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Gravimetric Missions in Japanese Lunar Explorer, SELENE
Gravimetric Missions in Japanese Lunar Explorer, SELENE H. Hanada1), T. Iwata2), N. Namiki3), N. Kawano1), K. Asari1), T. Ishikawa1), F. Kikuchi1), Q. Liu1), K. Matsumoto1), H. Noda1), J. Ping4), S. Tsuruta1), K. Iwadate1), O. Kameya1), S. Kuji1), Y. Tamura1), X. Hong4), Y. Aili5), S. Ellingsen6) 1) National Astronomical Observatory of Japan 2) Japan Aerospace Exploration Agency 3) Kyushu University 4) Shanghai Astronomical Observatory, Chinese Academy of Sciences 5)Urumqi Astronomical Observatory,Chinese Academy of Sciences 6) University of Tasmania ABSTRACT SELENE (SElenological and Engineering Explorer), is a mission in preparation for launch in 2007 by JAXA (Japan Aerospace Exploration Agency), it carries 15 missions, two of which (RSAT and VRAD) are gravimetric experiments using radio waves. The RSAT (Relay Satellite Transponder) mission will undertake 4-way Doppler measurements of the main orbiter through the Rstar sub-satellite. This is in addition to 2-way Doppler and ranging measurements of the satellites and will realize the first direct observation of the gravity fields on the far side of the Moon. The VRAD (Differential VLBI Radio Source) mission involves observing the trajectories of Rstar and Vstar using differential VLBI with both a Japanese network (VERA), and an international network. We have already finished development of the onboard instruments and are carrying out proto-flight tests under various conditions. We have also performed test VLBI observations of orbiters with the international network. 1. INTRODUCTION Although it is the nearest astronomical body to the Earth, there are many unsolved problems relating to the origin and the evolution of the Moon. Numerous lunar explorations have been made with the aim of elucidating these problems, however, we still know little of the deep interior of the Moon. -
Planetary Report Report
The PLANETARYPLANETARY REPORT REPORT Volume XXIX Number 1 January/February 2009 Beyond The Moon From The Editor he Internet has transformed the way science is On the Cover: Tdone—even in the realm of “rocket science”— The United States has the opportunity to unify and inspire the and now anyone can make a real contribution, as world’s spacefaring nations to create a future brightened by long as you have the will to give your best. new goals, such as the human exploration of Mars and near- In this issue, you’ll read about a group of amateurs Earth asteroids. Inset: American astronaut Peggy A. Whitson who are helping professional researchers explore and Russian cosmonaut Yuri I. Malenchenko try out training Mars online, encouraged by Mars Exploration versions of Russian Orlan spacesuits. Background: The High Rovers Project Scientist Steve Squyres and Plane- Resolution Camera on Mars Express took this snapshot of tary Society President Jim Bell (who is also head Candor Chasma, a valley in the northern part of Valles of the rovers’ Pancam team.) Marineris, on July 6, 2006. Images: Gagarin Cosmonaut Training This new Internet-enabled fun is not the first, Center. Background: ESA nor will it be the only, way people can participate in planetary exploration. The Planetary Society has been encouraging our members to contribute Background: their minds and energy to science since 1984, A dust storm blurs the sky above a volcanic caldera in this image when the Pallas Project helped to determine the taken by the Mars Color Imager on Mars Reconnaissance Orbiter shape of a main-belt asteroid. -
The Planetary Report
On the Cover: Volume XV Seen thro ugh eyes other than our own, the planet Earth Table of Number 3 appears as a stran ge but beautiful place. The Galilea spacecraft on its way to Jupiter took thi s image of West ' Contents 'May/June 1995 Africa and the Mediterranean Sea from about 600 ,000 kilometers (400,000 miles) away. The spacecraft's camera was looking through infrared filters sensitive to light wave lengths unfamiliar to the human eye. Images ta ken th is way provide information about things such as the location an d health of vegetati on an d the water conte nt of clouds. Features Basics of Galilea's portrai ts of the planet cou ld be valuabl e referen ce 14 Spaceflight: poi nts for future Earth-monitoring spacecraft. Phoenix Rises: (See page 10 for a complete caption.) Gravity Assist 4 NASA SETI Project Image: Pau l Geissler, Lunar and Planetary Laboratory, Over the years the term "gravity assist" Un ivers ity of Arizona Is Reborn has appeared time and again in our pages. Two years ago the congressional budget This ingenious technique has made many cutters took an ax to NASA's ambitious of our pioneering spacecraft missions pos program in the Search for Extraterrestrial sible. For example, the Galileo encounter Froln Intelligence. But dedicated researchers with Earth was part of a gravity-assist refused to give up, and they found a way to maneuver. It's a hard technique to explain, The save part of the program. Project Phoenix but here we lay it out for our readers. -
