Introduction

Total Page:16

File Type:pdf, Size:1020Kb

Introduction BR-110 layout 2/21/01 10:57 AM Page 2 INTRODUCTION The mandate of the European Space Operations Satellite nativation is the process by which a Centre is to conduct mission operations for satellite is brought to and kept in the desired ESA Satellites and to establish, operate and orbit and by which the required body maintain the necessary ground segment orientation (attitude) is acquired. It involves infrastructure. determination, prediction and control of the satellite orbit hand in hand with determination and control of the satellite attitude. Changes in Mission Operations orbit and attitude are effected by the Mission operations is the process involving execution of often complex manoeuvres operations planning, satellite monitoring and under ground control, using for example the control, in-orbit navigation, and data processing on-board thrusters. and distribution, by which the satellite mission objectives are achieved, be they the collection of meteorological or scientific data or the Ground Segment Infrastructure provision of a telecommunication service. ESOC has established a comprehensive ground segment infrastructure suitable and ready to Monitoring and control starts as soon as the support various types of missions, each having satellite is separated from the launch vehicle, its different demands, requirements and purpose being to activate the on-board systems constraints. This infrastructure encompasses all for the tasks ahead in the challenging facilities and services needed for mission environment of space. Soon afterwards, the operations and includes a network of ground payload has to be configured to enable it to stations around the world, a number of control play its part in exploiting the mission according centres, payload data-processing facilities, to plans based on the wishes of the users. It is a spacecraft control systems, simulation systems round-the-clock task performed throughout the and communications systems. All ground duration of the mission. facilities have to be highly reliable and maintainable: cost-effectiveness in operations is Whenever the satellite is visible from the achieved by careful introduction of new ground, health and status are monitored, a task technology. Lift-off of an Ariane-5 involving the analysis of as many as five launcher thousand telemetry parameters every minute. The infrastructure is primarily intended for ESA Operations are effected through instructions missions, but can be made available to external sent to the spacecraft in the form of Agencies and industry. Depending on the type telecommands to change on-board settings or of agreement, ESOC can provide all types of to activate payload equipment. Continuous service, from full mission operations to monitoring is necessary to verify correct consultancy. execution of up to one hundred commands per minute. 2 BR-110 layout 2/21/01 10:58 AM Page 3 Mission Success The mission operations phase is generally the final and arguably the most critical phase in a space project, during which the return on investment is to be realised: the return in this case is the quantity, quality and availabiliity of mission products or services, which in turn depend heavily on the effectiveness of mission operations. Mission success is then gauged by the return of mission products, and by the ability to recover from deficiencies or anomalies in the orbiting spacecraft. Since 1967 ESOC has successfully conducted more than 40 satellite missions (Appendix 1), each presenting a different challenge to the operations staff, including: – Science missions in near-Earth, highly swing-by around the Earth in 1990 took One of the first Control eccentric and interplanetary orbits, Giotto into an orbit in which it was to Rooms for the ESRO-2 – Microgravity missions in near-Earth orbit encounter comet Grigg-Skjellerup two years Mission – Earth observation missions in near-Earth later: the operations involved in the orbit hibernation and blind reactivation of the – Meteorological missions in geostationary spacecraft are of historical significance. orbit – The successful execution of the Eureca – Telecommunications missions in (European Retrievable Carrier) mission, geostationary orbit including the deployment and retrieval of the spacecraft by the US Space Shuttle Of particular note are the following missions, proved ESOC’s ability to control from the for which ESOC had full responsibility: ground complex rendezvous and docking – The navigation of the Giotto spacecraft to manoeuvres in space, in close cooperation encounter Comet Halley in 1986 was a with another Agency (NASA). spectacular success. After surviving the encounter, a historical gravity-assist Multi-mission control Area at ESOC 3 BR-110 layout 2/21/01 10:58 AM Page 4 Image composition of MOP-2 and ADC – Between 1977 and 1995, ESOC conducted Olympus and Hipparcos, the latter being of the six European Meteosat missions particular importance. In August 1989, involving full spacecraft monitoring and Hipparcos, which was intended to undertake a control, navigation, payload control, payload 100 000-star survey from geostationary orbit, data processing, image data extraction, data was left stranded in transfer orbit when its Meteosat MOP-1 dissemination and archiving. The service apogee boost motor failed to ignite. Within provided to the meteorological community three months a revised mission had been was exemplary in its quality and continuous defined and the necessary modifications to the availability. ground segment and on-board software had been made, enabling the mission to be In total, four otherwise doomed missions have conducted in the unfavourable