- Arecibo Observatory Contributes to the Exploration of Black Holes Started by this Year’s Nobel Prize Winners in Physics19 Nov, 2020
- UCF Delivers Engineering Options for Arecibo Observatory (AO)16 Nov, 2020
- Management Update (October 12, 2020) by Director Eng. Francisco Cordova13 Oct, 2020
- Summer Student Assists in Development of Newest AO Facility01 Oct, 2020
- STAR Academy: Training the Next Generation of STEM Professionals 29 Sep, 2020
- Management Update (August 11, 2020) by Director Eng. Francisco Cordova29 Sep, 2020
- Management Update (August 28, 2020) by Director Eng. Francisco Cordova29 Sep, 2020
- Arecibo STAR Teachers29 Sep, 2020
- Hunting for the Mysterious Origins of Fast Radio Bursts28 Sep, 2020
- Girls Educating Girls 28 Sep, 2020
- Cassini Data Solves Mystery of Arecibo Radar Signals on Titan28 Sep, 2020
- How to Build an Asteroid11 Sep, 2020
- A Holistic Approach to Understanding Asteroids11 Sep, 2020
- Sharing the Connection: Arecibo’s Planetary Radar & NASA’s OSIRIS-REx Mission to Bennu10 Sep, 2020
- Analyzing Gravitational Fields Around Small Bodies in Support of Future Spacecraft Missions09 Sep, 2020
- Broken Cable Damages Arecibo Observatory11 Aug, 2020
A Holistic Approach to Understanding Asteroids
Byadmin11 September 2020 Planetary

Image of laboratory setup at York University used for Dr. Hickson’s experimental study of the electromagnetic properties of mineral powders..
Planetary |
Asteroids, though often simply considered “rocks in space,” are actually composed of an array of different materials. It is important to know what asteroids are made of in order to determine the structure and formation of asteroids, and to assess any risk that an individual asteroid would pose if on a collision course with Earth.
A recent study led by AO postdoctoral researcher Dr. Dylan Hickson, published in the Journal of Geophysical Research: Planets, takes a holistic approach at interpreting planetary radar data to better understand asteroid composition.
“We conducted laboratory experiments on various mineral powders at different densities to measure the corresponding change in their electrical properties,” Dr. Hickson explained. “We compared these laboratory measurements with known theoretical models and combined them with radar scattering models to infer the density of asteroid surfaces observed using radar.” This work was conducted at York University.
These theoretical models are the ones that are used to decipher planetary radar observations, like those obtained at the Arecibo Observatory, so it was important to see how accurately the models reflected the laboratory studies. Without in-depth knowledge of how the electrical properties, like permittivity, scatter the radar signals, interpreting planetary radar observations can be challenging.
“That’s why this research was exciting to me,” Dr. Hickson related. “We used both laboratory experimentation and theoretical modeling to address a specific problem in planetary radar.”
“These two sides to the story are necessary to get the full picture,” he continued. “Having the opportunity to carry out both in the same project provided a broad perspective of a research area that has been active since the pre-Apollo era.”
“Having the opportunity to carry out both in the same project provided a broad perspective of a research area that has been active since the pre-Apollo era.” - Dr. Dylan Hickson, Postdoctoral Researcher at Arecibo Observatory
Through their laboratory measurements, Dr. Hickson and his team showed that the dielectric models they tested could be effective at determining the permittivity of geologic powders; however, they found that some models are more accurate than others.
“Ultimately, my goal is to learn more about the complex surfaces of near-Earth asteroids,” Dr. Hickson shared. “Much more laboratory experimentation is needed to better understand the electromagnetic properties of these geologic materials.”
About Arecibo
The Arecibo Planetary Radar Program is funded by NASA’s Near-Earth Object Observations Program. The Arecibo Observatory is operated by the University of Central Florida (UCF) in partnership with Universidad Ana G. Mendez - Universidad Metropolitana and Yang Enterprises Inc., under a cooperative agreement with the National Science Foundation (NSF).
Article written by Dr. Tracy Becker - AO Collaborator / SwRI Research Scientist
Contact: tbecker@swri.edu |
Head of Planetary Radar team |
Keywords: arecibo, observatory, planetary, hickson, radar, scattering, rocks, space, models, Geophysical, Research, Planets, electromagnetic, properties, mineral, powders