2024 Student Research Symposium Program

2024 Student Research Symposium Banner

The 2024 MDSGC Student Research Symposium was held on Friday, August 2, beginning at 8 a.m. EDT. The venue was the Mt. Washington Conference Center in Baltimore, MD. For GPS navigation, aim for “Johns Hopkins At Mt. Washington, Smith Avenue, Baltimore, MD” (link) and park in the nearby visitor parking lot/garage. Here is an image from Google showing the relative locations of parking and the conference venue:

Annotated google image showing visitor parking and conference venue relative locations.

This year’s symposium showcased presentations by student interns and researchers working at sites across Maryland. The cohort of presenters represented diverse institutions, including: Capitol Technology University, Hagerstown Community College, Morgan State University, NASA, Towson University, University of Maryland Baltimore County, University of Maryland College Park, and University of Maryland Eastern Shore.

The program follows.

2024 MDSGC Student Research Symposium

8:00 a.m.
Registration opens.

8:00 – 9:00 a.m.
Poster setup and networking. Breakfast provided.

9:00 – 10:20 a.m.
Oral Presentation Session 1.

10:20 – 10:30 a.m.
Group Photos.

10:30 – 11:30 a.m.
Poster Session.

11:30 – 12:55 p.m.
Oral Presentation Session 2.

12:55 – 2:00 p.m.
Lunch and small group discussion.

Oral Presentation Session 1, 9:00 – 10:20 a.m.

9:00 a.m.
Welcome and Introductory Remarks — Dr. Matt Collinge, MDSGC Deputy Director

9:10 a.m.
Launching Dreams: The Impact of Space Grant on My Career and Future Aspirations — Saimah Siddiqui (UMCP/JHU)

Saimah Siddiqui graduated in May 2024 with bachelor’s degrees in Aerospace Engineering and Mathematics from the University of Maryland, College Park. Her academic journey was notably shaped by her involvement in the Space Grant program, where she served as the Senior Launch Director for the Balloon Payload Program (BPP). This role provided her with invaluable hands-on experience and technical skills in aerospace technology.

Currently, Saimah is preparing to pursue a Master’s degree in Space Systems Engineering at Johns Hopkins University. With a strong foundation built through her recent education and leadership experiences in the Space Grant program, she is eager to advance her expertise and contribute to the field of space exploration and technological innovation.

9:40 a.m.
Sustainable Lunar Agriculture: Assessing the Impacts of Two Different Types of Lunar Regolith Simulant on Crop Growth — Leon Kelly (Duke/UMES)

The objectives of NASA’s Artemis project are to “Go, Land, Live, and Explore,” representing a comprehensive approach to lunar exploration. “Go” is launching missions to the Moon, “Land” is safely landing astronauts, “Live” is establishing sustainable living conditions, and “Explore” is conducting scientific investigations to expand human presence on the Moon. To achieve “Live,” a lunar settlement must sustain itself to support ongoing exploration. Our project addresses the challenges of sustaining astronauts by examining the growth of food crops on lunar regolith simulants using space-saving technologies such as aeroponics (growing plants without soil, in which the roots are suspended in the air and misted with a nutrient-rich water solution) and farmbot (an open-source farming technology that combines robotics, automation, and software to facilitate precision farming in small-scale agricultural settings) for plant cultivation. In addition, we investigated the effects of two types of lunar regolith simulants: Lunar Highland Simulant 1 (LHS-1) and Mexico Lunar Mare 1 (MLM-1) on the growth of spinach (Spinacia oleracea) and kale (Brassica oleracea), utilizing various mixtures of regolith simulants infused with horse manure under controlled conditions of light and water. Our findings revealed that higher concentrations of regolith simulants supported better plant growth that could be attributed to the growing layer of yellowish-green lichen, Rhizocarpon geographicum, a symbiotic organism composed of a fungus and an alga. This study highlights the potential of regolith-based substrates and symbiotic organisms to support crop cultivation in the lunar environment.

9:50 a.m.
Articulated Lunar Rover Project — Zoé Denito (CTU/UMCP)

During the internship at University of Maryland College Park we created an Articulating Rover as a “body” or testbed for the BIG Ideas project and future projects. The BIG Ideas project is a program where students work with NASA to create innovative and groundbreaking projects. They are currently designing wheels for the Lunar and Martian rover(s), using CAD and testing wheels for traction along with an inflatable devicel, with grousers, to help the rover cover more ground. The Articulating Lunar Rover (Luna) consists of two boxes and rotating joints made of aluminum, 3D printed Models of the BIG Ideas inflatable wheel designs, and a circuit to actuate the wheels. The Arduino Uno is the main part of the circuit which is connected to a joystick (which is tethered to the Rover), and four motors for rotating the wheels. The process of building the project is very rewarding, even though there were some time constraints and limited resources, we gained a lot of experience in programming with an Arduino, and circuitry.

10:00 a.m.
Evaluation of Precipitation Phase Algorithms in Southern New England — Connor Mahone (UMBC/NASA)

Precipitation’s global distribution, anomaly, and extremes are fundamental in nature. There are three sequential questions to determine the precipitation climatology: Is it precipitating? What is the phase of the precipitation? What is the amount of precipitation? The response to these three questions comes with uncertainty.  The oceans cover over 70% of Earth’s surface, therefore satellite-based precipitation products are the sole source of global precipitation mapping. NASA’s gauge-adjusted multi-satellite product, IMERG, has been operated and funded by the  Global Precipitation Measurement (GPM) mission and is the most used precipitation product globally.  The poor coverage of ground-based precipitation measurements across the land surface is one of the key reasons for the high demand for external precipitation resources.  NOAA’s Multi-Radar Multi-Sensor (MRMS) with high spatial and temporal resolution precipitation mapping using national weather radar and multiple gauge platforms, was adopted by the GPM program as a validation product for satellite-based precipitation estimates from IMERG. 