elliptical orbit. Eureca returning to the been recovered by ESOC, namely TD-1A, Geos-1, Outliving the planned mission duration, Space Shuttle Hipparcos operations continued for three years to successfully achieve all intended scientific objectives. The task of operations as conducted from ESOC is now a well-developed discipline involving highly skilled staff in intensive activities both in the preparations phase and in the operations execution phase. The philosophy for the control and operation of the various types of satellite intended to serve the needs of ESA’s different spheres of interest is founded on the principles established during more than 30 years’ experience. ESOC is recognised as a leading centre of excellence in Space Mission Operations that is unique in Europe. Conscious of the need to vigilantly maintain its high standards of quality, ESOC achieved ISO 9001 certification in 1999. This extensive expertise allied with the comprehensive and technologically advanced ground segment infrastructure, ensures that ESOC maintains its position as mission-operations authority for ESA satellites and guarantees that, as such, it constitutes an invaluable resource for the Agency’s future space projects. 4 BR-110 layout 2/21/01 10:58 AM Page 5 PREPARING THE MISSION Introduction The various units within ESOC then embark on In most cases, ESOC involvement starts when the execution of the preparatory tasks that the mission and satellite concept is being have to be completed during the period developed, especially as regards analysis of the covering the satellite’s development, integration type of orbit required, the provisions that need and test programme (usually about five years). to be included in the spacecraft design to The culmination of the preparatory phase is the facilitate the operational tasks and the ground- full readiness and availability of all facilities, segment facilities required to support the services and personnel and the ‘freezing’ of mission. Such involvement continues throughout all software systems, hardware and the assessment phase and the satellite Phase A documentation prior to the start of mission studies. operations. Once a mission has been selected, ESOC will be The principal activities to be undertaken by involved in providing operations requirements ESOC in the mission preparations phase cover a applicable to the spacecraft Phases B and C/D, in wide range of disciplines, as illustrated in the the formulation of a thorough specification of the Figure below and described in the following ground segment services and facilities needed to sections. support the mission and in establishing the necessary interfaces for exchange of data and information between the customer and ESOC. 5 BR-110 layout 2/21/01 10:58 AM Page 6 Mission Analysis Mission analysis is the term used to describe the mathematical analysis of satellite orbits, performed to determine how best to achieve the Table 1: Influence of orbit on satellite design mission objectives in terms of achievable orbit, launch vehicle, ground station utilisation, Mission Type will drive: operational complexity and lifetime. – Launch energy vs. satellite mass – Selection of launch vehicle and orbit injection strategy These very important aspects are considered by – Satellite Dimensions ESOC early in the formative stage of the mission design in close cooperation with the Project. Orbit Injection and Control requirements will determine: This is essential, since, later on, the results will – Orbit Control concepts (mono/bi-propellant/solid fuel) be given to the satellite Prime Contractor as – Number and type of manoeuvres needed design driving information, for the selected orbit – Fuel needed on board satellite and the derived operations concept will have an influence on many aspects of the satellite Actual Orbit will determine: design, as can be seen from Table 1. – Orbital lifetime
Recommended publications
  • Giotto Steals a Ride
    NEWS COM8ARYPROBE------------------------------------- JAPANESE UNIVERSITIES----­ Giotto steals a ride MurmUrS of complaint Washington Munich this is a bargain", says GEM project scien­ JAPAN's national university professors are THE Earth lost a minute fraction of its tist Gerhard Schwehm. Schwehm said that all employees of the government, which orbital velocity earlier this week as the the second flyby would be a unique oppor­ puts them in an odd position when they European Space Agency (ESA) Giotto tunity to expand knowledge of comets. It want to protest to the government about space probe stole a little of the Earth's will be especially interesting, he said, to university conditions. But last month, the energy to help it on its way to a rendezvous study the interaction of the coma of the Association of National Universities finally with the comet Grigg Skjellerup. It was comet and the solar wind, as well as to succeeded, after years of trying, in winning the first time the manoeuvre, the same compare the distribution and optical funds from the Ministry of Education, "gravity assist" that helped the NASA properties of dust around Comet Grigg Culture and Science to set up a committee Voyager probe on its journey from Jupiter Skjellerup with that around Comet to study their own financial difficulties. out to Saturn and Neptune, had been exe­ Halley, which had at least 100 times more The association represents all the 93 cuted using the gravitation field of Earth. of it. national universities directly supported by According to ESA researcher Trevor Giotto was one of five spacecraft to the government and has responsibility for Morley, Giotto will gain 3.1 km/sec in approach Comet Halley in 1986, but it setting up the general entrance examination.