Asteroid Retrieval Feasibility Study
Publications 4-2-2012 Asteroid Retrieval Feasibility Study John Brophy California Institute of Technology Fred Culick California Institute of Technology Louis Friedman The Planetary Society Pedro Llanos Embry-Riddle Aeronautical University - Daytona Beach, [email protected] et al. Follow this and additional works at: https://commons.erau.edu/publication Part of the Astrodynamics Commons, Space Vehicles Commons, and the The Sun and the Solar System Commons Scholarly Commons Citation Brophy, J., Culick, F., Friedman, L., Llanos, P., & al., e. (2012). Asteroid Retrieval Feasibility Study. , (). Retrieved from https://commons.erau.edu/publication/893 This Report is brought to you for free and open access by Scholarly Commons. It has been accepted for inclusion in Publications by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. Asteroid Retrieval Feasibility Study 2 April 2012 Prepared for the: Keck Institute for Space Studies California Institute of Technology Jet Propulsion Laboratory Pasadena, California 1 2 Authors and Study Participants NAME Organization E-Mail Signature John Brophy Co-Leader / NASA JPL / Caltech [email protected] Fred Culick Co-Leader / Caltech [email protected] Co -Leader / The Planetary Louis Friedman [email protected] Society Carlton Allen NASA JSC [email protected] David Baughman Naval Postgraduate School [email protected] NASA ARC/Carnegie Mellon Julie Bellerose [email protected] University Bruce Betts The Planetary Society -
Can't Go Home by Noelle Adams / Pfangirl PART 1
Can't go home By Noelle Adams / pfangirl PART 1 - SUFFOCATED A caged lioness. That's what Lara reminded Sam of now. Every time she looked at her best friend, the American thought of the big cat she'd seen in a German zoo during her globe- trotting childhood. It wouldn't lie still. It was pure feral energy, striding back and forth in its enclosure, muscles rippling beneath its pelt. Lara was the same. Lithe grace and power in human form, always moving, always intensely focused on some task or thing. Almost permanently scowling. Sam had always wondered which of her parents Lara inherited her effortless physicality from. Four years of knowing Lara, and Sam still wasn't sure. There were no photos for her to consult. The young archaeologist hardly spoke about her vanished mother and father. She avoided talking about them; evidently running from their memory like she ran from what had happened on Yamatai. In the one and a half months since the shipwreck – well, at least since she was released from hospital – Lara had been seized by a frantic, feverish vigour. They had travelled from Osaka to the UK, where Lara had spent a single day at her family's estate, ransacking her father's study. From there they headed to New York. This put Lara closer to her next intended stop – Roanoke Island. Although the city was a good base for Lara to work from while she planned her next expedition, there was a second, more distasteful reason for the archaeologist to be there: an exclusive television interview. -
THE MARS 2020 ROVER ENGINEERING CAMERAS. J. N. Maki1, C
51st Lunar and Planetary Science Conference (2020) 2663.pdf THE MARS 2020 ROVER ENGINEERING CAMERAS. J. N. Maki1, C. M. McKinney1, R. G. Willson1, R. G. Sellar1, D. S. Copley-Woods1, M. Valvo1, T. Goodsall1, J. McGuire1, K. Singh1, T. E. Litwin1, R. G. Deen1, A. Cul- ver1, N. Ruoff1, D. Petrizzo1, 1Jet Propulsion Laboratory, California Institute of Technology (4800 Oak Grove Drive, Pasadena, CA 91109, [email protected]). Introduction: The Mars 2020 Rover is equipped pairs (the Cachecam, a monoscopic camera, is an ex- with a neXt-generation engineering camera imaging ception). The Mars 2020 engineering cameras are system that represents a significant upgrade over the packaged into a single, compact camera head (see fig- previous Navcam/Hazcam cameras flown on MER and ure 1). MSL [1,2]. The Mars 2020 engineering cameras ac- quire color images with wider fields of view and high- er angular/spatial resolution than previous rover engi- neering cameras. Additionally, the Mars 2020 rover will carry a new camera type dedicated to sample op- erations: the Cachecam. History: The previous generation of Navcams and Hazcams, known collectively as the engineering cam- eras, were designed in the early 2000s as part of the Mars Exploration Rover (MER) program. A total of Figure 1. Flight Navcam (left), Flight Hazcam (middle), 36 individual MER-style cameras have flown to Mars and flight Cachecam (right). The Cachecam optical assem- on five separate NASA spacecraft (3 rovers and 2 bly includes an illuminator and fold mirror. landers) [1-6]. The MER/MSL cameras were built in two separate production runs: the original MER run Each of the Mars 2020 engineering cameras utilize a (2003) and a second, build-to-print run for the Mars 20 megapixel OnSemi (CMOSIS) CMOS sensor Science Laboratory (MSL) mission in 2008. -
