier to access large collection of images in astronomical archives and, thus, opens the possibility to explore them to find more information about certain objects, for instance, Near Earth Asteroids. We have started a citizen-science project that combines some automatic algorithms, Virtual Observatory techniques and the participation of many people that, not being professional astronomers, help to find professional results and make a significant contribution to the accurate knowledge of the orbits of NEAs. The project started in July 2011 and during its first year more than 3000 registered users have collaborated to make more than 164.000 measurements corresponding to around 7600 archive images and 1000 different NEAs. As a result of this work, around 2300 new data, for more than 500 objects, have been submitted to the Minor Planet Center for publication. The great reception of the system as well as the results obtained makes it a valuable and reliable tool for improving the orbital parameters of Near Earth Asteroids. -
Digital Tracking Observations Can Discover Asteroids Ten Times
Digital Tracking Observations Can Discover Asteroids Ten Times Fainter than Conventional Searches Aren N. Heinze1,2, Stanimir Metchev3,4,1, and Joseph Trollo3 ABSTRACT We describe digital tracking, a method for asteroid searches that greatly increases the sensitivity of a telescope to faint unknown asteroids. It has been previously used to detect faint Kuiper Belt objects using the Hubble Space Telescope and large ground- based instruments, and to find a small, fast-moving asteroid during a close approach to Earth. We complement this earlier work by developing digital tracking methodology for detecting asteroids using large-format CCD imagers. We demonstrate that the tech- nique enables the ground-based detection of large numbers of new faint asteroids. Our methodology resolves or circumvents all major obstacles to the large-scale application of digital tracking for finding main belt and near-Earth asteroids. We find that for both asteroid populations, digital tracking can deliver a factor of ten improvement over conventional searches. Digital tracking has long been standard practice for deep Kuiper Belt surveys, but even there our methodology enables deeper integrations than have yet been attempted. Our search for main belt asteroids using a one-degree imager on the 0.9m WIYN telescope on Kitt Peak validates our methodology, delivers sensitivity to asteroids in a regime previously probed only with 4-meter and larger instruments, and leads to the detection of 156 previously unknown asteroids and 59 known objects in a single field. Digital tracking has the potential to revolutionize searches for faint moving objects ranging from the Kuiper Belt through main belt and near-Earth asteroids, and perhaps even anthropogenic space debris in low Earth orbit. -
Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 8-2012 Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA Merek Austin Chertkow University of Tennessee, Knoxville, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Part of the Other Astrophysics and Astronomy Commons Recommended Citation Chertkow, Merek Austin, "Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA. " PhD diss., University of Tennessee, 2012. https://trace.tennessee.edu/utk_graddiss/1463 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Merek Austin Chertkow entitled "Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Physics. William Hix, Major Professor We have read this dissertation and recommend its acceptance: Kate Jones, Mike Guidry, Robert, Hinde Accepted for the Council: Carolyn R. Hodges Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Advancements in Modeling Self-Consistent Core-Collapse Supernovae with CHIMERA A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Merek Austin Chertkow August 2012 c by Merek Austin Chertkow, 2012 All Rights Reserved. -
FINAL PROGRAM #Aiaascitech
4–8 JANUARY 2016 SAN DIEGO, CA The Largest Event for Aerospace Research, Development, and Technology FINAL PROGRAM www.aiaa-SciTech.org #aiaaSciTech 16-928 WHAT’S IMPOSSIBLE TODAY WON’T BE TOMORROW. AT LOCKHEED MARTIN, WE’RE ENGINEERING A BETTER TOMORROW. We are partnering with our customers to accelerate manufacturing innovation from the laboratory to production. We push the limits in additive manufacturing, advanced materials, digital manufacturing and next generation electronics. Whether it is solving a global crisis like the need for clean drinking water or travelling even deeper into space, advanced manufacturing is opening the doors to the next great human revolution. Learn more at lockheedmartin.com © 2014 LOCKHEED MARTIN CORPORATION VC377_164 Executive Steering Committee AIAA SciTech 2016 2O16 Welcome Welcome to the AIAA Science and Technology Forum and Exposition 2016 (AIAA SciTech 2016) – the world’s largest event for aerospace research, development, and technology. We are confident that you will come away from San Diego inspired and with the tools necessary to continue shaping the future of aerospace in new and exciting ways. From hearing preeminent industry thought leaders, to attending sessions where cutting- edge research will be unveiled, to interacting with peers – this will be a most fulfilling week! Our organizing committee has worked hard over the past year to ensure that our plenary sessions examine the most critical issues facing aerospace today, such as aerospace science and Richard George Lesieutre technology policy, lessons learned from a half century of aerospace innovation, resilient design, Christiansen The Pennsylvania and unmanned aerial systems. We will also focus on how AIAA and other stakeholders in State University Sierra Lobo, Inc. -
