NASA's New Horizons
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Your abstract submission has been received Print this page You have submitted the following abstract to GSA Annual Meeting in Denver, Colorado, USA - 2016. Receipt of this notice does not guarantee that your submission was complete or free of errors. PLUTO IS THE NEW MARS! MOORE, Jeffrey M.1, MCKINNON, William B.2, SPENCER, John R.3, HOWARD, Alan D.4, GRUNDY, William M.5, STERN, S. Alan3, WEAVER, Harold A.6, YOUNG, Leslie A.3, ENNICO, Kimberly1 and OLKIN, Cathy3, (1)NASA Ames Research Center, Space Science Division, MS-245-3, Moffett Field, CA 95129, (2)Washington University, Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, One Brookings Drive, Saint Louis, MO 63130, (3)Southwest Research Institute, Boulder, CO 80302, (4)Department of Environmental Sciences, Univerisity of Virginia, PO Box 400123, Charlottesville, VA 22904-4123, (5)Lowell Observatory, Flagstaff, AZ 86001, (6)Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, [email protected] Data from NASA’s New Horizons encounter with Pluto in July 2015 revealed an astoundingly complex world. The surface seen on the encounter hemisphere ranged in age from ancient to recent. A vast craterless plain of slowly convecting solid nitrogen resides in a deep primordial impact basin, reminiscent of young enigmatic deposits in Mars’ Hellas basin. Like Mars, regions of Pluto are dominated by valleys, though the Pluto valleys are thought to be carved by nitrogen glaciers. Pluto has fretted terrain and halo craters. Pluto is cut by tectonics of several different ages. Like Mars, vast tracts on Pluto are mantled by dust and volatiles. -
New Horizons Pluto/KBO Mission Impact Hazard
New Horizons Pluto/KBO Mission Impact Hazard Hal Weaver NH Project Scientist The Johns Hopkins University Applied Physics Laboratory Outline • Background on New Horizons mission • Description of Impact Hazard problem • Impact Hazard mitigation – Hubble Space Telescope plays a key role New Horizons: To Pluto and Beyond The Initial Reconnaissance of The Solar System’s “Third Zone” KBOs Pluto-Charon Jupiter System 2016-2020 July 2015 Feb-March 2007 Launch Jan 2006 PI: Alan Stern (SwRI) PM: JHU Applied Physics Lab New Horizons is NASA’s first New Frontiers Mission Frontier of Planetary Science Explore a whole new region of the Solar System we didn’t even know existed until the 1990s Pluto is no longer an outlier! Pluto System is prototype of KBOs New Horizons gives the first close-up view of these newly discovered worlds New Horizons Now (overhead view) NH Spacecraft & Instruments 2.1 meters Science Team: PI: Alan Stern Fran Bagenal Rick Binzel Bonnie Buratti Andy Cheng Dale Cruikshank Randy Gladstone Will Grundy Dave Hinson Mihaly Horanyi Don Jennings Ivan Linscott Jeff Moore Dave McComas Bill McKinnon Ralph McNutt Scott Murchie Cathy Olkin Carolyn Porco Harold Reitsema Dennis Reuter Dave Slater John Spencer Darrell Strobel Mike Summers Len Tyler Hal Weaver Leslie Young Pluto System Science Goals Specified by NASA or Added by New Horizons New Horizons Resolution on Pluto (Simulations of MVIC context imaging vs LORRI high-resolution "noodles”) 0.1 km/pix The Best We Can Do Now 0.6 km/pix HST/ACS-PC: 540 km/pix New Horizons Science Status • -
New Horizons: Reconnaissance of the Pluto-Charon System and The
C.T. Russell Editor New Horizons Reconnaissance of the Pluto-Charon System and the Kuiper Belt Previously published in Space Science Reviews Volume 140, Issues 1–4, 2008 C.T. Russell Institute of Geophysics & Planetary Physics University of California Los Angeles, CA, USA Cover illustration: NASA’s New Horizons spacecraft was launched on 2006 January 19, received a grav- ity assist during a close approach to Jupiter on 2007 February 28, and is now headed for a flyby with closest approach 12,500 km from the center of Pluto on 2015 July 14. This artist’s depiction shows the spacecraft shortly after passing above Pluto’s highly variegated surface, which may have black-streaked surface deposits produced from cryogenic geyser activity, and just before passing into Pluto’s shadow when solar and earth