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Lunar Impact Crater Identification and Age Estimation with Chang’E
ARTICLE https://doi.org/10.1038/s41467-020-20215-y OPEN Lunar impact crater identification and age estimation with Chang’E data by deep and transfer learning ✉ Chen Yang 1,2 , Haishi Zhao 3, Lorenzo Bruzzone4, Jon Atli Benediktsson 5, Yanchun Liang3, Bin Liu 2, ✉ ✉ Xingguo Zeng 2, Renchu Guan 3 , Chunlai Li 2 & Ziyuan Ouyang1,2 1234567890():,; Impact craters, which can be considered the lunar equivalent of fossils, are the most dominant lunar surface features and record the history of the Solar System. We address the problem of automatic crater detection and age estimation. From initially small numbers of recognized craters and dated craters, i.e., 7895 and 1411, respectively, we progressively identify new craters and estimate their ages with Chang’E data and stratigraphic information by transfer learning using deep neural networks. This results in the identification of 109,956 new craters, which is more than a dozen times greater than the initial number of recognized craters. The formation systems of 18,996 newly detected craters larger than 8 km are esti- mated. Here, a new lunar crater database for the mid- and low-latitude regions of the Moon is derived and distributed to the planetary community together with the related data analysis. 1 College of Earth Sciences, Jilin University, 130061 Changchun, China. 2 Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China. 3 Key Laboratory of Symbol Computation and Knowledge Engineering of Ministry of Education, College of Computer Science and Technology, Jilin University, 130012 Changchun, China. 4 Department of Information Engineering and Computer ✉ Science, University of Trento, I-38122 Trento, Italy. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Edward East (1602–C
Valerie J. Finch, Adrian A. Finch, Anthony W. Finch Edward East (1602–c. 1695). Part 1 – Early Stuart period and Commonwealth Antiquarian Horology, Volume 38, No. 3 (September 2017), pp. 343–364 The AHS (Antiquarian Horological Society) is a charity and learned society formed in 1953. It exists to encourage the study of all matters relating to the art and history of time measurement, to foster and disseminate original research, and to encourage the preservation of examples of the horological and allied arts. To achieve its aims the AHS holds meetings and publishes books as well as its quarterly peer-reviewed journal Antiquarian Horology. The journal, printed to the highest standards fully in colour, contains a variety of articles and notes, the society’s programme, news, letters and high-quality advertising (both trade and private). A complete collection of the journals is an invaluable store of horological information, the articles covering diverse subjects including many makers from the famous to the obscure. The entire back catalogue of Antiquarian Horology, every single page published since 1953, is available on-line, fully searchable. It is accessible for AHS members only. For more information visit www.ahsoc.org Volume 38, No. 3 (September 2017) contains the following articles Mechanical clocks and the advent of scientific astronomy by Dietrich Matthes & Rocío Sánchez-Barrios NUMBER THREE VOLUME THIRTY-EIGHT SEPTEMBER 2017 Edward East (1602–c. 1695). Part 1 – Early Stuart period and Commonwealth by Valerie J. Finch, Adrian A. Finch, Anthony W. Finch Galileo, Huygens and the invention of the pendulum clock by Sebastian Whitestone Martin Burgess, sculptural clockmaker by Jonathan Betts The horological legacy of Stanley John Wise by Geoffrey A. -
July 2020 in This Issue Online Readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 Click on Images an Invitation to Join ALPO 3 for Hyperlinks
