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Josiah Parsons Cooke Jr.: Epistemology in the Service of Science, Pedagogy, and Natural Theology
Josiah Parsons Cooke Jr.: Epistemology in the Service of Science, Pedagogy, and Natural Theology Stephen M. Contakes and Christopher Kyle Abstract: Josiah Parsons Cooke established chemistry education at Harvard University, initiated an atomic weight research program, and broadly impacted American chemical education through his students, the introduction of labo- ratory instruction, textbooks, and influence on Harvard’s admissions require- ments. The devoutly Unitarian Cooke also articulated and defended a biogeo- chemical natural theology, which he defended by arguing for commonalities between the epistemologies of science and religion. Cooke’s pre-Mendeleev classification scheme for the elements and atomic weight research were moti- vated by his interest in numerical order in nature, which reflected his belief in a divine lawgiver. Keywords: Biography, philosophy of education, epistemology of science, natural theology, chemistry and religion. 1. Introduction Today, Harvard University’s Department of Chemistry and Chemical Biol- ogy is among the finest in the world, counting three Nobel laureates and 17 members of the National Academy of Sciences among its 37 faculty (Jacob- son 2010). Its road to this distinction began inauspiciously in 1850 with the appointment of a 23-year old largely self-taught chemist, Josiah Parsons Cooke, as Erving Professor of Chemistry and Mineralogy. Over the interven- ing 44 years, Cooke’s strenuous and fruitful efforts as a teacher, department builder, researcher, and science popularizer significantly advanced chemistry instruction both at Harvard and throughout the Unites States. His efforts were so successful that after his death Harvard President Charles W. Eliot claimed Cooke “created the Chemical and Mineralogical department of Har- vard University” (Eliot 1895, p. -
Public Events September 2018
Public Events September 2018 Subscribe to this publication by emailing Carol Chen atSubscribe [email protected] to this publication by emailing Shayla Butler at [email protected] Table of Contents Overview Fall Event Highlights ............................................................................................. 3 Northwestern Events Arts and Performances .......................................................................................... 8 Living Neighborhood and Community Relations Leisure and Social ......................................................................................... 10 1603 Orrington Avenue, Suite 1730 Norris Mini Courses Evanston, IL 60201 Around Campus www.northwestern.edu/communityrelations ARTica (art studio) Norris Outdoors Northwestern Music Academy Dave Davis Religious Services ......................................................................................... 13 Executive Director [email protected] Sports, Health, and Wellness 847-491-8434 Northwestern Wildcat Athletics ................................................................... 14 Recreation ..................................................................................................... 18 Academic Lectures To receive this publication electronically One Book, One Northwestern: Danielle Allen, Our Declaration .............. 20 every month, please email Shayla Butler at Academic Lectures ....................................................................................... 21 [email protected] -
Analysis of New High-Precision Transit Light Curves of WASP-10 B: Starspot
