Annualreport2006 Web.Pdf
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Perfect Little Planet Educator Guide Clark Planetarium Education Department
Perfect Little Planet Educator Guide Clark Planetarium Education Department Questions or comments can be directed to the Clark Planetarium Education Department at [email protected]. 1 Perfect Little Planet Educator Guide Table of Contents Vocabulary List. 3 Activities for the Imagination. 4 Word Search. .5 Two Astronomy Games. .7 A Toilet Paper Solar System Scale Model. .13 The Scale of the Solar System. 16 Solar System Models in Dough. .17 Solar System Fact Sheet. 20 2 Perfect Little Planet Educator Guide Vocabulary List Solar System Planet Asteroid Moon Comet Dwarf Planet Gas Giant "Rocky Midgets" (Terrestrial Planets) Sun Star Impact Orbit Planetary Rings Atmosphere Volcano Great Red Spot Olympus Mons Mariner Valley Acid Solar Prominence Solar Flare Ocean Earthquake Continent Plants and Animals Humans 3 Perfect Little Planet Educator Guide Activities for the Imagination The objectives of these activities are: to learn about Earth and other planets, use language and art skills, encourage use of libraries, and help develop creativity. The scientific accuracy of the creations may not be as important as the learning, reasoning, and imagination used to construct each invention. Invent a Planet Students may create (draw, paint, montage, build from household or classroom items, whatever!) a planet. Does it have air? What color is its sky? Does it have ground? What is its ground made of? What is it like on this world? Invent an Alien Students may create (draw, paint, montage, build from household items, etc.) an alien. To be fair to the alien, they should be sure to provide a way for the alien to get food (what is that food?), a way to breathe (if it needs to), ways to sense the environment, and perhaps a way to move around its planet. -
Annualreport2005 Web.Pdf
Vision Statement The Space Science Institute is a thriving center of talented, entrepreneurial scientists, educators, and other professionals who make outstanding contributions to humankind’s understanding and appreciation of planet Earth, the Solar System, the galaxy, and beyond. 2 | Space Science Institute | Annual Report 2005 From Our Director Excite. Explore. Discover. These words aptly describe what we do in the research realm as well as in education. In fact, they defi ne the essence of our mission. Our mission is facilitated by a unique blend of on- and off-site researchers coupled with an extensive portfolio of education and public outreach (EPO) projects. This past year has seen SSI grow from $4.1M to over $4.3M in grants, an increase of nearly 6%. We now have over fi fty full and part-time staff. SSI’s support comes mostly from NASA and the National Sci- ence Foundation. Our Board of Directors now numbers eight. Their guidance and vision—along with that of senior management—have created an environment that continues to draw world-class scientists to the Institute and allows us to develop educa- tion and outreach programs that benefi t millions of people worldwide. SSI has a robust scientifi c research program that includes robotic missions such as the Mars Exploration Rovers, fl ight missions such as Cassini and the Spitzer Space Telescope, Hubble Space Telescope (HST), and ground-based programs. Dr. Tom McCord joined the Institute in 2005 as a Senior Research Scientist. He directs the Bear Fight Center, a 3,000 square-foot research and meeting facility in Washington state. -
Curriculum Vitae - 24 March 2020