A publication of the Lunar Section of ALPO Edited by David Teske: [email protected] 2162 Enon Road, Louisville, Mississippi, USA Recent back issues: http://moon.scopesandscapes.com/tlo_back.html July 2020 In This Issue Online readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 click on images An Invitation to Join ALPO 3 for hyperlinks. Observations Received 4 By the Numbers 7 Submission Through the ALPO Image Achieve 4 When Submitting Observations to the ALPO Lunar Section 9 Call For Observations Focus-On 9 Focus-On Announcement 10 2020 ALPO The Walter H. Haas Observer’s Award 11 Sirsalis T, R. Hays, Jr. 12 Long Crack, R. Hill 13 Musings on Theophilus, H. Eskildsen 14 Almost Full, R. Hill 16 Northern Moon, H. Eskildsen 17 Northwest Moon and Horrebow, H. Eskildsen 18 A Bit of Thebit, R. Hill 19 Euclides D in the Landscape of the Mare Cognitum (and Two Kipukas?), A. Anunziato 20 On the South Shore, R. Hill 22 Focus On: The Lunar 100, Features 11-20, J. Hubbell 23 Recent Topographic Studies 43 Lunar Geologic Change Detection Program T. Cook 120 Key to Images in this Issue 134 These are the modern Golden Days of lunar studies in a way, with so many new resources available to lu- nar observers. Recently, we have mentioned Robert Garfinkle’s opus Luna Cognita and the new lunar map by the USGS. This month brings us the updated, 7th edition of the Virtual Moon Atlas. These are all wonderful resources for your lunar studies. -
Glossary of Lunar Terminology
Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites. -
Harrison's Barometric Compensation Keeping It Simple
Harrison’s Barometric Compensation Keeping it Simple: A Description from Practice Jonathan Betts Introduction The last few years have seen considerable excitement, and some controversy, over the astonishingly successful trials of Burgess Clock B at the Observatory. In association with this work, there have been a number of published articles, including one last year in which we at the Observatory narrated the main facts surrounding the trials of Clock B [Ref.1: ‘A Second in 100 Days – The Result’ Rory McEvoy, Horological Journal, September 2015, pp 407-410]. Other published papers have provided theories as to how Harrison’s system might work, giving lots of historical context to those theories, [Ref: 2. ‘The Harrison Hill Test’, M.K.Hobden, HSN 2012-5 et Seq.; 3. ‘Dominion and Dynamic Stability’, M.K. Hobden, HSN 2015-4, pp 9-19; and 4. ‘Investigating the Harrison Pendulum Oscillator’, John Haine & Andrew Millington, HSN2016-3] and in this issue John Haine and Andrew Millington continue their commentary on Harrison’s pendulum oscillator and provide a theoretical model for how the barometric compensation system works. Adjusting a Harrison Clock As is now well known, adjusting a Harrison-type pendulum clock for optimum performance, including introducing compensation for barometric pressure changes, involves carrying out a series of what has been termed ‘hill tests’. In discussing this work among horologists, it is clear that many are of the opinion that the whole business is exceedingly complicated and time consuming. To quote one commentator, adjusting a Harrison clock appears to involve “overwhelming time and effort in fine-tuning”. -
Read Ebook {PDF EPUB} My Time by Paul Harrison My Time [Harrison, Paul] on Amazon.Com
Read Ebook {PDF EPUB} My Time by Paul Harrison My Time [Harrison, Paul] on Amazon.com. *FREE* shipping on qualifying offers. My Time Dec 20, 2012 · Paul Harrison tells the story of his year as World Champion, revealing the determination and willpower that is required to remain at the top of stock car racing. From the exhilaration of victory to the pressure of performing under the gold roof, My Time is a unique behind-the- scenes account of this brutal motorsport. Paul Harrison tells the story of his year as World Champion, revealing the determination and willpower that is required to remain at the top of stock car racing. From the exhilaration of victory to the pressure of performing under the gold roof, My Time is a unique behind-the-scenes account of this brutal motorsport. Nov 01, 2012 · My Time. “I just feel that my time has come.”. When Paul Harrison uttered those words before the Formula 1 Stock Car World Final in 2011, he was about to make history. It was the culmination of a life spent trying to match his father’s achievement and wear the gold roof that signifies the World Champion. Paul Harrison tells the story of his year as World Champion, revealing the determination … Thank you for your patience while we retrieve your images. Home | Photo Galleries | Recent | Guestbook | Profile | Contact My Time › Customer reviews ... This is a great diary of Paul Harrison's year as World Champion. It's great to get into the stock car driver's mind and see behind the scenes, it really makes you appreciate the work that goes on to go racing every weekend. -