Both IMERG and MRMS have their own precipitation phase algorithms.  MRMS’s deterministic algorithm relies on High-Resolution Rapid Refresh (HRRR) air and wet-bulb temperature forecast, while IMERG’s probabilistic algorithm uses European Reanalysis (ERA5) wet-bulb estimates.  This study aims to evaluate these two algorithms utilizing data from a three-winter-long field campaign in Connecticut.  The campaign included an All-In-One (AIO) weather station, laser-optical PARSIVEL disdrometer, Precipitation Imaging Package (PIP), and Micro-Rain-Radar (MRR) among other instruments.   MRMS and IMERG algorithms utilizing the AIO temperatures are used as references.  MRMS and IMERG algorithms utilizing HRRR, ERA5, and NASA’s global modeling and assimilation office (MERRA-2) reanalysis have been evaluated. The phase algorithms of particle size and fall velocity-based PARSIVEL, PIP-derived and MRR-measured Doppler fall speed, and PIP-based bulk and equivalent density provided independent resources for the evaluation of MRMS and IMERG algorithms.   The study focused on phase transition events but also included snow events.

10:10 a.m.
Poster Flash Talks

      • Exploration of Emergent Technologies In Sustainable Lunar Agricultural Engineering — Alena Zheng (UMCP/UMES)
      • Thermal Analysis of the Nancy Grace Roman Space Telescope — Francesca Sciarretta (UMCP/NASA)
      • NASA Human Exploration Rover Challenge (HERC) — Ismail Shah (Oxon Hill HS)
      • Diamagnetic Loop Diagnostics in CMFX — Justin James (HCC/UMCP)
      • Articulated/Segmented Body Lunar Rover with Pivoting Joints — Danny Puwo (UMES/UMCP)
      • Evaluation of Precipitation Amount Products in Mid-Atlantic and Southern New England — Amalie Rebstock (UMBC/NASA)
      • Radiative Cooling Properties in Cellulose Materials — Bryan Yang (UMBC/UMES)
      • New Insulators and Mechanical Supports to Prevent Arcing in CMFX — Ismail Aadan (UMCP)
      • Design of an Arc Chamber for Plasma Impedance Matching — Makai Martin (UMES/UMBC)

Group Photos, 10:20-10:30 a.m.

Poster Session, 10:30 a.m. – 11:30 a.m.

Exploration of Emergent Technologies In Sustainable Lunar Agricultural Engineering — Alena Zheng (UMCP/UMES)

Smart agriculture employs advanced technologies to improve the productivity and quality of crops while simultaneously reducing labor with autonomous systems. FarmBot, an open-source robotic farming device, can be programmed to assist with planting, watering, and weeding. This advanced agricultural machinery has applications extending beyond Earth to potential space agricultural settings. Our project involves a focus on utilizing the watering aspect of the FarmBot to sustain our set-up of growing spinach with two lunar regolith simulant soils of varying concentrations. The spinach (Spinacia oleracea) plants exhibited the best growth, as indicated by the largest leaf widths, in the 75% regolith simulant concentrations for both types of simulants. This is determined to be due to the appearance of crustose lichen (Rhizocarpon geographicum) in these containers. Another avenue of space farming exploration includes aeroponics, a soil-less growing technique where roots are suspended in air and misted with nutrient-rich water. We are using a Tower Garden, a vertical aeroponic growing apparatus, to test the benefits of aeroponics. Both the FarmBot and Tower Garden are vital, accessible tools with the potential to revolutionize the future of farming from Earth to the Moon. (Click image for full size.)

Thermal Analysis of the Nancy Grace Roman Space Telescope — Francesca Sciarretta (UMCP/NASA)

The Nancy Grace Roman Space Telescope (RST) is a NASA observatory that will be stationed in Lagrange Point 2 (L2) orbit, where it will provide us with a panoramic view of the universe, helping to investigate dark matter and exoplanets. During my internship at NASA’s Goddard Space Flight Center (GSFC), I worked on RST’s High Gain Antenna System (HGAS) and performed a trade study on the effects of the effective emissivity (ε*) of multilayer insulation on the Ground Station Equipment (GSE). My work regarding HGAS will be compiled into a test report, and my trade study findings will lead to the verification of RST’s GSE heater performance, both of which are crucial to the overall mission. (Click image for full size.)

Thumbnail image of Francesca's poster about Thermal Analysis of the Roman Space Telescope.

NASA Human Exploration Rover Challenge (HERC) — Ismail Shah, Emmanuel Castillo, Elda Berhaneyessus, Michael Perez, Lareon Brent III, Hannah Magruder (Oxon Hill HS)

This project focussed on designing and optimizing a vehicle capable of traversing the Moon or Mars terrain, allowing the astronauts to travel further distances before running out of oxygen. The aim was to provide a means of transportation for up to 2 passengers to safely get around on the moon without the assistance of electrical power. The vehicle needed to be omitted from the use of electricity in the case of power failure on the base. One critical flaw during a power outage would be a lack of transportation required for the astronauts to get around the base and solve the electrical issue. Therefore our challenge was to develop a rover capable of transporting two astronauts around the slopes and undulating terrain to navigate to the task sites and complete a mission. This entire project was entered into the NASA HERC competition where the project was tested to determine if the vehicle was successful or not. (Click image for full size.)

