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Archive for October, 2007

Dropping The Drop Boxes: Current “Best Set” Keywords For Solid-State Terahertz DMol3 Calculations

Tuesday, October 30th, 2007

Of the few discussions I’ve had with fellow theoreticians, the general consensus is that employing drop boxes for defining parameters in quantum chemistry programs is methodologically akin to using solvents and starting materials as purchased from a chemical company “as is.” Certainly good enough to get something decent to happen because, of course, the companies providing the product need to stay in business, but certainly not ideal and, by their removal of the background steps and understanding of the generation methods, somehow lacking, neglecting the efforts of researchers “behind the scenes” that made the (pardon) gross simplification of “hitting the dirt running” possible.

The subject of this post is the Materials Studio (graphical interface) implementation of DMol3 (DOS/shell) and the settings available via the MS interface (coarse, medium, fine in many cases, with the actual values associated with these general settings varying slightly with the properties of the crystal cell). Are the standard options available for setting job parameters good enough to get a workable result out? In the case of “fine”, yes, with very few instances noted here of calculations behaving badly. Can one do better? Definitely. For terahertz spectroscopy studies alone, the parameter options provided by the Materials Studio interface are good enough to get something out to aid in assignments, and certainly good enough to convince anyone that ISOLATED-MOLECULE CALCULATIONS ARE ENTIRELY INAPPROPRIATE TO USE FOR THE ASSIGNMENT OF SOLID-STATE TERAHERTZ SPECTRA. At this point in the game, however, I would not consider them rigorously publication-quality results (I would not argue if agreement was good and the spectra clean, but I would certainly check the level of theory carefully), given that agreement can be improved and a better overall assignment achieved by tweaking the keyword list.

It is with that in mind (and Matt Hudson’s reminder) that I’m posting a keyword set that, over the course of a few hundred DMol3 calculations or so, has been found to provide a decent balance of time (longer than the menu options but only by %15 – %20 or so) and interpretive power (or predictive power if no one’s taken the Terahertz spectrum). Note that the “#” is the “comment/ignore” character, so much of the content below is ignored by DMol3.

####################################################################
#
# Input cheat-sheet for THz DMol3 solid-state calculations
# Quests, comms, complaints, Damian Allis, damian@somewhereville.com
#
# Definitely works with DMol3 version 3.2
#
####################################################################
###   Optimization Properties   ####################################
####################################################################
Calculate                    optimize
###   Optimize the structure
###
Opt_energy_convergence       5.0000e-007
###   Energy convergence (dE step to finish)
###
Opt_gradient_convergence     1.0000e-004 A
###   Conv when largest grad vector comp < this
###
Opt_displacement_convergence 1.0000e-004 A
###   Conv when largest atom disp < this
###
Opt_iterations               100
###   Steps to opt (large value for tight conv)
###
Opt_max_displacement         0.3000 A
###   Max length geom update vector
###
####################################################################
###   Electronic Structure Descriptions   ##########################
####################################################################
Spin_polarization            restricted
###   un/restricted wavefunction description
###
Charge                       0
###   System charge
###
###   Basis set approx's are not direct comparisons
Basis                        dnp
###   Basis     dnp    Gaussian approx 6-31G(d,p) basis set
###   Basis     dnd    Gaussian approx 6-31G(d) basis set
###   Basis     dn     Gaussian approx 6-31G basis set
###   Basis     min    Gaussian approx 3-21G basis set
###
Pseudopotential              none
###   Consider for transition metal systems
###
###   GGA Functionals - Gen Grad Approx: density and gradient
Functional                   bp
###   So far, bp is the best all-around THz freq functional
###   Functional                 blyp            ###
###   Functional                 bop             ###
###   Functional                 gga(p91)        ###
###   Functional                 hcth407         ###
###   Functional                 vwn-bp
###   So far, vwn-bp is the 2nd best THz freq functional
###   Functional                 rpbe            ###
###   Functional                 pbe             ###
###
###   LDA Functionals - Local Den Approx: density at position
###   Functional                 pwc             ###
###   Functional                 vwn             ###
###
####################################################################
###   Additional Electronic Structure Parameters   #################
####################################################################
###
###   Integration_grid - mesh points for numerical integr procedure
###                    value       ipa iomax iomin thres   rmaxp sp
###   Integration_grid xcoarse ###  6    3     1   0.01     10.0 1.0
###   Integration_grid coarse  ###  6    4     1   0.001    10.0 1.0
###   Integration_grid medium  ###  6    6     1   0.0001   10.0 1.0
Integration_grid   fine        ###  6    6     1   0.00001  12.0 1.2
###   Integration_grid xfine   ###  6    7     1   0.000001 15.0 1.5
###
Aux_density                  octupole
###   Max ang momentum multipolar fit funcs
###
Occupation                   fermi
###   Converger aid.  See manual for more
###
Cutoff_Global                4.0000 angstrom
###   Atom-centered basis set cut-off distance
###
Scf_density_convergence      1.0000e-008
###   Conv when density conv < this
###
Scf_charge_mixing            0.2000
###   Init charge density mix coeff restrict
###
Scf_iterations               100
###   Max iters for SCF (large b/c conv’rs)
###
Scf_diis                     6 pulay
###   Max size of DIIS subspace for SCF calc
###
###   Kpoint -> defined for each a,b,c lattice vector
###   General protocol (appropr of selections is theological):
###   If a,b,c    < 5        set kpoint to 5
###   If a,b,c  5 < X < 10   set kpoint to 4
###   If a,b,c 10 < X < 15   set kpoint to 3
###   If a,b,c 15 < X < 20   set kpoint to 2
###   If a,b,c    < 20       set kpoint to 1
###                                     a b c
Kpoints                      on     5 5 5
###   Max set here.  Adjust as approp
###
###   Print options
Print                        vib_hess
###   amount of printout.  Read manual.
###
####################################################################
###   Terahertz Vibrational Analysis   #############################
####################################################################
###
Symmetry                     on
###   Recalc symm after opt for use in freq
###
Mulliken_analysis            charge
###   Mulliken charges.  MS 4.2 broke this (!)
###
Hirshfeld_analysis           charge
###   Hirshfeld charges.
###
Frequency_analysis           on
###   Perform normal mode analysis
### 