Dr. Eric E. Mamajek Curriculum Vitae - 24 March 2020 Jet Propulsion Laboratory Phone: (818) 354-2153 4800 Oak Grove Drive FAX: (818) 393-4950 MS 321-162 [email protected] Pasadena, CA 91109-8099 https://science.jpl.nasa.gov/people/Mamajek/ Positions 2020- Discipline Program Manager - Exoplanets, Astro. & Physics Directorate, JPL/Caltech 2016- Deputy Program Chief Scientist, NASA Exoplanet Exploration Program, JPL/Caltech 2017- Professor of Physics & Astronomy (Research), University of Rochester 2016-2017 Visiting Professor, Physics & Astronomy, University of Rochester 2016 Professor, Physics & Astronomy, University of Rochester 2013-2016 Associate Professor, Physics & Astronomy, University of Rochester 2011-2012 Associate Astronomer, NOAO, Cerro Tololo Inter-American Observatory 2008-2013 Assistant Professor, Physics & Astronomy, University of Rochester (on leave 2011-2012) 2004-2008 Clay Postdoctoral Fellow, Harvard-Smithsonian Center for Astrophysics 2000-2004 Graduate Research Assistant, University of Arizona, Astronomy 1999-2000 Graduate Teaching Assistant, University of Arizona, Astronomy 1998-1999 J. William Fulbright Fellow, Australia, ADFA/UNSW School of Physics Languages English (native), Spanish (advanced) Education 2004 Ph.D. The University of Arizona, Astronomy 2001 M.S. The University of Arizona, Astronomy 2000 M.Sc. The University of New South Wales, ADFA, Physics 1998 B.S. The Pennsylvania State University, Astronomy & Astrophysics, Physics 1993 H.S. Bethel Park High School Research Interests Formation and Evolution -
Space Telescope
rnal 5 Monty tarium of the Space Telescope ............ New ............................................... a 29 Gibbous Gazette ........................................... 32 Mobile News Network ............................................ 36 Planetechnica: Slip Rings .............................. 41 Reports from Committees ................................. 43 Secretary's Report ............................................. 47 President's Message ....................................... 54 jane's Corner ............................................................ Seeing Is Believing! In The U.S. & Canada contact Pearl Reilly: 1-800-726-8805 fax : 1-504-764-7665 email : [email protected] Aufflonzoo DlSlntJur", of ZetSS Plaflelilnums In The Umtoo Stares & Canada Carl Zeiss, Planelarium Division 0-07740 Jena ~SEILER +49-3641-642406, fax: -643023 email: [email protected] I N B TRLJIVlENT 170 E. Kirkham Ave ., St.louis. MO 63119 Planetarium Office: #28 Houmas Place, Destrehan, LA 70047 The Planetarian (ISN 0090-3213) is published quarterly by the International Dl"Ylai-,.,,,.',-,,,,,, Society. ©1998, International Planetarium Society, Inc., all rights reserved. Opinions exp1ressed e by authors are personal opinions and are not necessarily the opinions of the International etarium Society, its officers, or agents. Acceptance of advertisements, announcements, 1.27, No.4 material does not imply endorsement by the International Planetarium Society, its officers agents. The Editor welcomes items for consideration for publication. Please consult -
Spitzer Team Says Debris Disk Could Be Forming Infant Terrestrial Planets 14 December 2005
Spitzer Team Says Debris Disk Could Be Forming Infant Terrestrial Planets 14 December 2005 an asteroid belt, roughly at the distance Jupiter is from our sun." "This object is very unusual in the context of all the others we've looked at," said University of Arizona assistant astronomy Professor Michael R. Meyer, a colleague in the discovery. Meyer directs a Spitzer Legacy project to study solar system formation and evolution in a sample of 328 young sun-like stars in the Milky Way. The project turned up the unusual system. "This is the only such debris disk among the 33 sun- like stars we've studied in our project so far, and one of only five such objects known," Meyer said. The star, named HD 12039, is about 30 million years old, or the age of the sun when the terrestrial planets are thought to have been 80 percent complete and the Earth-moon system formed, the Astronomers have found a debris disk around a astronomers said. It is roughly 137 light years sun-like star that may be forming or has formed its away, or the distance light travels in 137 years. terrestrial planets. The disk - a probable analog to our asteroid belt - may have begun a solar-system- HD 12039 is a "G" type star like our sun, a yellow scale demolition derby, where the rocky remains of star with surface temperatures between 5,000 and failed planets collide chaotically. 7,000 degrees Fahrenheit. It hasn't yet settled into the "main sequence," or mature nuclear-burning Image: Scientists can characterize a disk by phase as our sun has. -