Thumbnail image of NASA HERC poster by students from Oxon Hill HS.

Diamagnetic Loop Diagnostics in CMFX — Justin James (HCC/UMCP)

The Centrifugal Mirror Fusion Experiment (CMFX) harnesses azimuthal rotation of plasma through an ExB drift caused by an imposed radial electric field to enhance plasma confinement within a magnetic mirror.  The centrifugal forces caused by the rotation of the plasma, also change the total magnetic flux of the mirror. Four Diamagnetic Loops (DML) are wound around the outer wall of the vacuum vessel to measure these flux changes caused by the changing magnetic field. The voltage induced in the DMLs from the changing flux is then numerically integrated to obtain the magnetic flux. The magnetic field derived from the measured flux changes is used to estimate plasma density and assess plasma stability.  Integration, filtering, and detrending of this data is necessary to obtain useful signals when high amplitude noise is present. Because of this noise, new DMLs were constructed with an increased number of turns. Each DML contains 4 turns and is constructed from 18 AWG copper wire.  Cables are then attached to measure the induced voltage in the loops which is then sent to a digitizer for analysis.  RF-shielding foil covers the DML windings to reduce the pick-up of electromagnetic noise.  Details of the DMLs,  processing algorithms, and sample data are presented. (Click image for full size.)

Thumbnail image of CMFX poster by Justin James.

Articulated/Segmented Body Lunar Rover with Pivoting Joints — Danny Puwo (UMES/UMCP)

During the internship at University of Maryland College Park we created an Articulating Rover as a “body” or testbed for the BIG Ideas project and future projects. The BIG Ideas project is a program where students work with NASA to create innovative and groundbreaking projects. They are currently designing wheels for the Lunar and Martian rover(s), using CAD and testing wheels for traction along with an inflatable devicel, with grousers, to help the rover cover more ground. The Articulating Lunar Rover (Luna) consists of two boxes and rotating joints made of aluminum, 3D printed Models of the BIG Ideas inflatable wheel designs, and a circuit to actuate the wheels. The Arduino Uno is the main part of the circuit which is connected to a joystick (which is tethered to the Rover), and four motors for rotating the wheels. The process of building the project is very rewarding, even though there were some time constraints and limited resources, we gained a lot of experience in programming with an Arduino, and circuitry. (Click image for full size.)

Evaluation of Precipitation Amount Products in Mid-Atlantic and Southern New England — Amalie Rebstock (UMBC/NASA)

 Precipitation is a driving force for the water cycle and is one of the key sources of weather extremes. The changing global climate and consequent increase in extreme weather causes life to become more reliant on precipitation. The drought in Maryland is evident, as only 48 mm (1.9”) of rainfall fell during the first 50 days of Summer 2024.This information is based on a gauge report at Baltimore Washington International airport. Unfortunately, most of the global land is not equipped with precipitation measuring devices. This is due to topography, land use coverage, cost, and remoteness. With the addition of global ocean coverage (>70%), precipitation climatology relies on spaceborne precipitation retrievals and model outputs. NASA’s multi-satellite product, IMERG, operated and funded by the Global Precipitation Measurement (GPM) mission, is widely used in scientific research and operational applications. The NOAA’s Multi-Radar Multi-Sensor (MRMS) product has been widely employed to validate satellite and model precipitation estimates among many other applications. 

The GPM ground validation program has been deploying Platforms for In situ Estimation Rainfall Systems (PIERS) at granted institutes across the US. This study uses six PIERS+ sites which include a PARSIVEL disdrometer and tipping bucket gauges. The sites are located in the Mid-Atlantic region with an additional site in Connecticut. Some sites have additional instrumentation, including Pluvio weighing bucket gauge, additional tipping buckets, and additional PARSIVEL disdrometers. The study focuses on event rainfall totals for January to May 2024. The PARSIVEL disdrometer was the reference for the event definition and phase identification, while its rainfall totals compared to the gauges to determine the reference instrument. In addition to MRMS, the performance of the NOAA’s HRRR model, European ERA5 reanalysis, NASA’s MERRA-2 reanalysis were evaluated through comparison to the reference instrument. Future study will be conducted once IMERG data is available. (Click image for full size.)

Thumbnail image of Amalie Rebstock poster about Evaluation of Precipitation Amount Products.

Radiative Cooling Properties in Cellulose Materials — Bryan Yang (UMBC/UMES)

Radiative cooling properties in certain materials have the potential to reduce the urban heat island effect if applied at scale. An ideal passively cooling material should exhibit properties such that they are simultaneously high in solar reflectance whilst being effective at longwave infrared heat transfer through the atmospheric infrared window. Such properties effectively allow the material to cool passively without consuming electricity. Here, we explore the passive cooling capabilities of various cellulose composites by improving upon an existing experimental setup to determine their cooling power more reliably. (Click image for full size.)

Thumbnail image of Bryan Yang poster about Radiative Cooling Properties in Cellulose Materials

New Insulators and Mechanical Supports to Prevent Arcing in CMFX — Ismail Aadan (UMCP)

The Centrifugal Mirror Fusion Experiment (CMFX) vacuum chamber experiences electric arcing when enough deuterium becomes trapped on surfaces behind the insulator. The effects of arcing on the plasma include lowering the insulating voltage and damage to the limiter electrodes. To minimize the migration of gas behind the insulator, a new insulator design is being implemented. Another improvement to CMFX by this design is the use of machinable ceramic (Macor) for the supports which will provide an electrically neutral material that will provide additional insulation and prevent electric shorting to the ends of the chamber. (Click image for full size.)

