Visions Into Voyages for Planetary Sciences in the Decade 2013-2022: a Midterm Review
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Planetary Report Report
The PLANETARYPLANETARY REPORT REPORT Volume XXI Number 2 March/April 2001 Farewell, Mir Inside— The Planetary Society’s Cosmos 1: The First Solar Sail On the Cover: Volume XXI When Mir launched in February 1986, it was a show- Table of Number 2 case of Russian technology. But after 15 years of hard work, the aged space station has ended its run. Contents March/April 2001 This view of Mir over Earth’s blue skies was imaged during a fly-around by the space shuttle Atlantis follow- ing the joint docking activities between the two crews. Image: JSC/NASA Features Farewell to a Cold Warrior: Mir Station Obituary 4 As head of the Space Research Institute of the Soviet Academy of Sciences, Roald Sagdeev was there at the birth of the Mir space station. As an adviser to Soviet leader Mikhail Gorbachev, he watched Mir’s changing role in international space policy. Then, after marrying From Susan Eisenhower, the American president’s granddaughter, he moved to the United States The and saw Mir from a different perspective. A member of The Planetary Society’s Board of Editor Directors, he shares with Society members his memories of the long-lived space station. 8 A Bold New Voyage: he Planetary Society is preparing to The Planetary Society Prepares to Fly a Solar Sail It’s the first time a membership organization has undertaken an actual space mission, and launch its first space mission: the T only The Planetary Society is audacious enough to do it. This is the story of how we plan to Cosmos 1 solar sail. -
Arxiv:2001.00125V1 [Astro-Ph.EP] 1 Jan 2020
Draft version January 3, 2020 Typeset using LATEX default style in AASTeX61 SIZE AND SHAPE CONSTRAINTS OF (486958) ARROKOTH FROM STELLAR OCCULTATIONS Marc W. Buie,1 Simon B. Porter,1 et al. 1Southwest Research Institute 1050 Walnut St., Suite 300, Boulder, CO 80302 USA To be submitted to Astronomical Journal, Version 1.1, 2019/12/30 ABSTRACT We present the results from four stellar occultations by (486958) Arrokoth, the flyby target of the New Horizons extended mission. Three of the four efforts led to positive detections of the body, and all constrained the presence of rings and other debris, finding none. Twenty-five mobile stations were deployed for 2017 June 3 and augmented by fixed telescopes. There were no positive detections from this effort. The event on 2017 July 10 was observed by SOFIA with one very short chord. Twenty-four deployed stations on 2017 July 17 resulted in five chords that clearly showed a complicated shape consistent with a contact binary with rough dimensions of 20 by 30 km for the overall outline. A visible albedo of 10% was derived from these data. Twenty-two systems were deployed for the fourth event on 2018 Aug 4 and resulted in two chords. The combination of the occultation data and the flyby results provides a significant refinement of the rotation period, now estimated to be 15.9380 ± 0.0005 hours. The occultation data also provided high-precision astrometric constraints on the position of the object that were crucial for supporting the navigation for the New Horizons flyby. This work demonstrates an effective method for obtaining detailed size and shape information and probing for rings and dust on distant Kuiper Belt objects as well as being an important source of positional data that can aid in spacecraft navigation that is particularly useful for small and distant bodies. -
Astronomy Educator Profiles
Astronomy Educator Profiles Alexis Ann Acohido graduated of the University of Hawaii at Manoa in 2015, where she obtained her Bachelor’s of Science in mathematics. Born and raised on Oahu, she moved to Hawai‘i island last year and is currently part of the Public Information and Outreach department at Gemini Observatory in Hilo, Hawai‘i. In 2013, she was part of the Akamai Workforce Initiative and interned at the Institute for Astronomy on Maui where she worked on parallax ranging methods for point source objects. Alexis Ann Acohido Gemini Observatory Contact: [email protected] Christian Andersen is the Operations Manager at the Pacific International Space Center for Exploration Systems (PISCES), and leads the agency’s additive manufacturing & construction projects at its Laser Lava Lab. Andersen started his career conducting research in inertial confinement fusion at Lawrence Livermore National Laboratory, Ecole Polytechnique, and Rutherford Appleton Laboratories. As Operations Manager, he’s worked on a variety of PISCES projects in transitioning aerospace technologies to terrestrial applications and analogue field testing. Andersen is also a Lecturer and Affiliate Faculty in the Physics & Astronomy Department at the University of Hawaii at Hilo, and the Vice- Chair of the Space Resources Technical Committee for the AIAA (American Institute of Aeronautics and Astronautics). He holds a B.S. in Physics from San Jose State University and a M.S. in Engineering from Christian Andersen U.C. Davis. PISCES Contact: [email protected] Virginia Aragon-Barnes had a passion for science and a natural curiosity about how and why things worked from a very early age. -
