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Unique Sky Survey Brings New Objects Into Focus 15 June 2009
Unique sky survey brings new objects into focus 15 June 2009 human intervention. The Palomar Transient Factory is a collaboration of scientists and engineers from institutions around the world, including the California Institute of Technology (Caltech); the University of California, Berkeley, and the Lawrence Berkeley National Laboratory (LBNL); Columbia University; Las Cumbres Observatory; the Weizmann Institute of Science in Israel; and Oxford University. During the PTF process, the automated wide-angle 48-inch Samuel Oschin Telescope at Caltech's Palomar Observatory scans the skies using a 100-megapixel camera. The flood of images, more than 100 gigabytes This is the Andromeda galaxy, as seen with the new every night, is then beamed off of the mountain via PTF camera on the Samuel Oschin Telescope at the High Performance Wireless Research and Palomar Observatory. This image covers 3 square Education Network¬-a high-speed microwave data degrees of sky, more than 15 times the size of the full connection to the Internet-and then to the LBNL's moon. Credit: Nugent & Poznanski (LBNL), PTF National Energy Scientific Computing Center. collaboration There, computers analyze the data and compare it to images previously obtained at Palomar. More computers using a type of artificial intelligence software sift through the results to identify the most An innovative sky survey has begun returning interesting "transient" sources-those that vary in images that will be used to detect unprecedented brightness or position. numbers of powerful cosmic explosions-called supernovae-in distant galaxies, and variable Within minutes of a candidate transient's discovery, brightness stars in our own Milky Way. -
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. -
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Printer Friendly - - science news articles online technology magazine articles Printer Friendly Beyond Pluto We are only beginning to discover how vast and strange our solar system truly is By Kathy A. Svitil Illustrations by Don Foley DISCOVER Vol. 25 No. 11 | November 2004 | Astronomy & Physics As a child, Mike Brown had all the trappings of an astronomer-in-the-making, with space books, rocket drawings, and a poster of the planets on his bedroom wall. On it, Pluto was depicted as “this crazy and very eccentric planet,” he says. “It was everyone’s favorite crazy planet.” Brown still recalls the mnemonic he learned for the names of the planets: Martha visits every Monday and—a for asteroids—just stays until noon, period. “The ‘period,’ for Pluto, was always suspicious,” Brown says with a laugh. “It didn’t seem to fit. So maybe that was when I first got the idea that Pluto didn’t belong.” Nowadays Brown, a planetary astronomer at Caltech, has no doubt about Pluto’s place in the solar system: “Pluto is not a planet. There is no logical reason to call Pluto a planet.” Like a growing number of his colleagues, Brown believes Pluto is best understood as the largest known member of the Kuiper belt, a band of rocky, icy miniplanets that orbit the sun in a swath stretching from beyond Neptune to a distance of nearly 5 billion miles. “I don’t think it denigrates Pluto at all to say that it is not a planet. I think Pluto is a fascinating and interesting world, and being the largest Kuiper belt object is an honorable thing to be.” No longer is Pluto a lonely outpost in an otherwise empty frontier. -
Alactic Observer
alactic Observer G John J. McCarthy Observatory Volume 14, No. 2 February 2021 International Space Station transit of the Moon Composite image: Marc Polansky February Astronomy Calendar and Space Exploration Almanac Bel'kovich (Long 90° E) Hercules (L) and Atlas (R) Posidonius Taurus-Littrow Six-Day-Old Moon mosaic Apollo 17 captured with an antique telescope built by John Benjamin Dancer. Dancer is credited with being the first to photograph the Moon in Tranquility Base England in February 1852 Apollo 11 Apollo 11 and 17 landing sites are visible in the images, as well as Mare Nectaris, one of the older impact basins on Mare Nectaris the Moon Altai Scarp Photos: Bill Cloutier 1 John J. McCarthy Observatory In This Issue Page Out the