Spaceport Magazine, May 2018
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Will the Real Monster Black Hole Please Stand Up? 8 January 2015
Will the real monster black hole please stand up? 8 January 2015 how the merging of galaxies can trigger black holes to start feeding, an important step in the evolution of galaxies. "When galaxies collide, gas is sloshed around and driven into their respective nuclei, fueling the growth of black holes and the formation of stars," said Andrew Ptak of NASA's Goddard Space Flight Center in Greenbelt, Maryland, lead author of a The real monster black hole is revealed in this new new study accepted for publication in the image from NASA's Nuclear Spectroscopic Telescope Astrophysical Journal. "We want to understand the Array of colliding galaxies Arp 299. In the center panel, mechanisms that trigger the black holes to turn on the NuSTAR high-energy X-ray data appear in various and start consuming the gas." colors overlaid on a visible-light image from NASA's Hubble Space Telescope. The panel on the left shows NuSTAR is the first telescope capable of the NuSTAR data alone, while the visible-light image is pinpointing where high-energy X-rays are coming on the far right. Before NuSTAR, astronomers knew that the each of the two galaxies in Arp 299 held a from in the tangled galaxies of Arp 299. Previous supermassive black hole at its heart, but they weren't observations from other telescopes, including sure if one or both were actively chomping on gas in a NASA's Chandra X-ray Observatory and the process called accretion. The new high-energy X-ray European Space Agency's XMM-Newton, which data reveal that the supermassive black hole in the detect lower-energy X-rays, had indicated the galaxy on the right is indeed the hungry one, releasing presence of active supermassive black holes in Arp energetic X-rays as it consumes gas. -
The Most Dangerous Ieos in STEREO
EPSC Abstracts Vol. 6, EPSC-DPS2011-682, 2011 EPSC-DPS Joint Meeting 2011 c Author(s) 2011 The most dangerous IEOs in STEREO C. Fuentes (1), D. Trilling (1) and M. Knight (2) (1) Northern Arizona University, Arizona, USA, (2) Lowell Observatory, Arizona, USA ([email protected]) Abstract (STEREO-B) which view the Sun-Earth line using a suite of telescopes. Each spacecraft moves away 1 from the Earth at a rate of 22.5◦ year− (Figure 1). IEOs (inner Earth objects or interior Earth objects) are ∼ potentially the most dangerous near Earth small body Our search for IEOs utilizes the Heliospheric Imager population. Their study is complicated by the fact the 1 instruments on each spacecraft (HI1A and HI1B). population spends all of its time inside the orbit of The HI1s are centered 13.98◦ from the Sun along the the Earth, giving ground-based telescopes a small win- Earth-Sun line with a square field of view 20 ◦ wide, 1 dow to observe them. We introduce STEREO (Solar a resolution of 70 arcsec pixel− , and a bandpass of TErrestrial RElations Observatory) and its 5 years of 630—730 nm [3]. Images are taken every 40 minutes, archival data as our best chance of studying the IEO providing a nearly continuous view of the inner solar population and discovering possible impactor threats system since early 2007. The nominal visual limit- ing magnitude of HI1 is 13, although the sensitivity to Earth. ∼ We show that in our current search for IEOs in varies somewhat with solar elongation, and asteroids STEREO data we are capable of detecting and char- fainter than 13 can be seen near the outer edges. -
ARIEL – 13Th Appleton Space Conference PLANETS ARE UBIQUITOUS