    [Show full text]
  • Rosetta Craft Makes Historic Comet Rendezvous European Space Agency's Comet-Chasing Mission Arrives After 10-Year Journey
    NATURE | NEWS Rosetta craft makes historic comet rendezvous European Space Agency's comet-chasing mission arrives after 10-year journey. Elizabeth Gibney 06 August 2014 ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA Comet 67P/Churyumov–Gerasimenko, as seen by Rosetta from a distance of 285 kilometres. No one can deny that it was an epic trip. The European Space Agency's comet-chasing Rosetta spacecraft has arrived at its quarry, after launching more than a decade ago and travelling 6.4 billion kilometres through the Solar System. That makes it the first spacecraft to rendezvous with a comet, and takes the mission a step closer to its next, more ambitious goal of making the first ever soft landing on a comet. Speaking from mission control in Darmstadt, Germany, Matt Taylor, Rosetta project scientist for the European Space Agency (ESA), called the space mission “the sexiest there’s ever been”. Rosetta is now within 100 kilometres of its target, comet 67P/Churyumov–Gerasimenko (or 67P for short), which in July was discovered to be shaped like a rubber duck. After a six-minute thruster burn, at 11:29 a.m. local time on 6 August, ESA scientists confirmed that Rosetta had moved into the same orbit around the Sun as the comet. Rosetta is now moving at a walking pace relative to the motion of 67P — though both are hurtling through space at 15 kilometres per second. Unlike NASA’s Deep Impact and Stardust craft, and ESA’s Giotto mission, which flew by their target comets at high speed, Rosetta will now stay with the comet, taking a ring-side seat as 67P approaches the Sun, and eventually swings around it in August 2015.
    [Show full text]
  • Detecting, Tracking and Imaging Space Debris
    r bulletin 109 — february 2002 Detecting, Tracking and Imaging Space Debris D. Mehrholz, L. Leushacke FGAN Research Institute for High-Frequency Physics and Radar Techniques, Wachtberg, Germany W. Flury, R. Jehn, H. Klinkrad, M. Landgraf European Space Operations Centre (ESOC), Darmstadt, Germany Earth’s space-debris environment tracked, with estimates for the number of Today’s man-made space-debris environment objects larger than 1 cm ranging from 100 000 has been created by the space activities to 200 000. that have taken place since Sputnik’s launch in 1957. There have been more than 4000 The sources of this debris are normal launch rocket launches since then, as well as many operations (Fig. 2), certain operations in space, other related debris-generating occurrences fragmentations as a result of explosions and such as more than 150 in-orbit fragmentation collisions in space, firings of satellite solid- events. rocket motors, material ageing effects, and leaking thermal-control systems. Solid-rocket Among the more than 8700 objects larger than 10 cm in Earth orbits, motors use aluminium as a catalyst (about 15% only about 6% are operational satellites and the remainder is space by mass) and when burning they emit debris. Europe currently has no operational space surveillance aluminium-oxide particles typically 1 to 10 system, but a powerful radar facility for the detection and tracking of microns in size. In addition, centimetre-sized space debris and the imaging of space objects is available in the form objects are formed by metallic aluminium melts, of the 34 m dish radar at the Research Establishment for Applied called ‘slag’.