Clark Planetarium Productions Price List
CLARK PLANETARIUM PRODUCTIONS PRICE LIST Effective 1/1/2021 All prices are U.S. Dollars. [email protected] / +1 385 468 1226 PLANETARIUM SHOWS • Accidental Astronauts • Exploding Universe th Educational • Black Holes 10 Anniversary Edition • Perfect Little Planet • The Edge: Pluto and Beyond • Extreme Planets Shows • Attack of the Space Pirates • Secret of the Cardboard Rocket • Saturn: Jewel of the Heavens 5,001 - 10,001 - 30,001 - 50,001 - 100,001 - 200,001 - Annual Attendance 1 - 5,000 300,001 + 10,000 30,000 50,000 100,000 200,000 300,000 Seating Capacity* 1 - 25 26 - 50 51 - 80 81 - 120 121 - 170 171 - 230 231 - 300 301 + 50 Year $2,500 $4,000 $7,000 $11,000 $16,000 $22,000 $27,000 $32,000 1 Year $2,000 $3,200 $5,600 $8,800 $12,800 $17,600 $21,600 $25,600 ♪ Let it Snow ♪ Led Zeppelin (A Fulldome Audiovisual Experience) Entertainment ♪ ♪ Shows Rock the Dome Modern U2 (A Fulldome Audiovisual Experience) ♪ Rock the Dome Classic 5,001 - 10,001 - 30,001 - 50,001 - 100,001 - 200,001 - Annual Attendance 1 - 5,000 300,001 + 10,000 30,000 50,000 100,000 200,000 300,000 Seating Capacity* 1 - 25 26 - 50 51 - 80 81 - 120 121 - 170 171 - 230 231 - 300 301 + 50 Year $1,900 $3,000 $5,300 $8,300 $12,000 $16,500 $20,300 $24,000 1 Year $1,500 $2,400 $4,200 $6,600 $9,600 $13,200 $16,200 $19,200 *Show Pricing Policy Show prices are determined by annual attendance of the most recent calendar year in which the theater was fully operational: the total number of paying and non-paying individuals that attended any presentation in the licensee's theater. -
Bibliography Illustration by Lynette Cook Illustration by Lynette
Amaya Moro-Martín Bibliography Illustration by Lynette Cook Illustration by Lynette Refereed papers (first, second and third author) ! Does the presence of planets affect the observed frequency and properties of Kuiper Belt-like disks? Results from the Herschel DUNES and DEBRIS surveys. Moro-Martín, A., Marshall, J. P., Kennedy, G., Sibthorpe B., Matthews B. C., Eiroa C., Wyatt M. C., Maldonado, J., Rodriguez, D., Greaves J. S., Montesinos, B., Lestrade, J.-F., Booth, M., Duchene, G., Wilner, D., Horner, J. !Astrophysical Journal, in press (2015) Proper Motions of Young Stellar Outflows in the mid-IR with Spitzer II. HH 377/CEP E Noriega-Crespo, A., Raga, A. C., Moro-Martín, A. Flagey, N. and Carey, S. J. !New Journal of Physics, 16 (2014). Correlations between the stellar, planetary, and debris components of exoplanet sys- tems observed by Herschel Marshall, J. P., Moro-Martín, A., Eiroa, C., Kennedy, G., Mora, A., Sibthorpe, B., Lestrade, J.-F., Maldonado, J., Sanz-Forcada, J., Wyatt, M. C., Matthews, B., Horner, J., Montesinos, B., Bryden, G., del Burgo, C., Greaves, J. S., Ivison, R. J., Meeus, G., Olofsson, G., Pilbratt, G. L., & White, G. J. !Astronomy & Astrophysics, 565, 15 (2014) The SEEDS Direct Imaging Survey for Planets and Scattered Dust Emission in Debris Disk Systems Janson, M., Brandt, T. D., Moro-Martín, A., Usuda, T., Thalmann, C., Carson, J. C., Goto, M., Currie, T., McElwain, M. W., Itoh, Y., Fukagawa, M., Crepp, J., Kuzuhara, M., Hashimoto, J., Kudo, M., Kusakabe, N., Abe, L., Brandner, W., Egner, S. E., Feldt, M., Grady, C., Guyon, O., Hayano, Y., Hayashi, M., Hayashi, S., Henning, T., Hodapp, K., Ishii, M., Iye, M., Kandori, R., Knapp, G. -
Extrasolar Kuiper Belt Dust Disks 465