Background image credit NASA ARIEL – 13th Appleton Space Conference PLANETS ARE UBIQUITOUS OUR GALAXY IS MADE OF GAS, STARS & PLANETS There are at least as many planets as stars Cassan et al, 2012; Batalha et al., 2015; ARIEL – 13th Appleton Space Conference 2 EXOPLANETS TODAY: HUGE DIVERSITY 3700+ PLANETS, 2700 PLANETARY SYSTEMS KNOWN IN OUR GALAXY ARIEL – 13th Appleton Space Conference 3 HUGE DIVERSITY: WHY? FORMATION & EVOLUTION PROCESSES? MIGRATION? INTERACTION WITH STAR? Accretion Gaseous planets form here Interaction with star Planet migration Ices, dust, gas ARIEL – 13th Appleton Space Conference 4 STAR & PLANET FORMATION/EVOLUTION WHAT WE KNOW: CONSTRAINTS FROM OBSERVATIONS – HERSCHEL, ALMA, SOLAR SYSTEM Measured elements in Solar system ? Image credit ESA-Herschel, ALMA (ESO/NAOJ/NRAO), Marty et al, 2016; André, 2012; ARIEL – 13th Appleton Space Conference 5 THE SUN’S PLANETS ARE COLD SOME KEY O, C, N, S MOLECULES ARE NOT IN GAS FORM T ~ 150 K Image credit NASA Juno mission, NASA Galileo ARIEL – 13th Appleton Space Conference 6 WARM/HOT EXOPLANETS O, C, N, S (TI, VO, SI) MOLECULES ARE IN GAS FORM Atmospheric pressure 0.01Bar H2O gas CO2 gas CO gas CH4 gas HCN gas TiO gas T ~ 500-2500 K Condensates VO gas H2S gas 1 Bar Gases from interior ARIEL – 13th Appleton Space Conference 7 CHEMICAL MEASUREMENTS TODAY SPECTROSCOPIC OBSERVATIONS WITH CURRENT INSTRUMENTS (HUBBLE, SPITZER,SPHERE,GPI) • Precision of 20 ppm can be reached today by Hubble-WFC3 • Current data are sparse, instruments not absolutely calibrated • ~ 40 planets analysed -
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars Origins | Climate | Discovery Jacob Bean (University of Chicago) Presented on behalf of the FINESSE/CASE science team: Mark Swain (PI), Nicholas Cowan, Jonathan Fortney, Caitlin Griffith, Tiffany Kataria, Eliza Kempton, Laura Kreidberg, David Latham, Michael Line, Suvrath Mahadevan, Jorge Melendez, Julianne Moses, Vivien Parmentier, Gael Roudier, Evgenya Shkolnik, Adam Showman, Kevin Stevenson, Yuk Yung, & Robert Zellem Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars **Candidate NASA MIDEX mission for launch in 2023** Objectives FINESSE will test theories of planetary origins and climate, transform comparative planetology, and open up exoplanet discovery space by performing a comprehensive, statistical, and uniform survey of transiting exoplanet atmospheres. Strategy • Transmission spectroscopy of 500 planets: Mp = few – 1,000 MEarth • Phase-resolved emission spectroscopy of a subset of 100 planets: Teq > 700 K • Focus on synergistic science with JWST: homogeneous survey, broader context, population properties, and bright stars Hardware • 75 cm aluminum Cassegrain telescope at L2 • 0.5 – 5.0 μm high-throughput prism spectrometer with R > 80 • Single HgCdTe detector with JWST heritage for science and guiding Origins | Climate | Discovery Advantages of Fast Infrared -
NASA Program & Budget Update
NASA Update AAAC Meeting | June 15, 2020 Paul Hertz Director, Astrophysics Division Science Mission Directorate @PHertzNASA Outline • Celebrate Accomplishments § Science Highlights § Mission Milestones • Committed to Improving § Inspiring Future Leaders, Fellowships § R&A Initiative: Dual Anonymous Peer Review • Research Program Update § Research & Analysis § ROSES-2020 Updates, including COVID-19 impacts • Missions Program Update § COVID-19 impact § Operating Missions § Webb, Roman, Explorers • Planning for the Future § FY21 Budget Request § Project Artemis § Creating the Future 2 NASA Astrophysics Celebrate Accomplishments 3 SCIENCE Exoplanet Apparently Disappears HIGHLIGHT in the Latest Hubble Observations Released: April 20, 2020 • What do astronomers do when a planet they are studying suddenly seems to disappear from sight? o A team of researchers believe a full-grown planet never existed in the first place. o The missing-in-action planet was last seen orbiting the star Fomalhaut, just 25 light-years away. • Instead, researchers concluded that the Hubble Space Telescope was looking at an expanding cloud of very fine dust particles from two icy bodies that smashed into each other. • Hubble came along too late to witness the suspected collision, but may have captured its aftermath. o This happened in 2008, when astronomers announced that Hubble took its first image of a planet orbiting another star. Caption o The diminutive-looking object appeared as a dot next to a vast ring of icy debris encircling Fomalhaut. • Unlike other directly imaged exoplanets, however, nagging Credit: NASA, ESA, and A. Gáspár and G. Rieke (University of Arizona) puzzles arose with Fomalhaut b early on. Caption: This diagram simulates what astronomers, studying Hubble Space o The object was unusually bright in visible light, but did not Telescope observations, taken over several years, consider evidence for the have any detectable infrared heat signature. -
