The 3.4 micrometer emission feature in Comet Halley

Several teams of ground based observers reported observations of the emission feature centered at 3.36 micrometers in comet Halley following its discovery by the Vega 1 spacecraft. The position and shape of the band indicate a superposition of emissions by C-H groups. But the mechanism for the excitation of these C-H3 groups is still not agreed upon. Three possibilities are summarized. Elucidation of the emission mechanism is needed to determine whether the source is predominately solid or gas. In addition, is it shown that the derived carbon abundance in Halley depends strongly on the assumed mechanism

Comparison of the 3.36 micrometer feature to the ISM

It has been noted that the 3.36 micrometer emission feature is not the same as that of any ISM band at 3.4 micrometer. This is documented herein. There is no convincing analog to the cometary 3.36 micrometer emission feature seen in the Interstellar Matter band. This fact suggests that if the carbonaceous material in comets came from the ISM, it was either further processed in the solar nebula or has a different appearance because of the different excitation environment of the sun and ISM

The near-infrared polarization and color of Comet Halley: What can we learn about the grains

The near infrared polarization and JHK colors of light scattered by dust grains in comet Halley were measured over a wide range in phase angle and heliocentric distance. Colors were redder than solar with no statistically significant variation with phase angle, heliocentric distance, or pre- and post-perihelion. This suggests that the grain population did not change drastically over time and that the data may be combined and modeled. However, short term variations in visible polarization and dust albedo were seen in Halley. Also, near infrared colors became systematically bluer after the observations were completed. The near infrared colors of Halley fall in the range of those of other comets. The near infrared polarization is similar to the visible polarization of Halley and other comets in showing a negative branch at small phase angles and an approximately linear rise toward positive values at larger phase angles. Mie theory calculations and a size distribution based on spacecraft data were used to model the near infrared polarization and color of comet Halley. Numerous lines of evidence point to the presence of dark, absorbing, probably carbonaceous materials in comets

Love And Education In Plato\u27s Symposium

This paper seeks to illuminate the significance of Socrates\u27 entrance into a series of speeches by exploring the connection between love and learning in Plato\u27s Symposium. We begin by presenting historical and social contexts relevant to the dialogue and its author. We then turn to the dialogue, outlining the fundamental components of each speech and, moreover, analyzing each speech with the aim of eliciting educational implications which are later highlighted and expanded on by Socrates. We examine these pedagogical connotations through a thorough investigation of each speech, keeping a keen eye on Socrates. We approach our examination of Socrates’ speech in two key ways. The first is to examine how the educational implications found within the earlier speeches are later acknowledged and expanded on by Socrates. Furthermore, we also examine the way in which Socrates forms careful alterations of the previous speakers’ assertations to provide them with new meanings. Second, we examine Socrates\u27 approach in contrast with the prior speeches. In our examination of Socrates’ speech, we find that the structure of Socrates\u27 speech sharply contrasts with the overall narrative formatting of the prior speeches and the dialogue as a whole. We argue that Plato deliberately emphasizes Socrates\u27 approach by constructing a structure that contrasts with previous speeches. For further support of our interpretation, we turn to additional Platonic dialogues with the intent of gaining further insight into his educational approach.https://scholarworks.moreheadstate.edu/celebration_posters_2022/1029/thumbnail.jp

A "Starless" Core that Isn't: Detection of a Source in the L1014 Dense Core with the Spitzer Space Telescope

We present observations of L1014, a dense core in the Cygnus region previously thought to be starless, but data from the Spitzer Space Telescope show the presence of an embedded source. We propose a model for this source that includes a cold core, heated by the interstellar radiation field, and a low-luminosity internal source. The low luminosity of the internal source suggests a substellar object. If L1014 is representative, other "starless" cores may turn out to harbor central sources

Hydrologic Influences Within a Tidal Freshwater Forested Wetland

2012 S.C. Water Resources Conference - Exploring Opportunities for Collaborative Water Research, Policy and Managemen

Hydric conditions during incubation influence phenotypes of neonatal reptiles in the field

Phenotypic variation is strongly impacted by environmental conditions experienced during development. Substantial laboratory research has shown that reptiles with flexible-shelled eggs are particularly sensitive to hydric conditions, yet research on nests in the wild is sparse. In this 2-year field experiment, we explore the influence of hydric conditions during incubation on phenotypic traits of hatchling painted turtles (Chrysemys picta). Using a split-clutch design, we created two artificial nests adjacent to each maternally selected nest site. Half the eggs incubated in a nest that received regular supplemental watering, while the control nest was exposed to natural precipitation only. Our results suggest that the influence of the hydric environment on developing reptilian embryos is context dependent. Supplemental water applied to nests in a drier than normal season elicited the expected biotic responses, based on laboratory experiments. However, when the soil surrounding C. picta eggs was already highly moist, the additional water from supplemental application effectively stunted embryonic development. Our experiment confirms that hydric conditions of the soil during incubation in the wild can substantially influence phenotypic variation of reptiles with flexible-shelled eggs. Additionally, our experiment highlights the importance of complex interactions in the field that are often unexplored in laboratory experiments, reiterating the importance of validating laboratory work with field experiments

Spitzer Space Telescope Spectroscopy of Ices toward Low-Mass Embedded Protostars

Sensitive 5-38 μm Spitzer Space Telescope and ground-based 3-5 μm spectra of the embedded low-mass protostars B5 IRS1 and HH 46 IRS show deep ice absorption bands superposed on steeply rising mid-infrared continua. The ices likely originate in the circumstellar envelopes. The CO_2 bending mode at 15 μm is a particularly powerful tracer of the ice composition and processing history. Toward these protostars, this band shows little evidence for thermal processing at temperatures above 50 K. Signatures of lower temperature processing are present in the CO and OCN^- bands, however. The observed CO2 profile indicates an intimate mixture with H_(2)O, but not necessarily with CH_(3)OH, in contrast to some high-mass protostars. This is consistent with the low CH_(3)OH abundance derived from the ground-based L-band spectra. The CO_2 : H_(2)O column density ratios are high in both B5 IRS1 and HH 46 IRS (~35%). Clearly, the Spitzer spectra are essential for studying ice evolution in low-mass protostellar environments and for eventually determining the relation between interstellar and solar system ices