Enacting a Culture of Access in Our Conference Spaces

The article offers information on periodical\u27s rhetoric and writing studies conference held in September 2020. Topics discussed include prioritizing access in the service of love, justice, connection and liberation; proposing expansive frameworks for access in designing accessible writing classrooms and professional events; and major principles of definition of access, which reflect access\u27s complexity and liberatory potential such as dynamic, relational and intersectional

A chemical survey of exoplanets with ARIEL

Thousands of exoplanets have now been discovered with a huge range of masses, sizes and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host star. However, the essential nature of these exoplanets remains largely mysterious: there is no known, discernible pattern linking the presence, size, or orbital parameters of a planet to the nature of its parent star. We have little idea whether the chemistry of a planet is linked to its formation environment, or whether the type of host star drives the physics and chemistry of the planet’s birth, and evolution. ARIEL was conceived to observe a large number (~1000) of transiting planets for statistical understanding, including gas giants, Neptunes, super-Earths and Earth-size planets around a range of host star types using transit spectroscopy in the 1.25–7.8 μm spectral range and multiple narrow-band photometry in the optical. ARIEL will focus on warm and hot planets to take advantage of their well-mixed atmospheres which should show minimal condensation and sequestration of high-Z materials compared to their colder Solar System siblings. Said warm and hot atmospheres are expected to be more representative of the planetary bulk composition. Observations of these warm/hot exoplanets, and in particular of their elemental composition (especially C, O, N, S, Si), will allow the understanding of the early stages of planetary and atmospheric formation during the nebular phase and the following few million years. ARIEL will thus provide a representative picture of the chemical nature of the exoplanets and relate this directly to the type and chemical environment of the host star. ARIEL is designed as a dedicated survey mission for combined-light spectroscopy, capable of observing a large and well-defined planet sample within its 4-year mission lifetime. Transit, eclipse and phase-curve spectroscopy methods, whereby the signal from the star and planet are differentiated using knowledge of the planetary ephemerides, allow us to measure atmospheric signals from the planet at levels of 10–100 part per million (ppm) relative to the star and, given the bright nature of targets, also allows more sophisticated techniques, such as eclipse mapping, to give a deeper insight into the nature of the atmosphere. These types of observations require a stable payload and satellite platform with broad, instantaneous wavelength coverage to detect many molecular species, probe the thermal structure, identify clouds and monitor the stellar activity. The wavelength range proposed covers all the expected major atmospheric gases from e.g. H2O, CO2, CH4 NH3, HCN, H2S through to the more exotic metallic compounds, such as TiO, VO, and condensed species. Simulations of ARIEL performance in conducting exoplanet surveys have been performed – using conservative estimates of mission performance and a full model of all significant noise sources in the measurement – using a list of potential ARIEL targets that incorporates the latest available exoplanet statistics. The conclusion at the end of the Phase A study, is that ARIEL – in line with the stated mission objectives – will be able to observe about 1000 exoplanets depending on the details of the adopted survey strategy, thus confirming the feasibility of the main science objectives.Peer reviewedFinal Published versio

Disclosure of Mental Disability by College and University Faculty: The Negotiation of Accommodations, Supports, and Barriers

High-profile shootings and student suicides have made mental health issues on college campuses a major national issue. College students are usually the focus of this conversation, while little attention beyond anecdotal accounts has been paid to faculty with mental health issues. In response to this lack of broad-scale research, a first-of-its-kind cross-institutional survey of faculty with mental disabilities was conducted. Respondents self-identified as faculty with mental disabilities, mental illness or mental-health histories. Results from 267 respondents indicated that nearly 70% had no or limited familiarity with accommodations, and even fewer used them (87%). A majority of respondents (62%) disclosed to at least one person on campus, primarily colleagues (50%) and department chairs (21%). Respondents felt most supported by spouses/significant others (75% very or extremely supported) and friends (51%) rather than colleagues (29%) and supervisors (25%). In our discussion of these findings, we offer suggestions for practice that will improve environments, rather than focusing on case-by-case "fixes" for those who disclose. We also suggest directions for further research into this topic, which is frequently mentioned (in both scholarly and popular publications) but rarely investigated systematically or on a wide scale