Either copy+paste the above, or download DMol3_THz_complete.input.

For those a bit overcome by what Frank Zappa would refer to as the “statistical density” of the content above, the whole file reduces down to the following (the selection of Kpoints being the only keyword one has to think about below).

Calculate                    optimize
Opt_energy_convergence       5.0000e-007
Opt_gradient_convergence     1.0000e-004 A
Opt_displacement_convergence 1.0000e-004 A
Opt_iterations               100
Opt_max_displacement         0.3000 A
Spin_polarization            restricted
Charge                       0
Basis                        dnp
Functional                   bp
Integration_grid             fine
Aux_density                  octupole
Occupation                   fermi
Cutoff_Global                4.0000 angstrom
Scf_density_convergence      1.0000e-008
Scf_charge_mixing            0.2000
Scf_iterations               100
Scf_diis                     6 pulay
Kpoints                      on     5 5 5
Print                        vib_hess
Symmetry                     on
Mulliken_analysis            charge
Hirshfeld_analysis           charge
Frequency_analysis           on

Either copy+paste the above, or download DMol3_THz_min.input.

Yes, I am aware that I am recommending the replacement of one “standard” set of keywords (Accelrys) with another “standard” set (mine). Further, it must be noted that these above keywords are very much terahertz-specific, where the lowest-energy, largest-amplitude, most neighboring molecule-dependent solid-state properties are considered. This is NOT the “be all, end all” keyword set for every system (certainly not even for general inelastic neutron scattering spectroscopy use, where the agreement between theory and experiment is very dependent on the choice of density functional (blyp and bop seem to be the best in the 500 to 1500 cm-1 region, by the way)). And, far from trying to use this post to complain about theory, program, and parameters, I note that DMol3 has been the mainstay of my solid-state terahertz theoretical work to date and I’ve spoken quite favorably of it in the past. Any program with keywords and input parameters should be expected to have optimal settings for different tasks, a point in no way lost on researchers familiar with the variety of empirically-derived functionals in density functional theory. We don’t refer to the computational chemistry implementations of quantum theory as the “approximate methods” for nothing.

Since it is just a text file, settings above may undergo further refinement at a more rapid pace than a commercial interface. That said, if your goal is reasonable terahertz simulation with as standard a set of keywords as possible, the set above will (so far, anyway) bring you quite close to your destination.

