61 research outputs found

    The Mutual Orbit, Mass, and Density of Transneptunian Binary Gknhmdm (229762 2007 UK126)

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    We present high spatial resolution images of the binary transneptunian object Gkn'hmdm (229762 2007 UK126) obtained with the Hubble Space Telescope and with the Keck observatory on Mauna Kea to determine the orbit of G' hG' h, the much smaller and redder satellite. G' h orbits in a prograde sense, on a circular or near-circular orbit with a period of 11.3 days and a semimajor axis of 6000 km. Tidal evolution is expected to be slow, so it is likely that the system formed already in a low-eccentricity configuration, and possibly also with the orbit plane of the satellite in or close to the plane of Gkn'hmdm's equator. From the orbital parameters we can compute the system mass to be 1.4 10(exp 20) kg. Combined with estimates of the size of Gkn'hmdm from thermal observations and stellar occultations, we can estimate the bulk density as about 1 g cm(exp 3). This low density is indicative of an ice-rich composition, unless there is substantial internal porosity. We consider the hypothesis that the composition is not unusually ice-rich compared with larger TNOs and comet nuclei, and instead the porosity is high, suggesting that mid-sized objects in the 400 to 1000 km diameter range mark the transition between small, porous objects and larger objects that have collapsed their internal void space as a result of their much higher internal pressures and temperatures

    TNOs are Cool: A survey of the trans-Neptunian region V. Physical characterization of 18 Plutinos using Herschel PACS observations

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    We present Herschel PACS photometry of 18 Plutinos and determine sizes and albedos for these objects using thermal modeling. We analyze our results for correlations, draw conclusions on the Plutino size distribution, and compare to earlier results. Flux densities are derived from PACS mini scan-maps using specialized data reduction and photometry methods. In order to improve the quality of our results, we combine our PACS data with existing Spitzer MIPS data where possible, and refine existing absolute magnitudes for the targets. The physical characterization of our sample is done using a thermal model. Uncertainties of the physical parameters are derived using customized Monte Carlo methods. The correlation analysis is performed using a bootstrap Spearman rank analysis. We find the sizes of our Plutinos to range from 150 to 730 km and geometric albedos to vary between 0.04 and 0.28. The average albedo of the sample is 0.08 \pm 0.03, which is comparable to the mean albedo of Centaurs, Jupiter Family comets and other Trans-Neptunian Objects. We were able to calibrate the Plutino size scale for the first time and find the cumulative Plutino size distribution to be best fit using a cumulative power law with q = 2 at sizes ranging from 120-400 km and q = 3 at larger sizes. We revise the bulk density of 1999 TC36 and find a density of 0.64 (+0.15/-0.11) g cm-3. On the basis of a modified Spearman rank analysis technique our Plutino sample appears to be biased with respect to object size but unbiased with respect to albedo. Furthermore, we find biases based on geometrical aspects and color in our sample. There is qualitative evidence that icy Plutinos have higher albedos than the average of the sample.Comment: 18 pages, 8 figures, 8 tables, accepted for publication in A&

    How the Web was told: Continuity and change in the founding fathers’ narratives on the origins of the World Wide Web

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    The essay investigates the evolution of the “narratives of invention” used by the founding fathers of the World Wide Web in a selected corpus of papers written by Tim Berners-Lee and colleagues from 1989 up to 1993 and later in the books of James Gillies and Robert Cailliau and of Berners-Lee himself in 2000. Thanks to a textual analysis that cross these sources, we identify three main sets of common keywords that did not change and three couples of conflicting keywords that depict the evolution of the narratives over time. Change and continuity, intertwined with conservation and innovation, emerge as the key strategies of the Web’s founding fathers in narrating their idea

    Instrumenting a rowing ergometer for improved training

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    Rowing ergometers are used by athletes for indoor training and performance improvement. Typical commercial ergometers provide some information (for example power output and covered distance), but these indications are typically estimated starting from the fan speed and thus are not very reliable as already pointed out in the literature. The present paper presents the work done to fully instrument a commercial rowing ergometer in order to directly measure all relevant quantities for improved training: the seat, the handlebar and the stretchers have been redesigned and equipped with force and displacement sensors able to measure both the dynamic and kinematic behavior of the athlete. In this way the interaction of the athlete with the rowing machine is fully known, together with the direct measurement of the instantaneous rowing power output. Some results are also presented and discussed
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