occultation experiments will probe Pluto’s tenuous, and possibly hazy, atmosphere. Sunlit crescents of Pluto’s moons Charon, Nix, and Hydra are visible in the background. After flying through the Pluto system, the New Horizons spacecraft could be re-targeted towards other Kuiper Belt Objects in an extended mission phase. This image is based on an original painting by Dan Durda. © Dan Durda 2001 All rights reserved. Back cover illustration: The New Horizons spacecraft was launched aboard an Atlas 551 rocket from the NASA Kennedy Space Center on 2008 January 19 at 19:00 UT. Library of Congress Control Number: 2008944238 DOI: 10.1007/978-0-387-89518-5 ISBN-978-0-387-89517-8 e-ISBN-978-0-387-89518-5 Printed on acid-free paper. -
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. -
+ New Horizons
Media Contacts NASA Headquarters Policy/Program Management Dwayne Brown New Horizons Nuclear Safety (202) 358-1726 [email protected] The Johns Hopkins University Mission Management Applied Physics Laboratory Spacecraft Operations Michael Buckley (240) 228-7536 or (443) 778-7536 [email protected] Southwest Research Institute Principal Investigator Institution Maria Martinez (210) 522-3305 [email protected] NASA Kennedy Space Center Launch Operations George Diller (321) 867-2468 [email protected] Lockheed Martin Space Systems Launch Vehicle Julie Andrews (321) 853-1567 [email protected] International Launch Services Launch Vehicle Fran Slimmer (571) 633-7462 [email protected] NEW HORIZONS Table of Contents Media Services Information ................................................................................................ 2 Quick Facts .............................................................................................................................. 3 Pluto at a Glance ...................................................................................................................... 5 Why Pluto and the Kuiper Belt? The Science of New Horizons ............................... 7 NASA’s New Frontiers Program ........................................................................................14 The Spacecraft ........................................................................................................................15 Science Payload ...............................................................................................................16 -
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. -
New Horizons SOC to Instrument Pipeline ICD
New Horizons SOC to Instrument Pipeline ICD September 2017 SwRI® Project 05310 Document No. 05310-SOCINST-01 Contract NASW-02008 Prepared by SOUTHWEST RESEARCH INSTITUTE® Space Science and Engineering Division 6220 Culebra Road, San Antonio, Texas 78228-0510 (210) 684-5111 FAX (210) 647-4325 Southwest Research Institute 05310-SOCINST-01 Rev 0 Chg 0 New Horizons SOC to Instrument Pipeline ICD Page ii New Horizons SOC to Instrument Pipeline ICD SwRI Project 05310 Document No. 05310-SOCINST-01 Contract NASW-02008 Prepared by: Joe Peterson 08 November 2013 Revised by: Brian Carcich August, 2014 Revised by: Tiffany Finley March, 2016 Revised by: Tiffany Finley October, 2016 Revised by: Brian Carcich December, 2016 Revised by: Tiffany Finley, Brian Carcich, PEPSSI team April, 2017 Revised by: Tiffany Finley, PEPSSI team September, 2017 Contributors: ALICE specifics prepared by: Maarten Versteeg, Joel Parker, & Andrew Steffl LEISA specifics prepared by: George McCabe & Allen Lunsford LORRI specifics prepared by: Hal Weaver & Howard Taylor MVIC specifics prepared by: Cathy Olkin PEPSSI specifics prepared by: Stefano Livi, Matthew Hill, Lawrence Brown, & Peter Kollman REX specifics prepared by: Ivan Linscott & Brian Carcich SDC specifics prepared by: David James SWAP specifics prepared by: Heather Elliott Southwest Research Institute 05310-SOCINST-01 Rev 0 Chg 0 New Horizons SOC to Instrument Pipeline ICD Page iii General Approval Signatures: Approved by: ____________________________________ Date: ____________ Hal Weaver, JHU/APL, Project Scientist -
Every Planet Is a Comet to a Space Physicist: from Jupiter to Pluto HAO