Window on Your Left ........................................................................3 Valentine Dome ..............................................................................................4 Rocket Trivia ..................................................................................................5 Mars Time (Landing of Perseverance) ...........................................................7 Destination: Jezero Crater ...............................................................................9 Revisiting an Exoplanet Discovery ...............................................................11 Moon Rock in the White House....................................................................13 Solar Beaming Project ..................................................................................14 -
Spitzer to Size up Newly Found Planet
I n s i d e August 12, 2005 Volume 35 Number 16 News Briefs . 2 The story behind ‘JPL Stories’ . 3 Special Events Calendar . 2 Passings . 4 MRO launch postponed . 2 Letters, Classifieds . 4 Jet Propulsion Laborator y However, the object was so far away Spitzer that its motion was not detected until they reanalyzed the data in January of this year. In the last seven months, to size up the scientists have been studying the planet to better estimate its size and newly its motions. “It's definitely bigger than Pluto,” said found Brown, a professor of planetary astrono- my at Caltech. Scientists can infer the size of a solar planet system object by its brightness, just as one can infer the size of a faraway light bulb if one knows its wattage. The re- Artist’s concept of the flectance of the planet is not yet known. planet catalogued as Scientists cannot yet tell how much 2003UB313 at the light from the Sun is reflected away, lonely outer fringes of but the amount of light the planet re- our solar system. Later this month, the Spitzer Space Telescope flects puts a lower limit on its size. “Even if it reflected 100 percent of the light reaching it, it would Our Sun can be seen will look toward the recently discovered planet in the outlying regions of the solar system. The observation will still be as big as Pluto,” says Brown. “I'd say it’s probably one and a in the distance. bring new information on the size of the 10th planet, which lies half times the size of Pluto, but we’re not sure yet of the final size. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
INDEX to VOLUME 26 of the JOURNAL of the ASSOCIATION of LUNAR and PLANETARY OBSERVERS (The Strolling Astronomer) by Michael
INDEX TO VOLUME 26 OF THE JOURNAL OF THE ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS (The Strolling Astronomer) by Michael Mattei PUBLICATION DATA Issue Number 1-2, May, 1976.......Pages 1-40 3-4, August, 1976..... 41-84 5-6, November, 1976... 85-128 7-8, February, 1977... 129-172 9-10, May, 1977........ 173-216 11-12, August, 1977..... 217-260 AUTHOR INDEX Pages Ashbrook, Joseph An Amateur Program: Timing Eclipses of Jovian Satellites 233-235 Benton, Julius L. American and Italian Observations of Saturn in 1974-1975: Some Comparative Notes 166-168 A Simultaneous Observing Program for the Planet Saturn: Some Preliminary Remarks 164-166 Visual and Photographic Observations of Saturn: The 1974-75 Apparition 85-94 The 1975-76 Apparition of Saturn 173-184 The Planet Venus: A Summary of Five Morning Apparitions, 1967 - 1974 150-155 Two Eastern (Evening) Apparitions of the Planet Venus: 1973-74 and 1974-75 100-109 The 1976-77 Eastern (Evening) Apparition of the Planet Venus: Visual and Photographic Investigations 240-251 Budine, Phillip W. Jupiter in 1974-75: Rotation Periods 129-135 Jupiter in 1975-76: Rotation Periods 217-231 Measured Photographic Latitudes on Jupiter in 1975-76 231-233 Observed Latitudes of Jupiter's Belts and Zones in 1974-75 118-119 The A.L.P.O. at Kutztown, Pennsylvania 123-125 Capen, C.F. A Season for Vikings 41-46 Capen, Charles F. and Rhoads, Robert B. Mars 1971 Apparition - Martian Polar Hoods - ALPO Report II 1-8 Sassone-Corsi, Emilio and Sassone- Corsi, Paolo Some Systematic Observations of Saturn During its 1974-75 Apparition 8-12 Delano, Kenneth J. -
The Big Eye Vol 2 No 1