Thumbnail of Ismail Aadan poster about preventing arcing in CMFX

Design of an Arc Chamber for Plasma Impedance Matching — Makai Martin (UMES/UMBC)

A device for plasma impedance matching is being designed in the Dusty Plasma Laboratory (DPL) at the University of Maryland, Baltimore County (UMBC). The design consists of a high voltage tube modified to allow safe arcing between transmission lines. The distance between wires must be variable to millimeter or better accuracy while maintaining the insulating properties of the high voltage tube. Mechanisms are explored as methods to facilitate the required variable impedance. (Click image for full size.)

Thumbnail of Makai Martin poster about Design of an Arc Chamber for Plasma Impedance Matching

Oral Presentation Session 2, 11:30 – 12:55 p.m.

11:30 a.m.
Reconvene in presentation room

11:30 a.m.
Artemis Inspired Robotic Sensory Platforms to Advance Creativity and Engage Students — Anubhav Dixit (UMCP/UMES)

This summer internship project was undertaken at the University of Maryland Eastern Shore (UMES) under the auspices of synergistic projects titled AIRSPACES (Autonomous Instrumented Robotic Sensory Platforms to Advance Creativity and Engage Students) and DREAM (Developing Robotic Exploration with Agrobots and Moonbots) ongoing at the university funded by Maryland Space Grant and NASA-MSTAR program respectively. Autonomous navigation and artificial intelligence integration with the recently acquired Agilex Limo 4-wheeled multi-modal mobile robot equipped with various navigational sensors including LiDAR and stereo depth camera was the primary focus of the project efforts outlined. Limo works with open-source ROS and the Gazebo simulator allowing access to significant reserves of robotic application development capabilities both in virtual and physical domains providing a rich educational and research platform. A specially designed simulation table was also utilized to simplify the process of testing model applications.

11:40 a.m.
Multiplex Visibility Graphs for Neural Time Series Analysis — Arya Teymourlouei (UMCP)

Understanding the neural mechanisms associated with cognitive functions such as problem solving and decision making is crucial to the development of a human systems integrative architecture for long-term spaceflight missions. Such neural mechanisms are characterized by unique patterns of communication between brain regions. Therefore, we require robust methods for identifying the level of interaction between the neural activity recorded from different cortical locations (as EEG time series signals). While existing approaches do exist, they may not be enough to provide adequate insight. In this research, we evaluate a new method which is based on computing the similarity between graphs formed from the time series themselves (from a notion of visibility between data points). Initial results suggest that our method is an improvement over some existing approaches, but further investigation is required.

11:50 a.m.
NAM to RRAT Converter and Azimuth Limits — Mason Eberle (UMCP/NASA)

Flight Safety Analysts require tools to accurately carry out analysis for launches out of Wallops Flight Facility. Overtime, these tools become outdated. This summer internship focused on updating the old excel tools to interactive MATLAB Apps. These apps increase efficiency and allow more detailed risk-based assessment by Safety Analysts.

12:00 p.m.
CFD Nasal Drug Spray Modeling — Cortez Waller (MSU)

Long-duration space missions can lead to numerous upper airway issues for astronauts, potentially impacting their health and mission performance. Nasal drug sprays offer a promising solution to these problems. This project aims to investigate the suitability of over-the-counter nasal drug sprays for use in space. Using Computational Fluid Dynamics (CFD), we will model the droplet transportation of drug sprays under zero gravity conditions to evaluate their effectiveness and behavior in a microgravity environment. Additionally, we will investigate the contributing parameters that can assist in increasing the efficacy of these drug sprays in reaching a target location within the nasal passage. This will allow for an individualized nasal spray delivery system for each astronaut..

12:10 p.m.
Reducing Data and Time Needed to Reconstruct Paths Through Bounding Hulls — Nathan Au (UMBC/UMCP)

Consider autonomous agents in an unknown environment with very limited communication. They must leverage what limited information about the environment they can send to aid in an agent’s objectives. In our project, we explore the use of bounding hulls to reduce the necessary data needed for a sampling-based motion planning algorithm to reconstruct a path in minimal time. We consider three different map types (zig-zag, maze, forest) and the number of vertices in each constructed bounding hull. Our findings indicate that a bounding hull of as low as 4 vertices can significantly reduce the time it takes for another agent to reconstruct a path using RRT*.

12:20 p.m.
Navigating My Naval Academy Internship — Temitayo Adekoya (UMES/USNA)

USNA STEM is an organization that strives to increase the pursuit of STEM-based careers by directly teaching hands-on STEM learning modules to students and teachers alike. I spent my summer observing and helping USNA STEM, learning how hands-on activities can benefit me as a student and an engineer.

12:30 p.m.
Formulating Thermally Insulating Paint — Marwan Attia (UMBC/UMES)

Thermal management is crucial for ensuring the dependability and safety of space exploration missions. The extreme temperature fluctuations encountered during rocket launch, reentry, and in the vacuum of space pose significant risks to the lives of astronauts and the proper functioning of onboard equipment. Without proper thermal insulation, with temperatures exceeding 1600°C during atmospheric passage and plummeting to -270°C in space, the structural integrity of spacecraft is severely compromised. This research explores the potential development of an aerogel-based, novel thermally insulated paint designed to offer superior insulation properties. By reducing material weight and volume to effectively mitigate heat transfer, this innovative coating enhances the survivability of spacecraft. Additionally, the potential applications of this technology extend beyond aerospace, presenting a promising solution to global thermal challenges across various industries.