It is probably far less interesting to list my explanations for each choice (like the Kpoints settings, functional choice, the super-tight convergence criteria) than reading any comments you (the reader) might make, so I invite/encourage questions in the comment section that will keep record of choices, my reasons, and the logic of others.

en.wikipedia.org/wiki/Quantum_chemistry
www.accelrys.com/products/mstudio
www.accelrys.com/products/mstudio/modeling/quantumandcatalysis/dmol3.html
en.wikipedia.org/wiki/Time_domain_terahertz_spectroscopy
en.wikipedia.org/wiki/Frank_Zappa
www.zappa.com
en.wikipedia.org/wiki/The_Black_Page
www.accelrys.com
en.wikipedia.org/wiki/Inelastic_neutron_scattering
www.accelrys.com/reference/cases/studies/korter.pdf
en.wikipedia.org/wiki/Density_functional_theory

Molybdophosphonate Clusters As Building Blocks In The Oxomolybdate-Organodiphosphonate/Cobalt(II)-Organoimine System: Structural Influences Of Secondary Metal Coordination Preferences And Diphosphonate Tether Lengths

Friday, October 26th, 2007

In press, in the journal Inorganic Chemistry. This work includes a first attempt at an oxomolybdate crystal cell optimization using periodic boundary conditions (the same types of calculations I do for vibrational spectroscopy studies). Optimization issues related to the treatment of the high-spin cobalt atoms in DMol3 (a problem still being examined here) kept the unit cells from converging to structures with the coordination sphere of the cobalt found in the crystal cell, leaving the majority of the computational study to focus on the isolated-molecule analysis of the {Mo5O15(O3PCH3)2}4- cluster, the goal being an understanding of preferred binding modes to the oxomolybdate cluster by organic and organometallic groups (it seems to be based in sterics, not electronic structure). An interested in-progress result of the solid-state studies involved the calculation of hydrogen-bonding interactions within the crystal cell and their predicted importance in directing MoO4 orientations relative to the isolated oxometal cluster, a result found by performing an optimization on a “first guess” hydrogen position set (from one set of nearest-neighbor oxygen atom distances, Cell #1) followed by a re-optimization at “second guess” hydrogen positions that better preserve the crystal cell symmetry (Cell #2). The utility of deuteration and neutron diffraction studies are not lost on solid-state quantum chemists working with X-ray crystallographers.

inorg chem h box

N. Gabriel Armatasa, Damian G. Allisa, Andrew Prosvirinb, Gabriel Carnutuc, Charles J. O’Connorc, Kim Dunbarb, and Jon Zubietaa,*

a. Department of Chemistry, Syracuse University, Syracuse, NY 13244
b. Department of Chemistry, Texas A&M University, College Station, TX 77843
c. Department of Chemistry, University of New Orleans, New Orleans, LA 70148

Abstract: Hydrothermal conditions have been exploited in the preparation of a series of organic-inorganic hybrid materials of the cobalt-molybdophosphonate family. The reactions of MoO3, cobalt(II) acetate or cobalt(II) acetylacetonate, tetra-2-pyridyl pyrazine (tpyprz) and organodiphosphonic acids H2O3P(CH2)nPO3H2 (n = 1-5 and 9) of varying tether lengths yielded compounds of the general type {Co2(tpyprz)(H2O)m}4+/MoxOy{O3P(CH2)nPO3}z. The recurring theme of the structural chemistry is the entrainment of {Mo5O15(O3PR)2}4- clusters as molecular building blocks observed in the structures of nine phases (compounds 2-9 and 11). As noted previously, minor variations in reaction conditions can have profound influence on the structures of these bimetallic molybdophosphonates. Thus, for the propylene diphosphonate ligand, four unique structures 4-7 are observed, including two distinct three-dimensional architectures for compounds 5 and 6 whose formulations differ only in the number of water molecules of crystallization. It is noteworthy that with pentyldiphosphonate, a second phase 10 is obtained which exhibits a unique cluster building block, the hexamolybdate [Mo6O18{O3P(CH2)5PO3}]4-. In the case of methylenediphosphonic acid, the lack of spatial extension of the ligand precludes tethering of adjacent molybdate clusters and the formation of the common penta-molybdophosphonate building block. Consequently, a third structural motif, the trinuclear {(Mo3O8)(O3PCH2PO3)}2- subunit, is observed in compound 1. Trinuclear subunits have been described previously for the corresponding methylenediphosphonate phases of the copper-molybdophosphonate and nickel-molybdophosphonate families.