Moro-Martín et al.: Extrasolar Kuiper Belt Dust Disks 465 Extrasolar Kuiper Belt Dust Disks Amaya Moro-Martín Princeton University Mark C. Wyatt University of Cambridge Renu Malhotra and David E. Trilling University of Arizona The dust disks observed around mature stars are evidence that plantesimals are present in these systems on spatial scales that are similar to that of the asteroids and the Kuiper belt ob- jects (KBOs) in the solar system. These dust disks (a.k.a. “debris disks”) present a wide range of sizes, morphologies, and properties. It is inferred that their dust mass declines with time as the dust-producing planetesimals get depleted, and that this decline can be punctuated by large spikes that are produced as a result of individual collisional events. The lack of solid-state fea- tures indicate that, generally, the dust in these disks have sizes >10 µm, but exceptionally, strong silicate features in some disks suggest the presence of large quantities of small grains, thought to be the result of recent collisions. Spatially resolved observations of debris disks show a di- versity of structural features, such as inner cavities, warps, offsets, brightness asymmetries, spirals, rings, and clumps. There is growing evidence that, in some cases, these structures are the result of the dynamical perturbations of a massive planet. Our solar system also harbors a debris disk and some of its properties resemble those of extrasolar debris disks. From the cratering record, we can infer that its dust mass has decayed with time, and that there was at least one major “spike” in the past during the late heavy bombardment. -
Ringworld: Travellers' Tales from Saturn
Utah State University DigitalCommons@USU Public Talks Astrophysics 3-21-2009 Ringworld: Travellers' Tales from Saturn Shane L. Larson Utah State University Follow this and additional works at: https://digitalcommons.usu.edu/astro_pubtalks Part of the Astrophysics and Astronomy Commons Recommended Citation Larson, Shane L., "Ringworld: Travellers' Tales from Saturn" (2009). Public Talks. Paper 19. https://digitalcommons.usu.edu/astro_pubtalks/19 This Presentation is brought to you for free and open access by the Astrophysics at DigitalCommons@USU. It has been accepted for inclusion in Public Talks by an authorized administrator of DigitalCommons@USU. For more information, please contact [email protected]. RINGWORLD: Travellers’ Tales from Saturn Shane L. Larson Department of Physics Utah State University [email protected] Clark Planetarium Salt Lake City, UT 21 March 2009 1 Storyline Saturn Unveiled Emissaries Saturn up close Rings and Moons 2 Galileo Galilei In 1609, Galileo heard of the invention of the telescope By 1610, he had constructed one and observed the skies “I render infinite thanks to God for being so kind as to make me alone the first observer of marvels kept hidden in obscurity for all previous centuries.” Stars, the Moon, Venus, Mars, Jupiter, and Saturn 3 Saturn through a telescope Initially Galileo didn’t know what he was seeing “Saturn has ears.” Galileo’s early scopes weren’t the greatest! In 1655 Christiaan Huygens observed Saturn and proposed “It is surrounded by a thin, flat, ring, nowhere touching, inclined to the ecliptic.” This is what Saturn really looks like through a telescope! But we wanted to see Saturn up close, and personal.. -
GLPA Newsletter Incorporates Small Sections of Several NASA Images for Its Page Mastheads
IMAGE CREDITS Cover Design: Jackie Baughman ([email protected]) Cover Illustration: The cover of this issue features Jackie Baughman’s artistic interpretation of the Apollo 13 insignia. NASA’s original description of that mission insignia: “Apollo, the sun god of Greek mythology, was represented as the Sun, with three horses driving his chariot across the surface of the Moon, symbolizing how the Apollo flights have extended the light of knowledge to all mankind.” The current design of the GLPA Newsletter incorporates small sections of several NASA images for its page mastheads. These and other images can be accessed from NASA websites such as Mars Exploration, Scientific Visualization Studio, and Hubble Space Telescope websites at www.spacetelescope.org/images/, heritage.stsci.edu, and hubblesite.org/ gallery. And because all these photos are from