12:40 p.m.
Design and Optimization of a Liquid Propellant Rocket Nose Cone — Mahki Wimbish (MSU)

This study, conducted at Morgan State University, aims to analyze various nose cones with different lengths, shapes, and materials to determine which variation meets certain apogee, aerodynamic, and structural conditions. These conditions were calculated, modeled, and simulated to exhibit positive behavior during liftoff. The research was supported by the Base 11 award to build a Liquid Propellant Rocket (LPR) in 2020. Before analyzing the cones, familiarity with the software used throughout the study was essential to accurately interpret the results. The software includes OnShape, OpenRocket, and Autodesk Inventor. Initially, OnShape was used to plan the 3D modeling of the cone after gathering the dimensions from simulations. OpenRocket was then used to determine the necessary length, shape, material, and average apogee value by running various simulations with different nose cone configurations. After modeling and simulating the optimal cone variation, an experiment was conducted using Inventor due to its ability to do pressure analysis. The results from this experiment suggest that analyzing various nose cones with different parameters allows for accurate anticipation of rocket deployment, stability, and the ability to reduce aerodynamic drag and control airflow. This study will demonstrate these findings.

12:50 p.m.
Concluding Remarks

Lunch and small group discussions, 12:55 – 2:00 p.m.

MDSGC offers our sincere congratulations to our student presenters, a huge thanks to our internship mentors, collaborators, and supporting staff, and our hope that all attendees enjoyed and learned from these presentations!

April 8, 2024: Solar Eclipse

Image of 2017 solar eclipse. Photo credit: NASA/Bill Ingalls.

On Monday, April 8th, 2024, the Moon crossed in front of the Sun as seen from much of North America, giving millions of Americans another chance to experience a solar eclipse. Like in October 2023 and August 2017, Maryland experienced a partial solar eclipse. During a partial eclipse the Sun is never fully blocked by the Moon. This means that it is never safe to look directly at a partial eclipse without special eye protection — regular sunglasses are not okay! Please see below for more information on safe observing practices.

From Maryland, the beginning of Monday’s eclipse (aka “first contact”) was be at approximately 2:05 p.m. according to timeanddate.com, depending slightly on the viewer’s location. Maximum eclipse depth of approximately 90% coverage occurred at 3:21 p.m. and the show was all over at around 4:30 p.m.

For eclipse watchers in the Baltimore area, a couple of opportunities to come out (or stay in) and see the spectacle were:

Eclipse safety: It is very important not to look at the partial eclipse directly unless you have appropriate eye protection such as special eclipse glasses (NOT regular sunglasses) from a reputable manufacturer. Courtesy of NASA, here is a summary of information about eclipse safety. Key takeaways: either use special eclipse glasses or use an indirect viewing method, such as a projected image from a pinhole camera.

While Maryland experienced only a partial eclipse, a swath of the USA stretching from Texas to New England briefly fell into darkness as the Moon fully covered the Sun, creating the fateful (and amazing) condition known as a total eclipse. The image below shows the approximate locations where this occurred; for more detail see NASA’s Where & When.

Map of continental USA showing the path of totality for the April 8, 2024 solar eclipse.
Map of continental USA showing the path of totality for the April 8, 2024 solar eclipse. Credit: NASA.

To all eclipse watchers, we wish you clear skies!

Observatory Images

The following images are from our main 20-inch telescope using one of two cameras, a ZWO 1600MM Pro or Canon EOS 6D DSLR. Many of these images were acquired by observatory visitors, W. Balmer, and M. Prem, and most post-processing was carried out by M. Prem using SIRIL.

Friday, May 26rd, 2023

Color image of M101 with supernova SN2023ixf
M101: This well-known and lovely spiral galaxy is also known as the pinwheel galaxy due to its large spiral disk being oriented almost directly towards Earth. However, this image shows a very special guest that was not visible in this galaxy just a few short weeks before this image was taken: the core collapse supernova SN 2023ixf (appears as a large light-blue blob in the upper-right). While this supernova will fade over time, its host galaxy (known as Messier 101 or M101) is still very interesting due to its large star-forming regions visible scattered throughout its spiral structure. This image is shown in color based on another image of M101 from a few days prior (courtesy of M. Prem), which was used to transfer the colors, using the data taken from the observatory’s monochrome exposure as a luminance layer.
Monochrome image of galaxy M51
M51: Colloquially known as the whirlpool galaxy, M51 is a real treat of the Northern skies, appearing close to the big dipper. Of course, the two interacting galaxies in this image are actually much further away; so far in fact that their light takes over 23 million years to get to us. These are some of the best known interacting galaxies, with the gravitational disruptions causing large tidal streams visible in longer exposure images, and likely contributing to the formation of the well defined spiral arms of the larger galaxy. M51 was the first to be identified as a spiral galaxy (or a spiral nebula as they were known at the time). The smaller, dimmer galaxy IC 4278 is also visible in this image just a little way from M51; see if you can spot it!
Monochrome image of the galaxy M81
M81: Another bright spiral galaxy near the big dipper, this grand design spiral galaxy is in the process of interacting with the nearby galaxy M82. This image highlights the large brightness difference between the very bright core of the galaxy, and the significantly fainter arms, where there wasn’t enough light collected to make them easily stand out from the background. To make the arms visible at all, the stacked image was greatly stretched, with heavy noise reduction applied.
Monochrome image of galaxy M82
M82: A companion galaxy to the spiral galaxy M81, and one of the nearest starburst galaxies, with its starburst thought to have been caused by a previous interaction with M81. A starburst galaxy is one where the rate of star formation is much greater than normal, with M82’s center alone producing around 10 times the new stars that the entire Milky Way galaxy does. This huge amount of star formation causes M82 to be very luminous, with the dust lanes seen in the image silhouetting the brighter background. Not seen in this image, but possible to pick up in longer exposures, are large streams of hydrogen that form a so called superwind which is likely driven by the supernovae which are common in this galaxy.
Monochrome image of the globular cluster M13
M13: A favorite of northern hemisphere astronomers and a target that we have imaged several times before, this large grouping of stars contains the mass of around 600,000 suns packed together far tighter that the local neighborhood of our own solar system. Because of its shape, M13 is known as a globular cluster, as opposed to the more common open star clusters such as the Pleiades. To show the maximum number of stars, this image of M13 was processed to enhance the visibility of faint parts of the cluster while preserving details in its bright core, which combined with the slightly blurred stars to make this image appear different from our other image of M13 shown further down the page.