Cosmic Evolution Through Uv Surveys (Cetus) Final Report
COSMIC EVOLUTION THROUGH UV SURVEYS (CETUS) FINAL REPORT Thematic Activity: Project (probe mission concept) Program: Electromagnetic observations from space Authors of Final Report: Jonathan Arenberg, Northrop Grumman Corporation Sally Heap, Univ. of Maryland, [email protected] Tony Hull, Univ. of New Mexico Steve Kendrick, Kendrick Aerospace Consulting LLC Bob Woodruff, Woodruff Consulting Scientific Contributors: Maarten Baes, Rachel Bezanson, Luciana Bianchi, David Bowen, Brad Cenko, Yi-Kuan Chiang, Rachel Cochrane, Mike Corcoran, Paul Crowther, Simon Driver, Bill Danchi, Eli Dwek, Brian Fleming, Kevin France, Pradip Gatkine, Suvi Gezari, Lea Hagen, Chris Hayward, Matthew Hayes, Tim Heckman, Edmund Hodges-Kluck, Alexander Kutyrev, Thierry Lanz, John MacKenty, Steve McCandliss, Harvey Moseley, Coralie Neiner, Goren Östlin, Camilla Pacifici, Marc Rafelski, Bernie Rauscher, Jane Rigby, Ian Roederer, David Spergel, Dan Stark, Alexander Szalay, Bryan Terrazas, Jonathan Trump, Arjun van der Wel, Sylvain Veilleux, Kate Whitaker, Isak Wold, Rosemary Wyse Technical Contributors: Jim Burge, Kelly Dodson, Chip Eckles, Brian Fleming, Jamie Kennea, Gerry Lemson, John MacKenty, Steve McCandliss, Greg Mehle, Shouleh Nikzad, Trent Newswander, Lloyd Purves, Manuel Quijada, Ossy Siegmund, Dave Sheikh, Phil Stahl, Ani Thakar, John Vallerga, Marty Valente, the Goddard IDC/MDL. September 2019 Cosmic Evolution Through UV Surveys (CETUS) TABLE OF CONTENTS INTRODUCTION TO CETUS ................................................................................................................ -
The Critical Path? Knowledge Management Insights
National Aeronautics and Space Administration GSFC SUPPORTS COMMERCIAL CREW AND #LAUNCHAMERICA Page 8 How to intern JWST media while working team wins remotely top honors Page 36 Page 24 FLIGHT PROJECTS DIRECTORATE | Volume 28 • Number 2 Enabling exploration and earth + space science by transforming concepts and questions into reality www.nasa.gov CONTENTS PUBLISHED BY THE FLIGHT PROJECTS DIRECTORATE TCP TEAM Michelle Belleville Maureen Disharoon Page 8 Sarah Harnish Laura Paschal Code 400 Message from the Director . 4 Page: 36 SCaN Internship Project Behind the Badge . 70 Provides Unique Opportunities Reese Patillo An update from David F. Mitchell Getting to know the faces of 400 Jennifer Poston Page: 39 That was Then … This is Now WE’RE ON David Ryan THE WEB! Page: 42 Building the Workforce of the A Word from the Deputy . 6 SAR Saves Statistics . 74 Shannon Smith Future Messages from the FPD deputies The latest Search and Rescue beacon saves Paula Wood Page: 43 Flight Projects Virtual Showcase http://fpd.gsfc.nasa.gov COVID 19 Resources . 7 and Scavenger Hunt for Interns Did you Know? . 74 SUPERVISING We are in this together Page: 45 Let’s CONNECT Building diversity and inclusion awareness EDITOR Page: 46 What’s up with our FPDP? Donna Swann Articles Out and About . 75 Page: 48 JPSS in Your Community: Life’s highlights off campus Page: 8 Goddard and the Flight Projects Benefits beyond the Data Directorate Empower Crewed Have a story idea, news item or letter SpaceX Launch FPD Launch Schedule . 76 for The Critical Path? Knowledge Management Insights . 50 Where are we now? Let us know about it. -
2008 Spaceport News Summary
