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THE PLANETARY REPORT FAREWELL, SEPTEMBER EQUINOX 2017 VOLUME 37, NUMBER 3 CASSINI Planetary.Org CELEBRATING a LEGACY of DISCOVERIES
THE PLANETARY REPORT FAREWELL, SEPTEMBER EQUINOX 2017 VOLUME 37, NUMBER 3 CASSINI planetary.org CELEBRATING A LEGACY OF DISCOVERIES ATMOSPHERIC CHANGES C DYNAMIC RINGS C COMPLICATED TITAN C ACTIVE ENCELADUS ABOUT THIS ISSUE LINDA J. SPILKER is Cassini project scientist at the Jet Propulsion Laboratory. IN 2004, Cassini, the most distant planetary seafloor. As a bonus, it has revealed jets of orbiter ever launched by humanity, arrived at water vapor and ice particles shooting out of Saturn. For 13 years, through its primary and fractures at the moon’s south pole. two extended missions, this spacecraft has These discoveries have fundamentally been making astonishing discoveries, reshap- altered many of our concepts of where life ing and changing our understanding of this may be found in our solar system. Cassini’s unique planetary system within our larger observations at Enceladus and Titan have made system of unique worlds. A few months ater exploring these ocean worlds a major focus for arrival, Cassini released Huygens, European planetary science. New insights from these dis- Space Agency’s parachuted probe built to coveries also have implications for potentially study the atmosphere and surface of Titan habitable worlds beyond our solar system. and image its surface for the very first time. In this special issue of The Planetary Report, a handful of Cassini scientists share some results from their studies of Saturn and its moons. Because there’s no way to fit every- thing into this slim volume, they’ve focused on a few highlights. Meanwhile, Cassini continues performing its Grand Finale orbits between the rings and the top of Saturn’s atmosphere, circling the planet once every 6.5 days. -
Spacecraft Imaging for Amateurs an International Community of Space
Planetary Close-ups emily lakdawalla Spacecraft Imaging for Amateurs An international community of space This is Mars’s Big Sky Country, a windswept, nearly featureless plain. Tiny ripples in the rust-colored sand march farther than the eye can see, to a horizon so fl at one might be able to see the curvature of the planet. As far as anyone knows, those ripples have not budged in eons. But all is not still; gaze upward, and you might be surprised by the rapid motion overhead, where feathery cirrus clouds, frosty with bright crystals of water ice, fl oat on high Martian winds. The scene is from Meridiani Planum, composed from eight images captured by the Mars Exploration Rover Opportunity just before she reached a deep crater named Victoria, on the 950th Martian day of her mission. But the beautiful image was not created by anyone on the Mars Exploration Rover team; no scientist would likely have Earthbound produced it, because it owes its beauty as much to art as it observers never does to science. see Mars as a The image is the collaborative creation of a whole crescent, but amateur-imagesmith community; six people, each from spacecraft do. a diff erent country, had a hand in it. Twelve hours after The author cre- Opportunity took the photos, the data had been received on ated this view Earth and posted to the internet. Within another 17 hours, from six images rover fans had found the photos, assembled the mosaic, taken by Viking and shaded the sand and sky based on color photos Oppor- Orbiter 2 in tunity had taken of a similar landscape the day before. -
Nustar Observatory Guide