Sunday, May 21st, 2023 (guest image)

This galaxy is looking different! These images were taken by trained observatory guest Gavin W. (JHU) and Observatory Fellow William B. (JHU). It was processed by Gavin W. using SIRIL. It shows the nearby M101 spiral galaxy, where just this past week a new supernova has erupted. Over the next few weeks, the bright source of light marked “SN 2023ixf” will fade away and disappear completely. Currently it is out shining the combined brightness of all the other stars in its host galaxy! This is one of the nearest supernova to the Earth this decade, an exciting opportunity for astronomers around the world to study these violent stellar-deaths in detail.

Friday, May 19th, 2023

The Ring Nebula (M57) in narrowband H-alpha, O[III] filters. This nebula was generated by a Sun-like star that has finished fusing hydrogen into helium. The nebula is about 7000 years old. The beautiful blue center of the nebula is emission from diffuse oxygen gas left in the wake of the expanding shell of red hydrogen gas, which we isolated at this open house using special filters that cut out a lot of the light pollution from the city.
The Sombrero Galaxy. We only managed to take images in one filter (a Green filter) but even in monochrome, the dramatic dust-lane of this galaxy is impressive. We are viewing this distant galaxy “edge-on” where the dust and gas that orbits within the spiral arms blocks the light from the center of the galaxy.
The Eyes Galaxy. More monochrome green filter images, again showing a beautiful partially edge-on galaxy with spirals of dust along its arms.
A globular cluster, M13, “Great Globular Cluster in Hercules.” This group of stars are more than a hundred times more closely packed together than the stars near our Sun. These stars are almost three times as old as the sun, 12 Billion years old, and this cluster exhibits signs of having been “accreted.” This means that this cluster of stars could have been a much smaller galaxy that the Milky Way gobbled up!

Monday, January 16th, 2023

Comet C/2022 E3 (ZTF), otherwise known as “the Green Comet” or “the Neanderthal Comet” is shown here, about two weeks before its closest approach, having just passed periapsis (when it is closest to the Sun). Images were observed by W. Balmer in Blue, Green, and Red filters using our science camera, and processed by M. Prem using SIRIL. Because it is nearby, the comet has a large apparent motion compared to the background stars, and keeping the telescope fixed on the comet during an imaging sequence results in star trails as seen here.

Tuesday, November 22, 2022

Processed image of Orion Nebula
Orion Nebula. This image combines 31 DSLR exposures with a total integration time of over 15 minutes, processed to bring out detail, calibrate the colors and suppress noise. Glowing gas is reflecting and re-emitting the light of bright young stars, while darker clouds of cool gas and dust frame and partly obscure the view.

Thursday, October 27

Color image of the bubble nebula
Bubble Nebula. A single massive, hot star is responsible for most of the nebula’s emission. Gas expelled from the star’s own “wind” forms the shell; the gas in the shell and in surrounding clouds is excited by light from the star and glows. About an hour’s worth of exposures in narrow band filters sensitive to emission from hydrogen, oxygen, and sulfur gas were combined to form this image. Processing was used to calibrate the colors, bring out details, and suppress background noise.
Crab Nebula. A single exposure, processed to suppress background noise and enhance contrast, reveals details within this iconic celestial object. The nebula itself is the result of a supernova explosion whose light first reached Earth in the year 1054.

Friday, October 21

The following image was obtained with our ZWO 1600MM Pro camera with a narrow-band H-alpha filter.

Monochrome image of eagle nebula through H-alpha filter
Eagle nebula (H-alpha): The eagle nebula seen in this image is an active star-forming region. The energetic emissions from its young stars cause the gas in the nebula to glow in very specific colors, the strongest of which is called H-alpha, from atomic hydrogen gas. When observed through a filter that only lets through this color of light, a significant amount of detail can be seen, from the brightly glowing gas itself as well as the dust clouds that block some of the light. This image was made by stacking 10 exposures to reduce noise and then stretching to show the detail hidden in the shadows.
Image of Saturn and Titan
Saturn and Titan. This image was created by combining short exposures to capture the planet itself with deeper exposures to be able to detect its large moon, Titan.

Friday, October 14

These images are from our Canon EOS 6D with a light pollution filter.