Astronomy & Astrophysics manuscript no. wasp10 c ESO 2018 September 10, 2018 Analysis of new high-precision transit light curves of WASP-10 b: starspot occultations, small planetary radius, and high metallicity⋆ G. Maciejewski1,2, St. Raetz2, N.Nettelmann3, M. Seeliger2, Ch. Adam2, G. Nowak1, and R. Neuh¨auser2 1 Toru´nCentre for Astronomy, Nicolaus Copernicus University, Gagarina 11, PL–87100 Toru´n, Poland e-mail: [email protected] 2 Astrophysikalisches Institut und Universit¨ats-Sternwarte, Schillerg¨asschen 2–3, D–07745 Jena, Germany 3 Institut f¨ur Physik, Universit¨at Rostock, D–18051 Rostock, Germany Received ...; accepted ... ABSTRACT Context. The WASP-10 planetary system is intriguing because different values of radius have been reported for its transiting exoplanet. The host star exhibits activity in terms of photometric variability, which is caused by the rotational modulation of the spots. Moreover, a periodic modulation has been discovered in transit timing of WASP-10 b, which could be a sign of an additional body perturbing the orbital motion of the transiting planet. Aims. We attempt to refine the physical parameters of the system, in particular the planetary radius, which is crucial for studying the internal structure of the transiting planet. We also determine new mid-transit times to confirm or refute observed anomalies in transit timing. Methods. We acquired high-precision light curves for four transits of WASP-10 b in 2010. Assuming various limb-darkening laws, we generated best-fit models and redetermined parameters of the system. The prayer-bead method and Monte Carlo simulations were used to derive error estimates. -
A Hot Subdwarf-White Dwarf Super-Chandrasekhar Candidate
A hot subdwarf–white dwarf super-Chandrasekhar candidate supernova Ia progenitor Ingrid Pelisoli1,2*, P. Neunteufel3, S. Geier1, T. Kupfer4,5, U. Heber6, A. Irrgang6, D. Schneider6, A. Bastian1, J. van Roestel7, V. Schaffenroth1, and B. N. Barlow8 1Institut fur¨ Physik und Astronomie, Universitat¨ Potsdam, Haus 28, Karl-Liebknecht-Str. 24/25, D-14476 Potsdam-Golm, Germany 2Department of Physics, University of Warwick, Coventry, CV4 7AL, UK 3Max Planck Institut fur¨ Astrophysik, Karl-Schwarzschild-Straße 1, 85748 Garching bei Munchen¨ 4Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106, USA 5Texas Tech University, Department of Physics & Astronomy, Box 41051, 79409, Lubbock, TX, USA 6Dr. Karl Remeis-Observatory & ECAP, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg (FAU), Sternwartstr. 7, 96049 Bamberg, Germany 7Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA 8Department of Physics and Astronomy, High Point University, High Point, NC 27268, USA *[email protected] ABSTRACT Supernova Ia are bright explosive events that can be used to estimate cosmological distances, allowing us to study the expansion of the Universe. They are understood to result from a thermonuclear detonation in a white dwarf that formed from the exhausted core of a star more massive than the Sun. However, the possible progenitor channels leading to an explosion are a long-standing debate, limiting the precision and accuracy of supernova Ia as distance indicators. Here we present HD 265435, a binary system with an orbital period of less than a hundred minutes, consisting of a white dwarf and a hot subdwarf — a stripped core-helium burning star. -
Duck Island Yacht Club 2017 N 41° 16.6’ W 72° 28.0’
DUCK ISLAND YACHT CLUB 2017 N 41° 16.6’ W 72° 28.0’ Founded 1932 Check out Cindy’s New Location 688 Boston Post Road in Westbrook, CT 860-399-0007 Mon-Thurs 9am-8pm Fri & Sat 9 am-9pm Sun 10am-6pm [email protected] We deliver locally! We offer a wide variety of wines from around the world. Our coolers host a range of beer, ale, lager, IPA, ciders, including brands brewed here in CT! If we don’t have what you want- we can order it and have it to you in two days! We also make gift baskets to order. Join us Friday evenings from 6-8 pm for wine and beer tastings! Bob Connell – Manager – North Yard Tel: 860 399-5128 Fax: 860 399-8720 Email: [email protected] 2. Connecticut Yacht Rigging Connecticut Yacht Rigging is dedicated to bringing you the highest quality rigging work with unsurpassed customer support. We have over 30 years of experience in marine, architectural and custom rig- ging. Additionally, we are Navtec factory trained in hydraulic installation and repair. Our exceptional attention to detail guar- antees your project is fulfilled accurately and on schedule. Connecticut Yacht Rigging provides a wide Contact Us Today: range of yacht rigging services including: Dan Coan, owner 860-575-6985 • Inspections & Insurance Claims [email protected] • Offshore Preparation • Mainsail Handling & Furling Systems • Jib Furling Systems • Downwind Gear • Standing & Running Rigging • Anchoring Systems • Hydraulic Systems • Bowsprits • Mast Refurbishing • Deck Hardware • Custom Hardware, Mast Collars & Radar Brackets • Radar Mast and Arch Installation • Hydraulic installation and repair 3. -