NuSTAR Guest Observer Program NuSTAR Observatory Guide Version 3.2 (June 2016) NuSTAR Science Operations Center, California Institute of Technology, Pasadena, CA NASA Goddard Spaceflight Center, Greenbelt, MD nustar.caltech.edu heasarc.gsfc.nasa.gov/docs/nustar/index.html i Revision History Revision Date Editor Comments D1,2,3 2014-08-01 NuSTAR SOC Initial draft 1.0 2014-08-15 NuSTAR GOF Release for AO-1 Addition of more information about CZT 2.0 2014-10-30 NuSTAR SOC detectors in section 3. 3.0 2015-09-24 NuSTAR SOC Update to section 4 for release of AO-2 Update for NuSTARDAS v1.6.0 release 3.1 2016-05-10 NuSTAR SOC (nusplitsc, Section 5) 3.2 2016-06-15 NuSTAR SOC Adjustment to section 9 ii Table of Contents Revision History ......................................................................................................................................................... ii 1. INTRODUCTION ................................................................................................................................................... 1 1.1 NuSTAR Program Organization ..................................................................................................................................................................................... 1 2. The NuSTAR observatory .................................................................................................................................... 2 2.1 NuSTAR Performance ........................................................................................................................................................................................................ -
Nustar Unveils a Heavily Obscured Low-Luminosity Active Galactic Nucleus in the Luminous Infrared Galaxy Ngc 6286 C
Draft version October 26, 2015 A Preprint typeset using LTEX style emulateapj v. 04/17/13 NUSTAR UNVEILS A HEAVILY OBSCURED LOW-LUMINOSITY ACTIVE GALACTIC NUCLEUS IN THE LUMINOUS INFRARED GALAXY NGC 6286 C. Ricci1,2,*, et al. Draft version October 26, 2015 ABSTRACT We report on the detection of a heavily obscured Active Galactic Nucleus (AGN) in the Lumi- nous Infrared Galaxy (LIRG) NGC 6286, obtained thanks to a 17.5 ks NuSTAR observation of the source, part of our ongoing NuSTAR campaign aimed at observing local U/LIRGs in different merger stages. NGC6286 is clearly detected above 10keV and, by including the quasi-simultaneous Swift/XRT and archival XMM-Newton and Chandra data, we find that the source is heavily obscured 24 −2 [N H ≃ (0.95 − 1.32) × 10 cm ], with a column density consistent with being mildly Compton- −2 thick [CT, log(N H/cm ) ≥ 24]. The AGN in NGC 6286 has a low absorption-corrected luminosity 41 −1 (L2−10 keV ∼ 3 − 20 × 10 ergs ) and contributes .1% to the energetics of the system. Because of its low-luminosity, previous observations carried out in the soft X-ray band (< 10 keV) and in the in- frared excluded the presence of a buried AGN. NGC 6286 has multi-wavelength characteristics typical of objects with the same infrared luminosity and in the same merger stage, which might imply that there is a significant population of obscured low-luminosity AGN in LIRGs that can only be detected by sensitive hard X-ray observations. 1. INTRODUCTION 2012; Schawinski et al. -
THE PLANETARY REPORT JUNE SOLSTICE 2016 VOLUME 36, NUMBER 2 Planetary.Org
THE PLANETARY REPORT JUNE SOLSTICE 2016 VOLUME 36, NUMBER 2 planetary.org ILLUMINATING CERES DAWN SHEDS NEW LIGHT ON AN ENIGMATIC WORLD BREAKTHROUGH STARSHOT C LIGHTSAIL 2 TEST C MEMBERSHIP UPGRADES SNAPSHOTS FROM SPACE EMILY STEWART LAKDAWALLA blogs at planetary.org/blog. Black Sands of Mars ON SOL 1192 (December 13, 2015), Curiosity approached the side of Namib, a Faccin and Marco Bonora Image: NASA/JPL/MSSS/Elisabetta massive barchan sand dune. Namib belongs to a field of currently active dark basaltic sand dunes that form a long barrier between the rover and the tantalizing rocks of Mount Sharp. This view, processed by Elisabetta Bonora and Marco Faccin, features wind-carved yardangs (crests or ridges ) of Mount Sharp in the background. After taking this set of photos, Curiosity went on to sample sand from the dune, and it is now working its way through a gap in the dune field on the way to the mountain. —Emily Stewart Lakdawalla SEE MORE AMATEUR-PROCESSED SPACE IMAGES planetary.org/amateur SEE MORE EVERY DAY! planetary.org/blogs 2 THE PLANETARY REPORT C JUNE SOLSTICE 2016 CONTENTS JUNE SOLSTICE 2016 COVER STORY Unveiling Ceres 6 Simone Marchi on why Ceres is a scientific treasure chest for Dawn. Pathway to the Stars Looking back at years of Society-led solar sail 10 development as Breakthrough Starshot is announced. Life, the Universe, and Everything 13 Planetary Radio in Death Valley. ADVOCATING FOR SPACE Partisan Peril 18 Casey Dreier looks at the U.S. President’s impact on space policy and legislation. DEVELOPMENTS IN SPACE SCIENCE Update on LightSail 2 20 Bruce Betts details the progress we’ve made in the year since LightSail 1 launched. -
