15-E 24: Cultivating Consciousness: Exploring and Relating Carnivorous Plant Awareness and Preservation Preferences

poster Cultivating Consciousness: Exploring and Relating Carnivorous Plant Awareness and Preservation Preferences

Students: Khush Birjoo Mistry and Andrew Thomas Payne Bauer

Advisor: Dr. Megan Van Etten

Carnivorous plants come from a very exotic plant family with immense diversity and unique characteristics. These plants reside in multiple biomes worldwide, ranging from arid to tropical regions. Despite their impactful effect on the environment, they have been endangered for the past decades due to the rising levels of global warming and human interferences. Human preferences and awareness greatly contribute towards the frequency of carnivorous plants around the world. In this study, data was collected from students and faculty around the Penn State Scranton campus to obtain a consensus on the awareness and preferences towards the preservation of carnivorous plants. A survey was designed using carnivorous and non-carnivorous plant images, prompting individuals to prefer one plant over the other and to analysis carnivore plant awareness in the general population. Data gathered from the survey suggested that a significant amount of the population was able to recognize a carnivorous plant from a non-carnivorous plant, despite most of the population preferring a non-carnivorous plant over a carnivorous plant. Regarding preservation of carnivorous plants, a significant number of respondents agreed on the ecological importance of carnivorous plants. In conclusion the data suggests that despite majority of general population considering carnivorous plants to be threatening and uncomfortable, a high number of individuals believe in the preservation of these plants based on their ecological importance rather than their aesthetic appearance.

10-E 24: Competition in Plant Populations Affects How Plants Respond to Temperature Increase

poster display 10-E 24: Competition in Plant Populations Can Benefit How Plants Respond to Temperature Increase

Student: Cameron Zynel

Advisor: Dr. Megan Van Etten

Plants are incredibly important – humans rely on plants for vital food sources, medicines, and other consumer goods and plants play a key role in nearly all ecological processes. Climate change has the potential to have drastic negative effects on plants and therefore all life on this planet. While numerous studies have documented the negative effect of increased temperatures, this is not the only stress that plants must deal with, which could exacerbate the negative effect of temperature. To address this gap, I examined how increased temperature along with increased competition, can affect the growth of plants, specifically the Fast plant (Brassica rapa). Competition decreased plant height rate and leaf size while increased temperature led to taller plants but smaller leaves. These results suggest that both temperature and competition affect plant growth, which could have potential repercussions, particularly in agriculture where competition is often very high.

9-E 24: Plants are in for a Root Awakening when Temperatures Rise

Poster display 9-E 24: Plants are in for a Root Awakening when Temperatures Rise

Student: Amanda Delhagen

Advisor: Dr. Megan Van Etten

Rising temperatures due to climate change are projected to increase the average global surface temperature by 4.8°C by 2100 without mitigation efforts. Effects of elevated temperatures on plant traits like nutrient absorption and flowering time have been studied, but root development has received less attention despite the vital role roots play in nutrient and water uptake, and structure. This study investigated the impact of an elevated temperature of 76°F compared to the control at 68°F on root and above ground growth in Brassica rapa. The results showed that the higher temperature treatment stimulated a greater number of root branches, earlier flowering, and larger leaves. These findings show how root development is likely to be significantly impacted by rising temperatures.

7-E Exploring Differences in Tick Prevalence and Intensity Among Migratory Songbird Species in Northeastern Pennsylvania

First Place Empirical Categorygold medal

decorativeUniversity Libraries’ Excellence in Information Literacy Awardee

Student: Morgana CostanzoPoster display of 7-E Exploring Differences in Tick Prevalence and Intensity Among Migratory Songbird Species in Northeastern Pennsylvania

Advisor: Dr. Meg Hatch and Dr. Robert Smith

Studying how different species affect tick infestation is crucial for managing tick-borne diseases and ecosystem health because understanding these interactions can help identify key species that contribute to the abundance of tick populations. We examined the presence or absence of ticks (Ixodes) on the heads and mandibles of songbirds captured at Lackawanna State Park in Lackawanna County, PA. We were interested in whether there was a relationship between bird species and number of ticks present. Of the 12 species examined, there was a significant relationship between tick prevalence and species, with American Robins (Turdus migratorius), Common Yellow Throats (Geothlypis trichas), Eastern Towhees (Pipilo erythrophthalmus), and Wood Thrushes (Hylocichla mustelina) differing significantly than the other species examined. There were also four species on which no ticks were observed. Among two bird species with a considerable number of captures, there was no seasonal difference in tick intensity. Our study contributes to others that found differences in tick prevalence among various species of songbirds and may contribute to the further understanding of tick-borne diseases in birds.

