Search for Dust Emission from (24) Themis Using the Gemini-North Telescope

We report the results of a search for a dust trail aligned with the orbit plane of the large main-belt asteroid (24) Themis, which has been reported to have water ice frost on its surface. Observations were obtained with the GMOS instrument on the Gemini-North Observatory in imaging mode, where we used a chip gap to block much of the light from the asteroid, allowing us to take long exposures while avoiding saturation by the object. No dust trail is detected within 2' of Themis to a 3-sigma limiting surface brightness magnitude of 29.7 mag/arcsec^2, as measured along the expected direction of the dust trail. Detailed consideration of dust ejection physics indicates that particles large enough to form a detectable dust trail were unlikely to be ejected as a result of sublimation from an object as large as Themis. We nonetheless demonstrate that our observations would have been capable of detecting faint dust emission as close as 20" from the object, even in a crowded star field. This approach could be used to conduct future searches for sublimation-generated dust emission from Themis or other large asteroids closer to perihelion than was done in this work. It would also be useful for deep imaging of collisionally generated dust emission from large asteroids at times when the visibility of dust features are expected to be maximized, such as during orbit plane crossings, during close approaches to the Earth, or following detected impact events.Comment: 11 pages, 4 figures, accepted for publication in PAS

Vertical axis wind turbine

Includes bibliographical references.The objective of this project was to design and simulate a turbine capable of effectively harnessing wind energy into a viable and practical source of consumer electric energy. This was done by the optimization of three different portions of the design. First, restraint of the column that transferred the physical energy to the generator was optimized. This took into consideration the weight of the turbine portion of the structure, the torque seen due to the rotation of the blades, and the bending caused by the wind and other transverse loads upon the column. Second, the propeller design was optimized. This was done by designing and testing blades that had a low coefficient of drag on one side and a very high coefficient on the opposite side. Finally, the generator was optimized for the maximal electric output due to our expected revolutions per minute of the transfer column. The optimizations of the column portion of the project were done by an initial analysis of the structure by methods of strength of materials. Once broad dimensions were decided, they were further narrowed down by the help of analytical computer software, in this case, the Mechanica add-on for Pro/Engineer. The expected RPMs of the blade portion were determined by methods of fluid mechanics and also by simulation in Fluent, a fluid flow simulation software package. The generator was then optimized in the ELE lab for maximum electrical output from the resulting RPMs we expected the generator to see. What this project resulted in was a fully functional design of a vertical axis wind turbine that is capable of producing a significant amount of electrical energy.B.S. (Bachelor of Science

Development of a Cross-border Business-to-Business-to-Consumer (B2B2C) System to Enhance Enterprise Performance: A Case Study of Legend Harvest Group

This research focused on the efforts of Legend Harvest Group (LHG), a California startup, to realise its cross-border business-to-business-to-consumer (B2B2C) e-commerce business opportunities. The issues identified during the research demonstrated that an operational B2B2C system is more complicated than a manually operated business-to-business (B2B) trade. The complexities of cross-border e-commerce platforms include insufficient data transparency, logistical obstacles, and Customs hurdles. LHG encountered difficulties in understanding and dealing with these obstacles. My research focused on analysing the technological, operational and organisational requirements and finding the critical elements and leverage points of adopting a new B2B2C system. I developed a platform–system–technology–human (PSTH) conceptual framework based on my literature review that served as the theoretical blueprint of this action research. I adopted a participatory action research (PAR) method and a purposeful sampling strategy to conduct an action research study. The sampling population comprised LHG’s executives, as well as board members, officers, employees, and consultants associated with the company. I applied a qualitative approach as the most suitable choice in action research study, using interviews, semi-structured discussions, and observations to collect data. This research was based on three action cycles. Each action cycle consisted of four phases: reflect, plan, act and observe. The first action cycle (AC1) focused on scanning the environment to identify the barriers preventing LHG from adopting a B2B2C system. The second action cycle (AC2) addressed the technological, operational and organisational requirements, and collaborated with a Software-as-a-Service (SaaS) provider to implement a trial run and collect actual data. The third action cycle (AC3) involved an in-depth thematic analysis to evaluate the trial-run results and proposed an integrators network for LHG’s future B2B2C system development. Research accomplishments include initial identification of sixty-one emergent codes as barriers to LHG’s supply chain automation quest, categorisation of these codes into fifteen actionable themes, and, finally, selection of five actionable themes as critical elements to follow in adopting a B2B2C system, namely, process automation (A), SaaS adoption (S), supply chain integration (I), collaboration (C) and trust (T). From post-trial-run analysis, I recognised these five themes as the key integrators and proposed a B2B2C supply chain model to cope with the cross-border e-commerce platforms. The interdependent nature of these five integrators led to the conceptualisation of an “ASICT” network that can be used to tackle the platforms’ demands. Based on the research findings, I learned that a sustainable B2B2C system will depend not only on technology implementation such as SaaS adoption, supply chain integration and process automation, but also on human interaction such as collaboration and trust. This research concluded that these five “ASICT” integrators are critical elements, and that trust and collaboration are the key leverage points in the company’s efforts to develop a cross-border B2B2C system. The benefits projected by adopting the B2B2C system included not only reducing LHG’s transactional costs but also enhancing its enterprise performance by automating and integrating the supply chain, allowing the management to map operational efficiency with financial outcome and to transform the e-commerce supply chain into a value chain