PAC March 9 10 2020 Report
NASA ADVISORY COUNCIL PLANETARY SCIENCE ADVISORY COMMITTEE March 9-10, 2020 NASA Headquarters Washington, DC MEETING REPORT _____________________________________________________________ Anne Verbiscer, Chair ____________________________________________________________ Stephen Rinehart, Executive Secretary Table of Contents Opening and Announcements, Introductions 3 PSD Update and Status 3 PSD R&A Status 5 Planetary Protection 7 Discussion 8 Mars Exploration Program 8 Lunar Exploration Program 9 PDCO 11 Planetary Data System 12 PDS at Headquarters 13 Findings and Discussion 13 General Comments 13 Exoplanets in Our Backyard 14 AP Assets for Solar System Observations 15 Solar System Science with JWST 16 Mercury Group 17 VEXAG 17 SBAG 18 OPAG 19 MEPAG 19 MAPSIT 20 LEAG 21 CAPTEM 21 Discussion 22 Findings and Recommendations Discussion 23 Appendix A- Attendees Appendix B- Membership roster Appendix C- Agenda Appendix D- Presentations Prepared by Joan M. Zimmermann Zantech, Inc. 2 Opening, Announcements, Around the Table Identification Executive Secretary of the Planetary Science Advisory Committee (PAC), Dr. Stephen Rinehart, opened the meeting and made administrative announcements. PAC Chair, Dr. Anne Verbiscer, welcomed everyone to the virtual meeting. Announcements were made around the table and on Webex. PSD Status Report Dr. Lori Glaze, Director of the Planetary Science Division, gave a status report. First addressing the President’s Budget Request (PBR) for Fiscal Year 2021 (FY21) for the Science Mission Directorate (SMD), Dr. Glaze noted that it was one of the strongest science budgets in NASA history, representing a 12% increase over the enacted FY20 budget. The total PBR keeps NASA on track to land on the Moon by 2024; and to help prepare for human exploration at Mars. -
Big Data at the NASA/IPAC Infrared Science Archive (IRSA)
Big Data at the NASA/IPAC Infrared Science Archive (IRSA) Steve Groom IRSA: NASA/IPAC Infrared Science Archive Enabling research that has not yet been envisioned IRSA’s Charter ❋ IRSA is chartered to curate the science products of NASA’s infrared and submillimeter missions. IRSA’s Holdings ❋ All sky images and catalogs covering 20 wavelengths. ❋ Spitzer, NASA’s Infrared Great Observatory ❋ >1 PB since 2014 ❋ >100 billion table rows IRSA 2 09/29/16 IRSA: NASA/IPAC Infrared Science Archive Enabling research that has not yet been envisioned ❋ IRSA’s diverse holdings applicable across the range of NASA’s IRSA Holdings Growth Astrophysics themes 5000 4000 ❋ Richer content draws new, more 3000 complicated potential use cases 2000 Volume (TB) 1000 ❋ Holding the bits alone is not sufficient to enable new science 0 ➢ Archive provides support to 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 Year understand what the bits mean and which ones to use ➢ Archive assists users with logistics of access and analysis IRSA 3 09/29/16 100% IRSA’s Impact 90% 80% Spitzer Archival 70% 60% ❋ Archives can double the 50% 40% Both number of papers from a 30% mission. 20% Spitzer NonArchival 10% 0% 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 ❋ ~10% of refereed Year astrophysics journal articles 12 use data in IRSA’s holdings. 30 10 25 8 ❋ IRSA over 25 million queries 20 this year to date. 6 15 4 Papers that use NASA IR data 10 5 Queries (millions) Percent of Refereed Papers 2 0 0 2006 2007 2008 2009 2010 2011 2012 2013 -
Special Spitzer Telescope Edition No