2008 Spaceport News Summary The 2008 Spaceport News used the above banner for the year. Introduction The first issue of the Spaceport News was December 13, 1962. The 1963, 1964 and 1965 Spaceport News were issued weekly. The Spaceport News was issued every two weeks, starting July 7, 1966, until the last issue on February 24, 2014. Spaceport Magazine, a monthly issue, superseded the Spaceport News in April 2014, until the final issue, Jan./Feb. 2020. The two 1962 Spaceport News issues and the issues from 1996 until the final Spaceport Magazine issue, are available for viewing at this website. The Spaceport News issues from 1963 through 1995 are currently not available online. In this Summary, black font is original Spaceport News text, blue font is something I added or someone else/some other source provided, and purple font is a hot link. All links were working at the time I completed this Spaceport News Summary. The Spaceport News writer is acknowledged, if noted in the Spaceport News article. Followup From the 2007 Spaceport News Summary The followng is in the December 14, 2007, issue of the Spaceport News. Page 1 There is an article in the 2007 Spaceport News Summary about External Tank repairs to ET-124, flown on STS-117, after it was damaged by hail. Below is a photo in the VAB, showing the extent of some of the damage. A lot of scaffolding had to be installed, some of which is in visible in the photo. From The January 11, 2008, Spaceport News On page 1, “Apollo Tribute Bike roars through KSC”, by Linda Herridge, Staff Writer. -
Prelude To, and Nature of the Space Photometry Revolution
EPJ Web of Conferences 101, 0001(0 2015) DOI: 10.1051/epjconf/20151010000 1 C Owned by the authors, published by EDP Sciences, 2015 Prelude to, and Nature of the Space Photometry Revolution Ronald L. Gilliland1,a Space Telescope Science Institute and Department of Astronomy and Astrophysics, and Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA Abstract. It is now less than a decade since CoRoT initiated the space photometry revo- lution with breakthrough discoveries, and five years since Kepler started a series of similar advances. I’ll set the context for this revolution noting the status of asteroseismology and exoplanet discovery as it was 15-25 years ago in order to give perspective on why it is not mere hyperbole to claim CoRoT and Kepler fostered a revolution in our sciences. Primary events setting up the revolution will be recounted. I’ll continue with noting the major discoveries in hand, and how asteroseismology and exoplanet studies, and indeed our approach to doing science, have been forever changed thanks to these spectacular missions. 1 Introduction I would like to start by thanking Rafa Garcia, Jer´ omeˆ Ballot and the Science Organizing Committee for inviting me to give the introductory talk at this conference. It is a great honor for me to do so. Of course we’re here to discuss the results that come from CoRoT and Kepler; these were French and American missions respectively with Annie Baglin as the PI for CoRoT and Bill Borucki as the PI for Kepler. -
Appendix Program Managers/Acknowledgments
Flight Information Appendix Program Managers/Acknowledgments Selected Readings Acronyms Contributors’ Biographies Index Image of a Legac y—The Final Re-entry Appendix 517 Flight Information Approx. Orbiter Enterprise STS Flight No. Orbiter Crew Launch Mission Approach and Landing Test Flights and Crew Patch Name Members Date Days 1 Columbia John Young (Cdr) 4/12/1981 2 Robert Crippen (Plt) Captive-Active Flights— High-speed taxi tests that proved the Shuttle Carrier Aircraft, mated to Enterprise, could steer and brake with the Orbiter perched 2 Columbia Joe Engle (Cdr) 11/12/1981 2 on top of the airframe. These fights featured two-man crews. Richard Truly (Plt) Captive-Active Crew Test Mission Flight No. Members Date Length 1 Fred Haise (Cdr) 6/18/1977 55 min 46 s Gordon Fullerton (Plt) 2 Joseph Engle (Cdr) 6/28/1977 62 min 0 s 3 Columbia Jack Lousma (Cdr) 3/22/1982 8 Richard Truly (Plt) Gordon Fullerton (Plt) 3 Fred Haise (Cdr) 7/26/1977 59 min 53 s Gordon Fullerton (Plt) Free Flights— Flights during which Enterprise separated from the Shuttle Carrier Aircraft and landed at