The Illustrated Longitude
LONGITUDE The True Story of a Lone Genius Who Solved the Greatest Scientific Problem of His Time DAVA SOBEL Contents 1. Imaginary Lines 2. The Sea Before Time 3. Adrift in a Clockwork Universe 4. Time in a Bottle 5. Powder of Sympathy 6. The Prize 7. Cogmaker’s Journal 8. The Grasshopper Goes to Sea 9. Hands on Heaven’s Clock 10. The Diamond Timekeeper 11. Trial by Fire and Water 12. A Tale of Two Portraits 13. The Second Voyage of Captain James Cook 14. The Mass Production of Genius 15. In the Meridian Courtyard Acknowledgments Sources For my mother, Betty Gruber Sobel, a four-star navigator who can sail by the heavens but always drives by way of Canarsie. 1. Imaginary Lines When I’m playful I use the meridians of longitude and parallels of latitude for a seine, drag the Atlantic Ocean for whales. —MARK TWAIN, Life on the Mississippi Once on a Wednesday excursion when I was a little girl, my father bought me a beaded wire ball that I loved. At a touch, I could collapse the toy into a flat coil between my palms, or pop it open to make a hollow sphere. Rounded out, it resembled a tiny Earth, because its hinged wires traced the same pattern of intersecting circles that I had seen on the globe in my schoolroom— the thin black lines of latitude and longitude. The few colored beads slid along the wire paths haphazardly, like ships on the high seas. My father strode up Fifth Avenue to Rockefeller Center with me on his shoulders, and we stopped to stare at the statue of Atlas, carrying Heaven and Earth on his. -
Lunar Observing Report February 12Th 2011- Lichfield - 66% Waxing Gibbous
Lunar Observing Report February 12th 2011- Lichfield - 66% Waxing Gibbous It was with some trepidation that I ventured out on Saturday after my last experience with the new Televue 3.7mm Ethos. Would I suffer the same problems of kidney beaning blackouts and that horrid yellow/red ‘flaming halo’....? I’d had some thought provoking responses from far more 1 experienced observers to my query on the American forum; ‘Cloudy Nights’. Suggestions ranged from making sure the eyepiece was seated correctly in the diagonal, atmospheric distorsions, faulty eyepiece etc, yet the most common theme appeared to be the link between my scopes f/ratio (greater than f7), a small (less than) 0.5mm exit pupil, ultra wide (110-FOV) with a large eye lens - as well as trying to view a bright full moon too! As one commentator stated, ”the brightness of the full moon causes your eye's pupil to constrict, which makes it all too easy to sample only a portion of the (already small), exit pupil with your eye pupil (and interfering with eye placement), especially when you're looking 55 degrees off axis! Before trying to look around, I'd suggest trying to look on axis and letting your peripheral vision soak in the 110 degree field.” Also, “diameter of exit pupil figures are mostly consigned into side-to-side tolerance for eye positioning, and typically the manifestation is not so much blackouts but dimming of the view as one clips part of the light for any given point by letting the eye wander too much to one side or the other. -
Telling the Time in Norwich
Telling the time in Norwich Includes details of more than 50 viewable clocks and sundials Telling the time in Norwich Contents Introduction 1 Clockmaking in Norwich and Norfolk 3 The Gurney Clock 4 Clocks as memorials 5 Clocks as advertising 5 Ringing out the time 6 Clocks in the city landscape 6 The clocks directory 7 Sundials 24 Clocks and sundials shown on the maps 29 This project has been undertaken by the members of the Norwich Society Civic Environment Committee : Alan ‘Theo’ Theobald, John Trevelyan, Jonathan Hooton, Kate Nash, Michael Cross, Roy Holmes, Sue Pike and Sue Roe. Photographs are by committee members except where otherwise credited. The postcards are from the Norwich Society’s collection. The Society would like to thank Simon Michlmayr (S. Michlmayr & Co) and David Payne (British Sundial Society) for their time in discussing clocks and sundials, for the information they have imparted