Abstracts of Extreme Solar Systems 4 (Reykjavik, Iceland)
Abstracts of Extreme Solar Systems 4 (Reykjavik, Iceland) American Astronomical Society August, 2019 100 — New Discoveries scope (JWST), as well as other large ground-based and space-based telescopes coming online in the next 100.01 — Review of TESS’s First Year Survey and two decades. Future Plans The status of the TESS mission as it completes its first year of survey operations in July 2019 will bere- George Ricker1 viewed. The opportunities enabled by TESS’s unique 1 Kavli Institute, MIT (Cambridge, Massachusetts, United States) lunar-resonant orbit for an extended mission lasting more than a decade will also be presented. Successfully launched in April 2018, NASA’s Tran- siting Exoplanet Survey Satellite (TESS) is well on its way to discovering thousands of exoplanets in orbit 100.02 — The Gemini Planet Imager Exoplanet Sur- around the brightest stars in the sky. During its ini- vey: Giant Planet and Brown Dwarf Demographics tial two-year survey mission, TESS will monitor more from 10-100 AU than 200,000 bright stars in the solar neighborhood at Eric Nielsen1; Robert De Rosa1; Bruce Macintosh1; a two minute cadence for drops in brightness caused Jason Wang2; Jean-Baptiste Ruffio1; Eugene Chiang3; by planetary transits. This first-ever spaceborne all- Mark Marley4; Didier Saumon5; Dmitry Savransky6; sky transit survey is identifying planets ranging in Daniel Fabrycky7; Quinn Konopacky8; Jennifer size from Earth-sized to gas giants, orbiting a wide Patience9; Vanessa Bailey10 variety of host stars, from cool M dwarfs to hot O/B 1 KIPAC, Stanford University (Stanford, California, United States) giants. 2 Jet Propulsion Laboratory, California Institute of Technology TESS stars are typically 30–100 times brighter than (Pasadena, California, United States) those surveyed by the Kepler satellite; thus, TESS 3 Astronomy, California Institute of Technology (Pasadena, Califor- planets are proving far easier to characterize with nia, United States) follow-up observations than those from prior mis- 4 Astronomy, U.C. -
Mining the ESO WFI and INT WFC Archives for Known Near Earth
Astron. Nachr. / AN 000, No.00, 1–9 (0000)/ DOI please set DOI! Mining the ESO WFI and INT WFC archives for known Near Earth Asteroids. Mega-Precovery software ⋆ O. Vaduvescu1,2,3,⋆⋆, M. Popescu2,4,7, I. Comsa5, A. Paraschiv9,10, D. Lacatus9,10, A. Sonka6,7, A. Tudorica11,12, M. Birlan2, O. Suciu5,13, F. Char14, M. Constantinescu7, T. Badescu8,12, M. Badea8,11,12, D. Vidican7, C. Opriseanu7 1 Isaac Newton Group of Telescopes, Apartado de Correos 321, E-38700 Santa Cruz de la Palma, Canary Islands, Spain 2 IMCCE, Observatoire de Paris, 77 Avenue Denfert-Rochereau, 75014 Paris Cedex, France 3 Instituto de Astrofisica de Canarias, c/Via Lactea s/n, 38200 La Laguna, Tenerife, Spain 4 Polytechnic University of Bucharest, Faculty of Applied Sciences, Department of Physics, Bucharest, Romania 5 Babes-Bolyai University, Faculty of Mathematics and Informatics, 400084 Cluj-Napoca, Romania 6 Admiral Vasile Urseanu Observatory, B-dul Lascar Catargiu 21, sect 1, Bucharest, Romania 7 Bucharest Astroclub, B-dul Lascar Catargiu 21, sect 1, Bucharest, Romania 8 University of Bucharest, Faculty of Physics, Str. Atomistilor 405, 077125 Magurele - Ilfov, Romania 9 Institute of Geodynamics Sabba S. Stefanescu, Jean-Louis Calderon 19-21, Bucharest, Romania, RO-020032, Romania 10 Research Center for Atomic Physics and Astrophysics, Faculty of Physics, University of Bucharest, Atomistilor 405, CP Mg-11, 077125 Magurele - Ilfov, Romania 11 Bonn Cologne Graduate School of Physics and Astronomy, Germany 12 Rheinische-Friedrich-Wilhelms Universitaet Bonn, Argelander-Institut -
Arxiv:2103.08788V1 [Astro-Ph.EP] 16 Mar 2021
manuscript submitted to JGR: Planets 1I/`Oumuamua as an N2 ice fragment of an exo-Pluto surface: I. Size and Compositional Constraints Alan P. Jackson1∗, Steven J. Desch1† 1School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85087 Key Points: • A fragment of N2 ice would satisfy all known constraints on `Oumuamua's size, composition, and acceleration. • The presence of N2 ice in the solar system on Pluto makes it likely `Oumuamua is such a fragment • The existence of `exo-Plutos' in other stellar systems must be common. arXiv:2103.08788v1 [astro-ph.EP] 16 Mar 2021 ∗ORC-ID 0000-0003-4393-9520 †ORC-ID 0000-0002-1571-0836 Corresponding author: Alan P. Jackson, [email protected] {1{ manuscript submitted to JGR: Planets Abstract The origin of the interstellar object 1I/`Oumuamua has defied explanation. We perform calculations of the non-gravitational acceleration that would be experienced by bodies composed of a range of different ices and demonstrate that a body composed of N2 ice would satisfy the available constraints on the non-gravitational acceleration, size and albedo, and lack of detectable emission of CO or CO2 or dust. We find that `Oumuamua was small, with dimensions 45 m × 44 m × 7.5 m at the time of observation at 1.42 au from the Sun, with a high albedo of 0.64. This albedo is consistent with the N2 surfaces of bodies like Pluto and Triton. We estimate `Oumuamua was ejected about 0.4-0.5 Gyr ago from a young stellar system, possibly in the Perseus arm.