Key Words: migratory songbirds, tick prevalence, tick intensity, species differences, parasitology, avian ecology.

4-E 24: Observing Sunspots with the Scranton Campus Solar Telescopes

decorativeUniversity Libraries’ Excellence in Information Literacy Awardee

Student: Ceiwynn Longworth

Poster Observing Sunspots with the Scranton Campus Solar Telescopes
Advisor: Dr. Mario Freamat, Dr. Agnès Kim
Sunspots are dark regions that appear on the sun’s surface and are a significant part of the solar activity. They are concentrations of the sun’s magnetic field that prevent some of the heat produced in the solar core from reaching the surface, thus creating a darker appearance due to the lower temperatures. The sun goes through an 11-year solar cycle, through which the sunspots will wax and wane and migrate to the sun’s equator. Sunspots impact Earth’s magnetosphere, causing magnetic storms and disrupting power grids, so the study of sunspots goes beyond the interest in solar activity. It is a matter of societal concern. In this context, we prepared and enhanced our two campus telescopes. We used them to take images of the sun, observe and characterize the visible sunspots (given the local conditions and equipment limitations), and contrast our observations with published science. In this poster, we share our images and the preliminary analysis of our observations. We also hope to inspire interest in solar activity amongst other students.

3-E 24: The Differences of Mechanisms in High-Mass X-Ray Binary Pulsars and Magnetars

poster The Differences of Mechanisms in High-Mass X-Ray Binary Pulsars and Magnetars

Student: Holden Kersey

Advisor: Dr. Asif ud-Doula

High-Mass X-Ray Binary pulsars (HMXB pulsars) are fast-moving, magnetized neutron stars in a binary orbit alongside a companion star, wherein X-Rays are emitted from their magnetic poles. These X-rays are generated when the neutron star accretes material from its companion and magnetic field deflects it to its poles. Magnetars are also neutron stars, but they are highly magnetized and slower-moving. What sets magnetars apart from normal neutron stars is the strength of their magnetic field which can be of the order of 10^9T-10^15G making them the most powerful known magnets in the universe. The aim of this project is to show how HMXB pulsars and magnetars differ from each other. We examined two catalogues containing HMXB pulsars (Kim et al. 2023) and magnetars (Olausen & Kaspi, 2014) and extracted data which empirically tell us about their characteristics such as the period, rate of change of period, magnetic field, and luminosity. Our results show the differences between the accretion-powered HMXB pulsars and electromagnetic-powered magnetars.

1-E 24: Violations of Kepler’s Third Law Among Exoplanet Types

silver medalSecond Place Empirical Category

Students: Sadid Hassan, CJ Dunham
POSTER IMAGE Violations of Kepler’s Third Law Among Exoplanet Types

Advisor: Dr. Asif ud-Doula, Dr. Gillian Pearce

Currently, exoplanets are classified into four different categories based on their size: terrestrial, super-earth, Neptunian, and Gas Giants. According to Kepler’s Third Law of planetary motion, the squares of the orbital periods of these planets are directly
proportional to the cubes of the semi-major axes of their orbits. The understand the factors that could cause a divergence from the relationship, and whether those differences are a trend in that particular exoplanet type. It is expected that exoplanetary systems will follow Kepler’s Third Law if: 1. the exoplanets are much less massive than the parent star, 2. gravitational influence between the planets is not significant, 3. the stellar system is clear of dust and debris, and 4. the system does not contain multiple stars. Our preliminary results show that there are several systems of exoplanets that deviate from such Kepler’s Third Law with majority being among the terrestrial type.
Further, this research aims to explore the factors that could cause this shift, whether it be experimental errors or the existence of a hidden celestial body in the planetary system influencing the orbit of a particular planet.