Inclination Evolution of Protoplanetary Disks Around Eccentric Binaries
Mon. Not. R. Astron. Soc. 000, 000{000 (0000) Printed 11 October 2017 (MN LATEX style file v2.2) Inclination Evolution of Protoplanetary Disks Around Eccentric Binaries J. J. Zanazzi1?, and Dong Lai1 1Cornell Center for Astrophysics, Planetary Science, Department of Astronomy, Cornell University, Ithaca, NY 14853, USA 11 October 2017 ABSTRACT It is usually thought that viscous torque works to align a circumbinary disk with the binary's orbital plane. However, recent numerical simulations suggest that the disk may evolve to a configuration perpendicular to the binary orbit (\polar alignment") if the binary is eccentric and the initial disk-binary inclination is sufficiently large. We carry out a theoretical study on the long-term evolution of inclined disks around eccentric binaries, calculating the disk warp profile and dissipative torque acting on the disk. For disks with aspect ratio H=r larger than the viscosity parameter α, bend- ing wave propagation effectively makes the disk precess as a quasi-rigid body, while viscosity acts on the disk warp and twist to drive secular evolution of the disk-binary inclination. We derive a simple analytic criterion (in terms of the binary eccentricity and initial disk orientation) for the disk to evolve toward polar alignment with the eccentric binary. When the disk has a non-negligible angular momentum compared to the binary, the final \polar alignment" inclination angle is reduced from 90◦. For typical protoplanetary disk parameters, the timescale of the inclination evolution is shorter than the disk lifetime, suggesting that highly-inclined disks and planets may exist orbiting eccentric binaries. Key words: Physical data and processes: accretion, accretion discs; Physical data and processes: hydrodynamics; stars: binaries: general; protoplanetary discs. -
Proceedings of the American Academy of Arts and Sciences
1 • I / i PROCEEDINGS AMERICAN ACADEMY ARTS AND SCIENCES. NEW SERIES. Vol. IX. WHOLE SERIES. Vol. XVII. FROM JUNE, 1881, TO JUNE, 1882. SELECTED FROM THE RECORDS. BOSTON: UNIVERSITY PRESS: JOHN WILSON AND SON. 1882. X fi^ CONTENTS. PAQE I. Contributions from the Chemical Laboratory of Harvard College. By Josiah Parsons Cooke 1 II. On the Spectrum of Arsenic. By Oliver W. Huntington 35 III. Thermoelectricity. — Peltier and Thomson Effects. By Charles Bingham Penrose 39 IV. Thermoelectric Line of Copper and Nickel below 0°. By Charles Bingham Penrose 47 V. Crystalline Form of Cryolite. By W. H. Melville ... 55 VI. Researches on the Complex Inorganic Acids. Phospho-molyb- dates. By Wolcott Gibbs, M.D . 62 VII. An Indirect Determination of Chlorine and Bromine by Elec- trolysis. By' Leonard P. Kixnicutt 91 VIII. Contributions from the Chemical Laboratory of Harvard Col- lege. By Charles F. Mabery 94 "^ IX. On Certain Substances obtainedfrom Turmeric. — I. Curcumin. By C. Loring Jackson and A. E. Menke 110 X. Contributions from the Chemical Laboratory of Harvard Col- lege. By Henry B. Hill 125 XI. XV. — Simple Method for Calibrating T'hermometers. By Silas W. Holman 157 XII. Contributions to North American Botany. By Asa Gray . 163 XIII. The Wedge Photometer. By Edward C. Pickering . 231 XIV. On the Color and the Pattern of Insects. By Dr. II. A. Hagen 234 IV CONTENTS. PAGE XV. On Telephoning over long Distances or through Cables. By N. D. C. Hodges 268 XVI. On the Young Stages of some Osseous Fishes. With Plates. By Alexander Agassiz 271 XVII. XVI. -
12-Inch Alvan Clark Telescope Restoration