The cobalt series of compounds shares with the nickel phases a tendency toward catenation of the M(II)-tpyprz subunits, as manifested in compounds 2 and 7. However, the structural chemistry of compounds 1-11 of this study is quite distinct from that of the {Ni2(tpyprz)(H2O)m}4+/MoxOy{O3P(CH2)nPO3}z family, as well as that of the copper based family. The structural diversity of this general class of materials reflects the coordination preferences of the M(II) sites, the extent of aqua ligation to the M(II) sites, the participation of both phosphate oxygen atoms and molybdate oxo-groups in linking to the M(II) sites, and the variability in the number of attachment sites at the molybdophosphonate clusters. Since the charge densities at the peripheral oxygen atoms of the clusters are quite uniform, the attachment of {M2(tpyprz)}4+ subunits to the molybdophosphonates appears to be largely determined by steric, coulombic and packing factors.

Substitution of 2,2′-bipyridine, o-phenanthroline or terpyridine for the binucleating tpyprz ligand results in the one-dimensional structures of 12-14. Compounds 12 and 13 are unusual examples of “undecorated” molybdophosphonate chains, containing protonated variants of the pentamolybdate cluster.

pubs.acs.org/journals/inocaj/index.html
en.wikipedia.org/wiki/Periodic_boundary_conditions
www.accelrys.com/products/mstudio/modeling/quantumandcatalysis/dmol3.html
en.wikipedia.org/wiki/Neutron_diffraction
www.chem.tamu.edu/rgroup/dunbar/CurrentGroup/Group/andrew.htm
www.chem.uno.edu/ChemistryDepartmentfolder/OConnor.html
www.chem.tamu.edu/rgroup/dunbar
hemistry.syr.edu/faculty/zubieta.html
chemistry.syr.edu
www.syr.edu
www.chem.tamu.edu
www.tamu.edu
www.chem.uno.edu
www.uno.edu

Image Gallery Features At New Nano Site, www.nanohedron.com

Tuesday, October 23rd, 2007

In the midst of a blog marathon…

Peter Kutchukian, a current graduate student in the Department of Chemistry and Chemical Biology at Harvard, has started a new nanotechnology-related art/gallery site, www.nanohedron.com. As part of his first content round, which include a number of experimental, computational (myself included), and purely artistic nanoscale images, Peter requested a few from my gallery, which I was delighted to submit to his site. Included are the bearing assembly (below) and the ever-popular fused diamondoid single-walled carbon nanotube van der Waals crimp junction.

bearing assembly

His interest in some of the carbon nanotube/dative bond designs in the gallery also motivated me to finally repost the slides from my first nanotech talk, The Design of Carbon Nanotube-Based Dative Structures from Supramolecular Principles, at the Foresight Nanotech Institute 10th Conference on Molecular Nanotechnology from way back in 2002.

dative bond talk

www-shakh.harvard.edu/people/kutchukian.html
www.chem.harvard.edu
www.harvard.edu
www.nanohedron.com
www.somewhereville.com/?p=89
www.somewhereville.com/?page_id=10
www.somewhereville.com//?page_id=92
www.foresight.org
www.foresight.org/conference/MNT10/index.html

Syracuse Astronomical Society President’s Message for October, 2007

Tuesday, October 23rd, 2007

A repost of the original at the Syracuse Astronomical Society website.

The SAS board is, once again, very happy to be having our non-observing society meetings for the next few months at the MOST, joining the other attendees for the second year of their Space Science Series.

The MOST lectures and our usual Friday/Saturday viewing schedules no longer coincide, a problem that may disappear in shorter order as winter (if we have one) sets in and we close the observatory for the season. As always, keep track of the “Who’s Observing” page to see if anyone plans on going to Darling Hill.