NASA, they are free to use (with proper credit). Image Credits page background image: NGC 2074 in the Large Magellanic Cloud Credit: NASA, ESA, and M. Livio (STScI) Image Credits page inset image: M96: A Galactic Maelstrom Credit: ESA/Hubble & NASA and LEGUS Team State News Masthead: Young stars in the “wing” of the Small Magellanic Cloud Credit: NASA, ESA, CXC and University of Potsdam, JPL-Caltech, and STScI Bulletin Board Masthead: M13: A Celestial Snow Globe of Stars Credit: NASA, ESA, and Hubble Heritage Team (STScI/AURA) IPS Update Masthead: Big Blue Marble Earth Credit: R. Stockli, A. Nelson, F. Hasler, NASA/ GSFC/ NOAA/ USGS Hi everyone! It’s a brand new season and you have a brand new GLPA President. Although I’ve been on the Executive Committee as President-Elect for the President’s past two years, I’m still admittedly new to the Message committee. -
Hst and Spitzer Observations of the Hd 207129 Debris Ring
The Astronomical Journal, 140:1051–1061, 2010 October doi:10.1088/0004-6256/140/4/1051 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A. ! HST AND SPITZER OBSERVATIONS OF THE HD 207129 DEBRIS RING John E. Krist1, Karl R. Stapelfeldt1, Geoffrey Bryden1,2, George H. Rieke3, K. Y. L. Su3, Christine C. Chen4, Charles A. Beichman2, Dean C. Hines5, Luisa M. Rebull6, Angelle Tanner7, David E. Trilling8, Mark Clampin9, and Andras´ Gasp´ ar´ 3 1 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 2 NASA Exoplanet Science Institute, California Institute of Technology, 770 S. Wilson Ave., Pasadena, CA 91125, USA 3 Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA 4 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA 5 Space Science Institute, 4750 Walnut St. Suite 205, Boulder, CO 80301, USA 6 Spitzer Science Center, Mail Stop 220-6, California Institute of Technology, Pasadena, CA 91125, USA 7 Georgia State University, Department of Physics and Astronomy, One Park Place, Atlanta, GA 30316, USA 8 Department of Physics and Astronomy, Northern Arizona University, Box 6010, Flagstaff, AZ 86011, USA 9 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Received 2010 April 26; accepted 2010 August 14; published 2010 September 9 ABSTRACT A debris ring around the star HD 207129 (G0V; d 16.0 pc) has been imaged in scattered visible light with the ACS coronagraph on the Hubble Space Telescope (HST= ) and in thermal emission using MIPS on the Spitzer Space Telescope at λ 70 µm (resolved) and 160 µm (unresolved). -
Formation and Evolution of Planetary Systems: Upper Limits to the Gas Mass in Disks Around Sun-Like Stars
Formation and Evolution of Planetary Systems: Upper Limits to the Gas Mass in Disks Around Sun-like Stars I. Pascucci1, U. Gorti2, D. Hollenbach3, J. Najita4, M. R. Meyer1, J. M. Carpenter5, L. A. Hillenbrand5, G. J. Herczeg5, D. L. Padgett5, E. E. Mamajek6, M. D. Silverstone1, W. M. Schlingman1, J. S. Kim1, E. B. Stobie1, J. Bouwman7, S. Wolf7, J. Rodmann7, D. C. Hines8, J. Lunine9, R. Malhotra9 ABSTRACT We have carried out a sensitive search for gas emission lines at infrared and millimeter wave- lengths for a sample of 15 young sun–like stars selected from our dust disk survey with the Spitzer Space Telescope. We have used mid–infrared lines to trace the warm (300–100K) gas in the inner disk and millimeter transitions of 12CO to probe the cold ( 20K) outer disk. We report no gas line detections from our sample. Line flux upper limits are∼ first converted to warm and cold gas mass limits using simple approximations allowing a direct comparison with values from the lit- erature. We also present results from more sophisticated models following Gorti and Hollenbach (2004) which confirm and extend our simple analysis. These models show that the [S i] line at 25.23 µm can set constraining limits on the gas surface density at the disk inner radius and traces disk regions up to a few AU. We find that none of the 15 systems have more than 0.04 MJ of gas within a few AU from the disk inner radius for disk radii from 1 AU up to 40AU.