Fran Bagenal HAO Visiting University of Colorado Scientist 1987 - 1988 Every Planet is a Comet to a Space Physicist: From Jupiter to Pluto New Horizons! EARTH ! Side! Mission To Pluto !Juno Solar! Wind! Equatorial plane! Connected – Global circulation Polar view! to solar wind! driven by solar wind! – Coupled to the planet Closed magnetic – Large scale, quasi- field! static reconnection! Delamere & Bagenal 2010, 2013! – Io#=#primary# source# # –##Coupled#to# rota4ng#planet## Delamere & Bagenal The aurora is the signature 2010, 2013! of Jupiter’s attempt to spin up its magnetosphere –##Io#plasma# ejected#as# plasmoids# ?! # –##Boundary#layer# interac4on#via# small:scale# ?! intermi;ant# reconnec4on # SIDE VIEW Juno –##Minimal#solar# wind# Juno ionosphere# High-M coupling# A TOP VIEW solar wind EQUATORIAL # PLANE –##Viscous# boundary#layers# # High-β plasma TOP – Io plasma VIEW carried away ABOVE SHEATH Orbit insertion by solar wind# 4th July 2016 Juno Juno Juno passes directly through Juno passes directly through auroral field lines auroral field lines Measures particles precipitating Measures particles precipitatingIs Jupiter a into atmosphere creating aurora into atmosphere creating aurora colossal comet?? Plasma/radio waves reveal Plasma/radio waves reveal processes responsible for particle processes responsible for particle acceleration acceleration UV & IR images provides context UV & IR images provides context for in-situ observations for in-situ observations Juno’s orbit: perfect for exploring polar magnetosphere Juno’s orbit: perfect -
Five Years After a Jaw-Dropping Fly-By, Images of the Dwarf Planet's Far Side Reveal Possible Signs of Liquid Water, Mysteriou
Feature As the New Horizons spacecraft approached Pluto in 2015, it captured one part — the ‘near side’ — in high resolution (bottom) and the ‘far side’ at a lower resolution (top). The dark side of Pluto Five years after a jaw-dropping fly-by, images of the dwarf planet’s far side reveal possible signs of liquid water, mysterious shards of ice and new theories for the frigid world’s birth. By Shannon Hall NASA/JHUAPL/SWRI 674 | Nature | Vol 583 | 30 July 2020 ©2020 Spri nger Nature Li mited. All rights reserved. ©2020 Spri nger Nature Li mited. All rights reserved. hen NASA’s New Horizons their origin one of the biggest mysteries on fuzzy, the images revealed a world — at that spacecraft zipped past Pluto the dwarf planet. time still defined as a planet — that had more in 2015, it showed a world that “Pluto is the gift that keeps on giving,” says large-scale contrast than any other in the was much more dynamic than Richard Binzel, a planetary scientist at the Solar System, except Earth. anyone had imagined. The Massachusetts Institute of Technology in Cam- It was a tantalizing hint that suggested dwarf planet hosts icy nitro- bridge and a New Horizons co-investigator. Pluto might be a dynamic world — and was gen cliffs that resemble the quickly verified in July 2015 when New Hori- rugged coast of Norway, and A splashy start zons famously spotted a heart-shaped fea- Wgiant shards of methane ice that soar to the When Clyde Tombaugh, a young astronomer ture just north of the near side’s equator. -
The Long Duration New Horizons (NH) Mission to Pluto, Its
IAC-04-A.8.01 NEW HORIZONS MISSION TO PLUTO/CHARON: REDUCING COSTS OF A LONG-DURATION MISSION Alice F. Bowman Johns Hopkins University Applied Physics Laboratory, Laurel, MD (USA) [email protected] Albert A. Chacos, Christopher C. DeBoy, R. Michael Furrow, Karl E. Whittenburg Johns Hopkins University Applied Physics Laboratory, Laurel, MD (USA) [email protected], [email protected], [email protected], [email protected] ABSTRACT The long-duration and long light-time delay of NASA’s planned New Horizons mission to Pluto, its moon Charon, and the extended mission to one or more Kuiper Belt Objects poses unique chal- lenges to mission operations, especially in this time of limited space exploration budgets. A num- ber of courses of action can be followed to reduce wear on Observatory hardware, reduce opera- tions staffing costs, and reduce Deep Space Network usage and costs without