MOST Space Science Series 2.0

From the official release:

“The four-part 2007-2008 meritorious science speaker series at the Milton J. Rubenstein Museum of Science & Technology (MOST), 500 South Franklin St. in Syracuse’s historic Armory Square, will highlight Space Science. Our invited audience is citizens of Central New York with an interest in space – no experience with intergalactic space travel is necessary. It is our expectation to take you out there! Middle and high school students and their parents are also welcome.

The New York State NASA Space Grant at Cornell University, with support from the MOST, is pleased to offer the Central New York community this opportunity to explore and learn about our immediate neighbors to the most distant space matter.”

2008 International Observer’s Handbook

Click on the image for more information.

Until someone runs a cable line to the Observatory or we eventually get a decent cell phone signal for surfing the web at all hours of the night, reference books are de rigueur for any serious observing activity. With that in mind, Mike Brady sent off the following message announcing the release of the 2008 International Observer’s Handbook from the Royal Astronomical Society of Canada.

“A reminder that our friends to the north have just published their newest reference book, the 2008 International Observer’s Handbook, which is now available at

www.rasc.ca/publications/index.shtml

This is the Royal Astronomical Society of Canada’s 100th year of publication. FYI, I’ve never seen more facts packed into a small sized reference work!”

Ant: Light Pollution

Prof. John McMahon sent off the youtube video embedded below as a fun little discussion about a very unfunny subject to amateur astronomers. The subject of light pollution has received recent attention both on the state political level (with the SAS and myself endorsing A7438/S4364) and, recently, an interesting New Yorker article noted in last month’s message. The video below is intended to, dare I say, shed a little light on the topic.

Anatomy Of A Black Hole

The following demo came across digg.com last week (always a great place for notable space news as well). On the timescale of the Net, a demo still available from 2003 is nothing short of still having a pharaoh around to answer your Egyptology questions. Educational and animated, a tough pair to beat.

www.thinktechnologies.com/portfolio/demos/Blackhole.html

The First Photo From Space



From airspacemag.com. Click HERE for more information.

We’ve become accustomed to finding our cars on Google Earth, seeing “yet again” the most distance astronomical object ever photographed, and even real-time web streams from the ISS. As for the state-of-the-art just 61 years ago, check out the article from Air and Space Magazine from Oct/Nov 2006 (yes, a little late, but will make sense in a moment). Better still, the movie taken by strapping a video camera to a V-2 Rocket in New Mexico, also at airspacemag.com.

And, for a little before-and-after…

HiRISE Photo Gallery

From HiRISE. Click HERE for more information.

…or “How I spent my summer vacation and the government spent my tax dollars.” The HiRISE (High Resolution Imaging Science Experiment) site has put together a first gallery of color images taken as part of the planning stage for the Mars Science Laboratory. The technological progress is, to say the least, stunning, having started with grainy black-and-white just 65 miles above our own planet to now freely available color images taken high above in Martian orbit. You will note, for each, that many of these full-color images are available not in the kilobyte range but in the megabyte and, for the full versions, gigabyte regime, absolutely mammoth file sizes with stunning detail (stunning for now, anyway, until the NEXT camera settles into orbit).

“Cassini’s new view of land of lakes and seas”

From The European Space Agency. Click HERE for more information.

Somewhere between the two extremes above lies the European Space Agency North Pole radar mosaic image from Cassini’s visit to Titan, complete with fairly detailed views of the hydrocarbon lakes that made for numerous press releases when the Huygens probe fell through the Titan atmosphere and onto its surface way back in January 2005.

Space is the place,
Damian Allis, Ph.D.
sas@somewhereville.com

Links Used Above (Subject To Web Changes)