Publication in the Bulletin
Lunar and Planetary Information Bulletin July 2019 • Issue 157 Contents Featured Story From the Desk of Lori Glaze News From Space Meeting Highlights Spotlight on Education In Memoriam Milestones New and Noteworthy Calendar Featured Story Featured Story A Personal Journey to Ultima Thule: New Horizons in the Kuiper Belt As the New Horizons science team gathered in Laurel, Paul Schenk, Brian May, Joel Parker, and Andy Chaikin discuss a possible shape model for Ultima Thule, January 1, 2019. Credit: E. Whitman. Maryland, during the last week of 2018, many of us reflected back on a similar gathering three-and-a-half years earlier. In the summer of 2015, we all came together on a voyage of exploration to the planet Pluto and its moons. At that time, we didn’t know very much about our target, and this time we knew even less about “Ultima Thule,” a small, lonely 30-kilometer- wide object known as 2014 MU69 that was orbiting the Sun almost half a billion kilometers beyond Pluto. Unlike what we knew about Pluto, we did not even know Ultima Thule’s surface composition, its shape, or even the length of its day. We knew Ultima Thule was much smaller than — and hence would be a very different beast from — Pluto. So as the New Horizons team arrived at the Applied Physics Laboratory (APL) in Laurel, Maryland, to watch and enjoy the encounter sequence play out, we were completely in the dark. The only clues we had were stellar occultation observations of Ultima Thule from Argentina in 2017 that indicated it was elongate and might have either two separate or contacting lobes. -
New Horizons Ultima Thule Flyby Events
New Horizons Ultima Thule Flyby Events – Dec 31, 2018 – Jan 3, 2019 Event Date/Time Communications Event Speaker 31 Dec 12:00 PM K‐Center Opens at Noon Guest Ops team 1:00 Welcome Adrian Hill and VIP Welcome 1:05 The New Horizons Mission Alan Stern 1:25 What is the Kuiper Belt and what are Kuiper Belt Hal Weaver Objects 1:30 What We Know About MU69 – Ultima Thule Cathy Olkin 1:35 The Flyby of MU69 – Ultima Thule John Spencer NYE press 2:00 – 3:00 Daily media update on Webcast Mike Buckley; panel: Alan Stern, Helene Winters, John Spencer, Fred Pelletier. 3:15 ‐ 3:45 Flyby Ask Me Anything Webcast Moderator Adrian Hill; Panelists: Kelsi Singer; Alex Parker; Gabe Rogers 3:45 – 3:50 Song ‐ Acoustic Craig Werth – move to dining area 3:50 ‐ 4:45 Exploration for Kids Janet Ivey of Janet’s Planet ‐ dining area 4:45‐4:50 Closeout Afternoon 5:00 Doors Close for 2 hours – dinner break 7:00 PM K center reopens Kick off. 8:00 Welcome Adrian Hill and VIPs 8:10 Solar System Archaeology Ken Lacovara 8:15 NASA’s Study of Ancient Bodies. Small bodies mission panel. OSIRIS‐REx (Barnouin), Lucy (Levison), Psyche (Elkins), NH (Stern) *NASA Rep 9:00 Short break Transition to Guest ops. 9:15 Craig Werth Video Craig Werth 9:20 Doing Geology by Looking Up; Doing Walter Alvarez Astronomy by Looking Down 9:35 Pluto Flyby: Summer of 2015 Hal Weaver 9:50 Pluto and the Human Imagination David Grinspoon 10:10 Break 10:20 Meet the New Horizons Team Alan Stern and Helene Winters 10:30 Finding MU69 – Ultima Thule Marc Buie 10:45 MU69: What we expect to learn Panel: Silvia Protopapa, Hal Weaver, Cathy Olkin, John Spencer 11:00 The Eyes and Ears of New Horizons Kelsi Singer, Kirby Runyon. -
Geochemistry, Geophysics, Geosystems Becoming an Open Access Journal: FAQ
Geochemistry, Geophysics, Geosystems becoming an open access journal: FAQ Why is Geochemistry, Geophysics, Geosystems becoming an open access journal? AGU remains committed to open science and open data. As a part of our mission, we are focused on making science available to the widest possible audience. Since many researchers around the world have open access requirements by funders, this move to an open access model will make compliance easier. Authors will pay an open access article processing charge (APC) and retain copyright of their article which they can publish under a Creative Commons license (choose from CC-BY or CC-BY-NC-ND). There will be no excess page fees or any other additional fees for publication. In addition, there will be no subscription paywall, which means that more people will have access to your research so they can actively cite, read and share data for free. When will Geochemistry, Geophysics, Geosystems become open access? All articles in the journal will be open access as of 1 January 2022. After 8 September 2021, submissions received/accepted must agree to pay the open access article processing charge (APC), but there will be no excess page fees or any other additional fees for publication. What if I already have a paper under consideration to Geochemistry, Geophysics, Geosystems? If your paper: • is under consideration before 8 September 2021 and • publishes after 1 January 2021, then your paper will publish with copyright to the authors under a Creative Commons license for free (the fee will be waived). If your paper publishes in 2021, then the paper will publish as a subscription article (copyright AGU). -