Image of globular cluster M13
M13. This globular cluster is composed of stars that are about 11.65 billion years old, nearly 3 times older than the Solar System! Observatory open house attendees took 5 images with a total exposure time of 11 minutes which were aligned and combined to produce the image pictured here.
Image of planetary nebula M27
M27. This target, called Dumbbell Nebula or the Apple Core Nebula, is a cloud of gas and dust expelled by a dying, Sun-like star. At its center is the remnant of the progenitor star, called a “white dwarf.” It is only about 10,000 years old, a very short time in astronomy! A certain young attendee took one 3 minute image of M27, which we post-processed using “photometric color calibration” to match the colors in the image to catalogue colors from research images, and then applied a brightness stretch and de-noising filter.
Image of planetary nebula M57
M57. The Ring Nebula was a favorite of our open house attendees, who took about 20 minutes’ worth of images of this nebula. Similar to M27, this nebula was generated by a Sun-like star that has finished fusing hydrogen into helium. The nebula is about 7000 years old. The beautiful blue center of the nebula is emission from diffuse oxygen gas left in the wake of the expanding shell of red hydrogen gas. We combined, smoothed, and then stretched the images to produce the final picture.

A visualization of stellar open clusters

Partial screenshot showing the stellar position visualizer.

Have you ever wished you could venture beyond Earth and explore among the stars? We certainly have. Alas, for the time being such explorations remain in the domain of imagination and science fiction. However, thanks to the precision of modern stellar catalogs, we can map the nearby stars and render their positions on your computer screen, allowing you to explore among them from the comfort of home! Click to access one such stellar visualization, created by MDSGC volunteer M. Prem. The accompanying text explains what is displayed and how it works. Have questions? Please email us at mdsgo@jhu.edu.

Preserving Dark Skies for Astronomy

Flyer for Dark Skies talk

Happy April! International Dark Sky Week is coming up later this month. We are delighted to invite you to attend a special two-part event in celebration of dark skies!

  • 4/15/22 @ 7pm ET – Dark Skies Presentation: Join us on Friday, April 15th at 7pm in room 361 of the Bloomberg Center for Physics and Astronomy (Johns Hopkins University Homewood Campus). Dr. Sarah Marie Bruno (JHU), cosmologist, will discuss the impact of satellite constellations on ground-based astronomy, and the importance of preserving dark skies for astronomy and beyond. Light refreshments will be served directly following the talk.

    Preserving Dark Skies for Astronomy: The starry night sky has inspired humanity from the dawn of our history. However, the night sky we can see from Baltimore in 2022 looks vastly different from the skies that Galileo Galilei observed with his telescope or the skies that inspired the star stories of indigenous peoples in North America. Artificial lighting from ground-based sources and reflections off satellites can impact astronomy and impede our ability to witness the natural beauty of the skies. The Milky Way, once a fixture of human experience, is now hidden from view for over two thirds of the world’s population. Sadly, light pollution is only getting worse with the increasing number of commercial satellites flooding low-Earth orbits. While satellite constellations such as SpaceX’s Starlink will likely boost the global economy and increase internet accessibility worldwide, they will introduce additional light pollution and foreground contamination which may greatly impede astronomical observations from the ground. Specifically, solar reflections, radio frequency transmission, and thermal emission will impact ground-based astronomy in the optical, radio, and microwave frequencies, respectively. Bruno wilI (1) discuss the projected impact of the growing space industry on the field of astronomy, (2) present proposed strategies for mitigating these effects, and (3) reflect on the importance of preserving the dark sky environment not only for astronomy, but for human health and wellbeing. 
  • 4/15/22 @ 8:30pm ET – Observatory Open House: After Dr. Bruno’s talk, we will migrate up to the roof of the Bloomberg building for an observatory open house. We expect that observing will be possible beginning around 8:30pm. We will use the telescope in the observatory to view the stars and planets and an additional smaller telescope on the roof to observe the Moon. Join us in celebrating the beautiful dark skies above Johns Hopkins campus! 

Please note that due to space limitations on the Bloomberg roof, this event is restricted to the first 50 registrants. Please sign up here to attend.

The event is free to attend and free parking will be available on the Upper Muller Lot (located next to the Bloomberg building and accessible off of San Martin Drive.)

 Note: This event (both talk and observatory night) is subject to rescheduling depending on the weather. The following Friday (4/22) is a backup day. Registered attendees will receive an email by the evening of April 14th confirming whether the event will take place April 15th or be postponed to April 22nd. 

Interactive Astrophysics Stories

At the MDSGC Observatory, we’re always looking to share our enthusiasm about the Universe and its many fascinating phenomena. Therefore, we’re pleased to present this short series of interactive online astrophysics stories!

#4: Detecting Exoplanets via Transits

Snapshot of a simulated planetary transit across the face of its host star.

Since the first discoveries starting in the 1990s (see post below), the continued search for new exoplanets and the study of their properties has grown into a major area of astronomical research. As additional effort has been invested and new technologies have been developed, the primary techniques for finding and characterizing new exoplanets have also evolved. Follow this link over to our Exoplanet Transits story at ObservableHQ to learn about how astronomers have discovered most of the exoplanets we now know — and where we’re still looking to improve our knowledge!

#3: Hot Jupiter Systems

Still frame of an animation of a Hot Jupiter planet orbiting its host star.

Until the 1990s, the only planets known to science were the nine* of our own solar system. As technology progressed and astronomers began to focus their efforts on looking for planets around other stars, they received several great surprises in the form of just how different the first discovered “exoplanet” systems were, compared to ours. In the decades since, intense efforts have revealed a more detailed picture, and we now understand planetary systems to be a widespread if not universal phenomenon — as astronomers had hoped all along. But the earliest discovered systems continue to play an important role in our new understanding. Follow this link over to our Hot Jupiter story at ObservableHQ to learn more!