12-Inch Alvan Clark Telescope Restoration: Summary of Research and Final Recommendations Deborah Culmer and Hannah Johnson September, 2011 Introduction The first telescope installed at Lick Observatory was a second-hand purchase, with the telescope and its optic made by the premier telescope makers of the time, Alvan Clark and Sons of Cambridge, MA. The dome that housed it was the first structure built on Mt. Hamilton, from bricks fired in a kiln on location. That dome still stands; and until the 1970’s, the 12-inch refracting telescope was in operation, but without its original driver clock and gears (replaced with an electronic drive, perhaps in the 1950’s). Since it was decommissioned, the 12-inch has been in storage. The Lick Instrument Lab has retrieved it, and it is currently on location at UC Santa Cruz in anticipation of total restoration. In the summer of 2011, a research project was launched to determine to what era and condition the telescope should be restored. In recent years, there has been great interest in historical restoration of Alvan Clark telescopes (and others, to be sure). As a result of that interest, we had a pool of organizations and institutions from which to glean information. Two we visited in person; many more we contacted via email and conference calls. Based on our research and interviews, we offer our recommendations on the restoration of this historically important telescope. 1. Research In beginning this project, it was very important to understand the history of the 12-inch Alvan Clark, especially since it was the first telescope set up on Mt. -
Planets Transiting Non-Eclipsing Binaries
A&A 570, A91 (2014) Astronomy DOI: 10.1051/0004-6361/201323112 & c ESO 2014 Astrophysics Planets transiting non-eclipsing binaries David V. Martin1 and Amaury H. M. J. Triaud2;? 1 Observatoire Astronomique de l’Université de Genève, Chemin des Maillettes 51, CH-1290 Sauverny, Switzerland e-mail: [email protected] 2 Kavli Institute for Astrophysics & Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA Received 22 November 2013 / Accepted 28 August 2014 ABSTRACT The majority of binary stars do not eclipse. Current searches for transiting circumbinary planets concentrate on eclipsing binaries, and are therefore restricted to a small fraction of potential hosts. We investigate the concept of finding planets transiting non-eclipsing binaries, whose geometry would require mutually inclined planes. Using an N-body code we explore how the number and sequence of transits vary as functions of observing time and orbital parameters. The concept is then generalised thanks to a suite of simulated circumbinary systems. Binaries are constructed from radial-velocity surveys of the solar neighbourhood. They are then populated with orbiting gas giants, drawn from a range of distributions. The binary population is shown to be compatible with the Kepler eclipsing binary catalogue, indicating that the properties of binaries may be as universal as the initial mass function. These synthetic systems produce transiting circumbinary planets occurring on both eclipsing and non-eclipsing binaries. Simulated planets transiting eclipsing binaries are compared with published Kepler detections. We find 1) that planets transiting non-eclipsing binaries are probably present in the Kepler data; 2) that observational biases alone cannot account for the observed over-density of circumbinary planets near the stability limit, which implies a physical pile-up; and 3) that the distributions of gas giants orbiting single and binary stars are likely different. -
Solar Observatory
SOLAR OBSERVATORY Fig. 1. The Watson Solar Observatory c. 1920. Below the building was a twenty foot deep cellar, and a 55 foot horizontal shaft through the hill to a reflector at the surface on the north side. This building was erected by Professor James C. Watson using his own money and labor. Because of the stone reading "Watson Solar Observatory", the building became known as the Watson Mystery House. [series 9/1 Solar Obser- vatory folder, jf-4] The Solar Observatory was built by astronomer James Watson, with his own funds and labor for the purpose of looking for a hypothetical planet near the sun. The experiment did not reveal the planet, and the building was used for storage until its demolition in 1949. hen C. C. Washburn agreed to build an observatory for the University in 1876, the legisla- ture appropriated $3000 per year to fund the staffing and operation of the observatory. The Wperson hired for this job by President Bascom was James Craig Watson, the director of the observatory at Ann Arbor, Michigan. Watson had been a prodigy in astronomy, and was published at 19. His major professor Brunnow, when reproached for the small size of his teaching load exclaimed, "Yes I have only one student, but that one is Watson!"1 Watson became director of Michigan's obser- vatory at age 25 in 1863. Within a year he had discovered the first of what are called Watson's family of asteroids. In July of 1878 Watson went to Separation, Wyoming to observe a solar eclipse. -