Friends of Palomar Observatory P.O. Box 200 Palomar Mountain, CA 92060-0200 The Big Eye The Newsletter of the Friends of Palomar Observatory Vol. 2, No. 1 Solar System Now Palomar’s Astronomical Has Eight Planets Bandwidth The International Astronomical Union (IAU) recently downgraded the status of Pluto to that of a “dwarf plan- For the past three years, astronomers at the et,” a designation that will also be applied to the spheri- California Institute of Technology’s Palomar Obser- cal body discovered last year by California Institute of vatory in Southern California have been using the Technology planetary scientist Mike Brown and his col- High Performance Wireless Research and Education leagues. The decision means that only the rocky worlds Network (HPWREN) as the data transfer cyberin- of the inner solar system and the gas giants of the outer frastructure to further our understanding of the uni- system will hereafter be designated as planets. verse. Recent applications include the study of some The ruling effectively settles a year-long controversy of the most cataclysmic explosions in the universe, about whether the spherical body announced last year and the hunt for extrasolar planets, and the discovery informally named “Xena” would rise to planetary status. of our solar system’s tenth planet. The data for all Somewhat larger than Pluto, the body has been informally this research is transferred via HPWREN from the known as Xena since the formal announcement of its remote mountain observatory to college campuses discovery on July 29, 2005, by Brown and his co-discov- hundreds of miles away. -
Interview with Harold Zirin
HAROLD ZIRIN (1930-2012) INTERVIEWED BY SHIRLEY K. COHEN February 3, 10 and 17, 1998 Photo taken 1977 ARCHIVES CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California Subject area Astronomy, astrophysics Abstract An interview in three sessions, in February 1998, by Shirley K. Cohen with Harold Zirin, Professor of Astrophysics, emeritus, in the Division of Physics, Math and Astronomy at Caltech. Dr. Zirin received his undergraduate and graduate education at Harvard (AB, 1950; AM, 1951; PhD, 1953). He joined the Caltech faculty in 1964, became Chief Astronomer at the Big Bear Solar Observatory in 1970 and Director in 1980. The interview briefly covers Zirin’s youth and early education in New York City and Bridgeport, Connecticut, and notes his youthful interest in astronomy and success in school. Recalls Harvard astronomers Bart Bok, Harlow Shapley, Armin Deutsch, Donald Menzel. PhD work on stellar opacities under Philip Morse at MIT with Harvard’s approval; leads to first job at RAND Corporation and first move to California, 1952-1953. Denial of security clearance based on father’s membership in Communist party sends him back to Harvard for postdoc position. Move to Colorado to High Altitude Observatory and beginning of solar http://resolver.caltech.edu/CaltechOH:OH_Zirin_H observing; reminiscences of S. Chandrasekhar, G. Munch. Recruitment to Caltech by J. Greenstein, R. Leighton, 1964. Discusses history of solar observing at Mt. Wilson Observatory. Site survey for new Caltech solar observatory; role of astronomer Sue Kiefer; selection of Big Bear Lake site in San Bernardino Mountains (1967). Story of construction and operation of Big Bear Solar Observatory, concluding with its transfer to New Jersey Institute of Technology (1997). -
Geschichte Der Naturwissenschaft, Der Technik Und Der Medizin in Deutschland
German National Committee Geschichte der Naturwissenschaft, der Technik und der Medizin in Deutschland History of Science, Technology and Medicine in Germany 2009-2012 edited by Bettina Wahrig / Julia Saatz Braunschweig 2013 http://www.digibib.tu-bs.de/?docid=00055530 23/01/2014 Zusammengestellt mit Unterstützung der Deutschen Forschungsgemeinschaft (DFG) Dieser Bericht wurde aus Anlass des XXIV. Internationalen Kongresses für Wissenschaftsgeschichte in Manchester mit Unterstützung der Deutschen Forschungsgemeinschaft (DFG) erstellt. Der Bericht erscheint als PDF-File auf CD-ROM oder kann auch von der Homepage des Nationalkomitees der IUHPS/DHS heruntergeladen werden: <http://www-wissenschaftsgeschichte.uni-regensburg.de/NK.htm>. Verwiesen sei auch auf die Online-Datenbank WissTecMed*Lit, mit deren Hilfe die hier veröffentlichte Forschungsbibliographie erstellt wurde. Diese Datenbank zu wissenschafts-, medizin- und