Observational and Dynamical Characterization of Main-Belt Comet P/2010 R2 (La Sagra)

We present observations of comet-like main-belt object P/2010 R2 (La Sagra) obtained by Pan-STARRS 1 and the Faulkes Telescope-North on Haleakala in Hawaii, the University of Hawaii 2.2 m, Gemini-North, and Keck I telescopes on Mauna Kea, the Danish 1.54 m telescope at La Silla, and the Isaac Newton Telescope on La Palma. An antisolar dust tail is observed from August 2010 through February 2011, while a dust trail aligned with the object's orbit plane is also observed from December 2010 through August 2011. Assuming typical phase darkening behavior, P/La Sagra is seen to increase in brightness by >1 mag between August 2010 and December 2010, suggesting that dust production is ongoing over this period. These results strongly suggest that the observed activity is cometary in nature (i.e., driven by the sublimation of volatile material), and that P/La Sagra is therefore the most recent main-belt comet to be discovered. We find an approximate absolute magnitude for the nucleus of H_R=17.9+/-0.2 mag, corresponding to a nucleus radius of ~0.7 km, assuming an albedo of p=0.05. Using optical spectroscopy, we find no evidence of sublimation products (i.e., gas emission), finding an upper limit CN production rate of Q_CN<6x10^23 mol/s, from which we infer an H2O production rate of Q_H2O<10^26 mol/s. Numerical simulations indicate that P/La Sagra is dynamically stable for >100 Myr, suggesting that it is likely native to its current location and that its composition is likely representative of other objects in the same region of the main belt, though the relatively close proximity of the 13:6 mean-motion resonance with Jupiter and the (3,-2,-1) three-body mean-motion resonance with Jupiter and Saturn mean that dynamical instability on larger timescales cannot be ruled out.Comment: 23 pages, 13 figures, accepted for publication in A

α-Lactosylceramide Protects Against iNKT-Mediated Murine Airway Hyperreactivity and Liver Injury Through Competitive Inhibition of Cd1d Binding.

Invariant natural killer T (iNKT) cells, which are activated by T cell receptor (TCR)-dependent recognition of lipid-based antigens presented by the CD1d molecule, have been shown to participate in the pathogenesis of many diseases, including asthma and liver injury. Previous studies have shown the inhibition of iNKT cell activation using lipid antagonists can attenuate iNKT cell-induced disease pathogenesis. Hence, the development of iNKT cell-targeted glycolipids can facilitate the discovery of new therapeutics. In this study, we synthesized and evaluated α-lactosylceramide (α-LacCer), an α-galactosylceramide (α-GalCer) analog with lactose substitution for the galactose head and a shortened acyl chain in the ceramide tail, toward iNKT cell activation. We demonstrated that α-LacCer was a weak inducer for both mouse and human iNKT cell activation and cytokine production, and the iNKT induction by α-LacCer was CD1d-dependent. However, when co-administered with α-GalCer, α-LacCer inhibited α-GalCer-induced IL-4 and IFN-γ production from iNKT cells. Consequently, α-LacCer also ameliorated both α-GalCer and GSL-1-induced airway hyperreactivity and α-GalCer-induced neutrophilia when co-administered in vivo. Furthermore, we were able to inhibit the increases of ConA-induced AST, ALT and IFN-γ serum levels through α-LacCer pre-treatment, suggesting α-LacCer could protect against ConA-induced liver injury. Mechanistically, we discerned that α-LacCer suppressed α-GalCer-stimulated cytokine production through competing for CD1d binding. Since iNKT cells play a critical role in the development of AHR and liver injury, the inhibition of iNKT cell activation by α-LacCer present a possible new approach in treating iNKT cell-mediated diseases

The Transient Jupiter Trojan-Like Orbit of P/2019 LD2 (ATLAS)

Comet P/2019 LD2 has orbital elements currently resembling those of a Jupiter Trojan, and therefore superficially appears to represent a unique opportunity to study the volatile content and active behavior of a member of this population for the first time. However, numerical integrations show that it was previously a Centaur before reaching its current Jupiter Trojan-like orbit in 2018 July, and is expected to return to being a Centaur in 2028 February, before eventually becoming a Jupiter-family comet in 2063 February. The case of P/2019 LD2 highlights the need for mechanisms to quickly and reliably dynamically classify small solar system bodies discovered in current and upcoming wide-field surveys.Comment: 7 pages, 3 figures. Accepted for publication in Icaru