www.syracuse-astro.org
www.astro.cornell.edu/people/facstaff-detail.php?pers_id=104
www.cornell.edu
www.most.org
www.most.org/2_ee_calendar.cfm
www.syracuse-astro.org/phpBB2/viewforum.php?f=2
www.syracuse-astro.org/observatory.html
www.rasc.ca/handbook
www.rasc.ca
www.rasc.ca/publications/index.shtml
webserver.lemoyne.edu/~mcmahon/mcmahon.html
www.youtube.com
www.youtube.com/watch?v=skKpivApW7E
www.somewhereville.com/?p=83
www.selene-ny.org/bill.asp
www.newyorker.com
www.newyorker.com/reporting/2007/08/20/070820fa_fact_owen
www.syracuse-astro.org/index_september2007.html
www.digg.com
www.digg.com/space
www.thinktechnologies.com/portfolio/demos/Blackhole.html
earth.google.com
www.nasa.gov/mission_pages/station/main/index.html
www.airspacemag.com/issues/2006/october-november/FEATURE-FirstPhoto.php
www.airspacemag.com
www.airspacemag.com/multimedia/video/V2%20Photography%20of%20Earth.php
en.wikipedia.org/wiki/V-2_rocket
hirise.lpl.arizona.edu
hirise.lpl.arizona.edu/msl_color_oct_07.php
mars.jpl.nasa.gov/msl
www.esa.int
www.esa.int/esaCP/SEMZ262PL7F_index_0.html
saturn.jpl.nasa.gov/home/index.cfm
en.wikipedia.org/wiki/Titan
en.wikipedia.org/wiki/Hydrocarbon
en.wikipedia.org/wiki/Cassini-Huygens

Syracuse Astronomical Society President’s Message for September, 2007

Tuesday, October 23rd, 2007

A late, and brief, post just after the 2007 Summer Seminar.

SAS Summer Seminar Note

The 2007 Summer Seminar started rough Friday evening (starting so-so and eventually clouding into an official no-no for Perseid Meteor Shower viewing) but turned into a wonderful, well-attended Saturday night. A number of the “usual suspects” engaged in the daytime festivities, which included my own reasonable (after many false starts) assembly of solar filters for my 25×100 binoculars (and, after all that work, only ONE Sun spot). I will say that having proper equipment for daytime and nighttime viewing certainly does extend the usable hours of the day for doing astronomy and, let’s face it, if you had to start by being able to find one star in the sky, it might as well be the Sun. Prof. Gianfranco Vidali from the Syracuse University Physics Department served the doubly duty of presiding over the always chaotic prize raffle and providing a most wonderful presentation on the nature and chemistry of interstellar space (aspects of which are available on his website, physics.syr.edu/faculty/vidali.html). The sky Saturday night was near-flawless for viewing, with the Perseid show constantly turning too many necks ever-too late for catching the night’s brightest streaks. Those of us content with stationary viewing through our scopes were also treated to the night’s clear sky (and, perhaps, a bit too much dew).

A Nice Surprise from Oceanside Photo and Telescope

Oceanside Photo and Telescope (OPT for short) not only provided us the crown jewel of our prize raffle (for which the SAS Board and I are exceedingly grateful) but also sent us off our official SAS Rewards Card, which provides you, the SAS member (you mean you’re not?!) our society-wide discount on purchases through OPT. The discount works by phone and online (even in person if you’re around). All you need to do is let myself or any board member know so we can get you the club number (provided your membership is in good standing), after which OPT will provide you your own. For any questions, feel free to contact me or OPT (internetsales@optcorp.com, 1-800-483-6287).

Cafe Scientifique

Not only can you see Nature in action up at the Darling Hill Observatory, you can also hear all about it through the monthly meetings of Cafe Scientifique, “a place where scientists and scientifically interested non-scientists can come together informally to hear about interesting science, old and new, and discuss its implications in a friendly, cordial way, over drinks and snacks.” Now entering its third year (and now at the Ohm Lounge, in case anyone missed the location change from Ambrosia), the school-year meetings (September to May, first Tuesday of every month) serve as a public introduction to many, many areas of science by professors at local universities (Syracuse, Rochester Medical Center, Upstate Medical). The discussions are always lively and the questions are never bad, making it a perfect place to learn a fair share more about the topic at hand with a guided hand(s) than you might while trying to put the proper keywords into google. The next meeting is set for early October. For more information, keep a random track of the Cafe Scientifique website,

physics.syr.edu/cafescientifique/
The-Moon Wiki Website

While many credit the plough as responsible for human civilization, it is the Moon that provided the means for knowing when to use it! Our closest celestial neighbor and the easiest target of the night sky, the Moon now has its own information-filled wiki site, the-moon.wikispaces.com. From wikipedia, “A wiki is a collaborative website which can be directly edited by anyone with access to it.” If you’ve paid attention to the news lately, you know this can be a double-edged sword. That said, The-Moon Wiki is being maintained by a small number of dedicated astronomers and, one can only imagine, all data is being checked, making this an excellent resource for lunar history and observing.The Dark Side of the New YorkerAn illuminating story about light pollution in the New Yorker (Aug. 20, 2007). John McMahon provided us the link to the article, now available online in its entirety (for now, anyway).

www.newyorker.com/reporting/2007/08/20/070820fa_fact_owen

Additions to the Forster Collection

The images this month are being kept local, featuring, as always, the work of our own Stu Forster. It’s always delightful to see just how much structure exists in astronomical objects that our vision (and the atmosphere above us) reveal only after many, many exposures.