(*Those were the days, eh, Pluto?)

#2: Imaging a Star Cluster

Image of stars in Messier 67 taken from the Maryland Space Grant Observatory.

When it comes to practical astronomy, whether we’re idly admiring the night sky or concentrating closely on a telescopic view, star clusters are some of the most interesting things up there. The image above shows a portion of the star cluster Messier 67 obtained from our Observatory. (Another prime example of a star cluster is also one of the Fall sky’s highlights: the Pleiades, or Seven Sisters.) So what, apart from simple visual appeal, makes star clusters interesting for astronomers?

Follow this link over to our interactive Star Cluster Image story at ObservableHQ to learn more!

#1: The Earth-Moon System

Still frame from animation of the Earth-Moon system at the epoch of the dinosaurs, showing Earth's tidal bulge.

It was Fall as we wrote this, and in Earth’s northern hemisphere the days were getting shorter. DayLIGHT, that is! But did you know that actually, the length of Earth’s day is increasing as time goes on? What’s that all about, and what in the Universe could be responsible?

Follow this link over to our interactive Earth-Moon System story at ObservableHQ to find out!

After reading, send us your questions and let us know what you think at mdsgo@jhu.edu!

Observe the Moon

First quarter moon over Earth's limb; photo taken from ISS.
Image of the Moon over Earth’s limb, taken from the International Space Station in 2019.

While most of our attention may understandably be consumed by events taking place here on planet Earth, it’s a good practice to pause occasionally and take in a larger perspective. A fine occasion for such activity presents itself whenever clear skies align with favorable Moon phases.

Each year, International Observe the Moon Night, marked in 2020 on Saturday, September 26th, encourages Earthlings to point our gazes skyward and appreciate our closest celestial neighbor. (NASA organizes a list of events that might allow for an in person experience, as well as ways to participate from home.)

The first quarter lunar phase each month is widely considered to be best for viewing because of its evening visibility and the oblique angle of sunlight that throws its surface details into sharp relief. When looking at the Moon from Earth, we definitely recommend grabbing a pair of binoculars, if available, as any amount of magnification greatly enhances the visibility of surface features such as craters.

And while you’re thinking about gazing skyward, don’t forget to think about other ways to get your astronomy fix, and be sure to check out Sky & Telescope’s Sky at a Glance for more detail about what’s on the celestial menu these days.

Astronomy during the pandemic

NASA SOFIA image of the Milky Way.

While the MDSGC Observatory remains closed for the time being, with a little inspiration and effort we can still admire the night sky above us — and certainly now, as much as ever, we can all benefit from a cosmic perspective!

Here is a recent article by University of Arizona astronomer professor Chris Impey on ways to enjoy astronomy during the pandemic. It’s a must read for would be backyard astronomers. Of special note is the “Sky at a Glance” from Sky & Telescope, a highly useful guide to tracking the Moon, planets, and other noteworthy celestial events.

Another recommended activity that may be appealing is to construct a planisphere: a device that shows the locations of the stars in the sky each night. You can buy one, of course, or use free astronomy software such as Stellarium, but if you happen to live at a latitude not too different from Baltimore, MD (39.29 degrees North) and have access to a printer, you can also make your own using these files: planisphere instructions and planisphere cutouts. The second file has two pages, which need to be printed on separate sheets of paper. You’ll also need a paperclip.

Until we can once again welcome you to visit our Observatory, happy star-gazing!

NASA and ISS Videos

Aurora over Scandinavia at night from the International Space Station.

Watching live coverage of the successful NASA Mars Insight landing yesterday reminded us of some other excellent space videos we’ve seen lately.

Here’s one to mark NASA’s 60th anniversary. Like science fiction, but real:

Also celebrating an anniversary recently, in this case its 20th, was the International Space Station (ISS). A long sequence of Earth from orbit, with some landmarks identified:

As long as we’re on the topic, here’s one more from ISS. An inbound rocket launch:

Hope you enjoy them as much as we did. If you’re curious about the image at the top, click on it to learn more!

Quaternions Turn 175

Plaque on Broom (Brougham) Bridge in Ireland commemorating Hamilton's discovery of quaternions.

Tuesday, October 16, 2018, is the one hundred and seventy-fifth anniversary of the discovery of quaternions, one of the most difficult discoveries ever in the history of mathematical physics.  The discovery was made — in a sudden moment of inspiration following 11 years of studious toil — by Sir William Rowan Hamilton as he was crossing Brougham Bridge, in Ireland, with his wife.  On the spot, or so it is said, he carved his famous equations on the bridge.

Some years later, Hamilton recalled:

They started into life, or light, full grown, on the 16th of October, 1843, as I was walking with Lady Hamilton to Dublin, and came up to Brougham Bridge.  That is to say, I then and there felt the galvanic circuit of thought closed, and the sparks which fell from it were the fundamental equations between I, J, K; exactly such as I have used them ever since.  I pulled out, on the spot, a notebook, which still exists, and made an entry….

Although Hamilton’s original inscription does not survive, the plaque shown above hangs on the bridge to this day in commemoration both of Hamilton’s discovery and of his sudden inspiration. The plaque reads:

Here as he walked by
on the 16th of October 1843
Sir William Rowan Hamilton
in a flash of genius discovered
the fundamental formula
for quaternion multiplication
i2 = j2 = k2 = i j k = -1
& cut it on a stone of this bridge

Here’s to Hamilton, to quaternions, to bridges, and to inspiration!