the hands of a two-man crew. 4 Columbia Thomas Mattingly (Cdr) 6/27/1982 7 Free Flight No. Crew Test Mission Henry Hartsfield (Plt) Members Date Length 1 Fred Haise (Cdr) 8/12/1977 5 min 21 s Gordon Fullerton (Plt) 5 Columbia Vance Brand (Cdr) 11/11/1982 5 2 Joseph Engle (Cdr) 9/13/1977 5 min 28 s Robert Overmyer (Plt) Richard Truly (Plt) William Lenoir (MS) 3 Fred Haise (Cdr) 9/23/1977 5 min 34 s Joseph Allen (MS) Gordon Fullerton (Plt) 4 Joseph Engle (Cdr) 10/12/1977 2 min 34 s Richard Truly (Plt) 5 Fred Haise (Cdr) 10/26/1977 2 min 1 s 6 Challenger Paul Weitz (Cdr) 4/4/1983 5 Gordon Fullerton (Plt) Karol Bobko (Plt) Story Musgrave (MS) Donald Peterson (MS) The Space Shuttle Numbering System The first nine Space Shuttle flights were numbered in sequence from STS -1 to STS-9. -
Micrometeoroid Impacts on the Hubble Space Telescope Wide Field and Planetary Camera 2: Larger Particles
45th Lunar and Planetary Science Conference (2014) 1722.pdf MICROMETEOROID IMPACTS ON THE HUBBLE SPACE TELESCOPE WIDE FIELD AND PLANETARY CAMERA 2: LARGER PARTICLES. A. T. Kearsley 1, G. W. Grime 2, J. L. Colaux 2, V. V. Palit- sin 2, C. Jeynes 2, R. P. Webb 2, D. K. Ross 3,4 , P. Anz-Meador 3,4 , J.C. Liou 4, J. Opiela 3,4 , T. Griffin 5, L. Gerlach 6, P. J. Wozniakiewicz 1,7, M. C. Price 7, M. J. Burchell 7 and M. J. Cole 7 1Natural History Museum (NHM), London, SW7 5BD, UK ( [email protected] ) 2Ion Beam Centre, University of Surrey, Guildford, 3Jacobs Technology, Houston, TX, USA 4NASA-JSC, Houston, TX, USA, 5NASA-GSFC, USA, 5consultant to European Space Agency, ESA-ESTEC, Noordwijk, The Netherlands 6School of Physical Science, University of Kent, Canterbury, CT2 7NH, UK. Introduction: The Wide Field and Planetary Cam- Results: 63 impact features > 700µm across, each with era 2 (WFPC2) was returned from the Hubble Space paint spallation > 300 µm, showed combinations of Telescope (HST) by shuttle mission STS-125 in 2009. five main components (e.g. Fig. 3): a) an exposed sur- In space for 16 years, the surface accumulated hun- face of Al alloy, often with adhering fragments of dreds of impact features [1] on zinc orthotitanate paint, paint; b) a bowl-shaped pit or field of compound pits, some penetrating through into underlying metal. Larger penetrating into the alloy; c) frothy impact melt, de- impacts were seen in photographs taken from within rived mainly from paint (Fig. -
What Is CHEOPS?
Swiss and ESA satellite CHEOPS launching soon! CHEOPS will be launching into space on the 17th of December! You may be wondering: what is CHEOPS? CHEOPS stands for CHaracterising ExOPlanet Satellite. Its goal is to study transits of already-known exoplanets to gain more knowledge about them. What type of information are we looking for? Scientists want to know detailed information about planets outside our Solar System, such as the mass, planet size, and density, which will in turn help to figure out the composition of these exoplanets. Studying exoplanet composition and their atmospheres is important especially for astrobiology. A planet’s chemical composition can affect its habitability for life as we know it. Scientists usually look for biosignatures such as the presence of methane or oxygen in the planet’s atmosphere, which could indicate presence of past or present life. Artist’s impression of CHEOPS. Credits: ESA / ATG medialab. The major contributors CHEOPS is a collaboration between ESA and the Swiss Space Office. The mission was proposed and is now headed by Prof. Willy Benz, from the University of Bern, which houses the mission’s consortium. The science operations consortium is at the University of Geneva, where they have many collaborators, such as the Swiss Space Center at EPFL. As it is an ESA endeavour, many other European institutions are also contributing to the mission. For example, the mission operations consortium is located in Torrejón de Ardoz, Spain. The launch The satellite has already been shipped to Kourou, French Guiana, where it will be launched by the ESA spaceport.