The Concordiensis, Volume 1, Number 3
THE CONCORDIENSIS. VoL. I. ScHENECTADY, N. Y., January, 1878. No.3· UNION UNIVERSITY. REV. E. N. POTTER, D. D., PRESIDENT. UNION COLLEGE, DEPARTMENT OF MEDICINE. ALBANY MEDICAl: CoLLEGE.-Term commences First Tuesday in SCHENECTADY, N. Y. September and contmues twenty weeks. The plan of instruction combines clinical teaching, With lectures. Special opportunities for -0- the study of chemistry and of practical anatomy. ExPE!\s:Es.-Matriculation fee, $s. Term fee, $IOo. Perpetual the I. CLASSICAL CouRsE.-The Classical Course is the usual bacca Ticket, $rso. Graduation fee, $25. Dissecting fee, $s. Fee for labora laureate course of American colleges. Students may be permitted to tory course, $ro. Histological course, $ro. For Circulars, address, ding pursue additional studies in either of the other courses. PROF. JACOBs. MOS~ER, M.D., REGISTRAR, . z. .SciENTIFIC CouRSE.-ln the Scientific Course the modern lan Albany, N. Y. guages are substituted for the ancient, and the amount .of mathematical DEPARTMENT OF LAW. and English studies is increased. 3· SCHOOL OF CIVIL ENGINEERING.-The student in this depart THE ALEANY LAw ScHOOL.-The Course of Instruction consists of T, ment enjoys advantages nowhere surpassed, in the course of instruc three terms: the fin;t commencing September 4th, the Second N ovem tion, in its collectiOn of ·models, instruments and books, the ber 27th, and the third i\iarch sth; each term consisting of twelve 'endent. accumulations of many years by the late Professor Gillespie, and also weeks. The advantages for the study ot the l~w, at Albany, are as in unusal facilities for acquiring a practical knowledge of instrumental great as can be found anywhere. -
Women Who Read the Stars Sue Nelson Delights in Dava Sobel’S Account of a Rare Band of Human Computers
Some of the Harvard Observatory ‘computers’ in 1925. Annie Jump Cannon is seated fifth from left; Cecilia Payne is at the drafting table. HISTORY Women who read the stars Sue Nelson delights in Dava Sobel’s account of a rare band of human computers. here are half a million photographic magnitude, on the as computers at Harvard, a practice unique plates in the Harvard College Observa- photographic plates to the university. Within five years, the num- tory collection, all unique. They date to and computing its ber of paid female computers, from a range Tthe mid-1880s, and each can display the light location in the sky. of backgrounds, had risen to 14. Their efforts from 50,000 stars. These fragments of the Pickering was espe- would be boosted by philanthropist Cath- cosmos furthered our understanding of the cially interested in erine Wolfe Bruce, who in 1889 donated Universe. They also reflect the dedication and variable stars, whose US$50,000 to the observatory, convinced intelligence of extraordinary women whose light would brighten that the introduction of photography and stories are more than astronomical history: and fade over a spe- spectroscopy would advance the field. ARCHIVES UNIV. HARVARD COURTESY they reveal lives of ambition, aspiration and cific period. These The Glass The Glass Universe concentrates on a few of brilliance. It takes a talented writer to inter- fluctuations, captured Universe: How the Harvard computers. Williamina Fleming, weave professional achievement with per- on the plates, required the Ladies of a Scottish school teacher, arrived at the obser- sonal insight. By the time I finished The Glass constant observation, the Harvard vatory in 1879, pregnant and abandoned by Universe, Dava Sobel’s wonderful, meticulous but he couldn’t afford Observatory Took her husband.