sacrificing the health and safety of the Observatory or risking the successful completion of the primary mission. Major components in this system are an autonomy subsystem that can react quickly enough to safe the Observatory when it is out of contact with the ground station; the use of a beacon to indi- cate the health of the Observatory during the dormant phases of the mission; command loading and verification strategies to accommodate the long light-time delays; and the combining of op- erations personnel to take advantage of similarities of Observatories, supporting ground station setup, and procedures. When planned early in the mission development phase, these compo- nents are easily integrated into the operations concept and Observatory hardware to form a co- hesive plan to mitigate cost and risk. -
New Horizons Pluto Flyby
National Aeronautics and Space Administration PRESS KIT | July 2015 New Horizons Pluto Flyby www.nasa.gov Table of Contents NASA’s New Horizons Nears Historic Pluto Flyby .................................................................................................... 5 Media Services Information .................................................................................................................................... 6 Quick Facts .............................................................................................................................................................. 7 Meet Pluto ............................................................................................................................................................... 9 Why Pluto and the Kuiper Belt? .............................................................................................................................12 The Science of New Horizons ................................................................................................................................12 New Horizons Science Team .................................................................................................................................17 Mission Overview ...................................................................................................................................................18 Spacecraft Systems and Components .................................................................................................................. -
Flier 1 May 2020
MAY 2020 VOL. XLVIII, No .7 Published by and for the AIAA Long Island Section, The coronavirus (COVID-19) continues to spread. P.O. Box 491, Bethpage, NY 11714 OFFICERS: Please do everything you can to stay healthy. Here Chairman: Dave Paris (516) 458-8593 [email protected] is what the Centers for Disease Control (CDC) Vice-Chair: Greg Homatas (718) 812-2727 [email protected] recommends and what we urge you to do: Secretary: Nick DiZinno (631) 252-3440 [email protected] Treasurer: W. Glenn Mackey (631) 368-0433 [email protected] • If you’re sick or feeling unwell, stay home COUNCIL MEMBERS: • Stay home as much as possible Anthony Agnone, Joseph Fragola, Muhammad Hayan, Peter Kontogiannis, John Leylegian, Ron McCaffrey, • Avoid crowds as much as possible. Emil Schoonejans, Jason Tyll, and Gerry Yurchison • Avoid non-essential travel by car, airplane FLIER EDITORS: • Maintain 6-foot safety distances Dave Paris, [email protected] • Make sure to cover your cough or sneeze W. Glenn Mackey, [email protected] FLIER PUBLISHER: with a tissue, then throw it away or cough or Nick DiZinno (631) 252-3440 [email protected] SECTION WEBSITE: sneeze into your sleeve at the elbow https://engage.aiaa.org/longisland/ • Clean and disinfect things you use often like Webmaster: Nick DiZinno counters, bathrooms, and your cell phone • Wash your hands often with soap and water Note from the Chairman for a minimum of 20 seconds • Avoid contact with sick people Due to the scheduling delays and chaos resulting from • If you have questions or start to feel sick, the Coronavirus infestation, the Long Island Section call your healthcare provider Council has decided to accept the recommendation of • Follow the guidance from the CDC.