INFRARED SCIENCE INTEREST GROUP Special Spitzer Telescope Edition No. 4 | August 2020 Contents From the IR SIG Leadership Council In the time since our last newsletter in January, the world has changed. 1 From the SIG Leadership Travel restrictions and quarantine have necessitated online-conferences, web-based meetings, and working from home. Upturned semesters, constantly shifting deadlines and schedules, and the evolving challenge of Science Highlights keeping our families and communities safe have all taken their toll. We hope this newsletter offers a moment of respite and a reminder that our community 2 Mysteries of Exoplanet continues its work even in the face of great uncertainty and upheaval. Atmospheres In January we said goodbye to the Spitzer Space Telescope, which 4 Relevance of Spitzer in the completed its mission after sixteen years in space. In celebration of Spitzer, Era of Roman, Euclid, and in recognition of the work of so many members of our community, this Rubin & SPHEREx newsletter edition specifically highlights cutting edge science based on and inspired by Spitzer. In the words of Dr. Paul Hertz, Director of Astrophysics 6 Spitzer: The Star-Formation at NASA: Legacy Lives On "Spitzer taught us how important infrared light is to our 8 AKARI Spitzer Survey understanding of our universe, both in our own cosmic 10 Science Impact of SOFIA- neighborhood and as far away as the most distant galaxies. HIRMES Termination The advances we make across many areas in astrophysics in the future will be because of Spitzer's extraordinary legacy." Technical Highlights Though Spitzer is gone, our community remains optimistic and looks forward to the advances that the next generation of IR telescopes will bring. -
1 How Will Astronomy Archives Survive the Data Tsunami?
DATABASES HOW WILL ASTRONOMY ARCHIVES SURVIVE THE DATA TSUNAMI? Astronomers are collecting more data than ever. What practices can keep them ahead of the flood? G. Bruce Berriman, NASA Exoplanet Science Institute, Infrared Processing and Analysis Center Steven L. Groom, Infrared Processing and Analysis Center, California Institute of Technology Astronomy is already awash with data: currently 1 PB (petabyte) of public data is electronically accessible, and this volume is growing at 0.5 PB per year. The availability of this data has already transformed research in astronomy, and the STScI (Space Telescope Science Institute) now reports that more papers are published with archived data sets than with newly acquired data.17 This growth in data size and anticipated usage will accelerate in the coming few years as new projects such as the LSST (Large Synoptic Survey Telescope), ALMA (Atacama Large Millimeter Array), and SKA (Square Kilometer Array) move into operation. These new projects will use much larger arrays of telescopes and detectors or much higher data acquisition rates than are now used. Projections indicate that by 2020, more than 60 PB of archived data will be accessible to astronomers.9 THE TSUNAMI HAS ALREADY MADE LANDFALL The data tsunami is already affecting the performance of astronomy archives and data centers. One example is the NASA/IPAC (Infrared Processing and Analysis Center) IRSA (Infrared Science Archive), which archives and serves data sets from NASA’s infrared missions. It is going through a period of Growth in the -
IMVI the Orbital Torus of Arrokoth -- a Sample Project
IMVI ISSN (p) 2303-4882, ISSN 1840-4383 Open Mathematical Education Notes Vol. 9(2019), 87-102 www.imvibl.org / JOURNALS / IMVI OMEN DOI: 10.7251/OMEN1901087M The Orbital Torus of Arrokoth -- A Sample Project David L. Milligan University of South Florida, Tampa, FL, USA. [email protected] Abstract. In mathematics education there has been voluminous consideration of "alternative" approaches to deliver content. At every stage of formal education, motivating students to learn mathematics is accomplished by making the material relevant to them. In the undergraduate calculus sequence, concepts of mensuration are made “real” when students actively use the relevant processes. While textbooks generally offer examples and exercises for students, these are more effective when students have personal motivation via Action Learning, or what are often called “Projects.” The article presented here is an example of what might be composed by the student as an application project. It demonstrates that, in addition to the mathematics, there is an abundance of relevant discussion connected to a topic to gain the writer’s (and hopefully the reader’s, as well) interest. Projects are reviewed by course instructors and subject area