technikhistorischer Forschungsliteratur wird weiterhin aktualisiert im Internet zur Verfügung stehen: http://lit.wisstecmed.de/detail.php. Weitere Exemplare der CD-ROM können angefordert werden von b.wahrig[at]tu-braunschweig.de. This brochure was prepared for the XXIV. International Congress of History of Science in Manchester; compilation was supported by the German Research Foundation (DFG). The CD-ROM contains the complete text as a PDF file, which is also available for download from the homepage of the German National Committee <http://www-wissenschaftsgeschichte.uniregensburg.de/NK.htm>. The data have been compiled via the web based catalogue WissTecMed*Lit. This data base of publications on the history of science, technology and medicine shall be continuously updated and can be accessed at http://lit.wisstecmed.de/detail.php. Additional copies of the CD-ROM can be obtained by sending an email to: b.wahrig[at]tu- braunschweig.de. -
More Than a One-Hit Wonder. Falk, Dan Astronomy. Feb2006, Vol. 34 Issue 2, P40-45
More than a one-hit wonder. Falk, Dan Astronomy. Feb2006, Vol. 34 Issue 2, p40-45 Famous for discovering Pluto, Clyde Tombaugh reached far beyond the planets Clyde Tombaugh's life instantly changed when he discovered Pluto in 1930. Just 24 years old, and with only a high-school diploma, Tombaugh spotted the missing "Planet X." Shortly thereafter, he was awarded a scholarship for his scientific work and returned to school to earn bachelor's and master's degrees in astronomy. Now, 100 years after his birth, both amateur and professional astronomers celebrate this astronomy great. The day he discovered Pluto began like any other during the previous few months. Tombaugh had not been able to observe the night before because of the Moon's glare. So on February 18, 1930, he "blinked" two photographic plates from January 23 and 29. He would work for a half hour, then rest his eyes and brain for the same time, and return to blinking. The task required intense concentration. And at about 4 o'clock in the afternoon on a cold, wintry day in Flagstaff, Arizona, he found it. For 45 minutes, he checked his plates and examined another from January 21. Once Tombaugh was 100-percent positive he had found it, he reported the news to his boss. Twenty- five years of astronomers' searching was over. Finding a path Clyde William Tombaugh (1906-1997) was born in Streator, Illinois, and moved to Kansas at the age of 16 when his parents began farming in the small town of Burdett. Tombaugh would have been the quintessential American farm boy were it not for his fascination -- one might say, obsession -- with astronomy. -
1966 Number I
PACIFIC PtrRO!.t U M Gto!.oGls't NIiWS TETTER OF 'tiIE ?ACIIIC SECIIONI AME|TICANI ASSOCIATIONI OT PEIiTOLEU}A GEOLOGIStS Volume 20 Jonuory, 1966 Number I ASSOCIAnON AC'llvl'tlES SA I,A3 II IEATIJRED AT IONG BEACH CONVENIIION pRxsrDElJr ANNoUNCES 1e66 PACIFTC SCTIoN CANDIDATE! As one of the hlghligfrts of the Paclfic Section convention The Nomlnating comittee, under the chai-rmanship of l:E,rcrl ?,+?5 1n i,ong Beach, the A.A.P.G.-S.E.G.-S.E.P.M. Spencer F1ne, has announced the following nomJrtees for Joint luncheon on Thursday, l€,nch ?A, wlll feature a talk 1966-67 offlcers of the Paclfic Sectlon, A.A.P.G.: on the S€a lab II undersea proJect at l.a Jolla, to be presenteal by Scott Carpenter or one of h1s assoclates ln hesi-dent: Andreu ALpha - I\bb1l the recent proJect. The A.A.P.G. Technlcal Sesslons will Robert Knapp - Stantlard stress the thene, iloffshore 0i1.tr The Society of D(plora- tlon ceophysiclsts 1s arzanglng a technical program whlch Vice-Preslitent : John Curuan - Consultant v111 feature digital computlng and processing. Ed Hatl - Unlon secretary: 8111 Ednonalson - Consultant Jin C. Taylor - SheU CATEhIDAR Treasurer: cardner Pittmn - Tialefiater Ton wright - Standard Jamary t7 LOS ANGELES, l8tnday evening, our constitution provldes for ad.dltional candid,ates, as 7:00 P.M., I,lobil Audltoriun, follows: t'. The slate of candidates shall be 612 South Flower Street, announced jn the Paclfic Petroleum Geolog"ist at least one rsllurlan - Lower Devonlan month prior to the electlon. Add.ltlonal nonlnations nay Paleogeography and Ani-ua1 be naale by a wrltten petltlon of twenty-five or more Geography,[ by ]tr.