The Brady Emails #1

The last two points of note to the SAS were provided by email by our own Michael Brady.

I am very pleased to announce that one of our more recent SAS guest speakers is one of just nine 2007 inductees being honored on October 7, 2007 by the National Woman’s Hall of Fame.I will be attending this special ceremony and encourage anyone else interested in honoring the very real “Mother of the Spitzer Space Telescope” on this very special occasion. Judy’s work in infrared astronomy is a foundation for current and future research.

From the greatwomen.org website:

Dr. Judith L. Pipher (1940- ) Dr. Judith Pipher’s research in the field of Infrared Astronomy began in graduate school with work on some of the first rocket-borne telescopes. Since 1971, Dr. Pipher has served on the faculty of the University of Rochester, where she and her colleagues were the first U.S. astronomers to turn an infrared array toward the skies. Her experiments with ground-based and airborne telescopes culminated in development of a camera for, and infrared observations on, the Spitzer Space Telescope, launched in 2003.”

For more information, see www.greatwomen.org/news.php?action=view&id=56

The Brady Emails #2

From the Night Sky Network (NSN):

Seeing in the Dark, a visually stunning HDTV documentary on the rewards of first-person, hands-on astronomy –exactly what you do in your outreach!– that will air Wednesday, September 19 at 8:00 p.m. over PBS stations nationwide (check local listings).

We are encouraging NSN members to utilize the local airing of the program as an outreach opportunity. For example, the Challenger Center in Tallahassee, Florida will project the live HD broadcast onto their planetarium dome and is inviting the public and astronomy groups in for a free screening. It can also be projected onto an auditorium screen. Please note that you cannot charge entry for this event. Such live screenings provide the opportunity to get people to your facility and further educational outreach by fielding questions after the program. You can contact your area PBS station to confirm the local air time and coordinate promotion of the event with their public information officer. A locator for PBS stations is available on the home page at www.pbs.org.

Find more details about the show, as well as links to resources here:

www.astrosociety.org/seeinginthedark.html

Space is the place,
Damian Allis, Ph.D.
sas@somewhereville.com

Links Used Above (Subject To Web Changes)
www.syracuse-astro.org/august2007_summerseminar.html
en.wikipedia.org/wiki/Perseids
www.astro-physics.com/index.htm?products/accessories/solar_acc/astrosolar
en.wikipedia.org/wiki/Sunspot
en.wikipedia.org/wiki/Sun
physics.syr.edu/faculty/vidali.html
www.syr.edu
physics.syr.edu
www.optcorp.com
www.syracuse-astro.org/pdf/sas_brochure.pdf
www.syracuse-astro.org/observatory.html
physics.syr.edu/cafescientifique
www.ohmlounge.com
www.urmc.rochester.edu
www.upstate.edu
www.google.com
en.wikipedia.org/wiki/Plough
en.wikipedia.org/wiki/Moon
the-moon.wikispaces.com
en.wikipedia.org
en.wikipedia.org/wiki/Wiki
www.newyorker.com/reporting/2007/08/20/070820fa_fact_owen
www.newyorker.com
webserver.lemoyne.edu/~mcmahon/mcmahon.html
www.greatwomen.org
en.wikipedia.org/wiki/Spitzer_Telescope
spider.pas.rochester.edu/mainFrame/people/pages_old/Pipher.html
www.greatwomen.org/news.php?action=view&id=56
nightsky.jpl.nasa.gov
www.astrosociety.org/seeinginthedark.html
www.pbs.org

Obligatory


T R P Nanosys


Syracuse Astro


Ubuntu 4 Nano


N-Fact. Collab.

Nano Gallery

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  • Aerial Photos

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  • Syracuse Scenes

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