to us and for permission to use the photograph on page 2. David Payne’s Burlingham Sundial Trail can be accessed at https://sundialtrailsoftheburlinghamwalks.wordpress.com/ The Society has found the following publications and websites of use: • Norfolk and Norwich Clocks and Clockmakers (Clifford and Yvonne Bird, Phillimore 1996) • Norwich Knowledge (Michael Loveday, 2011) • The Medieval Churches of the City of Norwich (Nicholas Groves, Norwich HEART and East Publishing, 2010) • http://sundialsoc.org.uk/ [British Sundial Society] • https://greenwichmeantime.com/ • https://www.rmg.co.uk/discover/explore/greenwich-mean-time-gmt Introduction The Norwich Society’s Civic Environment Committee usually carries out an audit or survey each year. In 2017 we decided to look at public clocks and sundials. -
Science Concept 3: Key Planetary
Science Concept 6: The Moon is an Accessible Laboratory for Studying the Impact Process on Planetary Scales Science Concept 6: The Moon is an accessible laboratory for studying the impact process on planetary scales Science Goals: a. Characterize the existence and extent of melt sheet differentiation. b. Determine the structure of multi-ring impact basins. c. Quantify the effects of planetary characteristics (composition, density, impact velocities) on crater formation and morphology. d. Measure the extent of lateral and vertical mixing of local and ejecta material. INTRODUCTION Impact cratering is a fundamental geological process which is ubiquitous throughout the Solar System. Impacts have been linked with the formation of bodies (e.g. the Moon; Hartmann and Davis, 1975), terrestrial mass extinctions (e.g. the Cretaceous-Tertiary boundary extinction; Alvarez et al., 1980), and even proposed as a transfer mechanism for life between planetary bodies (Chyba et al., 1994). However, the importance of impacts and impact cratering has only been realized within the last 50 or so years. Here we briefly introduce the topic of impact cratering. The main crater types and their features are outlined as well as their formation mechanisms. Scaling laws, which attempt to link impacts at a variety of scales, are also introduced. Finally, we note the lack of extraterrestrial crater samples and how Science Concept 6 addresses this. Crater Types There are three distinct crater types: simple craters, complex craters, and multi-ring basins (Fig. 6.1). The type of crater produced in an impact is dependent upon the size, density, and speed of the impactor, as well as the strength and gravitational field of the target. -
On the Diameter-Depth Relationship of Lunar Craters
Acta Universitatis Carolinae. Mathematica et Physica Jiří Bouška On the diameter-depth relationship of lunar craters Acta Universitatis Carolinae. Mathematica et Physica, Vol. 9 (1968), No. 2, 45--57 Persistent URL: http://dml.cz/dmlcz/142224 Terms of use: © Univerzita Karlova v Praze, 1968 Institute of Mathematics of the Academy of Sciences of the Czech Republic provides access to digitized documents strictly for personal use. Each copy of any part of this document must contain these Terms of use. This paper has been digitized, optimized for electronic delivery and stamped with digital signature within the project DML-CZ: The Czech Digital Mathematics Library http://project.dml.cz 1968 ACTA UNIVERSITATIS CAROLINAE - MATHEMATICA ET PHYSICA No. 2, PAG. 45—57 PUBLICATION OF THE ASTRONOMICAL INSTITUTE OF THE CHARLES UNIVERSITY, No. 55 On the Diameter-Depth Relationship of Lunar Craters JlM BOUSKA Astronomical Institute, Faculty of Mathematics and Physics, Charles University, Prague (Received March 9, 1968) MacDonald's, Baldwin's, Markov's and present writer's results of the investigations of the diameter-depth relationship of lunar craters were analyzed. The relationship shows that all small craters are probably of impact origin. For many small lunar craters Ebert's rule is not valid. I. Introduction At the end of the last century Ebert (1890)* found that the ratios of the depths o of lunar craters to their diameters A decreased with increasing diameter. This relationship between diameter and depth of craters was later known as Ebert's rule. At Ebert's time only a few depths of lunar craters were known with sufficient accuracy.