Protons in the Near Lunar Wake Observed by the SARA Instrument on Board Chandrayaan-1
FUTAANA ET AL. PROTONS IN DEEP WAKE NEAR MOON 1 Protons in the Near Lunar Wake Observed by the SARA 2 Instrument on Board Chandrayaan-1 3 Y. Futaana, 1 S. Barabash, 1 M. Wieser, 1 M. Holmström, 1 A. Bhardwaj, 2 M. B. Dhanya, 2 R. 4 Sridharan, 2 P. Wurz, 3 A. Schaufelberger, 3 K. Asamura 4 5 --- 6 Y. Futaana, Swedish Institute of Space Physics, Box 812, Kiruna, SE-98128, Sweden. 7 ([email protected]) 8 9 10 1 Swedish Institute of Space Physics, Box 812, Kiruna, SE-98128, Sweden 11 2 Space Physics Laboratory, Vikram Sarabhai Space Center, Trivandrum 695 022, India 12 3 Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland 13 4 Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Japan 14 Index Terms 15 6250 Moon 16 5421 Interactions with particles and fields 17 2780 Magnetospheric Physics: Solar wind interactions with unmagnetized bodies 18 7807 Space Plasma Physics: Charged particle motion and acceleration 19 Abstract 20 Significant proton fluxes were detected in the near wake region of the Moon by an ion mass 21 spectrometer on board Chandrayaan-1. The energy of these nightside protons is slightly higher than 22 the energy of the solar wind protons. The protons are detected close to the lunar equatorial plane at 23 a 140˚ solar zenith angle, i.e., ~50˚ behind the terminator at a height of 100 km. The protons come 24 from just above the local horizon, and move along the magnetic field in the solar wind reference 25 frame. -
Solar System Solar System
Delta Science Reader SolarSolar SystemSystem Delta Science Readers are nonfiction student books that provide science background and support the experiences of hands-on activities. Every Delta Science Reader has three main sections: Think About . , People in Science, and Did You Know? Be sure to preview the reader Overview Chart on page 4, the reader itself, and the teaching suggestions on the following pages. This information will help you determine how to plan your schedule for reader selections and activity sessions. Reading for information is a key literacy skill. Use the following ideas as appropriate for your teaching style and the needs of your students. The After Reading section includes an assessment and writing links. OVERVIEW Students will: discover facts about the Solar System In the Delta Science Reader Solar System, students take a tour of the Sun and the explore the planets and other objects in the planets. Other space objects such as dwarf Solar System planets, comets, asteroids, and meteoroids discuss the function of a table of contents, are explored. Students read about the headings, and a glossary rotation and revolution of the planets and interpret photographs and graphics to the causes of night and day, seasonal answer questions changes, and the phases of the Moon. The book describes the work of a planetary complete a KWL chart geologist. In addition, students discover organize information in a variety of ways how telescopes work. delta science modules Solar System 119 © Delta Education LLC. All rights reserved. -
Lightsail 2 Set to Launch in June “We Are Go for Launch!” Said Planetary Society CEO Bill Nye
Lightsail 2 set to launch in June “We are go for launch!” said Planetary Society CEO Bill Nye. Funded by space enthusiasts, LightSail 2 aims to accomplish the 1st-ever, controlled solar sail flight in Earth orbit next month. Writing at the Planetary Society’s blog, Jason Davis this week (May 13, 2019) described the upcoming challenge of the launch of LightSail 2, a little spacecraft literally powered by sunbeams and dear to the hearts of many. He wrote: Weighing just 5 kilograms, the loaf-of-bread-sized spacecraft, known as a CubeSat, is scheduled to lift A one-unit CubeSat measures 10 centimeters per side. off on June 22, 2019, aboard a SpaceX Falcon Heavy LightSail is a three-unit CubeSat measuring 10 by 10 by 30 rocket from Kennedy Space Center, Florida. Once in centimetres. Here, an early LightSail model sits next to a space, LightSail 2 will deploy a boxing ring-sized solar loaf of bread for size comparison. sail and attempt to raise its orbit using the gentle push from solar photons. It’s the culmination of a 10-year project with an origin story linked to the three scientist-engineers who founded The Planetary Society in 1980. Indeed, although the Lightsail 2 project itself is 10 years old, the idea for lightsail or solar sail spacecraft goes back decades, at least. Carl Sagan – who was one of those Planetary Society founders -- popularized the idea for our time. Now the mantle for popularizing lightsails, and helping to bring the dream many steps closer to reality, has been passed to Bill Nye, the current CEO of the Planetary Society. -
Operation and Performance of the Mars Exploration Rover Imaging System on the Martian Surface
