26 research outputs found

    Ensemble Properties of Comets in the Sloan Digital Sky Survey

    Full text link
    We present the ensemble properties of 31 comets (27 resolved and 4 unresolved) observed by the Sloan Digital Sky Survey (SDSS). This sample of comets represents about 1 comet per 10 million SDSS photometric objects. Five-band (u,g,r,i,z) photometry is used to determine the comets' colors, sizes, surface brightness profiles, and rates of dust production in terms of the Af{\rho} formalism. We find that the cumulative luminosity function for the Jupiter Family Comets in our sample is well fit by a power law of the form N(< H) \propto 10(0.49\pm0.05)H for H < 18, with evidence of a much shallower fit N(< H) \propto 10(0.19\pm0.03)H for the faint (14.5 < H < 18) comets. The resolved comets show an extremely narrow distribution of colors (0.57 \pm 0.05 in g - r for example), which are statistically indistinguishable from that of the Jupiter Trojans. Further, there is no evidence of correlation between color and physical, dynamical, or observational parameters for the observed comets.Comment: 19 pages, 8 tables, 11 figures, to appear in Icaru

    Fabrication of MEMS Microshutter Arrays for Cryogenic Applications

    Get PDF
    Two-dimensional MEMS microshutter arrays are being developed for use as a high contrast field selector for the Near Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope (JWST). We present details of microshutter array fabrication and give results of work done to optimize the flatness of microshutter elements through film stress control for both room temperature and cryogenic (35K) operation

    <i>Spitzer</i> Microlensing Parallax Reveals Two Isolated Stars in the Galactic Bulge

    Get PDF
    We report the mass and distance measurements of two single-lens events from the 2017 Spitzer\textit {Spitzer} microlensing campaign. The ground-based observations yield the detection of finite-source effects, and the microlens parallaxes are derived from the joint analysis of ground-based observations and Spitzer\textit {Spitzer} observations. We find that the lens of OGLE-2017-BLG-1254 is a 0.60 ± 0.03 M ⊙ star with D LS = 0.53 ± 0.11 kpc, where D LS is the distance between the lens and the source. The second event, OGLE-2017-BLG-1161, is subject to the known satellite parallax degeneracy, and thus is either a 0.51−0.10+0.12 M⊙{0.51}_{-0.10}^{+0.12}\,{M}_{\odot } star with D LS = 0.40 ± 0.12 kpc or a 0.38−0.12+0.13 M⊙{0.38}_{-0.12}^{+0.13}\,{M}_{\odot } star with D LS = 0.53 ± 0.19 kpc. Both of the lenses are therefore isolated stars in the Galactic bulge. By comparing the mass and distance distributions of the eight published Spitzer\textit {Spitzer} finite-source events with the expectations from a Galactic model, we find that the Spitzer\textit {Spitzer} sample is in agreement with the probability of finite-source effects occurring in single-lens events

    The Digital Earth

    No full text
    The Digital Earth is a virtual representation of our planet that enables a person to explore and interact with the vast amounts of natural, cultural, and historical information being gathered about the Earth. This video describes the need for such a system, possible uses of a Digital Earth system, and the technologies and organizations that must come together in order for it to become a reality. Educational levels: Undergraduate lower division, Undergraduate upper division, Graduate or professional

    Lexical Learning in Bilingual Adults: The Relative Importance of Short-Term Memory for Serial Order and Phonological Knowledge

    Full text link
    Studies of monolingual speakers have shown a strong association between lexical learning and short-term memory (STM) capacity, especially STM for serial order information. At the same time, studies of bilingual speakers suggest that phonological knowledge is the main factor that drives lexical learning. This study tested these two hypotheses simultaneously in participants with variable levels of English-French bilingual proficiency. A word-nonword paired-associate learning task was administered, with nonwords obeying French phonotactic patterns. French phonological knowledge was estimated by a composite French proficiency score summarizing productive and receptive French vocabulary knowledge as well as quantitative and qualitative measures of French exposure. STM measures maximized retention of order information (serial order reconstruction) or retention of phonological item information (single nonword delayed repetition). The French proficiency score and the serial order STM measure independently predicted performance on the paired-associate learning task. These results highlight the conjoined role of phonological knowledge and serial order STM in lexical learning. Importantly, serial order STM remains a strong predictor of lexical learning, even for bilingual individuals who have broad phonological knowledge

    Pulse of the Planet

    No full text
    Akin to a living creature, Earths land, air, oceans, ice, and life fit together into a complex, interlocking system. Space affords a unique vantage point from which to observe the daily, seasonal, and annual changes in Earths systems. Using data from advanced satellites, NASA visualizations portray a majestic, and sometimes violent, natural world and also capture the influences humans have on the planet. Over 80 NASA-related earth science animations created over the past 8 years implementing realtime and non-realtime techniques have been used on this visual journey. Tools used included IDL, Lightwave3D, Final Cut Pro, Performer, Vis5D, and custom software. Educational levels: Undergraduate lower division, Undergraduate upper division, Graduate or professional

    MEMS Microshutter Arrays for James Webb Space Telescope

    No full text
    MEMS microshutter arrays are being developed at NASA Goddard Space Flight Center for use as an aperture array for a Near-Infrared Spectrometer (NirSpec). The instruments will be carried on the James Webb Space Telescope (JWST), the next generation of space telescope after Hubble Space Telescope retires. The microshutter arrays are designed for the selective transmission of light with high efficiency and high contrast, Arrays are close-packed silicon nitride membranes with a pixel size of 100x200 microns. Individual shutters are patterned with a torsion flexure permitting shutters to open 90 degrees with a minimized mechanical stress concentration. Light shields are made on to each shutter for light leak prevention so to enhance optical contrast, Shutters are actuated magnetically, latched and addressed electrostatically. The shutter arrays are fabricated using MEMS technologies
    corecore