supervisors. The one student plus two professionals requirement has merit supported by this example. For starters, the instructor need not be (in this case) a professional astronomer and the astronomers (subject area advisors) need not know all the mathematical details behind each equation presented in a project write-up. The student can draw from these two real sources for motivation, and there’s “action” for all participants. It is not difficult to sense that a project student will likely retain the information learned for a longer period and be ready to synthesize the concepts with other real-world situations as they may arise. -
THE PLANETARY REPORT JUNE SOLSTICE 2019 VOLUME 39, NUMBER 2 Planetary.Org
THE PLANETARY REPORT JUNE SOLSTICE 2019 VOLUME 39, NUMBER 2 planetary.org SMALL-BODY RENDEZVOUS JAGGED LITTLE WORLDS HOLD CLUES TO EARTH’S ORIGINS BUT YIELD NEW PUZZLES DEFENDING EARTH C SAMPLING AN ASTEROID C ADVOCATING FOR SPACE SPACE ON EARTH Precise Movements Earth-Bound Tracking Devices Help Manage Spacecraft DEEP-SPACE EXPLORATION by robotic space- maintenance and installation on pump and craft requires the support of thousands of oil-flow fittings. The hydrostatic bearing liter- workers back on Earth in facilities around ally floats the moving structure of the antenna, the world. Canberra, Australia hosts one of which weighs about 4 million kilograms (8 NASA’s 3 Deep Space Network (DSN) stations, million pounds), on a film of oil only 0.1 mil- operated by the Commonwealth Scientific and limeter (4 thousandths of an inch) thick, per- Industrial Research Organisation (CSIRO). Each mitting the gigantic antenna to smoothly track Doran Eichstädt/Seán NASA/SwRI/MSSS/Gerald DSN station hosts one 70-meter and multiple spacecraft as Earth rotates. 34-meter dishes that receive data from space- craft across the solar system. Here, mechanical “Space on Earth” seeks to highlight all kinds engineer Rachel Twomey (apprentice), servo of ground-based facilities worldwide that systems engineer Paul Richter, and mechanical are involved in planetary exploration. If engineer Clayton Locke discuss maintenance you’d like to make a suggestion for a facility on the hydrostatic azimuth bearing on the to feature in “Space on Earth,” please CSIRO 70-meter antenna. The team is performing email [email protected]. 2 THE PLANETARY REPORT C JUNE SOLSTICE 2019 SNAPSHOTS FROM SPACE Contents JUNE SOLSTICE 2019 12 Apollo 11 Little West Crater Panorama Mike Constantine looks back at humans’ first landing on the Moon. -
Discover NASA
SPACE SCIENCE INSTITUTE NEWSLETTER WINTER 2016 W Space Science Institute Newsletter THE CARINA NEBULA IMAGE CREDIT: NASA, ESA/ STSCI IN THIS ISSUE NCIL News… Big News in Astronomy Conference Highlights: Clouds Over Martian DPS, AGU and AAS Low Latitudes! By Dr. Karly Pitman, Executive Director Submitted by Dr. Todd Clancy – SSI NC While the rest of the world is Over the past two slowing down around the holidays, decades, the our scientists kick into high gear in importance of the winter months submitting grant clouds in Mars’ proposals, judging others’ proposals atmosphere has at review panels, and traveling to been established present results at national and through new More on Page 6… international conferences. This year, observations and Cassini Completes Final Close conference season kicked off with the modeling. A Enceladus Flyby! American Astronomical Society’s variety of cloud Division for Planetary Sciences forms reflects the (DPS) held Nov. 8-13, 2015 at the variety in Gaylord National Resort and saturation Figure 1. CRISM color Convention Center in National conditions (e.g. limb image of CO2 Harbor, MD. More on Page 10 atmospheric clouds – credit page 3. temperatures) and dynamical forcing ranging from local to global conditions. This range of behaviors spans narrow vertical pipes of uplift that force high altitude More on Page 2… perihelion (nearest to the Sun) cloud trails in the warm orbital phase of the Covering science news around Mars atmosphere, to the global low Boulder! latitude gird of the aphelion (farthest More on Page 5… from the Sun) cloud belt in the cold orbital phase of the Mars atmosphere.