Operation and Performance of the Mars Exploration Rover Imaging System on the Martian Surface Justin N. Maki Jet Propulsion Laboratory California Institute of Technology Pasadena, CA USA [email protected] Todd Litwin, Mark Schwochert Jet Propulsion Laboratory California Institute of Technology Pasadena, CA USA Ken Herkenhoff United States Geological Survey Flagstaff, AZ USA Abstract - The Imaging System on the Mars Exploration Rovers has successfully operated on the surface of Mars for over one Earth year. The acquisition of hundreds of panoramas and tens of thousands of stereo pairs has enabled the rovers to explore Mars at a level of detail unprecedented in the history of space exploration. In addition to providing scientific value, the images also play a key role in the daily tactical operation of the rovers. The mobile nature of the MER surface mission requires extensive use of the imaging system for traverse planning, rover localization, remote sensing instrument targeting, and robotic arm placement. Each of these activity types requires a different set of data compression rates, surface Figure 1. The Mars Exploration Spirit Rover, as viewed by coverage, and image acquisition strategies. An overview the Navcam shortly after lander egress early in the mission. of the surface imaging activities is provided, along with a presents an overview of the operation and performance of summary of the image data acquired to date. the MER Imaging System. Keywords: Imaging system, cameras, rovers, Mars, 1.2 Imaging System Design operations. The MER cameras are classified into five types: Descent cameras, Navigation cameras (Navcam), Hazard Avoidance 1 Introduction cameras (Hazcam), Panoramic cameras (Pancam), and Microscopic Imager (MI) cameras. -
Evidence from Opportunity's Microscopic Imager for Water on Meridiani Planum K
Evidence from Opportunity's Microscopic Imager for Water on Meridiani Planum K. E. Herkenhoff, et al. Science 306, 1727 (2004); DOI: 10.1126/science.1105286 This copy is for your personal, non-commercial use only. If you wish to distribute this article to others, you can order high-quality copies for your colleagues, clients, or customers by clicking here. Permission to republish or repurpose articles or portions of articles can be obtained by following the guidelines here. The following resources related to this article are available online at www.sciencemag.org (this infomation is current as of October 27, 2011 ): Updated information and services, including high-resolution figures, can be found in the online version of this article at: http://www.sciencemag.org/content/306/5702/1727.full.html Supporting Online Material can be found at: http://www.sciencemag.org/content/suppl/2004/11/30/306.5702.1727.DC1.html A list of selected additional articles on the Science Web sites related to this article can be on October 27, 2011 found at: http://www.sciencemag.org/content/306/5702/1727.full.html#related This article has been cited by 70 article(s) on the ISI Web of Science This article has been cited by 10 articles hosted by HighWire Press; see: http://www.sciencemag.org/content/306/5702/1727.full.html#related-urls This article appears in the following subject collections: Planetary Science www.sciencemag.org http://www.sciencemag.org/cgi/collection/planet_sci Downloaded from Science (print ISSN 0036-8075; online ISSN 1095-9203) is published weekly, except the last week in December, by the American Association for the Advancement of Science, 1200 New York Avenue NW, Washington, DC 20005. -
Mars Exploration Rovers: 4 Years on Mars
https://ntrs.nasa.gov/search.jsp?R=20080047431 2019-10-28T16:17:34+00:00Z Mars Exploration Rovers: 4 Years on Mars Geoffrey A. Landis This January, the Mars Exploration Rovers "Spirit" and "Opportunity" are starting their fifth year of exploring the surface of Mars, well over ten times their nominal 90-day design lifetime. This lecture discusses the Mars Exploration Rovers, presents the current mission status for the extended mission, some of the most results from the mission and how it is affecting our current view of Mars, and briefly presents the plans for the coming NASA missions to the surface of Mars and concepts for exploration with robots and humans into the next decade, and beyond. Four Years on Mars: the Mars Exploration Rovers Geoffrey A. Landis NASA John Glenn Research Center http://www.sff.net/people/geoffrey.landis Presentation at MIT Department of Aeronautics and Astronautics, January 18, 2008 Exploration - Landis Mars viewed from the Hubble Space Telescope Exploration - Landis Views of Mars in the early 20th century Lowell 1908 Sciaparelli 1888 Burroughs 1912 (cover painting by Frazetta) Tales of Outer Space ed. Donald A. Wollheim, Ace D-73, 1954 (From Winchell Chung's web page projectrho.com) Exploration - Landis Past Missions to Mars: first close up images of Mars from Mariner 4 Mariner 4 discovered Mars was a barren, moon-like desert Exploration - Landis Viking 1976 Signs of past water on Mars? orbiter Photo from orbit by the 1976 Viking orbiter Exploration - Landis Pathfinder and Sojourner Rover: a solar-powered mission