    [Show full text]
  • Stardust Comet Flyby
    NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Stardust Comet Flyby Press Kit January 2004 Contacts Don Savage Policy/Program Management 202/358-1727 NASA Headquarters, Washington DC Agle Stardust Mission 818/393-9011 Jet Propulsion Laboratory, Pasadena, Calif. Vince Stricherz Science Investigation 206/543-2580 University of Washington, Seattle, WA Contents General Release ……………………………………......………….......................…...…… 3 Media Services Information ……………………….................…………….................……. 5 Quick Facts …………………………………………..................………....…........…....….. 6 Why Stardust?..................…………………………..................………….....………......... 7 Other Comet Missions ....................................................................................... 10 NASA's Discovery Program ............................................................................... 12 Mission Overview …………………………………….................……….....……........…… 15 Spacecraft ………………………………………………..................…..……........……… 25 Science Objectives …………………………………..................……………...…........….. 34 Program/Project Management …………………………...................…..…..………...... 37 1 2 GENERAL RELEASE: NASA COMET HUNTER CLOSING ON QUARRY Having trekked 3.2 billion kilometers (2 billion miles) across cold, radiation-charged and interstellar-dust-swept space in just under five years, NASA's Stardust spacecraft is closing in on the main target of its mission -- a comet flyby. "As the saying goes, 'We are good to go,'" said project manager Tom Duxbury at NASA's Jet
    [Show full text]
  • SPICE for ESA Missions
    SPICE for ESA Missions Marc Costa Sitjà RHEA Group for ESA SPICE and Auxiliary Data Engineer PSIDA, Saint Louis, MO, EEUU 21/09/2017 Issue/Revision: 1.0 Reference: Presentation Reference Status: Issued ESA UNCLASSIFIED - Releasable to the Public SPICE in a nutshell Ø SPICE is an information system that uses ancillary data to provide Solar System geometry information to scientists and engineers for planetary missions in order to plan and analyze scientific observations from space-born instruments. SPICE was originally developed and maintained by the Navigation and Ancillary Information Facility (NAIF) team of the Jet Propulsion Laboratory (NASA). Ø “Ancillary data” are those that help scientists and engineers determine: ● where the spacecraft was located ● how the spacecraft and its instruments were oriented (pointed) ● what was the location, size, shape and orientation of the target being observed ● what events were occurring on the spacecraft or ground that might affect interpretation of science observations Ø SPICE provides users a large suite of SW used to read SPICE ancillary data files to compute observation geometry. Ø SPICE is open, very well tested, extensively used and provides tons of resources to learn it and implement it. Ø SPICE is the recommended means of archiving ancillary data by NASA’s PDS and by the IPDA Ø The ancillary data (kernels) comes from: The S/C, MOC/SGS, S/C manufacturer and Instrument teams, Science Organizations. Author Name | Presentation Reference | ESAC | 23/11/2015 | Slide 2 ESA UNCLASSIFIED - Releasable to the Public SPICE in a nutshell Components Data Files Contents Producers Source* • MOC provides data, SGS • Fdyn & S Spacecraft and target generates kernels.
    [Show full text]
  • Jjmonl 1603.Pmd
    alactic Observer GJohn J. McCarthy Observatory Volume 9, No. 3 March 2016 GRAIL - On the Trail of the Moon's Missing Mass GRAIL (Gravity Recovery and Interior Laboratory) was a NASA scientific mission in 2011/12 to map the surface of the moon and collect data on gravitational anomalies. The image here is an artist's impres- sion of the twin satellites (Ebb and Flow) orbiting in tandem above a gravitational image of the moon. See inside, page 4 for information on gravitational anomalies (mascons) or visit http://solarsystem. nasa.gov/grail. The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky It is through their efforts that the McCarthy Observatory Technical Support has established itself as a significant educational and Bob Lambert recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Mike Chiarella Roger Moore Route Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Cecilia Dietrich Marc Polansky Dirk Feather Joe Privitera Randy Fender Monty Robson Randy Finden Don Ross John Gebauer Gene Schilling Elaine Green Katie Shusdock Tina Hartzell Paul Woodell Tom Heydenburg Amy Ziffer In This Issue "OUT THE WINDOW ON YOUR LEFT" ............................... 4 SUNRISE AND SUNSET ...................................................... 13 MARE HUMBOLDTIANIUM AND THE NORTHEAST LIMB ......... 5 JUPITER AND ITS MOONS ................................................. 13 ONE YEAR IN SPACE ....................................................... 6 TRANSIT OF JUPITER'S RED SPOT ....................................