The proposed Caroline ESA M3 mission to a Main Belt Comet

We describe Caroline, a mission proposal submitted to the European Space Agency in 2010 in response to the Cosmic Visions M3 call for medium-sized missions. Caroline would have travelled to a Main Belt Comet (MBC), characterizing the object during a flyby, and capturing dust from its tenuous coma for return to Earth. MBCs are suspected to be transition objects straddling the traditional boundary between volatile–poor rocky asteroids and volatile–rich comets. The weak cometary activity exhibited by these objects indicates the presence of water ice, and may represent the primary type of object that delivered water to the early Earth. The Caroline mission would have employed aerogel as a medium for the capture of dust grains, as successfully used by the NASA Stardust mission to Comet 81P/Wild 2. We describe the proposed mission design, primary elements of the spacecraft, and provide an overview of the science instruments and their measurement goals. Caroline was ultimately not selected by the European Space Agency during the M3 call; we briefly reflect on the pros and cons of the mission as proposed, and how current and future mission MBC mission proposals such as Castalia could best be approached

SuperWASP Observations of the 2007 Outburst of Comet 17P/Holmes

We present wide-field imaging of the 2007 outburst of Comet 17P/Holmes obtained serendipitously by SuperWASP-North on 17 nights over a 42-night period beginning on the night (2007 October 22-23) immediately prior to the outburst. Photometry of 17P's unresolved coma in SuperWASP data taken on the first night of the outburst is consistent with exponential brightening, suggesting that the rapid increase in the scattering cross-section of the coma could be largely due to the progressive fragmentation of ejected material produced on a very short timescale at the time of the initial outburst, with fragmentation timescales decreasing from t(frag)~2x10^3 s to t(frag)~1x10^3 s over our observing period. Analysis of the expansion of 17P's coma reveals a velocity gradient suggesting that the outer coma was dominated by material ejected in an instantaneous, explosive manner. We find an expansion velocity at the edge of the dust coma of v(exp) = 0.55+/-0.02 km/s and a likely outburst date of t_0=2007 October 23.3+/-0.3, consistent with our finding that the comet remained below SuperWASP's detection limit of m(V)~15 mag until at least 2007 October 23.3. Modelling of 17P's gas coma indicates that its outer edge, which was observed to extend past the outer dust coma, is best explained with a single pulse of gas production, consistent with our conclusions concerning the production of the outer dust coma.Comment: 36 pages, 8 figures, accepted for publication in MNRA

Observational Constraints on the Catastrophic Disruption Rate of Small Main Belt Asteroids

We have calculated 90% confidence limits on the steady-state rate of catastrophic disruptions of main belt asteroids in terms of the absolute magnitude at which one catastrophic disruption occurs per year (HCL) as a function of the post-disruption increase in brightness (delta m) and subsequent brightness decay rate (tau). The confidence limits were calculated using the brightest unknown main belt asteroid (V = 18.5) detected with the Pan-STARRS1 (Pan-STARRS1) telescope. We measured the Pan-STARRS1's catastrophic disruption detection efficiency over a 453-day interval using the Pan-STARRS moving object processing system (MOPS) and a simple model for the catastrophic disruption event's photometric behavior in a small aperture centered on the catastrophic disruption event. Our simplistic catastrophic disruption model suggests that delta m = 20 mag and 0.01 mag d-1 < tau < 0.1 mag d-1 which would imply that H0 = 28 -- strongly inconsistent with H0,B2005 = 23.26 +/- 0.02 predicted by Bottke et al. (2005) using purely collisional models. We postulate that the solution to the discrepancy is that > 99% of main belt catastrophic disruptions in the size range to which this study was sensitive (100 m) are not impact-generated, but are instead due to fainter rotational breakups, of which the recent discoveries of disrupted asteroids P/2013 P5 and P/2013 R3 are probable examples. We estimate that current and upcoming asteroid surveys may discover up to 10 catastrophic disruptions/year brighter than V = 18.5.Comment: 61 Pages, 10 Figures, 3 Table

On-chip two-octave supercontinuum generation by enhancing self-steepening of optical pulses

Dramatic advances in supercontinuum generation have been made recently using photonic crystal fibers, but it is quite challenging to obtain an octave-spanning supercontinuum on a chip, partially because of strong dispersion in high-index-contrast nonlinear integrated waveguides. We show by simulation that extremely flat and low dispersion can be achieved in silicon nitride slot waveguides over a wavelength band of 500 nm. Different from previously reported supercontinua that were generated either by higher-order soliton fission in anomalous dispersion regime or by self phase modulation in normal dispersion regime, a two-octave supercontinuum from 630 to 2650 nm (360 THz in total) can be generated by greatly enhancing self-steepening in nonlinear pulse propagation in almost zero dispersion regime, when an optical shock as short as 3 fs is formed, which enables on-chip ultra-wide-band applications