    [Show full text]
  • ESA & ESOC Overview
    NASA PM Challenge 2010 Developing the International Program/Project Management Community 9/10 February 2010 Dr. Bettina Böhm Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 1 Used with Permission PURPOSE OF ESA / ACTIVITIES “To provide for and promote, for exclusively Space science peaceful purposes, cooperation among Human spaceflight European states in space research and Exploration technology and their space applications.” Earth observation Launchers [Article 2 of ESA Convention] Navigation ESA is one of the few space agencies Telecommunications in the world to combine responsibility Technology in all areas of space activity. Operations Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 2 ESA FACTS AND FIGURES Over 30 years of experience 18 Member States 2080 staff, thereof 880 in Program Directorates, 790 in Operations and Technical Support and 410 in other Support Directorates 3 500 million Euros budget Over 60 satellites designed and tested Over 60 satellites operated in-flight and 8 missions rescued 16 scientific satellites in operation Five types of launcher developed More than 180 launches made Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 3 ESA Locations EAC (Cologne) Salmijaervi ESTEC Astronaut training (Noordwijk) Satellite technology development and testing Harwell ESOC ESA HQ (Darmstadt) (Paris) Brussels Satellite operations and ground system technology development ESAC (Villanueva de la Cañada Oberpfaffenhofen
    [Show full text]
  • SPICE for ESA Planetary Missions
    Marc Costa Sitjà European Space Agency/ESAC (ESA SPICE Service) SPICE for ESA Planetary Missions Introduction The ESA SPICE Service (ESS) leads the SPICE operations for ESA Science and Exploration missions. The SPICE is an information system that uses ancillary data to group is responsible for the generation, development, maintenance and archive of the SPICE Kernel provide Solar System geometry information to scientists and Datasets for the ESA Planetary Missions (ExoMars 2016, Mars Express, Rosetta, BepiColombo, JUICE, engineers for planetary missions in order to plan and analyze Venus Express and Solar Orbiter). scientific observations from space-born instruments. SPICE is developed and maintained by the Navigation and Ancillary ESS develops and operates software to convert orbit, attitude, telemetry and spacecraft clock correlation Information Facility (NAIF) team of the Jet Propulsion data into the corresponding SPICE formats. ESS also provides consultancy and support to the Science Laboratory (NASA). Ground Segments and the Science Community of the planetary missions for SPICE and ancillary data management. SPICE Kernel Datasets ESA SPICE Operational The main purpose of the ESS for the Planetary Science Community is to provide a complete, consistent, high-quality, Service Home: Kernel Datasets: validated and up-to-date SPICE Kernel Dataset (SKD) for the given mission in order to be able to use SPICE with it. Available, SPICE Kernel Datasets: Releases and support to the community is provided Legacy Operations Study ESA NAIF PSA Mission Status (1) Studies (pre-operational): JUICE, BepiColombo, Solar Orbiter (and support to ALTEC for the ExoMars RSP kernels). These FTP Mirror Archive kernel datasets are characterized for being highly dynamic with changes in Instrument and S/C frames definitions.
    [Show full text]
  • Orbiting Debris: a Space Environmental Problem (Part 4 Of
    Orbiting Debris: A Since Environmential Problem ● 3 Table 2--of Hazardous Interference by environment. Yet, orbital debris is part of a Orbital Debris larger problem of pollution in space that in- cludes radio-frequency interference and inter- 1. Loss or damage to space assets through collision; ference to scientific observations in all parts of 2. Accidental re-entry of space hardware; the spectrum. For example, emissions at ra- 3. Contamination by nuclear material of manned or unmanned spacecraft, both in space and on Earth; dio frequencies often interfere with radio as- 4. Interference with astronomical observations, both from the tronomy observations. For several years, ground and in space; gamma-ray astronomy data have been cor- 5. Interference with scientific and military experiments in space; rupted by Soviet intelligence satellites that 14 6. Potential military use. are powered by unshielded nuclear reactors. The indirect emissions from these satellites SOURCE: Space Debris, European Space Agency, and Office of Technology As- sessment. spread along the Earth’s magnetic field and are virtually impossible for other satellites to Earth. The largest have attracted worldwide escape. The Japanese Ginga satellite, attention. 10 Although the risk to individuals is launched in 1987 to study gamma-ray extremely small, the probability of striking bursters, has been triggered so often by the populated areas still finite.11 For example: 1) Soviet reactors that over 40 percent of its available observing time has been spent trans- the U.S.S.R. Kosmos 954, which contained a 15 nuclear power source,12 reentered the atmos- mitting unintelligible “data.” All of these phere over northwest Canada in 1978, scatter- problem areas will require attention and posi- ing debris over an area the size of Austria; 2) a tive steps to guarantee access to space by all Japanese ship was hit in 1969 by pieces of countries in the future.
    [Show full text]
  • Learning from Fukushima: Nuclear Power in East Asia
    LEARNING FROM FUKUSHIMA NUCLEAR POWER IN EAST ASIA LEARNING FROM FUKUSHIMA NUCLEAR POWER IN EAST ASIA EDITED BY PETER VAN NESS AND MEL GURTOV WITH CONTRIBUTIONS FROM ANDREW BLAKERS, MELY CABALLERO-ANTHONY, GLORIA KUANG-JUNG HSU, AMY KING, DOUG KOPLOW, ANDERS P. MØLLER, TIMOTHY A. MOUSSEAU, M. V. RAMANA, LAUREN RICHARDSON, KALMAN A. ROBERTSON, TILMAN A. RUFF, CHRISTINA STUART, TATSUJIRO SUZUKI, AND JULIUS CESAR I. TRAJANO Published by ANU Press The Australian National University Acton ACT 2601, Australia Email: [email protected] This title is also available online at press.anu.edu.au National Library of Australia Cataloguing-in-Publication entry Title: Learning from Fukushima : nuclear power in East Asia / Peter Van Ness, Mel Gurtov, editors. ISBN: 9781760461393 (paperback) 9781760461409 (ebook) Subjects: Nuclear power plants--East Asia. Nuclear power plants--Risk assessment--East Asia. Nuclear power plants--Health aspects--East Asia. Nuclear power plants--East Asia--Evaluation. Other Creators/Contributors: Van Ness, Peter, editor. Gurtov, Melvin, editor. All rights reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying or otherwise, without the prior permission of the publisher. Cover design and layout by ANU Press. Cover image: ‘Fukushima apple tree’ by Kristian Laemmle-Ruff. Near Fukushima City, 60 km from the Fukushima Daiichi Nuclear Power Plant, February 2014. The number in the artwork is the radioactivity level measured in the orchard—2.166 microsieverts per hour, around 20 times normal background radiation. This edition © 2017 ANU Press Contents Figures . vii Tables . ix Acronyms and abbreviations .
    [Show full text]
  • In Situ Observations of Cometary Nuclei 211
    Keller et al.: In Situ Observations of Cometary Nuclei 211 In Situ Observations of Cometary Nuclei H. U. Keller Max-Planck-Institut für Aeronomie D. Britt University of Central Florida B. J. Buratti Jet Propulsion Laboratory N. Thomas Max-Planck-Institut für Aeronomie (now at University of Bern) It is only through close spacecraft encounters that cometary nuclei can be resolved and their properties determined with complete confidence. At the time of writing, only two nuclei (those of Comets 1P/Halley and 19P/Borrelly) have been observed, both by rapid flyby missions. The camera systems onboard these missions have revealed single, solid, dark, lumpy, and elongated nuclei. The infrared systems gave surface temperatures well above the free sublimation tempera- ture of water ice and close to blackbody temperatures. The observed nuclei were much more similar than they were different. In both cases, significant topography was evident, possibly reflecting the objects’ sublimation histories. Dust emission was restricted to active regions and jets in the inner comae were prevalent. Active regions may have been slightly brighter than inert areas but the reflectance was still very low. No activity from the nightside was found. In this chapter, the observations are presented and comparisons are made between Comets Halley and Borrelly. A paradigm for the structure of cometary nuclei is also described that implies that the nonvolatile component defines the characteristics of nuclei and that high porosity, large- scale inhomogeneity, and moderate tensile strength are common features. 1. INTRODUCTION It is important to emphasize that prior to the spacecraft encounters with Comet 1P/Halley in 1986, the existence of The nuclei of most comets are too small to be resolved a nucleus was merely inferred from coarse observations.
    [Show full text]
  • Comet Interceptor: a Mission to an Ancient World
    EPSC Abstracts Vol. 14, EPSC2020-574, 2020 https://doi.org/10.5194/epsc2020-574 Europlanet Science Congress 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Comet Interceptor: A mission to an ancient world Cecilia Tubiana1, Geraint Jones2,3, Colin Snodgrass4, and the the Comet Interceptor Team* 1Max Planck Institute for Solar System Research, Goettingen, Germany ([email protected]) 2Mullard Space Science Laboratory, University College London, Surrey, UK 3The Centre for Planetary Sciences at UCL/Birkbeck, London, UK 4Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh *A full list of authors appears at the end of the abstract Comets are the most pristine objects in our Solar System. Having spent most of their life at large distance from the Sun, where they remained mostly unaffected by solar radiation, comets are the most unaltered remnants from the era of planet formation. In June 2019, a multi-spacecraft project – Comet Interceptor – was selected by the European Space Agency (ESA) as its next planetary mission, and the first in its new class of Fast (F) projects [1]. The mission’s primary science goal is to characterise, for the first time, a long-period comet – preferably one which is dynamically new – or an interstellar object. An encounter with a comet approaching the Sun for the first time will provide valuable data to complement that from all previous comet missions: the surface of such an object would be being heated to temperatures above the its constituent ices’ sublimation point for the first time since its formation.
    [Show full text]